Theoretical spectra of terrestrial exoplanet surfaces

We investigate spectra of airless rocky exoplanets with a theoretical framework that self-consistently treats reflection and thermal emission. We find that a silicate surface on an exoplanet is spectroscopically detectable via prominent Si-O features in the thermal emission bands of 7-13 μm and 15-2...

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Bibliographic Details
Main Authors: Hu, Renyu (Contributor), Ehlmann, Bethany L. (Author), Seager, Sara (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor)
Format: Article
Language:English
Published: Institute of Physics Publishing, 2012-10-22T20:51:01Z.
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