Introduction
Background
The Girilambone copper deposits of New South Wales (NSW), Australia are noted for well-crystalised specimens of azurite, malachite, native copper and cuprite. These deposits are located ~45 km north-west of Nyngan and 100 km east-north-east of Cobar, NSW (Fig. 1). The focus of the present study is on the Girilambone (31°15′30.0797″S, 146°52′14.1934″E) and Girilambone North (31°13′19.4131″S, 146°50′54.1273″E) deposits, and excludes the Budgery, Budgerygar, Tritton and Great Hermidale deposits located to the southwest. The Girilambone deposit was mined in the Murrawombie pit, while the Girilambone North deposits were mined in the Hartmans, Larsens East, and Northeast pits (Fig. 2).
Index map of the study area. The map on the left shows the location of the study area within New South Wales (inset) and at the regional level. Red dots show copper deposits mentioned in this study. The map on the right shows the spatial relationships of the main copper deposits at Girilambone at finer detail. Tan ovals show the location of major open pit mines and adjoining low-grade stockpiles.
Detailed map of the Muriwombie pit, showing locations of malachite (green dots) and azurite (blue dots) samples presented in this study. The purple zones highlight the Northern and Eastern Shear Zones, while the pale blue zone shows the mine ore zone at 1.4% Cu cut-off from 1998. Key elevations are listed and brown lines show bench levels, not topographic relief. Blue spring symbols show location of major pit-water seeps, while green spring symbols show locations of active atacamite precipitation.
The Girilambone copper deposit was discovered initially by Thomas Hartman in 1875, and later pegged as 40 acres of mining claims in 1879 by Hartman, Charles Campbell, George Gibb, and George Hunter (McQueen, Reference McQueen2018). Hartman, Campbell and Gibb had previously discovered copper deposits in the Cobar district (Carne, Reference Carne1908). Mining at the main Girilambone deposit commenced in 1880, and takes its name from the locality which translates to ‘place of falling stars’ in the Wielwan Aboriginal language (McQueen, Reference McQueen2018). Initial operations by two separate companies were limited to shallow workings (<75 m) and yielded 42 tons of copper from 3100 tons of ore between 1880 and 1884 (Carne, Reference Carne1908). In 1896 the mine was re-opened by Girilambone Copper Mining Company Limited and in the next 11 years produced ~1,142 tons of copper (Chapman et al., Reference Chapman, Sharpe and Williams2005).
The deposits were largely idle until 1963–1973 when Utah Development Company explored Girilambone and delineated a 3.3 Mt resource averaging 2.12% Cu (Fogarty, Reference Fogarty, Cook, Ford, McDermott, Standish, Stegman and Stegman1996, Reference Fogarty, Birkman and Mackenzie1998). Similarly, Australian Selection Party Limited identified a 1.5 Mt resource averaging 1.8% Cu between 1974 and 1983 at Girilambone North (Fogarty, Reference Fogarty, Cook, Ford, McDermott, Standish, Stegman and Stegman1996, Reference Fogarty, Birkman and Mackenzie1998). In 1989 Nord Pacific Limited purchased the Girilambone deposits and identified 8 Mt of leachable copper reserves averaging 1.4% Cu, and in 1991 began mining operations as a joint venture with Straits Resources. The Murrawombie pit was started in 1992, and followed by exploitation of Girilambone North with the Northeast, Hartmans and Larsens East pits. Extraction of leachable copper between 1993 and 2002 was from a heap leach solution-extraction/electrowinning operation that yielded 115,063 tons of copper, though additional production from primary ore continued at the mill plant at the Tritton Mine (Straits Resources, 2003). The extraction of ore from underground operations at the Northeast and Larsen underground mines continued through 2016, when Murrawombie underground operations were initiated by the successor of Straits Resources, Aeris Resources. Murrawombie underground has yielded at least 500,000 tons of ~2% Cu ore, and has an estimated resource of 5.1 Mt at ~1.5% Cu for 75,000 tons of copper metal (Aeris Resources, 2021).
Geological and mineralogical setting
The Girilambone deposits have been described in detail for geology (Fogarty, Reference Fogarty, Cook, Ford, McDermott, Standish, Stegman and Stegman1996, Reference Fogarty, Birkman and Mackenzie1998; Shields, Reference Shields, Cook, Ford, McDermott, Standish, Stegman and Stegman1996; Aeris Resources, 2021) and mineralogy (Crane et al., Reference Crane, Sharpe and Williams2001; Chapman et al., Reference Chapman, Sharpe and Williams2005). Economic mineralisation is restricted to the basal unit of the Girilambone Group, the Caro schist. The Ordovician Girilambone Group is a sequence of schist, phyllite, greywacke and quartzite. Caro schist includes sericite schist, chlorite schist, graphite schist and a ‘pink quartzite’ that is closely linked with the primary mineralisation of the deposit.
