Theoretical spectra of terrestrial exoplanet surfaces

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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Dettagli Bibliografici
Autori principali:	Hu, Renyu, Ehlmann, Bethany L., Seager, Sara
Altri autori:	Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Natura:	Articolo
Lingua:	en_US
Pubblicazione:	Institute of Physics Publishing 2012
Accesso online:	http://hdl.handle.net/1721.1/74201 https://orcid.org/0000-0002-6892-6948

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