The decades old idea that our solar system’s Oort Cloud is continually perturbed by a heretofore undetected low mass Red Dwarf star remains the best explanation for periodicities found in Earth’s impact record. Or so says a well known physicist who has long championed this idea.

Ultra-Diffuse Galaxies are strange because they're as large as the Milky Way, but have far fewer stars. It's as if they're puffed up for some reason. Determining what's going on with them could help confirm the Lambda-CDM model. A new proposed instrument for the Extremely Large Telescope could give astronomers their best look yet at these strange galaxies.

NASA's ESCAPADE mission features a pair of identical spacecraft on their way to Mars. They launched outside of the normal launch window, so they'll perform powered slingshot maneuvers to boost their speed. Once there, they'll "fly" in formation and study how the solar wind interacts with what remains of Mars ancient magnetosphere.

We typically think of the Moon as a static, floating object that has remained the same for basically its entire lifetime, with an occasional asteroid impact serving as an exception. That understanding is grounded in physics - the Moon should have cooled rapidly after forming when a huge protoplanet hit the early Earth around 4.5 billion years ago. But, some lunar material returned from the Chang’e-5 mission was notably formed only around two billion years ago, yet appeared to be volcanic in origin. So how did a world that was supposed to have settled down without volcanism remain hot enough to create these materials more than two billion years after its violent birth? A new paper from Miao Chen of the Chengdu University of Technology and his colleagues, and recently published in the journal Planet, offers an explanation - tidal heating.

Flashback to 1977. Jimmy Carter was U.S. president, Star Wars was a box office hit, and the two Voyager spacecraft departed on an historic Grand Tour of the solar system. Now, teams at NASA’s Jet Propulsion Laboratory are working to keep the missions active, as they push the boundaries of interstellar space beyond the solar system.

In a pinch, we could use a stand-off nuclear blast to redirect a dangerous asteroid on short notice. There's no atmospheric shock wave in space, but the x-ray pulse could still deflect the space rock. But asteroids aren't round and uniform, so their weird shapes make it difficult.

When astronomers looked at photos of the early universe taken by the James Webb Space Telescope, they found something odd: an overabundance of bright galaxies about 400 to 500 million years after the Big Bang. But these galaxies should have been far less common so soon after the Big Bang. Researchers may have figured this out: Powerful ultraviolet (Lyman-alpha) radiation produced by dense clusters of young stars acted like a leaf blower, driving light-blocking gas and dust out of the galaxy and thereby making the galaxies appear brighter.

Targets of opportunity sometimes happen in astronomy, and we got a major one when the third interstellar object, 3I/ATLAS, was discovered in July 2025. And it just so happens that in the intervening years between the last known interstellar visitor (2I/Borisov in 2019), we got a major upgrade in our observational capabilities with the launch of the James Webb Space Telescope (JWST). A new paper from a team of researchers led by Dr. Silvia Protopapa of NASA’s Goddard Space Flight Center and the Southwest Research Institute, and published in The Astrophysical Journal Letters, details JWST’s findings on the water ice content of this most recent visitor from beyond our solar system.

Finding dim exoplanets hidden in the glare of their stars is an ongoing challenge in astronomy. Telescopes use coronagraphs to block out starlight, but even they have their limitations. Researchers have developed a new technique with the JWST that can find dim exoplanets more easily than ever.

Yesterday, on November 3rd, the deputy chief designer of China's crewed space program and chief designer of the lunar exploration program (Wang Xiang) unveiled an official statement detailing its [plans for a crewed mission to the Moon](https://english.spacechina.com/n17212/c4744561/content.html).

SETI can be more effective the more the targets in the search are refined. SETI's newest survey effort uses game theory to inform its search. It's based on the idea that other ETIs would almost certainly use the transit method to detect habitable worlds like Earth.

For a long time, planetary scientists thought that giant impacts drove a young planet's atmosphere away into space with all the heat they generated. But it turns out the opposite could be true. The mass a young planet gains through a giant impact increases its gravitational hold on its atmosphere.

Researchers have created a model lifeless Earth that couples the atmosphere with interior planetary processes. The model can reproduce Earth's modern habitable state without including life, showing that a planet that appears habitable isn't necessarily inhabited. The tool will be useful when and if the Habitable Worlds Observatory is launched, by helping identify false positives.

This summer, a team of students and researchers at the University of Alabama in Huntsville successfully conducted three rocket-motor firing tests on a prototype lunar landing pad. The tests showed the prototype’s ability to capture and redirect rocket exhaust through an integrated vent system, marking an important milestone in developing landing infrastructure for future Moon base operations.

When we make our home on other worlds, who will be in charge? Will it be an emperor? A billionaire? A rebel alliance? Or none of the above? Astrobiologist Jacob Haqq Misra runs through the legal and political options.

Astronomers are finding more dusty disks around white dwarf stars, and some of them are home to asteroids. But how these rocky asteroids are turned to dust and form these rings isn't clear. New research shows that the white dwarf's gravity alone can't shred them to dust.

The Vera Rubin Observatory has detected two more of the Milky Ways' dim, hard to see satellites. One is an ultra-faint dwarf galaxy, and one is a globular cluster. Each one is a missing piece of the puzzle in the Milky Way's merger history. By finding more of these satellites, our understanding of galaxy growth, and the role dark matter plays in it, will improve.

Astrophysicists think that black holes grow through a hierarchical merger framework. But the elusive Intermediate Mass Black Holes are the missing link between stellar mass black holes, and the gargantuan supermassive black holes like the one at the center of the Milky Way. The JWST may have found the ancient sources of IMBH heavy seeds: young massive clusters in the high-redshift Universe.

Samples from the asteroid Ryugu, and from carbonaceous chondrites that have crashed on Earth, present an apparent contradiction. Their fine-grained matrices have widely varied compositions of their clay-like minerals. That suggests that there were widely different aqueous environments in the same parent bodies, which seems unlikely. But new research may have solved that contradiction.

The sky in Vincent van Gogh’s The Starry Night (1889) matches, in both observation and shape, the pre-dawn sky over Saint-Rémy around 22 July 1889, when a waning crescent moon, Venus and the Hyades star cluster appeared close together, according to a study published inScientific Reports.