UV Surface Environments of M Star Planets: Surface Habitability and Temporal Biosignatures
Abstract
Habitable planets around active M stars can be subjected to high levels of UV radiation. Here we model the UV surface regimes on such planets as a first step toward determining the habitability and novel biosignatures for such worlds.
- Publication:
-
Habitable Worlds 2017: A System Science Workshop
- Pub Date:
- November 2017
- Bibcode:
- 2017LPICo2042.4128O