dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:50:26Z
dc.date.accessioned2014-05-20T14:16:18Z
dc.date.accessioned2022-10-05T15:11:28Z
dc.date.available2013-09-30T18:50:26Z
dc.date.available2014-05-20T14:16:18Z
dc.date.available2022-10-05T15:11:28Z
dc.date.created2013-09-30T18:50:26Z
dc.date.created2014-05-20T14:16:18Z
dc.date.issued2008-12-01
dc.identifierCelestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 102, n. 4, p. 273-296, 2008.
dc.identifier0923-2958
dc.identifierhttp://hdl.handle.net/11449/24908
dc.identifier10.1007/s10569-008-9167-0
dc.identifierWOS:000262311200001
dc.identifier5483476857978177
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/3898081
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.
dc.languageeng
dc.publisherSpringer
dc.relationCelestial Mechanics & Dynamical Astronomy
dc.relation2.121
dc.relation1,092
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectEnceladus
dc.subjectDione
dc.subjectMean-motion resonance
dc.subjectSatellites
dc.subjectSaturn satellites
dc.subjectTidal evolution
dc.titleDynamics of Enceladus and Dione inside the 2:1 mean-motion resonance under tidal dissipation
dc.typeArtigo


Este ítem pertenece a la siguiente institución