Modelling the atmosphere of potential habitable planets
Abstract
The list of planets discovered in the habitable zone of its star is continuously growing. We present a simple one-dimension radiative transfer model in order to better infer on the habitability of such systems. Particular focus is on the TRAPPIST-1 planets (Gillon et al. 2017), particularly on planets b, c, d, e and f.
- Publication:
-
Origins: From the Protosun to the First Steps of Life
- Pub Date:
- 2020
- DOI:
- 10.1017/S1743921319002874
- Bibcode:
- 2020IAUS..345..172I
- Keywords:
-
- planets and satellites: general