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Fig. B.1
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Comparison of Uranus adiabats calculated with different water EOSs. The dashed lines show adiabats from Cano Amoros et al. (2024), using AQUA. We calculated adiabats at similar conditions (T1bar = 72 K) using QEOS, shown with solid lines. Colors refer to different assumed water mass fractions in the planetary envelope.
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