Gravitational lensing occurs when things with mass create ripples and dents in the fabric of spacetime, and light has to follow along those lines, which sometimes create a magnifying glass effect. This both sounds and looks like something wild from science fiction, but it’s actually a very important tool in astronomy. The James Webb Space Telescope has been in the news a lot recently for just this: watching how light bends around massive galaxy clusters in space, revealing fainter, further away old galaxies behind them. 

Now, Slava Turyshev, a scientist at NASA’s Jet Propulsion Lab, is trying to harness one of these gravitational lenses closer to home, using our sun. In a new paper posted to the pre-print server arXiv, Turyshev computes all the detailed math and physics needed to show that it is actually possible to harness our sun’s gravity in this way, with some pretty neat uses. A so-called “solar gravitational lens” (SGL) could help us beam light messages into the stars for interstellar communication or investigate the surfaces of distant exoplanets.

“By harnessing the gravitational lensing effect of our star, astronomy would experience a revolutionary leap in observing capability,” says Nick Tusay, a Penn State astronomer not involved in the new work. “Light works both ways, so it could also boost our transmitting capability as well, if we had anyone out there to communicate with.”

When it comes to telescopes here on Earth, bigger is definitely better. To collect enough light to spot really faint far away objects, you need a huge mirror or lens to focus the light—but we can really only build them so big. This is where the SGL comes in, as an alternative to building bigger telescopes, instead relying on spacetime bent by the sun’s gravity to do the focusing for us. 

“Using the SGL removes the need to build larger telescopes and instead raises the problem of how to get a telescope out to the focal distance of the Sun (and how to keep it there),” explains Macy Huston, a Berkeley astronomer not involved in the new research. “And there’s a lot of work ongoing to try to solve this,” they add.

Turyshev is actively working on a mission design to send a one-meter telescope (less than half the size of the famous Hubble) out to the focus of the sun’s gravitational well. It’s quite a trek—this focal point is located about 650 AU out from our star, almost five times out from humanity’s current distance record holder, Voyager 1. To get out to such a huge distance in less than a lifetime, the team is relying on cutting-edge solar sail technology to move faster than ever before.

Currently, the James Webb Space Telescope is investigating the atmospheres of planets around other stars, and the future Habitable Worlds Observatory in the 2040s will hopefully be able to see enough detail in exoplanetary atmospheres to find hints of life. Turyshev’s mission would be the next big step towards confirming life on other worlds, hopefully launching around 2035. Once JWST and HWO identify possibly interesting worlds, the SGL telescope will then actually map the surface of an exoplanet in detail. Turyshev claims it would be able to see a planet blown up to 700 by 700 pixels—a huge improvement on direct imaging’s current 2 or 3 pixels. “If there is a swamp on that exoplanet, emitting methane, we’ll know that’s what is positioned on this continent on this island, for example,” he explains.

Looking further into the sci-fi future, this same SGL technology could be used not only “as a telescope we could use from the solar system to view other planetary systems in great detail” but also as an “interstellar communication network (for intentional communications),” says Huston. A laser positioned at the sun’s gravitational focus could send messages to other stars without losing as much signal as our current Earth-bound beacon tech.

“If we were to ever become an interstellar civilization, this [SGL] could potentially be the most effective means of communication between star systems,” says Tusay. Our radio transmissions, leaking out of Earth’s atmosphere since the early 1900s, rapidly become fainter the further away from our planet. Turyshev’s mathematical calculations show that signals sent from the SGL could be easily noticed at the distances of nearby stars, even when accounting for the noisy background of the real world. Transmission via the SGL is “not prohibited, it’s really encouraged by physics,” says Turyshev.

This tech wouldn’t solve all our interstellar roadblocks, though. We might be able to send messages, but we still don’t have a way of sending ourselves out amongst the stars to travel. There’d also be a huge delay in our galactic calls—more like sending a cross-country letter by horseback than FaceTiming with your friends. “Light still has a maximum speed,” reminds Tusay. As a result, sending a message to a star four light-years away would take four years to get there, and another four for the response to reach us. Still, the solar gravitational lens is one big step towards making our science fiction futures a reality.

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Reducing damaging “ultra-emission” methane leaks could soon become much easier–thanks to a new, open-source tool that combines machine learning and orbital data from multiple satellites, including one attached to the International Space Station.

Methane emissions originate anywhere food and plant matter decompose without oxygen, such as marshes, landfills, fossil fuel plants—and yes, cow farms. They are also infamous for their dramatic effect on air quality. Although capable of lingering in the atmosphere for just 7 to 12 years compared to CO2’s centuries-long lifespan, the gas is still an estimated 80 times more effective at retaining heat. Immediately reducing its production is integral to stave off climate collapse’s most dire short-term consequences—cutting emissions by 45 percent by 2030, for example, could shave off around 0.3 degrees Celsius from the planet’s rising temperature average over the next twenty years.

[Related: Turkmenistan’s gas fields emit loads of methane.]

Unfortunately, it’s often difficult for aerial imaging to precisely map real time concentrations of methane emissions. For one thing, plumes from so-called “ultra-emission” events like oil rig and natural gas pipeline malfunctions (see: Turkmenistan) are invisible to human eyes, as well as most satellites’ multispectral near-infrared wavelength sensors. And what aerial data is collected is often thrown off by spectral noise, requiring manual parsing to accurately locate the methane leaks.

A University of Oxford team working alongside Trillium Technologies’ NIO.space has developed a new, open-source tool powered by machine learning that can identify methane clouds using much narrower hyperspectral bands of satellite imaging data. These bands, while more specific, produce much more vast quantities of data—which is where artificial intelligence training comes in handy.

The project is detailed in new research published in Nature Scientific Reports by a team at the University of Oxford, alongside a recent university profile. To train their model, engineers fed it a total of 167,825 hyperspectral image tiles—each roughly 0.66 square miles—generated by NASA’s Airborne Visible/Infrared Imaging Spectrometer (AVIRIS) satellite while orbiting the Four Corners region of the US. The model was subsequently trained using additional orbital monitors, including NASA’s hyperspectral EMIT sensor currently aboard the International Space Station.

The team’s current model is roughly 21.5 percent more accurate at identifying methane plumes than the existing top tool, while simultaneously providing nearly 42 percent fewer false detection errors compared to the same industry standard. According to researchers, there’s no reason to believe those numbers won’t improve over time.

[Related: New satellites can pinpoint methane leaks to help us beat climate change.]

“What makes this research particularly exciting and relevant is the fact that many more hyperspectral satellites are due to be deployed in the coming years, including from ESA, NASA, and the private sector,” Vít Růžička, lead researcher and a University of Oxford doctoral candidate in the department of computer science, said during a recent university profile. As this satellite network expands, Růžička believes researchers and environmental watchdogs will soon gain an ability to automatically, accurately detect methane plume events anywhere in the world.

These new techniques could soon enable independent, globally-collaborated identification of greenhouse gas production and leakage issues—not just for methane, but many other major pollutants. The tool currently utilizes already collected geospatial data, and is not able to currently provide real-time analysis using orbital satellite sensors. In the University of Oxford’s recent announcement, however, research project supervisor Andrew Markham adds that the team’s long-term goal is to run their programs through satellites’ onboard computers, thus “making instant detection a reality.”

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The sun is setting earlier, giving you a longer chance to get a view of the night sky. You can see stars, planets, meteors, and more with this Celestron telescope deal at Amazon for Cyber Monday.

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A new image from NASA’s almost two-year-old James Webb Space Telescope features new details of a portion of our galaxy’s dense center for the first time. The image includes some parts of the star-forming hotspot that astronomers are still trying to fully understand. The region is named Sagittarius C and is about 300 light-years away from Sagittarius A*, or the supermassive black hole at the center of our galaxy.

[Related: Gaze upon the supermassive black hole at the center of our galaxy.]

“There’s never been any infrared data on this region with the level of resolution and sensitivity we get with Webb, so we are seeing lots of features here for the first time,” observation team principal investigator Samuel Crowe said in a statement. “Webb reveals an incredible amount of detail, allowing us to study star formation in this sort of environment in a way that wasn’t possible previously.” Crowe is an undergraduate student at the University of Virginia in Charlottesville.

The image features roughly 500,000 stars and a cluster of young stars called protostars. These are stars that are still forming and gaining mass, while generating outflows that glow in the midst of an infrared-dark cloud. A massive previously-discovered protostar that is over 30 times the mass of our sun is located at the heart of this young cluster. 

The protostars are emerging from a cloud that is so dense that the light from stars behind it cannot reach the JWST. This light trick makes the region look deceptively less crowded. According to the team, this is actually one of the most tightly packed areas of the image. Smaller infrared-dark clouds dot the image where future stars are forming. 

“The galactic center is the most extreme environment in our Milky Way galaxy, where current theories of star formation can be put to their most rigorous test,” University of Virginia astronomer Jonathan Tan said in a statement. 

JWST’s Near-Infrared Camera (NIRCam) also captured large-scale emission from ionized hydrogen that is surrounding the lower side of the dark cloud. According to Crowe, this is the result of energetic photons that are being emitted by young massive stars. The expanse of the region spotted by JWST came as a surprise to the team and needs more investigation. They also plan to further examine the needle-like structures in the ionized hydrogen, which are scattered in multiple directions.

“The galactic center is a crowded, tumultuous place. There are turbulent, magnetized gas clouds that are forming stars, which then impact the surrounding gas with their outflowing winds, jets, and radiation,” Rubén Fedriani, a co-investigator of the project at the Instituto Astrofísica de Andalucía in Spain, said in a statement. “Webb has provided us with a ton of data on this extreme environment, and we are just starting to dig into it.”

[Related: ‘Christmas tree’ galaxy shines in new image from Hubble and JWST.]

At roughly 25,000 light-years from Earth, the galactic center is close enough for the JWST to study individual stars. This allows astronomers to collect data on both how stars form, but also how this process may depend on the cosmic environment when compared to other regions of the galaxy. One question this could help answer is if there are more massive stars in the center of the Milky Way, as opposed to on the edges of the galaxy’s spiral arms.

“The image from Webb is stunning, and the science we will get from it is even better,” Crowe said. “Massive stars are factories that produce heavy elements in their nuclear cores, so understanding them better is like learning the origin story of much of the universe.”

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With their winding and buff arms made up of billions of stars, spiral galaxies offer some of the beautiful images of the universe. Our own Milky Way galaxy is a spiral galaxy, yet these types of swirling clusters are relatively scarce in a part of the universe called the Supergalactic Plane. A team of astrophysicists believes that the bright elliptical galaxies without a defined center are more common than swirling galaxies because of the difference in density of the environments found inside and outside of the Plane. The findings are described in a study published November 20 in the journal Nature Astronomy.

[Related: Behold six galactic collisions, masterfully captured by Hubble.]

Smoothing out the arms

The Supergalactic Plane is a flattened structure in the universe that extends nearly a billion light years across. Our own Milky Way galaxy is embedded within the Plane and is about 100,000 light years wide. There are dozens of enormous armless galaxy clusters called elliptical galaxies in the Plane, but not nearly as many disk-shaped galaxies with spiral arms. 

According to the new study, the different distributions of elliptical and disk galaxies are a natural occurrence. Galaxies experience frequent interactions and mergers with other galaxies in the Plane because the region is so densely packed. This galactic demolition derby then turns the spiral galaxies into elliptical galaxies. The arms are smoothed out and the lack of internal structure in the elliptical galaxy and presence of dark matter leads to the growth of supermassive black holes. Since the dark matter outweighs everything else, it has the power to shape the newly formed elliptical galaxy and tends to guide the growth of the central black hole.

The stars in an elliptical galaxy also orbit around the core in random directions and are generally older than those in spiral galaxies, according to NASA. 

In parts of the universe away from Plane, galaxies can evolve in relative isolation. This solitude helps them preserve their spiral structure.

“The distribution of galaxies in the Supergalactic Plane is indeed remarkable,” Carlos Frenk, a study co-author and astrophysicist at Durham University in the United Kingdom, said in a statement. “It is rare but not a complete anomaly: our simulation reveals the intimate details of the formation of galaxies such as the transformation of spirals into ellipticals through galaxy mergers.”

A galactic time machine

In the study, the team used a supercomputer simulation called Simulations Beyond the Local Universe. It follows the evolution of the universe over a period of 13.8 billion years from around the time of the Big Bang up to the present. 

[Related: Hubble image captures stars forming in a far-off phantom galaxy.]

Most cosmological simulations consider random patches of the universe, which cannot be directly compared to other observations. Instead, SIBELIUS works to precisely reproduce the observed structures in space, including the Supergalactic Plane. According to the team, the final simulation is remarkably consistent with observations of our universe through telescopes.

“The simulation shows that our standard model of the universe, based on the idea that most of its mass is cold dark matter, can reproduce the most remarkable structures in the universe, including the spectacular structure of which the Milky Way is part,” said Frenk.

Scientists have been studying the separation of elliptical and spiral galaxies since the 1960s. This partitioning features prominently in a recent list of cosmic anomalies that was compiled by cosmologist and 2019 Nobel laureate Professor Jim Peebles.

“By chance, I was invited to a symposium in honor of Jim Peebles last December at Durham, where he presented the problem in his lecture,” study co-author and astrophysicist at the University of Helsinki in Finland Till Sawala said in a statement. “And I realized that we had already completed a simulation that might contain the answer. Our research shows that the known mechanisms of galaxy evolution also work in this unique cosmic environment.”

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SpaceX’s second, unpiloted Starship test flight of the year ended in yet another fiery inferno on November 18. This time, the sudden end arrived roughly 8 minutes into its 90-minute scheduled mission. But although its Super Heavy first stage booster suffered a fatal “rapid unscheduled disassembly” in the Caribbean, the world’s most powerful rocket almost doubled its previous lifespan and passed multiple other crucial milestones.

Starship launched once again from its test site near Boca Chica, Texas, at 8:03am ET on Saturday, with all 39 of the Super Heavy booster’s Raptor engines remaining lit during the mission—a first for the spacecraft intended to eventually deliver humans to Mars. At two minutes and 41 seconds following liftoff, Starship’s hot-staging sequence—in which upper stage engines ignite and separate from the booster—also proceeded successfully, clearing yet another hurdle for SpaceX engineers. The reusable booster then performed its flip maneuver en route towards an intended safe return back to Earth, but exploded only a few seconds later. The booster’s fate wasn’t a huge surprise, however, as SpaceX mission control operators already suspected such a dramatic event could occur due to the immense “load on top of the booster.”

Meanwhile, the Starship upper stage continued to soar for another few minutes to roughly 92 miles above the Earth’s surface—well above the Kármán Line, an internationally recognized demarcation between the planet’s atmosphere and outer space. Moments before its scheduled Second Engine Cut Off, or SECO, the upper stage met its own explosive demise. Space X representatives cited a delay in Starship’s automated flight termination system, but do not yet know the exact cause for its malfunction. If successful, Starship would have circumnavigated Earth before performing a hard landing near Hawaii.

The results of April’s Starship test received considerable criticism from both Boca Chica locals and the Federal Aviation Administration for surrounding environmental damage sustained during launch. Starship’s Raptor engines burn approximately 40,000 pounds of fuel per second to reach 17 million pounds of thrust. Nearby Texan residents described the blowback as resembling a “mini earthquake” at the time, with at least one business owner’s store window shattering. The April 20 test flight blasted a 25-feet deep crater, ejecting clouds of dirt, dust, and debris into the air while smashing a bowling ball-sized fragment into a nearby NASA Spaceflight van. Much of the area near Starship’s launch site includes protected ecosystems, as well as land considered sacred by local Indigenous communities. The FAA soon issued 63 corrective actions needed before SpaceX could legally attempt another Starship test.

[Related: SpaceX’s Starship launch caused a ‘mini earthquake’ and left a giant mess.]

Unlike SpaceX’s outing, Starship’s upgraded launch mount reportedly better mitigated the resulting blowback—at least according to Elon Musk’s company assessment. The FAA, meanwhile, wasted no time in issuing its own statement on Saturday’s event.

“A mishap occurred during the [SpaceX] Starship OFT-2 launch from Boca Chica, Texas, on Saturday, Nov. 18,” the administration posted to X over the weekend. Although no injuries or public property damage was reported this time, the FAA promised to oversee the “SpaceX-led mishap investigation” to ensure the company will comply with “regulatory requirements.”

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Although NASA’s Psyche spacecraft is currently en route to its rendezvous with a unique, metal-heavy asteroid floating between Mars and Jupiter, it still has quite a while before it reaches its destination. But researchers aren’t waiting until the end of its 3.5 year, 280-million-mile journey to make the most of the project. Even after barely a month of spaceflight, Psyche is already achieving some impressive technological feats.

On November 16, NASA announced its Deep Space Optical Communications experiment aboard Psyche successfully achieved “first light” earlier this week, beaming a data-laden, near-infrared laser nearly 10 million miles back to Caltech’s Palomar Observatory. Additionally, DSOC operators were able to “close the link”—the vital process in which test data is simultaneously beamed through both uplink and downlink lasers. Although only the first of numerous test runs to come, it completes a necessary step within NASA’s ongoing plans to develop far more powerful communications tools for future space travel.

[Related: In its visit to Psyche, NASA hopes to glimpse the center of the Earth.]

Astronauts, ground crews, and private companies have all utilized radio wave frequencies for data transfers and communications since the late-1950’s, thanks to a global antenna array known as the Deep Space Network. As organizations like NASA aim to expand humanity’s presence beyond Earth in the coming decades, they’ll need to move away from radio systems to alternatives like infrared lasers. Not only are such lasers more cost efficient, but they are also capable of storing and transmitting far more information within their shorter wavelengths. Further along in DSOC’s development, for example, will hopefully accomplish data transmission rates between 10-to-100 times greater than today’s spacecraft radio systems.

“Achieving first light is one of many critical DSOC milestones in the coming months, paving the way toward higher-data-rate communications capable of sending scientific information, high-definition imagery, and streaming video in support of humanity’s next giant leap: sending humans to Mars,”  Trudy Kortes, NASA’s director of Technology Demonstrations, said in Thursday’s announcement.

NASA also noted that, while similar infrared communications has been successfully achieved in low Earth orbit as well as to-and-from the moon, this week’s DSOC milestone marks the first test through deep space. This is more difficult thanks to the comparatively vast, growing distance between Earth and Psyche. During the November 14 test, data took roughly 50 seconds to travel from the spacecraft to researchers in California. At its farthest distance from home, Psyche’s data-encoded photons will take around 20 minutes to relay. That’s more than enough time for both Earth and Psyche to drift further along their own respective cosmic paths, so laser arrays on the craft and at NASA will need to adjust for the changes. Future testing will ensure the terrestrial and deep space tech is up to the task.

[Related: NASA’s mission to a weird metal asteroid has blasted off.]

Once it becomes the new norm, Jason Mitchell, director of the Advanced Communications and Navigation Technologies Division within NASA’s Space Communications and Navigation (SCaN) program, believes optical lasers will offer a “boon” for researchers’ space missions data collection, and will help enable future deep space exploration.
“More data means more discoveries,” Mitchell said in NASA’s announcement.

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Hindsight is not quite 20/20 for NASA’s historic Apollo missions. For instance, the Apollo 12 lander successfully touched down on the moon at exactly 6:35:25 UTC on November 19, 1969. What happened to the lunar environment as astronauts touched down, however, wasn’t recorded—and exact details on the reactions between nearby rocks, debris, and lunar regolith to lander engines’ supersonic bursts of gas aren’t documented. And physically replicating Apollo 12’s historic moment on Earth isn’t possible, given stark differences in lunar gravity and geology, not to mention the moon’s complete lack of atmosphere.

This is particularly a problem for NASA as it continues to plan for astronauts’ potential 2025 return to Earth’s satellite during the Artemis program. The landing craft delivering humans onto the lunar surface will be much more powerful than its Apollo predecessors, so planning for the literal and figurative impact is an absolute necessity. To do so, NASA researchers at the Marshall Space Flight Center in Huntsville, Alabama, are relying on the agency’s Pleiades supercomputer to help simulate previous lunar landings—specifically, the unaccounted information from Apollo 12.

As detailed by NASA earlier this week, a team of computer engineers and fluid dynamics experts recently designed a program capable of accurately recreating Apollo 12’s plume-surface interactions (PSI), the interplay between landing jets and lunar topography. According to the agency, the Pleiades supercomputer generated terabytes of data over the course of several weeks’ worth of simulations that will help predict PSI scenarios for NASA’s Human Landing System, Commercial Lunar Payload Services, and even future potential Mars landers.

[Related: Meet the first 4 astronauts of the ‘Artemis Generation’]

NASA recently showed off one of these simulations—the Apollo 12 landing—during its appearance at SC23, an annual international supercomputing conference in Denver, Colorado. For the roughly half-minute simulation clip, the team relied on a simulation tool called the Gas Granular Flow Solver (GGFS). The program is both capable of modeling interactions to predict regolith cratering, as well as dust clouds kicked up around the lander’s immediate surroundings.

According to the project’s conference description, GGFS utilizing its highest fidelities can “model microscopic regolith particle interactions with a particle size/shape distribution that statistically replicates actual regolith.” To run most effectively on “today’s computing resources,” however, the simulation considers just one-to-three potential particle sizes and shapes.

[Related: Moon-bound Artemis III spacesuits have some functional luxury sewn in.]

The approximation of the final half-minute of descent before engine cut-off notably includes depictions of shear stress, or the lateral forces affecting a surface area’s erosion levels. In the clip, low shear stress is represented by a dark purple hue, while the higher shear stress areas are shown in yellow.

Going forward, the team intends to optimize the tool’s source code, alongside integrating increased computational resources. Such upgrades will allow for better, higher fidelity simulations to fine-tune Artemis landing procedures, as well as potentially plan for landing missions far beyond the lunar surface.

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A team using NASA’s James Webb Space Telescope has observed two of the most distant galaxies astronomers have ever seen. At close to 33 billion light years away from Earth, these distant regions can offer insight into how the universe’s earliest galaxies may have formed. The findings are detailed in a study published November 13 in The Astrophysical Journal Letters.

[Related: ‘Christmas tree’ galaxy shines in new image from Hubble and JWST.]

The galaxies UNCOVER z-13 and UNCOVER z-12 are the second and fourth most distant galaxies ever observed and are located in a region called Pandora’s Cluster (Abell 2744). The two galaxies are among the 60,000 sources of light in Pandora’s Cluster that were captured in some of the first deep field images the JWST took in 2022. This region of space was selected for this kind of imaging due to its location behind several galaxy clusters. The light creates a natural magnification effect called gravitational lensing. This happens when the gravitational pull of the clusters’ combined mass warps the space-time around it. It then magnifies any light that passes nearby and offers a larger view behind the clusters.

Other galaxies confirmed at this distance generally appear in images as red dots. However, these new galaxies are larger and look more like a peanut and a fluffy ball, according to the team.

“Very little is known about the early universe, and the only way to learn about that time and to test our theories of early galaxy formation and growth is with these very distant galaxies,” study co-author and astronomer Bingjie Wang from Penn State University said in a statement. “Prior to our analysis, we knew of only three galaxies confirmed at around this extreme distance. Studying these new galaxies and their properties has revealed the diversity of galaxies in the early universe and how much there is to be learned from them.” 

Wang is also a member of the JWST UNCOVER (Ultradeep NIRSpec and NIRCam ObserVations before the Epoch of Reionization) team that conducted this research. UNCOVER’s early goal is to obtain highly detailed images of the region around Pandora’s Cluster using JWST.

Since the light that is emitted from these galaxies had to travel for so long to reach Earth, it offers a window into the universe’s past. The team estimates that the light JWST detected was emitted by the two galaxies when the universe was about 330 million years old and that it traveled for about 13.4 billion light years to reach the space telescopes. 

However, the galaxies are currently closer to 33 billion light years away from Earth because of the expansion of the universe over this period of time. 

“The light from these galaxies is ancient, about three times older than the Earth,” study co-author, Penn State astronomer, and UNCOVER member Joel Leja said in a statement.  “These early galaxies are like beacons, with light bursting through the very thin hydrogen gas that made up the early universe. It is only by their light that we can begin to understand the exotic physics that governed the galaxy near the cosmic dawn.”

[Related: JWST takes a jab at the mystery of the universe’s expansion rate.]

The two galaxies are also considerably bigger than the three galaxies previously located at these extreme distances. While our Milky Way galaxy is roughly 100,000 light years across, galaxies in the early universe are believed to have been very compressed. A galaxy of 2,000 light years across like one of ones the team imaged came as a surprise.

“Previously discovered galaxies at these distances are point sources—they appear as a dot in our images,” Wang said. “But one of ours appears elongated, almost like a peanut, and the other looks like a fluffy ball. It is unclear if the difference in size is due to how the stars formed or what happened to them after they formed, but the diversity in the galaxy properties is really interesting. These early galaxies are expected to have formed out of similar materials, but already they are showing signs of being very different than one another.”

To make inferences about these early galaxies, the team used detailed models. They believed that in addition to being young (by space standards), the two galaxies also had few metals in their composition, and were growing rapidly and actively forming stars. 

“The first elements were forged in the cores of early stars through the process of fusion,” Leja said. “It makes sense that these early galaxies don’t have heavy elements like metals because they were some of the first factories to build those heavy elements. And, of course, they would have to be young and star-forming to be the first galaxies, but confirming these properties is an important basic test of our models and helps confirm the whole paradigm of the Big Bang theory.”

Astronomers will continue to use lensing clusters and the instruments aboard the JWST to continue to peel back the timeline of some of the universe’s first galaxies.  

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There are millions of pieces of space junk orbiting Earth these days, so what’s one more bit of detritus amidst the trash cloud?

According to NASA’s recent spacewalk debriefing, International Space Station denizens Jasmin Moghbeli and Loral O’Hara spent nearly seven hours conducting various repairs on a sun-tracking solar panel array. During their shift, however, one of their “crew lock bags” (astronaut-speak for a toolkit) accidentally got loose, and drifted away before either astronaut could catch it. While not a major issue in and of itself, this certainly highlights (yet again) the growing problem floating above humanity’s heads.

[Related: The FCC just dished out their first space junk fine.]

Thankfully, the lock bag didn’t contain anything of major importance. In a separate press conference last week, ISS deputy program manager Dana Weigel stated the bag’s contents included “some tethers and things like tool sockets” similar to the everyday household varieties, calling them “fairly common items” that aren’t a “huge impact” for the crew. Most importantly, Mission Control observed the bag’s current orbital trajectory and determined it presents a low risk of “recontacting” with the ISS, with “no action required.”

Meganne Christian, a European Space Agency 2022 astronaut class member, shared a clip on social media taken from Moghbeli’s helmet camera showing the toolbag’s escape into the cosmic abyss.

Since the toolbag isn’t in a stable orbit, experts estimate it will decay into Earth’s atmosphere sometime during March 2024. Given its size, the lost equipment will burn up completely during the descent, so there’s no need to stress or keep an eye to the sky—unless that’s your thing, of course.

The US Space Force already cataloged the new orbital debris as 58229/1998-067WC, and will track its movements over the course of its lifespan. Per The Register, the toolbag’s brightness is measured at a stellar magnitude +6, meaning you could hypothetically witness its atmospheric reentry with the naked eye during perfect weather conditions. That said, binoculars will probably increase the odds of seeing its fiery end.

[Related: Some space junk just got smacked by more space junk, complicating cleanup.]

But one toolbag’s atmospheric cremation does very little to solve the ongoing issue of space junk. After years of orbital industry expansion, the planet is surrounded by discarded rocket debris, satellites, and all manner of space travel detritus. It’s getting so bad that a recent project space junk cleanup project was suddenly complicated by its target colliding with another bit of trash.

Thankfully, governmental regulators are taking notice—earlier this year, the FCC issued its first ever space pollution fine to the satellite television provider, Dish Network, for failing to properly decommission one of its satellites last year. No penalties are expected for ISS astronauts Moghbeli and O’Hara; after all, they aren’t the first astronauts to drop the bag, so to speak. In 2008, two ISS astronauts accidentally lost a kit containing “two grease guns, scrapers, several wipes and tethers and some tool caddies.”

Update 11/17/2023 12:20PM : The Virtual Telescope Project has released this image, taken on November 15, 2023. The tool bag is still zooming around the Earth at roughly 17,500 mph until its projected March 2024 deorbit.

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Two of the most powerful space telescopes in the universe have joined forces to showcase a panorama of colorful galaxy clusters about 4.3 billion light-years away from Earth. The image of  galaxy cluster MACS0416 is from NASA’s James Webb Space Telescope (JWST) and the Hubble Space Telescope and combines both visible and infrared light. 

[Related: Euclid telescope spies shimmering stars and galaxies in its first look at the ‘dark’ universe.]

According to NASA, MACS0416 is a pair of colliding galaxy clusters that will eventually combine to form an even bigger cluster. It includes numerous galaxies outside of the cluster and some other light sources that vary over time. The variation is likely due to a phenomenon called gravitational lensing, where light is distorted and amplified from distant background sources.

Color coding

In the image, different colors represent the varying wavelengths of light. The shortest are blue, the intermediate are green, and the longest are red. The wavelengths range from 0.4 to 5 microns and the variation creates a particularly vivid landscape of galaxies.

The colors also give clues to how far away the galaxies are. The bluest galaxies are relatively close, tend to show intense star formation, and are best detected by Hubble. The more red galaxies tend to be further away and are best spotted by JWST. Some of the galaxies also appear very red because they have a large amount of cosmic dust that tends to absorb bluer colors of starlight.

“The whole picture doesn’t become clear until you combine Webb data with Hubble data,” Rogier Windhorst said in a statement. Windhorst is an astronomer at Arizona State University and principal investigator of the PEARLS program (Prime Extragalactic Areas for Reionization and Lensing Science), which took the JWST observations.

Oh Christmas tree

While the images are pleasant to look like, they were also taken for a specific scientific purpose. The team was using their data to search for objects varying in observed brightness over time, known as transients. All of these colors twinkling together in the galaxy look like shining colorful lights on a Christmas tree. 

“We’re calling MACS0416 the Christmas Tree Galaxy Cluster, both because it’s so colorful and because of these flickering lights we find within it. We can see transients everywhere,” said astronomer Haojing Yan of the University of Missouri in Columbia said in a statement. Yan is a co-author of one paper describing the scientific results published in The Astrophysical Journal.

The team identified 14 transients across the field of view. Twelve of the transients were located in three galaxies that are highly magnified by gravitational lensing. This means that they are likely to be individual stars or multiple-star systems that are very highly magnified for a short period of time. The other two transients are located within more moderately magnified background galaxies, so they are likely to be supernovae.

More observations with JWST could lead to finding numerous additional transients and in other similar galaxy clusters. 

Godzilla and Mothra 

One of the transients stood out in particular. The star system is located in a galaxy that existed roughly three billion years after the big bang and is magnified by a factor of at least 4,000. They nicknamed the star system Mothra in a nod to its “monster nature” of being both very bright and magnified. Mothra joins another lensed star the researchers previously identified that they nicknamed “Godzilla.” In Japanese cinema, Godzilla and Mothra are giant monsters known as kaiju.

In addition to the new JWST images, Mothra is also visible in the Hubble observations that were taken nine years ago. According to the team, this is unusual, because a very specific alignment between the foreground galaxy cluster and the background star is needed to magnify a star this much. The alignment should have been eliminated by the mutual motions of the star and the cluster.

An additional object within the foreground cluster could be adding more magnification. 

“The most likely explanation is a globular star cluster that’s too faint for Webb to see directly,” astronomer Jose Diego of the Instituto de Física de Cantabria in Spain said in a statement. “But we don’t know the true nature of this additional lens yet.” Diego is also a co-author of a paper published in the journal Astronomy & Astrophysics that details this finding. 

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If you live in and around Gulkana, Alaska and recently saw some eerie lights in the sky—don’t worry; they were all part of a science experiment. Earlier this week, researchers from the University of Alaska Fairbanks and several other US institutions created artificial auroras by sending radio pulses into the Earth’s ionosphere using HAARP (High Frequency Active Auroral Research Program) transmitters on the ground. The frequencies of these transmissions were between 2.8 and 10 megahertz. 

These transmitters act as heaters that excite the gasses in the upper atmosphere. When the gasses “de-excite,” they produce an airglow between 120 and 150 miles above ground, according to a notice about the project issued by the HAARP team. This is similar to how charged particles from the sun interact with gasses in the upper atmosphere to create natural auroras; the charged particles are steered by the Earth’s magnetic field to the north and south poles to form aurora borealis and aurora australis. Compared to those light displays, the artificial auroras are much weaker. 

So why did the researchers do all this? Studying this artificial airglow may provide insights on what happens when real aurora lights appear.

If you noticed a faint red or green splotch in the sky above Alaska between November 4 and November 8, chances are good that you saw the experiment in progress. HAARP also notes in its FAQ that these ionosphere-heating experiments have no detectable effects on the environment after 10 minutes or so. 

[Related: Why NASA will launch rockets to study the eclipse]

Additionally, the team also wants to understand how these superheated gasses in the ionosphere interact with each other. Insights into these dynamics could inform collision detection and avoidance features for satellite systems. Gathering more intel on auroras and other upper atmosphere phenomena like it can help scientists see how weather and particles from space are interacting with the environment around Earth, and how energy is transferred during these events. 

Disturbing the ionosphere is not the only way to study auroras. Launching rockets into the ionosphere, which sits just at the edge of space, is another popular approach. 

The goal of HAARP is to research the physical and electrical properties of the Earth’s ionosphere as it pertains to surveillance, military and civilian communications, as well as radar and navigation systems. Outside of studying auroras, HAARP has used its antenna array to peer inside a passing asteroid, observe solar storms, and conduct other tests related to space physics. Beyond the Earth, the team’s ambitions extend to the moon and to Jupiter. 

HAARP has had an interesting history. Despite conducting serious science, around 2014, controversy and conspiracy brewed around the program’s mysterious antenna field, then run by the US military, prompting scientists to host open houses with the public explaining what they can and can’t do with their technology. Its image problem remains despite the changes in ownership over the years. 

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What happens to glass if you leave it out in the open for several billion years—but with no air and no running water? We can find the answers to that question by studying naturally occurring glass on the moon. The moon may lack the features that usually weather rocks or minerals on Earth, but that doesn’t make this satellite completely inert. Scientists know that prolonged exposure to radiation leaves a mark on the lunar surface. Now, new research suggests that billions of years of radiation exposure appear to stiffen lunar glass, according to a team who published their work yesterday in the journal Science Advances.

The moon may not seem like an obvious place to find glass. But tiny glass spheroids riddle the lunar regolith—the rock chips and other loose material covering the lunar surface. Meteoroids constantly bombard the material, melting it into tiny pools. As the molten regolith cools back down, it hardens into glass. 

Glass is more than just a brittle, transparent sheet that fills windows. Scientists think of the stuff as the result of a liquid cooling rapidly without its atoms slotting into a defined structure. For that reason, some scientists consider glass to be its own separate state of matter.

And, even on the moon, glass does not last for billions of years without changing. Though the moon has neither a significant atmosphere nor running water to weather rocks like on Earth, the lunar surface is subject to something that our planet’s atmosphere typically filters out: radiation. Some of it comes from the sun; some arrives as cosmic rays from far greater distances. Regardless, over billions of years of radiation exposure, the effects build up.

[Related: Why do all these countries want to go to the moon right now?]

Geologists have long been interested in how radiation affects lunar soil. “There have been 20 years’ worth of study on it,” says Rhonda Stroud, a space materials scientist at Arizona State University, who was not an author of the paper. 

Much of that work involved taking facsimiles of lunar soil, which they call simulants, and exposing them to radiation. But, Stroud says, it’s hard to know how individual material particles react by studying vast quantities of them. “Any one little dust particle or sub-millimeter glass sphere could have its own age,” she says. “Things get buried, the regolith churns.”

Fortunately, we have actual lunar glass on Earth in the form of samples returned by our moon missions. Most recently, we can thank the Chang’e-5 lunar lander, which lifted off from China in November 2020 and returned less than a month later bearing 3.81 lbs of souvenirs. Chang’e-5 did not land in a place on the moon that experienced many impacts—and, consequently did not return with much glass. 

Still, scientists managed to sift through Chang’e-5’s bounty and pick out five particular glassy particles, each one about the width of a human hair. They examined each particle under a transmission electron microscope, allowing them to view its structure. They also pressed a tiny probe on each particle, allowing them to test how the particle reacted to force.

The researchers then “rejuvenated” the samples by heating them up to liquid temperatures of more than 1100 degrees F, holding them there for a minute, then letting them cool. They repeated the same microscope and pressure tests on the de-aged samples, allowing them to estimate what the particles looked like before hundreds of millions or even billions of years sitting on the moon and basking in radiation.

[Related: We finally have a detailed map of water on the moon]

They found a drastic change in a property that engineers call the Young’s modulus, which measures how much force a material needs to distort by a certain length. If the researchers’ rejuvenated samples were any indication, then prolonged radiation exposure increased the Young’s modulus of the glass by as much as 70 percent. More subtly, radiation also seemed to harden some of the particles.

These discoveries can help scientists figure out how glass behaves in the soil of other worlds. And the research team believes that it might also help us understand the behavior of the glass we make on Earth. 

In fact, this paper’s authors believe that lunar glass itself may soon be useful. In their vision, moon-dwellers might sift through the lunar regolith for glass beads and convert them into glass that they could use for their vehicles or habitats.

But it is not obvious to everyone how research like this yet translates into actual infrastructure. “The radiation from solar wind is very, very slow,” Stroud says. “I don’t think we need materials to withstand billions of years.”

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After over half a century of loyal service, the world’s last remaining Super Guppy aircraft continues to dutifully transport NASA’s gigantic rocket parts in its cavernous, hinged cargo bay. On Tuesday, the Huntsville International Airport posted a video and accompanying images to social media of the rotund plane arriving from Kennedy Space Center. Perhaps somewhat unsurprisingly, it sounds like a prop plane of that size can make a huge, rich racket on the tarmac.

[Related: Artemis II lunar mission goals, explained.]

Aboard the over 50-ton (when empty), turboprop plane this time around was the heat shield that protected last year’s Artemis I Orion spacecraft. The vital rocketry component capable of withstanding 5,000 degrees Fahrenheit resided in the Super Guppy’s 25-foot tall, 25-foot wide, 111-foot long interior during a nearly 690-mile journey to the Alabama airport, after which it was transported a few miles down the road to the Marshall Space Flight Center. From there, a team of technicians will employ a specialized milling tool to remove the heat shield’s protective Avcoat outer layer for routine post-flight analysis, according to NASA.

The Super Guppy is actually the third Guppy iteration to lumber through the clouds. Based on a converted Boeing Stratotanker refueling tanker and designed by the now defunct Aero Spacelines during the 1960s, an original craft called the Pregnant Guppy was supplanted by its larger Super Guppy heir just a few years later. This updated plane included an expanded cargo bay, alongside an incredibly unique side hinge that allows its forward section to open like a pocket watch. A final Super Guppy Turbine debuted in 1970, and remained in use by NASA for over 25 years. In 1997, the agency purchased one of two newer Super Guppy Turbines built by Airbus. This Guppy is the current and only such hefty boy gracing the skies. With its bulky profile, the Super Guppy’s travel specs are pretty impressive—it’s capable of flying as high as 25,000 feet at speeds as fast as 250 nautical miles per hour.

[Related: NASA’s weird giant airplane carried the future of Mars in its belly.]

Last PopSci checked in on the Super Guppy’s journeys was back in 2016, when it transported an Orion crew capsule potentially destined for a much further trip than the Artemis missions’ upcoming lunar sojourns—Mars. According to Digital Trends, the Super Guppy’s next flight could occur sometime next year ahead of NASA’s Artemis II human-piloted lunar flyby.

“Although much of the glory of America’s space program may be behind it, the Super Guppy continues to be one of the only practical options for oversized cargo and stands ready to encompass a bigger role in the future,” reads a portion of NASA’s official description.

Until then, feel free to peruse the official, 74-page Super Guppy Transport User’s Guide.

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NASA’s Juno spacecraft has been exploring Jupiter since it arrived at the planet in 2016. In recent years, the mission has turned its attention to the gas giant’s many moons, including the hellish volcanic world Io and the ice ball Europa. Now, in research published in Nature Astronomy, the Juno team revealed new photos of Jupiter’s largest moon, Ganymede, which show evidence of salts and organic compounds. These materials are likely the residue of salty sea water from an underground ocean that bubbled up to the frozen surface of Ganymede. And, excitingly, a salty ocean indicates conditions there might be conducive to life.

Ganymede is a particularly weird place. Not only is it Jupiter’s most massive satellite, it’s the biggest moon in the whole solar system—it’s even larger than the planet Mercury. It also is the only moon to have its own magnetic field, generated from a molten metal core deep in its interior. Like other icy worlds of the outer solar system, such as Europa or possibly Pluto, Ganymede probably has an ocean lurking under its icy crust. Some studies suggest multiple seas, stacked together in a layer cake of ice sheets and oceans, hide underground.

“Because Ganymede is so big, its interior structure is more complicated” than that of smaller worlds, explains University of Arizona geologist Adeene Denton, who is not affiliated with the new work. She notes that the moon’s massive size means there’s a lot of space for interesting molecules to mix about. But that also means they’re tricky to spot, because material must cover a large distance  to get to the surface where our spacecraft can see them.

Juno finally passed close enough to Ganymede—within 650 miles, less than the distance from New York City to Chicago—to take a close look at the chemicals on its surface using its Jovian InfraRed Auroral Mapper (JIRAM). This incredible instrument tracked the composition of Ganymede’s surface in great detail, noting features as small as 1 kilometer wide. If JIRAM were looking at New York City, it would be able to map Manhattan in ten-block chunks.

[Related: Astronomers find 12 more moons orbiting Jupiter]

Importantly, material on the surface of Ganymede might tell us about the water hiding below. If there are salts above, the subsurface ocean might have that same brine. Oceans, including the ones on Earth, acquire their salt from chemical interactions where liquid water touches a rocky mantle. This kind of exchange is “one of the conditions necessary for habitability,” says lead author Federico Tosi, research scientist at the National Institute for Astrophysics in Rome, Italy.

However, other current research suggests that Ganymede doesn’t have a liquid water layer directly touching its mantle. Instead, icy crusts separate the ocean from the rock. But because the team did see these salts in the JIRAM data, it suggests they were touching at one point in the past, if not now. “This testifies to an era when the ocean must have been in direct contact with the rocky mantle,” explains Tosi.

As for the organic chemicals that Juno detected, the team still isn’t completely  sure what flavor of compound they are. They’re leaning towards aliphatic aldehydes, a type of molecule found elsewhere in the solar system that’s known as an intermediate step necessary to build more complex amino acids. These usually indicate liquid water and a rocky mantle are interacting. This definitely isn’t a detection of life, but it’s interesting for the possibility of life lurking in Ganymede’s hidden oceans. “The presence of organic compounds does not imply the presence of life forms,” says Tosi. “But the opposite is true: life requires the presence of some categories of organic compounds.”

[Related: Why a 3,000-mile-long jet stream on Jupiter surprised NASA scientists]

Unfortunately, Juno won’t have a chance to swing by Ganymede again to search for more salty shores—instead, it’s headed toward the explosive Io. The probe’s most recent survey of these minerals was a “a unique opportunity to take a close look at this satellite,” Tosi says. We won’t have to wait too much longer, though, for a second visit. In about ten years, he adds, we’ll get another chance to explore these salty waters with the ESA JUICE mission, “which is expected to achieve complete and unprecedented coverage of Ganymede.”

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Excerpted from A City on Mars: Can We Settle Space, Should We Settle Space, and Have We Really Thought This Through? by Kelly and Zach Weinersmith. Copyright © 2023. Available from Penguin Press, an imprint of Penguin Publishing Group, a division of Penguin Random House.

On Earth, air pushes on your skin from every direction with a consistent pressure of about 14 pounds per square inch, or using ridiculous non-American units, 1 atmosphere. That’s about the weight of 1 liter of water on every square centimeter of your skin. You don’t notice this for the same reason a seabottom shrimp doesn’t notice that the surrounding liquid could implode a submarine—your body is adapted to the pressure near Earth’s surface. It counterbalances the typical push of your surroundings, and you only rarely experience sudden pressure changes. 

But consider a soda. When you buy a sealed bottle of Diet Pepsi, you know it’s full of gas, but you don’t see a lot of bubbles. That’s because the bottle is held at about four times the surface air pressure of Earth, keeping carbon dioxide suspended sedately inside. When you open the top, you expose its contents to Earth’s relatively gentle atmosphere. All that dissolved gas rushes out in the familiar bubbling foam. If you want to avoid the sudden burst of gas, you can always open your bottle forty meters under the sea, where the pressure will keep the gas in place, and the seawater will make the Diet Pepsi taste no worse. 

Your body is like the soda, except that the gas suspended in your fluids is nitrogen, absorbed from the atmosphere. If you were teleported to outer space, where the air pressure level is “none,” your bodily fluids would react like the Diet Pepsi when opened, only instead of a burst of foam, you’d get nitrogen bubbles blocking your veins and arteries, preventing the normal flow of blood, oxygen, and nutrients. This danger is familiar to divers going from low depths back to the surface. If you switch from high to low pressure too quickly, you get “decompression sickness,” colloquially known as “the bends” because it often affects joints, causing the sufferer to bend in agony. If it’s in your lungs, that’s “the chokes.” If it’s in your brain, you’ve got “the staggers.” 

If you’re exposed to space, most likely you’ll just have the death. In fact, the only people who’ve ever died in space were killed by sudden loss of pressure. It was June 30, 1971, and cosmonauts Georgy Dobrovolsky, Vik tor Patsayev, and Vladislav Volkov were returning from Salyut-1. The three cosmonauts spent weeks performing zero gravity acrobatics, televised for the adoring Soviet public. They entered the capsule, and after some brief issues getting the hatch to seal, undocked and began their descent. When the ground crew arrived and the capsule was opened, the men were found, still seated, serene in death. Attempts to revive them proved useless—each had suffered massive brain hemorrhaging. Subsequent investigation determined that when they undocked from their space station, a valve on the return craft had unexpectedly popped open, exposing them to a near-perfect vacuum. 

Decompression sickness isn’t just a danger during accidents; it’s an issue any time you use a pressure suit. You may imagine a space suit as something like bulky clothing, but normal clothing doesn’t have to provide a sealed habitat inside itself. It’d be more accurate to imagine a leather balloon that happens to be shaped like a human. And like a balloon, the higher the internal pressure, the harder it is to bend. In a human-shaped balloon, high pressure means difficulty bending at the joints. Like, a lot of difficulty. A phenomenon called “fingernail delamination” is well documented, and we encourage you not to learn what it is. Thus, although the International Space Station is kept at Earth pressure, both American and Russian space suits only have around one third of that. 

So, why don’t astronauts get bendy, choky, staggery, and deathy when they don space suits? Because they prebreathe pure oxygen before spacewalks, removing most of the nitrogen from their blood. No nitrogen, no nitrogen bubbles. Movies may have led you to believe heroic astronauts can slip on a space suit and leap to the rescue, but under current designs this would result in Brad Pitt clutching his joints and shambling to a very painful (if handsome) death. 

The astute nerd will ask why not just keep the ISS at the same low pressure as the suit. The short answer is that although humans can survive in low pressure as long as there’s enough oxygen floating around, engineers would have to design all equipment to operate in a low-pressure, pure-oxygen environment. 

But pure oxygen is dangerous. In 1967, during prep for the Apollo 1 flight, a spark went off in the crew’s capsule, causing an intense fire in the pure oxygen environment. The three astronauts—Edward White II, Roger Chaffee, and Gus Grissom—could not be rescued, because the sudden increase in temperature and pressure made it impossible to use the inward-opening hatch, while the intense heat prevented rescuers from saving them. 

Less well known is a similar and earlier incident from the Soviet Union. In early 1961, Valentin Bondarenko was training to be a cosmonaut, and one of the training exercises was to spend ten days in a high-oxygen pressurized chamber. Near the end of confinement, he removed a medical sensor from his body and wiped the sticky glue from the sensor off with an alcohol swab. He absent-mindedly threw it aside, where it landed on an electric hot plate. The resulting fire quickly got out of control, consuming his suit. Oxygen had to be bled out of the chamber before rescuers could reach him, and he died of shock soon after. This happened just a month before Gagarin became the first human to reach outer space. The Soviets preferred to keep their failures a secret, and so when the Apollo 15 astronauts left a plaque on the Moon with the names of astronauts and cosmonauts who lost their lives in the race for the Moon, Bondarenko was not included. His story was only finally shared a quarter century after his passing. 

Buy A City on Mars by Kelly and Zach Weinersmith here.

