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Will the new moon race turn Earth’s nearest neighbor into a dumping ground?

An 8,800-pound (4,000 kilograms) Falcon 9 rocket stage hit the moon last Wednesday (Aug. 5), stirring lunar regolith in a massive plume of dust observable all the way from Earth.

The rocket joined some 3,000 manmade objects scattered on the surface of our planet's companion. Some experts think it's about time we start treating the pristine lunar environment with a bit more respect.

Around 200 tons of Earth stuff have been either deliberately left on or crashed into the moon since the beginning of the space age. Some of this material has a prominent place in history books: The descent modules from all six Apollo landing missions, Soviet Lunakhod rovers from the 1970s and China's 2010s Yutu 1 and 2 robots still sit where they had been left or ran out of power.

But there is also a lot of stuff on the moon that wasn't really meant to end up there. Astronomer and space historian Jonathan McDowell says that many rocket stages and other objects left in orbit between Earth and the moon since the first lunar missions in the 1960s may have ended up on the gray dirt. Four years before the Falcon 9 upper stage crashed near Einstein Crater, for example, part of a Chinese Long March 3C rocket slammed into the moon's far side. And experts think such incidents could become increasingly common in the coming years, as exploration of the moon intensifies.

"We're in a transitional moment," McDowell told Space.com. "From the era when there was rare lunar exploration mostly by the U.S. and the Soviet Union, we've seen over the past decade other nations landing on the moon and the beginning of commercial missions. But governance has not kept up with this. We don't have an international set of agreements on how to operate near the moon, how to coordinate activities near the moon, and we're really going to need it because, not only is the amount of activity at the moon increasing, but the number of different players is greatly increasing, too."

Human activities on the moon are governed by the 1967 United Nations Outer Space Treaty, Marieta Valdivia Lefort, a policy officer at the Royal Astronomical Society in the U.K., told Space.com. Article IX of that treaty binds countries to "conduct the exploration of outer space in a way that avoids harmful contamination," she said. But what exactly constitutes such contamination is unclear, she added.

"There are international legal frameworks that apply to activities on the moon and include obligations concerning harmful contamination, but there is no dedicated international 'waste law' or comprehensive 'rubbish-management' system for it," Lefort wrote in an email. "The Outer Space Treaty does not define when contamination becomes 'harmful.' It does not set numerical waste limits, create approved disposal sites or require every object on the moon to be removed."

a photograph of a grey mottled surface on which a dark oval area is circled in white

South Korea's Danuri moon probe captured this photo of the spot where a SpaceX Falcon 9 upper stage hit the moon on Aug. 5, 2026. (Image credit: KARI)

The moon is big. Its surface area, around 14.7 million square miles (38 million square kilometers) rivals that of Asia, Earth's largest continent, which covers 17 million square miles (44 million square km). But the moon's low gravity — around 17% that of Earth — means the dust that an impact stirs up travels a long way and takes a long time to settle, McDowell said.

"It's not just a local event," he said. "It's an equivalent to a continental-level event. In the future, when you have permanent human bases and scientific experiments on the moon, you don't want rocket stages smashing into the moon on a regular basis, creating big plumes of dust that could contaminate instruments or disturb gravitational wave detectors."

Moreover, the artificial material introduced and the craters that arise when heavy rocket stages smash into the lunar surface are altering the lunar environment, potentially erasing yet unexplored scientific material.

"The moon is naturally struck by meteoroids, and those impacts form part of the geological record that scientists are trying to understand," Lefort wrote. "The main concern is the alteration of the moon's physical and chemical environment, particularly where repeated disturbances could damage or obscure valuable scientific evidence."

closeup of the cratered lunar surface, with a white area pointing to a newly formed double crater

A Chinese rocket body impacted the moon on March 4, 2022, creating a double crater roughly 95 feet (29 meters), as seen in this photo taken by NASA's Lunar Reconnaissance Orbiter. (Image credit: NASA/GSFC/Arizona State University)

Gregory Radisic, a space law expert at Australia's Bond University, told Space.com that the Falcon 9 crash was timely, as it can stir debate about responsible behavior in space before the moon gets too busy.

"It's not by good planning that this didn't hit something important," he said. "It's by pure luck that we're only having a conversation about theoretical problems down the line and that this did not destroy a million-dollar experiment or an important site of scientific study."

He added that spaceflight companies may start paying attention to the risks only after human lives are lost or expensive infrastructure suffers, resulting in tangible fines and consequences.

"When there is a loss of life or a loss of investment, the industry will start to care," Radisic said. "As long as things are losing aesthetic or scientific value, the industry is not likely going to care."

The Falcon 9 rocket stage that hit the moon was left in a high-altitude orbit around Earth in January 2025, after it propelled Firefly Aerospace's Blue Ghost and ispace's Resilience landers to the moon.

