What confines the rings of Saturn?
Radwan Tajeddine, Philip D. Nicholson, Pierre-Yves Longaretti, Maryame, El Moutamid, Joseph A. Burns

TL;DR
This paper clarifies that multiple satellites collectively confine Saturn's A ring through resonances and flux reversal, and estimates the ring's viscosity profile, contrasting with the B ring where Mimas alone suffices for confinement.
Contribution
It demonstrates the combined effect of several satellites on A ring confinement and provides a detailed viscosity profile, challenging the single-resonance confinement assumption.
Findings
A ring is confined by multiple satellite resonances, not just Janus.
The effective viscosity in the A ring decreases with radius from ~50 to <10 cm2 s-1.
Mimas alone can confine the B ring edge, with a relatively constant viscosity of ~24-30 cm2 s-1.
Abstract
The viscous spreading of planetary rings is believed to be counteracted by satellite torques, either through an individual resonance or through overlapping resonances. For the A ring of Saturn, it has been commonly believed that the satellite Janus alone can prevent the ring from spreading via its 7:6 Lindblad resonance. We discuss this common misconception and show that, in reality, the A ring is confined by the contributions from the group of satellites Pan, Atlas, Prometheus, Pandora, Janus, Epimetheus, and Mimas, whose cumulative torques from various resonances gradually decrease the angular momentum flux transported outward through the ring via density and bending waves. We further argue that this decrease in angular momentum flux occurs through 'flux reversal'. Furthermore, we use the magnitude of the satellites' resonance torques to estimate the effective viscosity profile…
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Taxonomy
TopicsAstro and Planetary Science
