Tuesday, August 11, 2026

Every Snowflake Needs a Speck of Dust and So Do Planets

A cut face of the Allende meteorite. The round grains are chondrules; the irregular white patches are calcium-aluminium-rich inclusions, the oldest solids in the Solar System.

A snowflake cannot form out of nothing. Water vapour will sit in the air quite happily, supercooled and reluctant, until it finds a speck of dust to build on and then it crystallises around it. Cosmochemists have had a version of that problem for decades. The early Solar System was a furnace of gas, and the first solid grains had to condense out of it somehow, yet condensing from a perfectly uniform gas is slow and difficult work. New research from Caltech, analysing fragments of a meteorite that fell over Mexico in 1969, suggests the seeds were already there. Buried inside the oldest solids we possess are specks of stardust from a star that lived and died before the Sun existed.



What If There's a Star Inside a Black Hole?

The shadow of the supermassive black hole at the centre of M87, the first ever directly imaged. We can photograph the boundary. What lies inside it remains a matter for the mathematics (Credit : Event Horizon Telescope Collaboration)

Ask what lies inside a black hole and the honest answer has always been a bit of a shrug and something about a singularity, a point where density becomes infinite and physics stops being able to tell you anything at all. It is the most unsatisfying answer in astrophysics, second only perhaps to what happened before the Big Bang. Now two theorists in China have produced a solution in which something else sits inside the horizon entirely, a neutron star, whole and intact, twelve kilometres across, its interior perfectly well behaved and apparently defying the laws of physics.



Watching the First Moments in a Star's Death

This artist's illustration shows a star exploding as a supernova. Astrophysicists caught the shock break out from a supernova 500 million light years away, the first indication of a massive stellar explosion. By detecting the break out, researchers were able to learn a lot about the progenitor and its surroundings. Image Credit: NASA/Swift/Skyworks Digital/Dana Berry

Astronomers were fortunate when the Einstein Probe detected the difficult-to-observe initial shock break out (SBO) from a supernova. The SBO is the first electromagnetic indication that a star is going to explode, and by observing it and the aftermath, researchers were able to determine what type of progenitor star exploded, and what it's pre-explosion environment was like.



Monday, August 10, 2026

The Odds of Finding Water on Mars

A cross section of buried Martian ice, exposed in bright blue where a steep slope has eroded away. HiRISE on Mars Reconnaissance Orbiter caught this one at 56 degrees south, the right latitude for ice, the wrong one for astronauts (Credit : NASA/JPL-Caltech/UA/USGS)

Mars has plenty of water, and almost all of it is in the wrong place. The poles are rich in ice, the equator, where you would actually want to land, has none within reach. That leaves the mid-latitudes, and until now the honest answer about what lies beneath them has been a bit of a shrug. Two new studies from the Planetary Science Institute have changed the shape of that answer. Rather than simply asking whether the data are consistent with buried ice, they have started calculating the odds and can now say, of a given patch of Martian ground, that there is a 64 per cent chance of finding ice if you dig there.



The Telescope That Points Itself

The Víctor M. Blanco 4 metre Telescope at Cerro Tololo, Chile. For two observing campaigns this year, the decisions about where to point it were made by a machine (Credit : CTIO/NOIRLab/NSF/AURA)

Time on a large professional telescope is one of the scarcest resources in science. Astronomers wait months for a few hours, and every one of those hours is a running argument with the weather, the Moon and the atmosphere. Point at the wrong target at the wrong moment and the data comes back soft, washed out, or useless, with the next chance half a year away. A team has now handed that argument to a machine. Their system was trained not on the rules astronomers use but on what astronomers actually did, night after night, for years.



Interstellar Travel III: Antimatter to the Rescue?

Vacuum to Antimatter-Rocket Interstellar Explorer System (VARIES) concept artwork. Credit and ©: Adrian Mann.

With the end of the Space Age and the winding down of the Cold War, scientists again returned to the question of interstellar flight. Having failed to realize a working concept that could be realized in the near term, more exotic ideas began to be considered, reflecting further breakthroughs in theoretical physics.



Ancient Maltese Seafarers Likely Navigated By The Stars

Sunset over the present-day main island of Malta.  Credit:  Bruce Dorminey

Ancient Maltese seafarers had both a complex cosmology and likely at least rudimentary skills in celestial navigation. It's thought that they used stars in the southern constellation of Crux to make their way around the south-central Mediterranean.



