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 inv
โฆ LIBER โฆ
A granular flow model for dense planetary rings
โ Scribed by Nicole Borderies; Peter Goldreich; Scott Tremaine
- Publisher
- Elsevier Science
- Year
- 1985
- Tongue
- English
- Weight
- 952 KB
- Volume
- 63
- Category
- Article
- ISSN
- 0019-1035
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