The motion of meteor swarms near commensurabilities with Jupiter

Details The motion of meteor swarms near commensurabilities with Jupiter The motion of meteor swarms near commensurabilities with Jupiter

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..651e&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, July 1988, p. 651-658. In Russian. In Russian.

Computer Science

Numerical Analysis

2

Jupiter (Planet), Meteoroid Showers, Orbital Resonances (Celestial Mechanics), Perturbation Theory, Numerical Analysis, Stochastic Processes

Scientific paper

The dynamic features of meteor swarms are considered on the basis of the resonant theory of perturbations. The parameters of the main resonant zones near the orbits of the principal meteor swarms are determined. Laws governing the variation of the spatial density of meteor swarms due to the properties of librational, circulational, and stochastic motion are established. Examples of the possible appearance of resonance features in the observed meteor showers are indicated.

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