Dust Size Distribution in Solar Nebula Inferred from Shock-Wave Heating Model for Chondrule Formation

Details Dust Size Distribution in Solar Nebula Inferred from Shock-Wave Heating Model for Chondrule Formation Dust Size Distribution in Solar Nebula Inferred from Shock-Wave Heating Model for Chondrule Formation

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1612m&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1612

Physics

Scientific paper

We simulated chondrule formation by the shock-wave heating model. We
could reproduce the size distribution of chondrules in ordinary
chondrites from narrow-ranged precursor size distibution, not from a
power-law precursor size distribution.

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