Comparison of density waves in the rings of Saturn and Uranus

Details Comparison of density waves in the rings of Saturn and Uranus Comparison of density waves in the rings of Saturn and Uranus

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992adspr..12..149y&link_type=abstract

(Planetary studies; Proceedings of Symposium 4 and the Topical Meeting of the Interdisciplinary Scientific Commission B /Meeting

Physics

Density Distribution, Satellite Perturbation, Saturn Rings, Uranus Rings, Planetology, Waves

Scientific paper

The similarity of density waves in the rings of Saturn and Uranus are addressed. It is found that all ring systems are grossly similar in that they all encircle the primary in its equatorial plane and exhibit responses to resonant satellite perturbations. The dominant response of Saturn's rings is the clearing of gaps and generation of density and bending waves. The Uranian rings appear to be confined by the presence of shepherd satellites. Three possible density waves have been identified, two in the epsilon ring and one in the delta ring.

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