The simple geology of the deposit has been complicated by subsequent structural events, and metamorphism and secondary enrichment/remobilisation. Two main periods of deformation include a folding of the pink quartzite into a broad and steeply plunging syncline which flattens with depth to the southeast. Subsequent brittle deformation produced the ‘Eastern Shear’ which is a steeply dipping normal fault. This fault is a zone of quartzite lenses within a matrix of hematite + chlorite schist and hosts significant secondary mineralisation and most of the original underground workings of the late 1800s to early 1900s (Shields, Reference Shields, Cook, Ford, McDermott, Standish, Stegman and Stegman1996).
The mineralogy of the deposit has been described in detail by Chapman et al. (Reference Chapman, Sharpe and Williams2005). Primary sulfide mineralisation includes layered, banded and massive pyrite and chalcopyrite within the pink quartzite, and disseminated pyrite and chalcopyrite within the lower pink quartzite and in the footwall schist. Some of the sulfide zones are reported as lenses up to 250 m by 45 m and open with depth (Fogarty, Reference Fogarty, Birkman and Mackenzie1998). Minor lead, zinc, silver and gold are associated with the sulfide zones (Chapman et al., Reference Chapman, Sharpe and Williams2005).
This primary sulfide mineralogy has been deeply weathered to produce a ‘classical copper oxidation zone’ (e.g. Williams, Reference Williams1990). At the surface, the pink quartzite weathered to produce a siliceous gossan that was more resistant to erosion than the surrounding units. This zone has voids, surrounded by massive iron and manganese oxide minerals. These voids are host to well-crystalised secondary minerals, especially those of copper. An assemblage of copper phosphate minerals overprint this zone, with an unusual profile of decreasing libethenite and increasing pseudomalachite with depth, probably resulting from the intensity of weathering of phosphate-bearing gangue minerals (Crane et al., Reference Crane, Sharpe and Williams2001). The oxidation zone is intensely leached in the upper 30 m, and extends to the water table at ~90 m depth. A supergene enrichment blanket consisting chiefly of earthy and sooty chalcocite extends below the modern water table.
The pronounced zonation relative to the occurrence of specific secondary copper minerals is germane to the present study. This zonation was first documented by Shields (Reference Shields, Cook, Ford, McDermott, Standish, Stegman and Stegman1996), who encouraged the author to study the origins of this zonation in the Murrawombie, Larsens and Northeast pits during fieldwork in 1997–1998. Malachite dominates the upper oxidation zone by Bench 5 (Reference Level 216 m), and is the most abundant secondary copper mineral in the deposit (Chapman et al., Reference Chapman, Sharpe and Williams2005). Malachite and pseudomorphs of malachite after azurite occur sporadically below this, where azurite begins to dominate. Azurite increases in abundance with depth, until it becomes the major ore mineral by Bench 21 (Reference Level 168 m). Azurite was not observed below Bench 35 (Reference Level 126 m). Native copper first appears in abundance below Bench 22 (Reference Level 165 m) and persists to about Bench 40 (Reference Level 111 m).
The regional weathering history is important in understanding the potential weathering history of the Girilambone deposit. Age determination of weathering profiles in the region includes palaeomagnetic dating of hematite fixation and Ar/Ar radiometric dating of manganese oxides (table 2 in McQueen et al., Reference McQueen, Chan, Khider K Greene and Scott2008; Smith et al., Reference Smith, Pillans and McQueen2009). These studies indicate a prolonged period of weathering from at least the Palaeocene and possibly the latest Cretaceous. This period experienced at least two major periods of deep chemical weathering under wet conditions followed by drying of profiles, with intense oxidative deposition and fixation of hematite. Evidence for these periods of weathering are preserved at a number of the ore deposits in the region, including at the McKinnons, New Cobar, Elura (Endeavor) and Mt Boppy deposits (McQueen et al., Reference McQueen, Chan, Khider K Greene and Scott2008).
Context of study
In May 1997 the author was fortunate to join Peter Williams, Jim Sharpe and Bernie Day on an expedition to examine copper deposits in Central Queensland. Over the next month we visited many deposits and planned future work at Cobar and Girilambone. However, Peter Williams was unable to join me for a visit to Girilambone in June or for a visit the next year when I returned for two more weeks of field work. Girilambone remains the only Australian copper deposit of significance that I have not visited with Peter. The 1997–1998 field seasons were generously supported by mine geologist Phil Shields and Straits Resources. Phil was very interested in the zonation of different secondary copper species within the deposit, and suggested stable isotope analyses to examine the conditions of formation. While field work was underway, significant deposits of well-crystalised copper mineralisation were encountered in all three active pits at Girilambone. On return to Sydney after this field work, Peter offered to store my samples and field gear in his garage until I returned for the 1999 field season. There the samples remained for years, until Peter was instructed to clean the garage, and shipped the samples to the author in 2003. The samples remained in the original shipping boxes until finally analysed in 2018.
