Dynamical evolution of V-type photometric candidates in the outer main belt

dc.contributorUniversidade Estadual Paulista (Unesp)
dc.creatorHuaman, M. E. [UNESP]
dc.creatorCarruba, V. [UNESP]
dc.creatorDomingos, R. C. [UNESP]
dc.date2015-03-18T15:54:43Z
dc.date2015-03-18T15:54:43Z
dc.date2014-11-01
dc.date.accessioned2023-09-12T03:03:35Z
dc.date.available2023-09-12T03:03:35Z
dc.identifierhttp://dx.doi.org/10.1093/mnras/stu1655
dc.identifierMonthly Notices Of The Royal Astronomical Society. Oxford: Oxford Univ Press, v. 444, n. 3, p. 2985-2992, 2014.
dc.identifier0035-8711
dc.identifierhttp://hdl.handle.net/11449/117003
dc.identifier10.1093/mnras/stu1655
dc.identifierWOS:000343399600073
dc.identifier4750709016042276
dc.identifier6652169083464327
dc.identifier0000-0002-0516-0420
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/8766488
dc.descriptionV-type asteroids, characterized by two absorption bands at 1.0 and 2.0 mu m, are usually thought to be portions of the crust of differentiated or partially differentiated bodies. Most V-type asteroids are found in the inner main belt and are thought to be current or past members of the Vesta dynamical family. Recently, several V-type photometric candidates have been identified in the central and outer main belt. While the dynamical evolution of V-type photometric candidates in the central main belt has been recently investigated, less attention has been given to the orbital evolution of basaltic material in the outer main belt as a whole. Here, we identify known and new V-type photometric candidates in this region, and study their orbital evolution under the effect of gravitational and non-gravitational forces. A scenario in which a minimum of three local sources, possibly associated with the parent bodies of (349) Dembowska, (221) Eos, and (1459) Magnya, could in principle explain the current orbital distribution of V-type photometric candidates in the region.
dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)
dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)
dc.descriptionNational Aeronautics and Space Administration
dc.descriptionPlanetary Science Division of the National Aeronautics and Space Administration
dc.descriptionUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.descriptionUniv Estadual Paulista, UNESP, BR-13874149 Sao Joao Da Boa Vista, SP, Brazil
dc.descriptionUniv Estadual Paulista, UNESP, Grp Dinam Orbital & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.descriptionUniv Estadual Paulista, UNESP, BR-13874149 Sao Joao Da Boa Vista, SP, Brazil
dc.descriptionFAPESP: 11/19863-3
dc.descriptionCNPq: 305453/2011-4
dc.format2985-2992
dc.languageeng
dc.publisherOxford Univ Press
dc.relationMonthly Notices Of The Royal Astronomical Society
dc.relation5.194
dc.relation2,346
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectcelestial mechanics
dc.subjectminor planets, asteroids: general
dc.titleDynamical evolution of V-type photometric candidates in the outer main belt
dc.typeArtigo


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