Orbital evolution of comets Kearns-Kwee /1963 VIII/ and Lexell /1770 I/ and some characteristics of cometary-orbit transformations in Jupiter's zone of influence

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Comets, Jupiter (Planet), Orbit Perturbation, Orbital Elements, Gravitational Effects, Planetary Gravitation, Secular Variations

Scientific paper

Characteristics of the secular evolution of cometary orbits are studied using the orbits of two comets, Kearns-Kwee and Lexell, which penetrated exceptionally deep into Jupiter's zone of influence. Three variants are considered for the orbital evolution of Kearns-Kwee over 400 years (1660 to 2060) and for that of Lexell over the period from 1770 to 2060. The following characteristics of orbital transformations are established: (1) Jupiter may capture a comet in two stages, first by transforming hyperbolic or elliptic transplutonian orbits into short-period orbits with aphelia between the orbits of Uranus and Neptune and then by capturing the comet into the Jupiter family; (2) Jupiter may reeject the comet from its family into another, very remote planetary family and then return it to the fold; and (3) for extremely deep penetration into its zone of influence and appropriate close-encounter conditions, Jupiter may eject a comet from its family into a transplutonian or long-period orbit or even send it along a hyperbola into interstellar space.

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