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A very dry start

When the solar system first came together, some of the young planets were too hot for water. “Earth and Mars should have formed extremely dry,” says Humberto Campins, an asteroid expert at the University of Central Florida—due to their locations in the solar system’s frost line.

When the sun was coalescing out of a collapsing cloud of gas and dust 4.6 billion years ago, its tremendous heat made a boundary. Outside of it, space was cool enough for ice grains to solidify. (This helps explain why far-out Jupiter and Saturn have ocean moons.) Inside of it, heat vaporized water. Earth and the other inner planets clumped together from the dry rock and dense metal that remained. Something must have happened, some millions of years later, to nourish those planets with water. Astronomers have explored several possible scenarios. 

Craters on the surface of our moon indicate that our side of the frost line was constantly hit with space rocks, including a particularly violent shower known as the Late Heavy Bombardment. Some experts think those projectiles—specifically meteorites, the bits of asteroids that fall to Earth—might have been more like cosmic water balloons. The hypothesis is supported by the 2010 discovery of a thin crust of frost on asteroid 24 Themis. More recently, NASA found water-bearing clay minerals in the near-Earth asteroid Bennu during a ground-breaking sample-retrieval mission.

Still, it’s possible that other processes were involved in delivering water to Earth, such as gas from the cloudy solar nebula that dissolved hydrogen into the planet’s magma layer. It’s also possible that there were multiple sources and steps.

“The pieces of the puzzle are not clear,” says Campins, who is a member of the team that probed Bennu’s contents. But he points to one major clue that “gives us an idea of where the water may be coming from”: the type of hydrogen that flows through our aquatic systems.

Matching elements

The most common form of hydrogen in the universe has a lone proton orbited by an electron. But there’s a slightly different version called deuterium with a proton and a neutron squished into the center. Astronomers have measured the proportion of deuterium to regular hydrogen in Earth’s water and looked for that “D-H ratio” in other objects around the solar system.

This lends to the idea that a bunch of space bodies hit Earth with noble gasses, H₂O, and who knows what else. “If most of the water gets contributed by asteroid impacts and most of the noble gasses are contributed by comets,” the elemental math seems to add up, Campins says. “But I think that nature is a little bit more complicated than that…it could be that the timing of those two was not the same.” 

In fact, newer evidence emphasizes a different kind of space rock from closer to home.

Local rocks

If space rocks brought water to the Red Planet, could they have done so elsewhere? “What we’re learning here may not only be applicable to our understanding of what we should expect on Mars,” Campins says, “but about the possibility of water and organic molecules being delivered to planets around other stars, which would give you an environment that could be conducive to the formation of life.”

Putting these lines of evidence together gives us a recipe that would have involved lots of damp local rocks and a few of the more distant ice balls. Hydrogen, nitrogen, and zinc isotopes “all tell the same story” of a wet Earth, Raymond says: Previously overlooked non-carbonaceous meteorites probably supplied about 70 percent of the planet’s water, and just a dash of carbonaceous meteorites touched up its vast blue surface. 

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On November 7, the European Space Agency (ESA) released the first five images taken with its premier Euclid space telescope. The images show spiral galaxies, star nurseries, and incredible celestial objects in incredibly sharp detail. 

[Related: Euclid space telescope begins its search through billions of galaxies for dark matter and energy.]

Perseus cluster of galaxies

IC 342 aka the ‘Hidden Galaxy’

Irregular galaxy NGC 6822

[Related: Your guide to the types of stars, from their dusty births to violent deaths.]

Globular cluster NGC 6397

The Horsehead Nebula

Dark matter and dark energy

In July, Euclid launched from Cape Canaveral Space Force Station in Florida. It’s on a mission of studying the mysterious influence of dark matter and dark energy on the universe and mapping one third of the extragalactic sky. According to the ESA, 95 percent of our cosmos appears to be made of these mysterious ‘dark’ entities. But we don’t understand what they are because their presence causes only very subtle changes in the appearance and motions of the things we can see.

“Dark matter pulls galaxies together and causes them to spin more rapidly than visible matter alone can account for; dark energy is driving the accelerated expansion of the Universe. Euclid will for the first-time allow cosmologists to study these competing dark mysteries together,” Carole Mundell, ESA Director of Science, said in a statement. “Euclid will make a leap in our understanding of the cosmos as a whole, and these exquisite Euclid images show that the mission is ready to help answer one of the greatest mysteries of modern physics.”

Euclid will observe the shapes, distances, and motions of billions of galaxies out to 10 billion light-years over the course of the next six years.

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Astronomers have discovered the most distant supermassive black hole ever observed. They had the help of a “cosmic magnifying glass,” or gravitational lensing. This happens when a massive celestial body creates a large curvature of spacetime so that the path of light around it can be bent as if by a lens.

The black hole is located in the galaxy UHZ1 in the direction of the galaxy cluster Abell 2744. The galaxy cluster is about 13.2 billion-years-old. The team used NASA’s Chandra X-ray Observatory and the James Webb Space Telescope (JWST) to find the telltale signature of a growing black hole. It started to form only 470 million years after the big bang when the universe was only 3 percent of its current age of about 13.7 billion years-old. The galaxy is much more distant than the cluster itself, at 13.2 billion light-years from Earth. 

[Related: Gravitational wave detector now squeezes light to find more black holes.]

Astronomers can tell that this black hole is so young because it is so giant. Black holes evaporate over time. Most black holes in galactic centers have a mass that is equal to roughly a tenth of the stars in their host galaxy, according to NASA. This early black hole is growing and as a mass that is on par with our entire galaxy. Astronomers have never witnessed a black hole at this stage before and studying it could help explain how some of the first supermassive black holes in the universe formed. The findings are detailed in a study published November 6 in the journal Nature Astronomy.

“We needed Webb to find this remarkably distant galaxy and Chandra to find its supermassive black hole,” study co-author and astronomer Akos Bogdan said in a statement. Bogdan is affiliated with the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts.

“We also took advantage of a cosmic magnifying glass that boosted the amount of light we detected,” Bogman added. This magnifying effect is known as gravitational lensing. The team took X-ray observations with Chandra for two weeks. They saw intense, superheated X-ray emitting gas—a supermassive black hole’s trademark—from the galaxy. The light coming from the galaxy and the X-ray from the gas around the supermassive black hole were magnified by the hot gas and dark matter coming from the galaxy cluster. This effect was like a “cosmic magnifying glass” and it enhanced the infrared light signals that the JWST could detect and allowed Chandra to see the faint X-ray source.

“There are physical limits on how quickly black holes can grow once they’ve formed, but ones that are born more massive have a head start. It’s like planting a sapling, which takes less time to grow into a full-size tree than if you started with only a seed,” study co-author and Princeton University astronomer Andy Goulding said in a statement. 

[Related: ‘Rogue black holes’ might be neither ‘rogue’ nor ‘black holes.’]

Observing this phenomenon could help astronomers answer how some supermassive black holes can hit enormous masses so soon after the explosion of energy from the big bang. There are two opposed theories for the origin of these supermassive black holes–light seed versus heavy seed. The light seed theory says that a star will collapse into a stellar mass black hole and then grow into a supermassive black hole over time. In the heavy seed theory, a large cloud of gas–not an individual star–collapses and condenses to form the supermassive black hole. This newly discovered black hole could confirm the heavy seed theory. 

“We think that this is the first detection of an ‘Outsize Black Hole’ and the best evidence yet obtained that some black holes form from massive clouds of gas,” study co-author and Yale University theoretical astrophysicist Priyamvada Natarajan said in a statement. “For the first time we are seeing a brief stage where a supermassive black hole weighs about as much as the stars in its galaxy, before it falls behind.”

The team plans to use this and more data coming in from the JWST and other space telescopes to create a better picture of the early universe. 

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On November 3, the Smithsonian’s National Museum of Natural History debuted a piece of the asteroid Bennu to the public for the first time. The sample was deposited on Earth by NASA’s OSIRIS-REx spacecraft on September 24. The spacecraft did not land, but instead dropped a capsule containing about nine ounces of asteroid samples down to Earth. The spacecraft continued on to a new mission called OSIRIS-APEX. It is set to explore the asteroid Apophis when it comes within 20,000 miles of Earth in 2029. 

On display is a 0.3-inch in diameter stone that weighs only 0.005-ounces. The stone was retrieved amidst rocks and dust collected by the spacecraft in 2020 after two years of exploring Bennu. 

[Related: NASA’s first asteroid-return sample is a goldmine of life-sustaining materials.]

OSIRIS-REx stands for Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer and is the first US mission to collect samples from an asteroid. The spacecraft traveled 1.4-billion-miles from Earth, to the asteroid Bennu, and then back again. Bennu is roughly 4.5 billion years old and dates back to the crucial first 10 million years of the solar system’s development. Its age offers scientists a window into what this time period looked like. The space rock is shaped like a spinning top and is about one-third of a mile across at its widest part–slightly wider than the Empire State Building is tall. It revolves around the sun between the orbits of Earth and Mars.

“The OSIRIS-REx mission is an incredible scientific achievement that promises to shed light on what makes our planet unique,” Kirk Johnson, the Sant Director of the National Museum of Natural History, said in a statement. “With the help of our partners at NASA, we are proud to put one of these momentous samples on display to the public for the first time.”

The sample was labeled OREX-800027-0 by NASA scientists at Houston’s Johnson Space Center and is being stored in a nitrogen environment to keep it safe from contamination. CT scans of the displayed stone revealed that it is composed of dozens of smaller rocks. The fragments were fused back together at some point and the entire stone was changed by the presence of water. The alterations to the stone produced clays, iron oxides, iron sulfides, and carbonates as its major minerals and even carbon. 

The samples from this mission hold chemical clues to our solar system’s formation. Evidence of essential elements like carbon in the rocks outside of the main sample container have already been uncovered by NASA scientists. These early samples also contain some water-rich minerals. Scientists believe that similar water-containing asteroids bombarded Earth billions of years ago, which provided the water that eventually formed our planet’s first oceans.

[Related: NASA’s OSIRIS mission delivered asteroid samples to Earth.]

“Having now returned to Earth without being exposed to our water-rich atmosphere or the life that fills every corner of our planet, the samples of Bennu hold the promise to tell us about the water and organics before life came to form our unique planet,” museum meteorite curator Tim McCoy said in a statement. McCoy has worked on the OSIRIS-REx mission for nearly two decades as part of an international team of scientists.

According to Space.com, a sizable crowd turned out to see the space rock and NASA Administrator Bill Nelson and other space agency and Smithsonian officials were present at the unveiling ceremony. Additional Bennu samples will be on display at a later date and at the Alfie Norville Gem & Mineral Museum at the University of Arizona in Tucson and Space Center Houston, next to to NASA’s Johnson Space Center.

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Tired of paying increasingly hefty monthly subscription fees for your streaming services, only to scroll nearly as long as a movie’s runtime just to find something to watch? Well, your choices are only going to expand thanks to NASA’s new streaming channel. But at least when NASA+ launches on November 8, it won’t come with any fees or commercials.

The commercial free on-demand platform will be available via the NASA App on iOS and Android devices, web browsers, as well as through Roku, Apple TV, and Fire TV. The ever-expanding catalog will include live coverage of launch events and missions, original videos, and multiple new series.

[Related: NASA’s first asteroid-return sample is a goldmine of life-sustaining materials.]

“We’re putting space on demand and at your fingertips with NASA’s new streaming platform,” Marc Etkind, NASA Headquarters’ Office of Communications associate administrator, said earlier this year. “Transforming our digital presence will help us better tell the stories of how NASA explores the unknown in air and space, inspires through discovery, and innovates for the benefit of humanity.”

Check out trailers for some of the first series to hit NASA+ this month:

NASA Explorers will offer viewers a multi-episode look at the agency’s recently concluded, seven-year OSIRIS-REx mission. Completed in September, OSIRIS-REx successfully returned samples collected in space from Bennu, a 4.5 billion-year-old asteroid traveling across the cosmos since the dawn of the solar system.

Other Worlds will focus on the latest updates and news from the James Webb Space Telescope (JWST) program. Launched in 2021 following a 17-year-long development on Earth followed by a six-month orbital tune up, the JWST provides researchers with some of the most spectacular glimpses of space ever achieved. Over the course of its decade-long lifespan, the JWST aims to capture information and imagery from over 13.5 billion years ago—when some of the universe’s earliest galaxies and stars began to form.

And for those looking to just bask in cosmic majesty, Space Out will allow viewers to do just that alongside “relaxing music and ultra-high-definition visuals of the cosmos, from the surface of Mars to a Uranian sunset.”

[Related: Moon-bound Artemis III spacesuits have some functional luxury sewn in.]

“From exoplanet research to better understanding Earth’s climate and the influence of the Sun on our planet along with exploration of the solar system, our new science and flagship websites, as well as forthcoming NASA+ videos, showcases our discovery programs in an interdisciplinary and crosscutting way, ultimately building stronger connections with our visitors and viewers,” Nicky Fox, associate administrator of NASA Headquarters’ Science Mission Directorate, said over the summer.

NASA+ comes as the space agency nears a scheduled 2025 return to the lunar surface as part of its ongoing Artemis program. When humans touch down on the moon for the first time in over 50 years, they apparently will do so in style, with both Prada-designed spacesuits and high-tech lunar cameras.

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We may be a spacefaring species, but only a tiny vanguard have actually explored beyond Earth’s atmosphere. Fewer than 700 people have flown in space, and the vast majority of those have been white men with a military background, screened for health and skills. But astronauts’ demographics are rapidly changing. Commercial space companies have sent space tourists on suborbital and orbital space flights, such as the all-civilian men and women of the SpaceX Inspiration 4 mission. Multiple companies plan to launch private space stations after the International Space Station is retired. NASA, meanwhile, has promised that a woman will be the first astronaut to set foot on the moon again when the Artemis III mission lands on the lunar south pole. And, in subsequent missions, the space agency plans to build long-term habitats on the moon. 

With more humans headed to space than ever, there’s an opportunity for all kinds of medical scenarios to crop up—especially those that haven’t occurred among the previous cadre of professional astronauts. Space travelers could have heart attacks, suffer traumatic injuries, or, as a result of one of the most human of activities, become pregnant.  

“It’s not a question of if, but when,” says physician Emmanuel Urquieta, the chief medical officer at the Translational Research Institute for Space Health, or TRISH, at Baylor College of Medicine. The problem, he says, is that the small sample of humans who have flown in space provides very little knowledge of how average body will respond to long-term flights. That goes double for conception, pregnancy, and the delivery of a baby, where there is no human spaceflight data at all. Numerous factors such as low gravity and high radiation are thought to pose risks to the healthy development of a fetus or the birth of a child. 

[Related: Space changes your brain in bigger ways than we thought]

These aren’t simply academic gaps to fill. “If we’re planning to develop habitation capabilities, and off-Earth colonies on the moon and Mars, this is something that will absolutely need to be solved,” Urquieta says. 

Scientists have just completed a very basic start. One new study published in the journal iScience by researchers at the Japan Aerospace Space Agency, JAXA, and the Japan Aerospace Space Agency may provide optimistic, if provisional, evidence that pregnancy in space is possible. At least, for mice. 

In August 2021, the research team sent frozen mouse embryos to the ISS, where, once thawed, they developed in the space station’s microgravity environment. After the embryos were returned to Earth about a month later, the study authors found that the small clusters of cells grew as normal. Each embryo formed two cellular structures known as a blastocyst and an inner cell mass; if allowed to develop further, those would go on to become the placenta and fetus, respectively. The researchers had worried that without gravity, the inner cell mass would not be able to coalesce in one space within the blastocyst. 

The research is another piece of evidence that mammalian fertility works in the conditions of spaceflight. Past experiments have shown that mouse sperm flown in space produced viable offspring when returned to Earth. Although there is a large gap between this early stage of embryonic development and birth of a healthy animal, the study team plans to conduct such a test in the future. 

And, of course, this finding was in mice. Urquieta cautions that it’s hard to tell how mouse results translate to human health even when experiments take place within Earth’s normal gravity. “A general challenge in human spaceflight is that a lot of the research that we have is from animal models,” he says. ”How much of those results could be extrapolated to humans still remains a question.”

[Related: What happens to your body when you die in space?]

Even if a fetus can develop in space, several key challenges must be addressed for a human mother off Earth. The first is nutrition, because pregnant people need sufficient protein and levels of folic acid to support a healthy fetal development. “Providing macro and micronutrients in spaceflight is going to be challenging,” Urquieta says, in a space station environment where fresh foods are in short supply. Lunar or Mars colonies probably won’t even have the luxury of regular deliveries from Earth. 

Then there’s radiation. Not all the mouse embryos developed successfully in the new study, and the researchers suspect that radiation could be the cause. “We know that radiation is very damaging in general to cells, and especially during the first three or four weeks of pregnancy,” Urquieta says. The ISS orbits low enough that it’s shielded by Earth’s magnetosphere, he says, but on the moon or a trip to Mars, the full brunt of galactic cosmic radiation could become a problem. 

Being pregnant on Earth isn’t a garden stroll, either, and it would probably be even less comfortable in space. Certain well-documented physiological changes in microgravity include shifting bodily fluids in for instance, with blood collecting in the head and overall blood volume decreasing. “There’s also space motion sickness, nausea, and vomiting. We know that that is also something common in pregnancy,” Urquieta says. “It would definitely exacerbate the non-pleasant symptoms.” 

Ultimately, he says, he researchers who study reproduction in space need to think about crawling before they walk—finding general solutions for astronaut radiation exposure and nutritional needs at lunar bases before tackling the specific requirements of pregnant astronauts. But given the likely inevitability of human space pregnancies, he says, “I think it’s important we start the conversations, and also increase awareness that this is going to be a very, very complex and challenging issue to solve.” 

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There’s an aviation term called the “death spiral”—when pilots’ skewed sensory perceptions contradict the accurate readings on their instruments, causing confusion and leading to bad course corrections. As the name implies, this often leads to tragic consequences—many experts believe such an issue contributed to John F. Kennedy, Jr.’s fatal crash in 1999, as well as the 1959 tragedy that killed Buddy Holly, Ritchie Valens, and The Big Bopper. Disorientation was also one of the causes in the 2021 helicopter crash that claimed Kobe Bryant’s life.

[Related: How pilots end up in a ‘death spiral’ ]

Such a scenario is terrifying enough on its own—but imagine a similar situation while floating in the vacuum of space. With no gravitational pull and few, if any, points of reference, working in such an environment could quickly become disorienting and potentially dangerous as astronauts lose their sense of direction.

Although NASA astronauts receive copious training to guard against spatial disorientation, the issue is still a huge concern, especially as private companies increasingly expand their own projects with both space tourism and governmental contracts. Thanks to a team of researchers, however, wearable sensors enhanced by vibrotactile feedback might one day help keep astronauts feeling grounded.

[Related: This US astronaut will have spent an entire year in orbit.]

“Long duration spaceflight will cause many physiological and psychological stressors which will make astronauts very susceptible to spatial disorientation,” Vivekanand P. Vimal, a research scientist at Brandeis University’s Ashton Graybiel Spatial Orientation Lab, explained in a recent profile. “When disoriented, an astronaut will no longer be able to rely on their own internal sensors which they have depended on for their whole lives.”

To explore these issues, Vimal and their colleagues conducted a series of trials involving 30 participants. The team taught 10 of them to treat their vestibular senses (which pick up onwhere they are in space and where they are going) with skepticism. Another 10 volunteers received the same training alongside the addition of vibrotactors—devices attached to their skin that buzz depending on their geospatial positioning. The final 10 participants only received the vibrotactors with no training whatsoever. Subjects then wore blindfolds and earplugs while white noise played in the background, and took their place inside an intentionally disorienting “multi-axis rotation device” (dubbed MARS).

Similar to an inverted pendulum, MARS first rotated upright subjects from side-to-side around a central axis to act as an analog to everyday gravitational cues on Earth. Subjects then used two joysticks to attempt to remain stabilized without swinging into either side’s crash boundary. A second phase involved the same parameters, but with the cockpit shifted on a horizontal angle (with the participants facing the ceiling) to better approximate a space environment without Earth’s gravitational reference points. Throughout each subject’s 40 trials, vibrotactors on 20 of the 30 participants buzzed if they shifted too far from a central balancing point, thus potentially queuing them to correct their position with their joysticks.

Vimal, alongside co-authors Alexander Sacha Panic, James R. Lackner, and Paul DiZio, published the results in a new study published on November 3 with Frontiers in Physiology. According to the team’s findings, all participants first felt disoriented during the analog tests due to conflicting input from their vestibular systems and vibrotactors. Those with prior training with their sensors performed best during the space phase, while training-only participants without the wearables “crashed” more often. This third group also accidentally destabilized themselves more frequently than the other two. However, the subjects performed far better while situated in the Earth analog position, with or without the vibrotactors’ aid—Vimal’s team suspects the devices may have been too weak, or participants needed more time to adjust to the devices. 

[Related: ISS astronauts are building objects not possible on Earth.]

With further testing and refinement, Vimal’s team believes engineers could integrate similar wearables into astronauts’ suits to provide orientation aid, both inside spacecraft and outside space stations. They may be small additions, but they are some that could save explorers from some very serious, scary, and possibly even fatal circumstances.

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The freshly released images from NASA’s Lucy spacecraft’s first asteroid flyby reveal that Dinkinesh is actually a binary pair. A binary asteroid pair has a larger main asteroid and a smaller satellite orbiting around it. In the weeks leading up to the flyby, the Lucy team had wondered if Dinkinesh was actually a binary system because Lucy’s instruments detected the brightness of the asteroid changing over time. This is a sign that something is getting in the way of the light, likely a body orbiting the main space rock. 

[Related: NASA spacecraft Lucy says hello to ‘Dinky’ asteroid on far-flying mission.]

From a preliminary analysis of the first available images, the team estimates that the larger asteroid body is roughly 0.5 miles at its widest and that the smaller body is about 0.15 miles in size.

Dinkinesh is another name for the Lucy fossil that this mission is named after. The 3.2 million-year-old skeletal remains of a human ancestor were found in Ethiopia in 1974. The name Dinkinesh means “marvelous” in the Amharic language. 

“Dinkinesh really did live up to its name; this is marvelous,” Hal Levison, Lucy principal investigator from the Southwest Research Institute, said in a statement. “When Lucy was originally selected for flight, we planned to fly by seven asteroids. With the addition of Dinkinesh, two Trojan moons, and now this satellite, we’ve turned it up to 11.”

The November 1 encounter primarily served as an in-flight test of the asteroid-studying spacecraft. It specifically focused on testing the system that allows it to autonomously track an asteroid as it whizzes by at 10,000 miles per hour. The team calls this its terminal tracking system.

“This is an awesome series of images. They indicate that the terminal tracking system worked as intended, even when the universe presented us with a more difficult target than we expected,” Lockheed Martin guidance and navigation engineer Tom Kennedy said in a statement. “It’s one thing to simulate, test, and practice. It’s another thing entirely to see it actually happen.”

It will take up to a week for the remainder of the data from the flyby to be downloaded to Earth. This week’s encounter was carried out as an engineering check, but the team’s scientists are hoping this data will help them glean insights into the nature of small asteroids.

“We knew this was going to be the smallest main belt asteroid ever seen up close,” NASA Lucy project scientist Keith Noll said in a statement. “The fact that it is two makes it even more exciting. In some ways these asteroids look similar to the near-Earth asteroid binary Didymos and Dimorphos that DART saw, but there are some really interesting differences that we will be investigating.”

[Related: Why scientists are studying the clouds of debris left in DART’s wake.]

The Lucy team plans to use this first flyby data to evaluate the spacecraft’s behavior and  prepare for its next close-up look at an asteroid. This next encounter is scheduled for April 2025, when Lucy is expected to fly by the main belt asteroid 52246 Donaldjohanson. This asteroid is named after American paleoanthropologist Donald Johnson, one the scientists who discovered the Lucy fossils.

Launched in October 2021, NASA’s Lucy mission is the first spacecraft set to explore the Trojan asteroids. This group of primitive space rocks is orbiting our solar system’s largest planet Jupiter. They orbit in two swarms, with one moving  ahead of Jupiter and the other lagging behind it. 

There are about 7,000 asteroids in this belt, with the largest asteroid estimated to be about 160 miles across. The asteroids are similar to fossils and represent the leftover material that is still hanging around after the giant planets including Saturn, Jupiter, Uranus, and Neptune formed.

Lucy will then travel into the leading Trojan asteroid swarm. After that, the spacecraft will fly past six Trojan asteroids, including binary asteroids like Dinkinesh: Eurybates and its satellite Queta, Polymele and its yet unnamed satellite, Leucus, and Orus. 

In 2030, Lucy will return to Earth for yet another bump that will gear it up for a rendezvous with the Patroclus-Menoetius binary asteroid pair in the trailing Trojan asteroid swarm. This mission is scheduled to conclude some time in 2033.

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On November 1, NASA’s Lucy spacecraft successfully completed its first asteroid flyby. The 56 feet-long spacecraft came within 230 miles of the asteroid Dinkinesh aka “Dinky.” This fairly small space rock is in the main asteroid belt between Mars and Jupiter. 

[Related: Meet Lucy: NASA’s new asteroid-hopping spacecraft.]

Dinkinesh is the first of 10 asteroids the probe will visit over the next 10 years. The asteroid is about 10 to 100 times smaller than the Jupiter Trojan asteroids that are the main target of the Lucy mission. Dinkinesh is another name for the Lucy fossil that this mission is named after. The 3.2 million-year-old skeletal remains of a human ancestor were found in Ethiopia in 1974.

Lucy zoomed by Dinkinesh at about 10,000 miles per hour.  This encounter was the first in-flight test of the spacecraft’s terminal tracking system. 

“The Lucy operations team has confirmed that NASA’s Lucy spacecraft has phoned home after its encounter with the small main belt asteroid, Dinkinesh,” NASA wrote in a blog post. “Based on the information received, the team has determined that the spacecraft is in good health and the team has commanded the spacecraft to start downlinking the data collected during the encounter.”

It will take NASA up to a week to download the data on how Lucy performed during this first in-flight test during the encounter. NASA planned for the high-resolution grayscale camera onboard Lucy to take a series of images every 15 minutes. Dinkinesh has been visible to Lucy’s Long Range Reconnaissance Imager (L’LORRI) as a single point of light since early September. The team began to use L’LORRI to assist with the navigation of the spacecraft. 

Lucy’s thermal infrared instrument (L’TES) should also begin to collect data. Since L’TES was not designed to observe an asteroid quite as small as Dinkinesh, the team is interested to see if it can detect the half-mile wide asteroid and measure its temperature during the encounter.

Astronomers plan to use the data from this approach to gain a better understanding of small near-Earth asteroids and if they originate from larger main belt asteroids. 

Launched in October 2021, NASA’s Lucy mission is the first spacecraft set to explore the Trojan asteroids. These are a group of primitive space rocks orbiting our solar system’s largest planet Jupiter. They orbit in two swarms, with one ahead of Jupiter and the other lagging behind it. Lucy is expected to provide the first high-resolution images of what these space rocks look like. 

There are about 7,000 asteroids in this belt with the largest about 160 miles across. The asteroids are similar to fossils and represent the leftover material that is still hanging around after the giant planets including Uranus, Neptune, Jupiter, and Saturn formed.

[Related: New image reveals a Jupiter-like world that may share its orbit with a ‘twin.’]

In 2024, Lucy will return towards Earth for a second gravity push that will give it the energy needed to cross the solar system’s main asteroid belt. It is expected to observe asteroid 52246 Donaldjohanson in 2025. This asteroid is named after American paleoanthropologist Donald Johnson, one the scientists who discovered the Lucy fossils.

It will then travel into the leading Trojan asteroid swarm. After that, the spacecraft will fly past six Trojan asteroids: Eurybates and its satellite Queta, Polymele and its yet unnamed satellite, Leucus, and Orus. 

In 2030, Lucy will return to Earth for yet another bump that will gear it up for a rendezvous with the Patroclus-Menoetius binary asteroid pair in the trailing Trojan asteroid swarm. This mission is scheduled to end some time in 2033.

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In the summer, astronomers spotted an airplane-sized asteroid—large enough to potentially destroy a city—on an almost-collision course with Earth. But no one saw the space rock until two days after it had zoomed past our planet. 

This asteroid, named 2023 NT1, passed by us at only one-fourth of the distance from Earth to the moon. That’s far too close for comfort. Astronomers weren’t going to let this incident go without a post-mortem. They’ve recently dissected what went wrong and how we can better prepare to defend our planet from future impacts, in a new paper recently posted to the preprint server arXiv.

We know from history that asteroids can cause world-shattering events and extinctions—just look at what happened to the dinosaurs. The study team estimated that, if NT1 hit Earth, it could have the energy of anywhere from 4 to 80 intercontinental ballistic missiles. “2023 NT1 would have been much worse than the Chelyabinsk airburst,” says University of California, Santa Barbara astronomer Philip Lubin, a co-author on the new work, referring to the meteor that exploded over a Russian city in 2013. As devastating as that would be, it’s “not an existential threat like the 10-kilometer hit that killed our previous tenants,” he adds.

The asteroid-monitoring system ATLAS, the “Asteroid Terrestrial-impact Last Alert System”—four telescopes in Hawaii, Chile, and South Africa—discovered NT1 after the rock flew by. ATLAS’s entire purpose is to scour the skies for space rocks that might threaten Earth. So with this set of eyes on the sky, how did we miss it? 

It turns out that Earth has what Brin Bailey, UC Santa Barbara astronomer and lead author on the paper, calls a “blindspot.” Any asteroid coming from the direction of the sun gets lost in the glare of our nearest star.” There’s another way for asteroids to sneak up on us, too: the smaller the asteroid, the harder it is for our telescopes to spot them, even when the rocks come from parts in the sky away from the sun.

[Related: NASA’s first asteroid-return sample is a goldmine of life-sustaining materials]

“Currently, there is no planetary defense system which can mitigate short-warning threats,” Bailey says. “While NT1 has no chance of intercepting Earth in the future, it serves as a reminder that we do not have complete situational awareness of all potential threats in the solar system,” they add. That leads to Lesson #1: We simply need better detection methods for planetary defense. 

If we can manage to detect an asteroid with a few years’ warning, we might be able to redirect it with the technology recently tested by NASA’s Double-Asteroid Redirection Test (DART) mission.For a case with very little warning, such as NT1, though, we’d need a different approach—that’s Lesson #2. Bailey and colleagues propose a method they call “Pulverize It” (PI). 

PI’s plan is exactly what it sounds like: break the asteroid into tiny pieces, small enough to burn up in the atmosphere or fall to the ground as much less dangerous little rocks. They’d do this by launching one or multiple rockets to send arrays of small impactors to space. The impactors—six-foot-long, six-inch-thick rods—would smash into the asteroid like buckshot, efficiently dismantling it. “Had we intercepted it [NT1] even one day prior to impact, we could have prevented any significant damage,” claims Lubin.

It sounds simple enough, but some astronomers aren’t quite convinced. “I think the PI method is impractical even though it does not violate the laws of physics,” says University of California, Los Angeles astronomer Ned Wright, who was not involved in the new work. “When a building is demolished by implosion using explosive charges, a weeks-long testing and planning phase is needed in order to place the charges in the right locations and set up the proper timing. The PI method seeks to do this measuring, planning, and placing the explosives all within a period of 1 minute or so just before the spacecraft hits the asteroid.”

[Related: NASA’s first attempt to smack an asteroid was picture perfect]

Lubin points out that unlike a careful demolition on Earth, the goal is a sudden, bomb-like explosion—an event that needs less prep to pull off. But whether we use PI or another line of defense, it’s clear that we need to plan ahead. Not only is there the hazy threat of an asteroid coming out of nowhere, there are two specific, extremely risky events headed our way: asteroid Apophis’ near flyby in 2029, and close approaches from the even larger Bennu (recently sampled by NASA’s OSIRIS-REx mission) in 2054, 2060, and 2135.

“Humanity now possesses the technology to robustly detect and defend the planet if we choose to do so,” says Lubin. “And a variety of people are working hard to ensure we can.”

This story has been updated: An earlier version indicated that the asteroid-destroying impactors would be filled with explosives. While that may be an option, most forms of the “Pulverize It” method use non-explosive metal rods.

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Sometimes, amazing science happens in the background with little to no public attention. All those years of hard efforts and incremental progress are left unseen except by those living and working through it. Now, a new book detailing the making of the James Webb Space Telescope (JWST) aims to change that by sharing photographs, diagrams, and behind-the-scenes information of the science and pioneers behind the project. 

Inside the Star Factory: The Creation of the James Webb Space Telescope, NASA’s Largest and Most Powerful Space Observatory gives us a full-body summary of an astronomical feat that required more than 100 million hours of labor over the course of 30 years. It covers everything from the initial conception of the idea to the Christmas Day launch in 2021, providing a robust picture of what went into designing, engineering, and testing such a masterpiece. Science writer Christopher Wanjek provides an in-depth overview of the history of JWST, but even more, the book serves as an “illustrated guide [that] shows readers the heady world of scientific discovery at the very limits of human knowledge.”

All of the 100-plus images of the telescope’s construction were taken by Chris Gunn, who joined the project 15 years ago and was the only photographer given such extensive access to the development and launch of JWST. Over his long career, he’s focused on creating intricate images and videos related to science and technology, with previous experience capturing the last servicing mission to the Hubble Space Telescope. His work puts faces to NASA’s biggest telescope endeavor, humanizing the entire assignment and showcasing those who dedicated so much of their time to a single goal. 

We had a chance to speak with Gunn about his new book to find out more about his process and experience. Here’s what he revealed. 

PopSci: How did you get involved with NASA and JWST? 

Gunn: I worked as a photographer on the last servicing mission to Hubble from 2006 to 2009. When that mission ended, I was asked to join the JWST team. I had never imagined being on such a long-term project. 

PopSci: What was the most challenging part about photographing the project? 

Gunn: The most challenging part about photographing this project was also the most exciting: the constantly evolving subject. Seeing parts of the observatory come together was amazing, but the trick was to keep a consistent look and feel in my photographs throughout the project. I started to pay more attention to the environments that I was shooting and bring elements of these environments into my compositions. When I could light my subjects, I took great care to do it subtly. Eventually, I realized that JWST’s geometry photographed beautifully but any distortion ate away at that beauty. Over time I became a more selective shooter with more restraint. 

PopSci: What’s your favorite moment (or moments) from your time with the team? 

Gunn: My favorite moments include the arrival of the first mirrors, the first time I saw the optical system deployed inside of NASA Johnson’s test chamber, and the mating of the optical system to the sunshield and main spacecraft bus. During each of these project milestones the cleanrooms were filled with a sense of awe and wonder. They aren’t particularly noisy in general, but they were super quiet for these moments. I had a sense that I was witnessing something great that humankind was achieving. 

PopSci: What were your go-to cameras and lenses? 

Gunn: One of the most interesting things about being on such a long-term project is seeing the progression in photographic technology as the years passed. I initially shot with Nikon’s D3s and D3X cameras, and finally settled on D4s for several years. Nikon’s 14-24mm 2.8 lens was my favorite lens early on. 

After the observatory was built, I switched to a medium-format Hasselblad-H camera boasting 50 megapixels. The Hassy gave me more resolution, and more importantly, allowed me to shoot with less distortion. Later in the project I acquired a mirrorless Hasselblad, which I used with adapted H lenses. The Hasselblad 50mm was probably my favorite lens as it offered a sharp, undistorted, and wide perspective. The medium format cameras also forced me to slow down and concentrate on composition. 

PopSci: Do you have a no. 1 photograph from the series? 

Gunn: I have quite a few favorites—they’re all in the book. If I had to choose one, it’s the image used for the cover. It was made at the tail end of a long day and depicts the one and only time that the secondary mirror was deployed using the flight motors. That’s the smaller mirror in the center. The center section of the primary mirror reflects the secondary mirror, and you can see the primary mirror in this reflection. Look closely and you also can see me in this reflection. The selfie was unintentional.

Buy Inside the Star Factory: The Creation of the James Webb Space Telescope, NASA’s Largest and Most Powerful Space Observatory here.

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As the darkest nights of the year approach in the Northern Hemisphere, the night skies will light up, giving us a chance to see three meteor showers. Our closest planetary neighbor Venus will also be particularly radiant this month. It is also the time of year to keep an eye out for the Aurora Borealis. Here are some of the events to look out for this month. If you happen to get any stellar sky photos, please tag us and include #PopSkyGazers.

[Related: Astronomers find 12 more moons orbiting Jupiter.]

November 2 to 3 – Jupiter at Opposition

The month kicks off with our solar system’s largest planet appearing at its biggest and brightest state of the year, which is called opposition. Jupiter hits opposition at 12 a.m. EDT on November 3 and will be visible in the eastern horizon for skygazers in the Northern Hemisphere. 

According to Larry Wassterman from the Lowell Observatory in Arizona, opposition occurs when a planet, Earth, and the sun lie along a straight line with Earth in the middle. The planet and the sun are on the opposite sides of Earth so they are considered in opposition. 

“The planet is as close to the Earth as possible and will appear as big and as bright as it can ever get. This is a great time to take a look and discover Jupiter in opposition for yourself. During Jupiter’s opposition, Earth will pass between Jupiter and the Sun, and the proximity will make Jupiter appear larger in the sky. On the day of opposition, Jupiter rises when the Sun sets,” Wassterman writes. 

November 5 and 6 – Southern Taurids Meteor Shower Predicted Peak 

November’s first meteor shower is predicted to peak November 5th and 6th. Both of the Taurids meteor showers don’t have very definite peaks. The meteors ramble along in space and are especially noticeable from late October into early November, when both the Southern and Northern Taurids overlap. 

According to EarthSky, under dark skies with no moon, both South Taurids produce about five meteors per hour and 10 total when the North and South Taurids overlap. Fireballs are also possible, like the ones that appeared in 2022. Taurid meteors are slower than those from other meteor showers, but can be very bright.  

The Taurids are visible almost everywhere on Earth, except for the South Pole. 

[Related: Meteorites older than the solar system contain key ingredients for life.]

November 9 – Moon and Venus Conjunction

Already the brightest planet in our solar system, Venus will shine particularly brilliantly early this month. Venus will put on a show in the eastern horizon at 2:55 AM EST. As the morning continues Venus will shift upwards, and be one teach one degree to the upper right by the time morning twilight begins at about  5:44 a.m. EST. For some viewers, the moon will pass in front of Venus, blocking it from view at this time. 

Visibility will be best in northern Canada, most of Greenland, Iceland, Svalbard, west Russia, most of Europe, parts of north Africa, and most of the Middle East.

November 11 through 13 – Northern Taurids Meteor Shower Predicted Peak

Due to the moon’s phases, the best chance for seeing the Northern Taurids this month is from November 11 through the 13. Ideal viewing times will be around midnight because the moon will only be about 2 percent full that night. The sky will be darker and more primed for you to spot any meteors under clear skies.

November 18 – Leonids Meteor Shower Predicted Peak

For the Leonids, the night sky will be free of moonlight when the shower is predicted to peak on November 18th. For best viewing, watch late on the night of November 17 until dawn on November 18. The morning of November 17 may also be worthwhile for viewing. It is possible to see 10 to 15 Leonid meteors per hour under a moonless sky. 

The Leonid meteor shower is famous for producing one of the greatest meteor storms in living history. On November 17, 1966, there were thousands of meteors per minute during a 15-minute span. Leonid meteor storms sometimes happen in cycles of 33 to 34 years, but this cycle did not occur during the 1990s as anticipated. 

The Leonids will be visible in both hemispheres.

[Related: The moon is 40 million years older than we thought, according to crystals collected by Apollo astronauts.]

November 27 – Full Beaver Moon

November’s full moon will reach peak illumination on November 27 at 4:16 a.m. EST. The moon will also appear very full and close on the night of November 26. According to the Farmer’s Almanac, it is called the Beaver Moon in reference to the time of year when beavers begin to shelter in their lodges, after storing up food for the winter. This was also when beavers pelts are at their thickest.

Some other names for November’s full moon include the Whitefish Moon or Adikomemi-giizis in Anishinaabemowin (Ojibwe), the Little Winter Moon or Gahsá’kneh in Seneca, and the Leaf Fall Moon or Yapa Huktugere Nuti in the Catawba language.

The same skygazing rules that apply to pretty much all space-watching activities are key this month: Go to a dark spot away from the lights of a city or town and let the eyes adjust to the darkness for about a half an hour. 

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For the first time, astronomers using data from the Keck II telescope have detected the presence of an infrared aurora on the planet Uranus. The discovery could shed light on some of the unknown properties of the magnetic fields of our solar system’s planets. It could also help explain why a planet so far from the sun is hotter than it should be. The findings are described in a study published on October 23 in the journal Nature Astronomy. 

[Related: Uranus got its name from a very serious authority.]

The NIRSPEC instrument (Near InfraRed SPECtrograph) at the Keck Observatory in Hawaii  was used to collect 6 hours of observations of Uranus in 2006. The study’s authors carefully studied 224 images to find signs of a specific particle–ionized triatomic hydrogen or H3+. They found evidence of H3+ in the data after collisions with charged particles. The emission created an infrared auroral glow over Uranus’ northern magnetic pole. The image itself is an artist’s rendition of the infrared aurora, superimposed on a Hubble Space Telescope image of Uranus.

Uranian auroras vs. Earth auroras

Auroras on the planet Uranus are caused when charged particles from the sun interact with the planet’s magnetic field the same way they do on Earth. The particles are funneled along magnetic field lines toward the magnetic poles. When they enter the Uranian atmosphere, the charged particles bump into atmospheric molecules. This causes the molecules to glow. 

The dominant gasses in Uranus’ atmosphere are hydrogen and helium and they are at much lower temperatures than on Earth. The presence of these gasses at these temperatures cause Uranus’ auroras to predominantly glow at ultraviolet and infrared wavelengths. By comparison, auroras on Earth come from oxygen and nitrogen atoms colliding with the charged particles and the colors are mostly blue, green, and red and can generally be seen with the human eye at the right latitudes. 

Uranus and Neptune are unusual planets in our solar system because their magnetic fields are misaligned with the axes in which they spin. Astronomers haven’t found an explanation for this, but clues could lie in Uranus’s aurora. 

Measuring the infrared

In the study, a team of astronomers used the first measurements of the infrared aurora at Uranus since investigations into the planet began in 1992. The ultraviolet aurorae of Uranus was first observed 1986, but the infrared aurora has not been observed until now, according to the team. 

By analyzing specific wavelengths of light emitted from the planet. With this data, they can analyze the light called emission lines from these planets, which is similar to a barcode. In the infrared spectrum, the lines emitted by the H3+ particles will have different levels of brightness depending on how hot or cold the particle is and how dense this layer of the atmosphere is. The lines then act like a thermometer taking the planet’s temperature.

The astronomers found that there were distinct increases in H3+ density in Uranus’s atmosphere with little change in temperature. This is consistent with ionization that is caused by the presence of an infrared aurora. These measurements can help astronomers understand the magnetic fields on the other outer planets in the solar system. They could also scientists identify other planets that are suitable for supporting life.

[Related: Ice giant Uranus shows off its many rings in new JWST image.]

“The temperature of all the gas giant planets, including Uranus, are hundreds of degrees Kelvin/Celsius above what models predict if only warmed by the sun, leaving us with the big question of how these planets are so much hotter than expected? One theory suggests the energetic aurora is the cause of this, which generates and pushes heat from the aurora down towards the magnetic equator,” study co-author and University of Leicester PhD student Emma Thomas said in a statement. 

Clues to life on exoplanets

According to Thomas, most of the exoplanets astronomers have discovered are in the sub-Neptune category, so they are a similar size as Neptune and Uranus. Similar magnetic and atmospheric characteristics could also exist on these exoplanets. Uranus’s aurora directly connects to the planet’s magnetic field and atmosphere, so studying it can help astronomers make predictions about the atmospheres and magnetic fields and their suitability for supporting life.

These results may also provide insight into a rare phenomenon on Earth called geomagnetic reversal. This occurs when the north and south poles switch hemisphere locations. According to NASA, pole reversals are pretty common in Earth’s geologic history and the last one occurred roughly 780,000 years ago. Paleomagnetic records show that over the last 83 million years, Earth’s magnetic poles have reversed 183 times. They’ve also reversed at least several hundred times in the past 160 million years. The time intervals between these reversals have fluctuated, but average about 300,000 years.

“We don’t have many studies on this phenomena and hence do not know what effects this will have on systems that rely on Earth’s magnetic field such as satellites, communications and navigation,” said Thomas. “However, this process occurs every day at Uranus due to the unique misalignment of the rotational and magnetic axes. Continued study of Uranus’s aurora will provide data on what we can expect when Earth exhibits a future pole reversal and what that will mean for its magnetic field.”

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The Indian Space Research Organization, or ISRO, is on a roll. India’s national space agency accomplished the first ever landing of a spacecraft, the Vikram lander, near the lunar south pole on August 23. On September 2, ISRO launched Aditya-L1, the agency’s first solar probe. 

And on October 21, ISRO completed a successful launch abort system test for the Gaganyaan, a spacecraft India hopes will carry three national astronauts around Earth on an orbital mission by 2026. That’s an ambitious leap from uncrewed space missions, but if India succeeds, it will join a club of just three other nations that have sent their own astronauts and craft to space—Russia, the US, and China. 

“India is the most impressive, exciting space story of the year,” says Rich Cooper, vice president of communications and outreach for the Space Foundation, a nonprofit that promotes space industry and exploration. “In a year full of a lot of accomplishments, India has more than put itself on the map.”

India’s space program goes back decades. ISRO launched its first satellite, Rohini-1, into orbit on a rocket of Indian manufacture in 1980. The agency became known for launching satellites, and later more distant space missions—such as the Mangalyaan Mars orbiter launched in 2013—under disciplined budgets. ISRO also plans to send an orbiter to Venus in 2025, and a second Mars orbiter to the Red Planet in 2024.

[Related: Meet the first 4 astronauts of the ‘Artemis Generation’]

“The Indian space program has been under the radar, I think, because it has always operated well, but with lower stakes and lower budget,” says Laura Forczyk, a space industry analyst and founder of the consultancy company Astralytical. But IRSO’s ambitions are clearly and justifiably ramping up in the wake of the Vikram landing, she says, as “successfully landing a lander and a rover on the moon is something that very few countries in the world have ever done.”

And even those countries that have done it before sometimes stumble: in 1957 Russia placed the first satellite, Sputnik, in orbit, and four years later sent the first human, Yuri Gagarin, to space. But in 2023, around the same time India was celebrating the Vikram success, Russia failed to make a soft landing on the moon with its Luna 25 mission. 

India’s progress hasn’t been in a vacuum—it’s been studying the successes and failures of Russia, US, and China’s space programs since the beginning, according to Cooper. “There are 60-plus years of human spaceflight lessons to learn, and India has been a marvelous student at looking at those lessons,” he says. “They more than did their homework.”

The Gaganyaan program plans to proceed similarly to NASA’s Artemis program, with multiple system and spacecraft tests before the first human climbs aboard a rocket. The first uncrewed test flight, Gaganyaan 1, is scheduled for sometime in 2024, and a second Gaganyaan 2, is scheduled for 2025. 

[Related: Why do all these countries want to go to the moon right now?]

Gaganyaan 3, in 2026, aims to put a trio of Indian astronauts in orbit around Earth for three days. From there, ISRO hopes to build a space station by 2035, and send Indian astronauts to the moon by 2040. That’s a familiar expansion method, according to University of North Dakota space studies professor Michael Dodge, as it was proposed by Werner von Braun, the Nazi rocket scientist who became the architect of NASA’s Apollo program. “This is a strategy that has been around for a very long time, historically speaking, and it looks like India is pursuing that in a very sort of systematic way,” Dodge says. 

Whether India’s timeline for growing its space program will hold is another question. Forczyk notes that Gaganyaan 1 was supposed to launch in 2020, but faced delays both from COVID-19 and those typical of a complicated human spaceflight program. It may take ISRO more time and money than they expect, and she thinks the launch of Gaganyaan 1 will likely slip into 2025. 

But a crewed mission by 2026? “I think that’s completely feasible,” Forczyk says. As Russia’s influence wanes, and that of India’s close rival China’s rises, the crewed Gaganyaan program is “a means of growing their own standing in the world.”

Dodge notes that national prestige has always been a part of space exploration, going back to the original space race between the US and the Soviet Union. But that prestige is about two things, “One of them is technological prowess, and being able to demonstrate to the world that you were among the elite, and your capability to use and explore space,” he says. ”But the other is a geopolitical overlay.”

What excites Forczyk about ISRO’s plans, in contrast to India’s anti-satellite missile test in 2019, is that they are a peaceful way for India to cultivate national and geopolitical prestige. The success of the Indian civilian space program can serve as a model for other nations as they make their own bids to become space powers in the 21st century. 

