Tuesday, January 27, 2026

Mapping the Invisible

Dark matter map for a patch of sky based on gravitational lensing analysis of a Kilo-Degree Survey (Credit : Kilo-Degree Survey Collaboration/H. Hildebrandt & B. Giblin/ESO)

Dark matter remains invisible to our telescopes, yet its gravitational fingerprints pervade the universe. Using NASA's James Webb Space Telescope, scientists have produced one of the most detailed dark maps ever created, revealing with unprecedented clarity how dark matter and ordinary matter have grown up together. The map shows that wherever galaxies cluster in their thousands, equally massive concentrations of dark matter occupy the same space, a close alignment that confirms dark matter's gravity has been shepherding regular matter into stars, galaxies, and ultimately the complex planets capable of supporting life.



Researchers Use AI To Find Astronomical Anomalies Buried In Archives

These six galaxies were among the almost 1,400 anomalous objects buried in the Hubble Legacy Archive. Researchers used AI tools to comb through the vast archive and detect anomalous objects. The discovered objects include a ring-shaped galaxy, a bipolar galaxy, a group of merging galaxies, and three galaxies with warped arcs created by gravitational lensing. Image Credit: ESA/Hubble & NASA, D. O’Ryan, P. Gómez (European Space Agency), M. Zamani (ESA/Hubble)

AI faces strong skepticism due to its potential for misuse, its drain on resources, and even its potential dumbing down of students. But new results illustrate its uses. A team of astronomers have used a new AI-assisted method to search for rare astronomical objects in the Hubble Legacy Archive. The team sifted through nearly 100 million image cutouts in just two and a half days, uncovering nearly 1400 anomalous objects, more than 800 of which had never been documented before.



This Rapidly Growing Black Hole Is Challenging Super-Eddington Accretion

This artist’s impression of a supermassive black hole system shows some of the detail in these puzzling objects. Infalling gas forms an accretion disk around the hole, with a bright corona of plasma nearest the black hole. The SMBH is also launching relativistic jets from its poles. Image Credit: NASA/JPL-Caltech

Why are SMBH in the early Universe so massive? According to astrophysical models, these extraordinarily large SMBH haven't had time to become so massive. Super-Eddington accretion might explain it, but can it explain a very unusual early SMBH recently discovered?



The HWO Must Be Picometer Perfect To Observe Earth 2.0

Artist's concept of the Habitable Worlds Observatory. Credit - NASA / Jonathan North / Walt Feimer / Aaron E. Lepsch

Lately we’ve been reporting about a series of studies on the Habitable Worlds Observatory (HWO), NASA’s flagship telescope mission for the 2040s. These studies have looked at the type of data they need to collect, and what the types of worlds they would expect to find would look like. Another one has been released in pre-print form on arXiv from the newly formed HWO Technology Maturation Project Office, which details the technology maturation needed for this powerful observatory and the “trade space” it will need to explore to be able to complete its stated mission.



Asteroid 2024 YR4 Has a 4% Chance of Hitting the Moon. Here’s Why That’s a Scientific Goldmine.

Oribtal path of Asteroid 2024 YR4. Credit - ESA Orbit Visualization Tool

There’s a bright side to every situation. In 2032, the Moon itself might have a particularly bright side if it is blasted by a 60-meter-wide asteroid. The chances of such an event are still relatively small (only around 4%), but non-negligible. And scientists are starting to prepare both for the bad (massive risks to satellites and huge meteors raining down on a large portion of the planet) and the good (a once in a lifetime chance to study the geology, seismology, and chemical makeup of our nearest neighbor). A new paper from Yifan He of Tsinghua University and co-authors, released in pre-print form on arXiv, looks at the bright side of all of the potential interesting science we can do if a collision does, indeed, happen.



Monday, January 26, 2026

Galilean Moons’ Water Differences Set During Formation

Diagram depicting the formation materials for the Galilean moons, with Io receiving anhydrous (non-water) rocks, Europa receiving hydrous (water-rich) rocks, while Ganymede and Callisto primarily received ices. (Credit: Southwest Research Institute)

How long did it take to establish the water content within Jupiter’s Galilean moons, Io and Europa? This is what a recent study published in The Astrophysical Journal hopes to address as a team of scientists from the United States and France investigated the intricate processes responsible for the formation and evolution of Io and Europa. This study has the potential to help scientists better understand the formation and evolution of two of the most unique moons in the solar system, as Io and Europa are known as the most volcanically active body in the solar system and an ocean world estimated to contain twice the volume of Earth’s oceans, respectively.



Icy Comets Get A Contribution From Stellar Furnaces

The JWST captured this image with its NIRCam instrument. It shows the actively forming protostar EC 53 (circled) in the Serpens Nebula. It doesn't show up in this image, but EC 53 has a protoplanetary disk where planets form. Researchers also used the JWST's MIRI to examine the protostar and its disk. They found crystal silicates throughout the disk, which helps explain why we find them in comets in our own Solar System. Image Credit: NASA, ESA, CSA, STScI, Klaus Pontoppidan (NASA-JPL), Joel Green (STScI); Image Processing: Alyssa Pagan (STScI)

Icy comets contain common crystals that can only be formed in extreme heat. But comets reside in the frigid outer reaches of the Solar System. How did these materials form, and how did they find their way into the Solar System's cold fringes?