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3-D orbital evolution model of outer asteroid beltThe 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.
Document ID
19930010056
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Solovaya, Nina A. (Sternberg Astronomical Inst. Moscow, Ussr)
Gerasimov, Igor A. (Sternberg Astronomical Inst. Moscow, Ussr)
Pittich, Eduard M. (Slovak Academy of Sciences Bratislava, Czechoslovakia)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991
Subject Category
Astrophysics
Accession Number
93N19245
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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IDRelationTitle19930009924Collected WorksAsteroids, Comets, Meteors 1991
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