Tuesday, June 30, 2026

Habitable Worlds Targets in New Star Activity Catalog

Artist's rendition of the planned Habitable Worlds Observatory. (Credit: NASA)

Searching for habitable worlds beyond our solar system consists of more than just having it orbit within its star’s habitable zone, which is the region where temperatures could be just right for liquid water to exist on the surface. On Earth, where water comprises approximately 75 percent of the planet’s surface, life is absurdly abundant. But what about the exoplanet’s star, specifically its activity and rotation? How could this influence how exoplanets are identified for current and future missions?



Astronomers Discover Another Galaxy With No Dark Matter

![The full trail of galaxies, with an inset image of DF9 taken by the Hubble Space Telescope. Credit: Keim et al. (2026)/DECaLS/HST](/article_images/YN_DF9-drak-galaxy_20260630_213201.jpg) *The full trail of galaxies, with an inset image of DF9 taken by the Hubble Space Telescope. Credit: Keim et al. (2026)/DECaLS/HST*

Astronomers using W. M. Keck Observatory on Maunakea, Hawaiʻi Island, have discovered the third known galaxy apparently lacking dark matter, part of a strange linear structure that may have formed during a violent collision between galaxies.



Nautilus Array to Track Missing Exoplanet Atmospheres

Illustration depicting the Nautilus Space Observatory constellation, which is a mission concept that could enhance the study of exoplanet atmospheres. (Credit: Nautilus team)

Exoplanet atmospheres have become prima targets for astrobiologists in the search for life beyond Earth. This is because exoplanet surfaces can’t be directly imaged yet, so astronomers must get creative with how to search for signs of life, also called biosignatures. Presently, powerful ground- and space-based telescopes like the Atacama Large Millimeter Array (ALMA) and NASA’s James Webb Space Telescope (JWST) are improving in their ability to observe and analyze exoplanet atmospheres. But did these atmospheres form and evolve, and what could this mean for the search for life beyond Earth?



It's Finally Begun! The Vera Rubin Observatory Creating What Will Be the Greatest Movie Ever Made

This is a 1.7 gigapixel image of stars in the constellation Lupus from the VRO and its LSST Camera. This is the largest digital camera in the world, and with it, the VRO can capture wide images of the sky in extreme detail. The VRO's long-awaited 10-year survey of the sky has now begun. Image Credit: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA

The Vera Rubin Observatory's long-awaited Legacy Survey of Space and Time has begun. This decade-long movie of the cosmos will capture anything that changes brightness, position, or both in the southern night sky. It will study grand subjects like dark energy and dark matter, and important things closer to home like near-Earth objects.



Monday, June 29, 2026

ESA’s ExoMars Trace Gas Orbiter Has Yet to Detect Methane On Mars

NASA's Curiosity Mars rover took this selfie on May 12, 2019. Credit:  NASA/JPL-Caltech/MSSS.

After more than eight years of searching and with instruments designed to detect it, the European Space Agency’s (ESA) Mars Trace Gas Orbiter has yet to find methane in the red planet’s atmosphere.



The "Shadow Blaster" Galaxy's Role in High-energy Cosmic Neutrinos

A conceptual view of the neutrino accelerator in the starburst galaxy “Shadow Blaster”. It lies in the same direction as the high-energy neutrino event IC 210922A. Actual radio observations by ALMA are shown in the zoom-in inset. Due to gravitational lensing, the ALMA observations show four distorted images of Shadow Blaster, which has been identified as the source of the neutrinos (indicated by the Greek letter nu). An artist’s conception of Shadow Blaster’s true appearance is shown in the circle. Credit: MITOS

On September 22, 2021, the IceCube Neutrino Detector in Antarctica caught a blast of neutrinos as it passed through the solar system. These neutrinos were remarkably high-energy and came from a galaxy 11 billion light-years away. That's a period of the Universe's history known as "Cosmic Noon". It's when star formation in galaxies was at its most active and that provided an interesting clue to their origin. The source of the neutrinos was nicknamed "Shadow Blaster" because the event that created the neutrinos was hidden by a dense cloud of dust, which made it invisible to optical observations.



An Alternative to Black Holes: Gravastars with Big Bangs Inside

The problem with stellar mass black holes is that general relativity can't account for their strangeness. But the theoretical gravastars, an alternative to black holes, don't clash with general relativity in the same way. Nobody has figured out how they could form through Einstein's equations, until now. Image Credit: Daniel Jampolski and Luciano Rezzolla, Goethe University Frankfurt

Stellar mass black holes may not be black holes at all. Instead, they could be a type of extremely compact star called a gravastar, which mimics a black hole. This is according to theoretical phsyicists who have discovered a solution to Einstein's Theory of General Relativity that doesn't automatically result in a black hole when a star collapses at the end of its life.