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Fig. 4

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Evolution models of K2-18b. Top panel : planetary radius as a function of age. The black errorbar corresponds to the measured radius and age. Bottom panel : heavy-element mass fraction at 2.4 Gyr (the planet’s age) as a function of pressure. We note that condensation was not considered in our models, which explains why some models have a high heavy-element mass fraction at low pressures.

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