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A Study of Chaos in the Asteroid Belt

  • M. Šidlichovský
  • D. Nesvorný
Part of the NATO ASI Series book series (ASIC, volume 522)

Abstract

Laskar’s results [1] on the chaotic motion of the inner planets, the existence of chaotic regions inside orbital resonances of asteroids, the movement of the rotational axis of Mars [2] and ultimately Earth’s unstable obliquity [3] brought the interest of astronomers back to the problem of chaos in the solar system. The possibilities of studies of chaos were recently widened from the original Poincaré mapping and Lyapunov characteristic coefficient (LCE) to Laskar frequency analysis [1] and [4], sup-map analysis [5], fast Lyapunov indicators [6] and local Lyapunov numbers distribution [7], [8] and [9].

Keywords

Solar System Chaotic Motion Chaotic Region Asteroid Belt Outer Planet 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Science+Business Media Dordrecht 1999

Authors and Affiliations

  • M. Šidlichovský
    • 1
  • D. Nesvorný
    • 2
  1. 1.Astronomical Institute of the Academy of Sciences of the Czech RepublicPraha 4Czech Republic
  2. 2.Instituto Astrônomico e GeofísicoUniversidade de São PauloSão PauloBrazil

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