“What we’re going to see is more countries that have historically not played a large role in space rise, because they see it as a means of demonstrating their technology, technological advancement,” Forczyk says. “A peaceful demonstration of advancement.” 

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When humans finally return to the moon as part of NASA’s Artemis program, they’ll arrive with a bevy of high-tech equipment to capture new, awe-inspiring glimpses of Earth’s satellite. But cameras have come a long way since the Apollo missions. In 2023, some incredibly advanced options are already almost moon-ready right off the shelf.

According to a recent update from the European Space Agency, engineers collaborating with NASA are finalizing a Handheld Universal Lunar Camera (HULC) with real-world testing in the rocky, lunar-esque vistas of Lanzarote, Spain. While resilient enough to travel to the moon, HULC’s underpinning tech derives from commercially available professional cameras featuring high light sensitivities and cutting-edge lenses. To strengthen the lunar documentation device, researchers needed to add a blanket casing that is durable enough to protect against ultra-fine moon dust, as well as the moon’s extreme temperature swings ranging between -208 and 250 degrees Fahrenheit. At the same time, the covering can’t impede usage, so designers also created a suite of ergonomic buttons compatible with astronaut spacesuits’ thick gloves.

[Related: Check out this Prada-designed Artemis III spacesuits.]

So far, HULC has snapped shots in near pitch-black volcanic caves, as well as in broad daylight to approximate the lunar surface’s vast spectrum of lighting possibilities. According to the ESA, HULC will also be the first mirrorless handheld camera used in space—such a design reportedly offers quality images in low light scenarios.

Even with the numerous alterations and adjustments, the HULC is still not quite ready for the Artemis III mission, currently scheduled for 2025. The ESA reports that at least one version of the camera will soon travel to the International Space Station for additional testing.

“We will continue modifying the camera as we move towards the Artemis III lunar landing,” Jeremy Myers, NASA lead on the HULC camera project, told the ESA on October 24. “I am positive that we will end up with the best product–a camera that will capture Moon pictures for humankind, used by crews from many countries and for many years to come.”

Images of Buzz Aldrin and Neil Armstrong striding across the lunar surface during the Apollo 11 moonwalk instantly became iconic photographs in 1969, but they were only a preview of many more to come. Over the next three years, 10 more astronauts documented their visits to the moon using an array of video and photographic cameras. When humans finally return as part of the Artemis program, HULC will be in tow to capture new, awe-inspiring glimpses of Earth’s satellite.

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Despite being our closest planetary neighbor, Venus is a pretty inhospitable place. It is about 100 times hotter than Earth and spacecraft exploring its thick atmosphere have been crushed in only two hours. However, Venus may have once had tectonic plate movements that are similar to what occurred during Earth’s early days. The new finding gives astronomers some novel scenarios to evaluate regarding the possibility of early life on Venus, its evolutionary past, and the history of the solar system. The findings are described in a study published October 26 in the journal Nature Astronomy. 

[Related: We finally know why Venus is absolutely radiant.]

In the study, researchers used atmospheric data from Venus and computer modeling to show that the composition of the planet’s current atmosphere and surface pressure could have only resulted from an early form of plate tectonics. This process is critical to life and involves multiple continental plates pushing, pulling, and sliding beneath one another. 

On Earth, these plate tectonics have intensified over billions of years. This process has formed new continents, mountains, and led to the chemical reactions that stabilized Earth’s surface temperature. It also created an environment that is more conducive for life to develop.

Venus went in the opposite direction and has surface temperatures of 867 degrees Fahrenheit, hot enough to melt lead. Astronomers have always believed that Venus has a “stagnant lid.” This means that the planet’s surface only has a single plate with minimal amounts of give, so most of the gasses remain trapped beneath the outer crust lid.

The team used current data on Venus’ atmosphere as the endpoint for these models and started by assuming Venus has had a stagnant lid through its entire existence. They were quickly able to see that computer simulations recreating the planet’s current atmosphere didn’t match up with where Venus is now. 

Next, the team simulated what would have had to happen on Venus for the planet to get to its current state. They eventually matched the numbers almost exactly when they accounted for limited tectonic movement early in Venus’ history followed by the stagnant lid model that exists today.

Due to the abundance of nitrogen and carbon dioxide present in Venus’ atmosphere, the team believes that Venus must have had plate tectonics about 4.5 billion to 3.5 billion years ago after the planet formed. They suggest that like on Earth, this early tectonic movement would have been limited in terms of the number of plates moving around and in how much they shifted. The process also would have been occurring on Venus and Earth at the same time. 

“One of the big picture takeaways is that we very likely had two planets at the same time in the same solar system operating in a plate tectonic regime—the same mode of tectonics that allowed for the life that we see on Earth today,” study co-author and Brown University planetary geophysicist Matt Weller said in a statement. 

[Related: A private company wants to look for life just above Venus.]

According to the team, this further bolsters the possibility that microbial life existed on ancient Venus. It also shows that at one point, both Earth and Venus were even more alike than scientists previously thought before diverging. Both planets are about the same size, have the same mass, density, and volume and live in the same solar neighborhood.

The work also shows the possibility that plate tectonics on all planets might simply come down to timing, so life itself may also be a product of the perfect timing. 

“We’ve so far thought about tectonic state in terms of a binary: it’s either true or it’s false, and it’s either true or false for the duration of the planet,” study co-author and Brown University geobiologist and geophysicist Alexander Evans said in a statement. “This shows that planets may transition in and out of different tectonic states and that this may actually be fairly common. Earth may be the outlier. This also means we might have planets that transition in and out of habitability rather than just being continuously habitable.”

Understanding the transition of tectonic states will be important for future studies of nearby moons and distant exoplanets. Jupiter’s fourth largest moon Europa has already shown evidence of Earth-like plate tectonics.

“We’re still in this paradigm where we use the surfaces of planets to understand their history,” Evans said. “We really show for the first time that the atmosphere may actually be the best way to understand some of the very ancient history of planets that is often not preserved on the surface.”

Future NASA DAVINCI missions will measure gasses in Venus’ atmosphere and could help solidify this study’s findings and the details of how this happened may hold important implications for Earth.

“That’s going to be the next critical step in understanding Venus, its evolution and ultimately the fate of the Earth,” Weller said. “What conditions will force us to move in a Venus-like trajectory, and what conditions could allow the Earth to remain habitable?”

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Gravitational wave observatories, such as the Laser Interferometer Gravitational-Wave Observatory (LIGO), are exercises in extreme sensitivity. LIGO’s two experimental ears—one in Louisiana, another in Washington state—listen to ripples in space-time left behind by objects that include black holes and neutron stars. To do this, LIGO carefully watches for minute fluctuations in miles-long laser beams. The challenge is that everything from rumbling tractors to the weather to quantum noise can cause disturbances of their own. A huge part of gravitational wave observation is the science of weeding out unwanted noise.

Now, following a round of upgrades, both of LIGO’s ears can hear 60 percent more events than ever before. Much of the credit goes to a system that corrects for barely perceptible quantum noise by very literally squeezing the light.

Physicists and engineers have been tinkering with light-squeezing in the lab for decades, and their work is showing real results. “It’s not a demonstration anymore,” says Lee McCuller, a physicist at Caltech. “We’re actually using it.” McCuller and his colleagues will publish their work in the journal Physical Review X on October 30.

Gravitational waves are an odd curiosity of how gravity works, as predicted by general relativity. As a falling rock casts ripples in water, sufficiently spectacular events—say, two black holes or two neutron stars merging together—cast waves in the fabric of space-time. Listening into those gravitational waves allows astronomers to peek at massive objects like black holes and neutron stars that are otherwise difficult to see clearly. Scientists can only pull this off thanks to devices like LIGO.

LIGO’s ears are shaped like very large Ls, their arms precisely 4 kilometers (2.49 miles) long. A laser beam, split in two, travels each down one of the arms. Those beams bounce off a mirror at the far end, and return back to the vertex, where they can be recombined into a single beam. Tiny shifts in space-time—gravitational waves—can subtly stretch and squeeze either arm, etching patterns in the recombined beam’s light.

The length shifts are extremely subtle, far too slight to even dream of seeing with the naked eye. The task of detecting such a slight shift becomes even trickier when LIGO detectors are prone to earthquakes, weather, and human activity, all of which create noise that rattles the mirrors or shakes up the laser beams.

Physicists have developed ways of cutting out all that noise. They can keep the arms in a vacuum, devoid of all other matter, to prevent sound waves. They can suspend mirrors to isolate them from vibrations. They can measure the noise of the outside world and adjust the instruments accordingly, like a very large noise-cancelling headset. 

But something that these methods cannot filter out is quantum physics. Even in a perfect vacuum, the inherent randomness of the universe at its tiniest scales—particles popping in and out of existence—makes its mark. “You’ve got a natural fluctuation on the level of your measurement that can mask a weak gravitational wave signal,” says Patrick Sutton, an astrophysicist at Cardiff University, a member of the LIGO-Virgo collaboration who wasn’t an author of the new study.

[Related: We’ve recorded a whopping 35 gravitational wave events in just 5 months]

LIGO detected the first-ever confirmed gravitational waves in 2016. Around the same time, its operators were thinking about ways to weed out the quantum disturbances. Physicists can manipulate light by trapping it within a crystal and “squeezing” it. They installed such a crystal on both LIGO detectors in time for the observatory’s third round of detections, which began in 2019.

The upgrade enabled LIGO to work with laser light with higher frequencies. But squeezing light like this came at a cost: making it more difficult to read lower-frequency light. This is problematic, because the gravitational waves from events we can detect—such as black hole mergers—tend to produce a good deal of lower-frequency light in LIGO.

So, after COVID-19 forced LIGO to shut down in mid-2020, its operators added a new chamber to their squeezing setup. This chamber allows a more adaptive approach, manipulating different properties of light at different frequencies. To do this, the chamber must trap light for 3 milliseconds—enough time for light to travel hundreds of miles. The chamber began operation when LIGO’s fourth, current observing run switched on earlier this year.

“It took a lot of engineering and design work and careful thinking to make this an upgrade that does its job and improves squeezing, but doesn’t introduce new noise,” McCuller says.

Both of LIGO’s detectors can now pick up gravitational waves from further into the cosmos and from a wider swath of space. LIGO now hears about 60 to 70 percent more events, according to Sutton. Better sensitivity also allows astronomers to measure gravitational waves with greatly increased precision, which lets them test the theory of general relativity. “It’s a significant jump,” Sutton says.

[Related: Astronomers now know how supermassive black holes blast us with energy]

LIGO’s fellow detector in Europe, Virgo, is implementing the same frequency-dependent squeezing based on its scientists’ own research. “We don’t currently know of any other technique that can improve upon this one,” McCuller says. “In terms of new techniques, this is the best one we actually know how to use at the moment.”

All the gravitational wave events we’ve seen so far came from two black holes or two neutron stars emerging: loud, violent events that leave equally violent splashes. But gravitational wave listeners would like to use gravitational waves to listen to other events, too, such as supernovas, gamma ray bursts, and pulsars. We aren’t quite there yet, but squeezing may get us closer by letting us take full advantage of the hardware we have.

“The key there is just to make the detectors ever more sensitive—bring that noise down and down and down—until, eventually we start seeing some,” Sutton says. “I think those will be very exciting days.”

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Humans have been changing the atmosphere from Earth’s surface for nearly two centuries—but now in the Space Age, we’re altering it from outer space, too. Atmospheric scientists recently found traces of unexpected metals in the stratosphere, the second-lowest layer of the atmosphere where ozone resides and meteors burn up into shooting stars. The researchers determined that this pollution came from spacecraft as they reenter Earth’s atmosphere, in research published last week in the journal Proceedings of the National Academy of Sciences. 

This study is “the first observational evidence that space activities are a very significant source of particulate pollution to the stratosphere” says Slimane Bekki, an atmospheric scientist at LATMOS not involved in the new work. “More importantly, nobody knows the impacts of these particles on the ozone layer,” he adds, pointing out the importance of this molecule in shielding humans from dangerous UV radiation.

Usually, mission planners’ main concern is to ensure that space debris doesn’t hit the ground, where it could hurt people or structures—but, as this research points out, what evaporates in the stratosphere could still be making an impact, even if it’s not a literal one. That material has to exist somewhere, and it looks like it’s lingering in the stratosphere. “We are finding this human-made material in what we consider a pristine area of the atmosphere. And if something is changing in the stratosphere—this stable region of the atmosphere—that deserves a closer look,” said co-author and Purdue atmospheric scientist Dan Cziczo in a press release. 

[Related on PopSci+: Rocket fuel might be polluting the Earth’s upper atmosphere]

The research team flew through the stratosphere across the continental US in aircraft specially designed to fly at high altitudes, equipped with air-analyzing instruments in their nose cones. These unique planes— NASA’s ER-2 and WB-57—cruise at around 65,000 feet, almost double the altitude of typical passenger jets. Flying as high as 70,000 feet, the research craft can go above 99 percent of the mass of Earth’s atmosphere.

Within the stratosphere, the collecting equipment on these planes recorded traces of the heavy metals niobium and hafnium. These elements aren’t found naturally in the atmosphere, but they are typically used in rockets and spacecraft shells. The team also measured higher-than-expected concentrations of over 20 metals, including copper, lithium, aluminum, and lead. All told, about 10 percent of aerosol particles in the stratosphere contain metals. 

Atmospheric scientists aren’t sure exactly how these changes will affect Earth. The stratosphere contains tiny blobs of sulfuric acid, which are now infused with the metals from old spacecraft. The presence of those metals could change the chemistry of the stratosphere, including how big the sulfuric acid drops grow. Even small tweaks high up could affect the way light bends, the transfer of heat, or how crystals of ice grow. 

The big question is how these changes will affect human life on the surface. Unfortunately, there’s no clear answer to that, but in the past small stratospheric changes have led to big impacts—like adding CFCs that ate away at the ozone layer. Eventually, there may need to be additional environmental precautions for spaceflight to prevent harm to the stratosphere.

[Related: This beautiful map of Earth’s atmosphere shows a world on fire]

“The only way for these particles not to appear in the upper atmosphere is for the satellites not to be launched in the first place,” explains University of Exeter atmospheric scientist Jamie Shutler, who was not part of the research team. “The possible ways forward are to launch less, make the satellites last for longer (so we need to launch less), or encourage industry to make the constituents of satellites public knowledge (so we can guide manufacturers as to the potential harmful effects).” He adds that this new finding “confirms our concern” about stratospheric contamination.

But before we can solve this problem, “the concept that reentry can affect the stratosphere has to be thought about,” says lead author Daniel Murphy, atmospheric scientist at NOAA. He emphasized that this idea is still incredibly new and will require much more research to understand the scale and potential consequences of this pollution.

Potential impacts are expected only to grow as the rate of spacecraft launches and reentries accelerate. In the last five years, space agencies and private companies have launched more than 5,000 satellites, noted Martin Ross, co-author on the work and climate scientist at The Aerospace Corporation, in a press release. “Most of them will come back in the next five, and we need to know how that might further affect stratospheric aerosols,” he said. The team expects that the proportion of particles containing metal could grow from 10 to more than 50 percent in the next few decades, especially thanks to upcoming plans to reduce space debris by hurling it back into the atmosphere.

Those efforts and upcoming launches, though, need to be aware of the possible effects on Earth—and researchers need to do more work to determine the extent of those effects. “Understanding our planet is one of the most urgent research priorities there is,” said Cziczo.

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Against all odds and expectations, both Voyager 1 and Voyager 2 are still going strong after nearly half a century of hurtling through—and far past—the solar system. To help boost the potential for the probes’ continued operations, engineers at NASA’s Jet Propulsion Laboratory have beamed out two software updates across the billions of miles separating them from the historic spacecraft. If successful, the pair of interstellar travelers could gain at least another five years’ worth of life, if not more.

On October 20, NASA announced plans to transmit a software patch to protect Voyager 1 and 2 against a glitch that occurred within the former’s system last year. In May 2022, NASA started noticing inaccurate readings coming from Voyager 1’s attitude articulation and control system (AACS). A few months later, engineers determined the AACS was accidentally writing commands into memory instead of actually performing them.

Although engineers successfully resolved an original data issue within Voyager 1 in 2022, the new patch will hopefully ensure such a problem won’t arise again in either probe. Receiving the patch will take over 18 hours to reach transmitters; Voyager 2 will get the patch first to serve as a “testbed for its twin” in case of unintended consequences like accidentally overwriting essential code. Given Voyager 1 and Voyager 2 are respectively 15 billion and 12 billion miles from Earth, engineers consider the farther craft’s data more valuable, as it still remains the farthest traveling human-made object. The NASA-JPL team will issue a command on October 28 to test the patch’s efficacy.

[Related: The secret to Voyagers’ spectacular space odyssey.]

The second planned tune-up for Voyager 1 and 2 involves the small thrusters responsible for controlling the probes’ communication antennas. According to NASA, spacecraft can generally rotate in three directions—left and right, up and down, as well as wheellike around a central axis. During these movements, propellant automatically flows through incredibly narrow “inlet tubes” to maintain the antennas’ contact with Earth.

But each time the propellant is used, miniscule residue can stick within the inlet tubings—while not much at first, that buildup is becoming problematic after the Voyager probes’ (many) decades’ of life. To slow the speed of buildup, engineers have edited the probes’ operational commands to allow both craft the ability to rotate nearly 1 degree farther in each available direction. This will reduce how often their thrusters need to fire. When engineers do need to enable thrusters, they now plan to fire them for longer periods of time, thus reducing the overall number of usages. 

[Related: How is Voyager’s vintage technology still flying?]

“This far into the mission, the engineering team is being faced with a lot of challenges for which we just don’t have a playbook,” Linda Spilker, Voyager mission project scientist, said via NASA’s update. “But they continue to come up with creative solutions.”

Experts estimate both the fuel lines and software adjustments could extend the Voyager program’s lifespan by another five years. According to NASA, however, “additional steps in the coming years to extend the lifetime of the thrusters even more.”

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The moon is our closest neighbor in space and the only celestial body humans have set foot on, yet we are still learning about it. In fact, Earth’s moon might actually be 40 million years older than scientists previously believed. By conducting an atom-by-atom analysis on crystals that were brought back by Apollo astronauts in 1972, a team of geochemists and plenary scientists now calculate that the igneous orb is at least 4.46 billion years old. The findings are described in a study published today in the journal Geochemical Perspectives Letters.

Intertwined fates

Heck is a curator for the meteorite collection at the Field Museum in Chicago and a professor at the University of Chicago. He says that studying the moon also helps us understand our own planet because of the topographical differences.

“Earth’s surface is much, much younger because there’s so much geologic activity [here] from volcanism and weathering,” explains Heck. “The moon’s surface is essentially an archive of solar system dynamics. This is a record that we don’t have on Earth, but our planet’s evolution is tied to these impacts that happened in the early solar system.”

A historical perspective

In the study, the team looked at moon dust brought back by the Apollo 17 crew. The 1972 lunar landing included NASA geologist Harrison Schmidt, who collected multiple rocks to study back on Earth. His samples contain very small crystals that were created billions of years ago and can help indicate when the moon was formed.

The energy created by the impact from the object that struck Earth and created the moon melted the rock that eventually became the lunar surface. That offers a clue to the elements that existed on the celestial body since its emergence versus the ones that appeared much later. For example, zirconium, a silver metal found on both the Earth and the moon, could not form and survive on the molten lunar surface: Any zircon crystals that are currently present on the moon must have formed after the magma ocean cooled. Determining the age of these structures can thus reveal the minimum possible age for the moon, assuming that they emerged right after the impact.

Looking atom by atom

Researchers have previously suggested that the moon is older than estimated, but this new study is the first to use an analytical method called atom probe tomography to pinpoint the age from the oldest known lunar crystal retrieved by humans.

“In atom probe tomography, we start by sharpening a piece of the lunar sample into a very sharp tip using a focused ion beam microscope, almost like a very fancy pencil sharpener,” study co-author and planetary scientist Jennika Greer said in a statement. “Then, we use UV lasers to evaporate atoms from the surface of that tip. The atoms travel through a mass spectrometer, and how fast they move tells us how heavy they are, which in turn tells us what they’re made of.”

This atom-by-atom analysis revealed how much of the zircon crystals had undergone radioactive decay—a process where atoms that have an unstable configuration shed some protons and neutrons. They then transform into different elements, like how uranium decays into lead. Based on the amount of conversion and the known half-lives of different chemical isotopes, experts can estimate the age of the sample.

“Radiometric dating works a little bit like an hourglass,” Heck said in a statement. “In an hourglass, sand flows from one glass bulb to another, with the passage of time indicated by the accumulation of sand in the lower bulb. Radiometric dating works similarly by counting the number of parent atoms and the number of daughter atoms they have transformed to. The passage of time can then be calculated because the transformation rate is known.”

The team working with the Apollo 17 sample found that the proportion of lead isotopes (the daughter atoms created during the decay) indicated that the crystals were about 4.46 billion years old, so the moon must at least be that old too. While this puts the moon’s age back 40 million years, that’s still a very short time compared to the universe’s roughly 13.7 billion-year history. 

“It’s amazing being able to have proof that the rock you’re holding is the oldest bit of the moon we’ve found so far. It’s an anchor point for so many questions about the Earth. When you know how old something is, you can better understand what has happened to it in its history,” Greer said.

From Apollo to Artemis

In future studies, clues pulled from these decades-old samples could be pooled with those from samples taken by upcoming Artemis lunar missions. Artemis III is scheduled for 2025 and will land on and explore the lunar South Pole. The Apollo 17 mission collected samples from the Taurus-Littrow valley on the eastern edge of Mare Serenitatis, so crystals from a different region of the moon could yield unimaginable discoveries. 

[Related: Scientists have new moon rocks for the first time in nearly 50 years]

“I am convinced that there is older stuff on the moon—we just haven’t found it yet. I even think we have older zircons in the Apollo samples. This is really the power of sample return,” says Heck. 

A mixture of new samples and future advances in technology could further anchor the timeline of how our solar system was formed and beyond.  “Maybe in 50 or 100 years or even later, new generations of scientists will have the tools we can only dream about today to address scientific questions we can’t even think about today,” says Heck. “These templates are a legacy for future generations.”

The post The moon is 40 million years older than we thought, according to crystals collected by Apollo astronauts appeared first on Popular Science.

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NASA plans to return humans to the moon in 2025 with the Artemis III mission. Before that, the space agency will conduct a vital preliminary mission in November 2024, when the Artemis II mission flies a crew of astronauts in lunar orbit for the first time since the 1970s. But the “important first step” toward those goals, as NASA put it in a recent blog post, is the planned launch of the IM-1 mission carrying the NOVA-C lunar lander in a few weeks. It will attempt to land several NASA science experiments near Malapert A, a crater in the southern lunar polar region. Those studies could help NASA prepare for astronaut operations in the area in 2025. 

Unlike the Artemis missions, though, NOVA-C isn’t a big NASA project. Instead, the truck-sized craft designed to ferry small payloads to the lunar surface was built, and will be operated by, the small Texas-based company Intuitive Machines. 

If it succeeds in landing near the lunar south pole, NOVA-C will be the first US soft landing on the moon since the 1970s, and the first ever commercial landing on the moon that hasn’t crashed or failed. So why is a small spacecraft built by a relatively small company a key part of NASA’s big moon program?

“There is a pattern that we have now seen of NASA trying to move to more commercial solutions and services, rather than do it all on their own,” says Wendy Whitman Cobb, a space policy expert and instructor at the US Air Force School of Advanced Air and Space Studies. It’s much like NASA’s Commercial Crew and Cargo programs, which contracted with SpaceX to fly astronauts and supplies to the International Space Station aboard its Dragon space capsules. 

[Related: Why do all these countries want to go to the moon right now?]

Now NASA is turning to commercial companies to prepare the way for humanity’s return to the moon. Intuitive Machines was one of the first companies to receive a contract—for $77 million— under NASA Commercial Lunar Payload Services, or CLPS program, back in 2019. NASA designed CLPS to fund private sector companies interested in building small, relatively inexpensive spacecraft to fly experiments and rovers to the moon, allowing NASA to simply purchase room on the spacecraft rather than developing and operating it themselves. 

In the case of NOVA-C, five NASA payloads will ride along with devices from universities including Louisiana State and Embry-Riddle Aeronautical University. ”The NASA payloads will focus on demonstrating communication, navigation and precision landing technologies, and gathering scientific data about rocket plume and lunar surface interactions, as well as space weather and lunar surface interactions affecting radio astronomy,” the space agency wrote in a blog post about the mission. 

“We don’t still don’t know a lot about the moon,” Whitman Cobb adds. The moon has variable gravity depending on where there are more metallic materials. “Finding out where those places are, how lunar dust is going to kick up when you’re trying to land or take off—all of these things are really key.”

That’s why NASA is sending payloads to ride along with NOVA-C. But the reason NOVA-C is landing where it is, about 300 kilometers from the south pole, has more to do with how the whole world is now thinking about the moon.

NOVA-C was originally destined to land in the Oceanus Procellarum, one of the large, dark areas known as mares, or “seas,” on the lunar surface. But in May, NASA and Intuitive Machines announced the change in plans and the new target near the south pole. 

[Related: We finally have a detailed map of water on the moon]

”The decision to move from the original landing site in Oceanus Procellarum was based on a need to learn more about terrain and communications near the lunar South Pole,” NASA announced in a blog post at the time. “Landing near Malapert A also will help mission planners understand how to communicate and send data  back to Earth from a location that is low on the lunar horizon.”

The reasons NASA wants to land near the lunar south pole with Artemis, and why the recent and successful Chandrayaan 3 mission of India, and the failed Russian Luna 25 mission, both targeted the lunar south pole are twofold: research and resources, according to Richard Carlson, a lunar geologist who retired from the Carnegie Institute for Science in 2021.  

“Both north and south polar regions have permanently shadowed craters where water has been detected from orbit,” he says. ”The real question is whether that water is a one micron surface coating of water on a few grains, or whether it’s a substantial abundance of water. Water of course being useful for a lot of things, from drinking water to turning it into hydrogen and oxygen, which is rocket fuel.”

The other motivation for going to the south pole is that it’s geologically very different from where the Apollo missions landed, according to Carlson. “They all landed on a pretty small portion of the moon on the Earth facing side of the moon on the nice flat mares, and that’s a rather unusual part of the moon geologically,” he says. ”If you think of studying the Earth this way, the Apollo lunar program would have basically landed on, let’s say, just North America, and that’s it.”

The lunar south polar region is much more geologically varied, with tall mountains and ridges, as well as rocks dug out from deep within the moon and scattered over the region by impact craters billions of years ago, Carlson says. But of course, such a landscape has its downsides for spacecraft coming from Earth. 

“You look at the pictures of the places that they selected [for Artemis III] and I wouldn’t want to land there. I mean, they’re really rough,” he says. “If we land on a rock, the spacecraft is going to fall over.” Sending small, uncrewed craft like NOVA-C to the moon’s south polar ahead of Artemis astronauts will test how difficult landing there really is. 

After all, as Witman Cobb notes, touching down anywhere on the moon is really hard. Before the failed Luna 25 landing on August 21, there were two failed commercial lunar landings. The Israeli company SpaceIL saw its Beresheet lander crash land in 2019, while the Hakuto-R M1 lander from Japanese company ispace crashed in April. 

”We haven’t seen a commercial company be successful in landing on the moon yet,” Whitman Cobb says. ”That’s really fascinating when you think about our capability of landing humans on the moon in the 1960s, and 1970s. That today, with all of the technology that we now have, this is still a really, really difficult thing to do.”

The post This private lander could be the first US machine on the moon this century appeared first on Popular Science.

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Best overall		Celestron StarSense Explorer DX 130AZ		SEE IT	A solid build and specs, paired with smartphone-guided sky recognition technology, makes this telescope perfect for starry-eyed explorers.
Best for viewing planets		Sky-Watcher Skymax 102mm Maksutov-Cassegrain Telescope		SEE IT	This telescope punches above its weight class in size and power, making it an ideal scope for checking out neighboring orbs.
Best for kids		Orion Observer II 60mm AZ Refractor Telescope Starter Kit		SEE IT	The entire package is designed to inspire kids during the window where they stare curiously out of the windows.

Telescopes under $500 can provide a passport to the universe without emptying your wallet. In their basic function, telescopes are our connection to the stars. For millennia, humankind has gazed skyward with wonder into the infinite reaches of outer space. And as humans are a curious bunch, our ancestors devised patterns in the movements of celestial bodies, gave them names, and built stories around them. The ancient Egyptians, Babylonians, and Greeks indulged in star worship. But you don’t have to follow those lines to geek out over the vastness of the night sky. It’s just so cool. Fortunately, whatever your motivation for getting under the stars, there is an affordable option for you on our list of the best telescopes under $500.

• Best overall: Celestron StarSense Explorer DX 130AZ
• Best for viewing planets: Sky-Watcher Skymax 102mm Maksutov-Cassegrain Telescope
• Best for astrophotography: William Optics Guide Star 61
• Best for kids: Orion Observer II 60mm AZ Refractor Telescope Starter Kit
• Best budget: Popular Science by Celestron Travel Scope 70 Portable Telescope

How we chose the best telescopes under $500

The under-$500 telescope market is crowded with worthy brands and models, so we looked at offerings in that price range from several well-known manufacturers in the space. After narrowing our focus based on personal experience, peer suggestions, critical reviews, and user impressions, we considered aperture, focal length, magnification, build quality, and value to select these five models.

The best telescopes under $500: Reviews & Recommendations

To get the best views of the stars, planets, and other phenomena of outer space, not just any old telescope will get the job done. There are levels of quality and a wide range of price points and features to sort through before you can be sure you’re making the right purchase for what you want out of your telescope, whether it’s multi-thousands, one of the best telescopes for under $1,000, or one of our top picks under $500.

Best overall: Celestron StarSense Explorer DX 130AZ

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Why it made the cut: Solid build and specs, paired with the remarkable StarSense Explorer app, make this telescope a perfect introduction to celestial observation.

Specs

• Focal length: 650mm
• Aperture: 130mm, f/5
• Magnification: 65x, 26x

Pros

• App aids in finding stars
• Easy to operate
• Steady altazimuth mount

Cons

• Eyepieces are both low power

Newbies to astronomy today can have a decidedly different experience than beginners who started stargazing before smartphones were a thing. Instead of carting out maps of the night sky to find constellations, the StarSense Explorer series from Celestron, including the DX 130AZ refractor, makes ample use of your device to bring you closer to the stars. 

With your smartphone resting in the telescope’s built-in dock, the StarSense Explorer app will find your location using the device’s GPS and serve up a detailed list of celestial objects viewable in real time. Looking for the Pleiades cluster? This app will tell you how far away it is from you and then lead you there with on-screen navigation. The app also includes descriptions of those objects, tips for observing them, and other useful info. 

The StarSense Explorer ships with an altazimuth mount equipped with slow-moving fine-tuning controls for both axes so you can find your target smoothly. And for those times you want to explore the night sky without tethering a smartphone, the scope’s red dot finder will help you zero in on your targets. The two eyepieces, measuring 25mm and 10mm, are powerful enough to snag stellar views of the planets but not quite enough to see the details a high-powered eyepiece would deliver.

Best for viewing planets: Sky-Watcher Skymax 102mm Maksutov-Cassegrain Telescope

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Why it made the cut: This telescope punches above its weight class in size and power, making it an ideal scope for viewing planets.

Specs

• Focal length: 1300mm
• Aperture: 102mm, f/12.7
• Magnification: 130x, 52x

Pros

• Great for viewing planets and galaxies
• Sharp focus and contrast
• Powerful

Cons

• Not ideal for deep-space viewing

Let’s be real—most consumers in the market for a moderately priced telescope are in it to gain spectacular views of the planets and galaxies, but probably not much else. And it’s easy to see why. Nothing makes celestial bodies come alive like viewing them in real time, in all their colorful glory.

If that sounds like you, allow us to direct you to the Sky-Watcher Skymax 102, a refracting telescope specializing in crisp views of objects like planets and galaxies with ample contrast to make them pop against the dark night sky. The Skymax 102 is based on a Maksutov-Cassegrains design that uses both mirrors and lenses, resulting in a heavy-hitting scope in a very compact and portable unit. A generous 102mm aperture pulls in plenty of light to illuminate the details in objects, and the 1300mm focal length results in intense magnification.

Two included wide-angle eyepieces measuring 25mm and 10mm deliver 130x and 52x magnification, respectively. The package also includes a red-dot finder, V-rail for mounting, 1.25-inch diagonal viewing piece, and a case for transport and storage. Look no further if you’re looking for pure colors across a perfectly flat field in a take-anywhere form factor.

Best for astrophotography: William Optics GuideStar 61 

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Why it made the cut: Top-notch specs and an enviable lens setup make this telescope ideal for astrophotography.

Specs

• Focal length: 360mm
• Aperture: f/5.9
• Magnification: 7x (with 2-inch eyepiece)

Pros

• Well-appointed specs
• Sturdy, durable construction
• Carrying case included

Cons

• Flattener is an extra purchase

Sometimes you want to share more than descriptions of what you see in the night sky, and that’s where this guidescope comes in, helping you to focus on the best full-frame image. You can go as deep into the details (not to mention debt) as your line of credit will allow in your quest to capture the most impressive images of space. Luckily, though, this is a worthy option at a reasonable price. 

The Williams Optics Guide Star 61 telescope is a refracting-type scope with a 360mm focal length, f/5.9 aperture, and 61mm diameter well-suited to capturing sharp images of planets, moon, and bright deep-sky objects. The GS61 shares many specs with the now-discontinued Zenith Star 61, including focal length, aperture, and diameter, as well as the FPL53 ED doublet lens for high-contrast images.

The scope’s optical tube is about 13 inches long and weighs just 3 lbs.—great for traveling with the included carrying case—with a draw-tube (push-pull) focuser for coarse focusing and a rotating lens assembly for fine focus. Attaching a DSLR camera to the Guide Star 61 is a fairly easy job, but note that the flattener for making that connection is a separate purchase.

Best for kids: Orion Observer II 60mm AZ Refractor Telescope Starter Kit

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Why it made the cut: The entire package is designed to get kids exploring space right out of the box.

Specs

• Focal length: 700mm
• Aperture: 60mm, f/11.7
• Magnification: 70x, 28x

Pros

• Capable of detailed views of moon and planets
• Lightweight construction
• Lots of handy accessories

Cons

• Not enough optical power to reach deep space

Parents have a limited window of time to recognize and develop their kids’ interests, so kindle a fascination with the stars through a star projector and then fan it with a telescope. That’s what makes the Orion Observer II such a great buy. Seeing the craters on the moon or the rings of Saturn for the first time can affirm your kids’ curiosity about space and expand their concept of the universe—and they can get those goosebumps while learning through this altazimuth refractor telescope.

The Orion Observer II is built to impressive specifications, with a 700mm focal length that provides 71x magnification for viewing the vivid details of planets in our solar system. True glass lenses (not plastic) are a bonus at this price point, and combined with either included Kellner eyepieces (25mm and 10mm), the telescope delivers crisp views of some of space’s most dazzling objects. 

Kids and parents can locate celestial objects with the included red-dot finder. The kit also includes MoonMap 260, a fold-out map that directs viewers to 260 lunar features, such as craters, valleys, ancient lava flows, mountain ranges, and every U.S. and Soviet lunar mission landing site. An included copy of Exploring the Cosmos: An Introduction to the Night Sky gives a solid background before they go stargazing. And with its aluminum tube and tripod, the entire rig is very portable, even for young ones, with a total weight of 4.3 pounds. Find more options for the best telescopes for kids here. (And/or go the opposite direction with a microscope for kids—a love of science begets more science.)

Best budget: Popular Science by Celestron Travel Scope 70 Portable Telescope

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EDITOR’S NOTE: Popular Science has teamed up with Celestron on a line of products. The decision to include this model in our recommendations was made by our reviewer independently of that relationship, but we do earn a commission on its sales—all of which helps power Popular Science.

Why it made the cut: With its feature set, portability, and nice price point, this scope is ready for some serious stargazing without a serious investment.

Specs

• Focal length: 400mm
• Aperture: 70mm, f/5.7
• Magnification: 168x

Pros

• Bluetooth remote shutter release
• Ships with two eyepieces
• Pack included

Cons

• Lacks optical power for deep space

Getting out of town, whether camping in the wilderness or driving in the countryside, is one of the attractions of stargazing. Out in the great wide open, far away from streetlights, the stars explode even to the naked eye. Add a handy telescope like the Popular Science Celestron Travel Scope 70 Portable Telescope—our pick for the best portable telescope under $500—and you’ll see much farther into space. The fact that it’s as affordable as it is moveable just adds to the value.

The Popular Science Celestron Travel Scope 70 Portable Telescope is a well-equipped refractor telescope built for backpacking and adventuring but without skimping on cool gadgets. Whether you’re gazing at celestial or terrestrial objects, the smartphone adapter will aid you in capturing images with your personal device, with an included Bluetooth remote shutter release.

Designed with portability and weight in mind, the entire package fits into an included pack with a total of 3.3 pounds—that includes the telescope, tripod stand, 20mm and 10mm eyepieces, 3x Barlow lens, and more. Download Celestron’s Starry Night software to help you get the most from your astronomy experience. 

Here are some other options from the Celestron and Popular Science collaboration:

• Popular Science StarSense Explorer DX 100AZ Smartphone App-Enabled Telescope
• Popular Science AstroMaster 80mm – Portable Refractor Telescope
• Popular Science StarSense Explorer DX 5” Smartphone App-Enabled Telescope 
• Popular Science by Celestron Outland X 12x50mm Monocular with Tripod, Smartphone Adapter, and Bluetooth remote

What to consider when buying the best telescopes under $500

Optics

There are three types of optics available on consumer telescopes, and they will help you achieve three different goals. Refractor telescopes use a series of glass lenses to bring celestial bodies like the moon and near planets into focus easily. Reflector telescopes—also known as Newtonian scopes for their inventor, Sir Isaac Newton—swap lenses for mirrors and allow stargazers to see deeper into space. Versatile compound telescopes combine these two methods in a smaller, more portable form factor, with results that land right in the middle of the pack. 

Aperture

Photographers will recognize this: The aperture controls the amount of light entering the telescope, like on a manual camera. Aperture is the diameter of the lens or the primary mirror, so a telescope with a large aperture draws more light than a small aperture, resulting in views into deeper space. F-ratio is the spec to watch here. Low f-ratios, such as f/4 or f/5, are usually best for wide-field observation and photography, while high f-ratios like f/15 can make deep-space nebulae and other bodies easier to see and capture. Midpoint f-ratios can get the job done for both.

Mounts

All the lens and mirror power in the world won’t mean much if you attach your telescope to a subpar mount. In general, the more lightweight and portable the tripod mount, the more movement you’ll likely get while gazing or photographing the stars. Investing in a stable mount will improve the viewing experience. The two common mount types are alt-az (altitude-azimuth) and equatorial. Altazimuth mounts operate in the same way as a camera tripod, allowing you to adjust both axes (left-right, up-down), while equatorial mounts also tilt to make it easier to follow celestial objects.

FAQs

Final thoughts on the best telescopes under $500

• Best overall: Celestron StarSense Explorer DX 130AZ
• Best for viewing planets: Sky-Watcher Skymax 102mm Maksutov-Cassegrain Telescope
• Best for astrophotography: William Optics Guide Star 61
• Best for kids: Orion Observer II 60mm AZ Refractor Telescope Starter Kit
• Best budget: Popular Science by Celestron Travel Scope 70 Portable Telescope

Although this group of sub-$500 scopes is fairly diverse, the Celestron StarSense Explorer DX 130AZ stands out in our best telescopes under $500 as the best place to start your interstellar journey due to its versatility and sky recognition app, which make for a fun evening of guided tours through the star patterns, no experience necessary. 

Why trust us

Popular Science started writing about technology more than 150 years ago. There was no such thing as “gadget writing” when we published our first issue in 1872, but if there was, our mission to demystify the world of innovation for everyday readers means we would have been all over it. Here in the present, PopSci is fully committed to helping readers navigate the increasingly intimidating array of devices on the market right now.

Our writers and editors have combined decades of experience covering and reviewing consumer electronics. We each have our own obsessive specialties—from high-end audio to video games to cameras and beyond—but when we’re reviewing devices outside of our immediate wheelhouses, we do our best to seek out trustworthy voices and opinions to help guide people to the very best recommendations. We know we don’t know everything, but we’re excited to live through the analysis paralysis that internet shopping can spur so readers don’t have to.

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Of all the pyrotechnics that blast through the cosmos, fast radio bursts (FRBs) are among the most powerful—and mysterious. While our radio telescopes have picked up hundreds of known FRBs, radio astronomers recently detected one of the most fascinating bursts yet. Not only does it come from a greater distance than any FRB observed before, it’s the most energetic, too.

A superlative FRB like this defies our already murky understanding of the bursts’ origins. FRBs are sudden surges of radio waves that typically last less than a second, if not mere milliseconds. And they are very, very high-energy: They can deliver as much energy in milliseconds as the sun emits in three days. Despite all that, we don’t know for certain how they form.

The new event, what astronomers lovingly call FRB 20220610A, first appeared as a blip in the Australian Square Kilometre Array Pathfinder, an arrangement of antennae in the desert about 360 miles north of Perth. When astronomers measured the burst’s redshift, they calculated that it left its source about 8 billion years ago, as they described in a paper published today in Science. 

After pinpointing the burst’s origin in the sky and following up with visible light and infrared telescopes, the authors managed to develop a blurry image of merging galaxies.

[Related: Two bizarre stars might have beamed a unique radio signal to Earth]

“The further you go out in the universe, of course, the fainter the galaxies are, because they’re farther away. It’s quite difficult to identify the host galaxy, and that’s what they’ve done,” Sarah Burke Spolaor, an astronomer who studies FRBs at West Virginia University, who was not an author of the study.

FRBs aren’t exciting just because they’re loud. To reach us, a burst from outside the Milky Way must traverse millions or billions of light-years of the near-empty space between galaxies. In the process, they’ll encounter an extremely sparse smattering of ionized particles. This is the stuff that prevents the bulk of the cosmos from being completely empty—what astronomers call the intergalactic medium, which might make up as much as half of the universe’s “normal” matter.

“We don’t know much about it, because it’s so tenuous that it’s difficult to detect,” says Daniele Michilli, an astronomer at the Massachusetts Institute of Technology, who also wasn’t a study author.

As an FRB crosses the intergalactic medium on its long voyage, the particles cause its radio waves to scatter, which leaves fingerprints that astronomers can pick apart. In this way, scientists can use FRBs to investigate the intergalactic medium. More faraway bursts like FRB 20220610A could allow astronomers to study the medium across wide swathes of the universe.

[Related: How astronomers traced a puzzling detection to a lunchtime mistake]

“It’s very exciting, definitely one of the great applications of fast radio bursts,” says Ziggy Pleunis, an astronomer who studies FRBs at the University of Toronto, who was also not part of the authors’ group. “Fast radio bursts currently are really the only thing that we know that interacts with the intergalactic medium in a meaningful enough way that we can measure properties.”

In the future, astronomers might even be able to use FRBs to study how the universe expands. To unweave that mystery, however, astronomers will need to detect FRBs from even deeper into the cosmic past than FRB 20220610A. “For a lot of applications, it’s still not quite far away enough,” Pleunis says. “But it certainly bodes well.” 

There’s a balancing act involved: Over a sufficiently long distance, the particles in the intergalactic medium will peel an FRB apart until it disperses into background noise. To survive, an FRB must be brighter and more energetic; in turn, by taking stock of how much a burst has dispersed, astronomers can estimate its original energy. 

By computing the numbers for FRB 20220610A, they found that it was the most energetic burst Earth has seen so far. (Another recently observed burst, FRB 20201124A, comes within the same order of magnitude, but FRB 20220610A is the record-holder.) A burst with this much energy throws something of a wrench into astronomers’ understanding, such as it is, of what creates FRBs in the first place.

We, again, don’t have a definitive answer to that question. Complicating the question, some FRBs are one-off flashes, while others repeat, hinting that the two types of FRBs may have two different origins. (To wit, FRB 20220610A seems to have been a one-off. But that other high-energy FRB, FRB 20201124A, seems to repeat.)

Nevertheless, astronomers have simulated a few scenarios, largely involving neutron stars. Perhaps FRBs burst from near a neutron star’s surface, or perhaps FRBs erupt from shockwaves through the material that neutron stars throw up.

But when this paper’s authors ran the numbers with their new FRB, they found that neither of those two scenarios could easily create an burst with this much energy—suggesting that theoretical astronomers have even more work to do before they can satisfactorily explain these events.

“What always strikes me about fast radio bursts is, every time we observe a new one, it breaks the mold of previous ones,” Spolaor says.

The post Oldest radio burst ever found could tell us what exists between galaxies appeared first on Popular Science.

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Jupiter and its dynamic atmosphere are ready for another closeup in a new image taken with the James Webb Space Telescope (JWST). Using the telescope’s data, scientists have discovered a new and never-before-captured high-speed jet stream. The jet stream sits over Jupiter’s equator above the main cloud decks, barrels at speeds twice as high as a Category 5 hurricane, and spans more than 3,000 miles. The findings were described in a study published October 19 in the journal Nature Astronomy.

[Related: This hot Jupiter exoplanet unexpectedly hangs out with a super-Earth.]

Jupiter is the largest planet in our solar system and its atmosphere has some very visible features, including the infamous Great Red Spot, which is large enough to swallow the Earth. The planet is ever-changing and there are still mysteries in this gas giant that scientists are trying to unravel. According to NASA, the new discovery of the jet stream is helping them decipher how the layers of Jupiter’s famously turbulent atmosphere interact with each other. Now, JWST is helping scientists look further into the planet and see some of the lower and deeper layers of Jupiter’s atmosphere where gigantic storms and ammonia ice clouds reside. 

“This is something that totally surprised us,” study co-author Ricardo Hueso said in a statement.  “What we have always seen as blurred hazes in Jupiter’s atmosphere now appear as crisp features that we can track along with the planet’s fast rotation.” Hueso is an astrophysicist at the University of the Basque Country in Bilbao, Spain.

The research team analyzed data from JWST’s Near-Infrared Camera (NIRCam) that was obtained in July 2022. The Early Release Science program was designed to take images of Jupiter 10 hours apart (one Jupiter day) in four different filters. Each filter detected different types of changes in the small features located at various altitudes of Jupiter’s atmosphere.

The resulting image shows Jupiter’s atmosphere in infrared light. The jet stream is located over the equator, or center, of the planet. There are multiple bright white spots and streaks that are likely very high-altitude cloud tops of condensed convective storms. Jupiter’s northern and southern poles are dotted by auroras that appear red and extend to the higher altitudes of the planet. 

“Even though various ground-based telescopes, spacecraft like NASA’s Juno and Cassini, and NASA’s Hubble Space Telescope have observed the Jovian system’s changing weather patterns, Webb has already provided new findings on Jupiter’s rings, satellites, and its atmosphere,” study co-author and University of California, Berkeley astronomer Imke de Pater said in a statement.  

The newly discovered jet stream travels at roughly 320 miles per hour and is located close to 25 miles above the clouds, in Jupiter’s lower stratosphere. The team compared the winds observed by JWST at higher altitudes with the winds observed at deeper layers by the Hubble Space Telescope. This enabled them to measure how fast the winds change with altitude and generate wind shears.

[Related: Jupiter formed dinky little rings, and there’s a convincing explanation why.]

The team hopes to use additional observations of Jupiter to determine if the jet’s speed and altitude change over time. 

“Jupiter has a complicated but repeatable pattern of winds and temperatures in its equatorial stratosphere, high above the winds in the clouds and hazes measured at these wavelengths,” Leigh Fletcher, a study co-author and planetary scientists at the University of Leicester in the United Kingdom, said in a statement. “If the strength of this new jet is connected to this oscillating stratospheric pattern, we might expect the jet to vary considerably over the next 2 to 4 years–it’ll be really exciting to test this theory in the years to come.”

The post Why a 3,000-mile-long jet stream on Jupiter surprised NASA scientists appeared first on Popular Science.

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The recent “ring of fire” solar eclipse looked stunning across portions of North and South America and we now have a new view of the stellar event. The Deep Space Climate Observatory (DSCOVR) satellite created the image of the eclipse on Saturday October 14, depicting the mostly blue Earth against the darkness of space, with one large patch of the planet in the shadow of the moon. 

[Related: Why NASA will launch rockets to study the eclipse.]

Launched in 2015, DSCOVR is a joint NASA, NOAA, and U.S. Air Force satellite. It offers a unique perspective since it is close to 1 million miles away from Earth and sits in a gravitationally stable point between the Earth and the sun called Lagrange Point 1. DSCOVR’s primary job is to monitor the solar wind in an effort to improve space weather forecasts. 

