Skip to main content

Formation of Satellite and Ring Systems: Comparatve Aspects

  • Conference paper
Comparative Planetology with an Earth Perspective
  • 85 Accesses

Abstract

There are four systems of a massive central body with a regularily structured satellite system in the Solar system: the planetary system and the satellite systems of Jupiter, Saturn and Uranus. Comparable structures in these four systems can be understood as indications for comparable processes of origin and formation. It is the aim of this paper to describe comparable properties, and to discuss possible physical processes in pre-satellite disks which can be the cause for this comparability.

This is a preview of subscription content, log in via an institution to check access.

Access this chapter

Chapter
USD 29.95
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
eBook
USD 39.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book
USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book
USD 54.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Purchases are for personal use only

Institutional subscriptions

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

The References

  • Cameron, A.G.W. (1978) Physics of the primitive Solar accretion disk, Moon and Planets, 98, 5–40

    Article  ADS  Google Scholar 

  • Harris, A.W. (1984) Origin of Planetary Rings, in Planetary Rings, ( R. Greenberg and A. Brahic, Eds., 641–659, U. of Arizona Press, Tucson

    Google Scholar 

  • Hayashi, C., Nakazawa, K., and Nakagawa Y. (1985) Formation of the Solar System, in Protostars and Planets II, eds. Black, D.C. and M.S. Matthews, 1100–1153, University of Arizona Press.

    Google Scholar 

  • Lang, K.R. (1992) Astrophysical Data, Planets and Stars, Springer Verlag

    Book  Google Scholar 

  • Lin, D.N.C. and J. Papaloizou (1985) On ther dynamical origin of the Solar system, in Protostars and Planets II, eds. D.C. Black and M.S. Matthews, 981–1072, University of Arizona Press

    Google Scholar 

  • Lissauer, J.J. and J.N. Cuzzi (1985) Rings and Moons:Clues to understanding the Solar nebula, in Protostars and Planets II, eds. D.C. Black and M.S. Matthews, 920–958, University of Arizona Press

    Google Scholar 

  • Safronov, V.S. (1972) in Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets,Moscow, Nauka, 1969), NASA-TT-F-667,1972

    Google Scholar 

  • Weidenschilling, S.J. and J.N. Cuzzi (1993) Formation of Planetesimals in the Solar Nebula, in Protostars and Planets III, eds. Levy, E.H. and J.I. Lunine, pp. 1031–1060, University of Arizona Press

    Google Scholar 

  • Wetherill, G.W. (1991) Formation of the Terrestrial Planets from Planetesimals, in Planetary Sciences, American and Soviet Research, ed. T. Donahue, Washington, Ntl. Acad. of Sciences Pres

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Editor information

Editors and Affiliations

Rights and permissions

Reprints and permissions

Copyright information

© 1995 Springer Science+Business Media Dordrecht

About this paper

Cite this paper

Möhlmann, D. (1995). Formation of Satellite and Ring Systems: Comparatve Aspects. 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_13

Download citation

  • DOI: https://doi.org/10.1007/978-94-017-1092-3_13

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-90-481-4636-9

  • Online ISBN: 978-94-017-1092-3

  • eBook Packages: Springer Book Archive

Publish with us

Policies and ethics