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Viscosity in a Dense Planetary Ring with Self-Gravitating Particles

✍ Scribed by Hiroshi Daisaka; Hidekazu Tanaka; Shigeru Ida


Publisher
Elsevier Science
Year
2001
Tongue
English
Weight
745 KB
Volume
154
Category
Article
ISSN
0019-1035

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✦ Synopsis


We have investigated the viscosity (the angular momentum flux) in dense, self-gravitating particle disks such as Saturn's main ring, by performing local N-body simulations. Viscosity could play important roles in evolution and structure formation of planetary rings. The ring's viscosity has been investigated with both theoretical and numerical approaches (e.g., Goldreich and Tremaine, 1978,