The system will be going down for regular maintenance. Please save your work and logout.

Show simple item record

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


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record