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Long Periods in the Three-Dimensional Motion of Trojan Asteroids

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Dynamical Trapping and Evolution in the Solar System

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 106))

Abstract

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.

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Author information

Authors and Affiliations

  1. Astronomisches Rechen-Institut, Heidelberg, Germany, Federal Republic

    R. Bien & J. Schubart

Authors
  1. R. Bien
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  2. J. Schubart
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Editor information

Editors and Affiliations

  1. Dept. of Engineering Science, University of Patras, Patras, Greece

    Vassilis V. Markellos

  2. Tokyo Astronomical Observatory, Mitaka, Tokyo, 181, Japan

    Yoshihide Kozai

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© 1983 D. Reidel Publishing Company, Dordrecht, Holland

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Bien, R., Schubart, J. (1983). Long Periods in the Three-Dimensional Motion of Trojan Asteroids. In: Markellos, V.V., Kozai, Y. (eds) Dynamical Trapping and Evolution in the Solar System. Astrophysics and Space Science Library, vol 106. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7214-8_19

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  • DOI: https://doi.org/10.1007/978-94-009-7214-8_19

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7216-2

  • Online ISBN: 978-94-009-7214-8

  • eBook Packages: Springer Book Archive

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