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hal.structure.identifierDepartment of Archaeology
dc.contributor.authorWALSH, K. J.
dc.contributor.authorMORBIDELLI, A.
hal.structure.identifiersSE 2011
dc.contributor.authorRAYMOND, Sean N.
dc.contributor.authorO'BRIEN, D. P.
dc.contributor.authorMANDELL, A. M.
dc.date.conference2011
dc.description.abstractEnWe present a scenario to reproduce Mars' small mass, as well as the S/C dichotomy of the asteroid belt, by taking into account the inward-then-outward gas-driven migration of Jupiter that is predicted by hydrodynamical simulations.
dc.language.isoen
dc.title.enThe Asteroid Belt and Mars' Small Mass Explained by Large-Scale Gas-Driven Migration of Jupiter
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.countryUS
bordeaux.conference.cityThe Woodlands - Texas
bordeaux.peerReviewedoui
hal.identifierhal-00666875
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00666875v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=WALSH,%20K.%20J.&MORBIDELLI,%20A.&RAYMOND,%20Sean%20N.&O'BRIEN,%20D.%20P.&MANDELL,%20A.%20M.&rft.genre=unknown


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