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- W4313593043 abstract "Thermodynamic calculations using the critically evaluated and optimized FactSage databases lead to the conclusion that chondrules of all types were formed from a “rain cloud” of undercooled liquid oxide droplets that were in equilibrium with the solar nebula. The droplets subsequently solidified rapidly and stochastically in the temperature and pressure gradients of the nebula to form solid chondrules that retained the compositions of the liquid droplets and thereafter were no longer in thermodynamic equilibrium with the nebular gas. This provides a simple unified model for the formation of chondrules in all chondrite meteorites including chondrule-like calcia alumina inclusions, anorthite-rich chondrules, and magnesio-silicate chondrules. Other models of chondrule formation, including the currently favored models of melting of pre-existing solids, are not consistent with thermodynamic calculations." @default.
- W4313593043 created "2023-01-06" @default.
- W4313593043 creator A5075815101 @default.
- W4313593043 date "2023-01-04" @default.
- W4313593043 modified "2023-09-25" @default.
- W4313593043 title "Thermodynamic Calculations Support a Rain Cloud Model of Chondrule Formation" @default.
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- W4313593043 doi "https://doi.org/10.1021/acsearthspacechem.2c00276" @default.
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