McDowell explained that, as the rocket stage was left relatively close to the moon, it got repeatedly influenced by lunar gravity, eventually spiralling into its surface.

"If you leave [an object] in an orbit that's in this middle region that is far enough that the moon's gravity is affecting it but not far enough out to go into orbit around the sun, then that orbit is very hard to predict," McDowell said. "The orbital uncertainties multiply over many passes and, eventually, if you get unlucky, the moon tugs it into an orbit where it's going to hit either the moon or Earth in a completely unpredictable way."

McDowell said that, since the January 2025 launch, SpaceX has been pushing its moon-mission rockets farther out into orbit around the sun.

"I hope that we're going to see a new norm evolve, and that what we have seen now is not how you dispose of your rocket stages in the future," he said. 


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Water can survive surprisingly close to the Milky Way’s supermassive black hole, James Webb Space Telescope finds

The heart of the Milky Way may be more hospitable to water than astronomers thought.

Using the James Webb Space Telescope (JWST), researchers detected water and cosmic dust around an aging star only 0.55 light-years from Sagittarius A* (Sgr A*), the supermassive black hole at the center of our galaxy.

The new study suggests that water and dust can form and survive surprisingly close to a supermassive black hole, where intense radiation and other harsh conditions might otherwise be expected to destroy them. The team used Webb's Mid-Infrared Instrument (MIRI) to study IRS 3, an aging star located in the crowded environment surrounding Sgr A*, which has a mass of about 4 million suns, according to a statement from the European Space Agency (ESA).

A bunch of stars against a reddish structure in space.

(Image credit: ESA/Webb, NASA & CSA, F. Peißker, J. Lu, F. Yusef-Zadeh, N. B. Sabha, C. Chan)

"Galactic centres are among the most extreme environments, so understanding whether stars can continue enriching their surroundings there is an important question," Florian Peißker, lead author of the study from the University of Cologne in Germany, said in the statement. "With Webb, we can directly observe how stars behave under these conditions and see that dust production remains remarkably resilient."

IRS 3 — one of the brightest mid-infrared sources in the galactic center — is an asymptotic giant branch star, meaning it has reached a late stage of stellar evolution in which it sheds large amounts of gas and dust through powerful stellar winds. Such dying stars act as cosmic recycling centers, returning material to space that can eventually become incorporated into future generations of stars and planets.

But IRS 3 lives in a particularly unforgiving neighborhood. The center of the Milky Way is densely packed with stars and exposed to intense radiation, raising questions about whether molecules and newly produced dust can persist there.

However, Webb's observations suggest they can. By combining observations of IRS 3's spectrum with simulations of how its light travels through different models of the surrounding material, researchers reconstructed the structure of the star's envelope. They found a layered, shell-like distribution of silicate dust extending roughly 10,000 astronomical units from the star (one astronomical unit, or AU, is the average distance between Earth and the sun). Temperatures within the envelope fall from about 1,700 degrees Fahrenheit (927 degrees Celsius) near the star to around minus 280 F (minus 173 C) in its outer regions. Webb's observations also revealed clear evidence of water within the envelope — the first such detection for IRS 3.

"The detection of water is especially exciting because it shows that molecular material can survive in an environment dominated by intense radiation," Macarena Garcia Marin, co-author of the study and an ESA astronomer, said in the statement.

While the observations don't reveal how much water is present, the detection shows that water can survive in the harsh environment near the galactic center. Water and dust are important ingredients in the chemistry that accompanies star and planet formation, meaning material shed by aging stars such as IRS 3 could eventually contribute to future generations of stars and planets.

Finding water and dust near Sgr A* therefore suggests that aging stars can continue enriching their surroundings even in the harsh conditions near a supermassive black hole. The findings could help astronomers better understand how material is recycled in the centers of galaxies and the role evolved stars play in supplying those regions with fresh dust and molecules.

Their findings were published Aug. 11 in the journal Astronomy & Astrophysics.

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India-US space ties deepen as NASA invites ISRO to join moon base program

NASA has formally invited India to participate in its effort to build a permanent base near the moon's south pole, adding a new dimension to the deep-space cooperation between the two countries.

The invitation was extended last week at the Indian space agency ISRO's headquarters in Bengaluru during the ninth meeting of the U.S.-India Civil Space Joint Working Group. The CSJWG was established in 2005 as a mechanism for bilateral space cooperation and for addressing challenges and pursuing mutual spaceflight goals.

"Building on our successful collaboration in science, NASA reaffirmed its interest in @ISRO joining Moon Base. We're going back to the moon to stay — and we're bringing our partners with us," NASA officials said via X on Tuesday (Aug. 11).

