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BORN EXTRA-ECCENTRIC: A BROAD SPECTRUM OF PRIMORDIAL CONFIGURATIONS OF THE GAS GIANTS THAT MATCH THEIR PRESENT-DAY ORBITS

hal.structure.identifierDepartment of Terrestrial Magnetism [Carnegie Institution]
dc.contributor.authorCLEMENT, Matthew
dc.contributor.authorDEIENNO, Rogerio
dc.contributor.authorKAIB, Nathan
dc.contributor.authorIZIDORO, André
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.description.abstractEnIn a recent paper we proposed that the giant planets' primordial orbits may have been eccentric (e J ∼ e S ∼ 0.05), and used a suite of dynamical simulations to show outcomes of the giant planet instability that are consistent with their present-day orbits. In this follow-up investigation, we present more comprehensive simulations incorporating superior particle resolution, longer integration times, and eliminating our prior means of artificially forcing instabilities to occur at specified times by shifting a planets' position in its orbit. While we find that the residual phase of planetary migration only minimally alters the the planets' ultimate eccentricities, our work uncovers several intriguing outcomes in realizations where Jupiter and Saturn are born with extremely large eccentricities (e J 0.10; e S 0.25). In successful simulations, the planets' orbits damp through interactions with the planetesimal disk prior to the instability, thus loosely replicating the initial conditions considered in our previous work. Our results therefore suggest an even wider range of plausible evolutionary pathways are capable of replicating Jupiter and Saturn's modern orbital architecture.
dc.language.isoen
dc.publisherElsevier
dc.title.enBORN EXTRA-ECCENTRIC: A BROAD SPECTRUM OF PRIMORDIAL CONFIGURATIONS OF THE GAS GIANTS THAT MATCH THEIR PRESENT-DAY ORBITS
dc.typeArticle de revue
dc.identifier.doi10.1016/j.icarus.2021.114556
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]
bordeaux.journalIcarus
bordeaux.page114556
bordeaux.volume367
bordeaux.peerReviewedoui
hal.identifierhal-03878969
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03878969v1
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