Letter | Published:

How Prometheus creates structure in Saturn's F ring

Abstract

Images of Saturn's narrow and contorted F ring returned by the Cassini spacecraft1 have revealed phenomena not previously detected in any planetary ring system. The perturbing effect of the inner shepherding satellite, Prometheus, seems to introduce channels through the F ring and a ‘streamer’—a line of particles that link the ring to the satellite. The detailed mechanism for the formation of these features has been lacking an explanation. Here we show that these phenomena can be understood in terms of a simple gravitational interaction as Prometheus approaches and recedes from the F ring every 14.7 hours. Our numerical models show that as Prometheus recedes from its closest approach to the F ring, it draws out ring material; one orbital period later, this affected region has undergone keplerian shear and is visible as a channel, in excellent agreement with structures seen in the Cassini images. Prometheus' periodic disruption of the F ring will become more pronounced as the two orbits approach their minimum separation in 2009. The model predicts that the appearance of streamers and the associated channels will vary in a regular fashion on a timescale of one orbital period.

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Acknowledgements

C.D.M., K.B., N.C. and M.W.E. are grateful to the UK Particle Physics and Astronomy Research Council for financial support. C.C. thanks the Astronomy Unit, Queen Mary, University of London and the Mexican Council for Science and Technology, CONACYT, for financial support. J.A.B. was supported by the Cassini project and Cornell University. C.C.P. acknowledges support from NASA/JPL and the Cassini project.

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Correspondence to Carl D. Murray.

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Reprints and permissions information is available at npg.nature.com/reprintsandpermissions. The authors declare no competing financial interests.

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Further reading

Figure 1: Cassini images of Saturn's F ring.
Figure 2: Numerical modelling of an encounter between Prometheus and the F ring.
Figure 4: Another comparison between a Cassini image and our model for the same configuration.
Figure 3: Comparison between a Cassini image and our model for the same configuration.

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