Beyond the lunar base invitation, "the two sides also agreed to advance discussions for cooperation on open scientific data sharing under the Accords," reads a Tuesday statement by the U.S. Embassy in India.

"The Accords" are the Artemis Accords, the U.S.-led diplomatic framework outlining principles for safe and responsible exploration of the moon and beyond. India signed on as the 27th signatory in 2023, joining a coalition that has now grown to 70 nations.

Official statements have provided few details on what India's participation in the Moon Base program would entail in practice. The meeting, however, brought together senior space officials from both countries, including V. Narayanan, the chairman of ISRO and secretary of India's Department of Space, and Sergio Gor, the U.S. Ambassador to India, who addressed the opening session, according to the statement.

The meeting was co-chaired by M. Sankaran, director of ISRO's U.R. Rao Satellite Centre, on the Indian side, and two people on the U.S. side — Wesley Brooks, assistant secretary of state for the U.S. Department of State's Oceans and International Environmental and Scientific Affairs, and Kathleen Karika, NASA associate administrator for International and Interagency Relations, the statement reads.

Over the coming decade, via its Artemis program, NASA plans to build out a sprawling, city-like base near the moon's south pole, a region of particular interest thanks to permanently shadowed craters there that are thought to contain substantial deposits of water ice.

Details of the planned architecture shared by NASA in May envision hilltop habitats to take advantage of sunlight and nuclear power systems located farther away to mitigate radiation risks. The space agency also plans to use small, hopping robots starting in 2028 to scout the south polar region ahead of moon base construction.

This effort to gather information and secure access to the surface is the first of three planned phases. Phase 2, from 2029-2032, is intended to establish the base's initial operating capability. Phase 3, from 2032 onward, aims to achieve a semi-permanent crew presence on the lunar surface, NASA said during the May update.

about 30 well-dressed people sit around a huge u-shaped table decorated with flowers, during a space conference

Senior space officials from India and the U.S. at the ninth meeting of the India-U.S. Civil Space Joint Working Group at ISRO headquarters in Bengaluru on Aug. 5-6, 2026, where NASA invited ISRO to join its Moon Base program. (Image credit: ISRO)

To prioritize infrastructure that supports sustained operations on the moon's surface, increase launch cadence and keep pace with China's lunar ambitions, NASA earlier this year paused development of its long-planned Gateway space station.

For India, the invitation to join NASA's Moon Base program comes as the country pursues its own ambitious lunar exploration and human spaceflight roadmap. Its plans for the 2040s include developing a moon base, establishing a space station in lunar orbit and sending Indian astronauts to the moon, with the broader goal of building long-term human presence beyond Earth.

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SpaceX rocket’s moon crash highlights ‘a tangible operational risk’ of lunar settlement

The moon dust has settled after a 4.5-ton SpaceX rocket body slammed into terrain near Einstein Crater on Aug. 5.

That impact site was imaged by South Korea's moon-orbiting Danuri spacecraft, as well as by NASA's Lunar Reconnaissance Orbiter (LRO). Reportedly, a Chinese commercial space debris monitoring satellite tracked and recorded the 5,400-mph (8,690-kph) moon punch, too.

Wandering through space for over a year, the leftover Falcon 9 upper stage had sent Firefly Aerospace's Blue Ghost-1 lander on its way to the moon back on Jan. 15, 2025. Also sent moonward on that flight was the Hakuto-R Mission 2's Resilience, a robotic lunar lander developed by the Japanese company ispace. While the moon has reclaimed its serenity, the implications of the uncontrolled collision continue to reverberate.

Close encounter

Interestingly, there was also the prospect of a too-close-for-comfort conjunction of the Falcon 9 upper stage and Danuri.

"We noticed roughly late June that there is an incoming Falcon 9 upper stage toward the moon, and also knew that it would be close to Danuri," Eunhyeuk Kim, a senior researcher at the Korea Aerospace Research Institute (KARI), told Space.com.

There was a huge uncertainty in the predicted trajectory of the upper stage, Kim said, while the orbit information of South Korea's Danuri lunar orbiter was quite accurate. "Therefore, we could not neglect the probability of an incoming and close encounter."

a photograph of a grey mottled surface on which a dark oval area is circled in white

Before-and-after imagery of the impact site. (Image credit: KARI)

Spacecraft maneuver

However, around mid July, the KARI/Danuri team performed a maneuver of the spacecraft in preparation of a near-total lunar eclipse on Aug. 28, said Kim. That eclipse will see 96% of the moon's visible surface passing through Earth's dark umbral shadow.

Kim said that the orbiter's maneuver brought a slight change in the phase of the spacecraft's orbit, which canceled the probable conjunction between the upper stage and Danuri.

At the time of the Aug. 5 impact, Danuri was flying over the moon's south pole area, far away from the hit zone, said Kim.