Sunday, August 9, 2026

NASA's MAVEN Illuminates New Understanding of Auroras at Mars

This illustration depicts charged particles from a solar storm stripping away charged particles of Mars' atmosphere, one of the processes of Martian atmosphere loss studied by NASA's MAVEN mission.
Credit: NASA/GSFC

NASA MAVEN (Mars Atmosphere and Volatile Evolution) mission scientists have uncovered a key puzzle piece in understanding certain types of auroras on Mars, finding that they form in a similar way to Earth-based auroras.



Friday, August 7, 2026

SpaceX Junk Hits the Moon. Not a Good Sign

Still pic of animation video of the SpaceX upper stage striking the lunar surface. Credit: NASASpaceNews

The spent upper stage from a SpaceX Falcon 9 rocket has struck the Moon, illustrating the hazard posed by debris in cislunar space. This problem will increase as launches to orbit and to the Moon become more common in the coming years.



Astronomers Find a New Object from the Early Universe Using Webb Data

The MACS J0308.9+2645 cluster, as captured by Webb's Near-Infrared Camera (NIRCam). Credit: NASA/ESA/CSA/STScI

Homer Dávila Gutierrez, director of SKYCR.ORG, has identified a gravitational arc candidate in the galaxy cluster MACS J0308.9+2645 from public data from the James Webb Space Telescope. The object had not been previously reported and is located at a photometric redshift close to 4.4. The preprint is available on arXiv and the manuscript is under review in Publications of the Astronomical Society of Japan.



Preview to Totality: A Resource Guide to August 12th Total Solar Eclipse

Totality as seen from western Australia in 2023. Credit: Eliot Herman.

It’s almost show time. We’re just a few days away now, from the only total solar eclipse of 2026. While eclipses are a surety as the celestial gears of the Universe grind on, there are always a few unknowns leading up to eclipse day. We wrote a recent guide to the upcoming total solar eclipse featuring totality across Greenland, Iceland, the North Atlantic and Spain on August 12th. As that date is now only a few days away, it’s a good time to look at prospects and resources to have at the ready leading up to eclipse day.



Thursday, August 6, 2026

Scientists Watch as a Distant World's Atmosphere Shrinks and Thins

A New Horizons parting shot of Pluto's thin, hazy atmosphere as it appeared in 2015. Scientists are measuring starlight as it streams through the atmosphere to get information about how the blanket of nitrogen and other gases is changing as Pluto moves farther from the Sun. Courtesy New Horizons, NASA. Public domain.

As dwarf planet Pluto moves along in its distant, high-obliquity 248-year orbit, its atmosphere is changing. That's because it's beginning to travel through colder, darker parts of the outer Solar System for the next 88 years. As a consequence, the mostly-nitrogen atmosphere is expected to grow gradually thinner and eventually freeze out over the coming decades. When that happens, the atmosphere will shrink.



Tuesday, August 4, 2026

Scientist Constructs "Big Picture" of Mars Water from Rover Data

A pictorial history of water on Mars by space artist Michael Carroll. This is based on Viking data and work done at NASA Ames. A study of rover measurements of water-related minerals on the Red Planet shows that water may well have been more widespread than previously thought. Courtesy Michael Carroll, public domain.

Rover data from more than 20 years ago has revealed clues to the existence of liquid water on ancient Mars. The NASA Spirit Rover carried a specialized instrument called a Mössbauer Spectrometer that performed mineralogical analyses of soil, rock, and dust on the surface of the Red Planet at Gusev Crater. Individual measurements didn't always indicate definitive proof of water, but when scientist Paolo de Souza of Edith Cowan University in Australia examined years' worth of measurements together, a definite pattern began to show up in the existence of minerals that could only exist in the presence of water. His analysis shows that Mars used to sport a lot more water than scientists expected and that the data showing its existence was in the data all along.



Venus Isn't Dead After All

There are huge rift valleys on Venus. They suggest that the planet is still geologically active. Credit: NASA/JPL/USGS

Simulations conducted by researchers at ETH Zurich suggest a strong likelihood that Venus’s rift valleys are still geologically active rather than being mere relics of a bygone era, as had been previously believed. This finding reshapes our understanding of Earth’s sister planet and will influence future missions to Venus.



