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hal.structure.identifiersSE 2011
dc.contributor.authorMAURIN, A. S.
hal.structure.identifiersSE 2011
dc.contributor.authorSELSIS, Franck
hal.structure.identifierFORMATION STELLAIRE 2011
dc.contributor.authorHERSANT, F.
hal.structure.identifiersSE 2011
dc.contributor.authorRAYMOND, Sean N.
dc.contributor.authorLECONTE, J.
dc.contributor.authorDELBO, M.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnShort-period exoplanets undergo strong tidal interactions that affect their orbital and spin evolution and their internal structure via tidal heating. Tidal models are, however, limited by uncertainties on key processes such as the dissipation rate. We show here that infrared photometric monitoring of eccentric rocky exoplanets can be used to determine the rotation period and constrain the tidal dissipation within the planet. The comparison of tidal models with measured rotation and dissipation rates of exoplanets would allow us to constrain unknown parameters and discriminate between models.
dc.language.isoen
dc.source.title2011epsc.conf.1351M
dc.title.enEffects of tides on the infrared light curve of rocky exoplanets
dc.typeCommunication dans un congrès
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.page1351
bordeaux.countryFR
bordeaux.title.proceeding2011epsc.conf.1351M
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00664602
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00664602v1
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