Some kinematic characteristics of fragmented meteoric bodies

Details Some kinematic characteristics of fragmented meteoric bodies Some kinematic characteristics of fragmented meteoric bodies

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975avest...9...83k&link_type=abstract

Astronomicheskii Vestnik, vol. 9, Apr.-June 1975, p. 83-87. In Russian.

Astronomy and Astrophysics

Astronomy

1

Meteorite Collisions, Meteoroid Concentration, Meteoroid Showers, Orbital Elements, Radio Meteors, Asteroids, Kolmogoroff Theory, Meteoroid Dust Clouds

Scientific paper

The distribution of detection heights, velocities, and orbital elements
of fragmented and ordinary meteoric bodies are compared using
Kolmogorov's criterion. It is shown that the detection heights of both
types coincide, but the orbits of fragmented meteoric bodies have larger
dimensions, eccentricities, and aphelion distances than ordinary bodies.

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