dc.contributor | Universidade Estadual Paulista (UNESP) | |
dc.creator | Callegari, N. | |
dc.creator | Yokoyama, T. | |
dc.date | 2014-02-26T17:29:06Z | |
dc.date | 2014-05-20T14:15:57Z | |
dc.date | 2016-10-25T17:39:10Z | |
dc.date | 2014-02-26T17:29:06Z | |
dc.date | 2014-05-20T14:15:57Z | |
dc.date | 2016-10-25T17:39:10Z | |
dc.date | 2007-05-01 | |
dc.date.accessioned | 2017-04-05T22:19:49Z | |
dc.date.available | 2017-04-05T22:19:49Z | |
dc.identifier | Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 98, n. 1, p. 5-30, 2007. | |
dc.identifier | 0923-2958 | |
dc.identifier | http://hdl.handle.net/11449/24783 | |
dc.identifier | http://acervodigital.unesp.br/handle/11449/24783 | |
dc.identifier | 10.1007/s10569-007-9066-9 | |
dc.identifier | WOS:000245966700002 | |
dc.identifier | http://dx.doi.org/10.1007/s10569-007-9066-9 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/869750 | |
dc.description | The 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.language | eng | |
dc.publisher | Springer | |
dc.relation | Celestial Mechanics & Dynamical Astronomy | |
dc.rights | info:eu-repo/semantics/closedAccess | |
dc.subject | Enceladus | |
dc.subject | Dione | |
dc.subject | Mean-Motion resonance | |
dc.subject | periodic orbits | |
dc.subject | regular and chaotic motion | |
dc.subject | secondary resonance | |
dc.subject | Saturn | |
dc.title | Dynamics of two satellites in the 2/1 Mean-Motion resonance: application to the case of Enceladus and Dione | |
dc.type | Otro | |