The fraction of potential meteorite-generating bodies among interplanetary solid bodies

Details The fraction of potential meteorite-generating bodies among interplanetary solid bodies The fraction of potential meteorite-generating bodies among interplanetary solid bodies

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991avest..25..200l&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 25, Mar.-Apr. 1991, p. 200-207. In Russian.

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4

Atmospheric Entry, Iron Meteorites, Meteoritic Composition, Stony Meteorites, Aerobraking, Fragmentation, Mathematical Models

Scientific paper

This paper presents a method developed for determining meteoroid types by semiempirical simulations of observed meteor heights with allowance for fragmentation. Dense stone and iron meteoroids account for 12 percent of all meteoroids entering the earth's atmosphere. The other meteoroids are very rich in volatile compounds, are very porous, or consist mainly of organic compounds.

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