Quasicontinuous fragmentation of meteorites

Details Quasicontinuous fragmentation of meteorites Quasicontinuous fragmentation of meteorites

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981avest..15...36l&link_type=abstract

(Astronomicheskii Vestnik, vol. 15, Jan.-Mar. 1981, p. 36-43.) Solar System Research, vol. 15, no. 1, July 1981, p. 27-34. Tran

Other

Fragmentation, Luminous Intensity, Meteorites, Stony Meteorites, Astronomical Photometry, Deceleration, Density Distribution, Meteor Trails

Scientific paper

Equations for calculating the luminuous intensity curves and estimating the deceleration and other characteristics of meteors produced by meteorites experiencing quasicontinuous fragmentation are derived. Comparison with observation data shows that all the basic observed characteristics of photographic meteors can be adequately explained within the framework of the model of quasi-continuous fragmentation of compact stone meteorites with an effective fragmentation energy of 1.6 x 10 to the 10th erg/g and a fragment mass of 0.00001-0.0001 g.

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