Saturday, October 31, 2026

Martian Polar Crater Ice Shifts with Seasonal Frost

NASA MRO HiRISE image of a north polar crater. (Credit: NASA/JPL-Caltech/Univ. of Arizona)

The planet Mars shares many landforms and weather patterns with the Earth, including changing seasons, volcanoes, canyons, dust storms and dust devils, and water ice. But one feature that Earth and Mars share among the eight planets in our solar system are polar ice caps. Both are one of each planet’s striking features, but the major difference is while Earth’s polar ice caps are both comprised of water, Mars’ north polar ice cap is only comprised of water while its southern polar ice cap is carbon dioxide. The reasons for this are determined by altitude, but Mars’ northern polar ice cap is one of the most studied regions primarily due to its water ice composition. But how does the north polar ice cap water ice change with the seasons compared to Earth, and what can this teach scientists about Mars’ climate history?



Ceres' Water Ice Can Mask Massive Surface Salt Deposits

Bright spots in Occator Crater on Ceres. (Credit: NASA / JPL-Caltech / UCLA / Max Planck Institute for Solar System Studies / German Aerospace Center / IDA / Planetary Science Institute)

The dwarf planet Ceres is arguably one of the most overlooked and underappreciated planetary objects in the entire solar system. This could be because while Ceres has the same dwarf planet designation as Pluto, Ceres is largely considered an “asteroid” since it resides the in main asteroid belt. However, along with being the largest object in the main asteroid belt, Ceres’ mass comprises between 25 to 30 percent of all the mass of the entire main asteroid belt. Despite its lack of recognition, Ceres’ interior is layered like most rocky planets, including Pluto, and its surface displays evidence of past water ice activity (also called cryovolcanism) with several “bright spots”, which are highly reflective salt deposits. But what can these salt deposits teach scientists about Ceres’ formation and evolution?



Space Outposts Beyond the Moon May Rely on Planetary AI

A conceptual AI visualization mapping lunar environmental data layers to identify target landing sites. (Credit: The Ohio State University)

NASA plans to return astronauts to the lunar surface in 2028 for the first time since Apollo 17 in 1972. But the famed agency has no intention of stopping there, as they plan to establish a permanent human presence on the Moon through a slow and meticulous process involving power, resource extraction, and habitat technologies. However, with the soaring use of artificial intelligence (AI) in our everyday lives, how could this emerging technology be used to identify new landing sites for future outposts on the Moon and possibly Mars?



Friday, October 30, 2026

Hera Probe Sees Asteroid Pair Separately for First Time

Hera's first image of the binary asteroid, Didymos and Dimorphos. (Credit: ESA)

Planetary defense is a growing concern among the scientific community, as efforts have been made to design and implement missions meant to deflect incoming threats to the Earth well in advance. In 2022, NASA intentionally collided the Double Asteroid Redirection test (DART) planetary defense spacecraft into the smaller asteroid of the binary asteroid, Didymos and Dimorphos, with the latter being the smaller one. While the goal was to ascertain if deflecting an asteroid is feasible, how did this influence the geological characteristics of Dimorphos, and what can it teach us about planetary defense missions?



What Could Split a Black Hole in Two?

Black holes collide more easily than they break apart. Scientists are studying possible ways that these behemoths could fragment under certain circumstances. Credit: NASA/ESA/STScI

We all know that black holes can collide. It has happened since black holes began to form, early in cosmic time. The result is always a clash that gives off gravitational waves and a giant bang. Since black holes have such strong gravity, it's almost impossible to imagine a way that any force could break one apart. Yet, that's the task that a group of scientists in Europe set for themselves.



Queen's University Belfast Students Find Neptune's Elusive Trojan Asteroids

Artist's Rendition of Neptune's Trojan populations, with a close-up of one such object. Credit: FlyAzure/J.Murtagh/NASA/JAXA

Astronomers at Queen’s University Belfast have led an international team studying new solar system bodies near Neptune, helping to unravel the mysteries of our solar system’s evolution.



This Ancient Meteorite Hints at Mars' Warm, Wet Past

This image shows a group of meteorite hunters in the Sahara Desert. Nomadic people from the region have become expert meteorite hunters, finding hundreds of them, which are typically recovered as groups of fragments. One found in Mali in 2022 has proven to be almost as old as Mars itself, one of the most ancient pieces of Mars ever recovered. Image Credit: University of New Mexico.

