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Models of Jupiter's Growth Incorporating Thermal and Hydrodynamic Constraints
Jack J. Lissauer, Olenka Hubickyj, Gennaro D'Angelo +1
[Abridged] We model the growth of Jupiter via core nucleated accretion, applying constraints from hydrodynamical processes that result from the disk-planet interaction. We compute…
On the Luminosity of Young Jupiters
M. S. Marley, J. J. Fortney, O. Hubickyj +2
Traditional thermal evolution models of giant planets employ arbitrary initial conditions selected more for computational expediency than physical accuracy. Since the initial condi…
Young Jupiters are Faint: New Models of the Early Evolution of Giant Planets
J. J. Fortney, M. S. Marley, O. Hubickyj +2
Here we show preliminary calculations of the cooling and contraction of a 2 MJ planet. These calculations, which are being extended to 1-10 MJ, differ from other published "cooling…