An analysis of the nature of the destruction of bolide-forming bodies

Details An analysis of the nature of the destruction of bolide-forming bodies An analysis of the nature of the destruction of bolide-forming bodies

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..19..243k&link_type=abstract

(Astronomicheskii Vestnik, vol. 19, July-Sept. 1985, p. 243-250) Solar System Research (ISSN 0038-0946), vol. 19, no. 3, Jan. 19

Other

Bolides, Meteorites, Astronomical Catalogs, Fragmentation, Heat Transfer Coefficients, Opacity

Scientific paper

A preliminary analysis of the physical parameters for bright bolides has been carried out for the material of the Prairie Network Catalog. Chondrite-type cosmic bodies are destroyed in the earth's atmosphere at significantly lower values of the heat-transfer coefficient than other types of bodies. To describe them, the development of a bolide model with a two-phase layer of ablation products and which allows for a convective component of heat transfer to the body are required. Upon entry into the earth's atmosphere, other cosmic bodies produce bolides which can be satisfactorily described in the framework of a model with a transparent layer of vapors. These bodies can experience intense fragmentation in the atmosphere.

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