A special device aboard the satellite called the Earth Polychromatic Imaging Camera (EPIC) imager took this view of the eclipse from space. According to NASA, the sensor gives scientists frequent views of the Earth. The moon’s shadow, or umbra, is falling across the southeastern coast of Texas, near Corpus Christi.

An annular solar eclipse occurs when the moon moves between Earth and the sun. The sun does not vanish completely in this kind of eclipse. Instead, the moon is positioned far enough from Earth to keep the bright edges of the sun visible. This is what causes the “ring of fire,” as if the moon has been outlined with bright paint.

While this year’s event could be seen to some degree across the continental United States, the 125-mile-wide path of annularity began in Oregon around 9:13 AM Pacific Daylight Time. The moon’s shadow then moved southeast across Nevada, Utah, Arizona, Colorado, and New Mexico, before passing over Texas and the Gulf of Mexico. It continued south towards Mexico’s Yucatan, Peninsula, Belize, Honduras, Nicaragua, Costa Rica, Panama, Colombia, and Brazil

Unlike the colorful Aurora Borealis, eclipses are much easier to predict. Scientists can say when annular and solar eclipses will happen down to the second centuries in advance. The precise positions of the moon and the sun and how they shift over time is already known, so scientists can see how the moon’s shadow will fall onto Earth’s globe. Advances in computer technology have also enabled scientists to even chart eclipse paths down to a range of a few feet.

[Related: We can predict solar eclipses to the second. Here’s how.]

The next annular solar eclipse will be at least partially visible from South America on October 2,2024. One of these ‘ring of fire’ eclipses will not be visible in the United States until June 21, 2039. However, a total solar eclipse will darken the sky from Maine to Texas on April 8, 2024. There is still plenty of time to get eclipse glasses or make a pinhole camera to safely watch the next big celestial event. 

The post What the ‘Ring of Fire’ eclipse looked like to a satellite nearly 1 million miles from Earth appeared first on Popular Science.

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A giant seismic event on Mars—a “marsquake”—that shook the Red Planet last year had an unexpected source, surprising astrophysicists from around the world. They suspected a meteorite strike. Instead, enormous tectonic forces within Mars’s crust, which caused vibrations that lasted for six hours, caused the quake and not a meteorite strike. The findings are described in a study published October 17 in the journal Geophysical Research Letters.

[Related: Two NASA missions combined forces to analyze a new kind of marsquake.]

NASA’s InSight lander recorded the magnitude 4.7 marsquake on May 4, 2022, which scientists named S1222a. Its seismic signal was similar to those of previous quakes that were caused by meteorite impacts, so the team began to search for an impact crater. 

In the new study, a team from the University of Oxford worked with the European Space Agency, Chinese National Space Agency, the Indian Space Research Organisation, and the United Arab Emirates Space Agency to scour more than 55 million square miles on Mars. Each group examined the data coming from its own satellites to look for a crater, dust cloud, or other signature of a meteorite impact. Because the search came up empty, they now believe that S1222a was caused by the release of huge tectonic forces from within the Martian interior. 

That doesn’t mean Mars’s tectonic plates are moving the way they do during an earthquake. The best available evidence suggests the planet is remaining still. “We still think that Mars doesn’t have any active plate tectonics today, so this event was likely caused by the release of stress within Mars’ crust,” study co-author and University of Oxford planetary geophysicist Benjamin Fernando said in a statement. “These stresses are the result of billions of years of evolution; including the cooling and shrinking of different parts of the planet at different rates.”

While Fernando explains that scientists do not fully understand why some parts of Mars seem to have more stress than others, these results can help them investigate further. “One day, this information may help us to understand where it would be safe for humans to live on Mars and where you might want to avoid!” he said.

S1222a was one of the last events recorded by NASA’s InSight mission before its end. The InSight lander launched in May 2018 and survived “seven minutes of terror” to touch down on Mars, where it studied the planet’s interior and seismology for years. The last of the spacecraft’s data was returned in December 2022, after increasing dust accumulation on its solar panels caused InSight to lose power. 

[Related: InSight says goodbye with what may be its last wistful image of Mars.]

In its four years and 19 days of service, InSight recorded more than 1,300 marsquakes. At least eight of these events were from a meteorite impact; the largest two formed craters that were almost 500 feet in diameter. If the S1222a event was formed by an impact, the team estimates that the crater to be would have been at least 984 feet in diameter.

The team is applying knowledge from this study to other work, including future missions to our moon and the tectonics that are similar to California’s famed San Andreas fault located on one of Saturn’s moons named Titan. They also hope that it encourages additional major international collaborations to study the Red Planet and beyond. 

“This has been a great opportunity for me to collaborate with the InSight team, as well as with individuals from other major missions dedicated to the study of Mars,” study co-author and New York University Abu Dhabi astrophysicist Dimitra Atri said in a statement. “This really is the golden age of Mars exploration!”

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Last Friday, NASA launched the Psyche spacecraft toward an asteroid of the same name. Psyche is blazing a trail as the first mission to a metal asteroid, and it’s also about to blaze a literal blue trail. The source of its bright wake—the probe’s remarkable propulsive system—will switch on within the first 100 days of the mission.

A mechanism known as a Hall thruster will propel the Psyche through space. This thruster glows blue as it ionizes xenon, a noble gas also used in headlights and plasma televisions, to move the spacecraft forward. This is the first time this tech, which has only been available for NASA spaceflight since 2015, has been used to travel beyond the moon—but what makes it so special, and why is Psyche using it?

When planning a space mission, engineers are focused on efficiency. Carrying chemical fuel along for the massive interplanetary journey would be like trying to drive around the entire world while having to keep all the gasoline you need in the trunk, because there are no rest stops along the way—it’s just not feasible. To get to its destination, Psyche would need thousands and thousands of pounds of chemical propellant.

[Related: How tiny spacecraft could ‘sail’ to Mars surprisingly quickly]

To get around this problem, engineers turned to electric thrusters. These come in many flavors: “There are many different types of electric thrusters, almost as many as there are different makers of cars,” explained NASA’s Psyche chief engineer Dan Goebel in a blog post. But space travel uses two kinds in particular, known as ion thrusters and Hall thrusters. “They can probably be considered the Tesla versions of space propulsion,” Goebel wrote. Rather than burning fuel, electric thrusters rip off the electrons from the propellant’s atoms in a process known as ionization. Then they chuck those ions out at some 80,000 miles per hour. This generates a higher specific impulse—which Goebel says is “equivalent to miles per gallon in your car,” but for spacecraft—than chemical fuels, enabling a thruster-powered spacecraft to go farther on less propellant.

Ion thrusters use high electric voltages to make a plasma (the fourth state of matter) and spew ions into space. NASA’s Dawn mission used these to get to dwarf planet Ceres, but they’re not the fastest—according to NASA, it would take the spacecraft four days to go from 0 to 60 miles per hour. Definitely not race car material! 

[Related: Want to learn about something in space? Crash into it.]

Hall thrusters, on the other hand, use a magnetic field to swirl electrons in a circle, producing a beam of ions. They don’t get quite as good “mileage” as ion thrusters, but they pack a bigger punch. The Psyche team picked this system because it allowed them to make a smaller, and therefore more cost-efficient, spacecraft. 

For the thrusters to work, the spacecraft needs power—which it gets from the sun, via solar panels—and something to ionize. For Psyche, that’s xenon gas. “Xenon is the propellant of choice because it’s inert (it doesn’t react with the rest of the spacecraft) and is easy to ionize,” explained Goebel. It also gives the thrusters their remarkable blue shine. Psyche carries about 150 gallons of the stuff, and gets about 10 million miles per gallon. 

Now that the mission has launched, the team will spend the next 100 days checking out all the spacecraft’s systems to ensure they’re ready for the journey. At some point in this period, those glimmering blue thrusters will turn on.

If Psyche proves to be a success, Hall thrusters will be likely to make an appearance on future space missions. They offer “the right mix of cost savings, efficiency, and power, and could play an important role in supporting future science missions to Mars and beyond,” said Steven Scott, program manager for the Psyche mission at the company Maxar, which built the thrusters, in a press release. Thanks to these propulsive devices, Psyche should reach its destination in the asteroid belt in just 3.5 years—and we can’t wait to see what lies at the end of its electric blue trail.

The post NASA’s Psyche spacecraft will blaze an unusual blue trail across the solar system appeared first on Popular Science.

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We had a great time checking out the Oct. 14 solar eclipse, but the next one that’s visible here in the U.S. won’t be until April 2024. Lots of interesting things will be happening in the sky between then and now, and you’ll need a good telescope to check them out. Right now, Amazon has substantial discounts on Celestron x PopSci telescopes that were already a solid value. There are three different options currently available depending on your star-gazing needs. Then, when the next eclipse rolls around, you can buy a dedicated solar eclipse filter and get a better look than all those jealous people with their (still pretty cool) pinhole cameras.

Popular Science StarSense Explorer DX 5” Smartphone App-Enabled Telescope $498 (was $599)

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This is the biggest and most powerful scope in the Celestron x PopSci lineup, and it’s just over $100 off right now. Its five-inch aperture and high-end coatings provide a clear, low-aberration image of the night sky. More importantly, it’s compatible with the Celestron app, which can help you find cool things going on in the sky above you and then help you locate them with your scope so you don’t have to go blindly hunting around the heavens. That’s especially important with a scope this powerful.

Popular Science StarSense Explorer DX 100AZ Smartphone App-Enabled Telescope $269 (was $349)

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This 100mm refractor provides a very solid field of view for astrophotography. It’s light and easy to move around, and it’s compatible again with Celestron’s app to guide you around the night sky. Plus, the integrated hood helps combat errant light from hitting the front element of the scope and causing image-ruining glare.

Popular Science AstroMaster 80mm – Portable Refractor Telescope $151 (was $239)

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This model is meant specifically for beginners, and the price makes it very appealing with this discount. The short tub provides a relatively loose view of celestial objects, so beginners won’t get frustrated trying to find specific areas. Plus, the short tube design keeps it small and light, so this is a great scope to keep as a backup for quick jaunts out into dark sky country without lots of gear.

EDITOR’S NOTE: Popular Science has teamed up with Celestron on a line of products. We do earn a commission on its sales—all of which helps power Popular Science.

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Best overall		Sega Toys Homestar Flux		SEE IT	Get a scientifically accurate recreation of the night sky at home.
Best for adults		BlissLights Sky Lite 2.0		SEE IT	Skip the kid stuff without breaking the bank.
Best budget		Infmetry Star Projector		SEE IT	This star light is designed ofor gaming rooms, home theaters,

Beyond a few bright celestial objects, the rise of light pollution has made it difficult for most people to experience a genuinely starry night sky—and that’s where star projectors come in. If artificial lights have obscured your view of the Milky Way, these compact devices provide a fun and comfortable way to observe the cosmos. All you need is a dark room with a power outlet and you’re ready to bask in the wonders of the universe. Many also function as night lights or pattern projectors that can spruce up a room without the celestial theme. While nothing can replace the awe-inspiring feeling of seeing millions of stars in person, the best star projectors can still leave you transfixed.

• Best scientifically accurate: Sega Toys Homestar Flux
• Best portable: NEWSEE Northern Lights Star Projector
• Best for adults: BlissLights Sky Lite
• Best for kids: Gdnzduts Galaxy Projector
• Best budget: Infmetry Star Projector

How we chose the best star projectors

I’ve been fortunate to visit areas less affected by light pollution, so I know what it’s like to gaze upon the grandeur of our galaxy. As an editor at TechnoBuffalo, I visited NASA’s Jet Propulsion Lab in Pasadena, Calif., to learn about the Mars rover. I also took a guided tour of the Goldstone Deep Space Communications Complex, where I saw enormous satellites used to communicate with faraway spacecraft. Over the last 10 years, I’ve written about gadgets and space for outlets like CNN Underscored, TechnoBuffalo, and Popular Science, and this guide, in a way, allows me to write about both. If you’re searching for a projector for movie night, you’re in the wrong place (though we do have a guide for the best projectors for indoors and outdoors). But if you enjoy the stars of the sky as much as you do the stars of the screen, read on.

The best star projectors: Reviews & Recommendations

Whether you’re looking to liven up your space with colorful lights or follow in the footsteps of Carl Sagan, a star projector is a novel way to explore the cosmos. When making our picks, we found a balance between fantastical projectors, options for kids and adults, and a more scientifically accurate model that’s great for those who love astronomy.

Best overall: Sega Toys Homestar Flux

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Why it made the cut: Sega’s Homestar Flux features the most scientifically accurate images out of all the star projectors we picked.

Specs 

• Dimensions: 6.3 x 6.3 x 5.9 inches (LWH)
• Weight: 1.36 pounds
• Power: USB

Pros 

• Supports multiple discs
• Projects up to 60,000 stars at once
• Great educational tool

Cons 

• Expensive

Sega’s Homestar Flux is the closest thing to a planetarium if you’re a fan of astronomy and intend to use your star projector as an educational tool. It can project up to 60,000 stars at once and covers a circle with a 106-inch diameter. Unlike the other star projectors on this list, Sega’s model supports interchangeable discs, allowing owners to explore different parts of the universe in incredible detail. The Homestar Flux comes with two discs, the Northern Hemisphere and the Northern Hemisphere with constellation lines; it also supports additional discs that feature the Andromeda Galaxy, the southern hemisphere, and more. 

These discs contain data from different missions of the National Aeronautics and Space Administration (NASA), the National Oceanic and Atmospheric Administration (NOAA), and the United States Naval Observatory (USNO). While Sega’s projector is pricey, it features the most scientifically accurate experience and is a must-have for would-be astronomers.

Best portable: NEWSEE Northern Lights Star Projector

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Why it made the cut: NEWSEE’s Northern Lights Star Projector lets you take the magic of the stars with you everywhere.

Specs 

• Dimensions: 4.7 x 4.7 x 4.8 inches (LWH)
• Weight: 1.15 pounds
• Power: USB-C

Pros 

• Battery powered
• 360-degree projection
• White noise mode
• Bluetooth streaming

Cons 

• Don’t expect high-fidelity audio

NEWSEE’s Northern Lights Star Projector is the only model we’re recommending that can be taken anywhere. The battery-powered projector can run for a couple of hours before needing to be recharged—though because it has a USB-C port, you can plug it into a portable charger to extend its life. The projector sits on a stand and can be rotated so that you can find the best angle for your room. This flexibility comes in handy because you may be using the projector in multiple rooms because of its portability.

You can program NEWSEE’s projector to display one of four different star patterns, and play five different white noises. This star projector can even be used as a Bluetooth speaker for playing any music from your digital library. However, you shouldn’t get your hopes up where audio fidelity is concerned—consider this a fun bonus feature. If you want to take a star projector to a friend’s place or on vacation, this is the one to grab.

Best for adults: BlissLights Sky Lite

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Why it made the cut: The Sky Lite from BlissLights will help you set the mood with the right lighting.

Specs 

• Dimensions: 5.95 x 2.91 x 5.95 (LWH)
• Weight: 1.68
• Power: AC adapter

Pros 

• Adjustable brightness
• Tilting base
• App controlled

Cons 

• Projector design is easy to tip over

The Sky Lite from BlissLights is an excellent option for adults because it offers brightness controls, and several lighting effects, making it easy to set the proper mood. While star projectors generally become the center of attention in whatever room they’re in, the Sky Lite is excellent as complementary lighting, casting colorful auroras during dinner, movie nights, and parties. Additionally, the Sky lite 2.0 supports a rotation feature and a shutoff timer so that you can have your magical night under the stars before nodding off to bed. 

Best for kids: Gdnzduts Galaxy Projector

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Why it made the cut: This galaxy projector features brightness controls and a shutoff timer, plus it doubles as a colorful night light.

Specs 

• Dimensions: 6.45 x 6.45 x 4.92 (LWH)
• Weight: 0.61 pounds
• Power: USB

Pros 

• Built-in speaker
• Shutoff timer
• Brightness controls

Cons 

• Doesn’t show constellations

This simple galaxy projector features 21 lighting effects, a shutoff timer, brightness controls, and doubles as a night light. That way, you can find the right effect you like, adjust the brightness, and set a timer before bed. You can also toggle the lasers on and off, turning off the stars and letting the nebula-like effect lull you to sleep. The Galaxy Projector also comes with a remote, making it easy for kids to operate. Whether you want to inspire your kid’s imagination or keep them feeling safe with a night light, the Galaxy Projector is an excellent choice.

Best budget: Infmetry Star Projector

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Why it made the cut: Infmetry’s Star Projector offers an array of features at an affordable price.

Specs 

• Dimensions: 7.1 x 7.1 x 7.5 inches (LWH)
• Weight: 1.37 pounds
• Power: USB

Pros 

• Affordable
• Five brightness modes
• Shutoff timer

Cons

• No nebula or aurora features

Infantry’s Star Projector casts 360 degrees of light through a precut dome, creating a night sky-like effect. This model also supports five brightness modes, a breathing mode, and four colors (white, yellow, blue, and green). There’s also a shutoff timer, so you can fall asleep with the projector on and wake up with it off. It’s not nearly as captivating as the other options on this list, but for the price, it’s a fun way to introduce someone to the wonders of the universe.

What to consider when buying the best star projectors

Generally, cheap star projectors are novelties that emit a mix of colorful swirling LED lights and class 2 lasers, which are low-power visible lasers—the same type used in laser pointers. While most models aren’t scientifically accurate, they provide a fanciful escape and can offer a calming experience. However, if you’re serious about astronomy and willing to spend more, you can find a star projector that can turn your room into a personal planetarium.

Most models we researched offer features like brightness and color controls, image rotation, and an automatic shut-off timer. We found picking the right star projector is more about finding the experience that matches your mood. Are you looking for the cosmic color of nebulae? What about scientifically accurate constellations? Whatever you’re after, there’s a star projector for everyone.

Projection type

You’d think that a star projector only projects, well, stars. But many of them can cover the broad cosmic spectrum and mimic everything from nebulae to auroras to constellations. As we mentioned, picking the right one is about capturing your interest and imagination. A projector that can cast a nebula or aurora is an excellent choice if you want to create a calming environment before going to sleep. A star projector with more scientifically accurate images is ideal for studying and educational use.

Brightness control

A good star projector uses an LED bulb and offers multiple brightness settings. While star projectors are most effective in a dark room, the models that project nebula and aurora make for great complementary lighting, such as during a party or movie night. They also make for good night lights and can help create a calming environment that encourages rest.

Color settings

In addition to adjusting brightness, most star projectors offer different color settings, similar to smart light bulbs. Users can create a scene that fits their mood through advanced color settings and change it with the press of a button. A green aurora may be suitable for calm and tranquility, while yellow may be ideal for happiness and optimism. Most star projectors allow color adjustments through a controller or smartphone app and support millions of color options.

Still vs. rotating

Star projectors generally offer different viewing modes: still and rotating. A projector that operates in still mode will cast light onto a surface and remain static. A projector with a rotating feature will put on a more dynamic light show by slowly rotating the lights. Many of the models we looked at are capable of switching between still and rotating modes.

Extra features

Beyond simply projecting lights onto a wall, some star projectors include extra features like white noise, app support, and shutoff timers. Some models can even be synced with your music so that you can put on a cosmic light show. While these features aren’t necessary, they make specific models more appealing, especially if you intend to use a star projector in a child’s room, because it can act as a night light and white noise machine and then shut off after a few hours.

FAQs

Final thoughts on the best star projectors

• Best scientifically accurate: Sega Toys Homestar Flux
• Best portable: NEWSEE Northern Lights Star Projector
• Best for adults: BlissLights Sky Lite
• Best for kids: Gdnzduts Galaxy Projector
• Best budget: Infmetry Star Projector

Star projectors are a fun and affordable way to add bright, colorful lights to your bedroom. That said, most are nothing more than novelties and put on light shows that vaguely resemble nebulae and auroras. If you’re searching for something with more scientifically accurate imagery, you can find some excellent options if you don’t mind spending more money. Better yet, we recommend traveling to a place unaffected by light pollution and experiencing the feeling of seeing millions of stars in person.

Why trust us

Popular Science started writing about technology more than 150 years ago. There was no such thing as “gadget writing” when we published our first issue in 1872, but if there was, our mission to demystify the world of innovation for everyday readers means we would have been all over it. Here in the present, PopSci is fully committed to helping readers navigate the increasingly intimidating array of devices on the market right now.

Our writers and editors have combined decades of experience covering and reviewing consumer electronics. We each have our own obsessive specialties—from high-end audio to video games to cameras and beyond—but when we’re reviewing devices outside of our immediate wheelhouses, we do our best to seek out trustworthy voices and opinions to help guide people to the very best recommendations. We know we don’t know everything, but we’re excited to live through the analysis paralysis that internet shopping can spur so readers don’t have to.

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On Saturday, October 14, you’ll be able to watch an annular “ring of fire” eclipse as the moon passes in front of the sun at a distance where it’s unable to cover all of Earth’s nearest star. But only an exclusive crowd will be able to witness the event in its fully blazing glory—unless you know where to look.

Although it may be too late to travel to one of the best locations to watch this year’s final solar eclipse, nearly everyone in all 50 US states will have a chance to catch at least a glimpse (sorry western Alaska and western Hawaii). The 125-mile-wide path of annularity, however, will stretch from Oregon to Texas and cross just nine states before continuing on to Central and South America. You’ll only be able to see the sun form a fiery halo around the moon along that route. If you’re outside its range, you can simply load up one of several official livestreams to see what you’re missing.

How to watch the October 14, 2023 eclipse in person

The path of annularity will enter the US in Oregon at 12:13 p.m. Eastern Time (9:13 a.m. Pacific Time) and leave Texas at 1:30 p.m. ET (12:03 p.m. Central Time). The “ring of fire,” will pass over 29 national park sites and dozens of other pieces of public land. Worldwide, about 33 million people will be able to see it firsthand, while everyone else will have to settle for a less dramatic experience.

No matter where you are, make sure you’re wearing protective glasses to avoid damaging your eyes if you plan to look directly at the eclipse, or make a pinhole camera to project the event onto a sheet of paper. And of course, weather conditions may make it hard or impossible to see anything, so take note of the forecast.

If you want to know exactly what to expect where you are, astronomy website Time and Date has an interactive map that will help you set your eclipse-viewing plans. Once you’ve opened the map, click the magnifying glass icon on the left to open the search menu. Type the name of any city or town into the search bar and select it from the list that populates underneath. A pin will appear on the map and a box full of eclipse data will show up under the search bar.

That data will show you how much of the moon will cover the sun at that location, when the eclipse will begin and end there, when maximum coverage will occur, and the weather forecast for that spot on the globe. If you click the play icon next to the duration, you’ll go to another page where you can watch a simulation of what the eclipse will look like at that exact spot.

How to watch the annular “ring of fire” eclipse online

Just because you aren’t part of the 0.41 percent of people in the world who will be able to physically bear witness to the celestial spectacle doesn’t mean you’re stuck with whatever’s happening in the sky above you. All you have to do is turn your eyes away from the wonders of the natural world and look at a screen—there are four livestreams we think will offer an exquisite show.

The Exploratorium’s livestreams

The San Francisco-based Exploratorium will be broadcasting two livestreams starting at 8 a.m. PT (11 a.m. ET), one from their telescopes in Valley of the Gods, Utah, and another from their telescopes in Ely, Nevada. They will also broadcast Spanish-language coverage of the event starting at 9 a.m. PT (12 p.m. ET) on YouTube.

According to Time and Date, annularity—the “ring of fire”— will last 4 minutes and 46 seconds at the Valley of the Gods. There are morning clouds in the forecast, though, so the view might be obscured, but this has the potential to be the most scenic livestream on our list. 

• Eclipse start: 9:10 a.m. Mountain Time (11:10 a.m. ET)
• “Ring of fire” start: 10:29 a.m. MT (12:29 p.m. ET)

In Ely, meanwhile, annularity will last for 3 minutes and 38 seconds. The weather is expected to be partly cloudy, so the eclipse could be hard to see.

• Eclipse start: 8:07 a.m. PT (11:07 a.m. ET)
• “Ring of fire” start: 9:24 a.m. PT (12:24 p.m. ET)

Time and Date’s livestream

Time and Date’s eclipse chasers will be broadcasting a livestream from Roswell, New Mexico. There, according to the website’s own interactive map, the annularity will last for 4 minutes and 41 seconds. It’s expected to be sunny there, so the view should be clear.

• Eclipse start: 9:15 a.m. MT (11:15 a.m. ET)
• “Ring of fire” start: 10:38 a.m. MT (12:38 p.m. ET)

NASA’s livestreams

NASA, of course, will also be livestreaming the eclipse, with feeds from Kerrville, Texas, and Albuquerque, New Mexico, starting at 11:30 a.m. ET. Annularity will last 4 minutes and 14 seconds at Kerrville, according to Time and Date.

• Eclipse start: 10:22 a.m. CT (11:22 a.m. ET)
• “Ring of fire” start: 11:50 a.m. CT (12:50 p.m. ET)

At Albuquerque, which is supposed to have sunny skies during the eclipse, annularity will last 4 minutes and 48 seconds.

• Eclipse start: 9:13 a.m. MT (11:13 a.m. ET)
• “Ring of fire” start: 10:34 a.m. MT (12:34 p.m. ET)

The space agency will also be broadcasting a live feed of three rocket launches that are part of its Atmospheric Perturbations around the Eclipse Path (APEP) mission to study how Earth’s ionosphere responds to a sudden drop in sunlight. You might want to cue that one up in a different browser window alongside the eclipse, or set up picture-in-picture on your device.

Whatever you do, just know that your scheduling calculations and technological machinations are probably way less complicated than all the math scientists do to predict the paths of future eclipses.

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The powdery material that NASA officials unveiled on Wednesday looked like asphalt or charcoal, but was easily worth more than its weight in diamonds. The fragments were from a world all their own—pieces of the asteroid Bennu, collected and returned to Earth for analysis by the OSIRIS-REx mission. The samples hold chemical clues to the formation of our solar system and the origin of life-supporting water on our planet.

The clay and minerals from the 4.5 billion-year-old rock had been preserved in space’s deep freeze since the dawn of the solar system. Last month, after a seven-year-long space mission, they parachuted to a desert in Utah, where they were whisked away by helicopter. 

And now those pristine materials sit in an airtight vessel in a clean room at NASA’s Johnson Space Center, where researchers like University of Arizona planetary scientist Dante Lauretta are getting their first chance to study the sample up close. 

“The electron microscopes were fired up and ready” by September 27, Lauretta said in a news conference. “And boy did we really nail it.” (Lauretta, the principal investigator, gave the mission its name, which stands for Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer.) The preliminary investigation of a tiny fraction of the sample revealed it is rich in water, carbon, and organic compounds.

Carbon is essential for all living things on Earth, forming chemical bonds with hydrogen, oxygen, and other elements necessary to build proteins and enzymes. “We’re looking at the kinds of minerals that may have played essential roles in the origin of life on Earth,” Lauretta said. 

The Bennu sample contained about 4.7 percent carbon, as measured by the Carnegie Institution for Science, according to Daniel Glavin, the OSIRIS-REx sample analysis lead at NASA’s Goddard Space Flight Center. This is “the highest abundance of carbon” the Carnegie team has measured in an extraterrestrial sample, Glavin said. “There were scientists on the team going ‘Wow, oh my God!’ And when a scientist says that ‘Wow;’ that’s a big deal.”

[Related: This speedy space rock is the fastest asteroid in our solar system]

The Bennu sample is also flush with organic compounds, too, which glowed like tiny stars within the dark sample when exposed to a black light. “We picked the right asteroid—and not only that, we brought back the right sample,” Glavin said. “This stuff is an astrobiologist’s dream.”

Asteroids like Bennu were most likely responsible for all of Earth’s wet features—the water in oceans, lakes, rivers, and rain probably arrived when space rocks landed on our young planet some 4 billion years ago. Bennu has water-bearing clay with a fibrous structure, which according to Lauretta, was the key material that ferried H₂O to Earth.

Under magnification, the clay has a sinuous shape. “We call this serpentine because they look like serpents or snakes inside the sample, and they have water locked inside their crystal structure,” he said. “That is how we think water got to the Earth.”

This is only the start. The OSIRIS-REx science team, as they catalog the sample, have months of more detailed work ahead. After six months, they will publish the catalog; scientists from around the world will be able to propose studies using the materials—though more than half the sample will be kept in reserve for research to take place years or even decades in the future. 

[Related: NASA’s mission to a weird metal asteroid will blast off … soon]

They have more than a half-pound of material to work with. OSIRIS-REx recovered an estimated 250 grams of Bennu material, more than four times the 60 grams the mission had targeted. And as the science team began dissembling the sample return capsule at Johnson Space Center, they discovered what NASA is calling bonus material: bits of Bennu adhering to the collector head and lid of the sealed canister that brought the bulk of the sample home. 

”The first thing we noticed was that there was black dust and particles all around the outer edge,” Lauretta said. “Already this is scientific treasure.”

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The 2018 winner of PopSci’s annual Best of What’s New continues to impress. NASA’s Parker Solar Probe is still edging closer to the sun than any other spacecraft has ever achieved, and it’s setting new speed records in the process. According to a recent status update from the space agency, the Parker Solar Probe has broken its own record (again) for the fastest thing ever made by human hands—at an astounding clip of 394,736 mph.

The newest milestone comes thanks to a previous gravity-assist flyby from Venus, and occurred on September 27 at the midway point of the probe’s 17th “solar encounter” that lasted until October 3. As ScienceAlert also noted on October 9, the Parker Solar Probe’s speed would hypothetically allow an airplane to circumnavigate Earth about 15 times per hour, or skip between New York City and Los Angeles in barely 20 seconds. Not that any passengers could survive such a journey, but it remains impressive.

[Related: The fastest human-made object vaporizes space dust on contact.]

The latest pass-by also set its newest record for proximity, at just 4.51 million miles from the sun’s plasma “surface.” In order not to vaporize from temperatures as high as nearly 2,500 degrees Fahrenheit, the Parker Solar Probe is outfitted with a 4.5-inch-thick carbon-composite shield to protect its sensitive instruments. These tools are measuring and imaging the sun’s surface to further researchers’ understanding of solar winds’ origins and evolution, as well as helping to forecast environmental changes in space that could affect life back on Earth. Last month, for example, the probe raced through one of the most intense coronal mass ejections (CMEs) ever observed. In doing so, the craft helped prove a two-decade-old theory that CMEs interact with interplanetary dust, which will improve experts’ abilities in space weather forecasting.

Despite its punishing journey, NASA reports the Parker Solar Probe remains in good health with “all systems operating normally.” Despite its numerous records, the probe is far from finished with its mission; there are still seven more solar pass-bys scheduled through 2024. At that point (well within Mercury’s orbit), the Parker Solar Probe will finally succumb to the sun’s extreme effects and vaporize into the solar winds— “sort of a poetic ending,” as one mission researcher told PopSci in 2021.

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The James Webb Space Telescope (JWST) is showing off its imaging prowess again, this time with a stellar image of NGC 346. This is the brightest and biggest star-making region in a satellite galaxy of the Milky Way called the Small Magellanic Cloud (SMC). The SMC is about 21,000 light-years away in the southern constellation Tucana. 

[Related: JWST takes a jab at the mystery of the universe’s expansion rate.]

The image that looks like Edgar Allan Poe’s ominous raven in some angles was taken using Webb’s Mid-Infrared Instrument (MIRI). The blue wisps of light show emissions from molecules like silicates and polycyclic aromatic hydrocarbons. The red fragments highlight dust that is warmed by the largest and brightest stars in the center.

An arc at the center left might be a reflection of light from the star near the center of the arc, and similar curves appear to be associated with strats at the lower left and upper right. The bright patches and filaments denote areas with large numbers of protostars. While looking for the reddest stars, the research team found 1,001 pinpoint sources of light. Most of these are young stars still snuggled up in their dusty cocoons.

This SMC is more primeval than the Milky Way since it possesses fewer heavy elements. According to NASA, these elements are forged in stars through nuclear fusion and supernova explosions, compared to our own galaxy.

“Since cosmic dust is formed from heavy elements like silicon and oxygen, scientists expected the SMC to lack significant amounts of dust,” NASA wrote in a press release. “However the new MIRI image, as well as a previous image of NGC 346 from Webb’s Near-Infrared Camera released in January, show ample dust within this region.”

Astronomers can combine JWST’s data in both the near-infrared and mid-infrared data to take a fuller census of the stars and protostars within this very dynamic region of space. This could help us better understand the galaxies that have existed billions of years ago, during an era known as Cosmic Noon. During Cosmic Noon, star formation was at its peak. Heavy element concentrations were lower, which we can see when we study the SMC.

[Related: The Whirlpool Galaxy’s buff, spiral arms grab JWST’s attention.]

This raven-like image is not the first JWST image that is picture perfect for spooky season. In September 2022, it released chilling new images of 30 Doradus aka the Tarantula Nebula. The nebula’s arachnid inspired nickname comes from its similar appearance to a burrowing tarantula’s silk-lined home. The Tarantula Nebula is about 161,000 light-years away from Earth in the Large Magellanic Cloud galaxy, which is home to some of the hottest and biggest stars known to astronomers.

JWST has also imaged the “bones” of  IC 5332, a spiral galaxy over 29 million light years away from the Earth in the constellation Sculptor. The uniquely shaped galaxy has a diameter of roughly 66,000 light years, making it slightly larger than our Milky Way galaxy. The MIRI aboard the new telescope observes the furthest reaches of the universe and can see infrared light, so it’s able to peer through the galaxy’s clouds of dust and into the “skeleton” of stars and gas underneath its signature arms. MIRI basically was able to take an x-ray of a galaxy, revealing IC 5332’s bones and a world that looks different, yet somewhat the same.

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On October 10, the European Space Agency (ESA) published some interim data from its nearly a decade-long Gaia mission. The data includes half a million new and faint stars in a massive cluster, over 380 possible cosmic lenses, and the position of over 150,000 asteroids within the solar system. 

[Related: See the stars from the Milky Way mapped as a dazzling rainbow.]

Launched in December 2013, Gaia is an astronomical observatory spacecraft with a mission to generate an accurate stellar census, thus mapping our galaxy and beyond. A more detailed picture of Earth’s place in the universe could help us better understand the diverse objects that make up the known universe. 

500,000 new stars and cluster cores

In 2022, Gaia’s third data release (DR3) contained data on over 1.8 billion stars, which built a rather complete view of the Milky Way and beyond. Even with all that data, there were still gaps in the ESA’s mapping. Gaia still hadn’t fully explored areas of the sky that were particularly densely packed with stars, overlooking the stars that shine a little less brightly than their neighbors. 

A key example of this is in globular clusters. These are some of the oldest objects in the known universe and are especially valuable for looking back into our cosmic past. However, their bright cores can sometimes overwhelm telescopes trying to get a clear view. 

Gaia selected Omega Centauri to help fill in the gaps in the stellar map. Omega Centauri is the largest globular cluster that can be seen from Earth and is a good example of one of the galaxy’s more ‘typical’ clusters. Gaia enabled a special mode to truly map a wider patch of sky that is surrounding the cluster’s core whenever the cluster came into view.

“In Omega Centauri, we discovered over half a million new stars Gaia hadn’t seen before – from just one cluster!” study co-author and astrophysicist from the Leibniz-Institute for Astrophysics Potsdam (AIP) Katja Weingrill said in a statement. “We didn’t expect to ever use it for science, which makes this result even more exciting.”

The data also allowed the team to detect new stars that are too close together to be properly measured.

“With the new data we can study the cluster’s structure, how the constituent stars are distributed, how they’re moving, and more, creating a complete large-scale map of Omega Centauri. It’s using Gaia to its full potential—we’ve deployed this amazing cosmic tool at maximum power,” study co-author and AIP astrophysicist Alexey Mints said in a statement. 

The half million new stars showed that Omega Centauri is one of the most crowded regions that Gaia has explored so far. 

Currently, Gaia is exploring eight more regions using these same techniques. The scoop from those exploration will be included in Gaia Data Release 4. It should help astronomers truly understand what is happening within these cosmic building blocks and more accurately confirm the age of our galaxy.

Spotting gravitational lenses 

Gravitational lensing happens when the image of a faraway object in space becomes warped by a disturbing mass, such as a galaxy or star, sitting between the observer and the object. The mass in the middle acts like a giant lens that can magnify the brightness of light and cast multiple images of the faraway source onto the sky. 

[Related: Gravitational Lens Splits Supernova’s Light 4 Different Ways.]

“Gaia is a real lens-seeker,” study co-author and Laboratoire d’Astrophysique de Bordeaux astrophysicist Christine Ducourant  said in a statement. “Thanks to Gaia, we’ve found that some of the objects we see aren’t simply stars, even though they look like them.”

Some of the objects here are not ordinary stars, but distant quasars. These quasars are extremely bright, high-energy galaxies powered by black holes. To date, Gaia has found 381 candidates for lensed quasars. This is a “goldmine” for cosmologists, says Ducourant , and the largest set of candidates ever detected at once. 

Detecting lensed quasars is challenging, since a lensed system’s constituent images can clump together on the sky in misleading ways.

“The great thing about Gaia is that it looks everywhere, so we can find lenses without needing to know where to look,” study co-author and Université Côte d’Azur astrophysicist Laurent Galluccio said in a statement. “With this data release, Gaia is the first mission to achieve an all-sky survey of gravitational lenses at high resolution.”

Asteroids and The Milky Way

One of the studies in this data release reveals more about 156,823 asteroids, pinpointing their positions over nearly double the previous timespan. In the fourth Gaia data release, the team plans to complete the set and include comets, planetary satellites, and double the number of asteroids.

[Related: Smashed asteroid surrounded by a ‘cloud’ of boulders.]

Another study maps the disc of the Milky Way by tracing the weak signals seen in starlight, faint imprints of the gas and dust that floats between the stars. The Gaia team stacked six million spectra to study these signals and the data will hopefully allow scientists to finally narrow down the source of these signals.

“This data release further demonstrates Gaia’s broad and fundamental value—even on topics it wasn’t initially designed to address,” study co-author and ESA Project Scientist Timo Prusti said in a statement. “Although its key focus is as a star surveyor, Gaia is exploring everything from the rocky bodies of the solar system to multiply imaged quasars lying billions of light-years away, far beyond the edges of the Milky Way. The mission is providing a truly unique insight into the Universe and the objects within it, and we’re really making the most of its broad, all-sky perspective on the skies around us.”

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On October 14, the Western Hemisphere will witness an annular solar eclipse. The moon will be too small and far away in our view to totally block out the sun’s disc. Instead, it will blot out its center, leaving a ring at the edges. The best locations to view that ring of fire in the sky will be along a path that cuts through Oregon, Texas, Central America, Colombia, and finally northern Brazil. You might decide to visit Albuquerque, New Mexico, where you’ll experience exactly 4 minutes and 48 seconds of an annular eclipse.

And if you’re seeking a true total eclipse, you only have to wait another six months. On April 8, 2024, at 2:10 p.m. Eastern (12:10 p.m. local time), Mazatlan, Mexico will become the first city in North America to see most of the sun vanish in shadow. The path of totality then arcs through Dallas and Indianapolis into Montréal, New Brunswick, and Newfoundland in Canada. We know all of these precise details—and more—thanks to our knowledge of where the moon and sun are situated in the sky at any given moment.

In fact, we can predict and map eclipses farther into the future, even centuries from now. Because they know the precise positions of the moon and the sun and how they shift over time, scientists can project the moon’s shadow onto Earth’s globe. And with cutting-edge computers, it’s possible to chart eclipse paths down to a range of a few feet.

A solar eclipse needs three things. It results when the moon blocks the sun’s light from our vantage point on Earth. So to predict an eclipse, you must know where and how the sun, moon, and Earth move in relation to each other. This isn’t quite as elementary as it may seem, because the solar system isn’t flat. The moon’s orbit slants about 5 degrees in relation to the sun’s path, which astronomers call the ecliptic. While our satellite passes between Earth and the sun around once a month—which we call a new moon—the two rarely seem to cross paths.

Solar eclipses can only occur when the moon is at one of the two points where the moon’s orbit crosses the ecliptic, known as a node. If the moon is new at this crossing, the result is a solar eclipse.

In centuries past, trying to predict eclipses meant predicting minute details of finicky orbits. But as astronomers learned more about how celestial objects moved, they began tabulating what they call ephemerides: predictions of where the moon, sun, and planets will be in the sky. Ephemerides are still the key to eclipse prediction.

[Related: Make a classic pinhole camera to watch the upcoming solar eclipse]

“All you need is the ephemeris data…you don’t have to actually track the orbit,” says C. Alex Young, a solar physicist at NASA’s Goddard Space Flight Center.

With ephemeris data, astronomers can pinpoint dates and times when the moon and sun cross paths. Once you know that date, mapping an eclipse is relatively straightforward. Ephemerides let scientists project the moon’s shadow onto Earth’s sphere; with 19th-century mathematics, they can calculate the shape and latitude of two features of that shadow, the umbra and penumbra. Then, by knowing what time it is and where Earth is angled in its rotation, it’s possible to determine the longitudes. Putting these together produces an eclipse map.

In the past, astronomers printed the ephemerides in almanacs, long tomes filled with page after page of coordinate tables. Just as all of astronomy has advanced into an era of computers, so have ephemerides. Scientists today mathematically model the paths of the moon, sun, planets, other moons, asteroids, and much more.

NASA’s Jet Propulsion Laboratory (JPL) regularly publishes a new compendium of celestial locations every few years. The most recent edition, 2021’s DE440, accounts for details like the moon’s core and mantle sloshing around and slowing its rotation. “Generally speaking, we know where the moon is from the Earth to about a meter, maybe a couple of meters,” says Ryan Park, an engineer at JPL. “We typically know where the sun is to maybe a couple hundred meters, maybe 300 meters.”

[Related: How to look at the eclipse without damaging your eyes]

Ephemerides serve other purposes, especially when planning spaceflight missions. But it’s largely due to more sophisticated ephemeris data that we can now reliably predict the motions of the moon for the centuries ahead. In fact, you can find detailed maps of solar eclipses nearly a millennium in the future. (If you’re lucky enough to be in Seattle on April 23, 2563 or in Amsterdam on September 7, 2974, prepare for total eclipse day.)

But these maps, like most eclipse maps, show the path of totality or annularity as a smooth line crossing Earth’s surface. That isn’t an accurate representation. “This was designed for pencil and paper calculation, so it makes a lot of simplifying assumptions that are just a tiny bit wrong,” says Ernie Wright, who makes eclipse maps for NASA Goddard, “for instance that the moon is a perfectly smooth sphere.”

Both the moon and Earth are jagged at the edge. Earth’s terrain can block some views of the sun, and the moon has its own patchwork of mountains and valleys. In fact, sunbeams passing through lunar vales create the Baily’s beads and “diamond ring” often seen at an eclipse’s edge. “We now have detailed terrain information of these mountains from the Lunar Reconnaissance Orbiter,” Young says.

Wright has helped devise a new way of mapmaking that swaps the Victorian-age mathematics out for modern computer graphics. His method turns Earth’s surface into a map of pixels, each one with different latitude, longitude, and elevation, with the sun and moon in the sky above. Then, the method calculates which pixels see which parts of the moon block which parts of the sun. 

“You then make a whole sequence of maps at, say, one-second intervals for the duration of the eclipse,” Wright says. “You end up with a frame sequence that you can put together to make a movie of the shadow.” This new technique—only possible with modern computers and ultraprecise ephemerides—may allow us to make eclipse maps that clearly show whether you can see an eclipse from, say, your house. 

“I think that’s going to provide a whole new set of maps in the future that are going to be much more accurate,” says Young. “It’s going to be pretty exciting.”

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NASA’s Artemis III astronauts are apparently going to look incredibly fashionable walking the lunar surface. On October 4, the commercial aerospace company Axiom Space announced a new collaboration with luxury fashion house Prada to design spacesuits for the upcoming moon mission currently scheduled for 2025.

According to Wednesday’s reveal, Prada’s engineers will assist Axiom’s systems team in finalizing its Axiom Extravehicular Mobility Unit (AxEMU) spacesuit while “developing solutions for materials and design features to protect against the unique challenge of space and the lunar environment.” Axiom CEO Michael Suffredini cited Prada’s expertise in manufacturing techniques, innovative design, and raw materials will ensure “not only the comfort of astronauts on the lunar surface, but also the much-needed human factors considerations absent from legacy spacesuits.”

[Related: Meet the first 4 astronauts of the ‘Artemis Generation’.]

NASA first unveiled an early prototype of the AxEMU spacesuit back in March, and drew particular attention to the fit accommodating “at least 90 percent of the US male and female population.” Given the Artemis mission has long promised to land the first woman on the lunar surface, such considerations are vital for astronauts’ safety and comfort.

In Wednesday’s announcement, Lorenzo Bertelli, Prada’s Group Marketing Director, cited the company’s decades of technological design and engineering experience. Although most well known for luxury fashion, Prada is also behind the cutting-edge Luna Rossa racing yacht fleet.

“We are honored to be a part of this historic mission with Axiom Space,” they said. “It is a true celebration of the power of human creativity and innovation to advance civilization.”

Despite Prada’s association with high fashion, the final AxEMU design will undoubtedly emphasize safety and function over runway appeal. After all, astronauts will need protection against both solar radiation and the near-vacuum of the lunar surface, as well as ample oxygen resources and space for HD cameras meant to transmit live feeds back to Earth. According to the BBC earlier this year, each suit will also incorporate both 3D-printing and laser cutters to ensure precise measurements tailored to each astronaut.

Although NASA’s first images of the AxEMU in March showcased a largely black-and-gray color palette with blue and orange accents, Axiom Space’s newest teases hint at an off-white cover layer more reminiscent of the classic Apollo moon mission suits. It might not be much now, but you can expect more detailed looks at the spacesuits in the coming months as the Artemis Program continues its journey back to the moon.

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It’s a well-known fact that staring at the sun is… not the best idea. In the same way that the sun can burn your skin, our home star can overwhelm your peepers with UV rays and literally scorch your retina.

That is a huge bummer, especially because watching a solar eclipse (when the moon covers the sun) is an incredibly cool experience. Thankfully, there are several ways to watch an eclipse without risking your vision, and one of them is building a pinhole camera out of a box, a piece of aluminum foil, and lots of tape. This is an easy and incredibly versatile project, and you can turn it into a permanent camera obscura when you’re done watching the eclipse. 

How to make a pinhole camera

1. Light-proof your box. Leaving one side open, use duct tape or electrical tape to seal the box and prevent any light rays from sneaking in. Pay special attention to the corners and wherever two pieces of cardboard meet. The pinhole will only allow a few rays of light into your box, so the projection of the sun will be dim. That means the darker your camera, the easier it will be to see the image.

As we said, this project is versatile. You can use a wide range of box sizes to make your pinhole camera, but cereal and shoe boxes work exceptionally well. We used the 15-by7 ½-by-5 ½-inch box that carried our neighbor’s latest online shopping spurt. 

Likewise, duct tape and electrical tape are the best choices to light-proof your box, but you can use any tape that will block light—dark washi tape or masking tape will also do the trick. Just keep in mind that you may have to apply multiple layers to achieve total darkness inside your box. 

[Related: A ‘ring of fire’ eclipse and Hunter’s Moon will bring lunar drama to October’s skies]

• Pro tip: Check your work by holding your box up to a light and looking inside. If you still see some shine coming through, apply another layer of tape. 

2. Determine your pinhole’s location and cover the inside of the opposite face with white paper. Measure one of the smallest sides of the box, cut a piece of white paper to the same size, and tape or glue it to the inside of the corresponding face. It doesn’t have to be perfect—as long as most of the side is covered, you’ll be good to go. Just make sure that the paper doesn’t have any wrinkles or folds, as they may distort the image of the sun. 

3. Measure the openings for the pinhole and the viewer. On the side opposite the one you covered with white paper, use your ruler and a pencil to measure two openings. The pinhole opening will be located in the upper left corner (about half an inch from the edges) and will be 2-by-2 inches (we’ll make it smaller later). 

The viewing opening will be located in the upper right corner of the box, half an inch from the top edge and an inch from the right edge of the box. This opening will be smaller—only 1 inch square.

4. Cut the openings. Using a box cutter or scissors, cut out the openings you drew. 

• Pro tip: If the openings end up being too big, don’t sweat it—you can always adjust their size with tape. 

5. Close and seal the box. Use your newly cut openings to make sure there are no other places where light might be sneaking in. Pay special attention to the corners of the box above and below your openings. Cover all the places where pieces of cardboard meet with tape. 

6. Cover the larger opening with aluminum foil. Cut a smooth 2 ½-by-2 ½-inch piece of aluminum foil. With the dull side facing you, carefully cover the big opening with the metallic sheet and tape it in place. Make sure you secure it tightly so no light can get into the box.  

