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.