Shock heating of chondrules

Details Shock heating of chondrules Shock heating of chondrules

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985metic..20..359t&link_type=abstract

Meteoritics (ISSN 0026-1114), vol. 20, pt. 2, June 30, 1985, p. 359-365.

Physics

1

Chondrule, Comets, Shock Heating, Solar System, Eccentric Orbits, Gas Density, Gas Heating, Kepler Laws, Mach Number, Meteorites, Shock Effects, Heating, Chondrules, Nebula, Hypotheses, Source, Size, Mass, Velocity, Gases, Cooling, Dust, Particles, Calculations, Models

Scientific paper

The present consideration of the hypothesis that chondrules may have been heated by shock waves in the early solar nebula suggests that, although suitable heating rates would be produced in the wake of cometary bodies in eccentric orbits, their coming to rest with respect to the nebula in a relatively short time indicates that the total mass of the exciting solid bodies would have to have been about 10 percent of that of the heated gas. Attention is given to the shock heating of the gas, the heating of the dust, and the area of the wake shock.

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