The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) and Johns Hopkins University (JHU) are thrilled to…


NSF National Radio Astronomy Observatory Collaborates with RIX Industries to Advance Cryogenic Cooling Technology for the Next Generation Very Large Array
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is excited to announce a collaboration with RIX Industries to explore innovative cryogenic cooling solutions for the Next Generation Very Large Array (ngVLA)

Lighting the Way: Cenca Bridge Wins Simons Foundation Funding for Expanding Astronomy Opportunities
Cenca Bridge, an internationally recognized nonprofit organization dedicated to fostering scientific research and education among marginalized students in Central…

NSF NRAO Achieves First Successful Observations with New NSF VLBA Digital Architecture
The new NSF VLBA New Digital Architecture (VNDA) produced its first fringes and subsequent images in January 2025, demonstrating the successful implementation of next-generation technology that will enhance the NSF VLBA’s scientific capabilities for years to come.

Image Release: the ngVLA Prototype Handover Ceremony
mtex antenna technology GmbH officially handed over the prototype antenna for the proposed Next Generation Very Large Array (ngVLA) to the U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) at a ceremony held at the NSF Very Large Array site on the Plains of San Agustin, New Mexico.

Unveiling the Birth Secrets of Massive Stars with the NSF NRAO Very Large Array
By observing the young star HW2 in Cepheus A, located 2300 light years from Earth, researchers have resolved the structure and dynamics of an accretion disk feeding material to this massive star. This finding sheds light on a central question in astrophysics: how do massive stars, which often end their lives as supernovae, accumulate their immense mass?