Abstract

Surface protonation is the most fundamental adsorption process of geochemical interest. Yet remarkably little is known about protonation of mineral surfaces at temperatures greater than 25°C. Experimentally derived standard enthalpies of surface protonation, ΔH r,1 °, ΔH r,2 °, and ΔH r,ZPC °, correspond to the reactions >SOH+H +=>SOH 2 + >SO −+H +=>SOH >SO −+2H +=>SOH 2 + respectively, and provide a starting point for evaluating the role of surface protonation in geochemical processes at elevated temperatures. However, the experimental data for oxides do not have a theoretical explanation, and data are completely lacking for silicates other than SiO 2. In the present study, the combination of crystal chemical and Born solvation theory provides a theoretical basis for explaining the variation of the enthalpies of protonation of oxides. Experimental values of ΔH r,1 °, ΔH r,2 °, and ΔH r,ZPC ° consistent with the triple layer model can be expressed in terms of the inverse of the dielectric constant (1/ε) and the Pauling bond strength per angstrom (s/r M-OH) of each mineral by equations such as ΔH r,ZPC °=ΔΩ r,Z[(1/ε)−(T/ε) 2(∂ε/∂T)]−B ′ Z(s/r M-OH)+H ′ Z. The Born solvation coefficient ΔΩ r,Z was taken from a prior analysis of surface equilibrium constants. The coefficients B Z ′ and H Z ′ were derived by regression of experimental enthalpies for rutile, γ-alumina, magnetite, hematite, and silica. This approach permits widespread prediction of the enthalpies of surface protonation. Predicted standard enthalpies of surface protonation for oxides and silicates extend over the ranges (in kcal.mole −1): ΔH r,1 ° ≈ −3 to −15; ΔH r,2 ° ≈ −0.5 to −18; ΔH r,ZPC ° ≈ −4 to −33. Minerals with the largest values of s/r M-OH (e.g., quartz and kaolinite) are predicted to have weakly negative enthalpies and a weak temperature dependence for their protonation equilibrium constants. Conversely, minerals with the smallest values of s/r M-OH (e.g., garnets and olivines) should have strong negative enthalpies and a strong temperature dependence for their protonation equilibrium constants.

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