Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets

Temporal Evolution of the High-energy Irradiation and Water Content of TRAPPIST-1 Exoplanets

The ultracool dwarf star TRAPPIST-1 hosts seven Earth-size transiting planets, some of which could harbor liquid water on their surfaces. Ultraviolet observations are essential to measuring their high-energy irradiation and searching for photodissociated water escaping from their putative atmosphere...

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Bibliographic Details
Main Authors: Bourrier, V. (Author), Bolmont, E. (Author), Stamenković, V. (Author), Wheatley, P. J. (Author), Burgasser, A. J (Author), Delrez, L. (Author), Demory, B.-O (Author), Ehrenreich, D. (Author), Gillon, M. (Author), Jehin, E. (Author), Leconte, J. (Author), Lederer, S. M. (Author), Lewis, N. (Author), Triaud, A. H. M. J. (Author), Grootel, V. Van (Author), de Wit, Julien (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-11-21T20:47:13Z.
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