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hal.structure.identifierLaboratoire de Cosmologie, Astrophysique Stellaire & Solaire, de Planétologie et de Mécanique des Fluides [CASSIOPEE]
dc.contributor.authorMORBIDELLI, Alessandro
hal.structure.identifierECLIPSE 2016
dc.contributor.authorRAYMOND, Sean N.
dc.date.issued2016-10
dc.identifier.issn2169-9097
dc.description.abstractEnOver the past two decades, large strides have been made in the field of planet formation. Yet fundamental questions remain. Here we review our state of understanding of five fundamental bottlenecks in planet formation. These are: 1) the structure and evolution of protoplanetary disks; 2) the growth of the first planetesimals; 3) orbital migration driven by interactions between proto-planets and gaseous disk; 4) the origin of the Solar System's orbital architecture; and 5) the relationship between observed super-Earths and our own terrestrial planets. Given our lack of understanding of these issues, even the most successful formation models remain on shaky ground.
dc.language.isoen
dc.publisherWiley-Blackwell
dc.rights.urihttp://hal.archives-ouvertes.fr/licences/copyright/
dc.subject.enAstrophysics - Earth and Planetary Astrophysics
dc.title.enChallenges in Planet Formation
dc.typeArticle de revue
dc.identifier.doi10.1002/2016JE005088
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1610.07202
bordeaux.journalJournal of Geophysical Research. Planets
bordeaux.page1962-1980
bordeaux.volume121
bordeaux.issue10
bordeaux.peerReviewedoui
hal.identifierhal-01387890
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01387890v1
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