2002
DOI: 10.2113/gsecongeo.97.3.481
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The Hishikari Au-Ag Epithermal Deposit, Japan: Oxygen and Hydrogen Isotope Evidence in Determining the Source of Paleohydrothermal Fluids

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Cited by 69 publications
(46 citation statements)
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“…Carbonate precipitation may have been enhanced after periods of increased surface evaporation or, alternatively due to magmatic fluid flashing. Although low sulfidation epithermal systems are most commonly dominated by meteoric fluids (Simmons et al, 2005), significant magmatic contributions have also been reported (e.g., Faure et al, 2002). An important difference between El Peñón and other low sulfidation deposits such as Golden Cross (New Zealand) or Hishikari (Japan) is the climate at the time of mineralization.…”
Section: Stable Isotope Datamentioning
confidence: 99%
“…Carbonate precipitation may have been enhanced after periods of increased surface evaporation or, alternatively due to magmatic fluid flashing. Although low sulfidation epithermal systems are most commonly dominated by meteoric fluids (Simmons et al, 2005), significant magmatic contributions have also been reported (e.g., Faure et al, 2002). An important difference between El Peñón and other low sulfidation deposits such as Golden Cross (New Zealand) or Hishikari (Japan) is the climate at the time of mineralization.…”
Section: Stable Isotope Datamentioning
confidence: 99%
“…1, Ibaraki and Suzuki, 1993). The deposit has been known to have extremely high grade gold ores since exploitation started in 1985 (Abe et al, 1986;Chadwick, 1989;Faure et al, 2002). Although the grade is now falling as mining progresses to deeper levels, production in 2002 was about 160,000 metric tons grading 45 g/t Au and 20 g/t Ag.…”
Section: Geologic Setting and Mineralizationmentioning
confidence: 99%
“…From this work they inferred that mineralizing fluids were a mixture of magmatic water and meteoric water. Faure et al (2002) expanded the existing oxygen and hydrogen isotope database to include six other veins, and also suggested that ore-bearing fluids may be mixtures of meteoric and magmatic waters.…”
Section: Geologic Setting and Mineralizationmentioning
confidence: 99%
“…Based on Hand O-isotope studies, the ore-forming fluids in these systems are a combination of heated meteoric water (O'Neil et al, 1973;John et al, 2003;Simmons et al, 2005;Saunders et al, 2008;Saunders et al, 2015) and primary magmatic fluids (Matsuhisa and Aoki, 1994;Hayashi et al, 2000;Faure et al, 2002;Heinrich et al, 2004;Williams-Jones and Heinrich, 2004;Saunders et al, 2008;Saunders et al, 2015).…”
Section: Chapter 1 -Introductionmentioning
confidence: 99%