Materials and methods
The sample suite for this study includes 24 carbonate mineral separates collected from high-grade surface benches (1997–1998) to obtain a representative suite of the principal copper carbonate minerals in cross-section throughout the depth of the pits as they were exposed in 1997–1998 (sample locations and elevation data Table 1; Figs 2 and 3). Raw samples had a mass of 10 to 250 grams each. To avoid analysis of impurities, samples were hand-picked from crushed and washed fractions. Only pure separates of each mineral phase were analysed.
Detailed map of the North East pit, showing locations of malachite (green dots) and azurite (blue dots) samples presented in this study. Key elevations are listed and brown lines show bench levels, not topographic relief. Blue spring symbols show location of major pit-water seeps.
Splits of these samples were mounted on epoxy resin to produce polished sections for microscopic observations and geochemical measurements. The surface of each polished section was examined by optical microscope (Zeiss AxioImager M2m) to obtain images for navigation under the Scanning Electron Microscope (SEM) with correlative microscopy. Mineral stoichiometry anticipated from optical observations was measured using a Zeiss (Sigma 200) field emission gun SEM equipped with two Bruker xFlash X-ray energy dispersive spectrometers (EDS) at Washington University in St. Louis, Missouri, USA. The SEM-EDS analyses used a probe current of 2.3 nA with an accelerating voltage of 20 kV at a working distance of 8.5 mm. Manual spot analysis was performed to confirm mineralogy.
Carbon and oxygen isotope analyses were performed at California State University Long Beach on hand-picked copper carbonate minerals. Analytical precision (1σ) was calculated on the basis of multiple measurements of well-characterised carbonate standards between sample runs and was better than 0.05‰ for δ13C and 0.04‰ for δ18O, after corrections for scale compression. Isotopic data are reported here relative to the Vienna Standard Mean Ocean Water (V-SMOW) for oxygen and to Vienna PeeDee Belemnite (V-PDB) for carbon (Coplen, Reference Coplen1995). Oxygen isotope data have been converted to temperature estimates using the isotope thermometer of Melchiorre et al. (Reference Melchiorre, Criss and Rose1999) for malachite and Melchiorre et al. (Reference Melchiorre, Criss and Rose2000) for azurite. Similar work has been long established for thermometry of carbonate minerals (e.g. Bowen, Reference Bowen1966). For these calculations, groundwater that the carbonates formed from was assumed to have an oxygen isotope value of –4.5‰, on the basis of both modern groundwater values from pit seeps (Table 2) and fluid-inclusion extrapolations, consistent with values reported in Melchiorre et al. (Reference Melchiorre, Criss and Rose2000). Thermometer reproducibility was checked by replicate analysis of laboratory standards and was better than ± 0.08‰ (1σ) for oxygen isotope analyses.
Pit water samples were collected from surface seeps in the mine. Electrical conductivity (EC), pH, Eh and water temperature were measured in situ with portable meters. Water samples were filtered with 0.5/μ filters and divided into two 250 ml glass bottles with Teflon closures. The bottle for cation analyses was acidified with 1 ml concentrated HNO3 and the bottle for anion analyses was not acidified. Sample bottles were new triple-rinsed cleanroom-grade containers. Nitric acid was added using disposable polyethylene pipettes. Cation and anion concentrations were determined by standard inductively coupled plasma optical emission spectrometry methods at the Australian Bureau of Rural Science under contract to Strats Resources. Reproducibility is better than ±5% for all elements. Stable isotope analyses for waters were prepared using the CO2 equilibration method for oxygen (Epstein and Mayeda, Reference Epstein and Mayeda1953) and the zinc reduction method (Coleman et al., Reference Coleman, Shepherd, Durham, Rouse and Moore1982). Results are reported in the usual δ notation relative to the V-SMOW standard. Precision is 0.1‰ for oxygen and 1‰ for hydrogen. Analyses were performed on a Delta Plus Advantage stable isotope ratio mass spectrometer at California State University San Bernardino, USA.
