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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 B1.

TP profile for the envelope (colors) and interior (dotted, gray) across all conditions in the grid, compared to the coexistence curves (median is black dashed, and 95% C.I. shown as gray shading), for different envelope metallicities (labeled for each panel). The color shadings encode the planet mass for the three temperatures explored in the grid (shades of blue for Teq = 381 K, green for Teq = 361 K, red for Teq = 336 K). The vertical and horizontal span in TP space is kept constant throughout all panels to illustrate the compositional dependence of the demixing window.

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