See the Perseid Meteors on a New Moon Year

A composite of the 2016 Perseids over Arizona. Credit: Rob Sparks.

You couldn’t ask for a better year for one of the top annual meteor showers. If skies are clear be sure to watch for one of the top skywatching draws of 2026: the August Perseid meteor shower. While the Perseids are a draw on any year, 2026 is special, and has a few things going for it in terms of the Moon phase, peak timing and prospects.



Monday, August 3, 2026

Interstellar Travel: the Birth of Fusion Drives

Logarithmic map of the Solar System and its closest stellar neighbors. Credit: Pablo Carlos Budassi

During the Space Age and Cold War, fusion-powered spacecraft systems were investigated as a possible means of reaching another star system within a human lifetime. Many of the proposed ideas are still on the table today, waiting for future advancements to make them realizable.



Zodiacal Dust in Exoplanetary Systems Could Hinder Our Search For Life On Other Worlds

A column of zodiacal light stretches skyward beyond Mount Teide in the Canary Islands. Credit: StarryEarth, CC BY-NC 2.0

Most exoplanetary systems have a plane of dust similar to the zodiacal dust of our solar system. This dust absorbs some of the very light we use to find biosignatures in exoplanet atmospheres, and could make our search for life more challenging.



Friday, July 31, 2026

Smashed Ice Worlds Formed Neptune's Inner Moons and Rings

Diagram illustrating the formation and evolution of Neptune's current moon system. (Credit: Davis et al. (2026))

The planet Neptune has 16 known moons, with its largest Moon, Triton, comprising more than 99.5 percent of the mass of all of them. Triton’s incredible size has led scientists to hypothesize it was a captured object originating from the Kuiper Belt, which wreaked havoc on Neptune’s original moon system upon its capture and subsequential elliptical orbit. Today, some remnants of these original moons are part of the dusty rings that orbit Neptune. But what did that original moon system consist of? Were they the same small worlds observed today or are they pieces of what was once much larger worlds?



Interstellar Travel: The Space Age and Nuclear Rockets

Given time and the right kind of commitment, could the dream of interstellar travel become a reality? Credit:

Given the state of our technology, it would take a spacecraft a ridiculously long time to reach even the nearest star in our galaxy. However, scientists continue to ponder ways in which we could achieve the dream of interstellar spaceflight. Here are a few of their best ideas.



Astronomers Measure the Long Reach of a Quasar

Schematic illustration of the hierarchical structure of the Universe, from a galaxy group (a collection of galaxies) to an individual galaxy and the supermassive black hole at its center. Although a black hole is more than 100 million times smaller than the radius of its host galaxy, it plays a crucial role in the galaxy's central region. ©Tohoku University

There are a number of things in the Universe that could wipe out life as we know it, but — for now, and for Earth — a blast from our galaxy's supermassive black hole isn't one of them. That's not to say that Sagittarius A* doesn't pose a danger. If it wakes up someday and blasts out a strong wind, that definitely could affect Earth. It could well have powered a quasar in the past, and could do so again.



Thursday, July 30, 2026

Mercury's Weak Magnetic Field Periodically Traps Solar Wind

Image of Mercury taken by NASA's MESSENGER spacecraft. (Credit: NASA, Johns Hopkins University Applied Physics Laboratory, and the Carnegie Institution of Washington)

The planet Mercury is the first planet from the Sun but also one shrouded in mystery. This is primarily due to the limited number of spacecrafts that have visited it, but this limited data has provided scientists with new and exciting characteristics previously thought impossible. One fascinating aspect is its magnetic field, which was first discovered in March 1974, which both surprised and puzzled scientists due to the planet’s small size, which is measured at about half the size of the continental United States from coast to coast.



What Killed Galaxies in the Early Universe?

An artist’s impression of the galaxy CRISTAL-02, with a huge plume of cold gas extending away from it. This plume is almost as long as the galaxy itself, which is a telltale sign that gas is being driven out of the galaxy. Credit Joshua Worth via Creative Commons CC-BY license
Licence type Attribution (CC BY 4.0)

Galaxies in the infancy of the Universe are the building blocks of more modern galaxies. They began as small "shreds" of material that coalesced over time to form larger ones. That's why astronomers use observatories such as the James Webb Space Telescope (JWST) to study the young Universe. The light from those early objects appears in the infrared part of the spectrum, which JWST is tuned to see.