In addition to the above samples, a sample of atacamite-group minerals was collected from where there was active precipitation from pit seep waters from the face of Bench 37 (114 m). This sample was collected from dry crusts and preserved in a borosilicate glass bottle with a Teflon seal closure. Mineral stoichiometry was measured using SEM-EDS at Washington University in St. Louis, Missouri, USA, as detailed for the rock samples above. Manual spot analysis was performed to confirm suspected mineralogy. Crystal system observations were inconclusive for specific identification, and detailed crystallographic work was not performed to distinguish between atacamite and clinoatacamite. Preparation for isotope analysis follows the methodology outlined in Eggenkamp et al. (Reference Eggenkamp, Middelburg and Kreulen1994). Chlorine stable-isotope analyses were performed by reacting 10 mg of the atacamite with 10 ml of 50% nitric acid for 24 hours. The resulting solution contained dissolved atacamite with no detectable non-soluble residues. This fluid was diluted with 100 ml cleanroom-grade deionised water. An aliquot of sample was reacted with AgNO3 to produce AgCl. The AgCl product was removed by filter and dried before reacting with excess CH3I under vacuum at 80°C to produce CH3Cl. Surplus CH3I was removed from the CH3Cl using a gas chromatograph column prior to analysis on a Thermo-Scientific Model252 stable isotope ratio mass spectrometer set up as a continuous-flow isotope ratio spectrometer at the University of California Riverside Facility for Isotope Ratio Mass Spectrometry (FIRMS). Measurement on sample unknowns were corrected to three standards obtained from University of Texas at Austin, and are reported in delta notation as δ37Cl relative to Standard Mean Ocean Chloride (SMOC). Reproducibility, on the basis of replicate analyses and standards is estimated at 1σ of ±0.5‰.
Results
Carbon stable-isotope values for malachite from the Girilambone main pit range from –15.2 to –10.4‰, whereas azurite values range from –10.2 to –9.3‰ (Table 1; Figs 2 and 3). Oxygen stable-isotope values for malachite from the Girilambone main pit range from 23.6 to 29.4‰, whereas azurite values range from 29.4 to 30.6‰ (Table 1). Oxygen isotope thermometry estimates using the isotope thermometer of Melchiorre et al. (Reference Melchiorre, Criss and Rose1999) for malachite and Melchiorre et al. (Reference Melchiorre, Criss and Rose2000) for azurite yield temperatures ranging from 21 to 52°C (malachite) and 26 to 32°C (azurite). Samples from the North East pit yielded results within these same ranges.
The four pit seep-water samples have elevated (above drinking water standards) electrical conductivity (EC) with a near neutral pH (Table 2; Figs 2 and 3). Regional EC and pH values range from 7200 to 3160 μS/cm and pH 6.4–7.1 (Khider and McPhail, Reference Khider and McPhail2005) while pit seep waters range from 30,000 to 19,500 and 7.0 to 7.7, respectively. These waters are dominated by sodium and chloride, with elevated magnesium and sulfate. Pit water sample 3, a site of active atacamite precipitation, has the most elevated chloride and copper levels. Stable isotope analyses of the waters indicate δ18O (V-SMOW) averages of –4.5‰ and δD averages –35.9‰ (Table 2). These values plot below the meteoric water line in the field of evaporative concentration. Chlorine isotope results for the atacamite sample collected from pit seep 3 (1 sample, analysed in triplicate) were δ37Cl (SMOC) of +0.15‰, +0.35‰ and +0.25‰, with an average of +0.25‰.
Discussion
Mineral zonation
While individual copper mineral species are known to occur as traces at all depths in the oxide zone, distinct zonation of these species is observed with depth at the Girilambone deposits (e.g. Chapman et al., Reference Chapman, Sharpe and Williams2005; this study). Malachite was observed to dominate nearer the surface, but decreases in abundance as the water table was approached. The pre-mining water table is reported at being “encountered at 325 foot depth” (99 m) from the surface (McQueen, Reference McQueen2018). Fieldwork in 1997 and 1998 shows that azurite gradually becomes one of the main copper ore minerals by Bench 18 (177 m) and remains so until about Bench 30 (141 m). At these latter depths cuprite and native copper increase in abundance until the chalcocite enrichment blanket is encountered near the water table. This generalised mineralogical sequence with depth is illustrated in Fig. 4. Localised variations to this sequence occur where fractures and perched water table lenses create pit seeps above the regional water table. In some locations, overprinting of copper mineral species suggests a more complex localised oxidation zone history produced by fluctuations in water table levels.
Photograph of a characteristic pit cross section through the Girilambone main deposit exposed by the Muriwombie pit. Scale bar of 3 m is approximate due to photography angle distortion across the image.
