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dc.contributor.authorTURBET, M.
hal.structure.identifierLaboratoire de Météorologie Dynamique (UMR 8539) [LMD]
dc.contributor.authorFORGET, F.
hal.structure.identifierECLIPSE 2017
dc.contributor.authorLECONTE, J.
hal.structure.identifierLaboratoire de Météorologie Dynamique (UMR 8539) [LMD]
dc.contributor.authorCHARNAY, B.
hal.structure.identifierLaboratoire de Planétologie et Géodynamique [UMR 6112] [LPG]
dc.contributor.authorTOBIE, G.
dc.date.conference2017-09-17
dc.description.abstractEnIt is widely believed that the carbonate-silicate cycle is the main agent to trigger deglaciations by CO2 greenhouse warming on Earth and by extension on Earth-like planets when they get in frozen state. Using a 3D Global Climate Model, we show that planets with Earth-like characteristics (size, mass, obliquity, rotation rate, ...) orbiting a Sun-like star may never be able to escape from a glaciation era if their orbital distance is greater than ˜1.27 Astronomical Units because CO2 would condense at the poles (here the cold traps) forming permanent CO2 ice caps. This limits the amount of CO2 in the atmosphere and thus its greenhouse effect.
dc.language.isoen
dc.title.enCO2 condensation can seriously limit the deglaciation of Earth-like planets
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.conference.titleEuropean Planetary Science Congress 2017
bordeaux.countryLV
bordeaux.conference.cityRiga
bordeaux.peerReviewedoui
hal.identifierhal-01622240
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01622240v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=TURBET,%20M.&FORGET,%20F.&LECONTE,%20J.&CHARNAY,%20B.&TOBIE,%20G.&rft.genre=unknown


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