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...
| Main Authors: | , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
Institute of Physics Publishing
2012
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| Online Access: | http://hdl.handle.net/1721.1/74201 https://orcid.org/0000-0002-6892-6948 |