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| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |

Instituto de Geociências, Universidade Estadual de Campinas, Caixa Postal 6152, 13.083-970, Campinas, SP, Brazil, and Centre for Global Metallogeny, School of Earth and Geographical Sciences, University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia
Instituto de Geociências, Universidade Estadual de Campinas, Caixa Postal 6152, 13.083-970, Campinas, SP, Brazil

Centre for Global Metallogeny, School of Earth and Geographical Sciences, University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia
Companhia Vale do Rio Doce, Caixa Postal 51, Serra dos Carajás, 68.516-000, Parauapebas, PA, Brazil
Corresponding author: e-mail, dgroves{at}segs.uwa.edu.au
| Abstract |
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SHRIMP II zircon dating of the host metavolcanic rocks gives a 207Pb/206Pb age of 2748 ± 34 Ma. This suggests a correlation between the Igarapé Bahia volcano-sedimentary sequence and the Grão Pará volcanic rocks, which have published ages of ca. 2.75 Ga. SHRIMP dating of monazite from the matrix of ore-bearing magnetite breccias gives a 207Pb/206Pb age of 2575 ± 12 Ma, confirming the epigenetic nature of the mineralization and placing it ~175 m.y. after accumulation of the host volcano-sedimentary sequence. The 2575 ± 12 Ma SHRIMP age of hydrothermal monazite from the Igarapé Bahia mineralization is indistinguishable from published conventional 207Pb/206Pb ages for zircons from the Archean A-type granites of the Carajás belt, indicating that mineralization processes at Igarapé Bahia were temporally related to these A-type Archean granites. The wide range of highly radiogenic 87Sr/86Sr ratios (0.7140.755) of carbonates from the Igarapé Bahia deposit suggests multiple crustal sources, consistent with a magmatic-hydrothermal origin. SHRIMP dating of zircon xenocrysts recovered from crosscutting diabase dikes indicates a maximum 207Pb/206Pb age of ~2670 Ma, consistent with field evidence and the age of host rocks, but does not unequivocably constrain the age of the ores.
The styles of hydrothermal alteration, mineralogy, and geochemistry of the Igarapé Bahia ore, as well as published fluid inclusion and stable isotope data, support its classification as a member of the world-class Olympic Dam-type Fe oxide Cu-Au-(U-REE) group of deposits, as previously argued by several authors. The SHRIMP age of 2575 ± 12 Ma for hydrothermal monazite indicates that Igarapé Bahia is an Archean example of this deposit group.
| Introduction |
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Previous genetic interpretations of the Igarapé Bahia deposit included syngenetic volcanic-hosted massive sulfide deposit (VHMS; Besshi-type) models (e.g., Ferreira Filho, 1985; Almada, 1998; Villas and Santos, 2001), epigenetic hydrothermal-magmatic models with ore related to Paleoproterozoic (ca. 1.88 Ga) granites (e.g., Lindenmayer et al., 1998), and multistage models that invoke an interplay of Archean and Proterozoic processes (e.g., Ribeiro, 1989; Mougeot et al., 1996). However, similarities with the Australian Olympic Dam deposit (Roberts and Hudson, 1983; Oreskes and Einaudi, 1990; Reeve et al., 1990) have encouraged several authors to propose an epigenetic hydrothermal model related to an alkaline magmatic component of unknown age (Oliveira et al., 1998; Tallarico et al., 1998; Soares et al., 1999; Tazava, 1999). Uncertainties in interpretation relate partly to poor exposure of fresh rocks but are mainly due to the absence of robust geochronologic data on the ore and host rocks.
The aim of this paper is to provide an overview of the geology and geochemistry of the Igarapé Bahia deposit and to constrain the age of the mineralization using SHRIMP geochronology. These data are used to test whether the deposit is contemporaneous with the Archean volcanic sequence or with alkaline granitoids of either Late Archean or Paleoproterozoic age.
| Regional Geology and Metallogeny |
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Basement rocks consist of gneiss and migmatite of the Xingu Complex and orthogranulites of the Pium Complex that were metamorphosed at ca. 2.8 Ga (Machado et al., 1991; Rodrigues et al., 1992; Pidgeon et al., 2000). According to Araújo et al. (1988), the Pium Complex represents slabs of infracrustal rocks uplifted through deep shear zones and could possibly represent the suture zone between the Rio Maria block and the Carajás belt. In the Carajás belt, the basement assemblage defines a broad, steeply dipping, east-westtrending ductile shear zone (Itacaiúnas shear zone), which experienced multiple episodes of reactivation during the Archean and Paleoproterozoic (Pinheiro and Holdsworth, 1997; Holdsworth and Pinheiro, 2000).
