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Modelling the atmosphere of potential habitable planets

Published online by Cambridge University Press:  13 January 2020

Nicolas Iro Open the ORCID record for Nicolas Iro [Opens in a new window]
Nicolas Iro*
Affiliation:
University of Vienna, Dept. of Astrophysics, Türkenschanzstr. 17, 1180Vienna, Austria email: nicolas.iro@univie.ac.at
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Abstract

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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.

Keywords

planets and satellites: general
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 14 , Symposium S345: Origins: From the Protosun to the First Steps of Life , August 2018 , pp. 172 - 175
Copyright
© International Astronomical Union 2020 

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