Science with a next-generation Very Large Array
The ngVLA will have broad impact on many of the high priority goals of modern astronomy & astrophysics, including the science priorities described in the New Worlds, New Horizons Astro2010 Decadal Survey. The ngVLA Science Working Groups (SWGs) have identified a number of key science programs that push the requirements of the telescope through a community driven Science Use Case capture exercise that is led by the ngVLA Science Advisory Council (SAC). Community members are still encouraged to submit additional Science Use Cases and to coordinate a contributed to the ngVLA Science Book with the appropriate SWG chair.
If you are interested in joining one of the SWGs, please contact the corresponding Science Working Group Chair directly. An initial set of science goals suggested by the four SWGs are described in white papers published in the ngVLA Memo Series.
ngVLA Key Science Goals (KSGs)
The ngVLA will measure the planet initial mass function down to a mass of 5–10 Earth masses and unveil the formation of planetary systems similar to our own Solar System by probing the presence of planets on orbital radii as small as 0.5 AU at the distance of 140 pc. The ngVLA will also reveal circumplanetary disks and sub-structures in the distribution of mm-size dust particles created by close-in planets and will measure the orbital motion of these features on monthly timescales.
The ngVLA will be able to detect predicted, as yet unobserved, complex prebiotic species that are the basis of our understanding of chemical evolution toward amino acids and other biogenic molecules. It will also allow us to detect and study chiral molecules, to include testing ideas on the origins of homochirality in biological systems. The detection of such complex organic molecules will provide initial chemical conditions data of forming solar systems and individual planets.
KSG3: Charting the Assembly, Structure, and Evolution of Galaxies from the First Billion Years to the Present
The ngVLA will provide an order-of-magnitude improvement in depth and area for surveys of cold gas in galaxies back to early cosmic epochs, and it will enable routine sub-kiloparsec scale resolution imaging of the gas reservoirs. The ngVLA will afford a unique view into how galaxies accrete and expel gas and how this gas is transformed inside galaxies. It does so by imaging their extended atomic reservoirs and circum-galactic regions, and by surveying the physical and chemical properties of molecular gas over the entire local galaxy population. These studies will reveal the detailed physical conditions for galaxy assembly and evolution throughout the history of the universe.