Ohmic dissipation in hot Jupiters
We present an isolated analytical model for the ohmic heating in the interior of hot jupiters, treating the wind zone as a parameterized boundary condition. Under a conserved estimation of the strength of induced field and the assumption of an isothermal-convective planet model, we conclude that the mechanism of ohmic heating may not explain the over ...
Huang, Chelsea (Xu), Cumming, Andrew
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Lyons JR.
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Biddle LI +4 more
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Sagear S, Ballard S.
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Bonidie V +9 more
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Gupta AF +59 more
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Challener RC +35 more
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Lunine JI, Bahcall N.
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Earth-mass planets with He atmospheres in the habitable zone of Sun-like stars. [PDF]
Lammer H +6 more
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Planets larger than Neptune have elevated eccentricities. [PDF]
Gilbert GJ, Petigura EA, Entrican PM.
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