Fig. 10
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Mass-radius diagram of the well-characterised small planet population (Mp < 40 M⊕, Rp < 4 R⊕, mass error better than 25%, radius error better than 8%) from the PlanetS catalogue (Otegi et al. 2020; Parc et al. 2024) (semi-transparent circles), coloured by insolation. TOI-2322 b and c are shown as a pentagon and a hexagon, respectively. The composition models of Zeng et al. (2019) are shown by the coloured curves.
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