dc.contributor.author	CLEMENT, Matthew
dc.contributor.author	KAIB, Nathan
hal.structure.identifier	ECLIPSE 2021
dc.contributor.author	RAYMOND, Sean
hal.structure.identifier	Guy's and St Thomas' Hospital [London]
dc.contributor.author	CHAMBERS, John
dc.date.issued	2021-10
dc.identifier.issn	0019-1035
dc.language.iso	en
dc.publisher	Elsevier
dc.title.en	The early instability scenario: Mars’ mass explained by Jupiter’s orbit
dc.type	Article de revue
dc.identifier.doi	10.1016/j.icarus.2021.114585
dc.subject.hal	Physique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv	2106.05276
bordeaux.journal	Icarus
bordeaux.page	114585
bordeaux.volume	367
bordeaux.peerReviewed	oui
hal.identifier	hal-03878984
hal.version	1
hal.popular	non
hal.audience	Internationale
hal.origin.link	https://hal.archives-ouvertes.fr//hal-03878984v1
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The early instability scenario: Mars’ mass explained by Jupiter’s orbit