Variation of the Equator due to a Highly Inclined and Eccentric Disturber

dc.contributor.authordo Nascimento, Clair [UNESP]
dc.contributor.authorYokoyama, Tadashi [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:50:36Z
dc.date.accessioned2014-05-20T14:16:25Z
dc.date.available2013-09-30T18:50:36Z
dc.date.available2014-05-20T14:16:25Z
dc.date.issued2009-01-01
dc.description.abstractThe New Horizons project is currently in progress, but until recently years ago, a mission to Neptune-Triton System predicted in the mid term 2008-2013 was one of the priorities of NASA's Solar System Exploration theme. Any way, it is important to increase our knowledge on the dynamics of the inner satellites of Neptune, since according to some authors, this was a key question in the mission to Neptune-Triton system. In a previous work, we presented the expansion of the disturbing function for the dynamics of this system. Here we derive the averaged classical equations of the precession of the equator for this problem. The highly inclined and retrograde orbit of Triton makes this problem very unusual. Therefore, the classical truncations in the inclinations are not acceptable, so that the precession equations must be obtained in closed form for the inclination. With a significant mass and due to its distance from Neptune, which is continuously decreasing, Triton should exert in the future, important precession on Neptune's equator. The effects of this precession on the inner satellites are shown, including some resonant cases predicted in the future. Although Triton's orbit is almost circular, no expansion in the eccentricity is needed. Copyright (C) 2009 C. do Nascimento and T. Yokoyama.en
dc.description.affiliationUniv Estadual Paulista, BR-13500970 Rio Claro, SP, Brazil
dc.description.affiliationUnespUniv Estadual Paulista, BR-13500970 Rio Claro, 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.sponsorshipFundação para o Desenvolvimento da UNESP (FUNDUNESP)
dc.format.extent10
dc.identifierhttp://dx.doi.org/10.1155/2009/467865
dc.identifier.citationMathematical Problems In Engineering. New York: Hindawi Publishing Corporation, p. 10, 2009.
dc.identifier.doi10.1155/2009/467865
dc.identifier.fileWOS000274898800001.pdf
dc.identifier.issn1024-123X
dc.identifier.lattes5483476857978177
dc.identifier.urihttp://hdl.handle.net/11449/24947
dc.identifier.wosWOS:000274898800001
dc.language.isoeng
dc.publisherHindawi Publishing Corporation
dc.relation.ispartofMathematical Problems in Engineering
dc.relation.ispartofjcr1.145
dc.rights.accessRightsAcesso aberto
dc.sourceWeb of Science
dc.titleVariation of the Equator due to a Highly Inclined and Eccentric Disturberen
dc.typeArtigo
dcterms.licensehttp://www.hindawi.com/journals/apm/apc/
dcterms.rightsHolderHindawi Publishing Corporation
unesp.author.lattes5483476857978177
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Geociências e Ciências Exatas, Rio Claropt

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