Oxygen isotope thermometry
The results of oxygen isotope analyses may be interpreted as temperatures of mineral formation. The thermometry estimates for azurite suggest temperatures of formation between 26 and 32°C (Table 1; Fig. 5), with temperatures generally increasing with depth. Malachite thermometry estimates present a more complex picture. Malachite formation temperatures show a similar trend of increasing with depth. However, the pseudomorph of malachite after azurite yielded a temperature estimate below this trend (21°C) while malachite growths on massive sulfide samples had temperatures of apparent formation much higher (49–52°C). When these special case samples are removed temporarily from the dataset, the remaining ‘main trend’ malachite samples range from 32 to 36°C (Fig. 5). The results of all malachite thermometry estimates suggest at least three generations of malachite formation: (1) higher temperature (~50°C) due to exothermic decomposition of sulfides. One of these samples came from shallow 1800s mine workings in the upper oxidation zone, while the other two came from deep in the active pit operations and have malachite that clearly formed post-mining. (2) Moderate temperatures (~33°C) for most ‘main trend’ malachite. (3) Lower temperature (~21°C) as late-stage retrograde mineralisation. Significantly, the trends of increasing temperatures of malachite and azurite formation with depth converge at the depth at which the regional water table was encountered (~100 m below the pre-mining surface). This divergence in apparent formation temperatures for these two minerals at the same depths suggests that malachite and azurite may not have formed contemporaneously, but rather at different times during oxidation.
Oxygen isotope thermometry estimates for copper carbonate samples shown vs. depth in the deposit as metres elevation above reference. Trend lines exclude pseudomorphs and carbonate on sulfide.
Carbon isotope values and carbon sourcing
Carbon isotope fractionation for malachite and azurite is known to be insensitive to temperature variation, making it an ideal tracer for identification of carbon sources (Melchiorre et al., Reference Melchiorre, Criss and Rose1999, Reference Melchiorre, Criss and Rose2000). Carbon isotope tracing has identified probable carbon sources such as metal-metabolising chemolithophile bacteria at Morenci, Arizona, USA (Melchiorre and Enders, Reference Melchiorre and Enders2003) and Great Australia, Queensland, Australia (Melchiorre and Williams, Reference Melchiorre and Williams2001) while other deposits suggest deep formation fluids (Melchiorre et al., Reference Melchiorre, McLaughlin, Bottrill and Hight2017) and dissolution of local carbonate rocks (some samples reported in Melchiorre and Enders, Reference Melchiorre and Enders2003).
Copper carbonate samples from the Girilambone deposits have carbon isotope values similar to many deposits where chemolithophile bacteria are known to play an important role in the breakdown of sulfide minerals within the oxidation zone. In fact, the Girilambone values for both azurite and malachite show a similar ‘main trend’ to the malachite reported in Melchiorre and Enders (Reference Melchiorre and Enders2003) with slightly lighter values at higher elevations within the oxidation zone (Fig. 6). This is consistent with mixing between an isotopically light bacterial carbon source and atmospheric carbon.
Carbon isotope values for copper carbonate samples shown vs. depth in the deposit as metres elevation above reference. The bag-plot encloses the trend of lower carbon isotope values near the surface. This trend encloses one of the sulfide-hosted samples that was obtained from old mine workings on the surface, while the two sulfide-hosted samples outside of this trend were from a deep portion of the deposit that presumably were exposed and oxidised much more recently.
The exceptions to this general behaviour are the malachite observed as pseudomorphs after azurite, and malachite growing on the sulfide samples. The δ13C value of the malachite pseudomorph after azurite is the heaviest of all at –6.6‰, while the malachite growths on massive sulfide were the lightest of all with an average of –14.9‰. These variations are several permil (‰) different from the ‘main trend’ of values (Fig. 6).
These values for malachite that deviate from the main trend still convey formation conditions consistent with field observations of the conditions of formation. The malachite pseudomorph sample has a δ13C value which is consistent with pre-industrial atmospheric values of –6.5 to –7.0‰ (Saurer et al., Reference Saurer, Borella, Schweingruber and Siegwolf1997; Grocke, Reference Grocke2002; McCarroll and Loader, Reference McCarroll and Loader2004; Leuenberger, Reference Leuenberger2007). It is known from textural relationships that the malachite pseudomorph sample formed late in the paragenetic sequence when most primary sulfides above the water table would have already been digested by a combination of metal-metabolising chemolithophile bacteria and inorganic chemical reactions. Carbon isotope values of pore gasses at this time would be more likely to reflect atmospheric or soil carbonate values.
For the malachite growths on sulfide minerals, the δ13C values are much lighter with an average of –14.9‰. These values are consistent with a probable carbon source of metal-metabolising chemolithophile bacteria broadly characterised as ‘Thiobacillus ferrooxidans’ as documented at Morenci, Arizona, USA (Melchiorre and Enders, Reference Melchiorre and Enders2003) and Great Australia, Queensland, Australia (Melchiorre and Williams, Reference Melchiorre and Williams2001). The observed rapid rate of decomposition of these sulfides and their exothermic behaviour are also consistent with bacterial decomposition of sulfides.
