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1 Department of Earth Sciences, The University of Western Ontario, London, Ontario N6A 5B7 Canada
2 Research School of Earth Sciences, The Australian National University, Canberra, A.C.T. 0200, Australia
E-mail of corresponding author: fvitali{at}julian.uwo.ca
Oxygen-isotope data were obtained for synthetic aluminum-hydroxide phases precipitated over 65125 mo and have been compared to results from similar experiments conducted for 356 mo. The Al(OH)3 polymorphs, gibbsite, nordstrandite, and bayerite, were synthesized, but gibbsite was dominant in most samples, and commonly the only phase present. Using pure gibbsite samples, the following oxygen-isotope fractionation factors,
gibbsite-H2O, were obtained: 1.0167 ± 0.0003 (9 ± 1°C), 1.0147 ± 0.0007 (24 ± 2°C), 1.0120 ± 0.0003 (51 ± 2°C). These values, and the associated equation for an oxygen-isotope geothermometer for the interval 060°C, 103ln
gibbsite-H2O = 2.04 x 106/T2 3.61 x 103/T + 3.65 (T in K), are not significantly different from those obtained from experiments of much shorter duration. These results, and the good agreement with
gibbsite-H2O values obtained for well-constrained natural systems, suggest that the experimentally determined fractionation factors describe equilibrium conditions for gibbsite that has precipitated directly from solution.
As also proposed by others using a modified-increment calculation, our synthesis experiments suggest that
Al(OH)3-H2O is polymorph-dependent at low temperatures and that a significant temperature-dependent trend exists in the values of
Al(OH) 3-H2O. However, previously calculated fractionation factors obtained using the modified-increment method are higher than those obtained from the experiments, with this discrepancy becoming larger as temperature decreases.
Key Words: Aluminum Hydroxides Fractionation Factor Gibbsite Oxygen Isotope Synthesis
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