Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have finally found clear evidence that the supermassive black hole at the center of the Milky Way, Sagittarius A*(Sgr A*), is blowing a hot cosmic wind – something scientists have been hunting for over 50 years.
Recent News
AUI Announces 2026 Scholarship Recipients
Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.
NSF Green Bank Observatory Shares Images, Data From Artemis II Mission
The pixels in the data in the upper left represent the Orion spacecraft. The vertical (range) axis indicates distance to the spacecraft with distance increasing downward in the image. The horizontal (Doppler) axis indicates a frequency shift from the expected return signal. This image of the Orion capsule was created while the spacecraft was over 213k miles (343k km) from Earth. Shared Will Armentrout, an NSF GBO scientist presenting to colleagues at the NSF GBO, “There are four people in those pixels.” Image credit: Data credit: JPL & NSF/AUI/NSF NRAO. Photo credit: NSF/AUI/NSF NRAO/J.Hellerman.
Radar signals received by world’s largest fully steerable radio telescope tracked spacecraft with NASA’s communications network for historic lunar test flight
The U.S. National Science Foundation Green Bank Telescope (NSF GBT) produced these data and images while supporting NASA’s Artemis II mission by helping to track the crewed Orion spacecraft throughout its historic journey around the Moon. The NSF GBT conducted five observations over the same number of days, for six hours each day, that the spacecraft was closest to the Moon, and farthest from the Earth at over 200,000 miles away.
“With the GBT, we were able to track the movement of the spacecraft within 0.2 millimeters per second of what NASA calculated in its projections,” shared Anthony Remijan, site director of the NSF Green Bank Observatory, “It’s like having a speedometer in your car that can track your speed within 0.0004 decimal places per hour.”
Besides supporting NASA’s Space Communications and Navigation (SCaN) program during the Artemis II mission, this work provided evidence of the important support the NSF GBT and the NSF National Radio Astronomy Observatory (NSF NRAO) can offer future space missions, for NASA and commercial aerospace companies. The NSF GBT provided radar support to NASA’s Double Asteroid Redirection Test (DART), and the NSF Very Long Baseline Array (NSF VLBA) provided precise tracking and data downlink of Intuitive Machines’ Nova-C lunar lander, Athena, during its mission to the Moon.
”It’s exciting when projects like this put our NSF facilities in national headlines,” adds Linnea Avallone, NSF Chief Officer for Research Facilities, “Being able to offer inter-agency support to our colleagues at NASA makes the most of all our capabilities.”
About NRAO
The Green Bank Observatory is a part of the National Radio Astronomy Observatory, a major 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 May 6, 2026.
Recent News
Milky Way’s Black Hole Finally Caught ‘Breathing’
Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have finally found clear evidence that the supermassive black hole at the center of the Milky Way, Sagittarius A*(Sgr A*), is blowing a hot cosmic wind – something scientists have been hunting for over 50 years.
AUI Announces 2026 Scholarship Recipients
Ten high school students have been awarded for academic achievement, community involvement and leadership skills.
NSF NRAO Leads Future of U.S. Radio Astronomy with First Light from Next Generation Very Large Array Prototype
The proposed array’s design will improve on the sensitivity and spatial resolution—with 10 times the effective collecting area and resolution—over the current NSF VLA and the Atacama Large Millimeter/submillimeter Array at the same wavelengths.