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Shredded stars reveal how black holes ignite trillion-sun flares Supermassive black holes are among the most enigmatic objects in the universe. They typically weigh millions or even billions of times the mass of the sun and sit at the centers of most large galaxies. At the heart of the Milky Way lies Sagittarius A*, our galaxy’s supermassive black hole, with a mass of about four million suns. But these black holes do not emit light, so astronomers can only detect them indirectly through their effects on nearby stars and gas. phys.org Go to SourceRead More →

Torsion balances set strongest direct limits yet on ultralight dark matter Dark matter is believed to make up a large fraction of the matter in the universe, yet its true nature remains unknown. Most past experiments have focused on heavier dark matter candidates, while much lighter dark matter, with masses closer to the mass of a neutrino, has been difficult to detect directly because its scattering signals are extremely weak. phys.org Go to SourceRead More →

Could dark matter be made of black holes from a different universe? New research suggests that relic black holes from before the big bang may still shape galaxies today. These black holes could explain dark matter, one of the biggest unsolved questions in cosmology. phys.org Go to SourceRead More →

The quietest place we’ve ever listened from We have been searching for signals from other civilizations for over sixty years. Radio telescopes on Earth have swept the sky, listened patiently, and found nothing but silence. It is a search that demands extraordinary sensitivity and that is the problem. Earth and our very existence itself are getting in the way. phys.org Go to SourceRead More →

Chandra explores interstellar medium of a bright low-mass X-ray binary Using NASA’s Chandra X-ray space telescope, astronomers have performed high-resolution X-ray spectroscopic observations of a bright low-mass X-ray binary known as GX 340+0. Results of the observational campaign, published April 3 on the arXiv pre-print server, shed more light on the composition of interstellar medium (ISM) in this system. phys.org Go to SourceRead More →

Information from starquakes provides theoretical evidence for ‘fossilized’ magnetism in stars For the first time, new theoretical models, published in Astronomy & Astrophysics, connect the magnetism at the surface of long-dead stellar remnants (white dwarfs) with recent evidence of magnetism at the cores of their dying progenitors (red giants). The team, led by astrophysicists at the Institute of Science and Technology Austria (ISTA), argues that these magnetic fields might originate early in the stars’ lives, and survive their entire evolution, emerging as “fossil fields” at the surfaces of older remnants. A better understanding of these processes can also help to better understand our own sun’sRead More →

Self-interacting dark matter may solve three cosmic puzzles A study led by UC Riverside physicist Hai-Bo Yu suggests that a new type of dark matter could explain three astrophysical puzzles across vastly different environments. Published in Physical Review Letters, the study proposes that dense clumps of self-interacting dark matter (SIDM)—each about a million times the mass of the sun—can account for unusual gravitational effects observed in gravitational lenses, stellar streams, and satellite galaxies. phys.org Go to SourceRead More →

Why do some stars in the galactic center survive while others are destroyed? The center of our galaxy is an extreme place. Surrounding the supermassive black hole Sagittarius A*, stars are packed densely into a region where gravity, radiation, and dark matter all interact in complex ways. It is a natural laboratory for testing some of the deepest ideas about astrophysics. phys.org Go to SourceRead More →

See and hear galaxies evolve from the dawn of the universe The most realistic picture yet of how galaxies formed and then evolved from the beginning of time has been revealed in a suite of new and unique audiovisual simulations. These data, accepted for publication in the Monthly Notices of the Royal Astronomical Society, show that the standard cosmological model can successfully explain the observed growth of galaxies, from the first billion years after the Big Bang to the present day, when key physics is included. phys.org Go to SourceRead More →

First Proba-3 science: Surprisingly speedy solar wind found in inner corona Since July 2025, the European Space Agency’s pair of Proba-3 satellites has already created 57 artificial solar eclipses. So far, the mission has collected more than 250 hours of high-resolution videos of the sun’s atmosphere, called the corona. That’s the same amount of observing time as about 5,000 total solar eclipse campaigns carried out on Earth. phys.org Go to SourceRead More →