Ancient Martian meteorites are like time-capsules from the planet's past. They're delivered to us by impacts that launch them into space, where some of them find their way to Earth. One recently discovered meteorite found in the Sahara desert adds weight to the idea that Mars was once warm and wet, and possibly habitable.



Thursday, October 29, 2026

Examining the Cat's Head Nebula with the Hubble and JWST

The Cat's Head Nebula proudly rises in this Hubble Space Telescope image. It's a star-forming region within the larger Carina Nebula, an even larger star-forming region. Recently, both the Hubble and the JWST imaged the Cat's Head as part of the ongoing scientific effort to understand the complex process of star formation. Image Credit: NASA, ESA, STScI. Image Processing: J. Depasquale (STScI).

Star formation is a complicated process. It involves metallicity, gas temperature and density, dust grains, and stellar feedback from existing stars. Sometimes, studying all these factors and how they work means studying some of Nature's most beautiful structures, like the Cat's Head nebula in the Carina Nebula.



A Brief-ish History of METI. Part II: From Interplanetary to Interstellar

The legacy of Arecibo's nearly 60 years of radio astronomy is strong even after its loss in a tragic 2020 collapse. Among its major accomplishments was hosting the first attempt at Messaging Extraterrestrial Intelligence (METI). Credit: University of Central Florida

The latter half of the 20th century saw a major expansion of the Search for Extraterrestrial Intelligence (SETI), accompanied by corresponding advances in Messaging Extraterrestrial Intelligence (METI). A key development was the first interstellar SETI and METI experiments: Project Ozma and the Arecibo Message.



No Comets Required? How the Growing Earth May Have Created Its Own Water

This illustration shows a rain of molten pebbles falling onto a molten Earth. New research and lab experiments show how iron oxide in these pebbles could've been reduced in Earth's ancient atmosphere, forming water vapour. Image Credit: University of New Mexico/Garai et al. 2026. NatGeo

Earth may not have needed comets and asteroids to deliver its water after it formed and cooled. Instead, water creation could have been part of the planet's formation process. New research explains how, and even shows that water creation could be a part of every rocky planet's formation.



Wednesday, October 28, 2026

Moon Habitats May Use Layered Mylar to Block Extreme Heat

Researchers at Penn Engineering demonstrate the flexibility and durability of stacked Mylar insulating layers, shown held between gloved fingers for scale. (Credit: Bargatin Lab)

Living on the Moon, with either trained astronauts or regular civilians, could become a regular occurrence in the near future. However, it’s easier said than done, as scientists and engineers continue developing new and advanced ways for protecting humans in the harsh lunar environment, which contrasts the mild and habitable temperatures of the Earth. The most important aspect is focusing on keeping humans alive, and this includes temperature regulation within the habitats. However, how can you maintain temperature regulation while being flexible enough to withstand physical changes like moving, handling, and compression and expansion?



NASA's New UV Space Telescope Will Launch in 2031

This artist's illustration shows NASA's UVEX (UltraViolet EXplorer) space telescope. Scheduled to launch in 2031, UVEX will perform a sky survey in Ultraviolet, complementing other sky surveys like the Nancy Grace Roman's surveys, and the ESA's Euclid surveys. Image Credit: SDL/NASA/JPL-Caltech

NASA has committed to launching a new, more powerful UV space telescope. Named UVEX, the UltraViolet EXplorer, it will launch in 2031. It's about 100 times more powerful than its predecessor, GALEX, whose mission ended in 2013. UVEX will perform a survey in UV that will complement infrared surveys by other telescopes.



Betelgeuse Is Disturbed By Its Companion Star

This artist's illustration shows the smaller, hotter companion star Siwarha creating a wake-like disruption in Betelgeuse's outer atmosphere. Credit: NSF/AUI/NSF NRAO/M. Weiss

Betelgeuse has a close-orbiting companion that disturbs the red supergiant into an egg-like shape. New observations show how the two stars interact and how this could help explain the varying brightness of Betelgeuse.



Ancient Comets Carried Organic Compounds, But They Didn't Survive Crashing Into Earth

This artist's illustration shows an ancient comet smashing into the ancient Earth. Scientists have wondered if comets could have delivered life's essential building blocks to our young planet, since we now know that comets carry organic molecules important for prebiotic chemistry. But new research says this picture is unlikely. Image Credit: Scarlett White

Perhaps the biggest mystery we face is life on Earth started. One hypothesis says that comets, which are known to carry important chemicals in abiogenesis, delivered these compounds to Earth, leading to the appearance of life. But new research concludes that that is highly unlikely.



