New radio images from the the U.S. National Science Foundation Very Large Array trace a pair of powerful plasma jets launched by galaxy VV 340a’s central supermassive black hole, which appear to be driving hot coronal gas out of the galaxy and shutting down future star formation.
Recent News
Radio Telescopes Uncover ‘Invisible’ Gas Around Record-Shattering Cosmic Explosion
Astronomers using the U.S. National Science Foundation Very Large Array and the Atacama Large Millimeter/submillimeter Array have revealed a dense cocoon of gas around one of the most extreme cosmic explosions ever seen, showing that a ravenous black hole ripped apart a massive star and then lit up its surroundings with powerful X-rays.
New Discovery Challenges Evolution of Galaxy Clusters
Peering back in time, around 12 billion years, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found the most distant and direct evidence of scorching gas in a forming galaxy cluster, SPT2349-56. The hot plasma, seen when the Universe was just 1.4 billion years old, is far hotter and more pressurized than current theories predicted for such an early system.
NSF Facilities Partner to Transform Data Processing for Next-Generation Radio Astronomy
NSF NRAO, NSF LCCF partnership will deliver state-of-the-art system to handle unprecedented volume of data produced by ngVLA telescope
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) has entered into a groundbreaking partnership with the NSF Leadership-Class Computing Facility (NSF LCCF), led by the Texas Advanced Computing Center, to pioneer a transformative data processing system for the next era of radio astronomy.
The partnership is in direct response to the astronomical data volumes anticipated from the upcoming Next Generation Very Large Array (ngVLA) project, which is expected to produce up to 40 petabytes (PB) of data each month—orders of magnitude greater than any of the current NRAO telescopes. . This scale will place NRAO at the forefront of data-intensive scientific exploration not just in astronomy, but across the broader scientific community.
“Radio astronomy is on the brink of a data revolution,” said Tony Beasley, Director of the NRAO. “Our next-generation facility will open new windows on the Universe, but the ability to manage, process, and analyze these immense data streams is essential to delivering the scientific breakthroughs we seek. Teaming up with the NSF LCCF, led by our partners at TACC, ensures our scientists will have access to computation and infrastructure on par with the world’s largest research efforts and technology companies.”
To meet these challenges, NSF NRAO is developing an advanced radio astronomy data processing system designed to harness and make sense of the flood of information expected from ngVLA. Unlike anything NRAO has undertaken before, this data ecosystem will operate on the scale of the world’s top supercomputing centers, incorporating high-performance computing, state-of-the-art data transport systems, cutting edge scalable and parallelizable algorithms, and advanced data management solutions.
TACC, an NSF Major Research Equipment and Facilities Construction (MREFC) site, is leading the U.S. NSF Leadership-Class Computing Facility, a next-generation powerhouse set to transform computational research when it launches in 2026. In partnership with NRAO astronomers, TACC experts are engineering end-to-end workflows for seamless data movement, storage, and computation. This effort includes a comprehensive conceptual design and close collaboration with NRAO’s software team to accurately forecast and meet their future computing demands.
“As observational astronomy enters the exascale era, computing and data continue to grow in importance for scientific discovery,” said Dan Stanzione, Executive Director of TACC. “The NSF Leadership-Class Computing Facility is pleased to assist with defining the cyberinfrastructure workflows needed by NSF’s largest radio astronomy instruments. In helping to assess the needed capacities and tradeoffs, the LCCF will be able to assist ngVLA to address some of the universe’s deepest mysteries.”
Currently no astronomy facility has operated at this magnitude of sustained data flow. The planned infrastructure will allow NRAO to enable next-generation discoveries for astronomers across the country.
For more details about this partnership and updates on the project’s progress, please visit NRAO News and TACC.
About NRAO
The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.
This news article was originally published on the NRAO website on August 26, 2025.
Recent News
The NSF Very Large Array Helps Reveal Record-Breaking Stream of Super-Heated Gas from Nearby Galaxy
New radio images from the the U.S. National Science Foundation Very Large Array trace a pair of powerful plasma jets launched by galaxy VV 340a’s central supermassive black hole, which appear to be driving hot coronal gas out of the galaxy and shutting down future star formation.
Radio Telescopes Uncover ‘Invisible’ Gas Around Record-Shattering Cosmic Explosion
Astronomers using the U.S. National Science Foundation Very Large Array and the Atacama Large Millimeter/submillimeter Array have revealed a dense cocoon of gas around one of the most extreme cosmic explosions ever seen, showing that a ravenous black hole ripped apart a massive star and then lit up its surroundings with powerful X-rays.
New Discovery Challenges Evolution of Galaxy Clusters
Peering back in time, around 12 billion years, astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have found the most distant and direct evidence of scorching gas in a forming galaxy cluster, SPT2349-56. The hot plasma, seen when the Universe was just 1.4 billion years old, is far hotter and more pressurized than current theories predicted for such an early system.