Illustration of the moon, with a white arrow pointing to a spot on its upper lefthand limb

Illustration of the moon, with an arrow pointing to the Falcon 9's upper stage impact site on Aug. 5, 2026. (Image credit: Bill Gray/Project Pluto)

High-speed ejecta

Dean Sladen is a quality manager and aerospace engineer in the United Kingdom for Accu Components, a high-precision manufacturing firm.

"As space agencies and private companies build out permanent lunar infrastructure, uncontrolled rocket stages evolve from a minor nuisance into a tangible operational risk," Sladen told Space.com. "A direct hit is the obvious worst-case scenario, but distant impacts also generate ground shocks and high-speed ejecta that can degrade sensitive equipment over time."

Sladen noted that lunar impacts have been a constant throughout history, with meteorites and comets bombarding the surface unhindered by an atmosphere. "Over the past 65 years, artificial objects have added a new dynamic to these events," he added.

An artist’s concept of astronauts working on the lunar surface.

An artist’s concept of astronauts working on the lunar surface. (Image credit: NASA)

Genuine hazard

Even modest hardware impacts permanently alter the lunar landscape, said Sladen. Given the moon's lack of a substantial atmosphere, there is no air resistance to slow debris down. An impact therefore hurls high-speed ejecta (fine regolith and rock fragments) across vast distances at bullet-like speeds.

"While this isn't a major threat to isolated missions today, as we establish permanent lunar infrastructure, high-velocity ejecta poses a genuine hazard to surface habitats, solar arrays and working astronauts," Sladen said.

To mitigate this issue, Sladen suggested that the industry will likely need designated impact zones or strictly controlled, targeted de-orbit protocols to ensure that spent hardware lands far from active installations.

"That said, human-made debris is only half the equation," Sladen continued. "Natural meteorites remain an ongoing background threat, and, while massive natural strikes are rare, they hit at significantly higher speeds and carry far more energy," Sladen said. "Controlling our own hardware is simply the part of the risk profile we actually have the power to manage."

Plume detections

In the meantime, while the Falcon 9 impact was tough to see from Earth, several observations from our planet reported the detection of sodium and lithium gas above the crash site.

The European Southern Observatory's (ESO) Very Large Telescope (VLT) in Chile, for example, saw the aftermath of the impact. The ESO reported that a chemical fingerprint of the impact was visible for five to 10 minutes, with an enormous plume of lunar material stirred up due to the hard-hitting hardware.

"I'm happy that ESO recorded some evidence of it through VLT, and Danuri has found the exact impact location," said William Jo, a graduate research assistant at the University of Texas, Austin who performed some pre-strike computer simulations.

"What we've learned so far is that the plume was too faint to see against the bright lunar surface, and only a large observatory telescope could pick some parts of it out against the dark sky, which is exactly what happened," Jo told Space.com. "The plume must have shot out high," he said, "and I'd like to know how high, or even whether we can replicate the signals."

Targets of opportunity

"Telescopes make the best spaceships," pointed out Elaina Hyde, director of the Allan I Carswell Observatory at York University in Canada. "We are always on the lookout for 'targets of opportunity' like this event."

Hyde organized a livestream event, training the observatory on the collision locale. They were unable to spot the impact, however.

"The lunar collision was not on our regular research program, but when it happened, we put it as a high-priority item to observe if the weather was clear," Hyde said. "Anything that happens quickly like this is often a target of opportunity, because you do not get a long time to plan the observation."

"However, since it was not visible from our location in Toronto, our 'null' or non detection can actually help to limit the estimates on how big the dust plume was and perhaps some of its properties," said Hyde.

The Lowell Discovery Telescope (LDT) in Arizona.

(Image credit: Lowell Observatory)

Impact response

Also on the moon impact watch were observers using Lowell Observatory equipment in Arizona.

These researchers managed to measure a response from the rocket stage impact, spotting a sizable sodium and lithium gas plume that lasted between five and 10 minutes after impact, reported Carl Schmidt, an assistant research professor at Boston University's Center for Space Physics.

Observers at the 4.3-meter Lowell Discovery Telescope (LDT) in Happy Jack, Arizona used a long slit spectrograph to detect the plume. Graduate students from Boston University continue to analyze data gleaned from the moon wallop.

Bright lithium plume

"At LDT, we saw a bright lithium plume from the rocket body and fainter sodium [signature], likely from the surface itself," Patrick Lierle of Boston University told Space.com. "The bright lithium plume extends more than halfway up our field of view." The LDT results are also credited to Emma Lovett, a Boston University graduate student.

William Jo said he's looking forward to the release of observational data about the impact before he and colleagues can refine their lunar ejecta simulation model.

