Recent advancements in 3D printing (also known as additive manufacturing) for metallic structures make it possible to print all-metal electromagnetic devices—like antennas and waveguides—on demand. A new partnership between the National Radio Astronomy Observatory, headquartered in Charlottesville, Virginia, and Optisys, LLC, headquartered in West Valley City, Utah, will explore the potential for leveraging this technology for radio astronomy applications.
Retaining and promoting female talent in science, technology, engineering, and mathematics (STEM) is a goal that must be embraced by large scientific facilities, civil society, academia, and the private sector. A STEM career can be long and full of obstacles for underrepresented minorities, including women, who are strongly influenced by family expectations, teacher bias, and work environments plagued by stereotypes. More female role models in STEM are needed to inspire and increase women’s participation, and they are currently insufficient to retain female employees and stimulate their professional growth into leadership positions.
An NRAO researcher is receiving an engineering award for an innovative development that is improving radio telescope performance and also is benefitting numerous other fields.
The formation of massive stars and planets. The deaths of stars and galaxies. The extreme and violent behaviors of black hole jets and quasars. An up-close and personal radar view of the Moon. These mysteries and more were unraveled in 2021 by radio astronomers leveraging the scientific and technological power of National Radio Astronomy Observatory (NRAO) facilities.
Dr. Tony Beasley, Director of the National Radio Astronomy Observatory and AUI Vice President for Radio Astronomy Operations, was today elected as a fellow of the American Association for the Advancement of Science (AAAS).
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA) and the Karl G. Jansky Very Large Array (VLA) made a rare detection of a likely stellar flyby event in the Z Canis Majoris (Z CMa) star system. An intruder—not bound to the system—object came in close proximity to and interacted with the environment surrounding the binary protostar, causing the formation of chaotic, stretched-out streams of dust and gas in the disk surrounding it.