Tuesday, October 27, 2026

NASA Systems Engineering Team Details HWO Mission Architecture

Illustration depicting the different Exploratory Analytic Case (EAC) designs, with EAC1 (a), EAC2 (b), and EAC3 (c). (Credit: Liu et al. (2026))

Finding an Earth-like world beyond the solar system is the Holy Grail of exoplanet research, and the field has experienced incredible technological advancements in searching for and identifying exoplanets since the first exoplanet was discovered in 1995. This includes both ground- and space-based telescopes, specifically the powerful James Webb Space Telescope. However, directly imaging exoplanets remains elusive, primarily due to the enormous technological challenge of imaging a point of light so far away.



Unveiling Starbirth Mysteries

A view of the Taurus Molecular Cloud from the Herschel Space Observatory. The bright region at the lower left is the pre-stellar core Lynds 1544. Astronomers looked at it using radio astronomy techniques to understand what's happening in a prestellar core. [ESA/Herschel/SPIRE]

In 1985, the physicist Heinz R. Pagels wrote, "Stars are like animals in the wild. We may see the youung, but never the actual birth, which is a veiled and secret event." In the decades since then, astronomers have drawn closer and closer to figuring out what actually goes in the veiled stellar nurseries throughout the Universe. The tale of starbirth we know today invokes collapse of clouds of gas and dust into prestellar cores, but it still has many unknowns, such as the role of magnetic fields in the clouds where stars are born.



Dead Planets Orbiting a Dead Star

This artist's illustration shows the white dwarf J1328−1450, a stellar remnant where fusion ended a long time ago. When the star died, it first expanded and vapourized its planets, and that formed the debris disk seen in the image. The disk has two concentric rings of gas moving at different speeds, with a clear gap between them. It's possible that a pair of planetesimals formed in the aftermath and are shepherding the disks at different speeds. Image Credit: ESO/L. Calçada

When a star like our Sun reaches its end, it becomes a kind of zombie star called a white dwarf. These bodies have left fusion behind and will radiate only remnant heat for a long, long time. Before they become white dwarfs, they expand, engulf, and destroy any nearby planets. Astronomers have spotted a debris disk around a white dwarf, made from the dust of destroyed planets. Observations show that two new resurrected planets have formed in this disk, creating dead planets orbiting a dead star.



Massive Stellar Collisions Could Explain Early Supermassive Black Holes

Dense stellar environments like this one were common in the early Universe. New research shows how stellar collisions were common, leading to Very Massive Stars that exploded as supernovae. These could've been the seeds for the early SMBH that the JWST spotted only a few hundred million years after the Big Bang. The same research shows a plausible connection between these environments, destructive stellar collisions, and Little Red Dots. Image Credit: ESA/Hubble & NASA, R. Cohen. (Terzan 4 globular cluster.)

Dense stellar environments were common in the early Universe. These environments fostered more numerous stellar collisions, and some of those would've been mergers that formed very massive stars. Those stars would've exploded as supernovae, becoming massive black holes, the potential seeds for today's supermassive black holes.



Monday, October 26, 2026

Asymmetric space waves map pressure on Earth's magnetic shield

Earth’s magnetic field simulation depicting solar wind flow (right) and top-side Kelvin–Helmholtz waves. Color gradient reflects plasma density. (Credit: Lauri Holappa / University of Oulu)

The Earth’s magnetic field is responsible for shielding us from harmful space weather, including solar radiation from the Sun but also cosmic rays originating from outside our solar system. Cosmic rays can include deep space supernovas, so the magnetic field takes the majority of the brunt from solar radiation. Without our magnetic field, the solar wind would slowly strip away our atmosphere, making life on our small, blue world impossible to exist. But where is the magnetic field doing the heaviest lifting regarding how it filters out incoming space radiation?



A Brief-ish History of METI. Part I: Early Ideas and Experiments

The Atacama Large Millimeter/submillimeter Array (ALMA) on the Chajnantor Plateau in the Chilean Andes, with the Large and Small Magellanic Clouds visible in the night sky. Credit: ESO/C. Malin

For as long as scientists have conducted SETI (Search for Extraterrestrial Intelligence) experiments, parallel efforts in Messaging Extraterrestrial Intelligence (METI) have also been mounted. In this series, we'll take a look at the major milestones in this field of study.



