Motion and disintegration of meteorites in planetary atmospheres

Details Motion and disintegration of meteorites in planetary atmospheres Motion and disintegration of meteorites in planetary atmospheres

Nov 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979kosis..17..875g&link_type=abstract

Kosmicheskie Issledovaniia, vol. 17, Nov.-Dec. 1979, p. 875-893. In Russian.

Physics

23

Atmospheric Effects, Atmospheric Entry, Meteorite Craters, Meteoritic Damage, Planetary Atmospheres, Atmospheric Density, Atmospheric Heating, Atmospheric Pressure, Cratering, Earth Atmosphere, Pressure Gradients, Shock Fronts, Tungusk Meteorite

Scientific paper

A common characteristic of the moon and terrestrial planets is an abundance of impact craters. A number of impact structures have been found on the earth. The problem of identifying the differences in crater characteristics, caused by the difference of the planetary atmospheres is seen to depend primarily on the determination of the nature of meteorite transformation in a planetary atmosphere.

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