The diffusion of comets according to the Tisserand constant

Details The diffusion of comets according to the Tisserand constant The diffusion of comets according to the Tisserand constant

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...13b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, May-June 1985, p. 13-16. In Russian.

Computer Science

Numerical Analysis

Celestial Mechanics, Comets, Diffusion, Orbital Mechanics, Solar System, Three Body Problem, Jupiter (Planet), Orbit Perturbation

Scientific paper

On the basis of a numerical analysis of the orbits of a number of real and 'hypothetical' comets, it is demonstrated that the diffusion of comets in the solar system is related to the Tisserand constant. It is pointed out that the diffusion is significant only for comets with Tisserand constants of more than 0.450. A list of Tisserand constants for the orbits of 29 periodic comets is provided.

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