Formation of the giant planets

@inproceedings{DAngelo2006FormationOT,
  title={Formation of the giant planets},
  author={Gennaro D’Angelo and Jack J. Lissauer},
  year={2006}
}
The observed properties of giant planets, models of their evolution and observations of protoplanetary disks provide constraints on the formation of gas giant planets. The four largest planets in our Solar System contain considerable quantities of hydrogen and helium, which could not have condensed into solid planetesimals within the protoplanetary disk. All three (transiting) extrasolar giant planets with well determined masses and radii also must contain substantial amounts of these light… 

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