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A Window for Water-hydrogen Demixing on Warm Metal-rich Sub-Neptunes

  • Authors: Caroline Piaulet-Ghorayeb, Daniel P. Thorngren, Eliza M.-R. Kempton, Justin Lipper, Leslie Rogers, Fernanda Correa Horta, Shi Lin Sun

Caroline Piaulet-Ghorayeb et al 2026 The Astrophysical Journal 1006 .

  • Provider: AAS Journals

Caption: Figure 4.

Impact of physical parameters varied across the grid on the TP and pressure–radius profiles. The left, middle, and right panels illustrate the impact of varying the planet mass, envelope metallicity, and envelope mass fraction, respectively. Aside from the parameter varied in each panel, all other parameters are kept fixed to Teq = 381 K, Mp = 5.1M, and fenv = 8.79% (bolded profiles). Decreasing the equilibrium temperature shifts the envelope profiles, as illustrated in Figure B1.

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