The Planetesimal Shock Model for Chondrule Formation: Improved Orbital Simulations and Extended Shock Fronts

Details The Planetesimal Shock Model for Chondrule Formation: Improved Orbital Simulations and Extended Shock Fronts The Planetesimal Shock Model for Chondrule Formation: Improved Orbital Simulations and Extended Shock Fronts

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2068h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2068

Physics

1

Scientific paper

The efficiency of potential chondrule formation in shock waves produced
by planetesimals passing through jovian resonances is evaluated further
using an improved planetesimal accretion and orbital evolution code.

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