Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-12-17
Icarus 156 (2002) 291
Astronomy and Astrophysics
Astrophysics
TeX file, 20 pages, no figures, 1 table, accepted by Icarus, Preprints available at http://www.ciw.edu/boss/ftp/planets/icaice
Scientific paper
10.1006/icar.2002.6816
The existence of Uranus and Neptune presents severe difficulties for the core accretion model for the formation of ice giant planets. We suggest an alternative mechanism, namely disk instability leading to the formation of gas giant protoplanets, coagulation and settling of dust grains to form ice/rock cores at their centers, and photoevaporation of their gaseous envelopes by a nearby OB star, as a possible means of forming ice giant planets.
Boss Alan P.
Haghighipour Nader
Wetherill George W.
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