Cosmogonic regularities in the complex of near parabolic comets

Details Cosmogonic regularities in the complex of near parabolic comets Cosmogonic regularities in the complex of near parabolic comets

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003kfnt...19..523k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, vol. 19, no. 6, p. 523-533

Physics

Scientific paper

The statistical analysis of near-parabolic of comets system (n = 1177 orbits, P> 200 years) has been executed. The distributions of comet orbital elements are obtained. It has been shown that the comet perihelia have the maximum concentration within heliocentric distances r = 0.7...0.9 A.U., volume density of perihelia with the distance r = 3.5 A.U. tends to zero. Similarly, the nodes concentrate at small heliocentric distances. It has been shown that near-parabolic comets pass in the solar system predominantly through the zone of terrestrial planets. The apsides of the majority of comets make a small angle with vector of the peculiar motion of the Sun. The poles of comet orbits find out heightened concentration about both poles of the ecliptic and to the point λ = 900, β = 530. A system of short perihelion Kreutz comets (n = 372 orbits, q < 0.01 A.U.) has been researched separately.

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