On the Method to Infer an Atmosphere on a Tidally Locked Super Earth Exoplanet and Upper Limits to Gj 876d
We develop a method to infer or rule out the presence of an atmosphere on a tidally locked hot super Earth. The question of atmosphere retention is a fundamental one, especially for planets orbiting M stars due to the star's long-duration active phase and corresponding potential for stellar-ind...
| Auteurs principaux: | , |
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| Autres auteurs: | |
| Format: | Article |
| Langue: | en_US |
| Publié: |
IOP Publishing
2012
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| Accès en ligne: | http://hdl.handle.net/1721.1/74031 https://orcid.org/0000-0002-6892-6948 |