Scientists Can Now Spot Hidden Sunspots on the Solar Far Side

Detailed image of the Sun with solar activity. Credit - NASA / GSFC / Solar Dynamics Observatory

Unlike the Moon, the Sun is constantly rotating from our perspective - but we still only see half of it at any given time. Since it takes 27 days to complete a full rotation, that leaves plenty of time for changes to happen to the side we can’t see that could directly impact Earth’s own space weather a few weeks later. Now a team of physicists led by Bibhuti Kumar Jha of the Southwest Research Institute has published a paper in The Astrophysical Journal Supplement Series that uses probability to map out what might be happening on the far side of the Sun, even if we can’t see it directly.



A Merger Solves a Puzzling Paradox in Orion

Protoplanetary disks in Orion seem to be younger than their stars. And Orion's expanding gas shell also seems to be younger. What's behind this? Image Credit: ESA/Hubble

Some of the Hubble Space Telescope's earliest observations were of the Orion Nebula. Those images showed proplyds, and subsequent observations uncovered a paradox centered on them. Given their rate of mass loss, those disks should have been destroyed long ago. Why weren't they?



Sunday, October 25, 2026

Rare Lunar Meteorites Could Fill Gaps In Moon’s Evolution

Researchers on an Antarctic icefield looking for meteorites.  Credit:  NASA

Almost all meteorites come from asteroids, not the Moon or Mars. But after decades of analysis of the Apollo samples, researchers still rely on lunar meteorites to better understand our anomalously large Moon.



Friday, October 23, 2026

White Dwarfs Are Actually…Yellow, Green, Pink, and Purple?

Artist’s illustration of a white dwarf appearing greenish from the sodium-rich planetary debris that enriches its atmosphere. (Credit: Mark A Garlick/University of Warwick)

The universe hosts a myriad of star types, including supergiants, giants, main sequence, red dwarfs, brown dwarfs, white dwarfs, and neutron stars. What makes these stars stand out are just their sizes, but their colors, as each one hosts a distinct color based on their surface temperature, specifically orange, red, blue, and white based on cooler to hotter temperatures. While the correlation between star colors and surface temperatures has long been known throughout astronomy, what if star colors could change based on specific criteria, including their atmosphere?



27 Exoplanet Targets for the World's First Private Space Telescope

An artist's illustration of 55 Cancri d, an exoplanet notable for being a Jupiter analog. It's one of the planets on a list of 27 targets for the Lazuli Space Telescope. It'll be the world's first private space telescope, and will use a coronagraph to image exoplanets. It's scheduled for a 2029 launch. Image Credit: NASA

Get ready for the age of private space telescopes. The Lazuli Space Telescope will launch in a few years and part of its mission is to observe exoplanets. New research presents a list of 27 exoplanet targets, some of which are very well-known and will certainly benefit from deeper observations.



The Largest Canyon in the Solar System is Still Tectonically Active

Artist's impression of the Valles Marineris canyon system on Mars. Credit: Mark Garlick/Science Photo Library

Scientists at Imperial College London and Columbia University have found that the largest canyon system in the solar system is still active and shaping Mars today, billions of years after it first formed.



Saudi Arabia Joins the Search for Alien Civilizations

Saudi Arabia has installed a pair of LaserSETI detectors in a region in a region named AlUla Manara, a site being established as the kingdom's first major astronomical observatory. They're part of a network of optical detectors will scan the heavens for laser signals from alien technological civilizations. Image Credit: LaserSETI.

Saudi Arabia is joining the search for alien signals coming from the cosmos. They're collaborating with SETI in the endeavour. SETI has announced that two LaserSETI instruments will be positioned in Saudi Arabia, adding to a growing network of optical sensors designed to detect laser pulses that could come from alien technological civilizations.



Thursday, October 22, 2026

Advancing Astronomy at MIT with X-ray Reverberation Mapping

Artist's concept of a supermassive black hole with an accretion disk and a relativistic jet. Credit: NASA

Professor Erin Kara of MIT's Kavli Institute for Astrophysics and Space Research is helping advance our understanding of the most extreme objects in the Universe by analyzing X-ray reverberations and other astrophysical data.



