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Title: Origin of meteor swarms of the Arietid and Geminid types

Journal Article · · Sol. Syst. Res. (Engl. Transl.); (United States)
OSTI ID:5874898

The author proposes a physical mechanism for the formation of meteor swarms on orbits of small size and very small perihelion distance, similar to the orbits of Arietid and Geminid meteor swarms, which are rarely encountered among the larger bodies of the solar system, and he justifies the mechanism mathematically. He shows that comets can transfer to such orbits from orbits of large size during evaporation of their ice nuclei under the action of reactive drag.

Research Organization:
Institute of Experimental Meteorology, Goskomgidromet
OSTI ID:
5874898
Journal Information:
Sol. Syst. Res. (Engl. Transl.); (United States), Vol. 19:2; Other Information: Translated from Astronomicheskii Vestnik, Vol. 19, No. 2, pp. 152-158, April-June, 1985
Country of Publication:
United States
Language:
English

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