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• W3104582507 abstract "Transiting planets with radii 2–3 R⊕ are much more numerous than larger planets. We propose that this drop-off is so abrupt because at R ∼ 3 R⊕ base-of-atmosphere pressure is high enough for the atmosphere to readily dissolve into magma, and this sequestration acts as a strong brake on further growth. The viability of this idea is demonstrated using a simple model. Our results support extensive magma–atmosphere equilibration on sub-Neptunes, with numerous implications for sub-Neptune formation and atmospheric chemistry." @default.
• W3104582507 created "2020-11-23" @default.
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• W3104582507 date "2019-12-17" @default.
• W3104582507 modified "2023-10-17" @default.
• W3104582507 title "Superabundance of Exoplanet Sub-Neptunes Explained by Fugacity Crisis" @default.
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• W3104582507 doi "https://doi.org/10.3847/2041-8213/ab59d9" @default.
• W3104582507 hasPublicationYear "2019" @default.
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