The nebular shock wave model for chondrule formation - Simulations and comparisons with meteoritic constraints

Details The nebular shock wave model for chondrule formation - Simulations and comparisons with meteoritic constraints The nebular shock wave model for chondrule formation - Simulations and comparisons with meteoritic constraints

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..591h&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 591.

Computer Science

Nebulae, Shock Waves, Chondrule, Computerized Simulation, Meteorites, Constraints, Accretion Disks, Heating

Scientific paper

Improved numerical simulations and analytical calculations are presented for gas dynamic shock waves, occurring in a relatively cool and dusty nebular environment, which will allow more detailed comparisons with meteoritic constraints. Simulations conducted for the case of a 1D, optically thick dust cloud indicate that radiative cooling times of the order of hours are possible.

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