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Evolution of Planetary Ringmoon Systems

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Book cover Comparative Planetology with an Earth Perspective

Abstract

The last few decades have seen an avalanche of observations of planetary ring systems, both from spacecraft and from Earth. Meanwhile, we have seen steady progress in our understanding of these systems as our intuition (and our computers) catch up with the myriad ways in which gravity, fluid and statistical mechanics, and electromagnetism can combine to shape the distribution of the submicron-to-several-meter size particles which comprise ring systems [1–5]. The now-complete reconnaissance of the gas giant planets by spacecraft has revealed that ring systems are invariably found in association with families of regular satellites, and there is an emerging perspective that they are not only physically but causally linked. There is also mounting evidence that many features or aspects of all planetary ring systems, if not the ring systems themselves, are considerably younger than the solar system.

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Authors and Affiliations

  1. Space Science Division, Ames Research Center, NASA, Moffett Field, California, 94035, USA

    Jeffrey N. Cuzzi

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  1. Jeffrey N. Cuzzi
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  1. Jet Propulsion Laboratory, Pasadena, CA, USA

    Moustafa T. Chahine  & Neil L. Nickle  & 

  2. University of Maryland, College Park, MD, USA

    Michael F. A’Hearn

  3. NASA Headquarters, Washington, DC, USA

    Jürgen Rahe

  4. Goddard Space Flight Center, Greenbelt, MD, USA

    Pamela Solomon

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Cuzzi, J.N. (1995). Evolution of Planetary Ringmoon Systems. In: Chahine, M.T., A’Hearn, M.F., Rahe, J., Solomon, P., Nickle, N.L. (eds) Comparative Planetology with an Earth Perspective. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1092-3_18

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  • DOI: https://doi.org/10.1007/978-94-017-1092-3_18

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