Libration of Laplace’s Argument in the Galilean Sstellites Theory View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1984

AUTHORS

J. Henrard

ABSTRACT

In the Galilean satellites motion, the Laplace argument λ1 - 3 λ2 + 2 λ3 librates around the value π. The amplitude of libration is very small so that the classical theories have not been set up to take into account large librations. On the other hand large librations have to be considered when we describe possible scenarii of capture into resonance by tidal effects. The aim of this paper is to present a new way of applying Hamiltonian perturbation methods to the problem of the Galilean satellites in such a way that the theory is valid for large librations. Preliminary results from such a theory are discussed. More... »

PAGES

255-262

References to SciGraph publications

  • 1979-06. How tidal heating in Io drives the galilean orbital resonance locks in NATURE
  • 1983-06. A second fundamental model for resonance in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1977-10. The long period behavior of the orbits of the Galilean satellites of Jupiter in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Book

    TITLE

    The Stability of Planetary Systems

    ISBN

    978-94-010-8854-1
    978-94-009-5331-4

    Author Affiliations

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/978-94-009-5331-4_23

    DOI

    http://dx.doi.org/10.1007/978-94-009-5331-4_23

    DIMENSIONS

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