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

Open Access

Fig. 2

Composition of the different models at the start (top) and end (bottom) of the simulation at 4.5 Gyr. The x-axis shows the normalised mass and the y-axis the fraction of high-Z material, water in our case. The compositions ‘compact’, ‘extended’, and ‘metal-rich’ correspond to Hot_Compact_Z, Cold_extended_Z, and Cold_high_Z in Müller et al. (2020), respectively.

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