Fig. 13

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Mass-radius relationships for supercritical water (SW) planets (Acuña et al. 2021; Mousis et al. 2020), planets with Earth-like cores and H/He atmospheres (Zeng et al. 2019), and dry planets with different Fe contents (Brugger et al. 2017). We assume high chemical equilibrium temperatures for supercritical and H/He volatile layers of 1200 K and 2000 K, respectively. The position of TOI-969 b is indicated as a magenta star.
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