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astro-ph2008★ 23 cited
Core instability models of giant planet accretion II: forming planetary systems
Yamila Miguel, Adrian Brunini
We develop a simple model for computing planetary formation based on the core instability model for the gas accretion and the oligarchic growth regime for the accretion of the soli…
astro-ph2008
Constraints to Uranus' Great Collision. IV. The Origin of Prospero
Gabriela Parisi, Giovanni Carraro, Michele Maris +1
It is widely accepted that the large obliquity of Uranus is the result of a great tangential collision (GC) with an Earth size proto-planet at the end of the accretion. We attempt…