期刊
CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY
卷 98, 期 1, 页码 5-30出版社
SPRINGER
DOI: 10.1007/s10569-007-9066-9
关键词
Enceladus; Dione; Mean-Motion resonance; periodic orbits; regular and chaotic motion; secondary resonance; Saturn
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.
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