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Long Periods in the Three-Dimensional Motion of Trojan Asteroids

Published online by Cambridge University Press:  12 April 2016

R. Bien  and
J. Schubart
R. Bien
Affiliation:
Astronomisches Rechen-Institut, Heidelberg, Germany, Federal Republic
J. Schubart
Affiliation:
Astronomisches Rechen-Institut, Heidelberg, Germany, Federal Republic

Abstract

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The long periods caused by Jupiter, or Jupiter and Saturn in the motion of a Trojan are studied by numerical integration. Orbital inclinations between 0° and 50° are considered. Results on the length of the periods and on their main effects in the osculating elements are presented. It turns out that secular resonances can be important for the evolution of Trojan orbits.

Type
Part III - Asteroids
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 153 - 161
Copyright
Copyright © Reidel 1983

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