Tuesday, September 22, 2026

3I/ATLAS Has An Extreme Taste For Heavy Water

Hubble image of interstellar comet 3I/ATLAS, which was used in the study. Credit - NASA, ESA, D. Jewitt (UCLA); Image Processing: J. DePasquale (STScI)

More and more details about 3I/ATLAS are filtering through the scientific process as time goes on. Our third known interstellar visitor attracted the attention of some of the most powerful observatories in the world when it was discovered in July 2025, and some of those telescopes found something peculiar - the isotopes it contained appeared different. A new paper submitted to The Astrophysical Journal Letters (and available in pre-print on arXiv) by Kenji Furuya of the RIKEN Pioneering Research Institute in Japan and his co-authors, shows how that isotopic discrepancy is likely due to the “low-metallicity” of the stellar nursery 3I/ATLAS was born in.



Space Rocks Carry Hundreds of Thousands of Complex Organic Molecules—and We Just Photographed Them

Some of the structures of the organic compounds found in the meteorites along with their chemical structures, as shown by AFM imaging. Credit - Brookhaven National Laboratory / J.W. Frye-Jones et al.

Scientists have known for a while that meteorites contain the “building blocks” of life - complex organic molecules such as amino acids, simple sugars, or even the chemical rungs of DNA. But anyone who has taken an organic chemistry class knows there are plenty of other carbon-based molecules out there, and a new study from Joseph W. Frye-Jones of the National High Magnetic Field Laboratory and Florida State, which was published in The Planetary Science Journal, found tens of thousands of types of previously unseen organic compounds in two of the world’s most famous meteorites.



Monday, September 21, 2026

A Rare, Distant Clump of Early Galaxies Reveals Ancient Cosmic Secrets

An annotated view of a map of the newly discovered proto-supercluster COSMOS-z3.1-A. It was discovered in data from a large survey of the Southern Hemisphere sky taken by the Dark Energy Camera mounted on the Blanco telescope on Cerro Tololo, Chile. Credit: CTIO/NOIRLab/DOE/NSF/AURA

The discovery of a very early and rare proto-supercluster of infant galaxies may help give clues to the formation of such clusters and their connection to the Cosmic Web.



Smashed Icy Moons Cool Too Rapidly to Retain Oceans

Diagram depicting Saturn's moon, Enceladus, and its subsurface ocean. (Credit: Southwest Research Institute)

There are more than 450 confirmed moons orbiting the eight major planets, but only a handful of them provide unique scientific value to pique the interests of the scientific community, specifically their potential for hosting life as we know it. This is due to the subsurface oceans that exist beneath icy crusts, including Jupiter’s Europa and Ganymede, and Saturn’s Enceladus. But what processes are responsible for producing these subsurface oceans, or potentially preventing them from forming in the first place?



Earth's Center of Mass Drifts Less Than We Thought

The Earth's center of mass drifts by millimeters over the years. Credit: NASA’s Scientific Visualization Studio

Earth's center of mass isn't stationary. It drifts seasonally and over the course of years. A new study measures this down to the scale of millimeters and finds the seasonal drift is smaller than we thought.



Solar Orbiter Catches the Sun’s Missing High-Speed Vibrations

Images from the EUI of the Solar Orbiter show the fine plumes and "transverse" wave motion in the upper atmosphere of the Sun. Credit - Science China Press

The Sun’s magnetic fields are a twisty, curvy, ever changing mess. In particular, our star’s polar regions host regions called polar coronal holes that host invisible magnetic highways that stretch out into interplanetary space. But there’s a lot we don’t know about how those highways actually work, and in particular how they give the particles that form the fast solar wind an extra “kick” that sends them zooming at hundreds of kilometers per second. A new paper from a team led by Dr. Yuhang Gao and Prof. Hui Tian at Peking University, and published recently in the journal National Science Review, thinks they might have found an answer by using high-speed shots from Solar Orbiter to detect never-before seen rapid, high-frequency magnetic waves in those areas.



Astronomers Uncover "Hypersoft" X-ray Sources

Image of M101, the Pinwheel Galaxy, one of the homes of some of the HSSs. Credit: X-ray: NASA/CXC/Univ. of Alabama/M. Muhibullah et al.; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/N. Wolk

X-rays showcase some of the most unique astronomical objects in the universe. Neutron stars and black holes siphoning gas from companion stars stick out like sore thumbs at this level of radiation. However, according to a new paper by Mustafa Muhibullah and Jimmy Irwin from the University of Alabama and Rosanne Di Stefano from the Center for Astrophysics at Harvard & the Smithsonian, there appears to be another group of ultra-bright X-ray emitters that we’ve completely missed until now. They call them Hypersoft X-ray Sources (HSSs) and, according to a press release accompanying the paper, might answer two long-standing astronomical questions.