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Rapid Formation of Ice Giant Planets

✍ Scribed by Alan P. Boss; George W. Wetherill; Nader Haghighipour


Publisher
Elsevier Science
Year
2002
Tongue
English
Weight
94 KB
Volume
156
Category
Article
ISSN
0019-1035

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✦ Synopsis


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.


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