Monitoring Earth from above is a messy, inconsistent business. Clouds can block a satellite view, the angle of the Sun can create huge shadows, and orbital paths might not take a system across the same general area for weeks. That inconsistency is hard to deal with for traditional software, and can even confuse standard deep learning algorithms. But, according to a new review paper by researchers Raul-Alexandru Gorgan and Dorian Gorgan of the Technical University of Cluj-Napoca, there’s a new type of frontier AI that could be able to help - bio-inspired Liquid Neural Networks.

Choosing what orbit to put a satellite in always comes with trade-offs. When it comes to Very Low Earth Orbit (VLEO), between 100-450 km, there are distinct advantages. Remote sensing cameras can take better pictures, comms and radar require less power, and atmospheric drag will automatically clean up dead satellites. But there’s also a cost - air friction requires any satellite in this orbit to use an engine near constantly to stay in orbit, which in turn requires fuel - typically in the form of expensive gases like Xenon. So, as part of his PhD thesis at the University of Stuttgart, which is available in arXiv, Francesco Romano decided to solve that problem by using the very air molecules that cause that friction as fuel for a plasma engine to keep satellites aloft indefinitely in VLEO.

Venus likely never had a moon and even if it did, it would have soon been torn asunder by the planet’s own gravity, says prominent planetary astrophysicist.

Light could only travel freely in the Universe after cosmic reionization. Before that, neutral hydrogen stopped photons from travelling. The JWST has found evidence of an overdensity of galaxies carving out a bubble of reionization. Is this how it all started?

As our telescopes have improved and we’ve been able to peer farther back in time, we’ve begun finding more fascinating features of the universe. But one thing we definitely haven’t found yet is Population III (Pop III) stars. These were the earliest stars in the universe, formed completely from pristine hydrogen and helium, with no “metals” (i.e. elements heavier than those two) polluting their processes. They are also theorized to be absolutely massive, and “die with passion” as Bill Wurtz once put it in a famous YouTube video. A new paper, available in pre-print form on arXiv by Tae Bong Jeon from the Cosmic Frontier Center at the University of Texas at Austin, looks at just how massive those starbursts could be, and whether the James Webb Space Telescope could detect one.

Scientists were shocked when they received the first images of Martian gullies. They were even more shocked as those gullies appeared to change over time. Their similarities to gullies seen on Earth were uncanny, but all of Earth’s gullies are formed by the water run-off, and Martian is too cold and has too sparse an atmosphere to have liquid water on its surface. Whatever has been causing those changing gullies couldn’t have been water, so what was it? A new paper from Apolline Leclef of the Institut d’Astrophysique Spatiale at Université Paris-Saclay and her colleagues, available in pre-print on arXiv, shows how they are likely caused by CO2 frost turning into a fluid.

We’ve found over 5,500 exoplanets so far. Dozens of them have been in the habitable zone of their parent stars, where, at least in theory, they could host an ocean. But we’ve never definitively found a liquid ocean on another planet. A new paper from researchers Eleanor Cornish and Tyler Robinson of the University of Arizona, available in pre-print on arXiv and submitted to the Astrophysical Journal, looks at a unique way we might be able to find one - by looking for its “glint”.

The eROSITA Consortium has issued the survey's second data release (DR2), nearly doubling the previously known eROSITA X-ray sources to two million.

Over a decade ago, the Fermi satellite detected an excess of gamma-ray emissions in the galactic center. Potential explanations included Sgr. A*, the Milky Way's SMBH, pulsars, and even self-annihilating dark matter. There's no clear answer yet, since the region is so difficult to observe. But recent research shows that dark matter can't be ruled out.

JAXA's Martian Moon eXploration (MMX) will be on its way to Mars and Phobos next month. It will collect samples from Phobos and return them to Earth. A new morphodynamic atlas of the small moon will help scientists collect and understand the samples.

