On the dynamics in the asteroids belt. Part I : General theory View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1989-06

AUTHORS

Alessandro Morbidelli, Antonio Giorgilli

ABSTRACT

The classical problem of the dynamics in the asteroids belt is revisited in the light of recently developed perturbation methods. We consider the spatial problem of three bodies both in the circular and in the elliptic case, looking for families of periodic or quasi periodic orbits. Some criteria for deciding the stability of these families are also indicated. More... »

PAGES

145-172

References to SciGraph publications

  • 1989-06. Motion near the 3/1 resonance of the planar elliptic restricted three body problem in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1986-04. The reducing transformation and Apocentric Librators in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1984-02. High-order resonances in the restricted three-body problem in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1978-04. Formal integrals for an autonomous Hamiltonian system near an equilibrium point in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1985-10. Rigorous estimates for the series expansions of Hamiltonian perturbation theory in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1983-06. A second fundamental model for resonance in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/bf00051203

    DOI

    http://dx.doi.org/10.1007/bf00051203

    DIMENSIONS

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