"That data, combined with our simulations, could tell us things like the composition of the lunar material, what orientation the impact hit at, and so on," Jo said.

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Supermassive black hole spews energy 300,000 light years into deep space

Supermassive black holes are best known for their immense gravity, pulling in everything that strays too close, even light. But new research suggests these cosmic giants can also hurl enormous amounts of energy outward, driving powerful disturbances that ripple hundreds of thousands of light-years through space.

A study led by Satoshi Yamada of Tohoku University in Japan found that winds generated by an actively feeding supermassive black hole are about 100 times more powerful than astronomers previously estimated.

These outflows, scientists say, inject an amount of energy comparable to several billion supernova explosions, driving turbulence through hot gas across distances of roughly 300,000 light-years —far beyond the boundaries of the host galaxy itself.

"Black holes are largely known for sucking matter in, but they also eject gas in the form of powerful winds," Yamada said in a statement. "These winds were thought to be contained within the galaxy, but our study revealed that the force is immensely more powerful than previously understood."

To measure the extent of those outflows, Yamada and his colleagues observed H1821+643, a bright quasar in the constellation Draco about 3.4 billion light-years from Earth. The galaxy hosting H1821+643 sits at the center of a dense galaxy cluster and harbors an active supermassive black hole estimated to be three to four billion times the mass of the sun.

During a weeklong observation in September 2024, Yamada and his team used XRISM, the X-ray satellite launched by Japan's space agency in 2023, to track the chemical signature of ionized iron atoms in the surrounding hot gas. By examining how the light from these iron ions stretched and broadened, the researchers were able to determine how fast the gas was moving and how turbulent it had become, according to the statement.

The observations revealed that the turbulence is driven by energy released from the quasar, with its effects reaching distances of about 300,000 light-years from the black hole, the study notes.

The result builds on years of observations of H1821+643, which is, in fact, the closest known quasar to Earth located within a galaxy cluster, according to NASA.

One of the more intriguing discoveries came in 2022, when observations of the black hole's spin using NASA's Chandra X-ray Observatory showed it rotates half as quickly as its smaller peers, which spin close to the speed of light.

"The million-dollar question is, why?" Christopher Reynolds, an astronomer at the University of Cambridge and co-author of the 2022 study, said in a statement at the time.

According to that study, one leading hypothesis is that giants like H1821+643 grew primarily through repeated mergers with other black holes arriving from different directions. Those chaotic collisions may have repeatedly disrupted the black hole's rotation instead of steadily spinning it up through a long-lived accretion disk.

While the exact origin of its sluggish spin remains an open question, the black hole's influence clearly extends far beyond its host galaxy.

"For the first time, we have shown that black holes influence the broader cosmic environment through a shock wave of astonishing power," Yamada said in the statement.

"Black holes are key drivers of gas flows and motion in space, transporting vast amounts of energy to different regions of the cosmos."

This research is also described in a paper published July 28 in the journal Nature Astronomy.

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Farthest ‘black hole star’ ever found could help solve the James Webb Space Telescope’s little red dot mystery

The most distant 'black hole star' yet found, existing in the universe less than 660 million years after the Big Bang, has provided a vital clue as to the origin of the mysterious "little red dots" that populate the James Webb Space Telescope's images of the early universe.

The consensus seems to be that these bizarre objects, which were first discovered in 2022, are growing supermassive black holes entombed within huge clouds of gas that have spectrums similar to cool, red stars, such as red giants. Recently, astronomers have been finding that some of these objects are placed within the center of young galaxies whose light has been traveling for about 12 billion years, give or take a billion, to reach us. Given their distance and faintness, black hole stars' light is difficult to disentangle from the light of a surrounding galaxy, especially when we know there is likely a galaxy there that's too faint for the JWST to resolve.

However, a newly discovered black hole star, unearthed during a JWST program called the Mirage or Miracle (MoM) survey, is acting as a kind of a missing link.

"The Mirage or Miracle survey was designed specifically to target sources considered 'risky,' meaning they could either be amazing discoveries or just interlopers, such as some cold nearby stars that look like distant galaxies," Jorryt Matthee of the Institute of Science and Technology Austria and a co-investigator on the MoM survey said in a statement. In particular, the survey focuses on objects that look like they could be very high redshift galaxies (around a redshift of 10 or more, which equates to having existed about at least 13.1 billion years ago).

The black hole star found by the survey has been named MoM-BH*-1 and is the best example yet of a "naked" black hole star, meaning astronomers are fairly certain it exists in space on its own rather than inside a burgeoning galaxy. This means all of its light is generated by accretion onto the black hole at the center of the cloud. Though we cannot see this accretion because of the obscuring gas cloud, this light energizes the surrounding cloud from within, causing it to glow just as energy generated within the sun causes its outer layers to radiate.