The James Webb Space Telescope (JWST) has opened up many wonders of the cosmos to scientists since it began its science operations a few years ago. But one thing that it hasn’t done is find an “exomoon”. These, as yet still theoretical, moons orbit exoplanets in other star systems, and JWST was supposed to find a plethora of them. However, so far it has found precisely none. It seems the cause is noise in the telescope’s instrumentation or noise from the star itself. But a new paper, available in pre-print form on arXiv from David Kipping, an astronomer at Columbia and also the host of the Cool Worlds YouTube Channel, shows how JWST can, in fact, find an exomoon. It likely just has to look for one in the same place repeatedly.

Ancient Swedish pagans had surprisingly accurate calendars and the ability to measure phases of the Moon to an incredible precision.

UK astronomers have uncovered new clues about the origin of 3I/Atlas – only the third known object from beyond our Solar System ever spotted in our cosmic neighbourhood.

Those "Little Red Dots" discovered by the James Webb Space Telescope, galaxies that existed during the very early Universe, could be sending neutrino particles that are reaching us today.

Astronomers observe faint light signals from stellar objects, study it intently, and try to understand what's behind these signals. In one case, the signals they detected masqueraded as an imminent supernova explosion. But more observations revealed a different reality.

Stephan's Quintet contains the most well-studied compact galaxy group. Japanese researchers have mapped star forming gas in the Quintet, along with its turbulence. The results show that the Quintet is an evolved group of interacting galaxies where gas struggles to settle down and form stars. Even where gas is concentrated, turbulence from interactions throttles star formation.

Astronomers have long searched for Dyson spheres as a sign of advanced alien civilizations. But if an alien civilization is dependent on advanced computing, we may be better served by looking for a Slysh halo.

We’ve been searching for life on Mars for a long time now, but so far we’ve come up empty. The fundamental problem is a Catch-22 of two of the key ingredients for life. Life as we know it needs liquid water and reasonable temperatures, both of which are available on Mars, but hardly ever at the same time. But a new paper from lead author Anna Bognar and her team at ELTE Eötvös Loránd University and the Konkoly Observatory describes a way for life to have access to both requirements at the same time - by hiding away in salt crystals.

The latest mission to the innermost planet in the solar system hit a milestone last week. After an eight year journey, BepiColombo finally separated from its propulsion stage to set itself up for an orbital insertion to Mercury. Taking place on September 3rd, the separation, which is part of a much longer series of logistical steps over the next few months, seemed to go without a hitch. But getting to that point was certainly a process, and still more challenges lie ahead.

A few hundred million years after the Big Bang, the first stars ignited - literally the “let there be light” moment for the universe. Now known to astronomers as Population III, or Pop III, stars, these giants were very different from the stars we know today. They were formed out of pristine hydrogen and helium, with almost no “metal” (i.e. other elements) holding them back. They were also huge, growing to tens to hundreds of times larger than the Sun. And they died young, in many cases collapsing into the universe’s earliest black holes. Some of those black holes even partnered up, eventually colliding into one another and creating gravitational waves that, if we have instruments sensitive enough, we could potentially detect. A new study led by astrophysicist N.V. Krishnendu of the University of Birmingham and their colleagues shows just how much we can learn about them with the new suite of gravitational detectors about to come online.

On Sunday July 5th, 2026, the Japan Aerospace Exploration Agency (JAXA) achieved the first-ever successful laser ranging experiment while making a flyby of an asteroid.

Did icy comets deliver water to the young Earth? That idea won't go away. Now, astronomers at Lund University in Sweden have found evidence of exocomets orbiting a young star named PDS 70. The observations suggest that these comets are delivering water to that system's inner regions.

What used to be a rare sight gracing the twilight sky is now becoming strangely commonplace. If you live on either U.S. coast, you have to good chance at seeing what’s become a common sky scene in our modern technocene era: a space launch jellyfish.

The Earth and the Moon have nearly identical isotopic compositions, and the Giant Impact Hypothesis strives to explain this. New research into the ancient impact shows how the temperature of both worlds, and how it affects the strength of the materials involved in the collision, shaped the outcome, including the isotopic compositions.

