Modelling the atmosphere of potential habitable planets

Nicolas Iro, Bruce G. Elmegreen, L. Viktor Tóth, Manuel Güdel

Research output: Contribution to journalArticle

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.

Original languageEnglish
Pages (from-to)172-175
Number of pages4
JournalProceedings of the International Astronomical Union
DOIs
Publication statusAccepted/In press - Jan 1 2019

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Planets
Atmosphere
planets
planet
atmospheres
atmosphere
habitability
modeling
lists
radiative transfer
stars

Keywords

  • planets and satellites: General

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

Cite this

Modelling the atmosphere of potential habitable planets. / Iro, Nicolas; Elmegreen, Bruce G.; Tóth, L. Viktor; Güdel, Manuel.

In: Proceedings of the International Astronomical Union, 01.01.2019, p. 172-175.

Research output: Contribution to journalArticle

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