Asteroid Formation with a Pre-Existing Jupiter

Details Asteroid Formation with a Pre-Existing Jupiter Asteroid Formation with a Pre-Existing Jupiter

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1796k&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1796

Physics

5

Scientific paper

If Jupiter formed quickly by the disk-instability mechanism, then growth
of Ceres-size asteroids requires: (1) little or no migration of Jupiter
before dissipation of the solar nebula, or (2) some asteroid growth
prior to Jupiter's formation.

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