New observations find that a few supermassive black holes are unexpectedly large given the size of their galaxies. This suggests the connection between black holes and galaxies isn't as strong as we thought.

Halley’s comet captures the imagination in a way that few other astronomical objects do. When it last made its approach toward the Sun (admittedly when this author, who is now middle-aged, was one year old in 1986), humanity responded with a fleet of spacecraft known informally as the “Halley Armada”. Yet, because of the comet’s trajectory, those spacecraft were only able to visit their target for a fleeting few hours, leaving planetary scientists wanting more. Now, a new paper by researchers at Khalifa University and their co-authors, and available in pre-print on arXiv, describes a mission plan that would allow a spacecraft to actually rendezvous with this most well-known comet for the first time ever.

We know the universe is constantly expanding. We also know that gravitationally bound objects, such as solar systems and black holes, seem to be immune to that expansion. But a new paper, available in pre-print on arXiv by theoretical physicists Valerio Faraoni and Massimiliano Rinaldi challenges that assumption. They suggest that black holes can’t just ignore the expanding universe around them. Instead they have to expand along with it.

Say what you want about the changes to the space industry that’s happened over the past 10-20 years, but one thing is for certain - there are a lot more people that have access to space now than there ever has been before. Some of them have some absolutely crazy stories about how they got there, and plenty of those have written their own books about their experiences, before, during, and after their flight. Add to that list A Heart for Space by Dr. Eiman Jahangir - a cardiologist that officially became an astronaut when he crossed the Kármán line on a Blue Origin flight in August 2024. But the story of how an Iranian-American cardiologist made it all the way to space has lessons for anyone that hopes to follow in his footsteps.

We’ve said it before, and we’ll say it again - space is hard. Another example, albeit lacking in the destructive displays of some past examples, is China’s recent delay of its Chang’e-7 lunar mission. The agency announced the mission would miss its late-August launch window with a very brief press release from the China National Space Administration and the China Manned Space Engineering Office. While that means a slight delay in China’s plan for the Moon, it’s only a matter of time before the cornerstone of the robotic lunar exploration program is back on the launch pad.

A new image from NSF–DOE Vera C. Rubin Observatory offers a spectacularly deep view into a famous region of sky known as the COSMOS field.

Gaia has discovered three stellar mass black holes, each with a small stellar companion. For two of these systems the companions orbit closer that we would expect. Just how these systems form is a bit of a mysteries, but there are clues.

Astronomers have directly detected an extremely faint radio signal from hydrogen gas billions of light years away, demonstrating a powerful new way to map the Universe.

Future gravitational wave observatories will be able to see the gravitational waves of close-orbiting binary stars. A newly studied white dwarf system could be one of the first systems we observe.

Out in the solar system, there is a giant rippling curtain of charged particles that is actually the largest structure in our solar system. Known as the Heliospheric Current Sheet (HCS), it marks the spot where the sun flips its magnetic north and south poles, and grows directly out of giant, glowing loops of plasma on its surface called helmet streamers. However, so far, studies of it have only occurred near Earth, using space-based instruments such as SoHo and Wind. But now, a new paper from Keiichi Ogasawara of the Southwest Research Institute (SwRI) and his team used the joint ESA/NASA mission Solar Orbiter to capture the HCS at only about ⅓ the distance to Earth - before interactions with interstellar space and the solar wind change it. In other words, this paper represents the clearest ever picture of what the solar system’s largest coherent structure is actually made out of.

The planet Venus is arguably the most mischievous planetary body in the solar system. This is because like Saturn’s largest moon, Titan, Venus is shrouded in a thick atmosphere that can’t be viewed with optical telescopes and require radar images to see the surface. Unlike Titan, whose atmosphere looks quite dull, Venus’s swirling and awe-inspiring clouds give observers the impression that its surface is covered in wonderous features. However, the truth is far from ideal, as Venus’s surface is a living hell with searing temperatures and crushing pressures. But, unlike its surface and Titan, Venus’s atmosphere provides many more ideal conditions, even Earth-like conditions. But while life would be hard to exist on its surface, could we find life in the atmospheric clouds of Venus?

