Abstract
We first recall the observations concerning the opaque rings of Saturn and Uranus. Then we describe a model which represents the kinematics of these rings. Finally we review how we treat collisions, self-gravity and satellite perturbations and what are the basic effects of these forces.
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Borderies, N. (1984). Dynamics of Ring-Satellite Systems around Saturn and Uranus. In: Duncombe, R.L., Dvorak, R., Message, P.J. (eds) The Stability of Planetary Systems. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5331-4_27
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DOI: https://doi.org/10.1007/978-94-009-5331-4_27
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