Evolution of meteor orbits under the influence of secular perturbations

Details Evolution of meteor orbits under the influence of secular perturbations Evolution of meteor orbits under the influence of secular perturbations

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982avest..15..180g&link_type=abstract

(Astronomicheskii Vestnik, vol. 15, July-Sept. 1981, p. 180-186.) Solar System Research, vol. 15, no. 3, Jan. 1982, p. 132-137.

Astronomy and Astrophysics

Astronomy

Meteoroids, Orbit Perturbation, Secular Variations, Solar Orbits, Apsides, Jupiter (Planet), Temporal Distribution

Scientific paper

Secular perturbations for 15 different meteor orbits are investigated over time intervals of 10,000-100,000 years, to obtain a qualitative picture of the evolution of the orbits. The Gauss-Halphen-Goryachev method is used, taking into account the perturbations of Jupiter, Saturn, Uranus and Neptune. The occurrence of N, S (or N, Q, S) branches in a stream is found possible due to the determining role of Jupiter and the character of perturbations from it when the direction of the line of apsides maintains relative stability. It is concluded that the age of meteor streams containing branches should not be less than 3000-4000 years.

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