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Pluto's Lyapunov numbers in different dynamical models
Published online by Cambridge University Press: 25 May 2016
Abstract
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.
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- Part II - Planets and Moon: Theory and Ephemerides
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- Copyright © Kluwer 1996
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