New results on the possible chaotic motion of Enceladus.

Details New results on the possible chaotic motion of Enceladus. New results on the possible chaotic motion of Enceladus.

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987cemec..43..361k&link_type=abstract

Celestial Mechanics, Volume 43, Issue 1-4, pp. 361-369

Computer Science

Enceladus:Orbital Evolution, Enceladus:Resonances, Enceladus:Three-Body Problem, Orbital Evolution:Enceladus, Resonances:Enceladus, Three-Body Problem:Enceladus, Three-Body Problem:Restricted

Scientific paper

New results are shown for the possible long term evolution of the orbit of Enceladus perturbed by Dione in the 2:1 resonance in the planar elliptic restricted problem. The numerical integrations of the secular variation equations (Ferraz-Mello and Dvorak, 1986) yield different types of chaotic behaviour. We also studied the onset of chaos for this dynamical system. Additionally, some illustrative pictures of the whole phase trajectory show the complex structure of phase space.

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