Abstract
We consider the system of planetary rings with shepherds as a restricted three or four-body problem, neglecting interactions between ring particles. We show that the generic occurrence of rings for the case of rotating short-range potentials can be extended to the case of gravitational potentials. The consecutive collision periodic orbits created by saddle-center bifurcations are of central importance.
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Benet, L., Seligman, T. H. and Trautmann, D.: 1999, ‘Chaotic scattering in the restricted three-body problem II: small mass parameters’, Celest. Mech. & Dyn. Astr. 71, 167-189.
Benet, L. and Seligman, T. H.: 2000, ‘Genetic occurrence of rings in rotating systems’, Phys. Letts.A 273, 331-339.
Borderies, N., Goldreich, P. and Tremaine, S.: 1984, In: R. Greenberg and A. Brahic (eds), Planetary Rings, University of Arizona Press, Tucson.
Brahic, A.: 1977, ‘System of colliding bodies in a gravitational field I: numerical simulation of the standard model’, Astron. Astrophys. 54, 895-907.
Elliot, J. L. and Nicholson, P. D.: 1984, In: R. Greenberg and A. Brahic (eds), Planetary Rings, University of Arizona Press, Tucson.
Goldreich, P. and Tremaine, S.: 1979, ‘Towards a theory for the uranian rings’, Nature 277, 97-99.
Hénon, M.: 1968, ‘Sur les Orbites Interplan´etaires qui Rencontrent Deux Fois la Terre’, Bull. Astron.(Serie 3) 3, 337-402.
Jung, C. and Scholz, H. J.: 1987, ‘Cantor set structures in the singularities of classical potential scattering’, J. Phys. A: Math. Gen. 20, 3607-3617.
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Benet, L. Occurrence of Planetary Rings with Shepherds. Celestial Mechanics and Dynamical Astronomy 81, 123–128 (2001). https://doi.org/10.1023/A:1013371423194
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DOI: https://doi.org/10.1023/A:1013371423194