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Low Velocity Encounters of Minor Bodies With the Outer Planets

Published online by Cambridge University Press:  12 April 2016

A. Carusi ,
E. Perozzi  and
G.B. Valsecchi
A. Carusi
Affiliation:
I.A.S-C.N.R, Reparto di Planetologia, Roma (Italy)
E. Perozzi
Affiliation:
I.A.S-C.N.R, Reparto di Planetologia, Roma (Italy)
G.B. Valsecchi
Affiliation:
I.A.S-C.N.R, Reparto di Planetologia, Roma (Italy)

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Previous studies of close encounters of minor bodies with Jupiter have shown that the perturbations are stronger either if the encounter is very deep or if the velocity of the minor body relative to the planet is low. In the present research we investigate the effects of low velocity encounters between fictitious minor bodies and the four outer planets. Two possible outcomes of this type of encounter are the temporary satellite capture of the minor body by the planet, and the exchange of perihelion with aphelion of the minor body orbit. Different occurrence rates of these processes are found for different planets, and the implications for the orbital evolution of minor bodies in the outer Solar System are discussed.

Type
Part VI - Miscellaneous Dynamics
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 377 - 395
Copyright
Copyright © Reidel 1983

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