Dynamics of two satellites in the 2/1 Mean-Motion resonance: application to the case of Enceladus and Dione

dc.contributorUniversidade Estadual Paulista (UNESP)
dc.creatorCallegari, N.
dc.creatorYokoyama, T.
dc.date2014-02-26T17:29:06Z
dc.date2014-05-20T14:15:57Z
dc.date2016-10-25T17:39:10Z
dc.date2014-02-26T17:29:06Z
dc.date2014-05-20T14:15:57Z
dc.date2016-10-25T17:39:10Z
dc.date2007-05-01
dc.date.accessioned2017-04-05T22:19:49Z
dc.date.available2017-04-05T22:19:49Z
dc.identifierCelestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 98, n. 1, p. 5-30, 2007.
dc.identifier0923-2958
dc.identifierhttp://hdl.handle.net/11449/24783
dc.identifierhttp://acervodigital.unesp.br/handle/11449/24783
dc.identifier10.1007/s10569-007-9066-9
dc.identifierWOS:000245966700002
dc.identifierhttp://dx.doi.org/10.1007/s10569-007-9066-9
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/869750
dc.descriptionThe dynamics of a pair of satellites similar to Enceladus-Dione is investigated with a two-degrees-of-freedom model written in the domain of the planar general three-body problem. Using surfaces of section and spectral analysis methods, we study the phase space of the system in terms of several parameters, including the most recent data. A detailed study of the main possible regimes of motion is presented, and in particular we show that, besides the two separated resonances, the phase space is replete of secondary resonances.
dc.languageeng
dc.publisherSpringer
dc.relationCelestial Mechanics & Dynamical Astronomy
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectEnceladus
dc.subjectDione
dc.subjectMean-Motion resonance
dc.subjectperiodic orbits
dc.subjectregular and chaotic motion
dc.subjectsecondary resonance
dc.subjectSaturn
dc.titleDynamics of two satellites in the 2/1 Mean-Motion resonance: application to the case of Enceladus and Dione
dc.typeOtro


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