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dc.contributor.authorHONG, Y.-C.
hal.structure.identifiersSE 2011
dc.contributor.authorRAYMOND, Sean N.
hal.structure.identifierLunar and Planetary Laboratory [Tucson] [LPL]
dc.contributor.authorLUNINE, J.I.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnThe large observed eccentricities of giant exoplanets provide evidence that most planetary systems have violent dynamical histories. Among the known mechanisms, planet-planet scattering is thought to have played the most important role in shaping the eccentricity distribution [3,4,6,9]. Here we directly simulate the orbital stability of satellites in orbit around giant planets during planet-planet scattering. During planetary close encounters, the approaching planet perturbs satellite orbits. Depending on the strength of encounters and satellites' orbital distances with respect to their parent planets, satellites may remain bound but undergo moderate eccentricity excitation and orbital distance modification, or they can be stripped from their parent planet. In some encounters, satellites can also be captured from another planet or the gas disk [8]. We present results of our systematic study of satellite stability for planets with different masses and mass gradients and orbital histories. We will map the final orbital distribution of exomoons and make testable predictions for the presence of exomoons around giant exoplanets.
dc.language.isoen
dc.source.title2011epsc.conf.1696H
dc.title.enStability of Giant Planet Moons during Planet-Planet Scattering Events
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.page1696
bordeaux.countryFR
bordeaux.title.proceeding2011epsc.conf.1696H
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00666842
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00666842v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=2011epsc.conf.1696H&rft.date=2011-10&rft.spage=1696&rft.epage=1696&rft.au=HONG,%20Y.-C.&RAYMOND,%20Sean%20N.&LUNINE,%20J.I.&rft.genre=unknown


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