Formation of the Kirkwood gaps in the asteroid belt View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1984-09

AUTHORS

A. Lemaitre

ABSTRACT

A possible mechanism to explain the depletion of the Kirkwood gaps in the asteroid belt would be the slow dissipation of the solar nebula at the origin of the Solar System. The effects of this dissipation on a uniform distribution of asteroids are explored by means of the adiabatic invariant theory for the 2/1, 3/1 and 5/2 resonance cases. The framework is the restricted, circular and planar three body problem. More... »

PAGES

329-341

References to SciGraph publications

  • 1982-05. Capture into resonance: An extension of the use of adiabatic invariants in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1977-09. The distribution of mass in the planetary system and solar nebula in ASTROPHYSICS AND SPACE SCIENCE
  • 1978-02. Physics of the primitive solar accretion disk in THE MOON AND THE PLANETS
  • 1983-07. The gravitational potential due to uniform disks and rings in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1984-02. High-order resonances in the restricted three-body problem 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/bf01235812

    DOI

    http://dx.doi.org/10.1007/bf01235812

    DIMENSIONS

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