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• W1988227418 abstract "A study has been carried out of the vaporization of a totally molten silicate magma of chondritic composition heated into the range 2500–3500 K. The motivation for this was to determine the changes in the composition of the mantle that would occur in the Mercury protoplanet should that body have been subjected to the high-temperature phase in the evolution of the primitive solar nebula, but the results are of more general interest. We have used both ideal and nonideal descriptions of the magma chemistry. An empirical model, based on ideal mixing of complex components, developed by Hastie and co-workers, was used to describe the nonideal magma. Comparison of our results of the nonideal magma calculations with experimental work on vaporization of chondritic material shows generally good agreement. We find that vaporization of about 70–80% of the original amount of silicate from a chondritic planet is required to produce an iron-rich body with a mean uncompressed density equal to that deduced for Mercury (5.3 g/cm3). At this point the silicate is depleted in the alkalis, FeO, and SiO2, and enriched in CaO, MgO, Al2O3, and TiO2 relative to chondritic material. We also predict the production of unique trace element abundance patterns which are depleted in easily oxidized elements relative to other trace elements of similar volatilities." @default.
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• W1988227418 date "1987-04-01" @default.
• W1988227418 modified "2023-10-02" @default.
• W1988227418 title "A vaporization model for iron/silicate fractionation in the Mercury protoplanet" @default.
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• W1988227418 doi "https://doi.org/10.1016/0012-821x(87)90196-8" @default.
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