Published June 19, 2019
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Imaging Cool Giant Planets in Reflected Light: Science Investigations and Synergy with Habitable Planets
- Creators
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Marley, Mark
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Lewis, Nikole
- Arney, Giada
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Bailey, Vanessa
- Batalha, Natasha
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Beichman, Charles
- Benneke, Björn
- Blecic, Jasmina
- Cahoy, Kerri
- Chilcote, Jeffrey
- Domagal-Goldman, Shawn
- Dressing, Courtney
- Fitzgerald, Michael
- Fortney, Jonathan
- Freedman, Richard
- Gelino, Dawn
- Gizis, John
- Guyon, Olivier
- Greene, Thomas
- Hammel, Heidi
- Hasegawa, Yasuhiro
- Jovanovic, Nemanja
- Konopacky, Quinn
- Kopparapu, Ravi
- Liu, Michael
- Lopez, Eric
- Lunine, Jonathan
- Lupu, Roxana
- Macintosh, Bruce
- Mandt, Kathleen
- Marois, Christian
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Mawet, Dimitri
- Mayorga, Laura
- Morley, Caroline
- Nielsen, Eric
- Roberge, Aki
- Serabyn, Eugene
- Skemer, Andrew
- Stapelfeldt, Karl
- Visscher, Channon
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Wang, Jason
Abstract
Planned astronomical observatories of the 2020s will be capable of obtaining reflected light photometry and spectroscopy of cool extrasolar giant planets. Here we explain that such data are valuable both for understanding the origin and evolution of giant planets as a whole and for preparing for the interpretation of similar datasets from potentially habitable extrasolar terrestrial planets in the decades to follow.
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Additional details
- Eprint ID
- 96561
- Resolver ID
- CaltechAUTHORS:20190619-110958838
- Created
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2019-06-19Created from EPrint's datestamp field
- Updated
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2023-06-02Created from EPrint's last_modified field
- Caltech groups
- Astronomy Department
- Series Name
- Astro2020 Science White Paper