Modeling Planetesimal Accretion in Protoplanetary Disks Perturbed by Massive Companions

Details Modeling Planetesimal Accretion in Protoplanetary Disks Perturbed by Massive Companions Modeling Planetesimal Accretion in Protoplanetary Disks Perturbed by Massive Companions

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2283k&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

Scientific paper

We present results from a new code for modeling accretion in
protoplanetary systems perturbed by massive companions. In a test case
using Jupiter and Saturn as the perturbers, lunar-sized planetary
embryos formed near 1 AU in about 25,000 years.

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