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

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Data

2007-05-01

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Coorientador

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Curso de graduação

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Springer

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Artigo

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Resumo

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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Inglês

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Celestial Mechanics & Dynamical Astronomy. Dordrecht: Springer, v. 98, n. 1, p. 5-30, 2007.

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