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From Newton to Chaos pp 199–208Cite as

Meteoroid Stream Dynamics

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Part of the book series: NATO ASI Series ((NSSB,volume 336))

Summary

The formation of meteoroid streams, the forces affecting their subsequent motion and the techniques used in order to understand their dynamical evolution are discussed. One example of Chaotic motion is given in the final section.

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Author information

Authors and Affiliations

  1. Astronomy Unit, Queen Mary & Westfield College, Mile End Rd, London, E1 4NS, UK

    I. P. Williams

Authors
  1. I. P. Williams
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Editor information

Editors and Affiliations

  1. Dept. of Physics and Astronomy, Glasgow University, G12 8QQ, Glasgow, UK

    Archie E. Roy

  2. Dept. of Mathematics, Glasgow Caledonian University, G4 0BA, Glasgow, UK

    Bonnie A. Steves

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© 1995 Springer Science+Business Media New York

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Williams, I.P. (1995). Meteoroid Stream Dynamics. In: Roy, A.E., Steves, B.A. (eds) From Newton to Chaos. NATO ASI Series, vol 336. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-1085-1_18

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  • DOI: https://doi.org/10.1007/978-1-4899-1085-1_18

  • Publisher Name: Springer, Boston, MA

  • Print ISBN: 978-1-4899-1087-5

  • Online ISBN: 978-1-4899-1085-1

  • eBook Packages: Springer Book Archive

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