"The spectrum we detected is our best evidence of a cloak of gas feeding an early forming black hole," Rohan Naidu of the University of Hawaii, who led the team who discovered MoM-BH*-1 and is co-leader of the MoM survey, said in the statement.

Six images of blurry red dots.

Some of the JWST's little red dot discoveries. (Image credit: NASA, ESA, CSA, STScI, Dale Kocevski (Colby College))

Intriguingly, MoM-BH*-1 lies close in space to a young galaxy at the same redshift, and estimates suggest that it will take another 100 million years for the black hole star to collide and merge with the galaxy. Naidu and Matthee's team modeled what the spectrum of the galaxy would look like after it has merged with MoM-BH*-1, and found that it would look very much like the little red dots already known to exist within galaxies.

"Considering the black hole star as a template for the black hole component of little red dots helps clarify many of the uncertainties about them," said Matthee. "If embedded in similar host galaxies, black hole stars like MoM-BH*-1 might well serve as the central engines of baby quasars."

In this way, MoM-BH*-1 provides strong evidence for the object at the heart of faint galaxies encompassing little red dots as being a black hole star. Recent observations of some little red dots at lower redshifts have shown the cloud of gas around the black hole begin to disintegrate, exposing the black hole and the X-rays produced by the accretion of gas onto it. These black holes appear to be growing fast, and the environments surrounding such active black holes become highly luminous, creating a quasar.

An illustration on the left of a star cut open so you can see the inside. In the center, a black hole with an accretion disk. On the right, a black circle surrounded by a sphere of red. This is a black hole star.

An artist's impression depicting the similarity between stars and black hole stars, except that black hole stars are at least 100,000 times larger than the sun. (Image credit: Rohan Naidu (University of Hawaii).)

"Astronomers have never lacked imagination: since the discovery of quasars, there has been no dearth of theories to explain how these black holes grew so massive so fast," said Naidu. "Something spectacular must have happened in the early universe. Now with JWST, we can directly observe this era and see for ourselves which scenarios actually occur."

Learning of the birth of supermassive black holes and whether they predate the galaxies that surround them was one of the primary science goals of the JWST before it launched. In this it has been tremendously successful so far. Despite little red dots having only been discovered four years ago, research into them and black hole stars is accelerating, with new findings coming out now almost on a weekly basis.

"These are incredibly exciting times with nearly a thousand papers and preprints on little red dots in the past two to three years," said Matthee. "Far from a mirage, this might well be a cosmic miracle."

The findings were published on Aug. 13 in the journal Nature.

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Green comet caught soaring over Namibia | Space photo of the day for Aug. 12, 2026

A green comet on a black backdrop with stars.

Comet 220P/McNaught soaring over Namibia on August 8, 2026. (Image credit: Gerald Rhemann and Michael Jäger)

What a view. Astrophotographers in Namibia have captured a bright green comet soaring overhead in a spectacular new photograph.

What is it?

In this incredible new photograph is the comet 220P/McNaught.

Discovered by Australian astronomer Robert H. McNaught, the comet orbits our sun once every 5.5 years. Back in June, the comet reached perihelion, or the closest point in its orbit around the sun. Around that time, the comet experienced a large outburst, which brightened it about 8,000 times.

The comet brightened back up this August to about 600 times its normal brightness — and it was during this period when astrophotographers Gerald Rhemann and Michael Jäger captured it streaking across the night sky over Namibia.

To capture the moment, the pair used a 12-inch Astrograph telescope with a ZWO ASI 6200 MM Pro camera.

Why is it incredible?

It's not every day you see a comet in the night sky. Even if one is overhead, often they're too tricky or too far away to spot without a telescope, and even then it can be a challenge.

It's also incredible that the moment captured in the new image showcases the comet 220P/McNaught with such spectacular clarity and detail. It must have been something truly special to witness.

While spotting a comet like this might not happen every day, we can sometimes see the debris trailing behind a comet as its tail burns up in our atmosphere. These burnt comet bits are actually the "shooting stars" we see in the night sky during a meteor shower.

Right now, the Perseids meteor shower is on its annual parade across the night sky. This meteor shower is made up of debris shed by the comet Swift-Tuttle as it swoops by on its annual trip across the solar system. Under dark skies, skywatchers can see up to 100 shooting stars thanks to Swift-Tuttle.

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Scientists create largest 2D map of the universe with 5.6 trillion pixels and nearly 4 billion cosmic objects

Astronomers have released the largest two-dimensional map of the universe ever created, offering a sweeping new view of nearly 4 billion celestial objects across roughly three-quarters of the sky.

