Astronomers using the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) instruments are unveiling new scientific research that probes some of the most extreme environments in the universe. This news will be shared in press conferences at the 248th American Astronomical Society (AAS) meeting in Pasadena, June 14th-18th.
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NSF Green Bank Telescope Tunes in to Artemis II
World’s largest fully steerable radio telescope partners with NASA’s communications network to support tracking for historic lunar test flight
The National Science Foundation’s Green Bank Telescope (NSF GBT) will support NASA’s Artemis II mission by helping to track the crewed Orion spacecraft throughout its historic journey around the Moon.
As part of NASA’s Space Communications and Navigation (SCaN) program, the NSF GBT will support Artemis II tracking and communications, adding extra sensitivity and coverage to the networks that keep astronauts connected with Earth. Using its 100-meter collecting area and highly sensitive receivers, the NSF GBT will conduct radar observations of Orion as it travels beyond low Earth orbit, contributing precise tracking data that supports the mission’s safety and navigation. The GBT will provide support for the Artemis II mission for five days of the roughly 10-day test flight, observing Orion for six hours each day while the crew is closest to the Moon.
Artemis II is the first crewed flight test of NASA’s SLS (Space Launch System) rocket and Orion spacecraft, sending four astronauts on a lunar flyby to test life-support, communications, and other critical systems in deep space. This is the first crewed mission beyond low Earth orbit since 1972’s Apollo 17, and the first crewed lunar flyby in more than 50 years.
“These joint observations with the GBT give NASA a unique view of the Artemis II mission,” shares Will Armentrout, a scientist with the NSF GBO, who helps coordinate GBT operations for this project. All other observations of the mission around the world will be passive—with telescopes picking up the signals that Orion is emitting from its on-board antennas. The GBT will be performing active observations, using radar, with NASA’s Jet Propulsion Laboratory. A NASA Deep Space Network (DSN) antenna in California will beam radio energy toward the Orion spacecraft, and the GBT will pick up the extremely faint reflection of the energy off of the Orion spacecraft.
“Radar lets us pinpoint the trajectory of the spacecraft without relying on its on-board communication antennas,” explains Armentrout. “Performing radar observations at the distance of the Moon requires powerful transmitters and really, really big radio telescopes, like the GBT, so this partnership lets us spotlight some of the very best space support capabilities that the U.S. has to offer. We’re honored to work with NASA on the first crewed Moon mission in decades and look forward to even more collaboration as launch cadence increases!”
By partnering with SCaN, the NSF GBT continues its legacy of enabling groundbreaking space exploration—from studying distant galaxies to helping guide humanity’s return to the Moon. Most recently, the NSF GBT provided radar observations for NASA’s Double Asteroid Redirection Test, the world’s first “planetary protection” mission. Conversations are currently underway to provide ongoing support to NASA’s DSN. This collaboration underscores the importance of combining national research facilities with NASA’s spaceflight infrastructure and demonstrating how ground-based radio astronomy assets can directly support human exploration beyond Earth orbit.
About GBO and NRAO
The Green Bank Observatory is a part of the National Radio Astronomy Observatory (NRAO), 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 April 1, 2026.
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Astronomers using the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) instruments are unveiling new scientific research that probes some of the most extreme environments in the universe. This news will be shared in press conferences at the 248th American Astronomical Society (AAS) meeting in Pasadena, June 14th-18th.
Cosmic Dawn Fuel Discovery Unlocks Early Galaxy Growth Secrets
Astronomers have discovered a huge reservoir of cold molecular gas, the direct fuel for star formation, in REBELS-25, a massive, star-forming galaxy.
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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.