Some Implications of Meteoritic Constraints for Chondrule Formation Models Including the Bow Shock Model

Details Some Implications of Meteoritic Constraints for Chondrule Formation Models Including the Bow Shock Model Some Implications of Meteoritic Constraints for Chondrule Formation Models Including the Bow Shock Model

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1551w&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1551

Physics

1

Scientific paper

The lack of chemical and isotopic fractionation in chondrules implies
that they formed in a uniform nebular midplane layer, not in turbulence.
If melted by bow shocks, the supersonic bodies were large, i.e., Moon-
to Mars-sized.

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