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The chaotic dynamics of comets and the problems of the Oort cloudThe dynamic properties of comets entering the planetary zone from the Oort cloud are discussed. Even a very slight influence of the large planets can trigger stochastic cometary dynamics. Multiple interactions of comets with the large planets produce diffusion of the parameters of cometary orbits and a mean increase in the semi-major axis of comets. Comets are lifted towards the Oort cloud, where collisions with stars begin to play a substantial role. The transport of comets differs greatly from the customary law of diffusion and noticeably alter cometary distribution.
Document ID
19910013666
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Sagdeev, Roald Z.
(Institute of Space Research Moscow, Ussr)
Zaslavskiy, G. M.
(Institute of Space Research Moscow, Ussr)
Date Acquired
September 6, 2013
Publication Date
January 1, 1991
Publication Information
Publication: NAS-NRC, Planetary Sciences: American and Soviet Research
Subject Category
Astrophysics
Accession Number
91N22979
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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