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The Stability of Some Asteroids

Published online by Cambridge University Press:  12 April 2016

R.O. Vicente
R.O. Vicente*
Affiliation:
Faculty of Sciences, University of Lisbon, Portugal

Abstract

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The utilization of two different stability criteria, namely, Hill's modified stability criterium and the method of surface of section, has been employed for asteroid orbits. The idea is to compute different criteria of stability for the same asteroids in order to compare the results and see the practical interest of the computations for researches about evolutionary trends of individual asteroids, groups and families of asteroids.

Type
Part III - Asteroids
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 137 - 139
Copyright
Copyright © Reidel 1983

References

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Vicente, R.O.: 1979 in Szebehely, V.G. (ed.) “Instabilities in Dynamical Systems”, D. Reidel Publ. Co., Dordrecht, Holland, pp. 211–225 Google Scholar