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Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186

hal.structure.identifierECLIPSE 2014
hal.structure.identifierUniversité de Bordeaux [UB]
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]
dc.contributor.authorBOLMONT, Emeline
hal.structure.identifierECLIPSE 2014
hal.structure.identifierUniversité de Bordeaux [UB]
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]
dc.contributor.authorRAYMOND, Sean N.
dc.contributor.authorJÉRÉMY, , Leconte
dc.contributor.authorALEXANDRE, , Correia
dc.contributor.authorELISA, , Quintana
dc.date.created2014
dc.date.issued2014-10
dc.date.conference2014
dc.description.abstractEnA large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.
dc.language.isoen
dc.subject.enPlanets and satellites: dynamical evolution and stability
dc.subject.enPlanet-star interactions
dc.subject.enstars: individual (Kepler-62
dc.subject.enKepler-186)
dc.subject.enmethods: N-body simulations.
dc.title.enTidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186
dc.typeCommunication dans un congrès
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1410.7428
bordeaux.page7428
bordeaux.volume1410
bordeaux.issue310
bordeaux.countryBE
bordeaux.conference.cityNamur
bordeaux.peerReviewedoui
hal.identifierhal-01078753
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01078753v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2014-10&rft.volume=1410&rft.issue=310&rft.spage=7428&rft.epage=7428&rft.au=BOLMONT,%20Emeline&RAYMOND,%20Sean%20N.&J%C3%89R%C3%89MY,%20,%20Leconte&ALEXANDRE,%20,%20Correia&ELISA,%20,%20Quintana&rft.genre=unknown


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