The Carajás region includes one of the best preserved Archean volcano-sedimentary successions in the world. These rocks, assembled under the Itacaiúnas Supergroup, record different metamorphic grades, ranging from virtually unmetamorphosed and undeformed, to lower greenschist facies (Grão Pará Group) in the innermost portions of the belt, and intensely sheared amphibolite and/or granulite facies (Salobo Group) at the northern edge of the Itacaiúnas shear zone (Docegeo, 1988; Olszewski et al., 1989). Volcanism occurred at ca. 2.75 Ga (e.g., Machado et al., 1991; Trendall et al., 1998). The Grão Pará Group is the dominant volcano-sedimentary sequence in the Carajás basin and includes low-grade metavolcanic rocks that host significant banded iron formation (BIF). These contain the giant iron deposits, such as Serra Norte, Serra Sul, Serra Leste, and Serra de São Felix, that contain total resources of 17.3 Bt at 66 percent Fe (Tolbert et al., 1971; Gibbs and Wirth, 1990).
Sandstone and siltstone deposited in a shallow marine to fluvial environment (Águas Claras Formation, Nogueira et al., 1994, 2000) overlie the volcanic rocks of the Grão Pará Group. A minimum age of 2645 ± 12 Ma for the Águas Claras Formation was determined by Dias et al. (1996) by conventional U-Pb analysis of zircons from crosscutting gabbro dikes. A SHRIMP U-Pb age of 2681 ± 5 Ma was determined by Trendall et al. (1998) from a sandstone sample containing zircons apparently derived from syndepositional volcanic rocks. Based on this age, Trendall et al. (1998) inferred that the Águas Claras Formation could represent the uppermost unit of a continuous accumulation in the Grão Pará basin that lasted less than 100 m.y.
The Carajás region has been intruded by granitic magmas of distinct ages and compositions. Paleoproterozoic intrusions (ca. 1.88 Ga; Machado et al., 1991) include several anorogenic granitic plutons, such as the Central Carajás and Cigano granitoids. The latter belong to the most extensive A-type Proterozoic province of the world (e.g., Santos et al., 2001) that covers thousands of square kilometers of the Amazon craton. Archean intrusions include granitoids and diorites of the Plaquê Suite (ca. 2.74 Ga; Huhn et al., 1999b) and younger alkaline granitoids (ca. 2.57 Ga), such as the Estrela Complex (Barros et al., 1992, 1997, 2001; Barros and Barbey, 1998), the Old Salobo Granite (2573 ± 2 Ma; Machado et al., 1991), and the Itacaiúnas Granite (Souza et al., 1996). The Estrela Complex is the best documented example of the Archean alkaline granitoids in the Carajás belt. According to Barros et al. (1997), it consists of an east-westtrending, heterogeneously sheared monzogranitic batholith that has a characteristic A-type geochemical signature defined by high K2O + Na2O, extremely high FeOtotal/FeOtotal + MgO ratios, and elevated Zr, Y, and Nb. Fabric analysis of the Estrela Complex indicates that magmatic activity was syntectonic and coincident with the closure of the Carajás basin (Barros and Barbey, 1998; Barros et al., 2001).
A striking feature of the Carajás region is the clustering of a variety of different types of Cu-Au deposits. The most abundant in the belt are Fe oxide Cu-Au-(U-REE) deposits that are hosted by a variety of rocks and have different orebody morphologies, although most are near-vertical (>75°) breccia bodies. The most significant examples of this deposit type are Salobo, with resources of 994 Mt at 0.94 percent Cu and 0.52 g/t Au (Farias and Saueressig, 1982; Vieira et al., 1988; Lindenmayer, 1990), Igarapé Bahia, with resources of 219 Mt at 1.4 percent Cu and 0.86 g/t Au (Ferreira Filho, 1985; Almada, 1998; Tazava, 1999; Tallarico et al., 2000), Sossego, with resources of 355 Mt at 1.1 percent Cu and 0.28 g/t Au (Cordeiro, 1999; Lancaster et al., 2000), Cristalino, with resources of 500 Mt at 1.0 percent Cu and 0.3 g/t Au (Huhn et al., 1999a), and Cento e Dezoito with resources of 170 Mt at 1.0 percent Cu and 0.3 g/t Au (Rigon et al., 2000).
