Particle interaction could be interpreted as a signal from a dark matter candidate — but more data is needed.
Space & AstronomyParticle PhysicsLife Sciences#Brookhaven National Laboratory#astronomy#astrophysics#Particle Physics#High Energy Physics#genomics#biology#climate
NASA’s Ames Research Center in California’s Silicon Valley invites media to learn more about NASA’s Nancy Grace Roman Space Telescope, scheduled to launch Sunday, Aug. 30, 2026, from NASA’s Kennedy Space Center in Florida. The Roman telescope will provide a wide, detailed view of the universe, helping scientists study dark energy, exoplanets, and cosmic structures. […]
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Researchers have successfully transmitted light particles containing quantum information through open air between Brookhaven Lab and Stony Brook University.
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Press ReleasesNational Radio Astronomy Observatory
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is a partner, have captured the first direct, high-resolution images of a magnetic field wrapped tightly around the outflow of gas streaming away from a forming star — evidence that solves a decades-old puzzle about how young stars sculpt the powerful jets that form them. The post Twisted Physics: Astronomers Solve 30-Year-Old Stellar Mystery appeared first on National Radio Astronomy Observatory .
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Press ReleasesNational Radio Astronomy Observatory
A team of astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA), of which the U.S. National Science Foundation National Radio Astronomy Observatory is a partner, has captured a massive stream of gas—one trillion miles, or .2 light years long—feeding the young triple-star system GW Orionis. These new observations provide the clearest evidence yet for how such “streamers” can tilt and twist the disks where planets are born. The post A Trillion Mile Cosmic Stream of Gas Feeds GW Orionis appeared first on National Radio Astronomy Observatory .
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Press ReleasesNational Radio Astronomy Observatory
Astronomers studying a rare stellar explosion first spotted as a brief burst of X-rays used radio observations to help show that the dying star did not produce the powerful jet often associated with gamma-ray bursts. The post NSF NRAO radio observations help rule out a relativistic jet in rare stellar explosion appeared first on National Radio Astronomy Observatory .
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