Open Access

Fig. 5

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Evolutionary sequence of the pressure-temperature profiles near the surface of the planet. The first profile (on the right) corresponds to t = 1 Myr, while the last one (on the left) is at t = 4.6 Gyr. The thick black lines show radiative zones. The blue dotted line is the profile measured by the Galileo space probe (from Lodders & Fegley 1998).

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