Radio Array Detects Polarized Light From a GRB

This illustration depicts Faraday rotation in the afterglow of a gamma-ray burst. A powerful jet (upper left) sends polarized radio waves outward through the thin wall of a surrounding bubble of magnetized gas called an HII region. As the light passes through this material, its polarization angle is twisted by the magnetic field. Because the effect is stronger at longer wavelengths, the red and blue waves, which represent different radio wavelengths, exit the bubble oscillating in different directions. By measuring this difference, astronomers were able to map the magnetic environment surrounding GRB 260310A for the first time. Credit: NSF/AUI/NSF NRAO/M.Weiss

On March 10, 2026, the Fermi telescope gamma-ray burst team reported the detection of a long-duration gamma ray burst that occurred when a star exploded inside a dense, highly magnetized cloud of hydrogen gas. That HII region is a bubble of ionized hydrogen created by winds from a massive young star. Astronomers immediately turned as many telescopes as possible to view the burst and its afterglow, including the NSF's Karl Jansky Very Large Array.



Wednesday, July 29, 2026

The Risks of Debris Between the Earth and the Moon for Future Exploration

Diagram of the flight path and retrograde orbit of the Artemis I mission that took it around the Moon. Credit: NASA

A new study from the Chinese Academy of Sciences (CAS) addresses the threat of debris in cislunar space, which could pose threats for future missions bound for the Moon.



Radio Astronomy is Getting a Big Boost from the VLA's New Sky Survey

The Karl G. Jansky Very Large Array in New Mexico. The VLA was upgraded in recent years, and its new sky survey is complete. It's the most detailed radio survey of the sky ever taken. Image Credit: By user:Hajor - Own work, CC BY-SA 3.0, https://commons.wikimedia.org/w/index.php?curid=138997

The National Radio Astronomy Observatory has completed a new survey with the updated Karl G. Jansky Very Large Array (VLA) in New Mexico. It's called the VLASS, the Very Large Array Sky Survey, and it's the most detailed radio survey of the sky ever completed. The VLA used the power of its 28 movable dishes to complete the survey.



White Dwarfs Eat More Planetary Debris Than Thought, But Magnetic Fields Hide It

This artist's illustration shows a white dwarf surrounded by a debris disk. Astronomers are finding more and more white dwarfs with metallic debris disks, which suggests the debris comes from planetary systems. New research examines how white dwarfs accrete this debris, showing that it's much more common than thought, and that white dwarfs accrete more planetary debris than thought. Image Credit: NASA, ESA, and G. Bacon (STScI)

Planetary debris disks around white dwarfs appear to be more plentiful than thought. That's because some white dwarfs are magnetic, and those magnetic fields create patches of metallic debris near the stars' poles, where it's more difficult to detect. This leads to an underestimation of debris, something new research is trying to correct.



Tuesday, July 28, 2026

A Wandering Black Hole Meets a Wandering Star

Artist's conception of a tidal disruption event that occurs when a star wanders too close to a supermassive black hole. Courtesy NRAO/AUI/NSF/NASA Hill

What happens when a black hole and a star meet in the middle of nowhere in a galaxy? It sounds like it could be a dramatic science fiction backdrop, with some hapless starship caught in the crunch. Actually, such encounters in real life are pretty rare. They happen maybe once every 100,000 years. But, when they do occur, the immense gravity of the supermassive black hole tears the star apart. It's an eerie-looking process. The star gets "spaghettified" — that is, pulled on one side by the black hole. That rips out a stream of gas from the star which eventually forms a disk around the black hole.



Samples of Lunar Rock Are Leading Scientists to Rethink the Moon's History

Image of the far side of the Moon taken by NASA's Lunar Reconnaissance Orbiter (LRO). Credit: NASA

Based on a new analysis of the Chang'e-6 lunar samples, scientists are again questioning the timing and intensity of the Late Heavy Bombardment period.



Astrobiology Offers Crucial Window Onto Earth’s Distant Past And Future

This artist's concept shows what the TRAPPIST-1 planetary system may look like, based on available data about the planets' diameters, masses and distances from the host star, as of February 2018.
NASA/JPL-Caltech

The search for extrasolar rocky planets circling other stars is more than mere science. It offers researchers a chance to gain crucial insight into how our own planet functions.