The newest DESI Legacy Imaging Surveys map covers three-quarters of the sky and catalogs nearly four billion objects. This publicly-available database contains stars, galaxies, supernovae, gravitational lenses, and much more.

The Sloan Digital Sky Survey (SDSS) has officially launched its twentieth data release (DR20), featuring updated data from multiple observations projects.

Pulsar Timing Arrays have been used to observe the background of gravitational waves in our galaxy. We aren't certain of their origin, but a new study shows a strong source could be early supermassive giants known as dark stars.

Cross-disciplinary research at Perimeter Institute and University of Maryland shows that dark photons could be lurking in more places than previously thought.

The Moon is busy in September. Coming off of eclipse season in August, the Moon visits no less than two planets, two bright stars and one open cluster in September, as it heads towards the Full Harvest Moon of 2026 on September 26th. No matter where on Earth you happen to be observing from this month, chances are, there’s an occultation of a bright celestial object by the Moon coming to a sky near you.

In 1992, Centaur 450P/LONEOS had a close encounter with Saturn, shifting its orbit closer to the Sun. Now astronomers can observe how a small icy body transforms into a comet over time.

Researchers at UCSB and UT Austin have determined that a galactic merger kicked a supermassive black hole into intergalactic space.

Researchers have figured out how to use lunar samples to determine the nature of volcanic activity on ancient Mercury. It's all based on SiO2, or silicon dioxide. Its abundance in a planet's crust reveals a lot about magma and volcanic activity.

Astronomers study dark matter through simulations of stellar streams around the Milky Way. They found that kinks and clumps within these streams aren't caused by dark matter clusters within the galactic halo.

Spacecraft famously have small bits of them disintegrate on reentry. That’s by design, as it is one of the easiest solutions to absorbing the incredible amounts of energy they experience. However, it also results in long turn around times while these heat shields are repaired, and the shields themselves act as “dead weight” limiting payload capacity. With the increased focus on reusable rockets, and the emphasis on payload capacity, engineers have been looking for alternative solutions to the reentry problem - and the one of the most promising is known as magnetohydrodynamic (MHD) braking. A new paper from researchers at the Tokyo Metropolitan University describes a new test setup that should help designers of these advanced braking systems truly capture what their system is doing upon reentry.

The search for dark matter has reached another milestone - in this case the start of science for one of the world’s newest detectors. The Super Cryogenic Dark Matter Search (SuperCDMS) SNOLAB just began its scientific operations in Ontario, and over the course of the next few years, hope to find direct evidence of “light” dark matter for the first time.

Keeping track of time in the universe is a difficult task. It’s constantly evolving and changing, and studying events that happened billions of years ago, while possible, isn’t exactly easy. A recent paper in the Monthly Notices of the Royal Astronomical Society from astronomers at The Ohio State University has unlocked a whole new way to tell time in space by using a new, perhaps unexpected element - manganese.

Dark matter is the invisible stuff that accounts for roughly 85% of the mass in the universe, and for decades, physicists have been trying to figure out what it's made of. Now an experimental facility located nearly a mile below ground in South Dakota has recorded a single interaction between subatomic particles that doesn't match what's expected from normal matter. Has a dark-matter particle been detected at last? It's too early to say, but the anomaly is definitely attracting attention from dark-matter detectives.

Extreme quasars near the dawn of time are giving astrophysicists clues to the formation of supermassive black holes.

If you visit the New Horizons mission website frequently, you'll notice that the spacecraft continues to generate excellent science as it plows its way through the Kuiper Belt. It recently woke up from its latest hibernation period in good health and is transmitting data it gathered back to Earth. The spacecraft, in addition to studying the Jupiter system in 2007, the Pluto system in 2015, and the Kuiper Belt Object Arrokoth in early 2019, has been doing some other fascinating solar system science since then thanks to two mission extensions in 2016 and 2023. Now, as a result of budget cuts at NASA, an important part of the NH science mission could end as early as October of this year.