Abstract
The energy parameters of ore-forming deep fluid systems (enthalpy and Gibbs free energy) for compounds of S, Cl, and B have been estimated by thermodynamic methods at a lithosphere depth of 1000–20 km. At a depth of 1000 km, ore-forming fluids are dominated by BF3. With a decrease in a depth to 100–20 km, the range of fluid ore-forming systems becomes wider due to the B, F, Cl, and S compounds providing a real basis for development of the voluminous ore-forming fluid systems at the top of the lithosphere.
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F. A. Letnikov, A. F. Letnikova, and B. S. Danilov, Dokl. Earth Sci. 453 (2), 1234–1237 (2013).
F. A. Letnikov, B. S. Danilov, and P. I. Dorogokupets, Dokl. Earth Sci. 437 (2), 548–551 (2011).
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Original Russian Text © F.A. Letnikov, B.S. Danilov, A.F. Letnikova, 2018, published in Doklady Akademii Nauk, 2018, Vol. 481, No. 3.
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Letnikov, F.A., Danilov, B.S. & Letnikova, A.F. Energy Parameters of Ore-Forming Deep Fluid Systems. Dokl. Earth Sc. 481, 877–878 (2018). https://doi.org/10.1134/S1028334X18070255
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DOI: https://doi.org/10.1134/S1028334X18070255