Galaxy Mergers May Not Stifle Star Formation After All, According to Illustris TNG

The JWST captured this image of a pair of merging galaxies named Arp 107. New simulations show that mergers like this, which are common, are not responsible for quenching galaxies. This contradicts the current understanding of galaxy mergers where a merger creates a powerful quasar that then stifles star formation. Image Credit: NASA, ESA, CSA, STScI

In recent years, the idea that galaxy mergers are responsible for quenching galaxies has grown in importance. This paradigm says that galaxies merge, their black holes form a powerful quasar, and that quasar stifles star formation. But new results from the IllustrisTNG simulations shows that this paradigm may not be accurate.



Martian Space Suits Will Need To Be 40% Lighter

Artist's concept of an astronaut working on Mars. Credit - NASA

Long before a human ever sets foot on the Red Planet, we already know how hard the environment is. Once one finally does, the only things protecting them from that harsh environment will be the infrastructure we’ve built up there, and the spacesuit that keeps that in a protective bubble. Unfortunately, modern space suits aren’t built with Martian gravity, which is 3/8ths of Earth’s, in mind. To prove that point, a team of NASA and industry engineers made a presentation at the 55th International Conference on Environmental Systems (ICES) that showed that the newest generation of spacesuits are simply too heavy to use on Mars.



Monday, July 27, 2026

JWST Could Spot Volcanic "Exo-Ios" Around Super-Jupiters

Artist's concept of SIMP 0136+0933 and its aurorae. (Credits: NASA, ESA, CSA, and Joseph Olmsted (STScI))

Jupiter’s moon, Io, is the most volcanically active planetary body in the solar system, boasting hundreds of active volcanoes spewing molten lava into space. This occurs from a process called tidal heating where Jupiter’s massive gravity constantly stretches and compresses the much smaller moon during the latter’s non-circular orbit. However, a lesser-known fact is that Io’s volcanic gases fuel Jupiter’s aurorae by traveling along Jupiter’s magnetic field lines, resulting in Jupiter’s bright aurorae observed by spacecraft and Earth-based telescopes. But what if this same phenomenon could be used to detect Io-like exomoons, also called exo-Ios, orbiting Jupiter-like exoplanets?



Chang'e-6 Samples Provide an Ancient Record of the Moon's Far Side.

Schematic illustration of the contrasting solar wind environments experienced by the lunar nearside and farside under the influence of Earth's magnetosphere. Credit: Zhang, X. et al. (2026)

The samples returned by the Chang'e-6 mission from the far side of the Moon reveal that the two hemispheres have had rather different experiences when it comes to space weather.



Little Red Dots Could Be Ancient Globular Clusters, Each Dominated by a Super-Massive Star

One of the JWST's confounding Little Red Dots is in the left panel, while the globular cluster (GC) 47 Tucanae occupies the right panel. Could these objects be the same thing at different points in evolution? Image Credit: NASA, ESA, CSA, STScI, Dale Kocevski/Colby College, ESO.

Little Red Dots are one of the mysteries uncovered by the JWST. Astronomers have been trying to figure out what they are, and have come up with multiple possibilities. New research says they could be ancient Globular Clusters with supermassive stars in their centers.



How NASA Plans to Build the Habitable Worlds Observatory

Artist's rendering of the HWO. Credit - NASA's Goddard Space Flight Center Conceptual Image Lab

We’ve been covering the journey of the Habitable Worlds Observatory for some time now. Over the past few years, it's gone from a proposal to a relatively fleshed-out plan for how and what the next Great Observatory should do—in this case, look at and characterize potentially habitable exoplanets. Back in August 2024, NASA set up the HWO Technology Maturation Project Office (TMPO) to coordinate the technological and scientific development needed to make the mission a success. They recently released a comprehensive plan for the first steps of that process in pre-print form on arXiv, and it’s very clear on what needs to happen before the Mission Concept Review (MCR) at the end of the decade.