The new map, created by the Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Surveys team, contains a staggering 5.6 trillion pixels and combines more than 263,000 telescope exposures collected over more than a decade. The observations span visible and near-infrared wavelengths, providing an enormous portrait of stars, galaxies and other cosmic phenomena across the sky, according to a statement from the National Science Foundation (NSF) NOIRLab. (You can explore the full data here.)

"It's part of the fabric of astronomy research now," David Schlegel, co-lead of the Legacy Surveys and a scientist at the U.S. Department of Energy's Lawrence Berkeley National Laboratory, said in the statement. "When you're working with astronomical objects today, you often start by pulling up the Legacy Imaging Viewer to see what you're looking at."

The latest 2D cosmic map represents the culmination of 13 years of observations and data processing. The Legacy Imaging Surveys were originally designed to help DESI determine where to point its thousands of robotic optical fibers, essentially creating the 2D foundation for DESI's much larger effort to map the universe in three dimensions.

Installed on the Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory in Arizona, DESI measures the spectra of galaxies and quasars. By determining their redshifts — how much their light has been stretched as the universe expands — astronomers can calculate their distances and transform a flat view of the sky into a 3D map of the cosmos.

DESI began its main survey in 2021 with the goal of tracing how the universe has expanded over billions of years and, in turn, helping scientists better understand dark energy, the mysterious phenomenon thought to be driving that expansion.

The project has since far surpassed its original targets. By April 2026, DESI had mapped more than 47 million galaxies and quasars, creating the largest high-resolution 3D map of the universe to date. Previous DESI results have also provided intriguing evidence that dark energy may evolve over time rather than remain constant, as predicted by the standard model of cosmology.

A large galaxy almost fills the screen. It's a spiral and very glowy and hazy.

Among the nearly four billion objects in the DESI Legacy Imaging Surveys' map is Messier 96 (NGC 3368), a majestic spiral galaxy nestled in the constellation Leo approximately 35 million light-years from Earth.  (Image credit: DESI Legacy Imaging Surveys/LBNL/DOE & KPNO/CTIO/NOIRLab/NSF/AURA)

DESI isn't the only project finding new ways to map the cosmos. Earlier this year, astronomers with the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) created a different kind of 3D map using faint Lyman-alpha emission from hydrogen between galaxies. That effort illuminated previously hidden structures dating to between 9 billion and 11 billion years ago, when the universe was experiencing a peak in star formation.

The new Legacy Imaging Surveys map, meanwhile, will have uses well beyond DESI. Previous versions of the dataset have already been referenced in more than 1,800 scientific papers, while the latest release could help astronomers search for rare objects and phenomena, study galaxy evolution and train artificial intelligence systems to analyze the enormous volumes of data expected from next-generation observatories.

"Explorations of our universe always start with images of the night sky. The DESI Imaging Legacy Surveys are just one step in this venerable human tradition," Arjun Dey, co-lead of the Legacy Imaging Surveys and an astronomer at NSF NOIRLab, said in the statement. "For our team, these data are fundamental to the investigation of the expansion history of the universe and the formation of our galaxy. But the skies belong to everyone, and this survey gives everyone the chance to marvel at their wonders."

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Scientists find 2 million active black holes, exploding stars and more, nearly doubling our view of the high-energy universe

Astronomers have nearly doubled the number of known cosmic X-ray sources, offering the most comprehensive public view yet of the universe's hottest and most energetic objects.

The second major public data release from the German-led eROSITA X-ray telescope contains a catalog of nearly 2 million X-ray-emitting objects, including supermassive black holes, galaxy clusters, stars and other extreme cosmic phenomena. The unprecedented dataset — called DR2 — will help astronomers investigate how black holes grow, galaxies evolve and the universe's largest structures formed, according to a statement from the Max Planck Institute for Extraterrestrial Physics.

"DR2 is the best inventory of the X-ray sky we have to date and opens the door to robust statistical studies of cosmic populations," Miriam E. Ramos-Ceja, Ground Segment Manager of the eROSITA instrument and lead author of the DR2 publication said in the statement.

The new release combines observations collected during eROSITA's first three all-sky scans over 556 days, allowing astronomers to detect increasingly faint X-ray sources that previous surveys missed.

Of the nearly 2 million detections, more than 1.9 million are point-like sources, most of them active supermassive black holes feeding at the centers of distant galaxies or stars within the Milky Way. These black holes offer astronomers a window into how galaxies grow and evolve over cosmic time, while the stellar sources help researchers better understand everything from stellar activity to the life cycles of stars.

Another roughly 64,000 sources are extended objects, including massive galaxy clusters, nearby galaxies and the glowing remnants of exploded stars (also known as supernovas). Galaxy clusters are especially valuable because they trace the universe's largest structures, helping scientists investigate the influence of dark matter and dark energy on the evolution of the cosmos.

