Convective mixing in distant and close-in giant planets - Dependences on the initial composition, luminosity, bloating, and semi-convection

Open Access

Fig. 4

Final composition of the compact and extended initial compositional structures for orbital distances of 0.05 and 0.03 AU. The standard case at 5.2 AU is shown for comparison. For the hot Jupiters, the bloating efficiency is in both cases 0.5%.

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