Sunday, July 26, 2026

Black Hole Collisions Tell a Tale of Repeating Mergers

GW250114, a powerful collision between two black holes recently observed in gravitational waves. Scientists are studying black holes to find out if they are "first-generation" or "second-generation" creations made during collisions. Credits: Image credit: Aurore Simonnet (SSU/EdEon)/LVK/URI

A black hole merger is one of the Universe's most energetic and massive events. During such a collision, two black holes orbit closer and closer until they collide and become a much more massive black hole. The event also gives off radiation and, as it happens, gravitational waves. They help tell the story of the two objects involved in the collision.



New Research Shows How Clouds Shape the Interiors of sub-Neptunes

An artist's representation of two scenarios for a sub-Neptune planet's atmosphere-interior interface. Credit: Hailey Nelson/ASU

Scientists at ASU's School of Earth and Space Exploration have demonstrated how clouds in a sub-Neptune's atmosphere shape the interior structure of the planet.



UCF Researchers Are Developing Tools to Help Find Habitable Planets

Visualization of the Habitable World's Observatory (HWO). Credit: NASA SVS/Jonathan North

Through the Photonics-Enabled Exoplanet Spectroscopic System (PEEPSS) program, researchers are developing a technology that will assist NASA's planned Habitable World's Observatory (HWO).



Are Aliens Harvesting the Spin of Stars?

Artist's impression of a star that might eventually become a magnetar. Credit - ESO/L. Calçada

One of the challenges of searching for “technosignatures” (i.e. signs that intelligent life somewhere in the universe has created technology) is understanding what to look for. Technology is a very broad area, and different types would show up as different features. One of the most commonly cited is a Dyson sphere, which attempts to encapsulate a star and capture it’s outgoing light to produce energy. But while we’ve looked for the mid-infrared waste heat these structures would produce for decades, we haven’t found a definitive instance of one. According to a new paper, available in pre-print on arXiv by Turkish high school student Sahin Torlakcik, that might be because we are looking for the wrong type of energy all together.



Saturday, July 25, 2026

JWST May Be Missing Water Hidden Deep Within Mini-Neptune Worlds

Artist's illustration of the sub-Neptune exoplanet, TOI-270 d. (Credit: NASA)

Sub-Neptune exoplanets, exoplanets that are slightly smaller than Neptune, have been designated as the most common type of planet in the Milky Way Galaxy based on their vast discovery numbers, totaling almost 3,300 out of the more than 6,300 confirmed exoplanets to date. Despite these numbers, the characteristics of sub-Neptunes remain relatively unknown. This is primarily due to our own solar system not having its own sub-Neptune to use as an analog, along with their atmospheres being thick and hazy. As a result, this makes telescopic observations, even from powerful instruments like NASA’s James Webb Space Telescope, extremely difficult.



Friday, July 24, 2026

New Images Reveal the Stunning Properties of the Black Hole at the Center of M87

The Black Hole at the Center of the super-giant elliptical galaxy M87. Credit: Event Horizon Telescope Collaboration

Researchers from the Shanghai Astronomical Observatory of the Chinese Academy of Sciences, together with international collaborators, carried out the first spatially resolved dual-frequency spectral study of the M87 black hole using observations obtained in 2018 with the Event Horizon Telescope (EHT) and the Global Millimeter VLBI Array (GMVA).



Are We Missing Alien Lighthouses?

Glowing beams from the 4 Laser Guide Star Facility. Credit - ESO/P. Horálek

Searching for extraterrestrial intelligence has so far meant primarily focusing on one particular type of signal - and that signal has normally been based on what our own current cutting edge technology is. But what if that’s the wrong way to look for signs of an alien intelligence? What if a resource-conscious civilization decided it was too complicated to send femto-second lasers in high energy bursts out across the universe. A new paper, available in pre-print on arXiv, from researchers Dániel Apai, Chia-Lung Lin, and Kevin Wagner, suggest that might actually be what happens, and that we should start looking for long-duration pulsing interstellar beacons.



Juno Measures the Heat Below Io's Restless Surface

The JunoCam instrument captured this image of the volcanic moon Io during Juno's flyby in December 2023. During this and the next flyby in February 2024, Juno used its Microwave Radiometer instrument to meausure the heat several meters under the moon's surface. Image Credit: NASA/JPL-Caltech/SwRI/MSSS. Image processing by Gerald Eichstädt

Juno's Microwave Radiometer (MWR) was built peer deep down into Jupiter's massive atmosphere. But during the spacecraft's extended mission, it's been studying the Galilean moons. During two flybys of volcanic Io, the spacecraft its MWR to measure the heat flowing from deep within the moon.



