ngVLA: Together We See More

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ngVLA: Together We See More

The Atacama Large Millimeter/submillimeter Array (ALMA) has shown us young star systems where planets are forming. The next-generation Very Large Array will go even deeper, observing Earth-size bodies in their youth. It will reveal how planets clear gaps in cold, dusty planetary disks. The ngVLA will also study how stellar winds clear primordial gas and dust from star systems.

Credit: NRAO/AUI/NSF

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More ngVLA Images & Videos

ngVLA Antenna Model for AR

Pebbles to Planets

Black Holes and Neutron Stars: ngVLA Key Science Goal 5

Understanding Gravity: ngVLA Key Science Goal 4

Galaxy Evolution: ngVLA Key Science Goal 3

Cosmic Origins of Life: ngVLA Key Science Goal 2

Young Planetary Systems: ngVLA Key Science Goal 1

ngVLA Artist Impressions: Galactic Ecosystem

The National Radio Astronomy Observatory is a facility of the U.S. National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
	Founded in 1956, the NRAO provides state-of-the-art radio telescope facilities for use by the international scientific community. NRAO telescopes are open to all astronomers regardless of institutional or national affiliation. Observing time on NRAO telescopes is available on a competitive basis to qualified scientists after evaluation of research proposals on the basis of scientific merit, the capability of the instruments to do the work, and the availability of the telescope during the requested time. NRAO also provides both formal and informal programs in education and public outreach for teachers, students, the general public, and the media.
	The U.S. National Science Foundation (NSF) is an independent federal agency created by Congress in 1950 "to promote the progress of science; to advance the national health, prosperity, and welfare; to secure the national defense..."
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