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Gaze into the Crystal Ball Nebula and See the Light Emitted by a Dying Star 1500 Years Ago

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NASA Ames Experts Available for Roman Space Telescope Interviews

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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Brookhaven and Stony Brook Researchers Demonstrate 'Wireless' Capability for Quantum Network

Researchers have successfully transmitted light particles containing quantum information through open air between Brookhaven Lab and Stony Brook University.

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Twisted Physics: Astronomers Solve 30-Year-Old Stellar Mystery

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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A Trillion Mile Cosmic Stream of Gas Feeds GW Orionis

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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NSF NRAO radio observations help rule out a relativistic jet in rare stellar explosion

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U.S. National Science Foundation, NSF National Radio Astronomy Observatory, and U.S. Naval Observatory Partner on Pathfinder for Next Generation Very Large Array

The U.S. National Science Foundation (NSF), the NSF National Radio Astronomy Observatory (NSF NRAO), and the U.S. Naval Observatory (USNO) are advancing a new collaboration to support the future of high-resolution radio astronomy and astrometry, with the development of a pathfinder instrument for the proposed Next Generation Very Large Array (ngVLA). The post U.S. National Science Foundation, NSF National Radio Astronomy Observatory, and U.S. Naval Observatory Partner on Pathfinder for Next Generation Very Large Array appeared first on National Radio Astronomy Observatory .

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