Chlorine isotope implications
The formation of atacamite-group minerals (referred to here as ‘atacamite’) from groundwater flowing from pit seeps along the northern side of the Murrawombie pit presents yet another opportunity to examine conditions of secondary mineral formation in the deposit. Significantly, older atacamite was only documented from a single sample at Girilambone, and that sample was from a stockpile and thus has no context for its original position in the oxidation zone (Chapman et al., Reference Chapman, Sharpe and Williams2005). This nearly complete absence of atacamite and other chloride minerals (including pseudomorphs that might indicate their past presence) at Girilambone is interpreted to reflect the low relative chloride activities during formation of the oxide zone (Williams, Reference Williams1990). The formation of atacamite in the active mining environment suggests a change in groundwater or pore fluid chemistry since the development of the oxidation zone.
The δ37Cl (SMOC) value of modern-forming atacamite at Girilambone (+0.25‰) is an exact match for the value reported for pyromorphite from Broken Hill, Australia and a close match for many evaporite and some oxidation zone minerals (Eggenkamp and Schuiling,Reference Eggenkamp and Schuiling1995). Significantly, Eggenkamp and Schuiling (Reference Eggenkamp and Schuiling1995) concluded that high values of δ37Cl up to +6‰ for atacamite, boleite and connellite were the result of formation early in the development of the oxidation zone when sulfide decomposition produced low pH. These low pH conditions liberated chlorine gas with attendant fractionation to elevate pore water δ37Cl values. The near-zero chlorine isotope values were interpreted by Eggenkamp and Schuiling (Reference Eggenkamp and Schuiling1995) to result from a seawater chloride source, and/or formation late in formation of the oxidation zone when pH values have risen as sulfide oxidation nears completion. The δ37Cl value for Girilambone atacamite is also consistent with values reported for the groundwater of the Great Artesian Basin of Australia (Zhang et al., Reference Zhang, Frape, Love, Herczeg, Lehmann, Beyerle and Purtschert2007), which concluded that chloride was sourced from marine aerosols and not the dissolution of sedimentary salt. This would potentially explain the non-seawater major-ion ratios of seep water (Table 2), though diagenetic processes could also explain the water chemistry differences. The Girilambone atacamite value is also consistent with atacamite from Chile at depths of ~50 m within the oxidation zone where deep sedimentary basin brine and freshwater mixing is suspected (Reich et al., Reference Reich, Palacios, Parada, Fehn, Cameron, Leybourne and Zúñiga2008; Reference Reich, Barnes, Breecker, Barra, Milojevic and Drew2019).
Girilambone oxide deposit genesis
Though there is evidence that some of the development of the oxidation zone at Girilambone occurred in stages coincident with minor water-table fluctuations and erosion, the dominant stage of oxidation appears to have been a single protracted event under relatively stable conditions. During this event, secondary chalcocite formed a main enrichment blanket at and near the present water-table elevation. At these same levels and above, cuprite and native copper dominate in a transition zone (Fig. 4).
Above the transition zone, basic copper carbonates are typically the main copper minerals. Isotopic evidence from malachite growing on copper sulfide samples from the eastern shear lode suggest elevated temperatures of formation (~50°C, from oxygen isotope values), probably due to exothermic decomposition of sulfides by chemolithotrophic bacteria (recorded as δ13C ≈ –14.9‰). Temperatures in this range are consistent with rapid oxidation, such as that observed when the chalcocite blanket was exposed at the Gunpowder mine in Queensland, Australia. During fieldwork at the Gunpowder mine, the author, Peter Williams, Jim Sharpe and Vera Munro-Smith could barely walk across the ~50°C ground which rapidly heated boot soles to unbearable levels. At Girilambone, these malachite-on-sulfide samples have grown in a post-mining environment and are interpreted as representing a potential end-member environment for the oxidation zone forming directly at the interface with decomposing masses of sulfide minerals.
The main stage of malachite formation records much lower temperatures of 32 to 36°C (Table 1). These values are still well above ambient air temperatures, but below that recorded by malachite on sulfides. This suggests malachite formation following peak sulfide decomposition and attendant heat dissipation, or formation at a greater distance from the exothermic sulfide decomposition. These same malachite samples show a trend of increasingly lighter δ13C values towards the pre-mining surface (Fig. 6). This may result from a light surficial carbon source, or preserve the upwards diffusive loss of CO2 from a deep source as an isotope gradient. It is suggested that the most plausible scenario is the exothermic decomposition of deep sulfides adjoining the water table to produce thermal and carbon isotope gradients.
