Physics
Scientific paper
Nov 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..375n&link_type=abstract
In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed
Physics
2
Comets: Migration
Scientific paper
An unified quadrature (in closed form) for determination of migration time of comets with arbitrary initial values of inclination (0≤i≤180°) and eccentricities (e<1) of their orbits from various hypothetical and real cometary's reservoirs in the Solar system (Oort's Cloud, Hills' Cloud, Kuiper Belt, space near planets, space near secondary planets) and an algebraic equation of 14-th degree (in realty the products of two polynomials of 7-th degree) for determination of the initial conditions at which cometary's nuclei escape the sphere of action of the central bodies or fall down on the central bodies, based on the double-averaged Hills' model of secular interactions between a comet, oblate central body (the Sun, a planet, a secondary planet) and perturbed body (the Galaxy nuclei, the Sun, a planet) are set up at the first time. The origin of high values of eccentricities and inclinations of typical cometary's orbit and possible interstellar origin of some comets are also discussed.
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