Constraining the Habitable Zone Boundaries for Water World Exoplanets
Abstract
We use coupled models of planet interiors, clathrate formation, liquid-gas equilibrium, and atmospheric radiative transfer to constrain the atmospheric abundance of CO2 and corresponding habitable zone boundaries for water-rich exoplanets.
- Publication:
-
Habitable Worlds 2017: A System Science Workshop
- Pub Date:
- November 2017
- Bibcode:
- 2017LPICo2042.4135M