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Young Jupiters are faint: new models of the early evolution of giant planets

✍ Scribed by J. J. Fortney; M. S. Marley; O. Hubickyj; P. Bodenheimer; J. J. Lissauer


Publisher
John Wiley and Sons
Year
2005
Tongue
English
Weight
210 KB
Volume
326
Category
Article
ISSN
0004-6337

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We present a three-dimensional cloud model designed for the study of formation and evolution of moist convective storms on the giant planets. This is a finite-difference model that solves the dynamic and thermodynamic equations forward in time under the anelastic approximation including microphysics