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The Asteroid Belt and Mars' Small Mass Explained by Large-Scale Gas-Driven Migration of Jupiter
hal.structure.identifier | Department of Archaeology | |
dc.contributor.author | WALSH, K. J. | |
dc.contributor.author | MORBIDELLI, A. | |
hal.structure.identifier | sSE 2011 | |
dc.contributor.author | RAYMOND, Sean N. | |
dc.contributor.author | O'BRIEN, D. P. | |
dc.contributor.author | MANDELL, A. M. | |
dc.date.conference | 2011 | |
dc.description.abstractEn | We 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.iso | en | |
dc.title.en | The Asteroid Belt and Mars' Small Mass Explained by Large-Scale Gas-Driven Migration of Jupiter | |
dc.type | Communication dans un congrès | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
bordeaux.country | US | |
bordeaux.conference.city | The Woodlands - Texas | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-00666875 | |
hal.version | 1 | |
hal.invited | non | |
hal.proceedings | non | |
hal.popular | non | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-00666875v1 | |
bordeaux.COinS | ctx_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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