A second style of Cu-Au deposit, characterized by a Cu-Au-(W-Bi-Sn) association, includes a number of small- to medium-sized deposits that appear to be genetically related to Proterozoic A-type magmatism. Representative examples are the Águas Claras Cu-Au-(W-Sn) deposit, with resources of 9.5 Mt of oxidized ore at 2.43 g/t Au (Soares et al., 1994; Silva and Villas, 1998) and the Breves Cu-Au-(W-Bi-Sn) deposit, with resources of 50 Mt of primary ore at 1.22 percent Cu, 0.75 g/t Au, 2.4 g/t Ag, 1,200 g/t W, 70 g/t Sn, 175 g/t Mo, and 75 g/t Bi (Tallarico et al., 2004).
A major question to be resolved in the Carajás copper-gold belt is the relationship between the relatively small (<50 Mt) Paleoproterozoic (ca. 1.88 Ga) Cu-Au-(W-Bi-Sn) deposits (Tallarico et al., 2004) and the much larger (>200 Mt) Fe oxide Cu-Au-(U-REE) deposits. One possibility is that they are both related to the ca. 1.88 Ga A-type granites, but a number of important differences between the deposits make this unlikely. In particular, the Fe oxide Cu-Au-(U-REE) deposits are characterized by (1) intense Fe metasomatism leading to the formation of fayalite (e.g., Salobo; Lindenmayer, 1990), grunerite, and/or Fe oxides (magnetite and/or hematite); (2) extensive carbonate alteration (mainly siderite), at least in the lower temperature deposits; (3) S-deficient nature of the ore sulfides (chalcopyrite, bornite, and primary chalcocite); (4) quartz-deficient nature of the gangue, (5) extreme low REE enrichment (approximately 104 x chondritic values), and (6) enrichment in U and Co. Given the common alkaline association of Fe oxide Cu-Au-(U-REE) deposits elsewhere in the world (e.g., Hitzman et al., 1992; Oreskes and Hitzman, 1993; Campbell et al., 1998; Groves and Vielreicher, 2001), it is possible that these deposits of the Carajás belt are related to more alkaline rocks than the 1.88 Ga A-type (e.g., Kerrich et al., 2000) granites, including the ca. 2.57 Ga alkaline complexes of the Carajás belt (e.g., Estrela Complex, Old Salobo Granite). In this case, the deposits of the Carajás belt would represent one of the oldest known members of the iron-oxide Cu-Au-(U-REE) group worldwide. A genetic link between copper-gold mineralization and Archean magmatism has been established recently for the Salobo iron-oxide copper-gold deposit. Requia et al. (2003) determined Re-Os ages from molybdenite and a Pb-Pb age from bornite-chalcopyrite-magnetite of 2576 ± 8 Ma, which overlaps the previously published age of 2573 ± 2 Ma for the Old Salobo Granite (Machado et al., 1991). These data confirm that main-stage mineralization at Salobo was contemporaneous with Archean granitoid magmatism of alkaline affinity in the region (Requia et al., 2003).
| Geology of the Igarapé Bahia Fe Oxide Cu-Au-(U-REE) Deposit |
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Supergene alteration and ore types
At Igarapé Bahia, weathering was responsible for the development of a 200-m-thick supergene profile (Zang and Fyfe, 1993; Angélica, 1996) in which gold and copper were dissolved, separated, and reprecipitated in different ore types. The upper part of the profile includes a gold-bearing gossan that extends to a depth of approximately 150 m. The gossan is composed mainly of goethite, hematite, gibbsite, and kaolinite and has traces of secondary copper minerals and REE-rich phosphates (florencite, crandalite, and rhabdophane). From 150 to 200 m, there is a transitional zone where supergene copper was precipitated. This copper-gold ore is composed of goethite and hematite, together with abundant secondary copper minerals, including native copper, chalcocite, digenite, cuprite, malachite, azurite, and pseudomalachite.
