Thursday, January 15, 2026

Red Dwarfs Are Too Dim To Generate Complex Life

This artist's illustration shows what the view might be from the surface of TRAPPIST-1f. It orbits a dim red dwarf star, and new research examines the idea that photosynthesis could occur in such dim, weak light. Without it, complex life is extremely unlikely. Image Credit: Mark Garlick

New research shows that complex life is unlikely to ever exist around cool, dim red dwarfs. About 33% of the Milky Way's stars are late M dwarfs, which are the smallest, coolest stars, and are the easiest stars to detect Earth-like planets around. The stars aren't bright enough for photosynthetic organisms to create a Great Oxygenation Event, which led to complex animal life here on Earth.



A New Atlas of the Milky Way’s Ghost Particles

The inside of the MiniBooNE neutrino detector (Credit : Fred Ulrich)

Every second, a trillion ghost particles stream through your body unnoticed, invisible messengers carrying secrets from the hearts of distant stars. Astrophysicists at the University of Copenhagen have now mapped exactly where these neutrinos originate across our Milky Way Galaxy and how many reach Earth, creating the most comprehensive picture yet of these elusive particles.



Wednesday, January 14, 2026

Two New Exoplanets And The Need For New Habitable Zone Definitions

This artist's illustration shows the exoplanets that orbit the small red dwarf Kepler-42. Second from the star is Kepler-42b, a rocky exoplanet about the size of Mars. Researchers are refining their search for habitable planets by developing the idea of temperate zone exoplanets. They're planets like Kepler-42b, that are both easily detected with the transit method, and are at the right distance for potential habitability as well as atmospheric characterization by the JWST. Image Credit: By NASA/JPL-Caltech - http://www.nasa.gov/mission_pages/kepler/multimedia/images/mini-planetary-system.html, Public Domain, https://commons.wikimedia.org/w/index.php?curid=18013575

How solid is our understanding of exoplanet habitability? Are the ideas of an Optimistic Habitable Zone and a Conservative Habitable Zone sufficient to advance our understanding? New research introduces an expanded exoplanet 'temperate zone,' highlighting planets that are amenable to atmospheric study by the JWST.



Solving the Mystery of Blue Flashes

Artist illustration of a Luminous Fast Blue Optical Transient (Credit : Bill Saxton, NRAO/AUI/NSF)

Brief, brilliant flashes of blue light occasionally appear across the universe, burning hundreds of times brighter than ordinary supernovae before fading within days. Astronomers have puzzled over these luminous fast blue optical transients for years, unable to determine whether they were unusual stellar explosions or something else entirely. Observations of AT 2024wpp, the brightest example ever detected, have finally solved the mystery.



Tuesday, January 13, 2026

When Baby Stars Throw Tantrums

HH80/81, Jets of ionised gas streak from a newly forming star (Credit : NASA, ESA, and B. Reipurth)

NASA’s Hubble Space Telescope has captured stunning new image of HH 80/81, a pair of objects created when supersonic jets from a newborn star slam into previously expelled gas clouds, heating them to extreme levels. These jets, powered by a protostar 20 times more massive than our Sun, stretch over 32 light years through space and travel at speeds exceeding 1,000 kilometres per second, making them the fastest outflows ever recorded from a young star.



Young Stellar Objects Are Prominent In A New Hubble Image

This Hubble image of NGC 1333, a reflection nebula about 1,000 light-years away, features multiple young stellar objects, including a young protostar with an edge-on view of its protoplanetary disk. Image Credit: NASA, ESA, K. Stapelfeldt (Jet Propulsion Laboratory) and D. Watson (University of Rochester); Processing: Gladys Kober (NASA/Catholic University of America)

A disparate collection of young stellar objects bejewels a cosmic panorama in the star-forming region NGC 1333 in this new image from NASA’s Hubble Space Telescope. To the left, an actively forming star called a protostar casts its glow on the surrounding gas and dust, creating a reflection nebula. Two dark stripes on opposite sides […]



Siwarha's Wake Gives it Away at Betelgeuse

This artist’s concept shows the red supergiant star Betelgeuse and its orbiting companion star. The companion orbits clockwise from this point of view. As it moves through the dense atmosphere, it generates a dense wake of gas that expands outward. The companion’s distance from Betelgeuse is to scale relative to the diameter of Betelgeuse. Artwork: NASA, ESA, Elizabeth Wheatley (STScI); Science: Andrea Dupree (CfA)

Betelgeuse is the star that everybody can't wait to see blow up, preferably sooner than later. That's because it's a red supergiant on the verge of becoming a supernova and there hasn't been one explode this close in recorded human history. It's been changing its brightness and showing strange surface behavior, which is why astronomers track its activity closely. Are these changes due to its aging process? Do they mean it's about to blow up? Probably not.