by
in - Porter, T.M. (Ed), 2002 - Hydrothermal Iron Oxide Copper-Gold & Related Deposits: A Global Perspective, volume 2;
ABSTRACT
The Khetri, Alwar and Lalsot-Khankhera Copper Belts contain widespread Cu±Au±Ag±Co±Fe±REE±U mineralization over a
Directly to the east of Khetri, a 50 km wide by > 100 km zone of calc silicate and albite-haematite alteration overprints and cross-cuts metamorphic fabrics. Calc silicate alteration comprises coarse-grained clinopyroxene - hornblende - epidote - apatite - scapolite - titanite - magnetite, whereas albite - haematite alteration comprises assemblages of albite - amphibole - haematite - magnetite - calcite, with variable K-feldspar, biotite, epidote, scapolite, titanite, apatite and fluorite, and locally abundant pyrite and chalcopyrite. Albite-haematite alteration is spatially related to vein systems and breccias, which commonly contain Cu-Au mineralization, massive magnetite-haematite vein-deposits, fluorite mineralization and rare uraninite deposits. Calc silicate alteration occurs on the margins of the Khetri Copper Belt, whereas albite-haematite alteration forms a central core to the Belt and locally overprints calc-silicate assemblages. A SHRIMP U-Pb titanite age in the assemblage albite - haematite - amphibole - calcite - titanite constrains the timing of regional alteration to 847±8 Ma. This overlaps the fission-track ages of garnet from ore assemblages at Madhan-Kudhan Cu mine at Khetri (897±125 Ma).
There is a variation in the sulfide-oxide mineralogy of Cu deposits across the >100 km wide Khetri Copper Belt, with four dominant types recognized: (1) chalcopyrite-pyrite-pyrrhotite ores hosted by graphitic schists at Akwali, in the west, (2) chalcopyrite - pyrite - pyrrhotite - magnetite - haematite ores at Khetri and Kho Dariba, in the east, (3) magnetite - haematite - chalcopyrite - pyrite ores hosted by albite-haematite alteration, in the central part of the Khetri Copper Belt, and (4) haematite - chalcopyrite - baryte ores in the eastern part of the Belt. Types (1) and (2) are hosted by mainly reduced rock types and can be classified as iron sulfide Cu-Au deposits, whereas types (3) and (4) are iron oxide Cu-Au deposits hosted by oxidized rocks. Copper mineralization in the Khetri Copper Belt is epigenetic, broadly synchronous with late (0.75-0.85 Ga) A-type granitoid emplacement, and has a mineralization and structural style, and regional- and deposit-scale alteration assemblages comparable to known IOCG and iron-sulfide Cu-Au mineralized districts.
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