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Pierrehumbert, R · 2022 · arXiv 2212.02644

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A window for water-hydrogen demixing on warm metal-rich sub-Neptunes

astro-ph.EP · 2025-12-01 · conditional · novelty 6.0

Water-hydrogen demixing occurs on warm sub-Neptunes with envelope metallicities of 150-700 times solar, including TOI-270 d, implying layered interiors and underestimated bulk metallicities when using fully-miscible models.

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  • A window for water-hydrogen demixing on warm metal-rich sub-Neptunes astro-ph.EP · 2025-12-01 · conditional · none · ref 64

    Water-hydrogen demixing occurs on warm sub-Neptunes with envelope metallicities of 150-700 times solar, including TOI-270 d, implying layered interiors and underestimated bulk metallicities when using fully-miscible models.