• Pro tip: To smooth out any creases, softly rub the top of any fingernail over the foil in a small, circular motion. 

7.  Use the thumbtack to poke a hole in the foil. Find the rough center of the 2-by-2-inch square under the aluminum sheet and gently push the tack through before pulling it back out—you want a clean, round hole. If you don’t have a thumbtack, you can use the tip of a toothpick or an embroidery needle. Just make sure that whatever you’re using has a point (it’ll make a neater hole) and that it’s approximately 0.2 millimeters wide. 

• Note: The width of your pinhole will determine how much light gets into the box. Too much light and the image will be blurry. If that’s the case, don’t worry—just replace the foil and try making a smaller pinhole. 

8. Put your pinhole camera to the test. Stand with your back facing the sun and look into the box through the viewport. Use your hands to block out as much light as possible and move around until you find the angle where sunlight enters through the pinhole. When this happens, you should see a small projection of the shape of the sun on the white paper you pasted inside the box. 

[Related: Total eclipses aren’t that rare—and you’ve probably missed a bunch of them]

Keep in mind that the weather is crucial in determining the quality of the image you’ll see inside your pinhole camera, and whether you can see the eclipse at all. The October 14 eclipse, in particular, will be annular, so the moon will be smaller than the sun and clouds, rain, or other inclement weather will make it hard to see the event, explains Franck Marchis, a SETI Institute astronomer and the chief scientific officer of Unistellar, a company that manufactures smart telescopes.

How a pinhole camera works

Images are light. Everything we see we perceive because there’s light bouncing off of it, beaming directly through our pupils and into our eyes. All cameras, including the humble pinhole camera you just made, operate under this basic principle. The better they filter the light, the sharper the resulting image will be. 

The sun, of course, is the ultimate light source. On a sunny day, rays from the star travel to Earth and bounce off of every surface they reach. This is a lot of light coming from all directions, so if we want to see only a small portion of the sun’s rays, we have to focus those rays and filter out the rest. That’s why the pinhole in your camera is so tiny or, in more technical terms, why its aperture is so narrow—it only lets a small amount of light into the box, just enough so you can see only a dim projection of the sun when you point the pinhole directly at it. 

The dimness of the image is not ideal, but it’s the tradeoff we make for sharpness—too much light results in a blurry, out-of-focus picture. This is important during a solar eclipse, as filtering the light will allow you to see the round shape of the sun become a crescent or a ring as the moon moves in and gradually blocks the sunlight. 

When the eclipse is over, use a skewer to widen your camera’s pinhole. When you look inside, you won’t only be able to see the sun, but a slightly brighter and inverted image of your surroundings. A bigger pinhole turns your box into a camera obscura, allowing more light in and projecting an image of the objects around you.  

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About 364 miles above Earth, the crew of the Inspiration 4 private mission in 2021 drew each other’s blood and administered ultrasound scans. Yet it’s not clear whether those experiments were subject to the same ethical rules that govern human studies on the ground. And it’s unlikely to be the last time humans in orbit are asked to study each other in this way. Jared Isaacman, the billionaire backer of Inspiration 4 plans to conduct more experiments on his Polaris Dawn mission scheduled for sometime in 2024. 

It’s different when the research happens on Earth. If a US citizen chooses to participate in a clinical trial or other biomedical experiment, even those run privately, ethics rules govern the scientists, doctors, and institutions in charge of the study. A physician or a university cannot penalize a person for refusing to participate, for instance, and an ethics board must approve any trials before they start. 

Those ethical rules are part of the territory when receiving federal funding. “If the federal government gives you $1 anywhere in your organization, even having nothing to do with the research, then any human subjects research you do has to follow what’s called the ‘Common Rule,’” says Paul Wolpe, a bioethicist at Emory University and the former chief of bioethics at NASA. 

The 1991 Common Rule, or more formally the Federal Policy for the Protection of Human Subjects, is codified in multiple federal agencies, including the Health and Human Services Department. Its reach even extends beyond the bounds of Earth to NASA’s research, managing how the agency must treat astronauts on the International Space Station. 

But civilians have begun flying to orbit in the spacecraft of private companies. And those that don’t take federal money are not formally subject to the Common Rule. So what if SpaceX or Axiom Space, say, makes it a condition that anyone flying on private space missions must take a pharmaceutical drug at the behest of a partner company to gauge how it is metabolized in microgravity? 

[Related: Private space missions will bring more countries to the ISS]

That was the topic of a new paper published in Science by Wolpe and his colleagues. They argue that the time to begin asking questions about the ethics of human experimentation on private spacecraft is right now, before it becomes ubiquitous.

”Commercial spaceflight is revving up right now. The temptation to do human subjects experimentation is already starting,” Wolpe says, urging for a quick consensus. “It’s not like we’re saying, ‘10, 15 years from now, we may do this. We’re saying, ‘Next week we may do this.’” 

The paper’s authors argue it’s possible to extend the ethical frameworks already used to govern human scientific research on the ground—and in space for NASA astronauts—by following four principles: social responsibility, scientific excellence, proportionality, and global stewardship. 

Social responsibility recognizes that the past public investments that make spaceflight possible mean that this research should be treated “like a community resource.” It also points out that experimentation in the early years of commercial spaceflight “will be critical for ensuring the safety of future missions,” the authors write.  

Scientific excellence means thinking about how poorly designed or conducted experiments return low quality results, and “bad science is also bad for business,” the authors write. 

Proportionality refers to the importance of ensuring human research in space, like that on Earth, maximizes benefits while reducing the potential for harm as much as possible. And, guided by global stewardship, the fruits of these studies should benefit everyone, the authors argue: “Spaceflight research should therefore engage, and be conducted by, individuals and communities representative of humankind’s diversity.”

Wolpe hopes the principles can serve as a starting point for commercial space companies to think about and implement ethical guidelines, just as private companies do for human research on Earth. This paper doesn’t propose any concrete rules just yet. But coming up with a standard set of them for human experimentation in commercial spaceflight would be in corporations’ interest, too, Wolpe notes. “If everybody agrees on the rules, and we all operate under these rules, then we know what the floor and the ceiling is,” he says. Ideally, these would protect participants—and safeguard companies from lawsuits, if someone is harmed on a mission.

[Related: Space tourism is on the rise. Can NASA keep up with it?]

But before a new ethical framework takes root in the commercial spaceflight industry, more conversations need to happen to characterize research and its participants, according to Sara Langston, a space lawyer and professor of spaceflight operations at the Daytona Beach Florida campus of the Embry-Riddle Aeronautical University. As to whether there is a gap in existing rules and regulations around human experiments in commercial spaceflight that needs to be filled, she adds, “we need to actually define the question more specifically in order to answer it.”

You can, for instance, make a distinction between passive and active research or experimentation, according to Langston. Active experimentation are activities such as drawing blood or consuming drugs. Passive experimentation could include passengers sharing their subjective experiences of the flight, more akin to a survey. ”I don’t know that passive research in itself needs any kind of regulatory or even ethical framework, because passive research has been done all the time for marketing purposes, such as surveys,” Langston says. 

And it will also be important to distinguish private astronauts—flight participants who bought a ticket or were invited onto the mission—and commercial ones, who are the paid employees of a space company. “This is important because the roles, rights, duties, and liabilities are going to be distinct for each of those categories,” Langston says. 

Getting a head start in discussing these issues is the point, according to Wolpe. “These things are beginning to be built into the conversations around commercial spaceflight,” he says. “They weren’t so much before.”

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It took eight years and the collaborative efforts of over 600 interdisciplinary undergraduate students, but Estonia’s second satellite is finally on track to launch later this week. Once in orbit thanks to a lift aboard one of the European Space Agency’s Vega VV23 rockets, the tiny  8.5 lb ESTCube-2 will test an elegant method to potentially help clear the skies’ increasingly worrisome space junk issue using a novel “plasma brake.”

Designed by Finnish Meteorological Institute physicist Pekka Janhunen, the electric sail (E-sail) technology harnesses the physics underlying Earth’s ionosphere—the atmosphere’s electrically charged outer layer. Once in orbit, Estonia’s ESTCube-2 will deploy a nearly 165-foot-long tether composed of hair-thin aluminum wires that, once charged via solar power, will repel the almost motionless plasma within the ionosphere.

[Related: The FCC just dished out their first space junk fine.]

“​​Historically, tethers have been prone to snap in space due to micrometeorites or other hazards,” Janhunen explained in an October 3 statement ahead of the mission launch. “So ESTCube-2’s net-like microtether design brings added redundancy with two parallel and two zig-zagging bonded wires.”

If successful, the drag should slow down the tiny cubesat enough to shorten its orbital decay time to just a two-year lifespan. Not only that, but it would do so without any physical propellant source, thus offering a lightweight, low-cost alternative to existing satellite decommissioning options.

“It is exciting to see if the plasma break is going to work as planned… and if the tether itself is as robust as it needs to be,” Carolin Frueh, an associate professor of aeronautics and astronautics at Purdue University, tells PopSci via email. “The longer a dead or decommissioned satellite is out there, the higher the risk that it runs into other objects, which leads to fragmentation and the creation of even more debris objects.”

According to Frueh, although drag sails have been explored to help with Low Earth Orbit (LEO) satellites’ end-of-life maneuvers in the past, “the plasma brake technology has the potential to be more robust and more easily deployable at the end of life compared to a classical large solar sail.”

After just seven decades’ worth of space travel, junk is already a huge issue for ongoing private- and government-funded missions. Literally millions of tiny trash pieces now orbit the Earth as fast as 17,500 mph, each one a potential mission-ender. Such debris could also prove fatal to unfortunate astronauts in their path. 

Although multiple international efforts are underway to help mitigate the amount of space junk, even the process of planning such operations can be difficult. Earlier this year, for example, an ESA space debris cleanup pilot project grew more complicated after its orbital trash target reportedly unexpectedly collided with other debris. On October 2, the Federal Communications Commission issued its first-ever orbital littering fine after satellite television provider Dish Network failed to properly deorbit a decommissioned, direct broadcast EchoStar-7 satellite last year.

“As satellite operations become more prevalent and the space economy accelerates, we must be certain that operators comply with their commitments,” Enforcement Bureau Chief Loyaan A. Egal said at the time.

Estonia’s second-ever satellite is scheduled to launch on October 7 from the ESA’s spaceport in French Guiana.

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This month, millions of Americans will have a chance to watch an annular eclipse, also known as a “ring of fire” for the scorching halo the sun forms around the moon. If you’re one of them, be careful: looking directly at a solar eclipse without eye protection can permanently damage your vision.

It doesn’t matter if our rocky satellite is blocking all or some of our nearest star—the sun is still an incredibly bright source of light. Don’t risk your eyesight for a quick glimpse or even a once-in-a-lifetime event. Thankfully, it’s pretty easy to protect your eyes while watching an eclipse..

What happens if you look at a solar eclipse

We are able to see thanks to photoreceptors. These cells, also known as rods and cones, are located at the backs of our eyes, and convert the light reflected by the world around us into electrical impulses that our brain interprets as the image we see. But when strong light, like that from the sun, hits our eyes, a series of chemical reactions occur that damage and often destroy these rods and cones. This is known as solar retinopathy, and can make our eyesight blurry. Sometimes, if the damage is too great in one area, you can lose sight completely.

[Related: Every sunset ends with a green flash. Why is it so hard to see?]

On a typical sunny day, you almost never have to worry about solar retinopathy. That’s because our eyes have natural mechanisms that ensure too much light doesn’t get in. When it’s really bright outside, our pupils get super tiny, reducing the amount of sunlight that can hit your photoreceptors. But when you stare directly at the sun, your pupils’ shrinking power isn’t enough to protect your peepers.

This is where your eyes’ second defense mechanism comes into play. When we look at something bright, we tend to blink. This is known as the corneal or blink reflex, and it  prevents us from staring at anything too damagingly bright. 

Just before a solar eclipse has reached its totality, the moon is partially blocking the sun, making it a lot easier for us to look up at the star without blinking. But that doesn’t mean you should—even that tiny sliver of sunlight is too intense for our sensitive photoreceptors.

[Related: Total eclipses aren’t that rare—and you’ve probably missed a bunch of them]

Unfortunately, if you practice unprotected sun-gazing, you probably won’t know the effects of your actions until the next morning, when the damage to your photoreceptors has kicked in.

And while solar retinopathy is extremely rare, it is by no means unheard of. If you search the term in medical journals, you’ll find case reports after almost every popular solar eclipse. Let’s try really hard to do better this time, eyeball-havers.

How to safely watch a solar eclipse

Watching the eclipse with your own two eyes is easy: just wear legitimate eclipse sunglasses. These are crucial, as they will block the sun’s rays enough for you to safely see the eclipse without burning your eyes out.

And if you don’t have eclipse glasses, you can still enjoy the view, albeit not directly. Try whipping up your own eclipse projector or a DIY pinhole camera so you can enjoy the view without having to book an emergency visit to the eye doctor.

This story has been updated. It was originally published in 2017.

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The 2023 Nobel prize in chemistry was jointly awarded to Moungi Bawendi, Louis Brus, and Alexei Ekimov for the discovery and developments of quantum dots. These nanoparticles are so small that their size determines their properties. Quantum dots can be found in modern computers, televisions, and LED lights, among numerous other applications.

[Related: In photos: Journey to the center of a quantum computer.]

Bawendi is a professor at the Massachusetts Institute of Technology, Brus is a professor emeritus at Columbia University, and Ekimov works for a company called Nanocrystals Technology in New York State.

“For a long time, nobody thought you could ever actually make such small particles,” Johan Åqvist, chair of the Nobel Committee for Chemistry, said during a news conference. “But this year’s laureates succeeded.”

Size matters in the nanoscale

Quantum dots are among the smallest components of nanotechnology. Typically, an element’s properties are governed by how many electrons it has. When that matter shrinks down  to nano-dimensions quantum phenomena arise. This means the element’s properties are now governed by the size of the matter instead of the number of electrons it has. 

Quantum dots are made of only a thousand atoms. By comparison, one quantum dot is to a soccer ball as a soccer ball is to the planet Earth.

The quantum dots that Bawendi, Brus, and Ekimov produced are particles small enough for their properties to be determined by quantum phenomena. They are among the smallest, but most important particles, nanotechnology.

“Quantum dots have many fascinating and unusual properties. Importantly, they have different [colors] depending on their size,” Åqvist said in a statement. 

The movement of electrons in quantum dots is highly constrained. This then affects how they absorb and release visible light, allowing for very bright colors. The quantum dots themselves are nanoparticles that glow red, blue, or green and the color depends on the size of the particles. Larger dots shine red and smaller dots shine blue. The change in color depends on how electrons act differently in more confined or less confined spaces. 

Big discoveries, super small particles

In 1937, physicists theorized that size-dependent quantum effects could arise in nanoparticles. However, it was almost impossible to sculpt in nano dimensions, so few believed that it was possible.

During the early 1980s, Ekimov created size-dependent quantum effects in colored glass. The color of the glass came from the nanoparticles of copper chloride. With this colorful experiment, Ekimov demonstrated that the particle size affected the color of the glass via quantum effects.

[Related: Quantum computers are starting to become more useful.]

A few years later, Brus became the first scientist in the world to prove that size-dependent quantum effects in particles were floating freely in a fluid. Brus and Ekimov were actually working independently from one another when they made their initial discoveries. 

In 1993, Bawendi revolutionized the chemical production of quantum dots. His techniques resulted in almost perfect particles, which was necessary for using the quantum dots in a wide range of applications. 

Quantum dots can now be found in computer monitors and television screens and even help biochemists and surgeons map tissues and remove tumors. 

Last year’s chemistry prize was also awarded to a trio of chemists: Carolyn R. Bertozzi for her work in bioorthogonal chemistry alongside K. Barry Sharpless and Morten Meldal for laying the foundation for click chemistry. 

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The Federal Communications Commission is officially doling out fines for space polluters, and the popular satellite television provider Dish Network earned the dubious honor of receiving the first ticket. On October 2, the FCC announced it slapped the telecommunications company with a $150,000 penalty after failing to properly deorbit its decommissioned, direct broadcast EchoStar-7 satellite last year. According to the FCC, the fine comes with an admission of liability, as well as an agreement to follow a “compliance plan” to help make way for the thousands of orbital projects in the works around the world.

[Related: FCC slaps voter suppression robocall scammers with a record-breaking fine.]

Space junk is already a huge concern for any industry requiring operations high above the planet, with literal millions of trash bits orbiting Earth at any given moment. In July, NASA director Bill Nelson told the BBC space junk poses a “major problem,” explaining that even something like a small paint chip striking an astronaut during a spacewalk at orbital speed (17,500 mph) “can be fatal.” Experts also worry about humans accidentally initiating a “Kessler cascade” or “Kessler syndrome.” In such situations, orbital space becomes so polluted that debris collisions are impossible to avoid, thus producing an exponentially increasing cycle of more collisions that create more debris. Were this to occur, the future of space exploration and travel could remain stymied until governments and companies begin complicated, costly cleanup efforts. 

Dish Network’s EchoStar-7 satellite launched and achieved geostationary orbit in 2002, and received FCC approval for an eventual orbital mitigation plan in 2012. According to the agreement, the telecoms company committed to eventually boost the satellite roughly 300 km above its operational arc. In February 2022, however, Dish Network revealed the satellite did not have enough remaining propellant to adhere to the original agreement’s altitude. In the end, the EchoStar-7 satellite only retired about 122 km above its geostationary arc—far lower than planned. Last year, the FCC also announced plans to finally begin tighter restrictions on satellites’ lifespans and decommissioning protocols.

[Related: Some space junk just got smacked by more space junk, complicating cleanup.]

“As satellite operations become more prevalent and the space economy accelerates, we must be certain that operators comply with their commitments,” Enforcement Bureau Chief Loyaan A. Egal said via Monday’s announcement. “This is a breakthrough settlement, making very clear the FCC has strong enforcement authority and capability to enforce its vitally important space debris rules.”

In August, a space debris cleanup pilot project overseen by the European Space Agency quickly turned into a logistical headache after its orbital trash target appeared to collide with another piece of debris. Luckily, the ESA and its partners at Swiss startup ClearSpace-1 stated at the time that their project appears able to progress as planned.

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The universe is expanding—but astronomers can’t agree how fast. And NASA’s superstar observatory, the James Webb Space Telescope, just confirmed there’s a problem in our understanding of the stretching cosmos. JWST’s new measurements are the most precise of their kind, but they don’t clear up a baffling mismatch in the two methods scientists track this growth. 

In 1929, astronomer Edwin Hubble discovered that all the galaxies we can see are moving away from us. The relationship between the distance to a galaxy and how fast it’s moving is now known as Hubble’s law. This law uses the also-eponymous Hubble constant to describe the rate at which the universe is expanding. It also tells us the age of the universe: Astronomers can use the Hubble constant to “rewind” time to when the universe would be a single point in space—the big bang.

There are two main ways to measure this fundamental number. One is by tracing tiny fluctuations in the cosmic microwave background from the beginning of the universe. The other is to watch flickering stars known as Cepheids. But those two methods disagree. This baffling mismatch is known as the Hubble tension, and it’s unclear if it’s a problem with our models of the universe or our measurements.

If it’s our measurements, the error might result from the way we survey Cepheid stars. Astronomers consider these objects to be a type of “standard candle,” a thing in space whose intrinsic brightness is known. We can observe how bright one of these stars looks in the sky. If it’s faint, it’s farther away. Brighter is closer. 

Researchers use the luminosity of these stars like a yardstick to measure distance. Then, with methods such as spectroscopy, they can gauge the motion of far-off galaxies. Putting those observations together tells us how fast the universe is expanding.

[Related: NASA releases Hubble images of cotton candy-colored clouds in Orion Nebula]

“When we use Cepheids like this, we need to be very, very sure we’re measuring their brightnesses correctly, otherwise our distance measurements will be off. However, Cepheids can be in crowded parts of their galaxies and if our telescopes aren’t sensitive enough, we can’t clearly distinguish a Cepheid from the stars around it,” explains astronomer Tarini Konchady, a program officer at the National Academies of Sciences, Engineering, and Medicine. 

Before JWST, the Hubble Space Telescope (HST) took the best measurements of Cepheid stars. HST couldn’t distinguish individual Cepheids where they were bunched in crowded regions, but JWST can—and it just did. JWST peered into two distant galaxies, and made measurements of the Hubble constant 2.5 times better than HST could. 

“Webb’s measurements have dramatically cut the noise in the Cepheid measurements,” said project lead Adam Riess, an astronomer at Johns Hopkins University in a NASA press release. “This kind of improvement is the stuff astronomers dream of!”

One of JWST’s major advantages is its ability to look at the cosmos in infrared light, which helps cut through dust between our telescopes and the Cepheids. “Sharp infrared vision is one of the James Webb Space Telescope’s superpowers,” Riess said.

[Related: How old is the universe? Our answer keeps getting more precise.]

However, the new measurements matched up with those from HST, just with smaller error bars—so we can’t confidently pin the mystery on those old numbers.

The new results from Riess and team are just the beginning, though, and they still have many more galaxies to observe with JWST. “I think the jury is still out on whether the JWST has completely eliminated crowding as a solution to the Hubble tension,” says University of Chicago astronomer Abigail Lee. “Analyzing the data for the rest of the 42 galaxies [that JWST plans to observe] will illuminate whether the Hubble tension is alive and real or if there are indeed just errors in the Cepheid measurements.”

The fate of the universe, or at least the Hubble tension, doesn’t just hinge on JWST. Many other facilities will come online in the next few years, providing more evidence for this investigation. The Vera Rubin Observatory, for example, is going to scan the whole Southern sky every few nights when it opens next year, and will likely discover many more Cepheid stars.

“We’re at a point where astronomers are going to be deluged by the most sensitive and wide-reaching data yet,” says Konchady. There might not be a clear answer yet, but astronomers are surely on the case to figure out this mystery.

This post has been updated to include additional details about astronomical methods for measuring the expansion rate.

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In space, the brightness of a galaxy is typically determined by its mass. However, some new research suggests that less massive galaxies can actually glow just as brightly as larger ones. Due to irregular and brilliant bursts of star formation, some  younger galaxies appear deceptively large. The new findings are detailed in a study published October 3 in the Astrophysical Journal Letters.

[Related: Our universe mastered the art of making galaxies while it was still young.]

The first stellar images released by the James Webb Space Telescope (JWST) in 2022 came with a bit of a quandary. To some astronomers, the young galaxies appeared to be too bright, too massive, and too mature to have formed so soon after the big bang, almost as if an infant grew into an adult after only a few years. 

“The discovery of these galaxies was a big surprise because they were substantially brighter than anticipated,” study co- author and Northwestern University astrophysicist Claude-André Faucher-Giguère said in a statement. “Typically, a galaxy is bright because it’s big. But because these galaxies formed at cosmic dawn, not enough time has passed since the big bang. How could these massive galaxies assemble so quickly? Our simulations show that galaxies have no problem forming this brightness by cosmic dawn.”

The period in cosmological history called Cosmic Dawn lasted from about 100 million years to 1 billion years after the big bang and is marked by the formation of the first stars and galaxies in the universe. 

“The JWST brought us a lot of knowledge about cosmic dawn,” study co-author and Northwestern University astrophysicist Guochao Sun said in a statement. “Prior to JWST, most of our knowledge about the early universe was speculation based on data from very few sources. With the huge increase in observing power, we can see physical details about the galaxies and use that solid observational evidence to study the physics to understand what’s happening.”

The team used advanced computer simulations to model how galaxies formed just after the big bang. Part of Northwestern’s Feedback of Relativistic Environments (FIRE) project, the simulations combine astrophysical theory and advanced algorithms to model how galaxies form. These models help researchers see how galaxies grow and change shape all while considering mass, energy, momentum, and chemical elements returned from stars. 

“The key is to reproduce a sufficient amount of light in a system within a short amount of time,” Sun said. “That can happen either because the system is really massive or because it has the ability to produce a lot of light quickly. In the latter case, a system doesn’t need to be that massive. If star formation happens in bursts, it will emit flashes of light. That is why we see several very bright galaxies.”

[Related: Your guide to the types of stars, from their dusty births to violent deaths.]

The simulations in the study created galaxies that were just as bright as the ones observed by JWST. They also found that the early galaxies formed at cosmic dawn likely had stars that formed in bursts. This is a concept called bursty star formation, where stars form in an alternating pattern. It begins with the formation of a bunch of stars at once, then millions of years with little to no stars, and then another burst of stars. By comparison, our Milky Way galaxy followed a very different pattern of star formation at a steady rate.

According to Faucher-Giguère, bursty star formation is particularly common in low-mass galaxies. However, the details of why this happens are still the subject of other research. The team on this study believes that it happens when the initial bursts of stars explode as supernovae a few million years later. The gas is kicked out and then falls back inwards to form new stars and drives the cycle again. 

When the galaxies get massive enough, they have significantly stronger gravity. So when the  supernovae explode, they aren’t strong enough to eject gas from the star system and the gravity binds the galaxy together. The result is a more steady state.

“Most of the light in a galaxy comes from the most massive stars,” Faucher-Giguère said in a statement. “Because more massive stars burn at a higher speed, they are shorter lived. They rapidly use up their fuel in nuclear reactions. So, the brightness of a galaxy is more directly related to how many stars it has formed in the last few million years than the mass of the galaxy as a whole.”

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NASA’s Psyche mission to a unique, metallic asteroid of the same name launched from Kennedy Space Center’s Launch Complex 39A at 10:20 a.m. Eastern on October 13 via a SpaceX Falcon Heavy rocket.

It was, finally, a smooth exit from Earth for the probe. Psyche had been scheduled to blast off on October 5, the first day of a window that stretches through October 25. But NASA officials announced a delay on September 28, citing issues with the spacecraft’s maneuvering thrusters, which are used to point the vehicle where it needs to go. “The change allows the NASA team to complete verifications of the parameters used to control the Psyche spacecraft’s nitrogen cold gas thrusters,” NASA officials wrote in the announcement. 

That weeklong delay was small, though, compared to the mission’s earlier hold-ups. Psyche was first set to launch in October of 2022, but issues with the navigation software developed by NASA’s Jet Propulsion Laboratory forced the agency to delay the mission by a year. 

This mission should be well worth the wait. It could help uncover details about unusual asteroids and our planet. And the pioneering technology and operations it will demonstrate during its nearly six-year mission will influence the design of future spacecraft. 

Psyche to Psyche

The destination of Psyche (a spacecraft) is 16 Psyche (an asteroid)—an object about 140 miles in diameter in the asteroid belt between Mars and Jupiter. It looks a bit like a cratered potato. 

Remote observations by astronomers have already determined 16 Psyche to be a highly metallic asteroid, rich in iron, and it is believed to be the exposed core of a small planet that never fully formed. Getting up close and personal with 16 Psyche could help scientists better understand Earth’s iron-rich core: It’s easier to send a spacecraft 280 million miles away to study an asteroid than to access Earth’s rocky center, 1,800 miles beneath our feet. Exploring the metallic object in space has implications for our planet’s geomagnetic field, which protects life from space radiation—that field is generated when our planet’s solid inner core spins within liquid metal surroundings. 

Thrusters and lasers

Psyche is one of NASA’s first spacecraft to use solar electric propulsion as its primary means of reaching an asteroid. Rather than relying on traditional chemical rockets, Psyche will use Hall effect thrusters, which use electrostatic fields to accelerate ions—charged particles—and expel them, generating thrust. (These are different machines from the nitrogen thrusters that caused the launch delay.) Such thrusters produce very low thrust—far less than a pound—but do so very efficiently, allowing Psyche to preserve its xenon gas propellant and build up speed over the vast distances it will cover. 

The electric thrusters will use solar power—though the sunlight it absorbs will shrink as Psyche approaches its destination. Still, it’s well prepared. While the spacecraft itself is the size of a large car, its twin solar panels are about the size of tennis courts. They’ll produce 21 kilowatts of energy near Earth and about two kilowatts when at asteroid Psyche. 

[Related on PopSci+: In its visit to Psyche, NASA hopes to glimpse the center of the Earth]

In addition to solar electric propulsion, Psyche will also test a new form of Earth-to-spacecraft transmission system called Deep Space Optical Communication. Deep Space Optical Communication encodes data in infrared lasers, rather than radio waves, and can potentially carry much more information to and from the Psyche spacecraft than can traditional methods. The laser communications are just a demonstration—Psyche will still stay in touch with Earth, and vice versa, using NASA’s radio-based Deep Space Network. 

Research on a metal world

When Psyche arrives at the asteroid 16 Psyche in 2029, it will set to work studying the iron asteroid’s magnetic properties. With the aid of an imager and two kinds of spectrometer, the probe will also use patterns of light absorption to determine what elements and compounds exist on this metal potato. 

But Psyche won’t simply scratch the surface. It will also study the asteroid’s internal structure by measuring the space rock’s gravity field. There’s no specific instrument to pull this off. Instead, scientists on the ground will use radio signals from Psyche to precisely measure the spacecraft’s orbit around the asteroid, measuring any slight perturbations that signal variations in the gravitational field, which in turn can tell scientists about the internal density of 16 Psyche. 

[Related: Smashed asteroid surrounded by a ‘cloud’ of boulders]

And while the Psyche mission has the unique potential to shed light on how planetary bodies are formed and function, it’s also a part of an expanding portfolio of NASA asteroid missions. NASA’s Lucy mission, which launched in 201, is currently on its way to fly by multiple asteroids near Jupiter between 2025 and 2033. NASA’s OSIRIS-REx asteroid sample return mission, meanwhile, just dropped pieces of the asteroid Bennu back on Earth on September 24. It’snow headed to visit the asteroid Apophis; the mission has been renamed to OSIRIS-APEX, or Origins, Spectral Interpretation, Resource Identification, and Security-APophis EXplorer.

Such missions have multiple goals: they help scientists better understand the formation of the early solar system and how planets like Earth, and they can also tell us about the makeup of asteroids that could one day pose a threat—and how to deflect them if necessary. 

Apophis, for instance, was at one time considered a very hazardous asteroid; though it won’t hit Earth, it will pass within 20,000 miles of our planet on April 13, 2029. 

The people of Earth don’t have to worry about any danger from 16 Psyche, though, as it will continue along in its orbit between Mars and Jupiter indefinitely, hundreds of millions of miles from our planet. 

That is, unless humans make changes to the metallic space rock. Mining asteroids is an old idea. But, as spacecraft improve, the estimated $10 quintillion worth of metal ore on Psyche and asteroids like it might begin to look pretty appetizing to companies that want to capitalize on resources in the heavens.

This post has been updated. It was originally published on October 2.

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Chances are you have heard about this one already. The moon will pass between Earth and the sun and cast a huge shadow on our planet in the process. With the right protective eyewear, it will be a sight to behold—the phenomenon produces a “ring of fire” as if the moon is outlined with flames.  

Astronomers have calculated precisely when the best views will be where you are, so consult this list when scheduling an outing to safely check out the sky. The duration will range from little more than one minute to almost five, depending where you are located in its path. This eclipse has a 125-mile-wide path of annularity that will begin in Oregon at 12:13 p.m. Eastern Daylight Time. It will leave the US at about 1:03 p.m. EDT and head southeastward toward Central and South America. 

October 21 and 22 – Orionids Meteor Shower Predicted Peak

The annual Orionid meteor shower is expected to peak on October 22 in a moonless sky, but the wee hours of the morning of October 21 could also yield some meteors. According to EarthSky, under a dark sky with no moon, the Orionids can produce a maximum of about 10 to 20 meteors per hour. On October 22, the moon will be setting around midnight, which means its light shouldn’t interfere with the shower. The best time to try and spot the shower is just after midnight into the early morning hours 

October 23 – Venus at Greatest Elongation

In August, the planet Venus moved between the Earth and the sun and rose in the east. Venus will be farthest from the sunrise on October 23 and should remain visible in the morning sky until May 2024, where it will be a very bright “morning star.” 

During this month’s greatest elongation, Venus will appear higher in the sky from the Northern Hemisphere than from the Southern Hemisphere. This is because of the steep angle of the path of the sun, moon, and planets in the mornings during the autumn months. 

October 28- Full Hunter’s Moon and Partial Lunar Eclipse

The same skygazing rules that apply to pretty much all space-watching activities are key this month: Go to a dark spot away from the lights of a city or town and let the eyes adjust to the darkness for about a half an hour.

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This article was originally published on Undark.

IN JANUARY 2023, Tara Sweeney’s plane landed on Thwaites Glacier, a 74,000-square-mile mass of frozen water in West Antarctica. She arrived with an international research team to study the glacier’s geology and ice fabric, and how its ice melt might contribute to sea level rise. But while near Earth’s southernmost point, Sweeney kept thinking about the moon.

“It felt every bit of what I think it will feel like being a space explorer,” said Sweeney, a former Air Force officer who’s now working on a doctorate in lunar geology at the University of Texas at El Paso. “You have all of these resources, and you get to be the one to go out and do the exploring and do the science. And that was really spectacular.”

That similarity is why space scientists study the physiology and psychology of people living in Antarctic and other remote outposts: For around 25 years, people have played out what existence might be like on, or en route to, another world. Polar explorers are, in a way, analogous to astronauts who land on alien planets. And while Sweeney wasn’t technically on an “analog astronaut” mission — her primary objective being the geological exploration of Earth — her days played out much the same as a space explorer’s might.

For 16 days, Sweeney and her colleagues lived in tents on the ice, spending half their time trapped inside as storms blew snow against their tents. When the weather permitted, Sweeney snowmobiled to and from seismometer sites, once getting caught in a whiteout that, she said, felt like zooming inside a ping-pong ball.

On the glacier, Sweeney was always cold, sometimes bored, often frustrated. But she was also alive, elated. And she felt a form of focus that eluded her on her home continent. “I had three objectives: to be a good crewmate, to do good science, and to stay alive,” she said. “That’s all I had to do.”

None of that was easy, of course. But it may have been easier than landing back on the earth of El Paso. “My mission ended, and it’s over,” she said. “And how do I process through all these things that I’m feeling?”

Then, in May, she attended the 2023 Analog Astronaut Conference, a gathering of people who simulate long-term space travel from the relative safety and comfort of Earth. Sweeney had learned about the event when she visited an analog facility in the country of Jordan. There, she’d met one of the conference’s founders, Jas Purewal, who invited her to the gathering.

The meeting was held, appropriately, at Biosphere 2, a glass-paneled, self-contained habitat in the Arizona desert that resembles a 1980s sci-fi vision of a space settlement — one of the first facilities built, in part, to understand whether humans could create a habitable environment on a hostile planet.

A speaker at the conference had spent eight months locked inside a simulated space habitat in Moscow, Russia, and she talked about how the post-mission period had been hard for her. The psychological toll of reintegration became a chattering theme throughout the whole meeting. Sweeney, it turned out, wasn’t alone.

Across the world, around 20 analog space facilities host people who volunteer to be study subjects, isolating themselves for weeks or months in polar stations, desert outposts, or even sealed habitats inside NASA centers. These places are intended to mimic how people might fare on Mars or the moon, or on long-term orbital stations. Such research, scientists say, can help test out medical and software tools, enhance indoor agriculture, and address the difficulties analog astronauts face, including, like Sweeney’s, those that come when their “missions” are over.

Lately, a community of researchers has started to make the field more formalized: laying out standards so that results are comparable; gathering research papers into a single database so investigators can build on previous work; and bringing scientists, participants, and facility directors together to share results and insights.

With that cohesion, a formerly quiet area of research is enhancing its reputation and looking to gain more credibility with space agencies. “I think the analogs are underestimated,” said Jenni Hesterman, a retired Air Force officer who is helping spearhead this formalization. “A lot of people think it’s just space camp.”

ANALOG ASTRONAUT FACILITIES emerged as a way to test drive space missions without the price tag of actually going to space. Scientists, for example, want to make sure tools work properly and so analog astronauts will test out equipment ranging from spacesuits to extreme-environment medical equipment.

Researchers are also interested in how astronauts fare in isolation, and so they will sometimes track characteristics like microbiome changes, stress levels, and immune responses by taking samples of spit, skin, blood, urine, and fecal matter. Analog missions “can give us insights about how a person would react or what kind of team — what kind of mix of people — can react to some challenges,” said Francesco Pagnini, a psychology professor at the Catholic University of Sacred Heart in Italy, who has researched human behavior and performance in collaboration with the European and Italian space agencies.

Some facilities are run by space agencies, like NASA’s Human Exploration Research Analog, or HERA, which is located inside NASA’s Johnson Space Center in Houston. The center also houses a 3D-printed habitat called Crew Health and Performance Exploration Analog, or CHAPEA, where crews will simulate a year-long mission to Mars. The structure looks like an artificial intelligence created a cosmic living space using IKEA as its source material.

“My mission ended, and it’s over,” Sweeney said. “And how do I process through all these things that I’m feeling?”

Most analog spots, though, are run by private organizations and take research proposals from space agencies, university researchers, and sometimes laypeople with projects that the facilities select through an application process.

Such work has been going on for decades: NASA’s first official analog mission took place in 1997, in Death Valley, when four people spent a week pretending to be Martian geologists. In 2000, the nonprofit Mars Society, a space-exploration advocacy and research organization, built the Flashline Mars Arctic Research Station in Nunavut, Canada, and soon after constructed the Mars Desert Research Station in Utah. (Both facilities have been used by NASA researchers, too.) But the practice was in place long before those projects, even if the terminology and permanent facilities were not: In the Apollo era, astronauts used to try out their rovers and space walks, along with scientific techniques, in Arizona and Hawaii.

Many facilities, according to Ronita Cromwell, formerly the lead scientist of NASA’s Flight Analogs Project, are located in two types of places: extreme environments or controlled ones. The former include Antarctic or Arctic research stations, which tend to be used to study topics like sleep patterns and team dynamics. The latter — sealed, simulated habitats — are primarily useful for human behavior research, like learning how cognitive ability changes over the course of a mission, or testing out equipment, like software that helps astronauts make decisions without communicating to mission control. That independence becomes necessary as crews travel farther from Earth, because the communication delays increase with distance.

During her work on NASA’s mission simulations, Cromwell saw their value. “What excited me is that we were able to create sort of spaceflight situations on the ground, to study spaceflight changes in the human body,” Cromwell said, “whether they be, you know, psychological, cognitive changes, or physiological changes.”

Psychiatry researchers from the University of Pennsylvania, for instance, recently found that members of a crew at HERA performed better on cognition tasks — like clicking on squares that randomly appear on a screen and memorizing three-dimensional objects — as their mission went on. Another recent HERA study, led by scientists at Northwestern and DePaul universities, found that over time, teams got better at executing physical tasks together, but worsened when they tried to work together creatively and intellectually, like brainstorming as many uses as possible for a given object. Those brain and behavioral changes could teach scientists about tight teams deployed in other remote, tedious, stressful situations. “I think space psychology can also speak a lot about everyday life,” said Pagnini.

On the physical side, an international team that included a NASA scientist recently used the Mars Desert Research Station to test whether analog astronauts could be quickly taught how to fix broken bones using a device that could work on Mars — or an earthly site far from medical facilities. Investigations into self-contained, sustainable living reveal how low-resource existence could work on Earth, too. For example, another crew, led by Griffith University medical researchers, performed an experiment extracting water from minerals in case of emergency.

“I think the analogs are underestimated,” said Hesterman. “A lot of people think it’s just space camp.”

While scientific research that actually takes place in space usually gets the spotlight, the ground-testing of all systems, including human ones, is necessary, if not always glamorous or publicly lauded. “I felt like I was in charge of a deep, dark secret,” said Cromwell, jokingly, of her work on the NASA analog program.

In fact, even people who work in adjacent fields sometimes haven’t heard of the field. Purewal, an astrophysicist, only learned about analog space research in 2020. With Covid-19 restrictions in place, though, most facilities had halted new missions. “If I can’t go to an analog, maybe I can bring the analog to me,” Purewal thought.

Amid the drapey willow branches and manicured hedges of her parents’ backyard in Warwick, England, she constructed a geodesic dome out of broomstick handles and tent-like materials. Purewal sequestered inside for a week, leaving only to use the bathroom — and then only while wearing a simulated spacesuit. She communicated with those outside her dome on a synthesized 20-minute delay and ate freeze-dried foods, which she came to hate, and insect protein from mealworms and locusts, which she came to like more than she anticipated.

While Purewal admits her personal analog was “low-fidelity,” it offered a test drive for more rigorous research. By 2021, Purewal had, with SpaceX civilian astronaut Sian Proctor, co-founded the Analog Astronaut Conference that Sweeney attended, along with an associated online community of more than 1,000 people. She also participated in an analog mission in someone else’s backyard — one surrounded by Utah State Trust Lands — in November 2022. Their endeavor was sponsored by the Mars Society and involved research on mental health, geologic research tools, and sustainable food supplies, all of which would be necessary if they were going to Mars.

BUT THEY WEREN’T HEADED to Mars, they were headed to Utah. About five minutes from the small town of Hanksville — home to “Hollow Mountain,” a gas station convenience store dug out of a rock formation — sits the turnoff to the Mars Desert Research Station. Operated by the Mars Society, the facility is 3.4 miles down a dirt track called N Cow Dung Road. The landscape looks otherworldly: mushroom-shaped rock formations; sandy, granular ground; and eroded hills of red rock.

The station sits in a flat spot surrounded by those hills, with a cylindrical living space two stories tall but just 26 feet in diameter. The habitat links out via above-ground “tunnels” to a greenhouse and a geodesic dome that resembles Purewal’s initial backyard creation, and houses a control center and lab.

In November 2022, Purewal brought a team there for two weeks, with Hesterman as commander. In the habitat, an astrobiology student tried to grow edible mushrooms in the crew’s food waste. Another team member wanted to see if they could make yogurt from powdered milk and bacteria. Purewal, meanwhile, was experimenting with an AI companion robot called PARO. Shaped like a baby harp seal, PARO is typically used to relieve stress in medical situations. The crew members interacted with PARO and wore bio-monitoring straps that measured things like heart rate as they did so.

Every day on “Mars” had a set of missions: spacewalks, splinting a broken ankle on a virtual reality headset, a tabletop emergency exercise about evacuating for noxious fumes, a fake pass-out to test emergency response protocol. Their personal protocols were working well, but Purewal and Hesterman, locked in together, had begun to fret about the quality and consistency of the analog enterprise more broadly. They started to think about creating standards: for the research, for the facilities themselves. At their Utah-Mars station, for instance, a pipe broke under their sink. There were electrical issues. A propane monitor was malfunctioning.

After their mission ended, they spoke with others, and heard about issues such as expired fire extinguishers, or the lack of safety training for participants who would be using specialized technologies and life support systems. They consulted Emily Apollonio, a former aircraft accident investigator. In 2022, she traveled to Hawaii to live at HI-SEAS, a 1,200-square-foot analog station located 8,200 feet above sea level on the Mauna Loa volcano. Apollonio thought HI-SEAS had avoidable problems. For one, the bathroom had only a composting toilet, which the mission crew weren’t allowed to pee in, and a urinal, which the women had to use, too.

With a draft version released this June, they hope to improve conditions for participants — ensuring, for instance, that facilities adhere to building codes and provide adequate medical support. They also want to encourage analog participants to follow research best practices to ensure rigorous outputs. The standards suggest, for instance, that each mission have its research plan pre-validated by the principal investigator and habitat director, a timeline for research completion, and an Institutional Review Board approval in place for human experiments. While projects with federal or institutional grant funding go through these steps anyway, the formality isn’t uniform across the board.

While some analogs already have rigorous protocols in place to protect participants, the safety issues and inclusivity gaps she heard about from colleagues helped inspire Apollonio to start a training and consulting company called Interstellar Performance Labs to help prepare would-be analog astronauts before their missions. She also started to work with Purewal, Hesterman, and others on a document called “International Guidelines and Standards for Space Analogs.”

The standards also detail the creation of a research database, putting all the writeups (peer-reviewed and otherwise) of analog projects in one place. That way, people aren’t duplicating efforts — as the mushroom-grower, it turns out, was — unless they mean to test the replicability of results. They can also better link their studies to space agencies’ established needs to be more directly helpful and relevant to the real world.

“I didn’t know where to look, I didn’t know where to go,” Apollonio said. “I couldn’t hear my thoughts.”

As part of this centralization effort, Purewal, Apollonio, Hesterman, and colleagues are also putting together what they call the World’s Biggest Analog: a simultaneous, month-long mission involving at least 10 isolated bases across the world, which together will simulate a large, cooperative future presence in space.

So far, though, attempts to give the community cohesion and coherency have yet to fully address the aspect of analog life that gives many participants trouble: the end of their mission. “Being in an analog mission was less difficult than coming out an analog mission,” said Apollonio, of her own experience.

Shortly after emerging from HI-SEAS, she walked around the streets of Waikiki with her husband. The lights, the noise — everything was too much. “I didn’t know where to look, I didn’t know where to go,” she said. “I couldn’t hear my thoughts.” After they chose a restaurant for dinner, and the server handed her a menu, she froze. “I have to choose my own food,” she realized. It was overwhelming, and that feeling didn’t abate.

Meanwhile, few other people understood the experience, said Hesterman. “You come home and you’re all excited, like, you want to tell everybody about it,” she continued. “You tell everybody about it once, and then they’re just done. On back to paying the bills and cutting the grass and stuff. You still want to talk about it.”

Purewal missed the team and the sense of shared purpose, and started to seek it outside the simulation. “I need to find this same feeling in my day-to-day life,” she said. “We all kind of need our crew.”

RESEARCH ON THE post-mission experience is scant, said Pagnini. In March 2023, he co-authored a review paper, commissioned by the European Space Agency, which aimed to lay out the state of research on human behavior and performance in space, including gaps in the science. Studying how astronauts react and cope “post-mission,” his research found, has been particularly neglected. The same is true of returning from analog space.

Pagnini says the research isn’t just relevant to analog or actual astronauts. Life in space has similarities to life on Earth — including in its difficulties. Italy’s heavily restrictive and prolonged Covid-19 lockdown, for instance, resembled going away on a mission. “When we got out of the lockdown phase, getting in touch with other people was kind of strange,” he said. Much of living a regular life on Earth was strange.

The strangeness also extends to other experiences, like military deployments and the subsequent return to domestic life. “The expectation is kind of that families will live happily ever after” once they’re reunited, said Leanne Knobloch, a professor of communication at the University of Illinois, who performed a large reintegration study on military couples. “So that’s why reintegration has sometimes been overlooked, but more and more researchers are starting to recognize that it is a challenging period, and it’s not the storybook ending that people make it out to be.”

She noted that her research, like that on the psychology of space travel and the post-mission experience, can apply to other arenas. “Any kind of situation where partners are separated and they come together, this research can help understand that puzzle piece more broadly,” she said.

Knobloch’s work includes suggestions for easing the transition, such as preparing people for the issues they’re likely to experience. “If you’re ready and expect that you might experience some of these problems, it won’t be so stressful,” she said. “Because you’ll recognize that they’re normal.”

Apollonio’s Interstellar Performance Labs, for one, is already planning to include education on “aftercare,” educating people about what she calls the “deorbiting effect” of returning to regular life.

WHEN THE DAY finally came for Sweeney to depart Thwaites Glacier, the aircraft seemed to materialize right out of the sky, as though the remote outpost had transformed into a busy airport. As she was leaving, she looked down at the camp where half her team remained. “You could just see how small our little footprint was,” she said. A speck in the middle of endless white space.

Since she landed in North America, Sweeney has savored time with her family. But the adjustment hasn’t been easy. “Each day that ticks by of being back, I started feeling pulled in different directions,” she said. With numerous projects ongoing — mentoring, speaking, doing her doctoral research — she felt her sense of self splintering. In Antarctica, she had been a smooth, singular whole.

But at the Analog Astronaut Conference in May, hearing about others’ similar readjustment difficulties, Sweeney felt some sense of normalcy. Having a community of support could help with post-mission struggles. Further research — aided by the new database and standardization measures — could help uncover best coping strategies, along with the keys to successful crew dynamics, stress creators and mitigators, and tools and designs that make the practicalities of a mission easier. Maybe someone will look at the database, see this scientific gap, and try to fill it.

Such research might resonate with Sweeney and others having trouble readjusting to their daily lives. “We have to get back to work, we have to go see our families, we want to pick up the projects we were doing before,” she said. “But also, we need to make space for the magnitude of the experience that we just had. And to be able to decompress from that.”

UPDATE: A previous version of this piece incorrectly stated that Tara Sweeney’s plane landed on Thwaites Glacier in November 2022. She arrived to McMurdo Station in Antarctica in November 2022, but did not land on Thwaites Glacier until January 2023. The piece also described a scene in which Sweeney left her camp on Thwaites Glacier, and incorrectly stated that she was departing Antarctica at that time. She remained in Antarctica for several weeks after she left the glacier. Lastly, a previous version stated that storms dumped feet of snow on the landscape. To clarify that the snow was not fresh snowfall, the piece has been updated to reflect that snow blew against the tents.

