Wednesday, November 4, 2026

Giant Impacts Help Rocky Planets Retain Their Atmospheres

Giant impacts like the one in this artist's illustration had a powerful effect on the planets that suffered them. Astronomers thought that these impacts drove the atmospheres of young planets into space. But new research shows that may not be true. Image Credit: By NASA/JPL-Caltech - http://www.nasa.gov/multimedia/imagegallery/image_feature_1454.html, Public Domain, https://commons.wikimedia.org/w/index.php?curid=8626942

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.



A Virtual Lifeless Earth Will Help Scientists Find Life on Exoplanets

This artist's illustration shows an Earth-like rocky planet with an atmosphere. Scientists at the University of Washington created a virtual Earth that realistically models how chemicals are exchanged between the planet's atmosphere, surface, crust, mantle, and core. The model can help astronomers study real exoplanets and determine whether their atmospheres show evidence of alien life, rather than just being potentially habitable. Image Credit: 852278-MCS. Creative Commons Attribution-Share Alike 4.0 International.

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.



Tuesday, November 3, 2026

Students Test Prototype Landing Pad to Make Lunar Operations Safe

Artist's concept of the lunar landing pad developed by students and researchers at UHA and Linc Research Inc. Credit: LINC Research Inc.

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.



What Will Politics Look Like on Other Planets? It's Likely to Be a Mishmash

Throngs salute Paul Atreides, who reigns as emperor of the known universe in the movie "Dune: Part Three." (Photo Courtesy Warner Bros. Pictures)

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.



Stubborn Asteroids Around White Dwarfs Resist Becoming Dust

This illustration shows a white dwarf and its debris disk, with three asteroids in the disk. New research shows that, for some reason, asteroids in this precarious situation aren't immediately torn to dust. Instead, they initially remain in larger, intact fragments. Image Credit: Pamela L. Gay / Planetary Science Institute

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.



Monday, November 2, 2026

The Vera Rubin Has Found Two More of the Milky Way's Dim Satellites

The Vera Rubin Observatory observing the Milky Way from its location on a mountain top in Chile. In its Early Data Preview 2, the observatory found two new satellites of the Milky Way. One is an ultra-faint dwarf galaxy, and the other is a globular cluster. They're probably the first of many more the observatory will discover. Image Credit: NSF-DOE Rubin Observatory/AURA/B. Quint

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.



The JWST May Have Found Where Heavy Black Hole Seeds Formed

The JWST found five dense, lensed star clusters only about 460 million years after the Big Bang. These clusters were ideally suited to being the birthplace for the elusive intermediate mass black holes (IMBHs). Image Credit: ESA/Webb, NASA & CSA, L. Bradley (STScI), A. Adamo (Stockholm University) and the Cosmic Spring collaboration. LICENCE:
CC BY 4.0 INT or ESA Standard Licence

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.