Minor bodies of the solar system - Meteorite orbit interrelation and 'mirror symmetry' in the C-distribution

Details Minor bodies of the solar system - Meteorite orbit interrelation and 'mirror symmetry' in the C-distribution Minor bodies of the solar system - Meteorite orbit interrelation and 'mirror symmetry' in the C-distribution

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..258t&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, March 1989, p. 258-269. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Astronomical Photography, Meteoroid Concentration, Solar System, Asteroids, Meteoroid Showers, Orbit Perturbation

Scientific paper

The population of large meteor bodies having masses ranging from several kilograms to many tons is revealed by means of photographic observations of bright fireballs. It is found that 39 of the 69 objects of this population are meteorite producing. A unique class of meteorite orbits having an extremely short period is found. An analysis of the distributions of minor bodies using Tisserand's constant C (the perturbing planet is Jupiter) revealed the possibility of genetic connections and families inside the complex of minor bodies.

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