Collisional Evolution of a Massive Planetesimal Disk During Slow Migration of the Outer Planets

Details Collisional Evolution of a Massive Planetesimal Disk During Slow Migration of the Outer Planets Collisional Evolution of a Massive Planetesimal Disk During Slow Migration of the Outer Planets

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.2107w&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

If the outer planets migrated by eroding a massive disk of
planetesimals, collisional lifetimes in the disk had to be comparable to
the migration timescale. This sets lower limits on the mean planetesimal
size and mass of the debris disk.

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