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Proceedings Paper

The Habitable Exoplanet (HabEx) Imaging Mission: preliminary science drivers and technical requirements
Author(s): Bertrand Mennesson; Scott Gaudi; Sara Seager; Kerri Cahoy; Shawn Domagal-Goldman; Lee Feinberg; Olivier Guyon; Jeremy Kasdin; Christian Marois; Dimitri Mawet; Motohide Tamura; David Mouillet; Timo Prusti; Andreas Quirrenbach; Tyler Robinson; Leslie Rogers; Paul Scowen; Rachel Somerville; Karl Stapelfeldt; Daniel Stern; Martin Still; Margaret Turnbull; Jeffrey Booth; Alina Kiessling; Gary Kuan; Keith Warfield
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Paper Abstract

HabEx is one of four candidate flagship missions being studied in detail by NASA, to be submitted for consideration to the 2020 Decadal Survey in Astronomy and Astrophysics for possible launch in the 2030s. It will be optimized for direct imaging and spectroscopy of potentially habitable exoplanets, and will also enable a wide range of general astrophysics science. HabEx aims to fully characterize planetary systems around nearby solar-type stars for the first time, including rocky planets, possible water worlds, gas giants, ice giants, and faint circumstellar debris disks. In particular, it will explore our nearest neighbors and search for signs of habitability and biosignatures in the atmospheres of rocky planets in the habitable zones of their parent stars. Such high spatial resolution, high contrast observations require a large (roughly greater than 3.5m), stable, and diffraction-limited optical space telescope. Such a telescope also opens up unique capabilities for studying the formation and evolution of stars and galaxies. We present some preliminary science objectives identified for HabEx by our Science and Technology Definition Team (STDT), together with a first look at the key challenges and design trades ahead.

Paper Details

Date Published: 24 August 2016
PDF: 10 pages
Proc. SPIE 9904, Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave, 99040L (24 August 2016); doi: 10.1117/12.2240457
Show Author Affiliations
Bertrand Mennesson, Jet Propulsion Lab. (United States)
Scott Gaudi, Jet Propulsion Lab. (United States)
The Ohio State Univ. (United States)
Sara Seager, Massachusetts Institute of Technology (United States)
Kerri Cahoy, The Ohio State Univ. (United States)
Shawn Domagal-Goldman, NASA Goddard Space Flight Ctr. (United States)
Lee Feinberg, NASA Goddard Space Flight Ctr. (United States)
Olivier Guyon, The Univ. of Arizona (United States)
Jeremy Kasdin, Princeton Univ. (United States)
Christian Marois, NRC, Herzberg Institute of Astrophysics (Canada)
Dimitri Mawet, California Institute of Technology (United States)
Motohide Tamura, The Univ. of Tokyo (Japan)
National Astronomical Observatory of Japan (Japan)
David Mouillet, Institut de Planétologie et d’Astrophysique de Grenoble (France)
Timo Prusti, European Space Agency (Netherlands)
Andreas Quirrenbach, Landessternwarte Heidelberg (Germany)
Tyler Robinson, Univ. of Washington (United States)
Leslie Rogers, Univ. of Chicago (United States)
Paul Scowen, Arizona State Univ. (United States)
Rachel Somerville, Rutgers Univ. (United States)
Karl Stapelfeldt, Jet Propulsion Lab. (United States)
Daniel Stern, Jet Propulsion Lab. (United States)
Martin Still, NASA Headquarters (United States)
Margaret Turnbull, Global Science Institute (United States)
Jeffrey Booth, Jet Propulsion Lab. (United States)
Alina Kiessling, Jet Propulsion Lab. (United States)
Gary Kuan, Jet Propulsion Lab. (United States)
Keith Warfield, Jet Propulsion Lab. (United States)

Published in SPIE Proceedings Vol. 9904:
Space Telescopes and Instrumentation 2016: Optical, Infrared, and Millimeter Wave
Howard A. MacEwen; Giovanni G. Fazio; Makenzie Lystrup; Natalie Batalha; Nicholas Siegler; Edward C. Tong, Editor(s)

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