Unlike visible light, X-rays reveal some of the universe's most energetic environments. Material spiraling toward a black hole can be heated to millions of degrees before crossing the event horizon, while neutron stars, supernova remnants and the enormous reservoirs of hot gas filling galaxy clusters also emit strongly in X-rays.

The size of the catalog gives astronomers a powerful new dataset for studying the high-energy universe. With nearly 2 million sources observed under the same conditions, astronomers can study how supermassive black holes have grown over billions of years, map the distribution of galaxy clusters to better understand the large-scale structure of the universe, and search for rare or unusual objects that may otherwise have gone unnoticed. Large, uniform surveys also make it easier to compare different classes of objects and identify long-term trends that smaller observations cannot reveal.

A circle in the center with tons of purple and blue dots on it.

A full version of the western X-ray sky from eROSITA. (Image credit: MPE, J. Sanders)

A gif showing a diagram that looks like a transparent sphere rotating left and right. A bunch of purple and red and some yellow dots are congregated on one side of the sphere, shooting outward.

This animation shows a representation of the active galactic nuclei (AGN) identified in the DR2 catalogue. Each dot shows a single object, where the distance from the three-dimensional center increases with the source's redshift, or how far away it is from us.  (Image credit: MPE/J. Sanders)

The release also includes optical and infrared counterparts for many of the X-ray sources, helping astronomers determine whether each object is a nearby star, a distant galaxy, an active supermassive black hole or another type of high-energy phenomenon. In the portion of the catalog where counterparts have been identified, about 88% are distant galaxies hosting actively feeding supermassive black holes, according to the statement.

"X-ray detection is only the first step," Mara Salvato, eROSITA spokesperson and chair of the follow-up working group, said in the statement. "By linking X-ray sources to their counterparts at other wavelengths, we can work out what these objects are, where they sit on the cosmic distance ladder, and build clean, well-defined samples on an unprecedented scale."

Although eROSITA stopped collecting scientific observations in early 2022, the mission completed enough sky scans beforehand to support additional public data releases. Researchers say the next Data Release 3 (DR3) is planned for 2028.

The eROSITA-DE DR2 catalogue is available to view online.

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1-billion-year-old Mars meteorite found in Algeria is like nothing we’ve seen from the Red Planet

A newly found Mars meteorite is revealing the secrets of a previously hidden time period of Red Planet geological history.

The 1.27-billion-year-old space rock, called Northwest Africa (NWA) 13441, was discovered in Algeria in 2019 — but its age was not confirmed until recently. Now scientists say the meteorite helps answer questions about a huge gap in the Martian geologic record: a span of time between 600 million years ago and 2.4 billion years ago.

This vast timespan has no known examples of meteorites containing igneous (solid magma) shergottites, which are the most abundant type of Martian meteorites, chunks of the Red Planet that were blasted away by impacts, ejected into space and eventually fell to Earth. The only meteorites known from this time range, roughly 1.3 billion to 1.4 billion years ago, are rarer types known as chassignites and nahklites. As such, the newly analyzed meteorite is opening new insights already about this time period.

"The characteristics of this meteorite were entirely surprising," stated Boston College Earth and environmental sciences professor Ethan Baxter, co-author of a study published Aug. 1 in the journal Geochimica et Cosmochimica Acta. "No other Martian meteorite like this has an age of 1.27 billion years old."

NWA 13441 was surprising to researchers in two ways. The first was its composition — while it is a shergottite, the space rock also contains isotopes (element types) of a rare-Earth metal called neodymium. Neodymium is usually found in chrondrites — another kind of meteorite made up of unmelted rocks — and chondrites were common in the solar system when it was formed 4.56 billion years ago.

This blended composition of shergottite and chrondrite suggests deeper parts of Mars have remained relatively untouched since the planet was formed, Baxter stated. That finding aligns with what scientists already know about Mars, which likely formed only five million years after the solar system was formed. (Mars also has no plate tectonics, making it different from Earth and which allows the earliest bits of it to remain undisturbed by the types of geologic processes that take place on our planet.)

a person's hand holds a black-and-tan rock

A different Mars meteorite found in Northwest Africa, known as 7635. It is a shergottite believed to be around 2.5 billion years old. (Image credit: Mohammed Hmani)

Peering deeper at the chondrites added a second surprise: the composition of the isotopes, or element types, are helping establish "new boundaries on the processes that happened in the very early solar system as Mars formed," the authors stated. The paper's abstract added this information suggests the meteorite may have come from a "previously unsampled" reservoir on the Red Planet lying between "enriched and depleted shergottite sources."

Scientists hope that more analysis of this meteorite will reveal "magmatic and volcanic activity on Mars," Seal said in the same statement. Next up will be looking at the meteorite's isotopes to figure out its connection to other meteorites formed early in Martian history.