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hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorTURBET, M.
hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorBOLMONT, E.
hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorCHAVEROT, G.
hal.structure.identifierObservatoire Astronomique de l'Université de Genève [ObsGE]
dc.contributor.authorEHRENREICH, D.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorLECONTE, J.
hal.structure.identifierPLANETO - LATMOS
dc.contributor.authorMARCQ, Emmanuel
dc.date.conference2021-11
dc.description.abstractEnIn this contribution, we will present the results of new 3-D numerical simulations of the atmosphere of young rocky planets (supposedly rich in water vapor) carried out with the LMD-Generic Global Climate Model (GCM). We will first show how and why clouds tend to accumulate preferentially on the night side of these planets as soon as water vapor is a major component of the atmosphere. We will then show how and why this result has major consequences on the conditions of formation of early oceans on Venus, as well as on Earth and exoplanets.
dc.language.isoen
dc.title.enDay-Night Cloud Asymmetry Inhibits Early Ocean Formation on Venus
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]
bordeaux.pageLPI Contribution No. 2629, id.4051
bordeaux.countryZZ
bordeaux.conference.cityVirtual Meeting
bordeaux.peerReviewednon
hal.identifierinsu-03582672
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//insu-03582672v1
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