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Perturbations to Saturn's F-ring strands at their closest approach to Prometheus

Planetary and Space Science
By: , and 

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Abstract

The strange morphology of the F ring of Saturn is thought to be caused by the perturbing effects of two close satellites, Prometheus and Pandora. The F ring and the satellites also experience periodic close encounters as a result of differential precession arising from Saturn's oblateness. Using the orbits of the F-ring strands derived by Murray et al. (1997, Icarus 129, 304-316) the behaviour of the ring particles at their closest approach to Prometheus is analysed using numerical simulations. The results show that a gap and a wave are formed in the ring at each encounter with the satellite. However, the gap is expected to have a short lifetime due to keplerian shear. ?? 2000 Elsevier Science Ltd. All rights reserved.

Additional publication details

Publication type Article
Publication Subtype Journal Article
Title Perturbations to Saturn's F-ring strands at their closest approach to Prometheus
Series title Planetary and Space Science
Volume 48
Issue 9
Year Published 2000
Language English
Larger Work Type Article
Larger Work Subtype Journal Article
Larger Work Title Planetary and Space Science
First page 817
Last page 827
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