This article was originally published on Undark. Read the original article.

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Solar sails that leverage the sun’s photonic rays for “wind” are no longer the stuff of science fiction—in fact, the Planetary Society’s LightSail 2 practical demonstration was deemed a Grand Award Winner for PopSci’s Best of What’s New in 2019. And while countless projects continue to explore what solar sails could hold for the future of space travel, a new study demonstrates just how promising the technology could be for excursions to Earth’s nearest planetary neighbor, and beyond.

According to a paper recently submitted to the journal Acta Astronautica, detailed computer simulations show tiny, incredibly lightweight solar sails made with aerographite could travel to Mars in just 26 days—compare that to conventional rocketry time estimates of between 7-to-9 months. Meanwhile, a journey to the heliopause (the demarcation line for interstellar space where the sun’s magnetic forces cease to influence objects) could take between 4.2 and 5.3 years. For comparison, the Voyager 1 and Voyager 2 space probes took a respective 35 and 41 years to reach the same boundary.

[Related: This novel solar sail could make it easier for NASA to stare into the sun.]

The key to such speedy trips is the 1 kg solar sails’ 720g of aerographite—an ultra-lightweight material with four times less density than most solar sail designs’ Mylar components. The major caveat to these simulations is that they involved an extremely miniscule payload weight, something that will most often not be the case for major interplanetary and interstellar journeys.

“Solar sail propulsion has the potential for rapid delivery of small payloads (sub-kilogram) throughout the solar system,” René Heller, an astrophysicist at the Max Planck Institute for Solar System Research and study co-author, explained to Universe Today earlier this month. “Compared to conventional chemical propulsion, which can bring hundreds of tons of payload to low-Earth orbit and deliver a large fraction of that to the Moon, Mars, and beyond, this sounds ridiculously small. But the key value of solar sail technology is speed.”

Another issue still that still needs addressing is deceleration methods needed upon actually reaching a destination. Although aerocapture—using a planet’s atmosphere to reduce velocity—is a possible option, researchers concede more investigation will be needed to determine the best, most efficient way to actually stop at a solar sail-equipped spacecraft’s intended endpoint. Regardless, the study only adds even more wind in the sails (so to speak) for the impressive interstellar travel method.

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The dark side of the moon, despite its name, is a perfect vantage point for observing the universe. On Earth, radio signals from the furthest depths of space are obscured by the atmosphere, alongside humanity’s own electronic chatter, but the lunar far side has none of these issues. Because of this, establishing an observation point there could allow for unimpeded views of some of cosmic history’s earliest moments—particularly a 400 million year stretch known as the universe’s Dark Ages when early plasma cooled enough to begin forming the  protons and electrons that eventually made hydrogen.

After years of development and testing, just such an observation station could come online as soon as 2026, in part thanks to researchers at the Lawrence Berkeley National Laboratory in California.

[Related: Watch a rocket engine ignite in ultra-slow motion.]

The team is currently working alongside NASA, the US Department of Energy, and the University of Minnesota on a pathfinder project called the Lunar Surface Electromagnetics Experiment-Night (LuSEE-Night). The radio telescope is on track to launch atop Blue Ghost, private space company Firefly Aerospace’s lunar lander, as part of the company’s second moon excursion. Once in position, Blue Ghost will detach from Firefly’s Elytra space vehicle, then travel down to the furthest site ever reached on the moon’s dark side. 

“If you’re on the far side of the moon, you have a pristine, radio-quiet environment from which you can try to detect this signal from the Dark Ages,” Kaja Rotermund, a postdoctoral researcher at Berkeley Lab, said in a September 26 project update. “LuSEE-Night is a mission showing whether we can make these kinds of observations from a location that we’ve never been in, and also for a frequency range that we’ve never been able to observe.”

More specifically, LuSEE-Night will be equipped with specialized antennae designed by the Berkeley Lab team to listen between 0.5 and 50 megahertz. To accomplish this, both the antennae and its Blue Ghost transport will need to be able to withstand the extreme temperatures experienced on the moon’s far side, which can span between -280 and 250 degrees Fahrenheit. Because of its shielded lunar location, however, LuSEE-Night will also need to beam its findings up to an orbiting satellite that will then transfer the information back to Earth.

“The engineering to land a scientific instrument on the far side of the moon alone is a huge accomplishment,” explained Berkeley Lab’s antenna project lead, Aritoki Suzuki, in the recent update. “If we can demonstrate that this is possible—that we can get there, deploy, and survive the night—that can open up the field for the community and future experiments.”

If successful, LuSEE-Night could provide data from the little known Dark Ages, which breaks up other observable eras such as some of the universe’s earliest moments, as well as more recent moments after stars began to form.

According to Berkeley Lab, the team recently completed a successful technical review, and is currently working on constructing the flight model meant for the moon. Once landed, LuSEE-Night will peer out into the Dark Age vastness for about 18 months beginning in 2026. 

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Albert Einstein didn’t know about the existence of antimatter when he came up with the theory of general relativity, which has governed our understanding of gravity ever since. More than a century later, scientists are still debating how gravity affects antimatter, the elusive mirror versions of the particles that abide within us and around us. In other words, does an antimatter droplet fall down or up? 

Common physics wisdom holds that it should fall down. A tenet of general relativity itself known as the weak equivalence principle implies that gravity shouldn’t care whether something is matter or antimatter. At the same time, a small contingent of experts argue that antimatter falling up might explain, for instance, the mystical dark energy that potentially dominates our universe.

“Everything about antimatter is challenging,” says Jeffrey Hangst, a physicist at Aarhus University in Denmark and a member of the ALPHA group. “It just really sucks to have to work with it.”

Adding to the challenge, gravity is extremely weak on the microscopic scale of atoms and subatomic particles. As early as the 1960s, physicists first thought about measuring gravity’s effects on positrons, or anti-electrons, which have positive rather than negative electric charge. Alas, that same electric charge makes positrons susceptible to tiny electric fields—and electromagnetism eclipses gravity’s force.

So, to properly test gravity’s influence on antimatter, researchers needed a neutral particle. The only “one of the horizon” was the antihydrogen atom, says Joel Fajans, a physicist at UC Berkeley and another member of the ALPHA group.

Antihydrogen is the first, most fundamental element of the anti-periodic table. Just as the garden-variety hydrogen atom consists of one proton and one electron, the basic antihydrogen atom consists of one negatively charged antiproton and an orbiting positron. Physicists only created antihydrogen atoms in the 1990s; they couldn’t trap and store some until 2010.

“We had to learn how to make it, and then we had to learn how to hold onto it, and then we had to learn how to interact with it, and so on,” says Hangst.

Once they overcame those hurdles, they were finally able to study antihydrogen’s properties—such as its behavior under gravity. For the new paper, the ALPHA group designed  a vertical vacuum chamber around a vertical tube devoid of any matter to prevent the antihydrogen from annihilating prematurely. Scientists wrapped part of the tube inside a superconducting magnetic “bottle,” creating a magnetic field that locked the antihydrogen in place until they needed to use it.

Building this apparatus took years on end. “We spent hundreds of hours just studying the magnetic field without using antimatter at all to convince ourselves that we knew what we were doing,” says Hangst. To produce a magnetic field strong enough to hold the antihydrogen, they had to keep the device chilled at -452 degrees Fahrenheit. 

The ALPHA group then dialed down the magnetic field to open the top and bottom of the bottle, and let the antihydrogen atoms loose until they crashed into the tube’s wall. They measured where those atomic deaths happened: above or under the position the antimatter was held in. Some 80 percent of atoms fell a few centimeters below the trap, in line with what a cloud of regular hydrogen atoms would do in the same setup. (The other 20 percent simply popped out.)

For instance, when the authors of the Nature study computed how rapidly the antihydrogen atoms accelerated downward with gravity, they found it was 75 percent of the rate physicists would expect for regular hydrogen atoms. But they expect the discrepancy to fade when they repeat these observations to find a more precise result. “This number and these uncertainties are essentially consistent with our best expectation for what gravity would have looked like in our experiment,” says William Bertsche, a physicist at the University of Manchester and another member of the ALPHA group.

But it’s also possible that gravity influences matter and antimatter in different ways. Such an anomaly would throw the weak equivalence principle—and, by extension, general relativity as a whole—into doubt.

“Any difference that you find between hydrogen and antihydrogen would be an extremely important clue to the baryogenesis problem,” says Fajans.

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About 40 light years away, a system of seven Earth-sized planets orbit a star that is much cooler and smaller than our sun— the exoplanetary system called TRAPPIST-1. When these exoplanets were discovered in 2016, astronomers speculated that they could one day support humans. Three of those worlds are located in the star’s habitable zone, also called the “Goldilocks zone,” where the conditions for life could be “just right.” Now, astronomers using the James Webb Space Telescope (JWST) have made important progress in understanding the atmosphere of one of its potentially habitable planets.

[Related: JWST’s double take of an Earth-sized exoplanet shows it has no sky.]

JWST observations ruled out the possibilities for a clear, extended atmosphere, failing to detect elements such as hydrogen. The telescope’s new detections also cut through the interference of the star at the center of this system, avoiding what astronomers call stellar contaminations. The findings are detailed in a study published September 22 in The Astrophysical Journal Letters.

The new study specifically sheds light on the nature TRAPPIST-1 b, the exoplanet that is closest to the system’s central star. The team from institutions in the United States and Canada used the JWST’s NIRISS instrument to observe TRAPPIST-1 b during two transits, when the planet passed in front of its star. 

The team used a technique called transmission spectroscopy to look deeper into the distant world. They saw the unique fingerprint left by the molecules and atoms that were found within the exoplanet’s atmosphere. “These are the very first spectroscopic observations of any TRAPPIST-1 planet obtained by the JWST, and we’ve been waiting for them for years,” study co-author and Université de Montréal doctoral student Olivia Lim said in a statement. 

In the past, stars at the center of solar systems may have hampered our understanding of far-off atmospheres. That’s because these suns can create “ghost signals” which fool observers into thinking they are seeing a particular molecule in the exoplanet’s atmosphere. This phenomenon, stellar contamination, is the influence of a star’s own features on the measurements of an exoplanet’s atmosphere.  A sun’s dark spots and bright faculae, or bright spots on its surface, can warp the chemical fingerprints that telescopes detect.

“In addition to the contamination from stellar spots and faculae, we saw a stellar flare, an unpredictable event during which the star looks brighter for several minutes or hours,” said Lim. “This flare affected our measurement of the amount of light blocked by the planet. Such signatures of stellar activity are difficult to model but we need to account for them to ensure that we interpret the data correctly.”

The team also used the observations to explore a range of atmospheric models for TRAPPIST-1 b. They ruled out the existence of cloud-free, hydrogen-rich atmospheres, which means that TRAPPIST-1 b likely does not have a clear and extended atmosphere around it. However, the data could not confidently rule out the possibility of a thinner atmosphere, perhaps made up of pure water, carbon dioxide, or methane. 

[Related: The James Webb Space Telescope just identified its first exoplanet.]

According to the team, this result underscores the importance of taking stellar contamination into account when planning future observations of all exoplanetary systems. This consideration is especially true for systems like TRAPPIST-1, because the system is centered around a red dwarf star which can be particularly active with frequent flare events and dark spots.

More observations will be needed to determine exactly what kind of atmosphere is surrounding this exoplanet and if it could support human life. “This is just a small subset of many more observations of this unique planetary system yet to come and to be analyzed,” study co-author and Université de Montréal astronomer René Doyon said in a statement. “These first observations highlight the power of NIRISS and the JWST in general to probe the thin atmospheres around rocky planets.”

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Trillions of particles from distant stars and galaxies are streaming through your body every second—you just can’t feel them. These ghost-like particles are called neutrinos. Although the universe spits them out constantly, these objects barely interact with matter—they can even slip through humanity’s toughest barriers, such as steel or lead walls. 

Some neutrinos come from supernovae, the extravagant deaths of the biggest stars; they’re also produced by radioactive decay in Earth’s rocks, reactions in the sun, and even our planet’s aurorae. These hard-to-see particles are all over the place and crucial to multiple areas of science, but we’re still in need of better ways of finding them. Now, a new observatory under construction in China’s Guangdong province—the Jiangmen Underground Neutrino Observatory, or JUNO—plans to hunt these elusive particles with better sensitivity than ever before. 

Like most neutrino detectors, it’s a huge vat filled with liquid for the neutrinos to interact with—the bigger the net, the more fish you’re likely to catch. “When it is completed, JUNO will be 20 times larger than the largest existing detector of the same type,” says Yufeng Li, a researcher and member of the JUNO collaboration at the Institute of High Energy Physics (IHEP) in Beijing. Currently under construction and expected to start operation in 2024, this detector will not only be bigger, but also more sensitive to slight variations in neutrinos’ energies than any of its predecessors. Li adds, it’s going to be “a unique and important observatory in the community.”

[Related: The Milky Way’s ghostly neutrinos have finally been found]

The observatory’s most ambitious goal is to preemptively spot neutrinos from stars that are dying but haven’t exploded yet. That way, telescopes can catch these stars in their final destructive act. “Neutrinos are expected to reach Earth hours earlier than photons because of their weakly-interacting nature,” explains Irene Tamborra, a physicist at the Niels Bohr Institute in Denmark not affiliated with the project. 

Astronomers still don’t know the finer details of how a star explodes, but observing the supernova as it starts might help give some clues. “The early detection of neutrinos will be crucial to point the telescopes in the direction of the supernova and catch its electromagnetic emission early on,” adds Tamborra. JUNO should be able to alert astronomers hours to days before a star is slated to explode, giving them time to prep and point their telescopes. It might even be able to measure the faint background of neutrinos coming from distant supernovae, all across the galaxy, which is of great interest to cosmologists trying to put together a picture of the whole universe. 

In addition to supernovae, the observatory will be searching for neutrinos from much closer to home: nuclear reactors. The nearby Yangjiang and Taishan nuclear power plants produce neutrinos, and physicists are hoping to get a taste of those neutrinos’ flavors with JUNO. Neutrinos come in three flavors (yes, they’re really called that!), known as the electron, tau, and muon neutrinos. They can flip between their different states in so-called oscillations. Scientists can calculate the number of neutrinos of each kind they expect from the power plant, and compare to what they actually observe with JUNO to better understand these flips.

[Related: This ghostly particle may be why dark matter keeps eluding us]

“It is also very likely that there will be surprise discoveries, as that often happens when powerful new experiments are deployed,” says Ohio State University astrophysicist John Beacom.

JUNO isn’t the only big observatory after neutrinos. The current largest liquid neutrino detector is Super-Kamiokande in Japan, and researchers there are planning a huge upgrade to make it the Hyper-Kamiokande. The United States is getting in the game too, currently using a detector at the Fermi National Accelerator Lab and planning its own multi-billion-dollar next-gen observatory, called the Deep Underground Neutrino Experiment. These projects are a few years away, though, so IHEP president Yifang Wang told Science that he gives JUNO “3-to-1 odds to get there first” to figure out some fundamental properties of neutrinos.

No matter who wins the race, this observatory is opening up one of our windows to the universe a bit wider. “JUNO is a huge step forward for neutrino physics and astrophysics,” Beacom says, “and I’m very excited to see what it will do.”

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A little less than one-third of the universe—around 31 percent—consists of matter. A new calculation confirms that number; astrophysicists have long believed that something other than tangible stuff makes up the majority of our reality. So then, what is matter exactly?

One of the hallmarks of Albert Einstein’s theory of special relativity is that mass and energy are inseparable. All mass has intrinsic energy; this is the significance of Einstein’s famous E=mc² equation. When cosmologists weigh the universe, they’re measuring both mass and energy at once. And 31 percent of that amount is matter, whether it’s visible or invisible.

That difference is key: Not all matter is alike. Very little of it, in fact, forms the objects we can see or touch. The universe is replete with examples of matter that are far stranger.

What is matter?

When we think of “matter,” we might picture the objects we see or their basic building block: the atom. 

Our conception of the atom has evolved over years. Thinkers throughout history had vague ideas that existence could be divided into basic components. But something that resembles the modern idea of the atom is generally credited to British chemist John Dalton. In 1808, he proposed that indivisible particles made up matter. Different base substances—the  elements—arose from atoms with different sizes, masses, and properties. 

Dalton’s schema had 20 elements. Combining those elements created more complex chemical compounds. When the chemist Dmitri Mendeleev constructed a primitive period table in 1869, he listed 63 elements. Today we have cataloged 118. 

But if only it were that simple. Since the early 20th century, physicists have known that tinier building blocks lurk within atoms: swirling negatively charged electrons and shrouded nuclei, made from positively charged protons and neutral neutrons. We know now, too, that each element corresponds to atoms with a certain number of protons.

[Related: How does electricity work?]

And it’s still not that simple. By the middle of the century, physicists realized that protons and neutrons are actually combinations of even tinier particles, called quarks. To be precise, protons and neutrons both contain three quarks each: a configuration type that physicists call baryons. For that reason, protons, neutrons, and the matter they form—the stuff of our daily lives—are often called “baryonic matter.”

Strange matter in the sky

In our everyday world, baryonic matter typically exists in one of four states: solid, liquid, gas, and plasma. 

Again, matter is not that simple. Under extreme conditions, it can take on a menagerie of more exotic forms. At high enough pressures, materials can become supercritical fluids, simultaneously liquid and gas. At low enough temperatures, multiple atoms coalesce together, creating the Bose-Einstein condensate. These atoms behave as one, acting in all sorts of odd quantum ways

Such exotic states are not limited to the laboratory. Just look at neutron stars: Their undead cores aren’t quite massive enough to collapse into black holes when they go supernova. Instead, as their cores crumple, intense forces rip apart their atomic nuclei and crush the rubble together. The result is essentially a giant ball of neutrons—and protons that absorb electrons, becoming neutrons in the process—and it’s very, very dense. A single spoonful of a neutron star would weigh a billion tons.

There are, potentially, hundreds of millions of neutron stars in the Milky Way alone. Deep in their centers, some scientists think, pressures and temperatures are high enough to rip neutrons apart too. Those neutrons may break the quarks that form them.

Physicists study neutron stars to learn about these objects—and what happened at the beginning of the universe. The matter we see around us did not always exist; it formed in the aftermath of the big bang. Before atoms formed, protons and neutrons swam alone through the universe. Even earlier, before there were protons and neutrons, everything was a superheated quark slurry.

Scientists can recreate that state, in some fashion, in particle accelerators. But that disappears in a flash that lasts a fraction of a second. It’s no comparison to the extremely long-lasting neutron stars  “You have a lab that basically exists forever,” says Fridolin Weber, a physicist at San Diego State University.

Matter in the grand scheme of the universe

Over the past several decades, astronomers have developed several ways to understand the universe’s basic parameters. They can examine its large-scale structure and identify  subtle fluctuations in the density of the matter they can see. They can watch how objects’ gravity bends passing light.

A specific way to measure matter density—the proportion of the universe made up of visible and invisible matter—is to pick apart the cosmic microwave background of the big bang. From 2009 to 2013, the European Space Agency’s Planck observatory prodded the afterglow to give scientists the best calculation of the matter density yet, 31 percent.

[Related: Does antimatter fall down or up? We now have a definitive answer.]

The most recent research used a different technique called the mass-richness relation, essentially examining clusters of galaxies, counting how many galaxies exist in each cluster, using that to calculate each group’s mass, and reverse-engineering the matter density. The technique isn’t new, but until now it was raw and unrefined.

“When we did our work, as far as I know, this is the first time that the mass-richness relation has been used to get a result that’s in very good agreement with Planck,” says Gillian Wilson, an astrophysicist at the University of California Riverside, and one of the authors of a paper published in The Astrophysical Journal on September 13. 

Yet remember, it’s not that simple. Only a small fraction—thought to be around 15 percent of matter, or 3 percent of the universe—is visible. The rest, most scientists think, is dark matter. We can detect the ripples that dark matter leaves in gravity. But we can’t observe it directly.

Consequently, we aren’t certain what dark matter is. Some scientists believe it is baryonic matter, just in a form that we can’t easily see: Perhaps it is black holes that formed in the early universe, for instance. Others believe it consists of particles that must barely interact at all with our familiar matter. Some scientists believe it is a mix of these. And at least some scientists believe that dark matter does not exist at all.

If it does exist, we might see it with a new generation of telescopes, such as eROSITA, the Rubin Observatory, the Nancy Grace Roman Space Telescope, and Euclid, that can scan ever greater swathes of the universe and see a wider variety of galaxies at different times in cosmic history. “These new surveys might change our understanding of the whole universe [and its matter],” says Mohamed El Hashash, an astrophysicist at the University of California Riverside, and another of the authors. “This is what I personally expect.”

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Every year or two, the solar system lines up just right, with the moon casting a shadow over part of Earth’s surface and blocking out the sun—a solar eclipse. In 2017, people across the United States flocked to see the “Great American Total Eclipse”, which was the first one visible in the continental states since 1979. Now, eclipse chasers and citizen scientists across North America are getting ready for the next big events: an annular eclipse on October 14, 2023 and a total eclipse on April 8, 2024. This will be the last eclipse visible in the continental US until August 2045, more than two decades away. 

People love eclipses for the novelty—how cool it is to see the sun disappear in the day. But these phenomena are both showstoppers and opportunities: a group of radio astronomers and citizen scientists called Radio JOVE is aiming to capitalize on the upcoming eclipses for science, part of NASA’s “Helio Big Year.”

Radio JOVE “initially started as an education and outreach project to help students, teachers, and the general public get involved in science,” explains project co-founder Chuck Higgins, an astronomer at Middle Tennessee State University. The project has been running since the late 1990s, when it began at NASA’s Goddard Space Flight Center. “We now focus on science and try to inspire people to become citizen scientists.” 

As its name suggests, Radio JOVE originally focused on the Jovian planet, Jupiter. “Serendipitously, it turns out that the same radio wavelengths we use for observing Jupiter are also useful for observing the sun,” says Thomas Ashcraft, a citizen scientist from New Mexico who has been observing with Radio JOVE since 2001. After the 2017 Great American Eclipse, its members became more involved with heliophysics, the study of the sun.

[Related: Total eclipses aren’t that rare—and you’ve probably missed a bunch of them]

As energy spews from the sun and travels to Earth, it interacts with our planet’s atmosphere; in particular, the sun’s rays create a layer of ionized particles, known as the ionosphere. Any radio waves coming from the sun have to pass through these particles above us. Communication technology takes advantage of this layer, bouncing radio waves off it to travel long distances.

The ionosphere’s plasma changes a lot between day and night. When the sun shines on this layer, particles break into ions. When the sun is absent, those ions calm down. During eclipses, when most of the sun’s light is blocked, similar changes happen in the short term change. By measuring those fluctuations precisely with a fleet of amateur observers, Radio JOVE hopes to improve our understanding of the ionosphere.

To do so, Radio JOVE is equipping citizen scientists across the country with small radio receivers and training them to observe radio waves from Earth’s ionosphere. The project offers some-assembly-required starter kits for around $200, and a whole team of experts and experienced observers are around to support new volunteers. 

[Related: The best US parks for eclipse chasers to see October’s annularity]

Right now, they’re prepping participants for a full day of observing during the October annular eclipse. Project members are already gathering data to have a baseline of the sun’s influence on a normal day, which they’ll compare to the upcoming eclipse data. And this is only a small taste before the big event: next year’s total eclipse. “The 2023 annular eclipse will be used as a training, learning, and testing experience in an effort to achieve the highest quality data for the 2024 total eclipse,” Higgins wrote in a summary for an American Geophysical Union conference.

Citizen science projects such as Radio JOVE not only collect valuable data, but they also involve a new crowd in NASA’s scientific community. Anyone interested in science can join in, and if Radio JOVE doesn’t suit your interests, NASA has a long list of other opportunities. For example, if you’re a ham radio operator, you can get involved with HamSCI, which also plans to observe the upcoming eclipse.

“NASA’s Radio JOVE Citizen Science Project allows me to further explore my lifelong interest in astronomy,” said John Cox, a Radio JOVE citizen scientist from South Carolina, in a NASA press release. “A whole new portion of the electromagnetic spectrum is now open to me.”

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Is Earth primarily a planet of life, a world stewarded by the animals, plants, bacteria, and everything else that lives here? Or, is it a planet dominated by human creations? Certainly, we’ve reshaped our home in many ways—from pumping greenhouse gases into the atmosphere to literally redrawing coastlines. But by one measure, biology wins without a contest.

 In an opinion piece published in the journal Life on August 31, astronomers and astrobiologists estimated the amount of information transmitted by a massive class of organisms and technology for communication. Their results are clear: Earth’s biosphere churns out far more information than the internet has in its 30-year history. “This indicates that, for all the rapid progress achieved by humans, nature is still far more remarkable in terms of its complexity,” says Manasvi Lingam, an astrobiologist at the Florida Institute of Technology and one of the paper’s authors.

[Related: Inside the lab that’s growing mushroom computers]

But that could change in the very near future. Lingam and his colleagues say that, if the internet keeps growing at its current voracious rate, it will eclipse the data that comes out of the biosphere in less than a century. This could help us hone our search for intelligent life on other planets by telling us what type of information we should seek.

To represent information from technology, the authors focused on the amount of data transferred through the internet, which far outweighs any other form of human communication. Each second, the internet carries about 40 terabytes of information. They then compared it to the volume of information flowing through Earth’s biosphere. We might not think of the natural world as a realm of big data, but living things have their own ways of communicating. “To my way of thought, one of the reasons—although not the only one—underpinning the complexity of the biosphere is the massive amount of information flow associated with it,” Lingam says.

Bird calls, whale song, and pheromones are all forms of communication, to be sure. But Lingam and his colleagues focused on the information that individual cells transmit—often in the form of molecules that other cells pick up and respond accordingly, such as producing particular proteins. The authors specifically focused on the 100 octillion single-celled prokaryotes that make up the majority of our planet’s biomass. 

“That is fairly representative of most life on Earth,” says Andrew Rushby, an astrobiologist at Birkbeck, University of London, who was not an author of the paper. “Just a green slime clinging to the surface of the planet. With a couple of primates running around on it, occasionally.”

Now, picture the reverse. For decades, scientists and military experts have sought out signatures of extraterrestrials in whatever form it may take. Astronomers have traditionally focused on the energy that a civilization of intelligent life might use—but earlier this year, one group crunched the numbers to determine if aliens in a nearby star system could pick up the leakage from mobile phone towers. (The answer is probably not, at least with LTE networks and technology like today’s radio telescopes.)

On the flip side, we don’t totally have the observational capabilities to home in on extraterrestrial life yet. “I don’t think there’s any way that we could detect the kind of predictions and findings that [Lingam and his coauthors] have quantified here,” Rushby says. “How can we remotely determine this kind of information capacity, or this information transfer rate? We’re probably not at the stage where we could do that.”

But Rushby thinks the study is an interesting next step in a trend. Astrobiologists—certainly those searching for extraterrestrial life—are increasingly thinking about the types and volume of information that different forms of life carries. “There does seem to be this information ‘revolution,’” he says, “where we’re thinking about life in a slightly different way.” In the end, we might learn that there’s more harmony between the communication networks nature has built and computers.

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At first glance, everything seems solid. Then, a small rip begins to spread across the middle of the structure as its siding expands. The module suddenly bursts apart, spraying debris in every direction as engineers cheer on from the safety of their control room. The sudden destruction—and the fifth such explosion—of a module intended for the International Space Station’s successor may not sound like the desired outcome, but, scientists say, it’s all part of the plan.

In Sierra Space’s September 20 progress update, the Colorado-based company released video of the explosion. The company aims to supply habitat spaces for Orbital Reef, Blue Origin’s NASA-backed space station project. During a recent Ultimate Burst Pressure (UPB) test, the engineering team essentially amped up the pressure within a one-third-scale LIFE module prototype until it popped. Said “pop” is certainly a sight to behold:

Unlike ISS construction materials, the LIFE modules are largely composed of “softgoods” such as Vectran, an incredibly strong and durable synthetic fiber spun from liquid-crystal polymers. When inflated, the LIFE module’s softgood design becomes rigid enough to withstand the low-earth orbit’s extreme environmental stresses. According to Sierra Space, the latest results offered a 33 percent margin over a full-scale LIFE module’s certification standard, nearly 20 percent better than the previous test design.

What makes the most recent UPB test especially impressive is that it was the first module prototype to include a steel “blanking plate” that acted as a cheaper stand-in for essential design features like windows.

[Related: NASA is spending big on commercial space destinations.]

“Inclusion of the blanking plate hard structure was a game-changer because this was the first time that we infused metallics into our softgoods pressure shell technology prior to conducting a UBP test,” Shawn Buckley, Sierra Space’s Senior Director Engineering and Product Evolution, said in the company’s announcement. “With this added component, once again, we successfully demonstrated that LIFE’s current architecture at one-third scale meets the minimum 4x safety factor required for softgoods inflatables structures.”

As Space.com notes, this marks the third UPB test for the module prototypes. Sierra Space has also overseen two “creep tests” in December 2022 and February 2023, during which the LIFE designs were subjected to higher-than-usual pressures for extended periods of time. With the latest success, Sierra Space says it’s now ready to move onto the next development phase—testing on full-scale LIFE module prototypes. If all goes as planned (a big “if,” given such endeavors’ complexities), future LIFE module iterations will be some of Orbital Reef’s central structures. Orbital Reef is currently intended to start construction in 2030.

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On the morning of September 24, a space capsule containing a pristine sample of the near-Earth asteroid Bennu entered Earth’s atmosphere wreathed in fire. During a 10 minute descent, the craft used its heat shield to dissipate speed through friction. It safely touched down on a military range in Utah, marking the end of NASA’s seven-year-long Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer—the OSIRIS-REx mission. The roughly 9 ounces of asteroid bits, doused in nitrogen to keep out any contaminants, are now in a clean room.

For more than half a decade, the members of this mission faced multiple technical challenges: building, testing, and launching the OSIRIS-REx spacecraft in 2016; rendezvousing with asteroid Bennu in 2018 about 207 million miles from Earth; using a robotic arm to grab half a cup’s worth of Bennu in 2020; and setting a course back to Earth in 2021. 

The scope of the OSIRIS-ReX mission stretches from the distant past into the relatively closer future. Nearly two decades ago, astronomers set out to not only get up close and personal with an ancient asteroid, but actually bring some home. And its scientific observations dip billions of years into the past. Samples from this more than 4.5 billion-year-old asteroid are likely to provide clues to the origin of life itself. It will also help prepare us for a moment, centuries from now, when Bennu could threaten to strike Earth. 

The power of a pristine asteroid 

The OSIRIS-REx sample is a chance to thoroughly examine what compounds may have been present in the early solar system. By bringing pieces of the space rock to Earth, researchers can use the most powerful laboratory techniques available—not just what tools can fit on a spacecraft. 

”It’s tremendously powerful to be able to get something back in the laboratory,” says Jason Dworkin is a biochemist and astrobiologist at NASA’s Goddard Space Flight Center. He’s been the project scientist for OSIRIS-REx since NASA accepted the mission proposal in 2011, and has been involved in the mission’s planning since its conception in 2004. “You can change your mind about what you’re looking for. As new discoveries come in, you can adjust your instrumentation. You can have devices that are not only too large to get on the spacecraft, but for us, even larger than the launch pad.” 

[Related: The asteroid that created Earth’s largest crater may have been way bigger than we thought]

Dworkin has long been interested in the ways interstellar chemistry can shed light on how the early Earth’s organic compounds combined to form life as we know it. It’s possible that material from asteroids, made of similar stuff as Bennu, helped deliver some necessary ingredients when they struck our planet.

We know the strikes happened, Dworkin says, but we don’t know how relevant the “asteroidal input” from objects like Bennu was.

Rapidly recovering the sample

Before scientists like Dworkin can probe the bits of rock for data, they have to get the samples safely into the lab. Sample collection teams—NASA experts and academic mission scientists, US military representatives, and scientists and engineers from Lockheed Martin, which built the OSIRIS-REx spacecraft—have spent the summer practicing to recover the Bennu sample as quickly as possible. 

As the capsule neared Earth’s atmosphere, the recovery teams boarded helicopters, using infrared imaging to track the capsule as it descended. They swiftly arrived to where the capsule came to rest, within a 36-mile by 8.5-mile area of the Department of Defense’s Utah Test and Training Range near Salt Lake City. The reason for the haste is to limit the chances that anything Earthly would contaminate the 8.8 ounces of pristine Bennu material. 

To further guard against this, the team recovering the capsule also took samples of soil and material from around the landing site. That way, if scientists detect something “extraordinary,” Dworkin says, “we can make sure that it cannot be explained by contamination or by something else from the environment.”

The capsule, which slowed from 27,650 mph when it entered Earth’s atmosphere to 11 mph when it landed, was taken to a temporary clean room at the military range. There, it will be disassembled and on Monday packaged for a flight to NASA’s Johnson Space Center in Houston, where the space agency has built a specialized clean room environment. This will be Bennu’s home on Earth.

“The sample comes back and is studied by the science team for two years,” Dworkin says. “Within six months, we produce a catalog of what we’ve observed based on how to describe the sample without damaging the sample using non-invasive techniques.”

What an asteroid on Earth can tell us

The science team has 12 major hypotheses and 54 sub-hypotheses to test, according to Dworkin, which fall into four broad categories. 

The first category is testing the observations that OSIRIS-REx made of Bennu while in space. NASA wants to know: If the results of remote instrument measurements of, say, the asteroid’s mineralogy hold up when tested on the ground? If so, this will be a baseline for additional remote studies of other asteroids NASA won’t send a spacecraft to sample. 

The second category, Dworkin’s favorite, is examining what organic compounds might exist in the sample. It may contain amino acids, sugars, and aldehydes. These are potentially some of the same ingredients that were present on Earth when life began. Studying how they exist on Bennu can reveal the chemical changes they’ve undergone over the eons in space. 

The history of the solar system is the third category. This is the tale, told by the sample, of our solar neighborhood: all the way “from the protosolar nebula to the formation of the crater out of which we collected the sample,” Dworkin says. In this view, as Bennu traveled in the frigid space, it was as if material from the solar system’s early days was held in cold storage.

[Related: Local asteroid Bennu used to be filled with tiny rivers]

And the fourth category of study will be analyzing if and how bringing a piece of Bennu home changes the sample. ”We saw images of it before we stowed it; is that the same, or did it change on the reentry into Earth’s atmosphere?” Dworkin says. “Do we have evidence of contamination from the spacecraft, from the sample processing and handling? 

Some of the answers to questions across all four categories could come within months to a few years. But NASA is preparing for the long haul. Today’s scientists will only have immediate access to about a quarter of the sample. The rest will be held in cold storage for decades, on the assumption that later generations will have better tools and more knowledge to bring to bear. 

NASA wants to avoid repeating mistakes the agency made with some of the Apollo-era moon samples, when tests weren’t as conservative with lunar material. “ “That’s arming the future, and making sure that future generations thank us instead of curse us,” Dworkin says.

There’s one final forward-looking aspect to the OSIRIS-REx mission. In the late 22nd century, sometime between 2170 and 2200, Bennu has a slim chance of hitting Earth. It’s “a small percentage, but not nothing,” Dworkin notes. Information gathered by OSIRIS-REx and subsequent sample studies could help scientists and political leaders decide, with decades of preparation, whether they need to take action to deflect Bennu to prevent a disastrous impact. 

”That’s a wonderful feeling to be able to work on a mission for so long, and have it pay off scientifically for the future, and perhaps planetary defense for the future,” Dworkin says. ”That happens when you start thinking about what happened four and a half billion years ago. You start thinking about the future too.”

Back in space, 20 minutes after this mission came to an end, the spacecraft’s new task began: OSIRIS is now headed for the 1,000-foot-wide asteroid Apophis.

This post was updated after the capsule’s successful landing.

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On April 20, the most powerful rocket ever flown stood on a launch pad in Boca Chica, Texas, its stainless steel skin gleaming in the sun. Moments later, rocket and launch pad would become fiery debris. It was the first, disastrous orbital test launch of the SpaceX Starship.

Within seconds of launching, the rocket’s ferocious thrust shattered the concrete pad at SpaceX’s Texas Starbase facility, sending debris flying as far as Port Isabel, a city six miles away. The rocket caught fire. Less than four minutes after launch, it began to tumble across the sky, and then it exploded.

The Federal Aviation Administration grounded Starship, pending an investigation into the explosion, but the rocket may soon fly again. On September 8, the FAA closed its inquiry, citing 63 corrective actions SpaceX would need to take before its second attempt to send Starship to orbit. 

“The FAA has approval authority on all commercial launches, and so they are the ones who grant companies launch licenses,” says Wendy Whitman Cobb, a space policy expert and instructor at the US Air Force School of Advanced Air and Space Studies. “Any time something blows up, they want to know why. Because they want to make sure that it’s safe not only to go up, but that it’s not going to harm anybody on the ground.”

SpaceX will have to demonstrate to the FAA that the company has successfully completed those 63 corrective actions and then apply for a modified launch license. “Once that is granted, they theoretically can go up whenever they want,” Whitman Cobb says. Neither FAA nor SpaceX have publicly said what those fixes are. But the actions presumably address the failures of the April launch.

There’s a lot riding on Starship’s success. It’s key to expanding SpaceX’s launch and Starlink satellite businesses. NASA plans to return humans to the moon in 2025 with a modified Starship as the lunar landing vehicle on the Artemis III mission. If SpaceX can fix the problems—and Whitman Cobb and other experts believe that’s likely—the company may put its rocket program and NASA’s moon program back on track. This investigation might also provide insights into launch pad construction that could one day help astronauts traveling to and from the moon. 

Failures to launch

Starship, despite not yet reaching orbit, holds the title for most powerful rocket ever launched—a superlative it took from the Soviet N1 rocket. Meant to power Soviet cosmonauts to the moon, the N1 first stage produced 10.2 million pounds of thrust. Starship has two stages in its “stack;” the first stage alone, the Super Heavy Booster, produces 16.7 million pounds of thrust. 

That record-breaking power is why it was bizarre that SpaceX chose to launch Starship from a concrete launch pad without features such as flame trenches. Those grooves are designed to divert a rocket’s plume away from the pad and the vehicle itself. SpaceX could have also used a water deluge system to flood the pad to help mitigate the rocket engines’ heat and acoustic shockwaves. 

[Related: SpaceX’s Falcon Heavy launches have been a slow burn—for an interesting reason]

“You would never normally launch a rocket with that much thrust without having a better designed active mitigation of the plume in the launch environment. Because you worry about the heat and the dynamic forces of the plume breaking materials and creating ejecta,” says University of Central Florida physicist Philip Metzger. ”If the ejecta had hit the launch vehicle in a way that caused the rocket to explode while it was still near the tower, it could have destroyed a lot of infrastructure that would have taken a very long time to rebuild.”

As it was, the April launch blew the launch pad apart and dug a crater “about as deep as a house,” he says. 

Lessons for the moon

Metzger has been studying the Starship launch and is currently writing a paper about the results. He wants to understand what went wrong—because the way things failed is important for the design of future rockets and landing pads on the moon or other celestial bodies. 

Most concepts for a lunar landing pad simply use flat concrete. “There’s no flame diverter, no flame trench, no water,” Metzger says. “I decided just because of the pure fun of solving the physics, and also because of what we might learn about lunar landing pads, that I was going to take this seriously.”

What he found was that chunks of concrete from the Boca Chica pad were flung away at more than 200 miles per hour. A cloud of hot water vapor and carbon dioxide, created by Starship’s methane- and liquid oxygen-burning Raptor engines, heaved sand skyward and carried it to Port Isobel. Metgzer realized the process must have been similar to the way pressure builds in a volcano before an eruption. 

“The only explanation we could come up with was that the landing pad cracked and the high pressure of the thrust drove gas through the cracks,” he says. This increased pressure beneath the pad until it erupted. Lunar landing pads must be designed to avoid this problem, he says, by adding vents for gases to escape or by constructing stronger pads that resist fracture. 

[Related: DOJ is suing SpaceX for years of workplace discrimination]

That could be difficult on the moon, where heavy construction will be hindered by a lack of resources, machinery, and an atmosphere. But on Earth, SpaceX may have a solution—a steel plate that is actively cooled with water to keep it from melting during a rocket launch. 

”That’s really a great idea,” Metzger says. “If their engineers did it correctly, it should be a complete solution to the problem.”

As for keeping the next Starship from blowing up in the sky, SpaceX says it found that leaked fuel had ignited inside the Super Heavy Booster. The resulting fires cut the booster off from the computer guiding its flight, which caused the rocket to tumble and then explode, according to an update on its website. The company has “significantly expanded Super Heavy’s pre-existing fire suppression system in order to mitigate against future engine bay fires,” the company says. 

Next moves

While neither the FAA nor SpaceX have said where the two are in the process, SpaceX Founder Elon Musk has suggested that his company has completed the corrective tasks, tweeting on September 5, before the FAA announcement, that ”Starship is ready to launch, awaiting FAA license approval.”

If the ball is truly in the FAA’s court and the regulator is simply reviewing the work SpaceX has done, “I don’t think it will take more than a few weeks,” Whitman Cobbs says. “That would be my best guess.” If that’s the case, she notes, then SpaceX and the FAA have moved with exceptional speed to get Starship ready for another launch attempt. Whitman Cobb contrasted SpaceX with its competitor Blue Origin, whose New Shepard rocket remains grounded more than a year after a failed launch on September 12, 2022. Blue Origin is “still in the FAA investigation mode, and have not been able to launch,” she says. “They’ve yet to apply for a modified launch license.”

Rapidly reworking Starship and its launch pad, though, doesn’t guarantee the next launch attempt will go flawlessly. But Whitman Cobb notes that SpaceX has been more willing than NASA or other rocket makers to test new spacecraft, watch them fail, and rapidly make changes. The eighth Starship prototype was destroyed in a fiery belly flop during a high-altitude test in December 2020, for instance, but the company pressed on. 

“Given the ability of SpaceX to succeed and prove its critics wrong in the past few years, I have no evidence to believe they wouldn’t be able to make this work,” she says. 

Metzger also notes that the person in charge of getting Starship ready to fly again is William Gerstenmaier, who, before joining SpaceX in 2020, was the former associate administrator for Human Exploration and Operations at NASA. “Gerstenmaier is a legend in the space community,” Metzger says. ”It’s in really good hands. I don’t know if there’s anybody better in the world than Bill Gerstenmaier to manage that sort of a project.”

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Rocket ignitions are always impressive, but they’re not the easiest to look at with the naked eye for pretty obvious reasons—you can’t be anywhere near their incinerating temperatures, and their brightness is generally blinding. Thanks to popular YouTubers’ high-speed video capabilities, however, curious minds can take a look at a recent test firing to see the complex, beautiful, and perhaps terrifying ignition in action.

The new footage comes courtesy of The Slow Mo Guys, a team of videographers specializing in… well, you can connect the dots. The YouTubers were given a front row seat at a test ignition for one of Firefly Aerospace’s Reaver engines, but unlike previous excursions, this project required quite a bit of preplanning. First off, The Slow Mo Guys only had one chance to nab the shot, since rockets traditionally use up huge amounts of fuel and resources—a single SpaceX Falcon9 rocket, for example, uses tens of thousands of gallons of kerosene and liquid oxygen. 

That single attempt also needed to be positioned, rigged, and timed to begin filming at enough of a distance that wouldn’t injure anything, or anyone. According to Slow Mo Guy Gav Free, a special enclosure capable of withstanding the intense heat and vibrations needed to house their slow-motion camera, while also calibrating the equipment to handle the explosion’s brightness. In the end, Free and his companions settled on exposing their film well over 40 percent darker than usual to account for the luminosity.

All that prep work definitely paid off, judging from the footage. At 2,000 frames-per-second (80 times slower than real time), viewers may be surprised to see an initial, bright green flame. This is produced as a rocket fuel mixture called triethylaluminium-triethylborane (TEA-TEB) combusts upon coming into contact with oxygen and air. After the initial green burst comes the yellow and orange flames—but with such a slow framerate, you can actually see those flames responding to the shockwaves generated by the engine thrust. According to Free, a rocket engine can generate upwards of 45,000 lbs of thrust in a vacuum at temperatures as high as 5,500 F.

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On October 14, the moon will cruise between Earth and the sun during an annular solar eclipse, casting an immense shadow on our planet. It will be a sight to behold, though you’ll want to wear protective glasses or glimpse it indirectly to avoid frying your eyeballs. Unlike 2017’s total eclipse, the sun won’t vanish completely; instead, the moon will be positioned far enough from our planet to leave the star’s brilliant edges visible. The result is a “ring of fire,” as though the moon has been outlined with a blowtorch. Every continental state will have at least a partial view of this event, but spotting this celestial circle could be well worth the travel. 

The eclipse’s 125-mile-wide path of annularity begins in the US in Oregon at 12:13 p.m. Eastern (9:13 a.m. Pacific). It will loom over the country until it leaves Texas at 1:03 p.m. (12:03 Central), continuing its southeastward journey to Central and South America. The best viewing conditions will be in places with low fog and high aridity, like Nevada and Utah, the two driest states in the country. “The place with the lowest chance of cloud cover is Albuquerque, New Mexico—but most of the path of annularity looks pretty good,” says University of Texas at San Antonio astrophysics professor Angela Speck, who co-chairs the American Astronomical Society’s Solar Eclipse Task Force.  

Oregon

The first US national park that the eclipse will pass over is Crater Lake, where water has filled a collapsed volcano, Mount Mazama. All of the park is in the annularity’s path, so prepare for crowds as well as limited parking and lodging.

Other Oregon parks in the path:
Shore Acres State Park

[Related: We’ve been predicting eclipses for over 2,000 years. Here’s how.]

California

Bat-filled caves, battlefields, and basaltic flows make up Lava Beds National Monument, a desert landscape that is the product of thousands of years of volcanic activity. Only the northeast sliver of this California park is directly in the annularity’s path, but the section just outside it may be a good vantage for another fascinating feature of the eclipse: Baily’s beads, short-lived bright dots caused when sunbeams stream through the crags and valleys of the lunar surface.

Nevada

The southern edge of the US path of annularity cuts through Great Basin National Park, where park staff will be available to guide viewers, according to the National Park Service. The agency also notes that, while the park tends to be less busy in October, eclipse watchers should be prepared for the event to bring out crowds.

Utah

Parsons-Bernstein ordered 20,000 eclipse glasses that will be distributed across Utah’s state parks on a first come, first serve basis. “In the entire state, there’s no less than 83 percent view of the annularity,” she says. But several areas are “dead-on 100 percent,” including 13 parks that are directly in the eclipse’s path. One of those is Goblin Valley State Park, which boasts rocky scenery so otherworldly that the movie Galaxy Quest used it as an alien planet.

Other Utah parks in the path:
Bryce Canyon National Park
Capitol Reef National Park
Canyonlands National Park
Escalante Petrified Forest State Park
Glen Canyon National Recreation Area
Goosenecks State Park
Kodachrome Basin State Park
Hovenweep National Monument
Natural Bridges National Monument
Rainbow Bridge National Monument
Territorial Statehouse State Park Museum

Arizona 

The moon’s shadow will zip into Arizona at speeds of around 3,150 mph, slowing to 2,626 mph as it leaves. It will pass through Navajo National Monument, where, for hundreds of years, Hopi, Navajo, and other Native Americans lived in the canyons. However, visitors to the Hopi Reservation and Navajo Nation should be aware that, in some traditions, eclipses are sacred times to pray or meditate indoors. 

Other Arizona parks in the path:
Canyon De Chelly National Monument

[Related: 7 US parks where you can get stunning nightsky views]

Colorado

Celebrating its remarkable Ancestral Pueblo cliff settlements, Mesa Verde National Park became a UNESCO World Heritage Site in 1978. Go for the eclipse, but stick around after nightfall on campgrounds and scenic overlooks: The park has one of the darkest skies in the continental US, and boasts stellar views of the Milky Way.

Other Colorado parks in the path:
Yucca House National Monument

New Mexico

The Manhattan Project National Historical Park at Los Alamos was once the secret city where physicists developed the atomic bomb. Now, certain areas are open to the public (many of the buildings are within an area secured by the Energy Department that’s only occasionally available by guided tour). But hikers can take the trail loop on Kwage Mesa, which will offer views of the annularity.

Other New Mexico parks in the path:
Aztec Ruins National Monument
Bandelier National Monument
Chaco Culture National Historical Park
Pecos National Historical Park
Petroglyph National Monument
Rio Grande Nature Center State Park
Salinas Pueblo Mission National Monument
Valles Caldera National Preserve

Texas

As the eclipse falls over the Lone Star State, it will darken 17 state parks as well as San Antonio Missions National Historical Park. Just after noon, it will depart the US for the Gulf of Mexico, but not before touching one last bit of public American land: the Padre Island National Seashore, which is just a quick drive from Corpus Christi and famous for its unique, biodiverse mudflats.

