The Transiting Exoplanet Survey Satellite

Author(s)
Ricker, George R; Vanderspek, Roland K; Seager, Sara; Levine, Alan M; Villasenor, Jesus N S.; ... Show more
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Abstract
The Transiting Exoplanet Survey Satellite (TESS) will discover thousands of exoplanets in orbit around the brightest stars in the sky. This first-ever spaceborne all-sky transit survey will identify planets ranging from Earth-sized to gas giants. TESS stars will be far brighter than those surveyed by previous missions; thus, TESS planets will be easier to characterize in follow-up observations. For the first time it will be possible to study the masses, sizes, densities, orbits, and atmospheres of a large cohort of small planets, including a sample of rocky worlds in the habitable zones of their host stars.
Date issued
2016-08
URI
http://hdl.handle.net/1721.1/114884
Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences; MIT Kavli Institute for Astrophysics and Space Research
Journal
Proceedings Volume 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Publisher
SPIE
Citation
Ricker, G. R., et al. "The Transiting Exoplanet Survey Satellite." Proceedings Volume 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 26 June - July 6, 2016, Edinburgh, United Kingdom, edited by Howard A. MacEwen et al., SPIE, 2016, p. 99042B. © 2016 SPIE
Version: Final published version
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