Similar trends are observed for azurite samples. Azurite temperatures are slightly lower than for malachite (27 to 32°C) and may indicate formation later than most malachite, when thermal decomposition of sulfides was waning. This is consistent with paragenetic relations noted in hand samples of Girilambone copper carbonate ores. Weak trends of increasing temperature with increasing depth for all main-stage copper carbonates indicate a thermal source at the water table, consistent with formation of the enrichment blanket and dissolution of primary sulfides. Azurite also has slightly heavier carbon isotope values, but a similar profile with depth in comparison to malachite. Both azurite and malachite samples from the main stage have carbon isotope values similar to other localities where microbial carbon is believed to be a significant carbon source (e.g. Melchiorre and Williams, Reference Melchiorre and Williams2001; Melchiorre and Enders, Reference Melchiorre and Enders2003). The malachite pseudomorph after azurite, arguably the last mineral to form in the main paragenetic sequence examined in this study, has the lowest temperature of formation and the heaviest carbon isotope value. These values are similar to modern ambient air temperatures and pre-industrial atmospheric carbon values (Saurer et al., Reference Saurer, Borella, Schweingruber and Siegwolf1997; Grocke, Reference Grocke2002; McCarroll and Loader, Reference McCarroll and Loader2004; Leuenberger, Reference Leuenberger2007).
It is suggested that the sequence of copper carbonate mineral formation followed a general trend. Malachite formation was first, as temperatures within the deposit were still quite warm from decomposition of primary sulfides. As malachite and other minerals formed, they progressively sealed fracture networks which restricted the discharge of CO2 and other gases produced by decomposition of sulfides by chemolithotrophic bacteria, similar to that recorded by Melchiorre and Enders (Reference Melchiorre and Enders2003). Of special importance was the formation of white and red clays (notes in Table 1). Veins and zones of azurite generally occur following malachite and in close association with these clays, similar to observations of this association made by the author at copper deposits across the southwestern USA and some locations in Australia (full discussion on page 179 in Melchiorre et al., Reference Melchiorre, McLaughlin, Bottrill and Hight2017 and references therein). It has been known for many years that malachite will often form before azurite in copper deposits where both minerals occur (e.g. Schwartz, Reference Schwartz1934). This trend of malachite formation before azurite probably records the changing partial pressures of CO2, where rising CO2 levels pass through the stability field of malachite and into the stability field of azurite (see figure 14 in Melchiorre et al., Reference Melchiorre, McLaughlin, Bottrill and Hight2017).
The typical partial pressure of CO2 in the atmosphere is ~10–3.5 atmospheres, which dictates that malachite will be the more stable carbonate (e.g. Williams, Reference Williams1990). An increase in CO2 pressure to 10–1.36 atmospheres or higher would result in the formation of azurite (e.g. Williams, Reference Williams1990; Kiseleva et al., Reference Kiseleva, Ogorodova, Melchakova, Bisengalieva and Becturganov1992). It is suggested that the generation of impermeable clay during weathering of the oxidation zone elevates p[CO2] levels by creating a comparatively closed system that can reach the high levels above atmospheric levels required for azurite formation. In some cases, the clay may be associated with a fault gouge (Melchiorre and Enders, Reference Melchiorre and Enders2003), while in others it may be associated with weathering of primary lithology (Melchiorre et al., Reference Melchiorre, McLaughlin, Bottrill and Hight2017). Regardless of origin, clay is clearly associated with azurite in the Girilambone deposits. It is suggested that these clays in the oxidation zone at Girilambone reduced the ability of CO2 generated by chemolithotrophic bacteria to escape upwards to the atmosphere. Initial development of the oxidation zone occurred in a system that was essentially open to the atmosphere and favoured formation of malachite. As secondary minerals, and especially clays, reduced permeability the partial pressures of CO2 rose into the stability field of azurite. However, this was not a closed system, and the leakage of CO2 produced isotopic fractionation by diffusion as lighter carbon was selectively lost towards the surface. The downward migration of fluids and the upward loss of CO2 became concentrated within specific sectors within the oxidation zone such as large fracture zones and permeable units. The result was formation of azurite higher in the oxidation zone than would be expected, within these structurally dictated pockets of elevated CO2. Similar ‘blow-out’ zones related to diagenetic compaction were noted in other deposits (Melchiorre et al., Reference Melchiorre, McLaughlin, Bottrill and Hight2017). Fluctuations in CO2 partial pressure probably occur when new pathways opened and old ones closed. However, the interbanding of azurite and malachite that would be produced by seasonal rains or frequent fluctuations (e.g. Melchiorre and Enders, Reference Melchiorre and Enders2003) are not commonly observed at Girilambone. It is also possible that erosion plays some role in the azurite formation at such apparently shallow depths in the oxidation zone. However the levels of erosion relative to the timing of deposit oxidation remain unquantified.
