Particle Residence Times in Solar Nebula Environments: Chemical Evolution Due to Radial Motions in an Evolving Disk

Details Particle Residence Times in Solar Nebula Environments: Chemical Evolution Due to Radial Motions in an Evolving Disk Particle Residence Times in Solar Nebula Environments: Chemical Evolution Due to Radial Motions in an Evolving Disk

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1101c&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1101

Computer Science

Scientific paper

We develop a Monte Carlo model to calculate particle paths in an
evolving solar nebula and to quantify the time spent in different
environments. The model is used to understand the nebular processing
experienced by meteoritic components.

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