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Physical Processes Affecting the Motion of Small Bodies in the Solar System and their Application to the Evolution of Meteor Streams

Published online by Cambridge University Press:  12 April 2016

Iwan P. Williams
Iwan P. Williams*
Affiliation:
Applied Mathematics Department, Queen Mary College, Mile End Road, London E1 4NS

Abstract

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In addition to planetary perturbations, the small particles which make up a meteor stream are subject to outward radiation pressure and the Poynting-Robertson effect. New particles can also be generated in a stream through being released from the nucleus of a comet. We summarise the main physical effects, discuss models for meteor stream evolution and give a brief account of the observational data available.

Type
Part II - Comets and Meteor Streams
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 83 - 87
Copyright
Copyright © Reidel 1983

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