As sulfides were consumed by exothermic oxidation and bacterial digestion, generation of CO2 waned and temperatures decreased. It was on this ‘retrograde’ side of maximum deposit oxidation that pseudomorphs of malachite after azurite began to form at essentially atmospheric temperatures and with pre-industrial atmospheric carbon isotope values. Eventually, CO2 production decreased to a point that the pre-existing chemistry of the local groundwater once again dominated the system. It is in this latest period that atacamite precipitation occurs as chloride-rich groundwater interacts with copper-rich oxidation fluids. It is possible that the documentation of a single sample of atacamite at Girilambone (Chapman et al., Reference Chapman, Sharpe and Williams2005) records an early period of weak weathering before CO2 began to dominate the system. However, that lone sample was from a stockpile and thus has no context for its original position in the oxidation zone or attendant paragenetic relationships.
It bears mentioning that the single dominant phase of oxidation suggested by the evidence is of unknown duration. It may have persisted for long enough to give the appearance of separate events, as evidenced by overprints of early malachite with later azurite overgrowths, which in turn was altered in places back to malachite pseudomorphs. This protracted period of oxidation and attendant mineralogical zonation could be interpreted as either temporal or spatial zonation. However, the documentation of deep intense weathering and the isotopic gradients measured with depth in the deposit suggest this was a single event that records a protracted period of oxidation-zone weathering reactions, and not discrete unrelated events.
Future workers should consider examining the relationship between the regional weathering history and the events captured during oxidation of the deposit. Without data on ages for the different levels of the weathering profiles at Girilambone it is difficult to reconcile the genesis stages indicated by this study and those of the regional weathering history. However, regional weathering history suggests that most of the weathering preserved at Girilambone would predate the Mid Miocene (17 Ma). The predominantly arid to semi-arid conditions following this period would generate more limited chemical weathering, as indicated by the relatively unweathered Miocene leucitites, which sit on a deeply weathered profile at Wilga Tank 65 km west of Girilambone (McQueen et al., Reference McQueen, Gonzalez, Roach, Pillans, Dunlap and Smith2007).
Conclusions
The Girilambone deposit is a textbook example of a classic oxidation zone profile. Unlike the oxidation profiles of porphyry copper deposits of western North America which have been overprinted by water-table fluctuations produced by active tectonics, the Girilambone deposit appears to have little modification to the original oxidation profile.
Oxidation of primary sulfides at Girilambone was an exothermic process facilitated by chemolithotrophic bacteria. The bacteria generated CO2 which migrated upwards to react with copper rich meteoric fluids of the vadose zone to precipitate malachite. Over time, secondary minerals like clays, iron oxides and basic copper carbonates reduced permeability of the oxidation zone. Unlike porphyry copper deposits of western North America, this deposit did not experience significant tectonic activity during oxidation to re-establish permeability. Thus the reduced permeability slowed the release of CO2 from the system and produced significantly elevated partial pressure of CO2 that was sufficient for azurite formation to dominate the system. The bacteria populations at Girilambone also appear to have been stable over time and not seasonal, as the deposit has no interbanded azurite and malachite typical of episodic bacterial populations triggered by seasonal precipitation (e.g. Melchiorre and Enders, Reference Melchiorre and Enders2003). The absence of significant Cu-carbonate banding at Girilambone may therefore serve as a palaeoclimate indicator. Deeper in the Girilambone oxidation zone, native copper and cuprite dominate, whereas chalcocite formed an enrichment blanket just above and at the modern water table. Eventually, as CO2 production from bacterial digestion of sulfides waned, pseudomorphs of malachite after azurite were generated as a retrograde reaction. In the modern Girilambone operations, local chloride-rich groundwater emerges as pit weeps which precipitate atacamite, while exposed remnants of sulfide masses form a rind of porous malachite. Local channelisation of fluids and perched water-table lenses generated exceptions to this oxidation zone sequence and created mineralogical overprints.
The Girilambone deposit thus serves as an end-member model for the development of an oxidation zone in an environment virtually free of the effects of active tectonics and significant fluctuation in the local water table. It is suggested that the oxidation zone of other deposits may be interpreted for history of recently active tectonics, palaeoclimate, and water table stability by comparison to the Girilambone deposit.
Acknowledgments
This paper would not have been possible without the help of three talented mining professionals who realize the benefit of research to their industry. First, Phil Shields provided generous time and expertise towards understanding the geology of the deposit and the collection of samples. Tony Thomas and Mark Welch provided administrative support for this project and guest lodging for the author. Specific thanks go to Peter Williams for his two decades of friendship and intellectual support of research projects on copper deposits of Australia. Instrumentation used in this study was provided by generous grants from the National Science Foundation, the W.M. Keck Foundation, and an internal VETI Grant by CSUSB. Travel support was provided by National Science Foundation International Travel Program. Greg Holk at CSU Long Beach provided access to carbonate stable isotope instrumentation. Jim Sickman and Delores Lucero at University of California Riverside provided chlorine analysis instrumentation and expertise. Anonymous reviewer #3 provided a wealth of useful information regarding the regional weathering history.
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