Even the Rubin's Test Camera Produces Stunning Images

IC 2177, or the Seagull Nebula, as captured by the Vera Rubin Observatory's Commissioning Camera in 2024. This image features the Seagull's head, a cloud of gas named Sharpless 2-292. Image Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA. Image Processing: T.A. Rector (University of Alaska Anchorage/NSF NOIRLab), D. de Martin & M. Zamani (NSF NOIRLab)

The Vera Rubin Observatory's Commissioning Camera operated for about 7 weeks in 2024, before the observatory released its well-known first look images. It's an engineering camera, and its job was to test the VRO's equipment and procedures. Now, the VRO has released the ComCam's image of the Seagull nebula. It's a pretty stunning image for an engineering camera.



Two Disks in One: How Accretion Disks Drive Black Hole Jets

This artist's illustration shows a rapidly-feeding supermassive black hole launching jets from its poles. For this to happen, the accretion disk has to have large-scale magnetic fields. But not all do, generating a contradiction. New research has an answer. Image Credit: Tohoku University.

SMBH jets are driven by thick, hot accretion disks with powerful magnetic fields. But there's a bit of a paradox. Some SMBH produce jets, even though they appear to have thin, cold accretion disks. New research has solved this paradox, showing that disks can be truncated into an outer cold disk and an inner hot disk.



New Evidence for an Old Prediction: Recoiling Supermassive Black Holes

This artist's impression shows a distant quasar, an extremely luminuos active galactic nuclei hosted by a supermassive black hole. We know that SMBH can merge, but theory says that in some mergers, the merger remnant recieves a powerful kick that drives it into a pendulum-like motion across the center of the galaxy. New research has uncovered statistical proof of these merger remnant SMBH. Image Credit: ESO/M. Kornmesser.

Theory says that during some SMBH mergers, the merger remnant receives a recoil kick from gravitational waves. Instead of sitting placidly in the galactic center, these recoiled SMBH are sent on a pendulum-like motion, back and forth through the galactic center. New research has found statistical evidence supporting their existence.



Wednesday, October 21, 2026

How Flare Ribbons Reveal Hidden Solar Explosions on the Sun

NASA’s Solar Dynamics Observatory captured this image of a solar flare – as seen in the bright flash on the right side – on Sept. 10, 2017. The image shows a combination of wavelengths of extreme ultraviolet light that highlights the extremely hot material in flares, which has been colorized. There's a lot to learn about flaring, and the ever-changing Sun itself, and new research made progress in understanding its flaring behaviour. Image Credit: NASA/SDO

Solar flaring is complex behaviour triggered by reconnection, when magnetic field lines break and then snap back to the Sun's surface. The flaring is complex behaviour, and its details are difficult to observe. Researchers found a new way to study flaring behaviour.



There Should Be Black Holes in our Neighbourhood. Can We Find Them?

This artist's illustration shows a stellar-mass black hole (left) accreting material from a much larger Wolf-Rayet star. In this case, the black hole is emitting bright energy and is hard to miss. But other stellar-mass black holes are more isolated, with little to feed on and emitting little radiation, and finding them is difficult. Image Credit: By ESO, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=9551709

Stellar-mass black holes should be in our neighbourhood within about 50 light years of the Solar System. But they're likely isolated, without much to feed on, making them difficult to find. Gaia found some candidates, but confirming them is tough.



There Must Be Stellar-Mass Black Holes in our Stellar Neighbourhood. Can We Find Them?

This artist's illustration shows a stellar-mass black hole (left) accreting material from a much larger Wolf-Rayet star. In this case, the black hole is emitting bright energy and is hard to miss. But other stellar-mass black holes are more isolated, with little to feed on and emitting little radiation, and finding them is difficult. Image Credit: By ESO, CC BY 4.0, https://commons.wikimedia.org/w/index.php?curid=9551709

Stellar-mass black holes should be in our neighbourhood within about 50 light years of the Solar System. But they're likely isolated, without much to feed on, making them difficult to find. Gaia found some candidates, but confirming them is tough.



Mars’s Most Mysterious Cloud Might Be Defying Textbook Cloud Physics

The Arsia Mons Elongated Cloud as seen from Mars Express. Credit - ESA/DLR/FU Berlin

It may not be as obvious, but just like Earth, Mars has seasons. And every day of every summer, an 1,800 kilometer long thin white cloud appears to the west of Arsia Mons, a 20 kilometer high extinct shield volcano. At least for a few hours, before it dissipates until it reappears the next morning. Scientists have known about this feature, which they call the Arsia Mons Elongated Cloud (AMEC), for decades, but planetary scientists have been unable to explain it using traditional atmospheric models. But a new paper, published in Nature Geoscience by a research team led by Dr. Jorge Hernández-Bernal of the Sorbonne, suggests that the cloud could be the first documented real-world example of a cloud flash-freezing out of thin air.



