# Habitability of planets on eccentric orbits: the limits of the mean flux approximation

2 ECLIPSE 2016
LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
Abstract : Contrary to Earth, which has a small orbital eccentricity, some exoplanets discovered in the insolation habitable zone (HZ) have high orbital eccentricities (e.g., up to an eccentricity of $\sim0.97$ for HD~20782~b). This raises the question of the capacity of these planets to host surface liquid water. In order to assess the habitability of an eccentric planet, the mean flux approximation is often used. It states that a planet on an eccentric orbit is called habitable if it receives on average a flux compatible with the presence of surface liquid water. However, as the planets do experience important insolation variations over one orbit and even spend some time outside the HZ for high eccentricities, the question of their habitability might not be as straightforward. We performed a set of simulations using the Global Climate Model LMDz, exploring the limits of the mean flux approximation when varying the luminosity of the host star and the eccentricity of the planet. We computed the climate of tidally locked ocean covered planets with orbital eccentricity from 0 to 0.9 receiving a mean flux equal to Earth's, around stars of luminosity ranging from $L_\odot$ to $10^{-4}~L_\odot$. Using here a definition of habitability based on the presence of surface liquid water, we find that most of the planets considered can sustain surface liquid water on the dayside with an ice cap on the nightside. However, for high eccentricity and high luminosity, planets cannot sustain surface liquid water during the whole orbital period. They completely freeze at apoastron and when approaching periastron an ocean appears around the substellar point. We conclude that the higher the eccentricity and the higher the luminosity of the star, the less reliable the mean flux approximation.
Type de document :
Article dans une revue
Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 591, pp.id.A106. 〈10.1051/0004-6361/201628073〉

https://hal.archives-ouvertes.fr/hal-01306074
Contributeur : Marie-Paule Pomies <>
Soumis le : vendredi 22 avril 2016 - 11:51:34
Dernière modification le : jeudi 11 janvier 2018 - 06:27:41

### Citation

Anne-Sophie, Libert, J. Leconte, Franck Selsis, Emeline Bolmont. Habitability of planets on eccentric orbits: the limits of the mean flux approximation. Astronomy and Astrophysics - A&A, EDP Sciences, 2016, 591, pp.id.A106. 〈10.1051/0004-6361/201628073〉. 〈hal-01306074〉

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