Orbit stability of minor planets in the outer part of the asteroid belt

Details Orbit stability of minor planets in the outer part of the asteroid belt Orbit stability of minor planets in the outer part of the asteroid belt

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mvsfa..31...72g&link_type=abstract

Moskovskii Universitet, Vestnik, Seriia 3 - Fizika, Astronomiia (ISSN 0579-9392), vol. 31, May-June 1990, p. 72-75. In Russian.

Astronomy and Astrophysics

Astronomy

Asteroid Belts, Librational Motion, Orbit Perturbation, Three Body Problem, Eccentric Orbits, Orbital Mechanics

Scientific paper

It is shown in the framework of the plane circular restricted three-body problem that, in the case of first-order resonances, asteroids that are unstable in the Hill sense can nevertheless have stable orbits. In the outer part of the asteroid belt, resonance effects can lead to stable resonance orbits characterized by librational motion. Limits and periods of eccentricity variation are calculated for a specific group of asteroids.

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