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Granular Gases pp 330-349 | Cite as

Numerical Simulations of the Collisional Dynamics of Planetary Rings

  • Heikki Salo
Chapter
Part of the Lecture Notes in Physics book series (LNP, volume 564)

Abstract

Numerical simulations of planetary ring dynamics are reviewed, with main emphasis on local 3-dimensional simulations, which utilize a co-moving calculation cell with periodic boundary conditions. Various factors affecting the local balance between collisional dissipation and viscous gain of energy from the systematic velocity field are considered, including gravitational encounters and collective gravitational forces besides physical impacts. Simulation examples of the effects of particle size distribution, particles’ spin motion, and different forms of the coefficient of restitution are given. Viscous stability properties are also briefly discussed: examples of both instabilities and overstabilities are given. In this context 2D-simulations are useful, eventhough physically unrealistic even for extremely flattened planetary ring systems.

Keywords

Orbital Period Velocity Dispersion Identical Particle Dense Ring Impact Frequency 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer-Verlag Berlin Heidelberg 2001

Authors and Affiliations

  • Heikki Salo
    • 1
  1. 1.Division of AstronomyUniversity of OuluOuluFinland

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