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dc.contributor.authorSOTIRIADIS, Sotiris
hal.structure.identifierNamur Center for Complex Systems [Namur] [NaXys]
dc.contributor.authorLIBERT, Anne-Sophie
hal.structure.identifierECLIPSE 2016
dc.contributor.authorRAYMOND, Sean N.
dc.date.issued2016-10
dc.date.conference2016-10-16
dc.description.abstractEnThe orbits of extrasolar planets are more various than the circular and coplanar ones of the Solar system. We study the impact of inclined and eccentric massive giant planets on the terrestrial planet formation process. The physical and orbital parameters of the giant planets considered in this study arise from n-body simulations of three giant planets in the late stage of the gas disc, under the combined action of Type II migration and planet-planet scattering. At the dispersal of the gas disc, the two- and three-planet systems interact then with an inner disc of planetesimals and planetary embryos. We discuss the mass and orbital parameters of the terrestrial planets formed by our simulations, as well as their water content. We also investigate how the disc of planetesimals and planetary embryos modifies the eccentric and inclined orbits of the giant planets.
dc.language.isoen
dc.title.enFormation of terrestrial planets in eccentric and inclined giant-planet systems
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.volume48
bordeaux.countryUS
bordeaux.conference.cityPasadena
bordeaux.peerReviewednon
hal.identifierhal-01379021
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2016-10-21
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01379021v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2016-10&rft.volume=48&rft.au=SOTIRIADIS,%20Sotiris&LIBERT,%20Anne-Sophie&RAYMOND,%20Sean%20N.&rft.genre=unknown


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