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Rapid Formation of Icy Super-Earths and the Cores of Gas Giant Planets

ASTROPHYSICAL JOURNAL LETTERS, no. 2 (2009): L140-L143

Cited: 72|Views24

Abstract

We describe a coagulation model that leads to the rapid formation of super-Earths and the cores of gas giant planets. Interaction of collision fragments with the gaseous disk is the crucial element of this model. The gas entrains small collision fragments, which rapidly settle to the disk midplane. Protoplanets accrete the fragments and g...More

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