Other Texas parks in the path:
Big Spring State Park
Choke Canyon State Park
Goose Island State Park
Kickapoo Cavern State Park
Lake Corpus Christi State Park
Mustang Island State Park

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An unexpected and astonishing find located more than 2.5 million light-years from Earth took top honors at the Royal Observatory Greenwich’s Astronomy Photographer of the Year awards this week. Amateur astronomers Marcel Drechsler, Xavier Strottner, and Yann Sainty captured an image of a massive plasma arc near the Andromeda Galaxy, a discovery that has resulted in scientists looking closer into the giant gas cloud.

“This astrophoto is as spectacular as [it is] valuable,” judge and astrophotographer László Francsics said in a press release. “It not only presents Andromeda in a new way, but also raises the quality of astrophotography to a higher level.”

[Related: How to get a great nightsky shot]

While “Andromeda, Unexpected” captured the prestigious overall winner title, other category winners also dazzled with photos of dancing auroras, neon sprites raining down from the night’s sky, and stunning far-off nebulas that might make you feel like a tiny earthling floating through space.

Sit back and scroll in awe at all the category winners, runners-up, and highly commended images from the 2023 Royal Observatory Greenwich’s Astronomy Photographer of the Year honorees.

Galaxy

Overall winner: Andromeda, Unexpected

Runner-Up: The Eyes Galaxies

Highly Commended: Neighbors

Aurora

Winner: Brushstroke

Runner-up: Circle of Light

Highly Commended: Fire on the Horizon

Our Moon

Winner: Mars-Set

Runner-Up: Sundown on the Terminator

Highly Commended: Last Full Moon of the Year Featuring a Colourful Corona During a Close Encounter with Mars

Our Sun

Winner: A Sun Question

Runner-Up: Dark Star

Highly Commended: The Great Solar Flare 

People & Space

Winner: Zeila

Runner-Up: A Visit to Tycho

Highly Commended: Close Encounters of The Haslingden Kind

Planets, Comets & Asteroids

Winner: Suspended in a Sunbeam

Runner-Up: Jupiter Close to Opposition

Highly Commended: Uranus with Umbriel, Ariel, Miranda, Oberon and Titania

Skyscapes

Winner: Grand Cosmic Fireworks

Runner-Up: Celestial Equator Above First World War Trench Memorial

Highly Commended: Noctilucent Night

Stars & Nebulae

Winner: New Class of Galactic Nebulae Around the Star YY Hya

Runner-Up: LDN 1448 et al.

Highly Commended: The Dark Wolf – Fenrir

The Sir Patrick Moore Prize for Best Newcomer

Winner: Sh2-132: Blinded by the Light

Young Astronomy Photographer of the Year

Winner: The Running Chicken Nebula

Runner-Up: Blue Spirit Drifting in the Clouds

Highly Commended: Lunar Occultation of Mars

Highly Commended: Roses Blooming in the Dark: NGC 2337

Highly Commended: Moon at Nightfall

Annie Maunder Prize for Image Innovation

Winner: Black Echo

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This post has been updated.

A new NASA-commissioned independent study report recommends leveraging NASA’s expertise and public trust alongside artificial intelligence to investigate unidentified aerial phenomena (UAP) on Earth. As such, today NASA Director Bill Nelson announced the appointment of a NASA Director of UAP Research to develop and oversee implementation of investigation efforts.

“The director of UAP Research is a pivotal addition to NASA’s team and will provide leadership, guidance and operational coordination for the agency and the federal government to use as a pipeline to help identify the seemingly unidentifiable,” Nicola Fox, associate administrator of the Science Mission Directorate at NASA, said in a release.

Although NASA officials repeated multiple times that the study found no evidence of extraterrestrial origin, they conceded they still “do not know” the explanation behind at least some of the documented UAP sightings. Nelson stressed the agency’s aim to begin minimizing public stigma surrounding UAP events, and begin shifting the subject “from sensationalism to science.” In keeping with this strategy, the panel report relied solely on unclassified and open source UAP data to ensure all findings could be shared openly and freely with the public.

[Related: Is the truth out there? Decoding the Pentagon’s latest UFO report.]

“We don’t know what these UAP are, but we’re going to find out,” Nelson said at one point. “You bet your boots.”

According to today’s public announcement, the study team additionally recommends NASA utilize its “open-source resources, extensive technological expertise, data analysis techniques, federal and commercial partnerships, and Earth-observing assets to curate a better and robust dataset for understanding future UAP.”

Composed of 16 community experts across various disciplines, the UAP study team was first announced in June of last year, and began work on their study in October. In May 2023, representatives from the study team expressed frustration with the fragmentary nature of available UAP data.

“The current data collection efforts regarding UAPs are unsystematic and fragmented across various agencies, often using instruments uncalibrated for scientific data collection,” study chair David Spergel, an astrophysicist and president of the nonprofit science organization the Simons Foundation, said at the time. “Existing data and eyewitness reports alone are insufficient to provide conclusive evidence about the nature and origin of every UAP event.”

Today’s report notes that although AI and machine learning tools have become “essential tools” in identifying rare occurrences and outliers within vast datasets, “UAP analysis is more limited by the quality of data than by the availability of techniques.” After reviewing neural network usages in astronomy, particle physics, and other sciences, the panel determined that the same techniques could be adapted to UAP research—but only if datasets’ quality is both improved and codified. Encouraging the development of rigorous data collection standards and methodologies will be crucial to ensuring reliable, evidence-based UAP analysis.

[Related: You didn’t see a UFO. It was probably one of these things.]

Although no evidence suggests extraterrestrial intelligence is behind documented UAP sightings, “Do I believe there is life in the universe?” Nelson asked during NASA’s press conference. “My personal opinion is, yes.”

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What’s it like to spend a whole year in space? In just a matter of days, US astronaut Frank Rubio will be able to tell the tale. On Wednesday, he broke the record for the longest space mission taken by a US astronaut by spending 355 days in low orbit. He and his fellow Expedition 69 crew members are awaiting three new members that will arrive at the end of the week, according to NASA. 

The seven Expedition 69 members are actually a mashup of two groups, one of which, including Rubio, has been onboard for nearly a year. A Russian Soyuz capsule isn’t expected to return him and his crewmates back to Earth until September 27—meaning his full space trip will hit 371 days. This return date was rescheduled from an original March 2023 timeline so Russia could prepare the vehicle, according to CNN.

When leaving for the International Space Station, Rubio was only expected to spend six months up there. When the Russian Soyuz capsule holding him sprang a coolant leak back in December, the Russian space agency ruled that the craft wasn’t safe enough to bring Rubio and his colleagues back. In March, it made a solo trip back home, while in February a new Soyuz capsule made its way to the ISS. 

[Related: “How Russia’s war in Ukraine almost derailed Europe’s Mars rover” ]

“Rubio’s journey in space embodies the essence of exploration,” NASA administrator Bill Nelson said in a social media statement on Monday, adding that Rubio’s dedication to space research paves the way for future endeavors by a new generation of astronauts. 

While Rubio’s feat beats out previous records set by retired NASA astronaut Mark Vande Hei in 2022 and Scott Kelly in 2015-2016, Russia still holds the record for longest trip to space. Between January 1994 and March 1995, astronaut Valeri Polyakov spent 437 continuous days in orbit. Another Russian astronaut, Gennadi Padalka, set the record of most cumulative days in space—879—over the course of five different flights in 2015.

This adventure certainly wasn’t planned, but Rubio is taking it in stride. “I think this [duration] is really significant, in the sense that it teaches us that the human body can endure, it can adapt and—as we prepare to push back to the moon and then from there, onward onto hopefully Mars and further on into the solar system—I think it’s really important that we learn just how the human body learns to adapt, and how we can optimize that process so that we can improve our performance as we explore further and further out from Earth,” he said in a recent interview with ABC’s Good Morning America.

At 11 AM Tuesday, NASA broadcasted a pre-recorded “space-to-ground” chat between Rubio and Vande Hei, during which Rubio acknowledged his family. “They’ve been a key component, as much as I appreciate the team and how critical the entire human space flight team has been to this, really my family has been the cornerstone that’s inspired me to keep somewhat of a good attitude as I’ve been up here,” he adds. “Having [family] made it so much easier to be up here, and I’m incredibly grateful for that.”

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Space tourism is already becoming so commonplace that Virgin Galactic’s second private astronaut flight on September 8 went off without much fanfare. And although a brief press announcement only announced the names of its three-man passenger list after the trip, the recap didn’t mention Galactic 03’s historic “first” cargo—fossilized bones from two of humanity’s closest ancestors.

According to Tim Nash’s Virgin Galactic biography, the “entrepreneur, adventurer, conservationist and member of the Hubbard Council of The National Geographic Society,” carried with him the clavicle of a nearly 2-million-year-old Australopithecus sediba, as well as a roughly 250,000-year-old thumb bone from Homo naledi. Both hominid remains were previously discovered within the Cradle of Humankind UNESCO World Heritage Site outside Johannesburg, South Africa—sebedi is considered one of the potential candidates that presaged humanity’s Homo genus.

The initiative’s organizers, including researchers at the University of Witwatersrand, Johnnesburg, intended the gesture to represent “humankind’s appreciation of the contribution of all of humanity’s ancestors and our ancient relatives,” said Lee Berger, a National Geographic Explorer in Residence, Carnegie Fellow and Director of the Centre for the Exploration of the Deep Human Journey. “Without their invention of technologies such as fire and tools, and their contribution to the evolution of the contemporary human mind, such extraordinary endeavors as spaceflight would not have happened.”

[Related: Virgin Galactic’s second commercial flight sent three tourists to space’s edge.]

Berger’s son, Matthew, discovered the sebida clavicle in 2008 when he was 9 years old during an expedition alongside his father within the Cradle of Humankind heritage site. Matthew Berger traveled last week to Virgin Galactic’s Spaceport America in New Mexico to hand deliver the bones to Nash, a conservationist involved with human origins research. Caretakers stored both bone fragments within a carbon fiber container prior to their suborbital excursion.

“These fossils represent individuals who lived and died hundreds of thousands of years ago, yet were individuals who likely gazed up at the stars in wonder, much as we do,” Berger said in a September 8 statement via the University of Witwatersrand.

“The magnitude of being among the first civilians going into space, and carrying these precious fossils, has taken a while to sink in, during all of the preparations for the flight,” Nash said via the University of Witwatersrand statement, “But I am humbled and honored to represent South Africa and all of humankind, as I carry these precious representations of our collective ancestors, on this first journey of our ancient relatives into space.”

Nash, alongside Las Vegas real estate entrepreneur Ken Baxter and British engineer and racecar company founder Adrian Reynald, purchased their Virgin Galactic seats as far back as 2004 from company founder and multibillionaire Richard Branson. Tickets for the few minutes’ worth of suborbital weightlessness alongside views of the Earth’s curvature reportedly cost between $250,000 and $450,000.

“We sincerely hope it brings further awareness of the importance of our country and the African continent to understanding the journey of humankind that has led to this historic moment where commercial spaceflight is possible,” says Cradle of Humankind World Heritage Site CEO Matthew Sathekge said via University of Witwatersrand’s announcement.

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Our understanding of the solar system is a work in progress. Pluto’s demotion to a dwarf planet was just one of many revisions—in recent decades astronomers have cataloged new dwarfs, like far-off Eris, and spotted more moons around our gas giant neighbors. And now some researchers think there’s evidence for a new planet hiding beyond Neptune.

Two astronomers in Japan, Patryk Sofia Lykawka and Takashi Ito, claim there is a planet a little larger than Earth lurking in the Kuiper belt, the ring of icy debris where Pluto also resides, as they published last week in The Astronomical Journal. The pair hasn’t seen this world directly, but their computer models show that such a planet could explain the wonky observed orbits of other Kuiper belt objects.

The disturbance in this belt “predicts the existence” of an undiscovered planet with 1.5 to 3 times the mass of Earth, says lead author Lykawka, an astronomer at Japan’s Kindai University. “The solar system would officially have nine planets again.”

[Related: There might be an ice giant planet hiding in our solar system]

The Kuiper belt is somewhat similar to the asteroid belt: It contains small bits of rock and ice, all leftovers from the violent process of making planets. A few objects there have strange orbits, where their paths around the sun are extremely tilted or elongated (more egg-shaped than circular like Earth’s orbit). These weird orbits suggest that something massive must be pushing them around, tugged by  its gravity—something as big as an  undiscovered planet.

“It may be that this planet will be uncovered even in the next few years, if it exists on a relatively nearby orbit,” says Yale astronomer Malena Rice, who wasn’t involved in the new work.

Lykawka and Ito’s simulations show that a planet could explain the oddities in the Kuiper belt. The world, which they referred to as the Kuiper Belt Planet (KBP), would be located about 6 to 12 times further from the sun than even distant Neptune. The KBP’s orbit would also have to be tilted from the plane of the solar system by about 30 degrees, which is pretty weird. Dwarf planet Pluto sticks out because it’s off-kilter compared to the eight major planets—and its orbit is only tilted by about 17 degrees.

This bizarre and distant Earth-like planet, though, isn’t the first hidden world to be proposed. In 2016, astronomers from Caltech claimed to have evidence for a super-Earth, referred to as Planet 9 or Planet X, even farther out in the solar system. Those researchers also proposed Planet 9 as a way to explain the quirks of the Kuiper Belt; it caused quite a stir among scientists, who debated for years whether those idiosyncrasies were real or just the result of flawed observations.

Lykawka claims that the KBP hypothesis is superior to Planet 9 because it relies on other observations that haven’t caused as much dispute. “We demonstrated that a hypothetical Earth-like planet located in the far outer solar system could explain several properties of the distant Kuiper Belt and be compatible with observations simultaneously,” he says. “The Planet 9 model has yet to demonstrate that.” 

Yet other researchers don’t think the KBP is necessary. Konstantin Batygin, an astronomer at Caltech who was part of the initial Planet 9 research, agrees that there are oddities in the Kuiper belt that have to be explained by some sort of additional object beyond Neptune. “However, all of this has been understood for quite some time within the framework of the Planet 9 model,” he says, questioning the need for this new work, whose predictions for a hidden planet overlap substantially with the existing Planet 9 hypothesis. 

[Related: What will we name the solar system’s next planet?]

Batygin’s model suggests Planet 9 is somewhat bigger and farther: about five to six times the mass of Earth at 500 astronomical units (AU) away from the sun. Meanwhile, the KBP would be between 200 and 500 AU from the sun. (These are extreme distances—1 AU is equal to the gap between Earth and the sun.) Planet 9 would have an odd tilt to its orbit, to, of 20 degrees.

But we won’t know for sure if there’s a hidden planet, whether it looks like Planet 9 or the KBP, until astronomers actually pinpoint it in the night sky. Astronomers have been looking for Planet 9 for years, and that hunt includes some regions where the newly-proposed planet could be. “Those searches are still ongoing,” Rice says. “It’s incredible just how much parameter space remains to be searched in the outer solar system where hidden planets could be lurking.”

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If all goes according to plan, a tennis ball-sized robot modeled after a children’s toy will soon briefly explore the moon’s surface as part of Japan’s first soft lunar landing. As recently highlighted by Space.com, the Japanese space agency, JAXA, is currently overseeing its Smart Lander for Investigating Moon (SLIM) probe mission, which launched on September 6 alongside the country’s XRISM X-ray satellite payload. Unlike more powerful launches, it will take less than 9-foot-wide SLIM between three and four months to reach lunar orbit, after which it will survey the roughly 1000-foot-wide Shioli Crater landing site from afar for about another month.

Afterwards, however, the lander will descend towards the moon, and deploy the Lunar Excursion Vehicle 2 (LEV-2) once it reaches around six-feet above the surface. The probe’s sphere-shaped casing will then divide into two halves on either side of a small camera system. From there, LEV-2 will begin hobbling atop the SLIM landing site and surrounding area for around two hours, until its battery reserve is depleted.

[Related: India’s successful moon landing makes lunar history.]

Per JAXA’s description, LEV-2 was developed by its Space Exploration Innovation Hub Center associate senior researcher Hirano Daichi. Daichi collaborated with a team from Doshisha University as well as the toy manufacturer TOMY to create the tiny space explorer. Meanwhile, Sony provided the two cameras that will survey the moon. According to Daichi, the team turned to children’s toys for their “robust and safe design… which reduced the number of components used in the vehicle as much as possible and increased its reliability.”

“This robot was developed successfully within the limited size and mass using the downsizing and weight reduction technologies and the shape changing mechanism developed for toys by TOMY,” continued Daichi.

If successful, JAXA engineers hope the soft lunar landing method can be adapted to larger craft in the future, including those piloted by human astronauts. “By creating the SLIM lander humans will make a qualitative shift towards being able to land where we want and not just where it is easy to land, as had been the case before,” reads JAXA’s project description. “By achieving this, it will become possible to land on planets even more resource scarce than the moon.”

Beyond just this project, it’s been an active time for lunar exploration. In August, India completed the first successful lunar landing at the moon’s south pole via its Chandrayaan-3 probe. Last year, NASA’s Artemis-1 rocket also kickstarted the space agency’s long standing goal towards establishing a permanent moon base.

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UFOs were, for decades, the stuff of science fiction and conspiracy theory circles. But the highest levels of the US government have started seriously considering these phenomena—redubbing them Unidentified Anomalous Phenomena, or UAPs. There have been hearings on Capitol Hill, Pentagon reports, and a NASA working group, all looking into more than 100 currently unexplained UAP sightings, often made by military pilots who caught something unfathomable on their sensors. And plenty of civilians see things they don’t know how to explain, either. 

Even if UAPs have gone mainstream, the vast majority of human sightings turn out to be perfectly explicable, though occasionally rare, phenomena. And Jonathan McDowell, an astrophysicist at the Center for Astrophysics | Harvard & Smithsonian, hears about them all. 

“I get a lot of social media questions and emails, and occasionally cold calls from random people who have seen something weird in the sky,” McDowell says. Around 90 percent of the conversations, he says, go something like this: ‘Is this space debris, Jonathan?’ No, it’s just a meteor, because it blew up in only two seconds. Or: ‘Is this a UFO?’ No, it’s a Falcon 9 [rocket] launch. ‘Is this aliens?’ Well, that depends on where you think Elon comes from.”

But it’s rarely ignorance or credulity that leads people to mistake a rocket launch or an aircraft for a UAP. Instead, it’s just how human perception works.

“Our ability to estimate how far away something is sucks when it’s not in a context where we have the usual clues,” McDowell says. A close-by insect moving in a peculiar way might be confused for something much farther. Or a shining light might appear close—when it’s actually Venus, 35 million miles or so away. 

[Related: UFO research is stigmatized. NASA wants to change that.]

Even professionals can be fooled. Every once in a while, a satellite or spacecraft gets temporarily mistaken as a new asteroid. “If you have a spacecraft in a very high orbit around the Earth, the rate at which it’s moving across the sky is actually similar to an asteroid moving in orbit around the sun,” McDowell says. “There have been multiple cases where an object has been picked up by the asteroid surveys, given a temporary asteroid designation, and then it’s maneuvered. And we go, ‘Oh, that’s probably not an asteroid.’”

When it comes to the general public spotting what they think are UAPS, McDowell finds they usually turn out to be phenomena in three main categories: Rocket launches, spacecraft, and celestial objects. 

Rocket launches

If you’ve ever watched a rocket launch, in person or through a video, you can see a contrail as the craft shoots from the launchpad to the heavens. But once a rocket reaches space, its exhaust can lose that familiar linear shape, creating seemingly otherworldly sights under the right conditions.

The first weird thing rockets can create occurs about two minutes after launch, when they finally get above most of Earth’s atmosphere. No longer contained by thick air, the exhaust plume might spread out over hundreds of miles, according to McDowell, producing some bizarre forms that almost look oceanic. “Those are often described as jellyfish,” he says. “People are much less able to sort of recognize those as being rocket plumes and those often get reported as UFOs.”

Another type of rocket launch weirdness happens when rockets shut down and restart in space. This might be to change an orbit, or when a rocket vents its leftover propellant after delivering its payload. 

“You’ve got this big cloud of gas that then gets ejected from the rocket and forms ice crystals that reflect the sunlight,” McDowell says, ”so you get these big kind of comet-like clouds” moving through the sky. Even professional astronomers have been tricked by rocket fuel dumps, who reported them to the International Astronomical Union as new comet sightings. 

But the most striking rocket trail phenomenon are the striking, spiraling geometric patterns in the sky, such as those that appeared over Norway in 2009. At first glance, it is utterly unnatural. You might think it’s “a Stargate wormhole opening up in space and the aliens are invading,” McDowell says. But as weird as they look, the spirals are no portals. Instead, it’s the result of a spinning or tumbling rocket, which releases contrails “like a garden sprinkler.” In the case of the Norwegian spiral, it was actually a Russian military rocket maneuvering above Earth’s atmosphere. 

If you want to hunt down a bizarre rocket-exhaust plume for yourself, it’s important to realize the strange sights hinge on the relative position of the exhaust, the sun, and the observer: You’re most likely to catch one around dawn or dusk, when it’s dark for you on the ground, but the high-altitude rocket exhaust can catch the sun rays.

Spacecraft and satellites

There’s another category of artificial space objects that we commonly mistake for UAPs: Starlink satellite trains, which, in McDowell’s experience, “really freak people out.” 

SpaceX began launching its Starlink satellites in 2019, lofting between 22 and 60 of them at a time to provide broadband internet. As of September 2023, there are more than 4,700 Starlink satellites in orbit, according to McDowell’s personal satellite tracking website. It takes a couple of weeks after launch for Starlink satellites to fully separate from each other and move into their operational orbits at around 340 miles altitude. In their early days of flight, they can catch the sun and produce a bizarre geometric pattern in the sky—a long, bright straight line. 

“They march across the sky in this line, like little kids in the crocodile coming home from school,” McDowell says (using the British expression for pairs of kids in a line). “They’re close enough together that you can’t see them as separate dots. Even if you see them separately, to have them marching in lockstep across the sky as 20 different objects, that definitely looks like an alien invasion to your gut.”

To catch Starlink or other satellites as they fly overhead, McDowell recommends using the website heavens-above.com. “It tells you what time the satellite is going to go over, and if you click on the time, it gives you a nice star chart showing the path of that satellite across the sky, as seen from your location,” he says. The website doesn’t show Starlink satellites by default, because they’re so  numerous but you can click a link to see the Starlink constellation.

[Related: How scientists decide if they’ve actually found signals of alien life]

The reentry of satellites, spacecraft, or space debris can also look pretty weird, too. It might not be easy to tell what’s happening, though. “That’s where it gets tricky because if you see bright stuff overhead in the sky breaking up, that can be one of two things,” McDowell says. “It can be a natural meteor, or it can be a reentering piece of space debris.”

They key distinction, he says, is that meteors shoot across the sky fairly quickly, then vanish. A deorbiting satellite or other debris will have multiple pieces that cross the sky as it breaks up over time. 

There is a particular type of reentry that is sometimes mistaken for UAPs or natural meteors—the return of a spacecraft like the SpaceX Crew Dragon. “That looks more like a fireball, like a natural meteor, except that it lasts much longer,” McDowell says. “And if it’s breaking up, that’s really bad news.”

Celestial objects 

The last type of thing McDowell commonly hears about being mistaken for UAPs are natural objects that are very, very far away—Venus, for instance. He estimates, before dash cams and cell phones started picking up meteors, space debris and the like, the planet caused about half of all UFO reports. “Venus is the classic UFO.”

When very faint, high clouds move at night, this foreground motion can trick human perception. The result is the sense that a bright light—in this case, the planet—is traveling across the sky, when in fact it’s only the clouds. 

Comets also sometimes trigger UAP questions, McDowell says. The Comet Nishimura, which makes its closest approach to Earth on September 12, could turn some heads, if it becomes bright enough to be visible to the naked eye. 

“People aren’t used to seeing comets, so if they haven’t heard in the news there’s a bright comet around, they might think that’s a UFO,” he says. 

As quick as people are to label many different sights in the sky as UAPs, McDowell notes there’s one common object in the night sky he rarely hears about: The International Space Station.

“I think it’s just that the number of times the ISS is passing over you is comparatively rare, maybe,” he says. “People don’t seem to worry about that as much for some reason.”

If you would like to catch the ISS or China’s Tiangong space station as they zoom overhead, heavens-above.com can also help you plot their course over your location so you can look up at the right time, according to McDowell. For the planets or other celestial objects, he recommends the interactive sky charts at skyandtelescope.org. 

“You can put in your position and the time of the night that it is and you get a map of the sky tuned for your experience,” he says. “You can see where the bright planets are relative to constellations.” 

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Just in time for spooky season, astronomers have detected a dark and hungry space monster. The newly spotted black hole named Swift J0230 is gradually eating huge chunks of a star that is very much like our own sun. Every time this star passes close to Swift J0230, it loses the equivalent mass of three Earths. The findings are described in a study published September 7 in the journal Nature Astronomy.

[Related: Astronomers used dead stars to detect a new form of ripple in space-time.]

A bright X-ray flash that seemed to come from the center of a nearby galaxy called 2MASX J02301709+2836050 first alerted a team of astronomers from the University of Leicester. This galaxy is about 500 million light-years away from the Milky Way and the black hole Swift J0230 was officially spotted via a new tool developed by the scientists at NASA’s Neil Gehrels Swift Observatory. 

The team scheduled more observations of this black hole and found that instead of decaying away as they expected, it would shine brightly for 7 to 10 days before abruptly switching off and repeating this process about every 25 days.

“Given that we found Swift J0230 within a few months of enabling our new transient-hunting tool, we expect that there are a lot more objects like this out there, waiting to be uncovered,” study co-author and University of Leicester astrophysicist Kim Page said in a statement. 

According to the team, similar behavior has been observed in quasi-periodic eruptions and periodic nuclear transients. This is where a star has its material ripped away by a black hole as it is orbiting close by. However, black holes can differ in how often they erupt and whether the eruption is predominantly in X-rays or optical light. The regularity of Swift J0230’s emissions fell somewhere between these two types of outbursts, suggesting that it could form the ‘missing link’ between them.

“This is the first time we’ve seen a star like our sun being repeatedly shredded and consumed by a low mass black hole,” study co-author and University of Leicester astronomer Phil Evans said in a statement. “So-called ‘repeated, partial tidal disruption’ events are themselves quite a new discovery and seem to fall into two types: those that outburst every few hours, and those that outburst every year or so. This new system falls right into the gap between these, and when you run the numbers, you find the types of objects involved fall nicely into place too.”

For the study, the team used models proposed for these two classes of events as a guide. They concluded that Swift J0230’s outbursts represent that a sun-sized star is in an elliptical orbit around a low-mass black hole smack in the center of its galaxy. As this star’s orbit takes it closer to the intense gravitational pull of the black hole, the material equivalent to the mass of three Earths is sucked from the star’s atmosphere and heated up as it plummets into the black hole. The intense heat is about 3.6 million degrees Fahrenheit and releases the surge of X-rays that the Swift satellite first detected. 

[Related: Black hole collisions could possibly send waves cresting through space-time.]

The team estimates that the black hole is about 10,000 to 100,000 times the mass of our sun—shockingly  small for the supermassive black holes that are usually found at the center of galaxies. By comparison, the black hole at the center of our own galaxy is believed to be about 4 million solar masses, while most are in the region of 100 million solar masses.

This is the first discovery for the new transient detector on the Swift satellite, which was developed by the University of Leicester team and running on their computers. 

“This type of object was essentially undetectable until we built this new facility, and soon after it found this completely new, never-before-seen event. Swift is nearly 20 years old and it’s suddenly finding brand new events that we never knew existed,” said Evans. “I think it shows that every single time you find a new way of looking at space, you learn something new and find there’s something out there you didn’t know about before.”

The team was supported by the UK Space Agency and the UK Science and technology Facilities Council (STFC).

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Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) radio telescope have detected the magnetic field of a galaxy that is so far away from Earth, that its light has taken more than 11 billion years to get here. With the telescope, we are seeing this galaxy just as it was when our universe was only 2.5 billion years old.

[Related: Our universe mastered the art of making galaxies while it was still young.]

The findings are detailed in a study published September 6 in the journal Nature. Finally seeing this cosmic artifact could give astronomers some vital clues to how the magnetic fields of galaxies like the Milky Way came to be. Magnetic fields are present in many of the universe’s astronomical bodies from stars to planets and up to galaxies. 

“Many people might not be aware that our entire galaxy and other galaxies are laced with magnetic fields, spanning tens of thousands of light-years,” study co-author and University of Hertfordshire astrophysicist James Geach said in a statement.

It is not yet fully clear both how early in our universe’s lifetime and how quickly the magnetic fields in galaxies form. To date, astronomers have only mapped magnetic fields in galaxies close to us.

“We actually know very little about how these fields form, despite their being quite fundamental to how galaxies evolve,” study co-author and Stanford University extragalactic astronomer Enrique Lopez Rodriguez said in a statement. 

In this new study, the team used data from ALMA and the European Southern Observatory (ESO) and discovered a fully formed magnetic field in a distant galaxy. It’s similar in structure to what is observed in nearby galaxies, and while the magnetic field is about 1,000 times weaker than our planet’s magnetic field, it extends over more than 16,000 light-years.

Observing a fully developed magnetic field this early in the history of the universe is an indication that magnetic fields spanning entire galaxies can form pretty quickly, even while younger galaxies are still growing.  

According to the team, intense star formation in the universe’s early days may have played a role in accelerating the development of the magnetic fields and that the fields can influence how later generations of stars will eventually form. 

[Related: Secrets of the early universe are hidden in this chill galaxy cluster.]

These new findings show off the inner workings of galaxies, according to study co-author and ESO astronomer Rob Ivison. “The magnetic fields are linked to the material that is forming new stars,” Ivison said in a statement. 

To detect this light, the team searched for light emitted by dust grains in a distant galaxy named 9io9. When a magnetic field is present, galaxies are full of dust trains that tend to align and the light that they emit becomes polarized. When this happens, the light waves oscillate along a preferred direction instead of randomly. When ALMA detected and mapped the more polarized signal coming from galaxy 9io9, it confirmed the presence of a magnetic field in a very distant galaxy for potentially the first time. 

“No other telescope could have achieved this,” said Geach. 

The team hopes that with this new discovery and future observations of distant magnetic fields, astronomers will get closer to how fundamental components of galaxies form. 

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Nuclear fuel cells the size of poppy seeds could power NASA’s Artemis lunar base once it begins operations around 2030. Designed by researchers at Bangor University’s Nuclear Futures Institute in the UK, the miniscule power source—dubbed “Trisofuel”—is intended to run on a micro nuclear generator roughly the size of a small car created by Rolls Royce. According to a report in the BBC, engineers intend to begin fully testing their new fuel within the next few months. If successful, Trisofuel’s uses could even extend far beyond the moon’s surface.

Momentum is quickly building towards establishing a permanent human presence on the moon, likely near its south pole where scientists hope to find water-based ice to help support habitation. NASA’s ongoing Artemis project is making progress towards its proposed end-of-decade base construction, most recently with its first successful mission in November 2022. Last month, India made history as the fourth nation to land a probe on the moon via its Chandrayaan-3 spacecraft, as well as the first to do so at the lunar south pole.

[Related: India’s successful moon landing makes lunar history.]

Given its size and relative power, a resource like Trisofuel could be vital to lunar bases’ success. With its portability, however, the new nuclear fuel cell could easily be adapted to a range of other scenarios, both here on Earth and beyond.  Phylis Makurunje, a researcher involved Trisofuel testing, explained to the BBC that the tiny fuel pellets could be used to power rockets that one day take humans to Mars. “It is very powerful—it gives very high thrust, the push it gives to the rocket. This is very important because it enables rockets to reach the farthest planets,” Makurunje explained.

Trisofuel may be so strong, in fact, that it could nearly halve the time it takes to reach the Red Planet—from an estimated nine months down to between four-to-six months. “Nuclear power is the only way we currently have to provide the power for that length of space travel,” Bangor University professor Simon Middleburgh said in a release. “The fuel must be extremely robust and survive the forces of launch and then be dependable for many years.”

At a much more localized level, researchers believe that micro generators running Trisofuel could also be deployed to disaster zones with compromised electrical grids.

Having a reliable, powerful fuel source is one thing—having structures to house such systems is another hurdle altogether. Of course, researchers are currently hard at work optimizing construction options for proposed lunar base designs. Potential building materials could even be drawn from the moon itself, using lunar regolith to reinforce 3D-printed bricks to compose base structures.

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Update (September 5, 2023): India successfully launched its Aditya-L1 solar observatory on September 2 at 2:20 am EST. It is expected to arrive at its first destination between the Earth and the sun in January 2024.

On August 23, the Indian Space Research Organization (ISRO) pulled off the Chandrayaan-3 mission, depositing the Vikram lander and Pragyan rover near the lunar South Pole. India is now the fourth nation to land on the moon—following Russia, the US and China— and the first to land near the lunar South Pole, where the rover has already detected sulfur and oxygen in the moon’s soil. Fresh off of this success, ISRO already has another mission underway, and its next target is something much bigger—the sun.

The ISRO’s Aditya-L1 spacecraft, armed with an array of sensors for studying solar physics, is scheduled to launch around 2 a.m. Eastern on September 2, atop a PSLV-C57 rocket from the Satish Dhawan Space Center in Sriharikota, in southeast India.

Aditya-L1 will begin a four-month journey to a special point in space. About 932,000 miles away is the sun-Earth L1 Lagrangian, an area where the gravity of Earth and the sun cancel out. By entering into an orbit around L1, the spacecraft can maintain a constant position relative to Earth as it orbits around the sun. It shares this maneuver with the NASA-ESA Solar and Heliospheric Observatory, or SOHO, which has been in the sun-observation business since 1996. If it reaches the L1 orbit, Aditya-L1 will join SOHO, NASA’s Parker Solar Probe, ESA’s Solar orbiter, and a handful of other spacecraft dedicated to studying the closest star to Earth. 

“This mission has instrumentation that captures a little bit of everything that all of these missions have already done, but that doesn’t mean we’re going to replicate science,” says Maria Weber, a solar astrophysicist at Delta State University in Mississippi, who also runs the state’s only planetarium at that campus. ”We’re getting more information and more data now at another time, a new time in the solar cycle, that previous missions haven’t been able to capture for us.” The sun undergoes 11-year patterns of waxing and waning magnetic activity, and the current solar cycle is expected to peak in 2025, corresponding with more sunspots and solar eruptions.

Aditya-L1 will carry seven scientific payloads, including four remote sensing instruments: a coronagraph, which creates an artificial eclipse for better study of the sun’s corona, an ultraviolet telescope, and high and low X-ray spectrographs, which can help study the temperature variations in parts of the sun. 

[Related: Would a massive shade between Earth and the sun help slow climate change?]

“One thing I’m excited about is the high-energy component,” says Rutgers University radio solar physicist Dale Gary. Aditya-L1 will be able to study high-energy x-rays associated with solar flare and other activity in ways that SOHO cannot. And L1 is a good position for that sort of study, he says, since there is a more stable background of radiation against which to measure solar X-rays. Past measurements made in Earth orbit had to contend with Van Allen radiation belts. 

Aditya-L1’s ultraviolet telescope will also be unique, Gary says. It measures ultraviolet light, which has shorter wavelengths than visible light; the shortest or extreme UV light, near the X-ray spectrum, has already been measured by SOHO, but Aditya will capture the longer UV wavelengths.

That could allow Aditya-L1 to study parts of the sun’s atmosphere that have been somewhat neglected, Gary says, such as the transition region between the chromosphere, an area about 250 miles about the sun’s surface, and the corona, the outermost layer of the sun that begins around 1,300 miles above the solar surface and extends, tenuously, out through the solar system. 

Although ground-based telescopes can take some measurements similar to Aditya’s, the spacecraft is also kitted out with “in situ” instruments, which measure features of the sun that can only be observed while in space. “It’s taking measurements of magnetic fields right where it’s sitting, and it’s taking measurements of the solar wind particles,” Weber says. 

Like all solar physics missions, Aditya-L1 will inevitably serve two overall purposes. The first is to better understand how the sun—and other stars— work. The second is to help predict that behavior, particularly solar flares and coronal mass ejections. Those eruptions of charged particles and magnetic fields can impact Earth’s atmosphere and pose risks to satellites and astronauts. In March 2022, a geomagnetic storm caused by solar radiation caused Earth’s atmosphere to swell, knocking 40 newly launched SpaceX Starling satellites to fall out of orbit. 

“We live with this star and so, ultimately, we want to be able to predict its behavior,” Weber says. “We’re getting better and better at that all the time, but the only way we can predict its behavior, is to learn as much as we can even more about it.”

[Related: Why is space cold if the sun is hot?]

Aside from Aditya-L1’s scientific mission, its success will mark another feather in the cap of ISRO, another step in that space agency’s hard work to make India a space power, according to Wendy Whitman Cobb a space policy expert and instructor at the US Air Force School of Advanced Air and Space Studies (who was commenting on her own behalf, not for the US government). 

“India has had some pretty expansive plans for the past two decades,” she says. “A lot of countries say they’re going to do something, but I think India is that rare example of a country who’s actually doing it.”

Of course, space is hard. ISRO’s first lunar landing attempt with Chandrayaan-2, in 2019, was a failure, and there’s no guarantee Aditya-L1 will make it to L1. “It’s a technical achievement to go into the correct orbit when you get there,” Gary says. “There’s a learning curve. It would be very exciting if they accomplish their goals and get everything turned on correctly.”

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The James Webb Space Telescope (JWST) has taken some new images of a star that exploded during the Reagan Administration. The space telescope’s NIRCam (Near-Infrared Camera) helped capture the images of a world renowned supernova called Supernova 1987A (SN 1987A) in September 2022. The jaw-dropping new images were officially made public on August 31. 

[Related: An amateur astronomer spotted a new supernova remarkably close to Earth.]

Supernova 1987A is roughly 168,000 light-years away from Earth and located in the Large Magellanic Cloud–a satellite dwarf galaxy of the Milky Way. The supernova is the remnants of a blue supergiant star called Sanduleak–69 202. It was believed to hold a mass about 20 times that of the sun before the explosion was detected in February 1987. It is also the closest observed supernova since 1604, when Kepler’s Supernova illuminated the Milky Way. Supernova 1987A has been the target of observations at wavelengths ranging from gamma rays to radio waves for nearly 40 years. 

The latest image shows a central structure of inner ejecta similar to a keyhole. Clumpy gas and dust pack up the center that is ejected by the supernova explosion. According to NASA, the dust is so dense that even near-infrared light that Webb can detect can’t penetrate it, shaping the dark “hole” in the keyhole. 

Surrounding the inner keyhole is a bright equatorial ring which forms a band around the “waist” of the supernova which connects the two faint arms of hourglass-shaped outer rings. The equatorial ring is formed from material ejected tens of thousands of years before the supernova even exploded.. Bright hot spots in the ring appeared as the supernova’s shock wave hit it, and now exist externally to the ring, with diffuse emission surrounding it. These are where the supernova shocks hit more exterior material.

The Hubble and Spitzer Space Telescopes and the Chandra X-ray Observatory have also observed Supernova 1987A, but JWST’s sensitivity and spatial resolution abilities showed a new feature in this supernova remnant–small crescent-like structures. The crescents are believed to be part of the outer layers of gas that shot out from the supernova explosion. They are very bright, which may be an indication of an optical phenomenon called limb brightening. This results from being able to observe the expanding material in three dimensions. “The viewing angle makes it appear that there is more material in these two crescents than there actually may be,” NASA wrote in a press release.

Before JWST, the now-retired Spitzer telescope observed this supernova in infrared throughout its entire 16 year lifespan, providing astronomers with key data about how Supernova 1987A’s emissions evolved over time. However, Spitzer couldn’t observe the supernova with the same level of clarity and detail as JWST.  

[Related: JWST captures an unprecedented ‘prequel’ to a galaxy.]

There are still several mysteries surrounding this supernova, namely some unanswered questions about the neutron star that should have formed in the aftermath of the supernova explosion. There is some indirect evidence for the neutron star in the form of X-ray emission that was detected by NASA’s Chandra and NuSTAR X-ray observatories. Additionally, some observations taken by the Atacama Large Millimeter/submillimeter Array indicate the neutron star may be hidden within one of the dust clumps at the heart of the remnant.

JWST will continue to observe the supernova over time, using the NIRSpec (Near-Infrared Spectrograph) and MIRI (Mid-Infrared Instrument) instruments that give astronomers the ability to capture new, high-fidelity infrared data over time. 

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By year’s end, NASA will begin testing a fridge-sized laser communications upgrade aboard the International Space Station. It’s a major relay system demonstration for the ISS, and one which could chart a path forward for how humans communicate not just in low-orbit, but on the lunar surface and beyond. 

Although radio has long served as both piloted and unpiloted missions’ primary communications method, as Space.com notes, laser communication arrays boast a number of benefits. From a purely logistical standpoint, the equipment is both cheaper and lighter-weight than radio devices. Meanwhile, lasers’ shorter wavelengths ensure far more information can be transferred at one time compared to radio waves.

Once launched aboard a forthcoming SpaceX commercial resupply services mission, NASA’s Integrated LCRD Low Earth Orbit User Modem and Amplifier Terminal (ILLUMA-T) will work alongside the agency’s Laser Communications Relay Demonstration (LCRD) launched in December 2021. ILLUMA-T will use infrared light to send and receive laser communications at a higher data rate than previously available. Once installed, these transmissions’ higher rates will allow for more videos and images to transmit back to Earth, all at around 1.2 gigabits-per-second—comparable to a solid internet connection here on Earth.

[Related: NASA is testing space lasers to shoot data back to Earth.]

“Laser communications offer missions more flexibility and an expedited way to get data back from space,” said Badri Younes, former deputy associate administrator for NASA’s Space Communications and Navigation (SCaN) program. “We are integrating this technology on demonstrations near Earth, at the Moon, and in deep space.”

After installation, ILLUMA-T will first beam data to-and-from the LCRD satellite hovering 22,000 miles above Earth in geosynchronous orbit. Meanwhile, the LCRD will transmit data back to Earth at two stations in California and Hawaii—spots chosen for their comparatively low cloud cover, which often impedes laser transmissions.

“ILLUMA-T is not the first mission to test laser communications in space but brings NASA closer to operational infusion of the technology,” NASA wrote in a recent statement,  In 2022, a small CubeSat in low Earth orbit began testing laser communications as part of the TeraByte InfraRed Delivery System. Before that, the Lunar Laser Communications Demonstration also transferred data to-and-from lunar orbit during 2014’s Lunar Atmosphere and Dust Environment Explorer mission. Still, NASA explains that all of these tests combined will further help advance aerospace communications between Earth, the moon, Mars, and beyond.

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Summer skygazing season in the Northern Hemisphere is quickly drawing to a close.  September 1 marks the beginning of meteorological autumn, and we are racing towards the Autumnal Equinox. While the temperatures may finally start to get a little bit cooler, the night sky is staying pretty hot with a very bright Mercury beginning in mid-September, a meteor shower, and the last supermoon of the year. Here are some events to look out for this month and if you happen to get any stellar sky photos, please tag us and include #PopSkyGazers.

[Related: Climate change is affecting fall foliage, but not in the way you think.]

September 1- Aurigid Meteor Shower Predicted to Peak

The day after August’s Blue Moon, the Aurigid meteor shower is predicted to reach its peak. This meteor shower has been active since August 28 and will wrap up on September 5. From the eastern US, the shower will likely be visible around 11:30 PM each night when its radiant point rises above the eastern horizon. It is predicted to remain active until dawn breaks at around 5:51 AM. In the Sky estimates that viewers could see about five meteors an hour and that the bright moon will likely cause some viewing interference. 

September 12 – Nishimura Comet at Closest Approach

Anyone can buy a certificant to get a star named after them, but only the lucky can have comets named for them. That’s what happened earlier in August when Hideo Nishimura of Kakegawa, Japan was photographing the night sky and captured an image of Comet C/2023 P1 (Nishimura). The comet orbits the sun every 520 years and is expected to be at its closest approach to our planet this month, as long as it survives a cozy orbit around the sun even tighter than the planet Mercury’s loop. According to EarthSky, Comet Nishimura should become a binocular object during the first mornings of September if it survives its orbit. Observers with an unobstructed view to the east-northeastern horizon might get good binocular views of Comet C/2023 P1 (Nishimura) about 45 minutes before sunrise. It’s expected to pass at 78 million miles from Earth and does not pose any threat. 

[Related: ‘Oumuamua isn’t an alien probe, but it might be the freakiest comet we’ve ever seen.]

September 18 – Venus at its Greatest Brightness

In addition to the planet Mercury lighting up the sky most of this month, our solar system’s brightest planet will be at its most radiant around the middle of September. Venus will be shining brightly at a magnitude of -4.5 early in the morning in the eastern sky. It will continue to remain pretty bright for the rest of the month and reach its peak altitude until October 20.

September 23 – Autumnal Equinox 

Fall officially arrives in the Northern Hemisphere at 2:50 AM EDT on Saturday, September 23. The autumnal equinox occurs at the exact same moment around the world. It is the second equinox of the year, after March’s Spring equinox. During an equinox, the sun crosses an imaginary extension of Earth’s equator line called the celestial equator. The equinox happens precisely when the sun’s center passes through this imaginary line. In the Northern Hemisphere, the autumnal equinox happens when the sun crosses the equator from north to south. When the sun crosses from south to north, it marks the spring or vernal equinox, which is what happens in the Southern Hemisphere in September. 

The days will continue to get shorter than the nights, since the sun will rise later and set earlier. This continues up until the winter solstice in December, when the days begin to slowly grow longer again. 

[Related: We finally know why Venus is absolutely radiant.]

September 29 – Full Harvest Supermoon

September’s full moon, or the Harvest Moon, will reach its peak illumination at 5:58 AM EST. According to the Farmer’s Almanac, the full moon that happens nearest to the fall equinox always takes on the name Harvest Moon. The Harvest Moon also rises at roughly the same time, around sunset, for several consecutive evenings. This traditionally gives farmers several extra evenings of moonlight, helping them to finish harvesting before the frosts of fall are scheduled to arrive. This year’s Harvest Moon is also the last of four supermoons of 2023 and it will be 224,658 miles away from Earth. 

Additional names for September’s full moon include the Corn Moon or Mandaamini giizis in Anishinaabemowin (Ojibwe), the Gourd Moon or Wade Nuti in the Catawba Language of the Catawba Indian Nation, South Carolina, and the Falling Leaf Moon or Poneʔna-wueepukw Neepaʔuk in the Mahican Dialect of the Stockbridge-Munsee Band of Wisconsin.

The same skygazing rules that apply to pretty much all space-watching activities are key this month: Go to a dark spot away from the lights of a city or town and let the eyes adjust to the darkness for about a half an hour. 

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NORMALLY, creating a universe isn’t the job of the Large Hadron Collider (LHC). Most of the back-breaking science—singling out and tracking Higgs bosons, for example—from the world’s largest particle accelerator happens when it launches humble protons at nearly the speed of light.

But for around a month near the end of each year, LHC switches its ammunition from protons to bullets that are about 208 times heavier: lead ions.

When the LHC crashes those ions into each other, scientists can—if they have worked everything out properly—glimpse a fleeting droplet of a universe like the one that ceased to exist a few millionths of a second after the big bang.

This is the story of quark-gluon plasma. Take an atom, any atom. Peel away its whirling electron clouds to reveal its core, the atomic nucleus. Then, finely dice the nucleus into its base components, protons and neutrons.

When physicists first split an atomic nucleus in the early 20th century, this was as far as they got. Protons, neutrons, and electrons formed the entire universe’s mass—well, those, plus dashes of short-lived electrically charged particles like muons. But calculations, primitive particle accelerators, and cosmic rays striking Earth’s atmosphere began to reveal an additional menagerie of esoteric particles: kaons, pions, hyperons, and others that sound as if they’d give aliens psychic powers.

It seemed rather inelegant of the universe to present so many basic ingredients. Physicists soon figured out that some of those particles weren’t elementary at all, but combinations of even tinier particles, which they named with a word partly inspired by James Joyce’s Finnegans Wake: quarks.

Quarks come in six different “flavors,” but the vast majority of the observable universe consists of just two: up quarks and down quarks. A proton consists of two up quarks and one down quark; a neutron, two down and one up. (The other four, in ascending order of heaviness and elusiveness: strange quarks, charm quarks, beauty quarks, and the top quark.)

