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Mass–Radius Relationships for Irradiated Ocean Planets

  • Authors: Artyom Aguichine, Olivier Mousis, Magali Deleuil, and Emmanuel Marcq

2021 The Astrophysical Journal 914 84.

  • Provider: AAS Journals

Caption: Figure 3.

Color maps showing ﹩{\gamma }_{+}﹩ (top panel) and ﹩{\gamma }_{-}﹩ (bottom panel) in the H2O phase diagram. The phase diagram of water is identical to the one shown in Figure 1. Ma19+, Ma19-, and WP02- are the (P,T) profiles defined in the case of a 1 ﹩{M}_{\oplus }﹩ planet fully made of H2O, with the atmospheric part shown with short dashes. Ma19- and WP02- interiors are almost indistinguishable, hence are represented by the same color, and all atmospheric profiles are identical, although the gravity at the boundary is different for each case.

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