3-D orbital evolution model of outer asteroid belt

Details 3-D orbital evolution model of outer asteroid belt 3-D orbital evolution model of outer asteroid belt

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..565s&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 565-568 (SEE N93-19113 06-90)

Physics

Asteroid Belts, Planetary Evolution, Planetary Orbits, Three Body Problem, Three Dimensional Models, Asteroids, Inclination, Jacobi Integral, Stability

Scientific paper

The evolution of minor planets in the outer part of the asteroid belt is
considered. In the framework of the semi-averaged elliptic restricted
three-dimensional three-body model, the boundary of regions of the
Hill's stability is found. As was shown in our work, the Jacobian
integral exists.

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