The common origin and evolution of the meteoric bodies which produce radio and photographic meteors

Details The common origin and evolution of the meteoric bodies which produce radio and photographic meteors The common origin and evolution of the meteoric bodies which produce radio and photographic meteors

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982avest..15..216l&link_type=abstract

(Astronomicheskii Vestnik, vol. 15, Oct.-Dec. 1981, p. 216-219.) Solar System Research, vol. 15, no. 4, Apr. 1982, p. 160-163. T

Astronomy and Astrophysics

Astronomy

Interplanetary Dust, Meteoroids, Radio Meteors, Astronomical Photography, Orbital Elements

Scientific paper

On the basis of an analysis of orbit catalog data for radio meteors and photographic meteors, it has been shown that taking the geometric observability factor into account for photographic meteors leads to similar distributions of the orbital elements of meteoric bodies in the broad interval of masses from 0.000001 g to 10 g. This indicates a common nature for the origin and for the basic mechanisms of the disappearance of the majority of the dust particles of these masses in the interplanetary dust cloud.

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