At this point, the list of ingredients ends. You can’t ordinarily chop a proton or neutron into quarks in our world; in most cases, quarks can’t exist on their own. But by the 1970s, physicists had come up with a workaround: heating things up. At a point that scientists call the Hagedorn temperature, those subatomic particles are reduced to a high-energy soup of quarks and the even tinier particles that glue them together: gluons. Scientists dubbed that soup quark-gluon plasma (QGP).

It’s a tantalizing recipe because, again, quarks and gluons can’t normally exist on their own, and reconstructing them from the larger particles they build is challenging. “If I give you water, it’s very difficult to tell the properties of [hydrogen and oxygen atoms],” says Bedangadas Mohanty, a physicist at India’s National Institute of Science Education and Research and at CERN. “Similarly, I can give you protons, neutrons, pions…but if you really want to study properties of quarks and gluons, you need them in a box, free.”

This isn’t a recipe you can test in a home oven. In units of the everyday world, the temperature in a hadronic system is about 3 trillion degrees Fahrenheit—100 thousand times hotter than the center of the sun. The best appliance for the job is a particle accelerator. 

But not just any particle accelerator will do. You need to boost your particles with sufficient energy. And when scientists set out to create QGP, LHC was no more than a dream of a distant future. Instead, CERN had an older collider only about a quarter of LHC’s circumference: the Super Proton Synchrotron (SPS).

As its name suggests, SPS was designed to crash protons into fixed targets. But by the end of the 1980s, scientists had decided to try swapping out the protons for heavy ions—lead nuclei—and see what they could manage. In experiment after experiment across the 1990s, CERN researchers thought they saw something happening to the nuclei. 

“Somewhat to our surprise, already at these relatively low energies, it looked like we were creating quark-gluon plasma,” says Marco van Leeuwen, a physicist at Dutch National Institute for Subatomic Physics and at CERN. In 2000, his team claimed they had “compelling evidence” of the achievement.

Across the Atlantic, CERN’s counterparts at Long Island’s Brookhaven National Laboratory had been trying their hands with equal parts optimism and uncertainty. The uncertainty faded around the turn of the millennium, when Brookhaven switched on the Relativistic Heavy Ion Collider (RHIC), a device designed specifically to create QGP.

“RHIC turned on, and we were deeply within quark-gluon plasma,” says James Dunlop, a physicist at Brookhaven National Laboratory.

So there are two major QGP factories in the world today: CERN and Brookhaven. With this pair of colliders, for the brief flickers for which the quantum matter exists in the world, physicists can watch the plasma materialize in what they call “little bangs.”

Going back and forth in time

The closer in time to the big bang that you travel, the less the universe resembles your familiar one. As of this writing, the James Webb Space Telescope has possibly observed galaxies from around 320 million years after the big bang. Go farther back, and you’ll reach a very literal Dark Ages—a time before the first stars, when there was little to illuminate the universe except the cosmic background.

In this shadowy age, astronomy steadily gives way to subatomic physics. Go even farther back, to just 380,000 years after the big bang, and electrons are just joining their nuclei to form atoms. Keep going back; the universe is ever smaller, denser, hotter. Seconds after the big bang, protons and neutrons haven’t joined together to form nuclei more complex than hydrogen. 

Go back even farther—around a millionth of a second after the big bang—and the universe is hot enough that quarks and gluons stay split apart. It’s a miniature version of this universe that physicists seek to create.

Physicists puzzle over that universe in office blocks like the exquisitely modernist one overlooking CERN’s visitors center. Look out this building’s window, and you might see the terminus of a Geneva tram line. Cornavin, the city’s main railway station, is only 20 minutes away.

CERN physicists Urs Wiedemann and Federico Antinori meet me in their office. Wiedemann is a theoretical physicist by background; Antinori is an experimentalist, presiding over heavy-ion collision runs. Studying QGP requires the talents of both.

“The existence of quark-gluon plasma we have established,” says Antinori. “What is most interesting is understanding what kind of animal it is.”

For instance, their colleagues who first created QGP expected to find a sort of gas. Instead, QGP behaves like a liquid. QGP, in fact, behaves like what’s called a perfect liquid, one with almost no viscosity. (Yes, the early universe may have been, very briefly, a sort of superheated ocean. Many creation myths might find a distant mirror inside a particle accelerator.)

Both Antinori and Wiedemann are especially interested in watching the liquid come into being, watching atomic nuclei rend themselves apart. Some scientists call the process a “phase transition,” as if creating QGP is like melting snow to create liquid water. But turning protons and neutrons into QGP is far more than melting ice; it’s creating a transition into a very different world with fundamentally different laws of physics. “The symmetries of the world we live in change,” Wiedemann says.

This transition happened in reverse in the very early universe as it cooled down past the Hagedorn temperature. The quarks and gluons clumped together, forming the protons and neutrons that, in turn, form the atoms we know and love today.

But physicists struggle to understand this process with mathematics. They come closer by examining QGP collisions in the lab.

QGP is also a laboratory for the strong nuclear force. One of the four fundamental forces of the universe—alongside gravity, electromagnetism, and the weak nuclear force that governs certain radioactive processes—the strong nuclear force is what holds particles together at the hearts of atoms. The gluons in QGP’s name are the strong nuclear force’s tools. Without them, charged particles would electromagnetically repel each other and atoms would rip themselves apart.

Yet while we know quite a lot about gravity and electromagnetism, the inner workings of the strong nuclear force remain a secret. Moreover, scientists want to learn more about the role the strong nuclear force plays.

“You can say, ‘I understand how an electron interacts with a photon,’” says Wiedemann, “but that doesn’t mean that you understand how a laser functions. That doesn’t mean that you know why this table doesn’t break down.”

Again, to understand such things, they’ve got to crash heavy ions together.

With the likes of SPS, scientists could look at droplets of QGP and confirm they existed. But if they wanted to actually peer inside and see their properties at work—to examine them—they’d need something more powerful.

“It was clear,” says Antinori, “that one had to go to higher energies than were available at the SPS.”

The universe-faking machine

Crossing from CERN’s campus into France, it’s impossible to tell that this green and pleasant vale—under the grace of the Jura Mountains—sits atop a 17-mile-long ring of superconducting magnets and steel. Scattered around that ring are different experiments and detectors. The search for QGP is headquartered in one such detector.

The road there passes through the glistening hamlet of Saint-Genis-Pouilly, where many of CERN’s staff live. On the pastoral outskirts sits a cluster of industrial cuboids and cooling towers.

Apart from a mural on the corrugated metal facade overlooking a parking lot, the complex doesn’t really advertise that this is where scientists look for QGP—that one of these warehouselike buildings is the outer cocoon of a large ion collider experiment called, well, A Large Ion Collider Experiment (ALICE).

CERN physicist Nima Zardoshti greets me beneath that mural: ALICE’s detector, the QGP-watcher, depicted in a pastel-colored mural. Zardoshti leads me inside, past a control room that wouldn’t look out of place in a moon-landing documentary, around a corner covered in sheet metal, and out to a precipice. A concrete shield caps it, several stories below. “This concrete is what stops radiation,” he explains.

Beneath it, occluded from sight, sits the genuine article, a machine the size of a small building that weighs nearly the same as the Eiffel Tower. The detector sits more than 180 feet beneath the ground, accessible by a mine lift. No one is allowed to go down there while the LHC is running, save for CERN’s fire department, which needs to move in quickly if any radioactive or hazardous materials combust.

The heavy ions that collide inside that machine don’t originate in this building. Several miles away sits the old SPS, transformed into LHC’s first steppingstone. SPS accelerates bunches of lead nuclei up to very near the speed of light. Once they’re ready, the shorter collider unloads them into the longer one.

But unlike SPS, LHC doesn’t do fixed-target experiments. Instead, ALICE creates a magnetic squeeze that goads lead beams, racing in opposite directions, into violently crashing head-on.

Lead ions make fine ingredients. A lead-208 ion has 82 protons and 126 neutrons, and both of those are “magic numbers” that help make the nuclei as spherical as nuclei can become. Spherical nuclei create better collisions. (Across the Atlantic, Brookhaven’s RHIC uses gold ions.)

ALICE’s detector isn’t a camera; QGP isn’t like a ball of light that you can “see.” When these lead ions collide at high energies, they erupt into a flash of QGP, which dissipates into a perfect storm of smaller particles. Instead of watching for light, the detector watches the particles as they cascade away. 

A proton-proton collision might produce a few dozen particles—maybe a hundred, if physicists are lucky. A heavy-ion collision produces several thousand.

When heavy ions collide, they create a flash of QGP and spiky jets of more “normal” particles: often combinations of heavy quarks, like charm and beauty quarks. The jets pierce through the QGP before they reach the detector. Physicists can reconstruct what the QGP looked like by examining those jets and how they changed as they passed through.

First those particles crash through silicon chips not unlike the pixels in your smartphone. Then the particles pass through a time projection chamber: a cylinder filled with gas. Still streaking at high energy, they shoot through the gas atoms like meteors through the upper atmosphere. They knock electrons free of their atoms, leaving brilliant trails that the chamber can pick up.

For fans of particle physics equipment, the time projection chamber makes ALICE special. “It’s super useful, but the downside of it, and why other experiments don’t use it, is it’s very slow,” says Zardoshti. “The process takes, I think, roughly something on the order of a millionth of a second.”

ALICE creates about 3.5 terabytes of data—around the equivalent of three full-length feature films—each second. Physicists process that data to reconstruct the QGP that produced the particles. Much of that data is processed right here, but much of it is also processed by a vast global network of computers.

From particle accelerators to neutron stars

Particle physics is a field that always has one foot extended decades into the future. While ALICE kicked into operation in 2010, physicists had already begun sketching it out in the early 1990s, years before scientists had even detected QGP at all. 

One of their current big questions is whether they can make QGP by smashing ions smaller than lead or gold. They’ve already succeeded with xenon; later this year, they want to try with an even scanter substance like oxygen. “We want to see: Where is the transition where we can make this material?” says Zardoshti. “Is oxygen already too light?” They expect the life-giving element to work. But in particle physics, there’s no knowing for certain until after the fact.

In the longer term, ALICE’s stewards have big plans. After 2025, the LHC will shut off for several years for maintenance and upgrades, which will boost the collider’s energy. Alongside those upgrades will come a wholesale renovation of ALICE’s detector, scheduled for installation as early as 2033. All of this is planned out precisely many years in advance.

CERN’s stewards are daring to draft a device for an even more distant future, a Future Circular Collider that would be more than three times the LHC’s size and wouldn’t be online till the 2050s. No one is sure yet if it will pan out; if it does, it will require securing an investment of more than 20 billion euros.

Higher energies, larger colliders, and more sensitive detectors all make for stronger tools in QGP-watchers’ arsenals. The particles they’re seeking are tiny and incredibly short-lived, and they need those tools to see more of them.

But while particle physicists have spent billions of euros and decades of effort bringing fragments of the very early universe back into reality, some astrophysicists think the universe might have been showing the same zeal.

Instead of a particle accelerator, the universe can avail itself of a far more powerful appliance: a neutron star. 

When an immense star, far larger than the mass of our sun, ends its life in a spectacular supernova, the shard of a core that remains begins to cave in. The core can’t be too large, or else it will collapse into a black hole. But if the mass is just right, the core will reach pressures and temperatures that might just tear atomic nuclei apart into quarks. It’s like the ALICE experiment at scale in a more natural setting—the unruly universe, where it all began.

Read more PopSci+ stories.

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The James Webb Space Telescope (JWST) has captured a stellar new image of the Whirlpool Galaxy (aka M51 or NGC 5194), a grand-design spiral galaxy about 27 million light-years away from Earth. According to the European Space Agency (ESA), grand-design spiral galaxies like this one have prominent, well-developed spiral arms, unlike other spiral galaxies that have more ragged or disrupted spiral arms. 

[Related: Herschel Space Telescope’s First Images Give Promising Glimpse of What’s to Come.]

M51 lies in the constellation Canes Venatici (or The Hunting Dogs) and is trapped in a bit of a tumultuous relationship with the dwarf galaxy NGC 5195. The interaction between these two galactic neighbors has been one of the more well studied galaxy pairs in the sky. M51’s gravitational influence on its smaller companion is believed to be partially responsible for the grand nature of its prominent and distinct spiral arms. 

This new galactic portrait uses data from JWST’s Near-InfraRed Camera (NIRCam) and Mid-InfraRed Instrument (MIRI). This new observation is one of a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers (FEAST). The FEAST observations were designed for astronomers and the public to learn more about stellar feedback and star formation environments outside of the Milky Way galaxy. 

Stellar feedback describes the outpouring of energy from stars into the environments which form them. It is a crucial process in determining the rates at which stars form, and is important to building accurate models of star formation. 

“Stellar feedback has a dramatic effect on the medium of the galaxy and creates a complex network of bright knots as well as cavernous black bubbles,” the ESA wrote in a statement. 

In the new image, the dark red regions trace the filamentary warm dust permeating the medium of the galaxy. These rosy regions show the reprocessed light from complex molecules forming on dust grains. The orange and yellow portions show areas of ionized gas created by recently formed star clusters.

Before JWST became operative in 2022, other observatories including those made at the Atacama Large Millimetre Array in the Chilean desert and the Hubble Telescope gave astronomers a glimpse of star formation. These observations occurred at either the onset, when the dense gas and dust clouds where stars will form, or after the stars have been destroyed with their energy their natal gas and dust clouds. JWST is opening up a new observational window to the earlier stages of star formation and stellar light. 

“Scientists are seeing star clusters emerging from their natal cloud in galaxies beyond our local group for the first time. They will also be able to measure how long it takes for these stars to pollute with newly formed metals and to clean out the gas (these time scales are different from galaxy to galaxy),” wrote the ESA.

[Related: Our universe mastered the art of making galaxies while it was still young.]

More observations and study of these processes is expected to lead to a better understanding of how the whole star formation cycle and metal enrichment process are regulated within galaxies. It also could help present a more clear time scale for when planets and brown dwarfs form because once gas and dust is removed from newly formed stars, there isn’t any material left to form planets.

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Outer space is a rough place for the human body. The effects of space travel on our health pose substantial challenges to our future in the cosmos. Beyond Earth, astronauts literally lose bone and muscle while being exposed to potentially cancer-causing radiation. As they plan to go on longer trips—like to the moon and Mars, such as in NASA’s Artemis program—biologists need to prepare to keep these explorers safe on these extended voyages. 

Part of that is understanding exactly how space changes our bodies, from the macroscopic scale of our organs all the way down to our microscopic cells. To that end, Swedish biologists used an experiment here on Earth to simulate what happens to a human’s immune system in microgravity, the “weightlessness” experienced by space travelers. In a new research paper, published last week in Science Advances, the study authors report significant genetic changes to these guardian cells. 

The immune system is a crucial system in the human body, protecting us from a barrage of bacteria and viruses that dwell on our lively planet. If an astronaut’s immune system is damaged by the conditions of outer space, they may not be able to fight off infections when they return to Earth, and viruses that were lingering dormant in their system might even come back with a vengeance. 

[Related: Most of us have viruses sleeping inside us, and spaceflight wakes them up]

To study this on Earth, volunteer test subjects lived in space-like conditions for 21 days, essentially floating on what are called “dry immersion” beds. Researchers analyzed the participants’ blood and found that the genes in their T cells, a type of germ-fighting white blood cell, had altered in ways that might make them less effective at protecting against pathogens.

“T cells significantly changed their gene expression—that is to say, which genes were active and which were not—after seven and 14 days of weightlessness,” says co-author Lisa Westerberg, an immunologist from Sweden’s Karolinska Institute. “T cells began to resemble more so-called naïve T cells, which have not yet encountered any intruders. This could mean that they become less effective at fighting tumor cells and infections.” 

But there’s some good news. After a return to usual gravity, some of the cells’ changes reverted back to normal, Westerberg and her colleagues observed. This suggests human bodies have the potential to re-adapt once they’re back on Earth—at least, based on this research, for 21-day trips. It’s still unclear how longer-term spaceflight, like the perilous possibly years-long journey to and from Mars, would affect astronauts, their genes, and their immune systems.

[Related: Space stations could wage war on hitchhiking bacteria with self-cleaning tech]

This isn’t the first time that scientists have noticed changes in DNA due to space travel. NASA’s famous “Twins Study”, in which astronaut Scott Kelly lived aboard the International Space Station while his twin brother Mark Kelly remained on Earth, revealed that a year in space does affect and sometimes damage genes. We also know that space can harm blood cells and bone marrow, destroying them to the point that astronauts could experience so-called “space anemia.” (Although new research shows there might be a way to combat that, using fat cells.)

The truly novel bit of this new research is how it ties cellular changes to the human body’s broader functions, allowing researchers to brainstorm fixes to the problem at a cellular level. Several clinical trials are underway for new drugs and therapies to treat similar cell-related issues on Earth, including certain cancers, allergies, and autoimmune disorders. “We therefore think this study can pave the way for new treatments that reverse these changes to the immune cells’ genetic program,” says Westerberg.

Prepping for Mars or beyond, then, has the potential to help both Earth-bound patients and spacefaring travelers, providing a better understanding of the human body no matter where it is in the universe.

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The US Department of Justice filed a lawsuit against SpaceX on Thursday for allegedly refusing to consider hiring asylum seekers and refugees. According to a DOJ statement, Elon Musk’s rocket and satellite company “routinely discouraged” applicants because of their citizenship status from at least September 2018 to May 2022, thus violating the Immigration and Nationality Act (INA).

The DOJ argues SpaceX, in multiple job postings and public statements, “wrongly claimed” that federal “export control law” regulations forced the company to only hire US citizens and green card holders. The allegedly willful misinterpretation of the law was repeatedly and publicly echoed by SpaceX CEO Elon Musk. In June 2020, for example, Musk posted to X (formerly Twitter) that “U.S. law requires at least a green card to be hired at SpaceX, as rockets are advanced weapons technology.”

But as the DOJ’s announcement notes, the jobs in question weren’t only advanced engineering and tech roles, but a “variety of other positions, including welders, cooks, crane operators, baristas, software engineers, marketing professionals, and more.” According to the DOJ, SpaceX falsely claimed to be legally prohibited from hiring refugees in a total of 14 job postings, public announcements, and other online recruiting communications.

According to the INA, employers cannot discriminate against hiring asylees or refugees unless a specific executive order, government contract, law, or other federal regulation prevents them. “In this instance no [such situation] required or permitted SpaceX to engage in the widespread discrimination,” argues DOJ representatives.

[Related: SpaceX’s Starship launch caused a ‘mini earthquake’ and left a giant mess.]

Musk, however, has already doubled down on his and fellow employees’ previous assertions via an August 24 post to X, claiming SpaceX was “told repeatedly” that hiring non-permanent US residents would violate international arms trafficking laws. “This is yet another case of weaponization of the DOJ for political purposes,” added Musk, who purchased the social media platform formerly known as Twitter in October 2022. Lawyers like Rebecca Bernhard, a partner at Dorsey & Whitney specializing in employment-related issues involving work visas and immigration challenges, doubt the validity of Musk’s defense.

“While it is lawful for an employer to refuse to provide employer-sponsorship to a potential employee (for example, by not sponsoring the individual for an H-1B), it is not lawful to require that the employee be a US citizen,” she explains via email. Bernhard argues that while, “There are other classes of immigrants who have work authorization in the US and do not need employer sponsorship… To require someone be a US citizen would discriminate against these individuals.”

One potential exception, however, are employers subject to the International Traffic in Arms Regulations (ITAR) or the Export Administration Regulations (EAR). Bernhard notes that, “it appears the DOJ is claiming SpaceX fraudulently relied on this exception.” 

“While I cannot comment on whether SpaceX is subject to ITAR or EAR, I can state that the DOJ takes the anti-discrimination provisions of the INA very seriously, aggressively enforces them, and interprets the ITAR and EAR exceptions very narrowly,” adds Bernhard.

The DOJ filing seeks fair consideration and back pay for those affected by the alleged discriminatory practices.

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When it comes to building a sustainable settlement on Mars, the technological and engineering challenges are steep. But they take a back seat to the Human Resources department. Forget sophisticated vehicles or sensitive instrumentation—the most temperamental, fragile things we send to the Red Planet will be humans.

After all, NASA’s Opportunity rover roamed Mars for 14 years, separated from Earth by a half-hour communications delay, scoured by dust storms and irradiated by cosmic rays, and never complained or got into a fight with a colleague. 

Humans, though, will be sequestered “in a confined space about the size of a small RV for three years,” James Driskell, a research psychologist at the Florida Maxima Corporation, says of most plausible NASA Mars mission scenarios. Driskell and his company have consulted with the space agency and the US military on the psychological issues of crews in isolated and stressful situations. In tight quarters, “people get angry at each other.”

Current Mars plans, such as NASA’s proposed Artemis mission, would send astronauts there and back on a three-year round trip. But you can imagine how stressful dynamics—danger, isolation, other people—might increase on a permanent base or research station, if crews stayed for a decade (or forever). Or, rather than using your imagination, you can rely on the computer simulation of a Mars settlement produced by George Mason University Computational Social Scientist Anamaria Berea and her colleagues. 

In a forthcoming study that hasn’t yet undergone full peer review, Berea and her colleagues detail how they used an “agent-based modeling” approach—a computer system not all that different from a large video game—to calculate the survivability of different population sizes of Mars settlers. They’ve incorporated personality types, too, for the long haul. They came to two main conclusions: that only a few tens of initial settlers are needed to create a sustainable colony, and that people with more agreeable social traits did better for themselves and the larger settlement. 

[Related: Rodent astronauts suggest trips to Mars will make us anxious, forgetful, and afraid]

The new study originated as a response to other papers suggesting that between 100 and 300 people would be the minimum necessary to begin a sustainable settlement on Mars. The nonprofit Blue Marble Science Institute, which studies questions of planetary science and habitability, contacted Berea to see whether her team could verify the other studies’ minimally viable population numbers. 

Berea says she had a better idea: Creating a simulation for a space habitat that included “human, social, and behavioral factors.” Berea and her team at the computational social sciences department had created simulated humans, who were assigned a set of skills necessary for running a Mars settlement, such as producing food or maintaining life support systems. 

Each faux settler had one of four aggregate personality types: There were the “agreeables,” highly social and low in scores of aggressions or competitiveness; “socials,” extroverts with a bit more of a competitive edge; “reactives,” who were more still competitive and fixated on fixed routines; and “neurotics,” highly competitive people with difficulty coping with changes in routine or boredom. Settlement members could die in accidents, or due to “health” conditions determined by the available food and life support resources, but could also be replenished by resupply shuttles every 18 months—the researchers chose not to model sex and reproduction. 

After running multiple computer models for more than 20 simulated years, the study authors found that settlements could begin with far fewer than 100 settlers and remain sustainable, despite accidents or dips in food supplies. The lowest number to kickstart a sustainable settlement was 22 people, but that is not a hard limit, according to Berea. “It’s somewhere between 10 and 50,” she says. “It’s in the tens; It’s not in the hundreds like the other papers were saying.”

[Related: NASA rover finds evidence of carbon-based chemistry in Martian crater]

They also found that agreeable personality types were the most likely to survive to the end of each simulation run. But Bera is careful to note that the agents—the algorithmic representations of humans—do not remain static through the simulation, just as people, whatever their personalities, change over time. “The neurotic that puts his or her foot down on the planet on day zero might not be the neurotic on day 100. They interact, and they adjust,” she says.

This can be seen in real-world Mars mission simulations, such as the Hawaii Space Exploration Analog and Simulation (HI-SEAS) missions, which places crews of six people in a simulated Mars habituated on the rocky lava slopes of Mauna Loa. There, it’s vital to anticipate the ways people change over time. 

“For the first few weeks, usually of people living under stressful conditions, they can still kind of have a ‘honeymoon period’ where everyone’s still very polite and patient and can kind of get along despite some challenges,” says astrobiologist Michaela Musilova, the former director of HI-SEAS from 2018 until 2022. “Usually after the first few weeks is when people really start to struggle and if they’re not prepared for it properly.” 

That struggle could take the form of depression or rudeness with other crew members or mission control. Over the 30 simulated Moon and Mars missions for which Musilova served as commander, she found the answer was to consciously forge bonds between crew members using shared meals and evening recreation, such as karaoke. 

“The more the crew bonded, the longer the ‘honeymoon period’ lasted and even when it wore off, the crew still behaved politely towards one another,” she says. 

Musilova also found that selecting as diverse a group of people as possible, in terms of skills, life experience and ethnicity, helped ensure a better functioning team. 

That’s one thing that Berea and her colleagues didn’t model—all of their simulations contained equal numbers of the four personality types they had defined, rather than trying to build teams composed of different proportions of different types of people. Purposefully screening for personality is something Driskell notes is important for building teams going into difficult and isolated conditions. 

“What type of trait profiles do we want in that team? That sociability and extraversion is really good, but you don’t want a team full of it, because then they’re going to really want to just interact and get along and talk,” Driskell says. At the same time, he adds, you have people who are very competent and follow the rules and keep things running, but who are just a complete pain to live with. “Everybody’s got an example of somebody who was extremely technically adept, but you just could not get along with them,” he says. “I guess Elon Musk is a good example.”

Neither human nor computer simulations of Mars missions can ever fully predict the experience of putting human boots on the Red Planet, but each approach also takes a different slice of the problem. Computer simulations such as Berea’s and her colleagues can give researchers some idea of the large-scale population dynamics and psychology of a Mars settlement over many years. A 12-month HI-SEAS Mars mission, meanwhile, helps tease out real-life psychological nuance you can’t get from a computer model. 

Berea hopes to do more to integrate both approaches in the future, noting that NASA has just launched a new Mars analog mission, the Crew Health and Performance Exploration Analog (CHAPEA) in the Mars Dune Alpha habitat. “Once they are done with that project, it would be great to get the data and compare that with our model for validation,” she says.

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In 2022, NASA’s Artemis I mission traveled 1.4 million miles into space. When the Orion spacecraft flew by the moon, future trees were on board. The uncrewed spacecraft contained seeds for five tree species, including sweetgums, Douglas-firs, sycamores, loblolly pines, and giant sequoias. After the 25.5 day mission, the Forest Service successfully germinated the seeds. Now, community organizations and schools across the United States now apply to receive a seedling grown from one of the tree seeds that flew by the moon that will grow to become official Artemis Moon Trees. 

[Related: Artemis I’s solar panels harvested a lot more energy than expected.]

NASA and the United States Department of Agriculture Forest Service will distribute the Artemis Moon Tree seedlings in an effort to “create new ways for communities home on Earth to connect with humanity’s exploration of space for the benefit of all” and promote STEM in the classroom and beyond. 

Institutions that can apply for a seedling include universities, museums, science centers, organizations that serve K-12 schools, and government organizations. Applications are posted here and are due by Friday October 6. 

The Artemis I Mission launched on November 16, 2022 and was the first integrated test of NASA’s latest deep space exploration technology: the Orion spacecraft itself, the all-powerful Space Launch System rocket, and the ground systems at Kennedy Space Center. Orion returned to Earth after 25.5 days in space, where it journeyed 270,000 miles away from Earth, orbited the moon, and collected crucial data along the way. A plush Snoopy zero-gravity indicator, LEGO minifigures, and three ‘moonikins,’ were also aboard the spacecraft with the Artemis seeds.

“NASA’s Artemis moon trees are bringing the science and ingenuity of space exploration back down to Earth,” NASA Administrator Bill Nelson said in a statement. “Last year, these seeds flew on the Artemis I mission 40,000 miles beyond the Moon. With the help of the USDA, this new generation of Moon trees will plant the spirit of exploration across our communities and inspire the next generation of explorers.”

[Related: Before the Artemis II crew can go to the moon, they need to master flying high above Earth.]

The Artemis seeds are also the second generation of Moon Trees. In 1971, Apollo 14 Command Module Pilot Stuart Roosa, carried hundreds of tree seeds about the mission as a part of his personal kit. Roosa was a former Forest Service smokejumper, a group of specially trained wildland firefighters who are often the first to respond to remote firefighters. When Apollo 14 returned, the Forest Service germinated the seeds and the first generation of Apollo Moon Tree seedlings were then planted around the United States.

NASA and the Forest Service hope that this next 21st Century generation of Moon Trees carry on the legacy of inspiration launched over 50 years ago. 

“The seeds that flew on the Artemis mission will soon be Moon Trees standing proudly on campuses and institutions across the country,” Forest Service chief Randy Moore said in a statement. “These future Moon Trees, like those that came before them, serve as a potent symbol that when we put our mind to a task, there is nothing we can’t accomplish. They will inspire future generations of scientists, whose research underpins all that we do here at the Forest Service.”

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Blue moons, black moons, pink moons, strawberry moons, micromoons, supermoons. For some reason, your news aggregation algorithm of choice thinks you really really really want to know all about these moons. “Catch This Weekend’s AMAZING SUPERMOON,” one headline (or, perhaps, 500 of them) will announce. “The Supermoon Isn’t Actually A Big Deal And You’re All Ruining Astronomy,” another will grouse.

The latest example is the full moon that will peak on August 30 around 9:36 p.m. Eastern Daylight Time: the so-called ”blue supermoon”. It’s the second-to-last supermoon of 2023, and should appear the brightest and biggest of all the full moons this year. It will also coincide with—and reduce the visibility of—the end of the Perseid meteor shower.

Here’s everything you need to know about this headline-grabbing moon, the next one, and all the rest.

What is a full moon?

Look, it’s okay if you don’t know. There are probably loads of folks who walk around pretending they totally know why that thing in the sky seems to get bigger and smaller at regular intervals who totally do not.

[Related: How to take a picture of the moon that doesn’t look like a tiny, white blob]

The moon orbits Earth, and it’s tidally locked—that means it always shows us the same face, instead of twirling around like our planet does. That’s why you can always see the man on the moon (or the moon rabbit, depending on your cultural preferences) even as the satellite spins around us. But while the moon is big and bright in the sky when it’s full, that’s only because it’s reflecting light from the sun. The moon is also always moving, so it’s getting hit with sunlight at different angles. It’s invisible to us during the “new moon,” because the celestial body is parked right between us and the sun; the so-called dark side of the moon is lit up like Las Vegas, but the side we can see is in shadow. A full moon happens when Earth is right between the sun and the moon, so sunlight hits the part we can see. All the other phases are just the transition from one of those extremes to the other.

What is a supermoon?

A moon’s supermoon status is often the subject of fierce debate. This is because, as EarthSky explains, a supermoon may sound more scientific than a blood Moon or Worm Moon, but it’s still not a term with a scientific definition. In fact, it was coined not by an astronomer, but by an astrologer named Richard Nolle in 1979. Basically, whether or not a particular moon is a supermoon boils down to how different stargazers (amateur and otherwise) calculate just how relatively close a full moon has to be to be considered super.

The moon isn’t always exactly the same distance from Earth, because its orbit isn’t perfectly circular. We call the closest point perigee (when it averages a distance of about 225,803 miles), and the most distant point apogee (when it averages a distance of about 251,968 miles). These shifts are not insignificant, but they’re also far from earth-shattering.

The reason you care about this middling change in distance is that it turns a moon super. When a full moon happens close to perigee, it’s going to look a smidge bigger than if it happened at apogee. Maybe. If you’re lucky. Honestly, the difference is not that profound, but if you’re in a position to photograph the supermoon next to something that showcases the slight increase in scale, it can look pretty cool. Our 2023 supermoons—the ones where perigee for the months lines up with the full moon—fall in July, August, August again, and September. So we’re currently halfway through supermoon season.

And just to really remind you that words are meaningless and the moon is always just the moon no matter what we decide to call it: It sometimes makes its closest monthly (or even annual) approach to Earth on a night we can’t see it, aka on the new moon.

What is a blue moon?

A blue moon is a nickname for when two full moons fall in the same calendar month. Astronomer David Chapman explained for EarthSky that this is merely a quirk of our calendar; once we stopped doing things based on the moon and started trying to follow the sun and the seasons, we stopped having one reliable full moon per month. The moon cycle is 29.53 days long on average, so on most months we still end up with a single new moon and a single full one. But every once in awhile, things sync up so that one month steals a full moon from another.

In March of 2018, we had our second blue moon of that year, to much acclaim. And while that’s not necessarily special in an oh-gosh-get-out-and-look-at-it kinda way, it’s certainly special: We hadn’t previously had two in one year since 1999. In 2018 (and in 1999) both January and March stacked full moons on the first and last nights of the month, leaving February in the dark. The next time this will happen is 2037.

Even getting two blue moons in a 12-month cycle is rare, but we have individual blue moons every few years. (The next one after August 2023 won’t be until May 2026.) Also, fun fact: It’s not actually blue. A moon can indeed take on a moody blue hue, but this only happens when particles of just the right size disperse through the sky—and it has nothing to do with the moon’s status as “blue.” Big clouds of ash from volcanic eruptions or fires can do the trick, but it doesn’t happen often, and the stars would certainly have to align for two such rare instances to occur at once.

Is there another kind of blue moon?

Surprise! There’s another kind of moon that some farmer’s almanacs refer to as blue. Just as there’s typically one full moon a month, there are generally three full moons a season. And just as there are sometimes two full moons in a month due to our calendar almost-but-not-quite following the lunar cycle, there are sometimes four full moons in a season. April 2019’s full moon landed right as spring began, leaving enough time for another three. Some breathlessly referred to this as a rare occurrence, but it happens every couple of years.

Weirdly, the blue moon moniker is applied not to the fourth full moon in a season (which actually only happens once-in-a-you-know-what) but to the third. Why? Who knows. What’s the fourth full moon in a season called? A full moon. ¯\_(ツ)_/¯

Similarly, the term “black moon” most commonly refers to the second new moon in a calendar month, but can also refer to the third new moon in a season with four of them. The phrase has also historically been applied to months without full moons, as well as months without new moons. Each of these circumstances occur about once every 19 years, and only in February.

What’s a sturgeon moon?

There won’t be anything fishy about a sturgeon moon’s appearance. Instead, as NASA notes, this refers to what some Algonquin tribes called the moon during August; at this time of year, Native Americans fished for sturgeon in the Great Lakes. There are other names for it, too, like the ”green corn moon.”

Sometimes you’ll see a headline that promises a moon with so many qualifiers it makes your head spin. A superblueblood wolf moon, perhaps? Lots of websites will tell you that “wolf moon” is the traditional name of the first full moon of the year in “Native American” cultures, which is kind of a weird thing to claim given that there are 573 registered Tribal Nations in the US alone today, not to mention historically. The idea that hungry, howling wolves were such a universal constant in January that all of North America, with its disparate cultures, geographies, and languages, spontaneously came up with the same nickname is—well, it’s silly. It’s a silly idea.

[Related: Landing on the moon only made us love it more]

The Farmer’s Almanac now lists a handful of alternatives for historical August moon names: the black cherries moon (Assiniboine), ricing moon (Anishinaabe), and harvest moon (Dakota), to name just a few.

Many cultures have traditional names for the full moon in a given month or season, so there’s quite a list to draw from if you’re trying to really plump up a story on a perfectly pedestrian full moon. But these are all based on human calendars and activities and folklore; you will not go outside and see a fish-scale moon in August or a fuchsia moon in April (or a moon full of beavers in November, for that matter), though I wish it were so.

What is a new moon?

Every 29.531 days, the relative positions of the sun, moon, and Earth conspire to leave our satellite—which doesn’t produce its own light, but shines thanks to the reflected light of our host star—in the dark. The sun’s rays are still striking the moon’s surface, but they’re hitting the (obviously inappropriately named) dark side that faces away from us. The moon appears to grow and shrink in the sky throughout the month thanks to shifts in its position relative to Earth and the sun. Fun fact: while basically everyone knows what a crescent moon is and why it’s so-called, you might not know that the bulbous shape of a moon somewhere between a straight split down its face and a full circle is called “gibbous,” from the Latin word for hunched or humped.

What is a micro moon?

It’s the opposite of the super one. Size isn’t everything. In a previous version of this article, I wrote that while we had such a moon coming up in September 2019, we probably wouldn’t see tons of news outlets crowing over the Micro full corn moon. I was only half right: There were plenty of headlines crowing, though they decided to dub it the harvest micromoon instead.

As is the case with supermoons, you shouldn’t expect to see a noticeable difference in a micromoon’s size.

What is a black moon?

You may be familiar with the concept of a blue moon (see above), which rather dramatically refers to the second full moon in a month. A black moon is the same thing, but for the second new moon in a month. This happens about once every three years. What’s it look like? Well, it looks like a new moon. That means you can’t really see it. But by all means, get out there and do some stargazing.

In case you haven’t yet really grasped the fact that all of these moons are just the result of our arbitrary and often nonsensical calendar system, consider this: In some time zones, a new month at the end of the month will actually rise on the first day of the next month.

What’s a pink moon?

While spring moons may be referred to as pink moons, they won’t actually look pink. Atmospheric conditions can conspire to change the hue of the moon as seen from the ground—NASA has a neat picture of a positively purple one, which is just gorgeous—but there’s no reason to think full moons in April look anything but the usual grayish color. The full pink moon is so-named, according to the Farmer’s Almanac, because its April rise often coincides with the blossoming of a pink North American wildflower called Phlox subulata.

What is a blood moon?

Objectively the most metal moon (sorry, black moon), these only occur during total lunar eclipses (which can happen a few times a year in any given location). When the moon slips through our shadow, our planet gives it a reddish cast. The moon can also look orange whenever it’s rising or setting, or if it hangs low in the horizon all night—the light bouncing off of it has to travel through thicker atmosphere there, which scatters more blue light away. But you’ll probably only see that deep, sinister red during an eclipse.

[Related: Volunteer astronomers bring wonders of the universe into prisons]

A lot of headlines about moons are just silly (you do not need to be particularly excited about a blue moon, it just looks like a regular ol’ moon), but you should definitely roll out of bed to look at a blood moon if one is going to be visible in your region. But anyone who crams both “blood” and “eclipse” into their moniker for a moon is just trying to win the search engine optimization game; a blood moon is just a lunar eclipse that’s going through a goth phase. Ryan F. Mandelbaum at Gizmodo makes the case that we should really just stop throwing the phrase “blood moon” around and call them lunar eclipses, which is tough but fair, because they’re lunar eclipses and not evidence of bloody battles between the sky gods.

A flower blood supermoon, meanwhile? We can get behind that.

This post has been updated. It was originally published on March 2018.

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Having already done a decent job of it here on Earth, humans are well on their way to polluting the skies just beyond our atmosphere. After nearly 70 years of modern rocketry and satellite projects, there are literally millions of centimeter-and-larger discarded objects orbiting the planet—alongside an estimated 130 million tinier bits of space trash. Cleaning up all that debris is already presenting a challenge for experts and legislatorsReportedly, it’s gotten so bad that pilot projects can’t even get off the ground without being forced to recalibrate their objectives.

According to the European Space Agency working alongside Swiss startup ClearSpace, project planners will need to alter their proof-of-concept “derelict object” removal mission currently scheduled for 2026. The reason? It appears the space junk intended for capture and controlled deorbiting has been hit by another piece of space junk. ESA and ClearSpace representatives estimate the most likely cause is a “hypervelocity impact of a small, untracked object” that slammed into their 113kg, two-meter-wide rocket debris target first jettisoned during a 2013 ESA mission. Although the collision appears to have resulted in a “low-energy release of new fragments,” the team’s preliminary assessment indicates a “negligible” increase in collision risks for future missions.

[Related: “How harpoons, magnets, and ion blasts could help us clean up space junk.”]

The ClearSpace-1 mission team is currently continuing as planned as more data is collected on their slightly banged-up target, while a full analysis isn’t expected for at least “several weeks.” Until then, ClearSpace and the ESA are treating the new complication as a fine example of why such projects are already so necessary.

“This fragmentation event underlines the relevance of the ClearSpace-1 mission. The most significant threat posed by larger objects of space debris is that they fragment into clouds of smaller objects that can each cause significant damage to active satellites,” ESA reps explained. “To minimize the number of fragmentation events, we must urgently reduce the creation of new space debris and begin actively mitigating the impact of existing objects.”

As Universe Today also notes, fast-tracking these projects is incredibly important in order to avoid what is known as the “Kessler cascade” or “Kessler syndrome.” In these scenarios, the orbital space above Earth becomes so junky that debris collisions are essentially impossible to avoid, thus producing more debris, which begets more collisions, and so forth. Like our other pollution-based problems here on Earth, it’s difficult to estimate a time frame for an exact tipping point—but suffice to say, agencies like the ESA will know it when they see it. Barring additional orbital shenanigans, here’s to hoping projects like ClearSpace-1 will achieve their goals and get much-needed space cleanup underway.

Update August 25, 2023 9:17am: In a statement provided to PopSci, P.J. Blount, Cardiff University law lecturer and executive secretary for the International Institute of Space Law wrote:

“Space debris is an increasing problem that puts the benefits we receive from space at risk. Reducing the overall amount of debris will be critical to avoiding the onset Kessler syndrome. This will need to be a global effort, which will require coordination and cooperation of the major space powers. In the near term, it is unlikely that we will see new international law emerge to help address this issue. National level legislation, might help to alleviate some pressures operators face but will not be able to sufficiently address the debris problem without a global effort.”

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With its vanishing clouds and now a large dark spot, the planet Neptune appears to be going through some things. Here’s a bit about why the eighth planet in our solar system is causing all this drama. 

[Related: Neptune’s faint rings glimmer in new James Webb Space Telescope image.]

Is Neptune the new Jupiter? 

Astronomers using the European Southern Observatory’s Very Large Telescope (VLT) have observed a large dark spot and a smaller bright spot next to it in Neptune’s atmosphere. This is the first time that the planet’s dark spots have ever been observed using an Earth-based telescope The findings were published on August 24 in the journal Nature Astronomy. These new spots are only occasional features in the blue background of Neptune’s atmosphere and the new results are providing clues to their mysterious nature and origin. Spots are common in the atmospheres of giant planets, with Jupiter’s Great Red Spot being the most famous. In 1989, a dark spot was first discovered on Neptune by NASA’s Voyager 2 before the spots disappeared just a few years later. 

The international team of researchers used the VLT to rule out the possibility that the dark spots are caused by a ‘clearing’ in the planet’s clouds. The team’s new observations indicate that the dark spots are likely due to air particles darkening in the layer below the main visible haze layer, as these hazes and ices mix in Neptune’s atmosphere.

The team used the VLT’s Multi Unit Spectroscopic Explorer (MUSE) to split the reflected sunlight from Neptune and its spot into component colors, or wavelengths, so that they could  study the spot in more detail than was possible before. 

The observations also offered up a surprise result. 

“In the process we discovered a rare deep bright cloud type that had never been identified before, even from space,” study co-author and University of California, Berkeley planetary scientist Michael Wong, said in a statement. 

These unusual luminous clouds appeared as a bright spot along the larger main dark spot, showing that the new “deep bright cloud” was actually at the same level in the atmosphere as the main dark spot. The team says this is a completely new type of feature compared to the smaller ‘companion’ clouds of high-altitude methane ice that astronomers have previously observed. 

The case of the disappearing clouds

About four years ago, Neptune’s ghostly, cirrus-like clouds largely disappeared, and only a patch of clouds hovering over the ice giant’s south pole exists today. Using almost 30 years worth of observations captured by three different space telescopes, scientists have finally determined that the diminished cloud cover could be in sync with the solar cycle. The findings were recently published in the journal Icarus.

[Related: Neptune’s bumpy childhood could reveal our solar system’s missing planets.]

“These remarkable data give us the strongest evidence yet that Neptune’s cloud cover correlates with the Sun’s cycle,” study co-author and University of California, Berkeley astronomer Imke de Pater said in a statement. “Our findings support the theory that the sun’s (ultraviolet) rays, when strong enough, may be triggering a photochemical reaction that produces Neptune’s clouds.”

The level of activity in the sun’s dynamic magnetic field will increase and decrease during the solar cycle. According to NASA, every 11 years, the magnetic field flips, as it becomes more tangled like a bundle of string. During periods of more heightened activity on the sun, more intense ultraviolet radiation bombards our solar system.

The team used data from the Lick Observatory in California, the W.M. Keck Observatory in Hawaii, and NASA’s 30-year-old Hubble Space Telescope and observed 2.5 cycles of cloud activity over the 29-year period of Neptune observations. The planet’s reflectivity increased in 2002 and dimmed in 2007. Then, the ice giant brightened again in 2015 before it darkened to its lowest level ever seen in 2020. That’s when most of the cloud cover faded away.

“It’s fascinating to be able to use telescopes on Earth to study the climate of a world more than 2.5 billion miles away from us,” study co-author and Keck Observatory staff astronomer Carlos Alvarez said in a statement. “Advances in technology and observations have enabled us to constrain Neptune’s atmospheric models, which are key to understanding the correlation between the ice giant’s climate and the solar cycle.”

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On the one hand, the sun provides life-giving heat and light. On the other, it spews an incessant stream of potentially harmful charged particles. These particles form the solar wind, and it is no less formidable than our star’s other products. Without Earth’s magnetic field to shield our planet’s surface, we would constantly face a bombardment of ionizing radiation.

But astronomers have never been completely certain where those particles come from or how they travel into interplanetary space. Now, they’ve found a promising clue. Using ESA’s Solar Orbiter spacecraft, researchers have found miniature jets that seem to channel particles up through holes in the sun’s corona and away from the star. These jets might combine to blow the solar wind, a group of astronomers suggests in a paper published in the journal Science on Thursday.

The corona, a star’s outermost layer, is a sheath of undulating plasma. It is almost always hidden in visible light, although it’s thousands of times hotter than the layers below. We might only see this outer layer during a solar eclipse, when the moon blots out the rest of the sun. 

But the corona is not one even layer. Imaging the sun in ultraviolet reveals shifting dark swatches: regions where the corona’s plasma is cooler and less dense. Astronomers call these areas coronal holes.

[Related: Why is space cold if the sun is hot?]

Coronal holes also seem to resculpt the sun’s powerful, endlessly changing magnetic field. In these parts, lines that guide the sun’s magnetic field seem to blow outward. “Usually, magnetic fields loop back to the solar surface, but in these open field regions the lines of force stretch into interplanetary space,” says Lakshmi Pradeep Chitta, an astronomer at the Max Planck Institute for Solar System Research in Göttingen, Germany, and one of the paper’s authors.

It’s also within coronal holes that the sun’s magnetic field lines can knot about themselves. When that happens, the magnetic field realigns and reconnects, creating fierce electrical surges. Those energetic outbursts siphon matter from deeper layers of the sun and toss them away in jets that can stretch more than a thousand miles across. Astronomers had long suspected that these jets fuel the solar wind, but didn’t know if these jets could provide enough particles to fill the solar wind we observe.

Sun-watching spacecraft like Yohkoh and SOHO have been able to see jets since the 1990s. But astronomers say that none have the sightseeing abilities of Solar Orbiter, which launched in 2020. At its closest approach, Solar Orbiter dips closer to the sun than Mercury.

“Solar Orbiter has the advantage of being located close to the sun, so it can detect smaller and fainter jets,” says Yi-Ming Wang, an astronomer at the US Naval Research Laboratory, who was not an author of the paper.

In March 2022, Chitta and his colleagues focused one of Solar Orbiter’s ultraviolet cameras upon a coronal hole situated near the sun’s south pole. When they did, they glimpsed a type of miniature jet never before seen by humans. Each of these tiny jets carried around one-trillionth the energy of a full-size version. The authors dubbed these “picoflare jets,” dipping into SI system prefixes.

These adorable-sounding surges don’t stick around. Each fleeting picoflare jet lasts about a minute. But this is still the sun—a place of immense power. A single solar picojet might create enough energy to power a small city for a year.

[Related: How a sun shade tied to an asteroid could cool Earth]

The authors scoured only one small part of the sun, but they saw picoflare jets in every corner they looked. It’s likely they cover much of the sun’s surface. Myriads of miniature jets, then, might combine into a large-scale process that transfers charged particles away from the star and out toward the planets.

“We suggest that these tiny picoflare jets could actually be a major source of mass and energy to sustain the solar wind,” Chitta says.

In years past, many astronomers thought of the solar wind as a steady flow, streaming away from the sun at a constant rate. But, if surging picoflare jets drive the solar wind, then the phenomenon might actually be ragged, uneven, and constantly in flux. Picoflare jets may not be the only source of the solar wind, but if Chitta and colleagues are correct, they’re at least a significant contributor.

Fortunately, scientists in a few years’ time will have plenty of additional tools to peer into the sun. Alongside the Solar Orbiter—and future sun-seeing spacecraft, such as the Japanese-led SOLAR-C—they’ll have more powerful solar magnetograms, instruments that allow them to directly measure the sun’s magnetic field from places like Southern California and Maui, able to track the magnetic fluctuations powering the sun’s jets from right here on Earth.

The post Mini jets of energy could power the sun’s violent winds appeared first on Popular Science.

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