Physics
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992kfnt....8...55g&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 8, Jan.-Feb. 1992, p. 55-61. In Russian.
Physics
Comets, Jupiter (Planet), Saturn (Planet), Solar Activity, Celestial Mechanics, Solar Planetary Interactions, Three Body Problem
Scientific paper
The characteristics of comets with aphelia from 7.46 to 14.2 AU were analyzed. The statistical criteria used show that they differ considerably from the Jupiter family. This is particularly evident in the parameters q, i, J (Jacobi constant), and L (perihelion longitude), in the dependence H10(q), in the dynamics of the increase of the number of comets, and in the response of comets to solar activity. The analysis of the J values with reference to Jupiter and Saturn shows that the comets belong to the family of the latter. The assumption that this group of comets is an intermediate one is rejected.
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