Tuesday, October 20, 2026

Scientists Use Ancient Rains to Map the Possible Origin Life on Mars

This artist's concept depicts the early Martian environment (right) – believed to contain liquid water and a thicker atmosphere – versus the cold, dry environment seen on Mars today (left). Credit: NASA's Goddard Space Flight Center.

Billions of years ago, rain may have helped shape where the chemistry of life could begin on Mars. A new study maps how formaldehyde, an important prebiotic molecule, may have reached the surface. This map could help guide future missions searching for signs of past life on Mars.



JAXA's Martian Moons eXploration Mission is on its Way to Mars and Phobos

JAXA launched its MMX sample return mission to Phobos on October 20th. It was sent on its way in an H3 launch vehicle, Japan's next-generation heavy-lift launch vehicle. It will reach Mars in August 2027, and after several years will return a sample from Phobos to Earth. Image Credit: JAXA.

JAXA successfully launched its Martian Moon eXplorer on its way to Mars and Phobos. It'll reach Mars in about six months, and will orbit the planet for about a month before transferring to an orbit around Phobos. It will deploy a small lander, which will help select a sample-gathering location for the main part of the mission. By 2031, the regolith sample from Phobos should be back on Earth.



The Gas Near Sagittarius A-star is Enriched in Metals, Probably from Supernovae Explosions

This image shows the Milky Way in infrared, and the galactic center in x-rays. New research based on JWST data shows how the gas near the supermassive black hole in the Milky Way's center is metal-enriched. It's probably because of supernovae explosions that synthesized the metals. Image Credit: By NASA - NASA, Public Domain, https://commons.wikimedia.org/w/index.php?curid=22554706

The region near Sagittarius A-star, the Milky Way's supermassive black hole, is enriched in metals, although only modestly. The likely cause is supernovae explosions, which synthesize elements heavier than hydrogen and helium. Over time, this metal-rich gas found its way towards the SMBH. The increased metallicity and heat from the supernova affect how fast gas flows into the SMBH.



JWST Tracks Shifting Water Clouds and Churning Gases on the Coldest Known Brown Dwarf

Artist's conception of a brown dwarf. Credit - NASA / JPL-Caltech

When picturing a star, typically people think of giant balls of burning gas in the sky that emit enough light they are hard to miss. Planets, on the other hand, come in one of two general categories - rocky worlds like Earth or gas giants similar to Jupiter. But there is a third category of astronomical object that doesn’t really fit either of those descriptions, and also doesn’t exist in our own solar system. Known as a brown dwarf, they are sometimes called a “failed star” as they form the same way stars do, but never reach the critical mass of material to create active fusion in the cores. They are also much too massive to be considered a regular planet. But a new paper from researchers led by Brittany Miles of the University of Arizona describes one similarity between the coldest known brown dwarf and some of the planets in our solar system - it has water-ice clouds.



Monday, October 19, 2026

Webb Captures This Golden Galaxy Cluster in All it's Glory

Webb captures the massive galaxy cluster MACS J0454.1-0300, made of many golden elliptical galaxies. Credit: NASA/ESA/CSA

The NASA/ESA/CSA James Webb Space Telescope Picture of the Month features the brilliant golden galaxies belonging to the MACS J0454.1-0300 galaxy cluster.



The ESA's Euclid Space Telescope Has Discovered A New Comet

The Euclid space telescope captured this image of the comet C/2026 S1 (Euclid), the first comet discovered by the space telescope. This is a happy accident, since Euclid's mission is to measure billions of galaxies and study the force that drives the expansion of the Universe, dark energy. Euclid has observed other comets, but this is the first one it's discovered. Image Credit: ESA/Euclid/Euclid Consortium/NASA, M. Pöntinen et al. 2026. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence

The ESA's Euclid space telescope was launched in July, 2026, and its mission is to observe billions of galaxies. The goal is to measure their redshifts over 10 billion years of Universal expansion, to better understand dark matter and dark energy. Surprisingly, the telescope has discovered a brand new comet, now named C/2026 S1 (Euclid).



