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?



NASA's Psyche Spacecraft Captured a Time-Lapse Video of its Mars Flyby

In May, NASA's Psyche spacecraft performed a gravity-assist maneuver that sent in on its way to its target, the metal-rich asteroid 16 Psyche. The flyby was also an opportunity to test the spacecraft's instruments, including its multispectral camera. NASA has released a time-lapse video of the encounter. Image Credit: NASA/JPL

NASA's Psyche mission used a gravity assist maneuver at Mars to gain velocity and adjust its trajectory to its eventual target. The asteroid 16 Psyche is a metal-rich asteroid that may be the remnant rocky core of a protoplanet. The flyby not only shepherded the spacecraft on to its target, it was also an opportunity to test Psyche's science instruments and cameras. NASA has released a timelapse of the flyby.



Astronomers Are Still Trying to Understand How a Galaxy's Spiral Arms Form

The Whirlpool Galaxy (M51) is the classic grand design spiral galaxy. It was the first object recognized as a spiral, though at the time astronomers thought they were nebulae. Astronomers have been pondering spiral galaxies for a long time, trying to understand how their spiral arms persist. New research has at least a partial answer. Image Credit: NASA, ESA, S. Beckwith (STScI) and the Hubble Heritage Team (STScI/AURA)

Spiral galaxies, including grand spirals like the Whirlpool galaxy, are plentiful. But it's still a mystery how their spiral arms form and persist for hundreds of millions of years, and why some galaxies have one, two, or three or more arms. New research based on Euclid data finds links between galaxy mass, star formation rate, and number of arms, and hints at their formation.



Astronomers Catch a "Dark Comet" Red-Handed

Artist's depiction of a near-Earth asteroid with an elongated orbit. Credit - NASA/JPL-Caltech

Our ability to track and visualize small rocks in space is still improving. And occasionally we’ll find a space rock that will remind us of that fact. One such rock is detailed in a new paper, led by Davide Farnocchia of NASA’s Jet Propulsion Laboratory, and recently published in Nature Astronomy, where the research team discovered what they thought was a normal, run of the mill asteroid, was actually a “dark comet”.



Monday, July 20, 2026

Astronomers Determine that Exoplanets Around Barnard's Star are Extremely Uninhabitable

Artist’s illustration of exoplanets orbiting Barnard’s Star. Credit: [International Gemini Observatory/NOIRLab/NSF/AURA/P. Marenfeld](https://www.gemini.edu/gallery/images/noirlab2510a/)

Scientists have painted the most detailed portrait yet of the planetary system orbiting Barnard’s Star. Unfortunately, the picture is not encouraging, as all four planets appear to be "extremely uninhabitable."



Meet Our Newest Stellar Neighbours That Hid in the Glare of Other Stars

This artist's illustration shows a white dwarf and its much larger red dwarf binary companion. Astronomers have four more of these binary stars in the Sun's neighborhood. They're called post-common-envelope binaries, and they're hard to detect because the bright red dwarf hides the white dwarf from telescopes. Image Credit: Mark A. Garlick/University of Warwick

Astronomers have found four new white dwarfs within about 65 light years. Even though the sky has been studied thoroughly, these escaped detection. That's because they're tight binaries with red dwarf partners, and the much brighter red dwarfs hide the white dwarfs. The binaries used to share common envelopes.



A Star Orbiting Our Galaxy's Supermassive Black Hole Tests the Limits of Relativity

Illustration of a sunlike star passing very close to a supermassive black hole. Credit: ESO, ESA/Hubble, M. Kornmesser

A Sun-like star orbits the supermassive black hole in our Milky Way so closely that it comes within the distance of Neptune's orbit of the Sun. It has a top speed of more than 8% of light speed. With such extreme motion the star gives astronomers the opportunity to test the limits of general relativity.



Chandrasekhar and the Limits of Physics, Part 1: Triumph

The Helix Nebula, the glowing shell thrown off by a dying star, with a hot white dwarf at its heart. White dwarfs, and the 1.4 solar mass limit that governs them, were Chandrasekhar's breakthrough. Credit: NASA/JPL-Caltech / Wikimedia Commons (public domain).

The story of Subrahmanyan Chandrasekhar, who as a teenager on an ocean voyage worked out that white dwarf stars have a maximum mass of 1.4 Suns. A tour of degeneracy pressure, the relativistic insight everyone else missed, and the number that would define his life.



Sunday, July 19, 2026

The First Breath of Another World

Artist's impression of the planet LHS 1140 b and its host star (Credit : ESO/spaceengine.org)

Astronomers have detected an atmosphere around a rocky planet in another star's habitable zone for the very first time. It’s a milestone that brings us a step closer to answering whether life could exist beyond our Solar System. Predicted by a mathematical model before it was ever observed, and confirmed using a rare planetary alignment 48 light years away, this discovery does more than identify one intriguing world, it provides us with a whole new way to search for others like it.



