Dynamics of Enceladus and Dione inside the 2:1 mean-motion resonance under tidal dissipation

Página do item simplificado
dc.contributor.authorCallegari, N. [UNESP]
dc.contributor.authorYokoyama, T. [UNESP]
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:50:26Z
dc.date.accessioned2014-05-20T14:16:18Z
dc.date.available2013-09-30T18:50:26Z
dc.date.available2014-05-20T14:16:18Z
dc.date.issued2008-12-01
dc.description.abstractIn a previous work (Callegari and Yokoyama, Celest. Mech. Dyn. Astr. 98:5-30, 2007), the main features of the motion of the pair Enceladus-Dione were analyzed in the frozen regime, i.e., without considering the tidal evolution. Here, the results of a great deal of numerical simulations of a pair of satellites similar to Enceladus and Dione crossing the 2:1 mean-motion resonance are shown. The resonance crossing is modeled with a linear tidal theory, considering a two-degrees-of-freedom model written in the framework of the general three-body planar problem. The main regimes of motion of the system during the passage through resonance are studied in detail. We discuss our results comparing them with classical scenarios of tidal evolution of the system. We show new scenarios of evolution of the Enceladus-Dione system through resonance not shown in previous approaches of the problem.en
dc.description.affiliationUNESP, Dept Estat Matemat Aplicada & Computacao, Rio Claro, SP, Brazil
dc.description.affiliationUnespUNESP, Dept Estat Matemat Aplicada & Computacao, 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.description.sponsorshipIdFAPESP: 06/58000-2
dc.description.sponsorshipIdFAPESP: 06/61379-3
dc.description.sponsorshipIdFAPESP: 06/04997-6
dc.description.sponsorshipIdCNPq: 306276/2007-0
dc.format.extent273-296
dc.identifierhttp://dx.doi.org/10.1007/s10569-008-9167-0
dc.identifier.citationCelestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 102, n. 4, p. 273-296, 2008.
dc.identifier.doi10.1007/s10569-008-9167-0
dc.identifier.issn0923-2958
dc.identifier.lattes5483476857978177
dc.identifier.urihttp://hdl.handle.net/11449/24908
dc.identifier.wosWOS:000262311200001
dc.language.isoeng
dc.publisherSpringer
dc.relation.ispartofCelestial Mechanics & Dynamical Astronomy
dc.relation.ispartofjcr2.121
dc.relation.ispartofsjr1,092
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectEnceladusen
dc.subjectDioneen
dc.subjectMean-motion resonanceen
dc.subjectSatellitesen
dc.subjectSaturn satellitesen
dc.subjectTidal evolutionen
dc.titleDynamics of Enceladus and Dione inside the 2:1 mean-motion resonance under tidal dissipationen
dc.typeArtigo
dcterms.licensehttp://www.springer.com/open+access/authors+rights?SGWID=0-176704-12-683201-0
dcterms.rightsHolderSpringer
unesp.author.lattes5483476857978177
unesp.campusUniversidade Estadual Paulista (Unesp), Instituto de Geociências e Ciências Exatas, Rio Claropt

Arquivos

Licença do Pacote
Agora exibindo 1 - 2 de 2
Nenhuma Miniatura disponível
Nome:
license.txt
Tamanho:
1.71 KB
Formato:
Item-specific license agreed upon to submission
Descrição:
Nenhuma Miniatura disponível
Nome:
license.txt
Tamanho:
1.71 KB
Formato:
Item-specific license agreed upon to submission
Descrição:

Coleções

Artigos - Estatistica, Matemática Aplicada e Computação - IGCE