NASA NTRS · 19930010056
3-D orbital evolution model of outer asteroid belt
Abstract
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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Solovaya, Nina A., Gerasimov, Igor A., Pittich, Eduard M.. 1992-01-01. 3-D orbital evolution model of outer asteroid belt. https://ntrs.nasa.gov/citations/19930010056
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