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...

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Bibliographic Details
Main Authors: Seager, Sara (Contributor), Deming, Drake (Author)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2012-10-16T18:00:24Z.
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