Space Science Reviews

, Volume 116, Issue 1, pp 457–470

Dynamics and Composition of Rings

Article

DOI: 10.1007/s11214-005-1966-y

Cite this article as:
Sicardy, B. Space Sci Rev (2005) 116: 457. doi:10.1007/s11214-005-1966-y

Abstract

Planetary rings are found around all four giant planets of our solar system. These collisional and highly flattened disks exhibit a whole wealth of physical processes involving dust grains up to meter-sized boulders. These processes, together with ring composition, can help understand better the formation and evolution of proto-satellite and proto-planetary disks in the early solar system. The present chapter reviews some fundamental aspects of ring dynamics and composition. The forthcoming exploration of the Saturn system by the Cassini mission will bring both high resolution and time-dependent information on Saturn’s rings.

Keywords

rings disks dynamics planetary formation 

Copyright information

© Springer Science + Business Media, Inc. 2005

Authors and Affiliations

  1. 1.Observatoire de Paris and Université Pierre et Marie CurieMeudonFrance
  2. 2.Bruno Sicardy, Observatoire de Paris, LESIAMeudon CédexFrance

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