Change of meteor stream density due to planetary perturbation

Details Change of meteor stream density due to planetary perturbation Change of meteor stream density due to planetary perturbation

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..188e&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, July-Sept. 1985, p. 188-194) Solar System Research (ISSN 0038-0946), vol. 19, no. 3, Jan. 19

Astronomy and Astrophysics

Astronomy

Meteoroid Concentration, Orbit Perturbation, Solar Orbits, Draconid Meteoroids, Equations Of Motion, Leonid Meteoroids, Numerical Differentiation, Orbital Elements, Quadrantid Meteoroids

Scientific paper

A method for estimating local spatial density changes in meteor streams due to planetary perturbation is developed. The evolution of density in the orbits of several meteor streams affected by perturbation from Jupiter is studied. It is shown that there is the possibility both of a decrease and of a considerable temporary increase of local density due to planetary perturbation. Examples are given of stable periodic oscillations in stream density.

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