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Published October 1976 | public
Journal Article

Hydrogen isotope fractionation between OH-bearing minerals and water

Abstract

Hydrogen isotope fractionation factors between hydroxyl-bearing minerals and water were determined at temperatures ranging between 400 and 850°C. The hydrogen isotope exchange rates for the mineral-water pairs examined were very slow. In most cases it was necessary to use an interpolation method for the determination of the hydrogen isotope equilibrium fractionation factor, α_e. For the temperature range of 450–850°C the hydrogen isotope fractionation factors for the mica-water and amphibole-water systems are simply expressed as a function of temperature and the molar fractions of the six-fold coordinated cations in the crystal, regardless of mineral species, as follows: 10^3 In α_(e(mineral-water)) = − 22.4 (10^6T^(−2)) + 28.2 + (2X_(Al) − 4X_(Mg) − 68X_(Fe)), where X is the molar fraction of the cations. As the equation indicates, for any specific composition of the OH-bearing minerals, the change of α_e with temperature, over the temperature range investigated, is the same for all minerals studied. Thus for any specified values of X_(Al), X_(Mg), and X_(Fe) for these minerals, the relationship between α_e and T is 10^3 In α_e = αT^(−2) + k. Consequently, hydrogen isotope fractionation among coexisting minerals is temperature independent and cannot be used as a hydrogen isotope geothermometer. Some exceptions to the above general observations exist for minerals such as boehmite and kaolinite. In these minerals hydrogen bonding modifies the equilibrium hydrogen isotopic fractionation between mineral and water.

Additional Information

© 1976 Pergamon Press. Received 23 November 1975; accepted in revised form 7 April 1976. We wish to thank Professor H. P. TAYLOR, JR. and Professor A. L. ALBEE for stimulating discussions and for supplying the samples for some of this work. Our gratitude to Dr. PAUL KNAUTH for a critical reading of this manuscript. We also thank Mrs. E. BINGHAM for performing the emission spectrographic analyses. Financial support was provided by the National Science Foundation Grant No. GA-12945.

Additional details

Created:
August 19, 2023
Modified:
October 25, 2023