Fig. A.1
Our H2O (left) and SiO2 (right) EOS: pressure (color) vs. temperature and density. Rectangles mark the relevant regimes of the Uranus inner Z region (white), gradient region (gray), and envelope (black), based on the models of this work. The regime for the adiabatic Uranus (Nettelmann et al. 2013) is shown (dashed purple) for comparison. The EOS range for Uranus models is much larger than the range for the adiabatic structure.
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