The primary copper-gold mineralization occurs below 200 m and consists mainly of Fe chlorite, siderite, and magnetite-rich breccias.
Hypogene hydrothermal alteration and breccia types
The ore-bearing breccias of Igarapé Bahia are essentially polymictic. They are classified according to matrix mineralogy as Fe chlorite breccias, siderite breccias, and magnetite breccias. The rock fragments have angular to subrounded shapes and diameters that range from a few millimeters up to 20 cm. The fragment to matrix ratio is highly variable, possibly reflecting different fluid/rock ratios or different mechanical processes accompanying brecciation.
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Iron chlorite breccias and siderite breccias possess virtually the same matrix mineralogy, which is typically fine grained and includes Fe chlorite, siderite, magnetite, chalcopyrite, and minor tourmaline. Siderite breccias contain a much higher percentage of siderite, clearly distinguishing them from the iron chlorite breccias (dominated by Fe chlorite) in thin section.
At the Acampamento Sul and Furo Trinta orebodies, mineralization is hosted preferentially by siderite breccias, whereas at the Acampamento Norte and Alemão orebodies, mineralization is associated with magnetite breccias. Mineralized iron chlorite breccias occur at the margins of all orebodies (Fig. 4).
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Scanning electron microscopy (SEM) investigation of the breccias has revealed the presence of trace amounts of molybdenite, galena, cobaltite, hessite, altaite, cassiterite, ferberite, scheelite, uraninite, parisite, bastnäsite, allanite, monazite, apatite, and fluorite. The breccia matrix also is reported to include chloride-rich minerals such as ferropyrosmalite (Tazava, 1999) and scapolite (Althoff et al., 1994).
Several vein types crosscut the mineralized breccias and the host metavolcanic sequence. Veins are discordant to bedding and rarely display comb structures. The most common types are calcite + chalcopyrite ± fluorite ± stilpnomelane veins, ankerite ± chalcopyrite ± gold veins, siderite ± calcite ± chlorite ± chalcopyrite veins, and chalcopyrite ± biotite ± K-feldspar ± tourmaline ± REE mineral veins. The chronology of the veins is unclear due to poor exposure and equivocal relationships in drill core.
Primary copper-gold mineralization
Primary copper mineralization at Igarapé Bahia comprises xenomorphic and poikiloblastic chalcopyrite in the matrix of breccias. Rarely, chalcopyrite is rimmed by chalcocite, digenite, and covellite due to oxidation reactions along grain boundaries. In magnetite breccias, unlike siderite and Fe chlorite breccias, the chalcopyrite is intergrown with bornite. Rare pyrite occurs as inclusions in chalcopyrite in the more sulphur rich assemblages.
The major copper-rich ores contain gold in all breccia bodies. Additional subeconomic copper is disseminated or occurs in veins or nodules in distal, altered host rocks with negligible gold content.
Chalcopyrite nodules occur in the laminated upper unit of sedimentary rocks (Fig. 3A), where the primary bedding is deformed around the nodules. The nodules are mineralogically zoned, with rims enriched in inclusions of euhedral Fe chlorite in association with minor albite and quartz and cores consisting of massive chalcopyrite, with inclusions of K-feldspar, cobaltite, thorite, monazite, and apatite. The chalcopyrite nodules are interpreted to be epigenetic because they are linked to veins with the same mineralogy and zoning pattern, which are both discordant and concordant to the sedimentary bedding (Fig. 3A-B). Rarely, these sedimentary rocks also have strata-bound replacement textures with infilling of the more porous and permeable layers of the laminated rocks with chalcopyrite.
Native gold occurs in the matrix of the breccias as fine-grained (520-µm) inclusions in gangue minerals (quartz, siderite, and chlorite), chalcopyrite, and rarely magnetite. The gold grains contain up to 12 wt percent Ag, but the bulk Ag grades of the ore are subeconomic. Gold may also contain inclusions of tellurides (hessite, Ag2Te) and sulfides (argentite and/or acanthite, Ag2S).
