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Pluto's Lyapunov numbers in different dynamical models

Published online by Cambridge University Press:  25 May 2016

R. Dvorak
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraβe 17, A-1180 Vienna, Austria
E. Lohinger
Affiliation:
Institut für Astronomie, Universität Wien, Türkenschanzstraβe 17, A-1180 Vienna, Austria

Abstract

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We present the results of numerical integrations of Pluto and some fictitious Plutos in three different models (the circular and the elliptic restricted three body problem and the outer solar system). We determined the “extension” of the stable region in these models by means of the Lyapunov Characteristic Numbers and by an analysis of the orbital elements.

Type
Part II - Planets and Moon: Theory and Ephemerides
Copyright
Copyright © Kluwer 1996 

References

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