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• W2051246393 abstract "Observational and theoretical considerations, including near-surface energy constraints, suggest a model of Io that features a surface layer of sulfur overlying an active silicate crust. Such a model would imply frequent contact between silicate magma intrusions and the sulfur layer. This contact could produce volcanic plumes driven by high-temperature sulfur vapor. Plumes driven by sulfur vapor meet observational constraints for a wide range of possible conditions, in contrast to the special conditions required for plume generation by SO2. Characteristics of the two models are compared, and it is suggested that high-spatial-resolution infrared radiometry could identify the driving volatile." @default.
• W2051246393 created "2016-06-24" @default.
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• W2051246393 date "1980-11-01" @default.
• W2051246393 modified "2023-09-25" @default.
• W2051246393 title "Io: Energy constraints and plume volcanism" @default.
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• W2051246393 doi "https://doi.org/10.1016/0019-1035(80)90019-6" @default.
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