The Geology of the Nifty Copper Deposit, Throssell Group, Western Australia: Implications for Ore Genesis
Anderson, B.R. and Gemmell, J.B. and Berry, R.F. (2001) The Geology of the Nifty Copper Deposit, Throssell Group, Western Australia: Implications for Ore Genesis. Economic Geology, 96 (7). pp. 1535-1565. ISSN 0361-0128 ![[img]](http://eprints.utas.edu.au/style/images/fileicons/application_pdf.png) | PDF - Full text restricted - Requires a PDF viewer 1892Kb | |
Official URL: http://dx.doi.org/10.2113/96.7.1535 AbstractThe Nifty syndeformational, sediment-replacement Cu deposit is located approximately 450 km southeast of
Port Hedland, Western Australia, in subgreenschist-grade rocks of the Neoproterozoic Paterson orogen. The
resource of 99 million metric tons (Mt) @1.7 percent Cu is hosted in a syncline within carbonaceous and
dolomitic shales of the upper Broadhurst Formation.
The Cu mineralization occurred during Neoproterozoic DY2 deformation and formed at the center of a
zoned hydrothermal alteration system. Interbedded dolomitic and carbonaceous shale of the upper and lower
units of the Nifty member was altered S in two stages. Early siliceous S alteration with minor chlorite, pyrite,
hematite, sericite, and stilpnomelane, which was replaced by syntectonic black quartz in the core of the deposit.
On the fringes of the alteration, framboidal pyrite in the carbonaceous shale was replaced by quartz, chalcopyrite,
euhedral pyrite, sphalerite, and galena. Inward is a sequence of interlayered hydrothermal quartzdolomite
and unaltered shale beds. The hydrothermal quartz-dolomite first appears as spots and 2- to
4-mm-thick veins with light gray diffuse margins. In areas of intense spotty alteration, dolomitic alteration
forms bedding-parallel zones. Farther inward and proximal to the highest ore grade is silicified dolomitic shale,
which grades into fine-grained quartz and chalcopyrite, with minor fluorapatite and carbonaceous material.
Synmineralization fluid inclusions are small (10 microns) liquid-vapor inclusions with homogenization temperatures
between 200 degrees to 370 degrees C (median 270 degrees C) and salinity of 8 to 27 wt percent NaCl equiv (median 15 wt % NaCl equiv). Sulfur isotope data from framboidal pyrite range between delta 34 SCDT of -27 and +16 per mil, chalcopyrite delta 34 SCDT ranges between -6 and +6 per mil, and delta 34 SCDT for euhedral, synmineralization pyrite ranges between -12 to +12 per mil. Carbon and oxygen isotope results from synmineralization vein stage carbonates
and dolomitic alteration overlap with delta 13 CVPDB values from +2 to -10 per mil and delta 18O VSMOW values from 14 to
21 per mil. It is likely that decarbonation of host rock caused the large shift in delta 13 CVPDB values.
The formation of the Nifty Cu deposit is linked to deformation (tectonic loading) associated with the Miles
orogeny driving fluids from deep in the Yeneena basin. Hydrothermal fluids were focused along DY2 thrust
faults. During tightening of the Nifty syncline, thrust faulting penetrated carbonaceous and dolomitic shales,
allowing hydrothermal fluids to react with the Nifty member. Early fluid pulses were weakly oxidized and contained low concentrations of base metals. These fluids altered the host rock and precipitated green quartz.
The fluid evolved to a hotter, more saline, reduced and moderately acidic fluid with significant Cu concentration.
These fluids reacted with the dolomite-dominated Nifty member, forming the dolomitic alteration and
siliceous replacement of carbonaceous shale and dolomitic mudstone. Chalcopyrite precipitation was controlled
mainly by changes in pH accompanied by a slight decrease in temperature. The mineralization and alteration
styles at Nifty are similar to the copper orebodies at Mount Isa. Item Type: | Article |
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Keywords: | sediment-hosted copper deposit, paragenesis, structural control, hydrothermal alteration, fluid inclusions |
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Subjects: | 260000 Earth Sciences > 260100 Geology |
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Collections: | UNSPECIFIED |
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ID Code: | 1968 |
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Deposited By: | Mrs Katrina Keep |
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Deposited On: | 27 Sep 2007 |
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Last Modified: | 23 Jan 2008 14:27 |
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