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dc.contributor.authorBOND, J. C.
dc.contributor.authorO'BRIEN, D. P.
hal.structure.identifiersSE 2011
dc.contributor.authorRAYMOND, Sean N.
dc.date.issued2011-10
dc.date.conference2011
dc.description.abstractEnExtrasolar terrestrial planets are likely to have compositions unlike anything previously observed. Previous work on this issue has not examined the impact giant planet migration may have on these planetary compositions beyond looking at possible water content. We present 12 simulations incorporating planetary migration. In all cases, migration was found to dramatically alter the planetary composition, acting to broaden the feeding zones and decrease radial variations in composition. Furthermore, migration was found to assist in the delivery of water-rich material to accreting planets.
dc.language.isoen
dc.source.title2011epsc.conf..160B
dc.title.enThe Diversity of Extrasolar Terrestrial Planets: adding migration into the mix.
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.page160
bordeaux.countryFR
bordeaux.title.proceeding2011epsc.conf..160B
bordeaux.conference.cityNantes
bordeaux.peerReviewedoui
hal.identifierhal-00666857
hal.version1
hal.invitednon
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00666857v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=2011epsc.conf..160B&rft.date=2011-10&rft.spage=160&rft.epage=160&rft.au=BOND,%20J.%20C.&O'BRIEN,%20D.%20P.&RAYMOND,%20Sean%20N.&rft.genre=unknown


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