Mars Express Captures 'Metallic' Waves Rolling Across an Ancient Martian Crater

Image of the Kaiser crater taking by Mars Express. Credit - ESA/DLR/FU Berlin

When we think of Mars as the “Red Planet”, the image that comes to mind is just that - a lot of red. That comes from the oxidization of the dust and rocks that cover the planet's surface, but there are some instances where the Red Planet still has a few visual tricks up its sleeve. One such trick was recently captured by the European Space Agency’s venerable Mars Express orbiter, which captured what seems to be a set of metallic waves inside a giant impact basin. But on closer inspection, it becomes clear they aren’t liquid metal or some sort of alien architecture, but a manifestation of Mars’ complex environment.



Thursday, July 23, 2026

Spin-Reversing Comet May Face Self-Destruction

Artist’s illustration of comet 41P, measured at about 1 kilometer (0.6 miles) in diameter, depicted approaching the Sun, resulting in outgassing from the evaporating ice. (Illustration Credit: NASA, ESA, CSA, Ralf Crawford (STScI)

Comets are known for providing breathtaking observations of their long and shiny tails when they travel too close to the Sun. This happens because comets are made of ice and primarily orbit far from the Sun, but as their icy core heats up it evaporates, resulting in the aforementioned breathtaking observations. But while evaporating comets make for great public photos, scientists who study comets are focused on these snowballs of gas and dust and how they are remnants of the origins of the solar system about 4.6 billion years ago.



Hubble Discovers the First "Missing" Black Hole in this Famous Star Cluster

Astronomers found Omega Centauri’s first stellar-mass black hole, which has a visible star companion that is shown in greater detail. Credit: ESA/NASA/MPIA/STScI

Combining over 20 years of archival data from Hubble with new data from the James Webb Space Telescope, a team of astronomers has found the first of the "missing" black holes.



Chandrasekhar and the Limits of Physics, Part 4: Vindication

The remnant of Tycho's supernova, a Type Ia explosion, in X-ray light. Such blasts happen when a white dwarf reaches the Chandrasekhar limit. Credit: NASA / Wikimedia Commons (public domain).

The collapsing stars Eddington swore couldn't exist turned out to be everywhere, and half a century later the world handed Chandrasekhar his Nobel. How the 1.4 solar mass limit became one of the most important numbers in modern astronomy.



Probing the Universe's Missing Matter With Mysterious Fast Radio Bursts

This illustration shows a Fast Radio Burst form a distant galaxy reaching Earth. In new work, researchers used thousands of FRBs to probe the Universe for its missing matter. Image Credit: ESO/M. Kornmesser

Astronomers aren't certain where Fast Radio Bursts come from. But they still have utility. They can use them to find the Universe's "missing matter."



Wednesday, July 22, 2026

The Milky Way Flipped its Disk Billions of Years Ago

The Milky Way in the sky over the ESO's La Silla Observatory in Chile's Atacama Desert. The Milky Way's thick disk is full of older stars and rotates more slowly than its thin disk, which is full of younger stars. New research says a cosmic flip is responsible for this puzzling arrangement. Image Credit: ESO/B. Tafreshi (twanight.org)

The Milky Way has two disks, the thin disk where most of the stars dwell, and the thick disk, populated by much older stars. The ESA's Gaia mission showed us that the thick disk rotates more slowly than the thin disk. The culprit, according to powerful simulations, was a disk flip in the MW's past, driven by a merger.



Tuesday, July 21, 2026

Electrically Charged Mars Storms Threaten Future Exploration

Orbital image of the global dust storm occurring in Martian Year 34 (mid-2018), which enveloped the entire Red Planet. (Credit: NASA/ESU)

Martian dust storms are some of the most fascinating and mysterious planetary surface processes ever observed, as Earth, Mars, and Saturn’s moon Titan are the only known planetary bodies to have active dust storms. However, the major difference for Mars is its dust storms can blanket the entire planet at once, resulting in the surface becoming completely unobservable and blocking out sunlight, with the scientific community concerned this might hinder robotic, and even human, space exploration. But what if covering the surface and blocking sunlight wasn’t the only issue Martian global dust storms pose for future missions?