Achievement Unlocked: Microblazar Confirmed

This artist's illustration shows an astrophysical jet emitted by an active supermassive black hole. When of these jets is aimed at Earth, we call it a blazar. Astrophysicists have found the first microblazar, a stellar mass black hole emitting with one jet aimed at Earth. It may be the source of the highest-energy particles in the galaxy. Image Credit: NASA/JPL-Caltech

Researchers have confirmed the existence of the first microblazar. Unlike blazars, which are extragalctic and powered by supermassive black holes, microblazars are inside the Milky Way, and are powered by stellar mass black holes. The microblazar may be the source for the most energetic particles in the galaxy.



Saturday, October 17, 2026

New Research Reveals How Long Stays in Space Affects the Human Genome

Human cells with fluorescently labeled chromatin (green) and microtubules (magenta) appear elongated after 24-hour exposure to fluid flows. Credit: Kanellakopoulos/Zidovska/NYU

A new study in Science Advances addresses the pressing questions about how long-duration exposure to microgravity affects the human genome.



Enigmatic Mercury Will Remain A Puzzle Until Someone Sends A Lander

Mercury, the innermost planet in our solar system.

Despite the upcoming Bepi Colombo visit to Mercury, we need a lander mission to fully understand our solar system’s innermost planet.



Friday, October 16, 2026

In the Search for Exoplanets, Some Failures Are A Success

This artist's illustration shows the pair of stars that make up the binary star 70 Ophiuchi AB (70 Oph AB.) The pair is close to Earth, only about 16.7 light years away. Astronomers conducted a search for massive planets in the system in an attempt to find nearby large terrestrial planets. None were found, but in this case, that isn't necessarily a failure. Image Credit: Hans Anderson/Michigan News

Astronomers used decades of archival data and new radial velocity measurements to search for exoplanets around a neaby binary star, 70 Oph AB. They didn't find any, which can seem like a failure. But in this case, their work only ruled out large, Jupiter-mass planets at certain distances. There could still be Earth-sized planets there, and their precise findings will only fuel a deeper search with more powerful telescopes.



The Flavor of Neutrinos Could Determine How a Large Star Dies

Illustration of the stages of a dying star as it collapses into a black hole. Credit: NASA/ESA/P. Jefferies (STScl)

Neutrinos come in three different flavors. A new study finds that neutrino flavor could play a significant role in whether a dying star becomes a supernova or collapses directly into a black hole.



A Radio Phoenix Beyond the Zone of Avoidance

This composite image shows the Treble Clef, an unusual and remarkable radio wave formation beyond the Milky Way's Zone of Avoidance. The Zone of Avoidance is opaque in optical light, but not in radio, infrared, and x-rays. Astronomers used the Chandra X-ray observatory and SRG/eROSITA to study the object, revealing its nature and its history. Image Credit: X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

Years ago, astronomers spotted a strange radio formation beyond the Zone of Avoidance. The formation resembles a treble clef, a symbol in musical notation, and the nickname has stuck. Determining what created it has been difficult, but new research has revealed that the Treble Clef is a radio phoenix.



A Distant Supercluster of Galaxies Points To Self-Interacting Dark Matter

Hubble image of the El Gordo supercluster with the estimated dark matter highlighted in blue. Credit: NASA Hubble

The El Gordo supercluster is unusually large given its distance. How could such a large galaxy cluster form so quickly? The answer could be that dark matter is self-interacting in an interesting two-state way.



Thursday, October 15, 2026

Scientists Detect Rare Type of Wood Alcohol in Space

A rare form of the organic alcohol methanol is present around at least one of the very young stars in the Perseus molecular cloud. Credit ©: Ekaterina Moerova/MPIfR/NASA/CXC/SSC/NOAO/DSS/NCBI

As part of the ALMA COMPASS Large program, an international research team has detected a rare form of methanol in space for the first time.



Host Stars Shape Their Planetary Systems Into Two Families

A team of astronomers have found a comprehensive link between solar system architectures and their host stars. They describe it as a 'genetic link' between the host star's size and metallicity, and the type of planets and their positions. The host star shapes the birth, dynamical evolution, and future stability of the entire planetary system. Image Credit: INAF / Universitat de Valencia / image generation assisted by Gemini AI

New research draws a link between a host star and the characteristics of its planetary system. Higher mass stars create one family of systems, while lower mass stars create another. These results provide a new, more detailed template for understanding exoplanet systems.