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Geophysical and atmospheric evolution of habitable planets

hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorLAMMER, Helmut
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierCentre de Recherche Astrophysique de Lyon [CRAL]
dc.contributor.authorSELSIS, Franck
hal.structure.identifierPLANETO - LATMOS
hal.structure.identifierInteractions et dynamique des environnements de surface [IDES]
dc.contributor.authorCHASSEFIÈRE, Eric
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorBREUER, Doris
hal.structure.identifierNetherlands Institute for Radio Astronomy [ASTRON]
dc.contributor.authorGRIESSMEIER, Jean-Mathias
hal.structure.identifierPolar Geophysical Institute of Russian Academy of Sciences [PGI]
dc.contributor.authorKULIKOV, Yuri N.
hal.structure.identifierInstitute of Computational Modelling of the Russian Academy of Sciences [ICM SB RAS]
dc.contributor.authorERKAEV, Nikolai V.
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorKHODACHENKO, Maxim L.
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorBIERNAT, Helfried K.
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorLEBLANC, François
hal.structure.identifierFinnish Meteorological Institute [FMI]
dc.contributor.authorKALLIO, Esa
hal.structure.identifierSwedish Institute of Space Physics [Kiruna] [IRF]
dc.contributor.authorLUNDIN, Richard
hal.structure.identifierCentre de biophysique moléculaire [CBM]
dc.contributor.authorWESTALL, Frances
hal.structure.identifierInstitute of Physics [Graz]
dc.contributor.authorBAUER, Siegfried
hal.structure.identifierNASA ExoPlanet Science Institute [NExScI]
dc.contributor.authorBEICHMAN, Charles
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorDANCHI, William
hal.structure.identifierUniversidad Autónoma de Madrid [UAM]
dc.contributor.authorEIROA, Carlos
hal.structure.identifierResearch and Scientific Support Department, ESTEC [RSSD]
dc.contributor.authorFRIDLUND, Malcolm
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorGRÖLLER, Hannes
hal.structure.identifierInstitute of Physics [Graz]
dc.contributor.authorHANSLMEIER, Arnold
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorHAUSLEITNER, Walter
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHENNING, Thomas
hal.structure.identifierMax-Planck-Institut für Astronomie [MPIA]
dc.contributor.authorHERBST, Tom
hal.structure.identifierHarvard-Smithsonian Center for Astrophysics [CfA]
dc.contributor.authorKALTENEGGER, Lisa
hal.structure.identifierInstitut d'astrophysique spatiale [IAS]
dc.contributor.authorLÉGER, Alain
hal.structure.identifierInstitute of Physics [Graz]
dc.contributor.authorLEITZINGER, Martin
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorLICHTENEGGER, Herbert I. M.
hal.structure.identifierDepartment of Radio and Space Science [Göteborg]
dc.contributor.authorLISEAU, René
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, Jonathan
hal.structure.identifierInstitut für Theoretische Physik [Braunschweig]
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorMOTSCHMANN, Uwe
hal.structure.identifierInstitute of Physics [Graz]
dc.contributor.authorODERT, Petra
hal.structure.identifierIstituto Nazionale di Astrofisica [INAF]
dc.contributor.authorPARESCE, Francesco
hal.structure.identifierDepartment of Geology and Petroleum Geology [Aberdeen]
dc.contributor.authorPARNELL, John
hal.structure.identifierSTFC Rutherford Appleton Laboratory [RAL]
dc.contributor.authorPENNY, Alan
hal.structure.identifierLandessternwarte Königstuhl [ZAH] [LSW]
dc.contributor.authorQUIRRENBACH, Andreas
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorRAUER, Heike
hal.structure.identifierLeiden Observatory [Leiden]
dc.contributor.authorRÖTTGERING, Huub
hal.structure.identifierObservatoire de Paris - Site de Meudon [OBSPM]
dc.contributor.authorSCHNEIDER, Jean
hal.structure.identifierDLR Institut für Planetenforschung
dc.contributor.authorSPOHN, Tilman
hal.structure.identifierInstitut für Theoretische Physik [Braunschweig]
dc.contributor.authorSTADELMANN, Anja
hal.structure.identifierSpace Research Institute of Austrian Academy of Sciences [IWF]
dc.contributor.authorSTANGL, Günter
hal.structure.identifierSRON Netherlands Institute for Space Research [SRON]
dc.contributor.authorSTAM, Daphne
hal.structure.identifierUniversity College of London [London] [UCL]
dc.contributor.authorTINETTI, Giovanna
hal.structure.identifierSTFC Rutherford Appleton Laboratory [RAL]
hal.structure.identifierDepartment of Physics and Astronomy [Milton Keynes]
dc.contributor.authorWHITE, Glenn J.
dc.date.issued2010
dc.identifier.issn1531-1074
dc.description.abstractEnThe evolution of Earth-like habitable planets is a complex process that depends on the geodynamical and geophysical environments. In particular, it is necessary that plate tectonics remain active over billions of years. These geophysically active environments are strongly coupled to a planet's host star parameters, such as mass, luminosity and activity, orbit location of the habitable zone, and the planet's initial water inventory. Depending on the host star's radiation and particle flux evolution, the composition in the thermosphere, and the availability of an active magnetic dynamo, the atmospheres of Earth-like planets within their habitable zones are differently affected due to thermal and nonthermal escape processes. For some planets, strong atmospheric escape could even effect the stability of the atmosphere
dc.language.isoen
dc.publisherMary Ann Liebert
dc.subject.enAtmosphere evolution
dc.subject.enGeophysics
dc.subject.enHabitability
dc.subject.enTerrestrial planets
dc.title.enGeophysical and atmospheric evolution of habitable planets
dc.typeArticle de revue
dc.identifier.doi10.1089/ast.2009.0368
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.journalAstrobiology
bordeaux.page45-68
bordeaux.volume10
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-00470583
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00470583v1
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