Dynamical evolution of V-type asteroids in the central main belt

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dc.contributor.authorCarruba, V. [UNESP]
dc.contributor.authorHuaman, M. E. [UNESP]
dc.contributor.authorDomingos, R. C. [UNESP]
dc.contributor.authorDos Santos, C. R. [UNESP]
dc.contributor.authorSouami, D.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionInstituto Nacional de Pesquisas Espaciais (INPE)
dc.contributor.institutionUniv Namur
dc.contributor.institutionUniv Paris 06
dc.date.accessioned2014-12-03T13:09:14Z
dc.date.available2014-12-03T13:09:14Z
dc.date.issued2014-04-01
dc.description.abstractThe origin of this large population of V-type objects is not well understood. Since it seems unlikely that Vestoids crossing the 3J:-1A mean-motion resonance with Jupiter could account for the whole population of V-type asteroids in the central and outer main belt, origin from local sources, such as the parent bodies of the Eunomia, and of the Merxia and Agnia asteroid families, has been proposed as an alternative mechanism.In this work, we investigated the dynamical evolution of the V-type photometric candidates in the central main belt, under the effect of gravitational and non-gravitational forces. Our results show that dynamical evolution from the parent bodies of the Eunomia and Merxia/Agnia families on time-scales of 2 Byr or more could be responsible for the current orbital location of most of the low-inclined V-type asteroids.en
dc.description.affiliationUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.description.affiliationInst Nacl Pesquisas Espaciais, BR-12227010 So Jos Dos Campos, SP, Brazil
dc.description.affiliationUniv Namur, Dept Math, Namur Ctr Complex Syst, NAXYS, B-5000 Namur, Belgium
dc.description.affiliationUniv Paris 06, F-75005 Paris, France
dc.description.affiliationUniv Paris 06, CNRS, UMR 8630, Observ Paris,SYRTE, F-75005 Paris, France
dc.description.affiliationUnespUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.description.sponsorshipFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.description.sponsorshipConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.description.sponsorshipNational Aeronautics and Space Administration
dc.description.sponsorshipPlanetary Science Division of the National Aeronautics and Space Administration
dc.description.sponsorshipIdFAPESP: 11/19863-3
dc.description.sponsorshipIdCNPq: 305453/2011-4
dc.format.extent3168-3179
dc.identifierhttp://dx.doi.org/10.1093/mnras/stu192
dc.identifier.citationMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 439, n. 3, p. 3168-3179, 2014.
dc.identifier.doi10.1093/mnras/stu192
dc.identifier.issn0035-8711
dc.identifier.lattes4750709016042276
dc.identifier.lattes6652169083464327
dc.identifier.orcid0000-0002-0516-0420
dc.identifier.urihttp://hdl.handle.net/11449/112112
dc.identifier.wosWOS:000334114900077
dc.language.isoeng
dc.publisherOxford University Press
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.relation.ispartofjcr5.194
dc.relation.ispartofsjr2,346
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectcelestial mechanicsen
dc.subjectminor planetsen
dc.subjectasteroids: generalen
dc.titleDynamical evolution of V-type asteroids in the central main belten
dc.typeArtigo
dcterms.licensehttp://www.oxfordjournals.org/access_purchase/self-archiving_policyb.html
dcterms.rightsHolderOxford Univ Press
unesp.author.lattes4750709016042276
unesp.author.lattes6652169083464327[3]
unesp.author.orcid0000-0002-0516-0420[3]
unesp.author.orcid0000-0003-2786-0740[1]
unesp.author.orcid0000-0003-3094-2755[2]
unesp.campusUniversidade Estadual Paulista (Unesp), Faculdade de Engenharia, Guaratinguetápt

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