2018
DOI: 10.1007/s00126-018-0850-0
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Trace element geochemistry of sphalerite in contrasting hydrothermal fluid systems of the Freiberg district, Germany: insights from LA-ICP-MS analysis, near-infrared light microthermometry of sphalerite-hosted fluid inclusions, and sulfur isotope geochemistry

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Cited by 136 publications
(61 citation statements)
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“…More in general the fluid inclusion features of SW Sardinia are comparable with those of the fluid trapped in inclusions of ore and gangue minerals in post-Variscan (i.e., Jurassic-Cretaceous) Ba-F-(Pb-Zn-Ag) and Pb-Zn. Ag deposits in Sardinia and Central-Western Europe [96][97][98][99][100][101][102]. From these analogies we can assume that at least the late depositional phase of the Co-Ni mineralization of SW Sardinia can be related to the circulation of a post-Variscan, Triassic to Jurassic-Cretaceous low-temperature H2O-NaCl-CaCl2 brine.…”
Section: Discussionmentioning
confidence: 99%
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“…More in general the fluid inclusion features of SW Sardinia are comparable with those of the fluid trapped in inclusions of ore and gangue minerals in post-Variscan (i.e., Jurassic-Cretaceous) Ba-F-(Pb-Zn-Ag) and Pb-Zn. Ag deposits in Sardinia and Central-Western Europe [96][97][98][99][100][101][102]. From these analogies we can assume that at least the late depositional phase of the Co-Ni mineralization of SW Sardinia can be related to the circulation of a post-Variscan, Triassic to Jurassic-Cretaceous low-temperature H2O-NaCl-CaCl2 brine.…”
Section: Discussionmentioning
confidence: 99%
“…In general, a shallow formation depth was proposed for Jurassic-Cretaceous deposits related to the flow of NaCl-CaCl2 brines. For example, a maximum cover of about 1500 m was considered for the Wittichen mineralization (SW Germany) by [95], whereas a thickness of 2-3 km the eroded cover was estimated for the hydrothermal vein-style mineralization of Cretaceous age of Freiberg (Germany) by [102]. Thus, assuming that also the Ni-Co mineralization of SW Sardinia were formed at similar shallow depth for a maximum thickness of cover of 3 km, corresponding to a maximum hydrostatic pressure of 30 MPa and a lithostatic pressure of 76 MPa (considering an average rock density of 2.6 g/cm 3 ).…”
Section: Discussionmentioning
confidence: 99%
“…This technological element, as well as germanium and gallium, is mostly recovered as a by-product from the production of other metals, chiefly zinc in sulfide minerals (i.e., sphalerite) [6], although important resources are described in tin ore as well [7,8]. Major hosts for indium include a variety of mineralization styles such as volcanic-hosted massive sulfide and stratabound carbonate-hosted deposits, greisen, polymetallic vein-type (s.l., including xenothermal deposits), porphyry tin, skarn and epithermal deposits, and important resources are reported in Bolivia, Peru, China, Japan, Canada, and Russia [9][10][11][12][13][14][15][16][17][18][19][20].…”
Section: Introductionmentioning
confidence: 99%
“…High concentrations of In have been described in sphalerite, cassiterite, chalcopyrite, stannite, tennantite, and tin sulfosalts [14]. Indium is not exploited as a primary commodity, but rather as a co-product or by-product of base metals, chiefly in zinc [15][16][17][18][19], but also in tin [20] and copper [21] ores.…”
Section: Introductionmentioning
confidence: 99%