Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) 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.
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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.
NSF NRAO radio observations help rule out a relativistic jet in rare stellar explosion
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.
University of Florida and NSF NRAO Forge Path for Discovery
Pictured from left to right Eric Murphy (NSF NRAO ngVLA Project Scientist), Anna-Lisa Paul (UF Interdisciplinary Center for Biotechnology Research Director), Tony Beasley (NSF NRAO Director), and Robert Ferl (UF Astraeus Space Institute Director) in front of ngVLA prototype antenna. Credit: NSF/AUI/NSF NRAO
New partnership brings the future of astronomy and science education, inspiring students and communities
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) and the University of Florida (UF) have announced a dynamic new partnership to advance science education and public outreach at a future Next Generation Very Large Array (ngVLA) antenna site in Florida.
This collaboration, signed with a Memorandum of Understanding (MOU) at the debut of the ngVLA prototype antenna in New Mexico last week, brings together world-class scientific expertise and educational leadership to create unique opportunities for students, educators, and the public across Florida. If constructed, the ngVLA, a flagship project recommended by the Astro2020 Decadal Survey, would be the most advanced radio telescope of its kind, capable of probing the universe with unprecedented sensitivity and resolution
The ngVLA Florida LONG station—one of 10 such planned sites nationwide—will not only contribute to groundbreaking discoveries in astronomy and physics but also serve as a hub for hands-on science education, STEM training, and community engagement. The partnership envisions:
- Innovative educational programs for K-12, high school, and university students
- Public outreach events and a potential visitor center to inspire curiosity in science
- Research and training opportunities for UF students, including engineering and astronomy projects
- Site-based science activities and technology demonstrations for all ages
Potential locations for the Florida ngVLA antenna include UF-affiliated sites such as the Southwest Florida Research and Education Center in Immokalee,the Everglades Research and Education Center in Belle Glade and the DeLuca Preserve in Yeehaw Junction, ensuring deep local ties and broad accessibility.
“By uniting the cutting-edge resources of NRAO with the educational mission of UF, this partnership will spark discovery, empower future scientists, and ensure Florida plays a leading role in the next era of astronomical exploration,” said Robert Ferl, distinguished professor and director of the UF Astraeus Space Institute.
The NSF NRAO is actively engaged in conversations with other universities to identify locations for other ngVLA antenna LONG stations. “There is enormous potential for these collaborations to create even more educational opportunities for students and communities across the country,” adds NSF NRAO ngVLA project scientist Eric Murphy, “We’re excited to be formalizing our plans and signing MOUs with other universities soon.”
About NRAO
The National Radio Astronomy Observatory and the Green Bank Observatory are major facilities 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 April 29, 2025.
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Twisted Physics: Astronomers Solve 30-Year-Old Stellar Mystery
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) 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.
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.
NSF NRAO radio observations help rule out a relativistic jet in rare stellar explosion
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.