An atomic level study of rhenium and radiogenic osmium in molybdenite

被引:40
|
作者
Takahashi, Yoshio
Uruga, Tomoya
Suzuki, Katsuhiko
Tanida, Hajime
Terada, Yasuko
Hattori, Keiko H.
机构
[1] Hiroshima Univ, Grad Sch Sci, Dept Earth & Planetary Syst Sci, Hiroshima 7398526, Japan
[2] Hiroshima Univ, Lab Multiple Isotope Res Astro Geochem Evolut, MIRAGE, Hiroshima 7398526, Japan
[3] Japan Synchrot Radiat Res Inst, Spring 8, Sayo Cho, Hyogo 6795198, Japan
[4] Japan Agency Marine Earth Sci & Technol, Inst Res Earth Evolut, Yokosuka, Kanagawa 2370061, Japan
[5] Univ Ottawa, Dept Earth Sci, Ottawa, ON K1N 6N5, Canada
基金
日本学术振兴会;
关键词
D O I
10.1016/j.gca.2007.08.007
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
Local atomic structures of Re and radiogenic Os in molybdenite from the Onganja mine, Namibia, were examined using X-ray absorption fine structure (XAFS). Rhenium L-M-edge X-ray absorption near-edge structure (XANES) and extended Xray absorption fine structure (EXAFS) show that the oxidation state of Re, the interatomic distances between Re and the neighboring atoms, and the coordination number of Re to S are very similar to those of Mo in molybdenite. The results confirm that Re is present as Re(W) in the Mo site in molybdenite. Measurement of L-M-edge XANES and EXAFS of a minor concentration (8.55 ppm) of radiogenic Os was accomplished in fluorescence mode by removing the interfering X-rays from Re and other elements using a crystal analyzer system. The data indicate that the oxidation state of radiogenic Os is Os(III) and Os(IV) and clearly different from Os(11) in natural sulfide minerals, such as OsS2 (erlichmanite). XANES data also suggest that radiogenic Os does not form a secondary Os phase, such as OsS2 or Os metal, in molybdenite. EXAFS of radiogenic Os was successfully simulated assuming that Os is present in the Mo site in molybdenite. The data are consistent with the XANES data; Os does not form Os phases in molybdenite. The EXAFS simulation showed that the interatomic distance between Os and S is 2.27 angstrom, which is 0. 12 angstrom smaller than the distances of Re-S and Mo-S (2.39 angstrom) in molybdenite. Similar valences and ionic sizes of Re and Mo in molybdenite support the fact that large amounts of Re can be incorporated into the Mo site as has been observed in previous studies, whereas the different properties of Os compared to Mo and Re suggested here support much lower abundance of common Os in molybdenite. This makes molybdenite an ideal mineral for the Re-Os geochronometer as shown in many studies. However, the shorter distance between radiogenic Os and S compared to those of Re-S and Mo-S in molybdenite suggests that the radiogenic Os has a smaller ionic size than Re(W) and Mo(W). Furthermore, Os may be partly present as Os(III). Smaller and lower charge Os can diffuse faster than larger and higher charge Re in molybdenite at a given set of conditions. Hence, our study provides an atomic-level explanation for the high mobility of Os compared to Re, which has been suggested by earlier workers using laser ablation ICP-MS. (c) 2007 Published by Elsevier Ltd.
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页码:5180 / 5190
页数:11
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