Modelling the atmosphere of potential habitable planets

Author(s)
Nicolas Iro
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.

Organisation(s)
Department of Astrophysics
Journal
Proceedings of the International Astronomical Union
Volume
14
Pages
172-175
No. of pages
4
DOI
https://doi.org/10.1017/S1743921319002874
Publication date
01-2020
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Public Health, Environmental and Occupational Health, Astronomy and Astrophysics, Nutrition and Dietetics, Medicine (miscellaneous), Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/aaf0e252-c128-4a5a-bbc8-a723379aabf5