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On the Emmenthal distribution of highly inclined asteroids

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dc.contributor.authorCarruba, V. [UNESP]
dc.contributor.authorMachuca, J. F. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2014-05-20T13:28:04Z
dc.date.available2014-05-20T13:28:04Z
dc.date.issued2011-12-01
dc.description.abstractHighly inclined asteroids are objects with sin (i) > 0.3. Among highly inclined asteroids, we can distinguish between objects with inclinations smaller than that of the centre of the ?6= g - g6 secular resonance and objects at higher inclinations. Using the current mechanisms of dynamical mobility, it is not easy to increase the values of an asteroid with an initial small inclination to values higher than that of the centre of the ?6 resonance. The presence of highly inclined objects might therefore be related to the early phases of the Solar system.en
dc.description.affiliationUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
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.sponsorshipIdFAPESP: 06/50005-5
dc.description.sponsorshipIdCNPq: 302183/2008-6
dc.description.sponsorshipIdCNPq: 473345/2009-9
dc.format.extent1102-1114
dc.identifierhttp://dx.doi.org/10.1111/j.1365-2966.2011.19576.x
dc.identifier.citationMonthly Notices of The Royal Astronomical Society. Malden: Wiley-blackwell, v. 418, n. 2, p. 1102-1114, 2011.
dc.identifier.dimensionspub.1036749272
dc.identifier.doi10.1111/j.1365-2966.2011.19576.x
dc.identifier.fileWOS000297987400032.pdf
dc.identifier.issn0035-8711
dc.identifier.issn1365-8711
dc.identifier.issn1365-2966
dc.identifier.lattes4750709016042276
dc.identifier.orcid0000-0003-2786-0740
dc.identifier.orcid0000-0002-1772-414X
dc.identifier.urihttp://hdl.handle.net/11449/9306
dc.identifier.wosWOS:000297987400032
dc.language.isoeng
dc.publisherWiley-Blackwell
dc.publisherOxford University Press (OUP)
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.relation.ispartofjcr5.194
dc.relation.ispartofsjr2,346
dc.rights.accessRightsAcesso abertopt
dc.sourceWeb of Science
dc.sourceDimensions
dc.subjectcelestial mechanicsen
dc.subjectminor planets, asteroids: generalen
dc.titleOn the Emmenthal distribution of highly inclined asteroidsen
dc.typeArtigopt
dcterms.licensehttp://www.oxfordjournals.org/access_purchase/self-archiving_policyp.html
dcterms.rightsHolderWiley-blackwell
dspace.entity.typePublication
relation.isDepartmentOfPublicationcf723ce7-c9ee-4e06-b772-346bd0a102bb
relation.isDepartmentOfPublication.latestForDiscoverycf723ce7-c9ee-4e06-b772-346bd0a102bb
relation.isOrgUnitOfPublicationa4071986-4355-47c3-a5a3-bd4d1a966e4f
relation.isOrgUnitOfPublication.latestForDiscoverya4071986-4355-47c3-a5a3-bd4d1a966e4f
unesp.author.lattes4750709016042276
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

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