Prospects for the characterization of habitable planets

With thousands of exoplanets now identified, the characterization of habitable planets and the potential identification of inhabited ones is a major challenge for the coming decades. We review the current working definition of habitable planets, the upcoming observational prospects for their charact...

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Main Authors: Mazevet, Stephane, Affholder, Antonin, Sauterey, Boris, Bixel, Alex, Apai, Daniel, Ferriere, Regis
Format: Article
Language:English
Published: Académie des sciences 2023-08-01
Series:Comptes Rendus. Physique
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Online Access:https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.154/
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author Mazevet, Stephane
Affholder, Antonin
Sauterey, Boris
Bixel, Alex
Apai, Daniel
Ferriere, Regis
author_facet Mazevet, Stephane
Affholder, Antonin
Sauterey, Boris
Bixel, Alex
Apai, Daniel
Ferriere, Regis
author_sort Mazevet, Stephane
collection DOAJ
description With thousands of exoplanets now identified, the characterization of habitable planets and the potential identification of inhabited ones is a major challenge for the coming decades. We review the current working definition of habitable planets, the upcoming observational prospects for their characterization and present an innovative approach to assess habitability and inhabitation. This integrated method couples for the first time the atmosphere and the interior modeling with the biological activity based on ecosystem modeling. We review here the first applications of the method to asses the likelihood and impact of methanogenesis for Enceladus, primitive Earth, and primitive Mars. Informed by these applications for solar system situations where habitability and inhabitation is questionned, we show how the method can be used to inform the design of future space observatories by considering habitability and inhabitation of Earth-like exoplanets around sun-like stars.
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institution Kabale University
issn 1878-1535
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spelling doaj-art-53d8c7e4cf48448194d5d94987b2e6492025-02-07T13:52:56ZengAcadémie des sciencesComptes Rendus. Physique1878-15352023-08-0124S224926410.5802/crphys.15410.5802/crphys.154Prospects for the characterization of habitable planetsMazevet, Stephane0Affholder, Antonin1Sauterey, Boris2Bixel, Alex3Apai, Daniel4Ferriere, Regis5Observatoire de la Côte d’Azur, Université Côte d’Azur, CNRS, 96 boulevard de l’observatoire, F06304 Nice cedex 4, FranceInstitut de Biologie de l’École Normale Supérieure, ENS, Université Paris Sciences et Lettres, Paris, FranceInstitut de Biologie de l’École Normale Supérieure, ENS, Université Paris Sciences et Lettres, Paris, FranceDepartment of Astronomy, The University of Arizona, Tucson, AZ 85721, USA; Lunar and Planetary Laboratory, The University of Arizona, Tucson, AZ 85721, USADepartment of Astronomy, The University of Arizona, Tucson, AZ 85721, USA; Lunar and Planetary Laboratory, The University of Arizona, Tucson, AZ 85721, USADepartment of Ecology and Evolutionary Biology, University of Arizona, Tucson, USA; Institut de Biologie de l’École Normale Supérieure, ENS, Université Paris Sciences et Lettres, Paris, France; International Research Laboratory for Interdisciplinary Global Environmental Studies (iGLOBES), CNRS, ENS, Université Paris Sciences et LettresWith thousands of exoplanets now identified, the characterization of habitable planets and the potential identification of inhabited ones is a major challenge for the coming decades. We review the current working definition of habitable planets, the upcoming observational prospects for their characterization and present an innovative approach to assess habitability and inhabitation. This integrated method couples for the first time the atmosphere and the interior modeling with the biological activity based on ecosystem modeling. We review here the first applications of the method to asses the likelihood and impact of methanogenesis for Enceladus, primitive Earth, and primitive Mars. Informed by these applications for solar system situations where habitability and inhabitation is questionned, we show how the method can be used to inform the design of future space observatories by considering habitability and inhabitation of Earth-like exoplanets around sun-like stars.https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.154/planetsexoplanetshabitable zonehabitable planetshabitability
spellingShingle Mazevet, Stephane
Affholder, Antonin
Sauterey, Boris
Bixel, Alex
Apai, Daniel
Ferriere, Regis
Prospects for the characterization of habitable planets
Comptes Rendus. Physique
planets
exoplanets
habitable zone
habitable planets
habitability
title Prospects for the characterization of habitable planets
title_full Prospects for the characterization of habitable planets
title_fullStr Prospects for the characterization of habitable planets
title_full_unstemmed Prospects for the characterization of habitable planets
title_short Prospects for the characterization of habitable planets
title_sort prospects for the characterization of habitable planets
topic planets
exoplanets
habitable zone
habitable planets
habitability
url https://comptes-rendus.academie-sciences.fr/physique/articles/10.5802/crphys.154/
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AT affholderantonin prospectsforthecharacterizationofhabitableplanets
AT sautereyboris prospectsforthecharacterizationofhabitableplanets
AT bixelalex prospectsforthecharacterizationofhabitableplanets
AT apaidaniel prospectsforthecharacterizationofhabitableplanets
AT ferriereregis prospectsforthecharacterizationofhabitableplanets