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dc.contributor.authorVERAS, Dimitri
hal.structure.identifierSSE 2012
dc.contributor.authorRAYMOND, Sean N.
dc.date.created2012-01-10
dc.date.issued2012
dc.identifier.issn0035-8711
dc.description.abstractEnRecent gravitational microlensing observations predict a vast population of free-floating giant planets that outnumbers main sequence stars almost twofold. A frequently-invoked mechanism for generating this population is a dynamical instability that incites planet-planet scattering and the ejection of one or more planets in isolated main sequence planetary systems. Here, we demonstrate that this process alone probably cannot represent the sole source of these galactic wanderers. By using straightforward quantitative arguments and N-body simulations, we argue that the observed number of exoplanets exceeds the plausible number of ejected planets per system from scattering. Thus, other potential sources of free-floaters, such as planetary stripping in stellar clusters and post-main-sequence ejection, must be considered.
dc.language.isoen
dc.publisherOxford University Press (OUP): Policy P - Oxford Open Option A
dc.subject.enAstrophysics
dc.subject.enEarth and Planetary Astrophysics
dc.title.enPlanet-Planet Scattering Alone Cannot Explain the Free-Floating Planet Population
dc.typeArticle de revue
dc.identifier.doi10.1111/j.1745-3933.2012.01218.x
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.identifier.arxiv1201.2175
bordeaux.journalMonthly Notices of the Royal Astronomical Society
bordeaux.pageL117-L121
bordeaux.volume421
bordeaux.issue1
bordeaux.peerReviewedoui
hal.identifierhal-00666823
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00666823v1
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