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dc.contributor.authorCLEMENT, Matthew
dc.contributor.authorKAIB, Nathan
hal.structure.identifierECLIPSE 2021
dc.contributor.authorRAYMOND, Sean
hal.structure.identifierGuy's and St Thomas' Hospital [London]
dc.contributor.authorCHAMBERS, John
dc.date.issued2021-10
dc.identifier.issn0019-1035
dc.language.isoen
dc.publisherElsevier
dc.title.enThe early instability scenario: Mars’ mass explained by Jupiter’s orbit
dc.typeArticle de revue
dc.identifier.doi10.1016/j.icarus.2021.114585
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv2106.05276
bordeaux.journalIcarus
bordeaux.page114585
bordeaux.volume367
bordeaux.peerReviewedoui
hal.identifierhal-03878984
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03878984v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Icarus&rft.date=2021-10&rft.volume=367&rft.spage=114585&rft.epage=114585&rft.eissn=0019-1035&rft.issn=0019-1035&rft.au=CLEMENT,%20Matthew&KAIB,%20Nathan&RAYMOND,%20Sean&CHAMBERS,%20John&rft.genre=article


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