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- W1979005199 abstract "The Galileo probe showed that Jupiter's atmosphere is severely depleted in neon compared to protosolar values. We show, via ab initio simulations of the partitioning of neon between hydrogen and helium phases, that the observed depletion can be explained by the sequestration of neon into helium-rich droplets within the postulated hydrogen-helium immiscibility layer of the planet's interior. We also demonstrate that this mechanism will not affect argon, explaining the observed lack of depletion of this gas. This provides strong indirect evidence for hydrogen-helium immiscibility in Jupiter." @default.
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- W1979005199 date "2010-03-22" @default.
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- W1979005199 title "Sequestration of Noble Gases in Giant Planet Interiors" @default.
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- W1979005199 doi "https://doi.org/10.1103/physrevlett.104.121101" @default.
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