The Planetesimal Shock Model for Chondrule Formation: Improved Orbital Simulations and Extended Shock Fronts
Abstract
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.
- Publication:
-
42nd Annual Lunar and Planetary Science Conference
- Pub Date:
- March 2011
- Bibcode:
- 2011LPI....42.2068H