NASA's Perseverance Rover Uncovers Evidence of 4 Billion Year Old Impacts

NASA’s Perseverance took this selfie at “Witch Hazel Hill” on Jezero Crater’s rim on May 10th, 2025. Credit: NASA/JPL-Caltech/MSSS

Old rocks exposed on the rim of Jezero Crater preserve a roughly 4-billion-year-old cosmic “weather report” from the solar system’s most dynamic era.



Saturday, July 18, 2026

NASA’s Artemis III Lander Test Will be a "Dress Rehearsal" for Returning to the Moon!

Artist's impression of the Starship and Blue Moon Human Landing System (HLS) concepts on the lunar surface. Credit: SpaceX/Blue Origin

Before Artemis astronauts land on the Moon’s surface in 2028, NASA will conduct the Artemis III demonstration mission in 2027, allowing teams on Earth and in orbit to practice rendezvous and docking operations between commercial human landing systems and the Orion spacecraft. Data from that mission, along with future uncrewed demonstration missions at the Moon,



Submillimeter Array Catches a Gamma-Ray Burst Thanks to new Fast-Response System

An artist's impression of a superluminous supernova and an associated gamma-ray burst being driven by a rapidly spinning neutron star. Credit: CfA

The Submillimeter Array's (SMA) new semi-automated alert system demonstrates how the radio interferometer quickly responds to discoveries from space-based telescopes.



On The Hunt For Earth’s First Complex Life

Bear Island in the Barents Sea which is a paleontological hotbead known for preserving ancient microfossils.  Credit:  Wikipedia

Finding microfossils of Earth’s oldest complex life is a bit like chasing an astrobiological rainbow. The eukaryotic pot of gold at rainbow’s end always seems just a bit out of reach.



Friday, July 17, 2026

The Dark Energy Camera's New Image is Reminiscent of van Gogh

The 570 megapixel Dark Energy Camera captured this image of the Corona Australis Molecular Cloud. It's one of the nearest star forming regions to Earth. R Coronae Australis, a variable binary system, lights up the orange cloud on the left. Dust lanes, newborn stars, and nebulae fill the frame. The globular cluster NGC 6723 is prominent in the upper right, though it's much farther away than Corona Australis. Image Credit: Dark Energy Survey/DOE/FNAL/DECam/CTIO/NOIRLab/NSF/AURA.  Image processing: R. Colombari & M. Zamani (NSF NOIRLab)

The Dark Energy Camera (DECam) has a massive 570 megapixel camera, and its new image is of the Corona Australis Molecular Cloud. Corona Australis is one of the closest star-forming regions to Earth. It's not as well-studied as the Orion Molecular Cloud or Ophiuchus, but as DECam's new iage of Corona Australis shows, it's just as fascinating.



What's It Like to Travel Near the Speed of Light? Part 4: The Hot View

A Saturn V rocket accelerates off the pad. Sustained acceleration is exactly what conjures the faint quantum glow of Unruh radiation. Credit: NASA (public domain).

An accelerating observer finds their empty vacuum glowing with real particles, a bizarre effect called Unruh radiation. It's a cousin to Hawking radiation, but with no black hole required, just a rocket and its throttle.



X-Ray Eyes Reveal the Magnetic Secrets of the Lighthouse Pulsar's Cosmic Wake

False color image of the Lighthouse Pulsar. Credit : X-ray: Chandra: NASA/CXC/Stanford Univ./J.T. Dinsmore et al.; IXPE: NASA/MSFC/J.T. Dinsmore et al., Radio: CSIRO/ATNF/ATCA; Optical: 2MASS/UMass/IPAC-Caltech/NASA/NSF; Image processing: NASA/CXC/SAO/L. Frattare

Space Telescope Maps Magnetic Fields of "Lighthouse" Pulsar kerryhensley45577 Mon, 07/13/2026 - 10:49 Space Telescope Maps Magnetic Fields of "Lighthouse" Pulsar https://science.nasa.gov/missions/ixpe/nasa-space-telescope-maps-magnetic-fields-of-lighthouse-pulsar/



FCC Approves First Launch for Space Reflector Constellation

An artist's conception of Eärendil-1 in orbit. Credit: Reflect Orbital.

The United States Federal Communications Commission (FCC) recently approved the first test launch of Reflect Orbital’s Eärendil-1 satellite. Sporting an 18 by 18 meter-wide reflector once unfurled, the satellite will test the ability to reflect sunlight back to Earth, on demand. The company envisions more than 50,000 reflectors girding the Earth in low Earth orbit by 2035, while many in the astronomical community have raised concerns on the project's impact.



Thursday, July 16, 2026

Satellite Images of Pengiun Poo Reveal Climate Change's Impact on the Species

Nesting Adélie penguins on Antarctica's King George Island. Credit: Michael Polito, UC Santa Cruz

Researchers utilized 30 years of Landsat satellite imagery to analyze the color and spectral signatures of Adélie penguin guano across Antarctica, marking the first time space-based observations have captured food-web and population dynamics at a continental scale.