Thursday, November 12, 2026

Euclid's First Data Release: A Stepping Stone to its 3D Map of the Sky

This graphic gives an overview of Euclid's first data release, DR1-Foundation. The two main survey regions are shown in the middle, overlain on the Milky Way's plane. A full Moon is shown on the left for reference. Each of the boxes are zoom-ins progressing from large regions down to individual objects. Overall, it illustrates how the Wide and Deep surveys work together to image large regions of the sky and to zoom-in on smaller objects. Image Credit: ESA/Euclid/Euclid Consortium/NASA, image processing by J.-C. Cuillandre and E. Bertin. Licence: CC BY-SA 3.0 IGO or ESA Standard Licence

The ESA's Euclid Space Telescope has released its first huge batch of data. It's all part of the telescope's mission to study dark energy and dark matter. The telescope is busy creating the largest ever 3D map of the Universe with its huge 600 megapixel camera, and new images give us some highlights.



A Brief-ish History of METI. Part III: The Legacy of Frank Drake & Carl Sagan

Artist's illustration of Voyager 1 with the orbits of Jupiter, Saturn, Uranus and Neptune represented by red circles. (Image credit: NASA, ESA, and G. Bacon (STScI))

Carl Sagan and Frank Drake were pivotal to the development of the Search for Extraterrestrial Intelligence (SETI) and Messaging Extraterrestrial Intelligence (METI), as exemplified by the Pioneer Plaques and Voyager Golden Records.



Asteroid Bennu's Sample Delivers Another Surprise

This illustration shows NASA's OSIRIS-REx spacecraft about to gather a sample from asteroid Bennu. Scientists found amino acids and some of the building blocks of DNA in the sample. New research compares the isotopic composition of those samples with similar chemicals found on the Murchison meteorite to understand how they formed in the early Solar System. Image Credit: Goddard Space Flight Center/University of Arizona/NASA

Researchers compared the samples from asteroid Bennu with the Murchison meteorite and measured the amino acid β-alanine in both. Using new techniques, they were able to measure not only their isotopic compositions, but isotopic differences between individual atoms in the same molecule. The results show that some of the same pre-cursors to life formed in different conditions and positions in the protoplanetary disk.



Solving the Space Junk Crisis Isn't Just About Counting Trash—It’s About Control and Economics

Artist's depiction of the ADRAS-J mission to rendezvous with a defunct rocket stage. Credit - Astroscale

If people ever think about cleaning up space debris, they typically think of something equivalent to a giant garbage truck in the sky, collecting lost astronaut tools and dead satellites then hauling them back down to Earth to be deposited in a landfill. But dealing with space debris doesn’t work that way, and a new paper, available in pre-print on arXiv from Dr. Slava Turyshev of NASA’s Jet Propulsion Laboratory, who we typically cover for his work on the Solar Gravitational Lens idea, makes a good argument as to why.



Astrophysicists Want to Forecast When a Black Hole Launches Its Jets

This illustration shows an x-ray binary system, where a black hole draws gas from a donor star, usually a main sequence star. The gas gathers in a rotating accretion disk around the black hole, and some of it is ejected in powerful jets. The material in the disk becomes super-heated and emits x-rays. Japanese researchers watched four x-ray binaries and their disks for clues to how to predict when they launch their powerful jets. Image Credit: NASA/CXC/M.Weiss.

Astrophysical jets are enormously powerful and energetic phenomena. Black holes launch them from their poles and they can extend enormous distances into space, disrupting star formation in adjacent regions. Astrophysicists want to be able to forecast when they're launched so they can understand theire extreme physics better. New research is making progress in understanding when they are triggered.



Wednesday, November 11, 2026

The Ice Giants' Magnetic Fields are Very Strange Compared to Earth's

These images show the Uranus-like (left) and Neptune-like (right) dynamo models for the ice giants. The tubes represent the magnetic fields, and the small gold arrows indicate the local field direction. Image Credit: Yan et al. 2026

Uranus and Neptune, the Solar System's ice giants, have interiors unlike the other planets. As a result, they also have magnetic fields unlike the others. They're messy and tilted, and Voyager 2, the only spacecraft to even flyby them, showed us how messy they are. New research uses models to try to understand what's going on with the pair of planets and their weird fields, and found that it's likely they change on very short timescales. They could already be much different than when Voyager 2 visited in the late 1980s.



Planets Don't Just Disappear, But They Can Wobble Out of Sight if Their Neighbour is Close Enough

This artist's illustration shows a hot Jupiter, a giant planet very close to its star with a very short orbital period. TESS watched one hot Jupiter transit its star for seven years, until it wasn't visible anymore. New research says that another nearby giant planet is responsible for tugging the hot Jupiter out of view. Image Credit: C. Carreau / ESA.

TESS watched an exoplanet about 1,000 light years away as it repeatedly transited in front of its star for seven years. But astronomers were surprised to find that the hot Jupiter disappeared. Of course, planets don't just disappear. Something interrupted its transits from our point of view, and astronomers think they've figured out what happened. An unseen, nearby giant planet companion tugged on it until TESS couldn't see it anymore.