4:00 PM - 4:15 PM
[HRE11-07] Spatial variation of the δ18O and δD isotopic signatures of ore-forming fluids within a Au-bearing vein in the Hishikari deposits, Kagoshima, Japan
Keywords:Oxygen and hydrogen isotopes, fluid inclusion microthermometry, serial sampling, Hishikari Au-Ag deposits, low-sulfidation epithermal deposits
The spatial variation of δ18O of quartz (n = 41), adularia (n = 8), and smectite, chlorite, illite, and chlorite-smectite mixed layer (n = 8), as well as the δD values of smectite, chlorite, illite, and chlorite-smectite mixed layer (n = 8) were systematically analyzed in relation to Au grade. Additionally, fluid inclusion microthermometry was also conducted for all samples with fluid inclusions suitable for observation to calculate the δ18O of H2O of the ore-forming fluids. Results show that the modes of homogenization temperatures range from 160 to 240 °C, with most samples having the mode of 200 – 210 °C. The average salinities fall within a narrow range from 2.3 to 3.9 wt. % NaCl eq., with an average of 3.0 wt.% NaCl eq. The δ18O values of quartz and adularia relative to Vienna Standard Mean Ocean Water (VSMOW) do not vary significantly. The δ18O of quartz ranges from +6.3 to +9.2 ‰ with an average of +7.5 ‰ while the δ18O of adularia ranges from +4.6 to +9.1 ‰ with an average of +5.9 ‰. On the other hand, the calculated δ18O of H2O of the ore-forming fluids from the early adularia (δ18Owater = -3.7 to +1.2 ‰, average = -2.2 ‰) is slightly higher than that from the later quartz (δ18Owater = -6.8 to -0.8 ‰, average = -3.7 ‰), which suggests a decrease in δ18O as mineralization progresses, possibly due to the dilution effect of mixing with 18O-depleted meteoric water (e.g. Matsuhisa and Aoki, 1994). The range of δ18O and δD of H2O calculated from mixed smectite, chlorite-smectite, and illite in the altered host rock (δ18Owater = +3.6 to +8.9 ‰, δDwater = -77 to -62 ‰) are higher than those from smectite and chlorite-smectite in the vein (δ18Owater = +1.3 to +8.5 ‰, δDwater = -132 to -92.5 ‰). This may have been due to varying contributions from local meteoric waters (18O-depleted and D-enriched), meteoric waters that reacted with the 18O-enriched and D-depleted sedimentary basement rocks, and contributions from primary magmatic waters (18O- and D-enriched). Another possibility is the lower temperature in hydrothermal alteration than that of vein formation.
Statistical analysis showed that the calculated δ18O of H2O of the ore-forming fluids from quartz, adularia, and clay minerals have a positive relationship with Au grade. This is also supported by the distribution of higher δ18O values (> -2.0 ‰) of the waters located at the high Au-grade zone (> 1,000 ppm) at the center part of the vein. The relatively higher δD values of H2O (> -110 ‰) were also found in the high Au-grade zone.
References
Matsuhisa, Y. and Aoki, M. (1994) Temperature and oxygen isotope variations during formation of the Hishikari epithermal gold-silver veins, southern Kyushu, Japan. Economic Geology, 89, 1608-1613.