| Geochemistry |
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Iron chlorite, siderite, and magnetite breccias have similar REE patterns (Fig. 5) characterized by strong low REE enrichment (~104 chondritic values). Although the absolute concentrations of REE vary the patterns for altered metavolcanic rocks, quartz diorite dikes, and mineralized breccias show similar low REE enrichment. The REE pattern of BIF differs significantly from that of the ore-bearing breccias, arguing against a syngenetic sea-floor volcanic origin for the Igarapé Bahia mineralization, as previously suggested by Villas and Santos (2001). The contrasting La/Lu ratios of the host metavolcanic rocks (70250) and the ore-bearing breccias (1,0002,500) indicate that low REE were selectively concentrated during hydrothermal alteration and mineralization. The positive correlation between La, Ce, P, Cu, and Au (Fig. 6) supports the suggestion that the low REE minerals (e.g., monazite) are part of the ore paragenesis and, therefore, are suitable for dating mineralization.
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| Sampling and Analytical Procedures for SHRIMP Analysis |
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The host metavolcanic rock samples from the lower unit display an isotropic fabric defined by abundant fine-grained chlorite associated with minor albite and quartz. The primary mineralogy has been obliterated by intense chlorite alteration. The abundance of chlorite and the limited amount of quartz indicate a mafic composition, which is confirmed by previous geochemical investigations of the Igarapé Bahia metavolcanic rocks (e.g., Ferreira Filho, 1985).
The diabase dikes crop out as extremely weathered saprolite. Fresh samples are only obtained by drilling some 200 m below the surface. Field relationships indicate that the dikes crosscut both the host volcanic rocks and the ore (mineralized breccias). The samples collected for geochronology show no evidence of hydrothermal alteration or overprinting, display an ophitic texture, and are characterized by abundant plagioclase and clinopyroxene with accessory magnetite.
Magnetite-rich breccias crop out as extremely altered gossans. Fresh material was only reached through drilling below a 200-m-vertical depth. The breccia samples may include fragments of host metavolcanic rock and BIF that occur in the matrix of euhedral magnetite with minor chlorite, siderite, fluorite, grunerite, biotite, microcline, and sericite. Copper sulfides (mostly chalcopyrite with lesser bornite) are paragenetically late and surround other phases in the matrix. Gold is present as inclusions within copper sulfides.
The separation of zircons was carried out at the Universidade Federal de Ouro Preto, Brazil, with final handpicking at the University of Western Australia. The samples were crushed, and a <60-mesh fraction was collected and cleaned. The final selection of zircons was handpicked and mounted in epoxy resin disks together with chips of the 564 Ma CZ3 zircon standard (Pidgeon et al., 1994; Nelson, 1997). The disks were polished to expose the zircon grains in section. After detailed photography and SEM imaging, the disks were cleaned and coated with high-purity gold.
Uranium-Th-Pb isotope analyses of sectioned single zircons were carried out on the sensitive high-resolution ion microprobe (SHRIMP II) at the Curtin University of Technology, following the procedures documented by Compston et al. (1986), Williams and Claesson (1987), and Smith et al. (1998). Data were processed using the software package SQUID 1.00 (Ludwig, 2001a).
Monazite analyses were performed in situ on fragments of samples that were split or drilled from polished thin sections and mounted in epoxy disks. The monazite Pb/U standard VK1 (488 Ma) was cast in a separate mount. Analytical and data reduction methods for monazite are described by Foster et al. (2000) and Rasmussen et al. (2001).
The uncertainties in the radiogenic Pb isotope ratios are governed principally by ion-counting precision in the isotopes of direct interest and also in 204Pb, which provides a measure of common Pb. Because the 204Pb content indicated by the analyses of most of the sample zircons is similar to that obtained from the standard zircon analyses, it is assumed that all the Pb came from the gold coat of the sample surface. The data used for age determinations all required very low common Pb corrections and are therefore insensitive to the choice of common Pb composition. All analyses with higher levels of common Pb have other indications of isotopic disturbance, and the common Pb cannot be assumed to be original, so the choice of composition is necessarily an estimate. The total Pb in each analysis was corrected from common Pb by stripping initial 206Pb, 207Pb, and 208Pb from the measured amounts, using the observed 204Pb and Pb with the composition of Broken Hill galena.
Ages were calculated using U decay constants from Jaffey et al. (1971). Analytical uncertainties given in the tables and shown in plots are 1
. The ages from pooled data are weighted means, with uncertainties given as 95 percent confidence limits. Plots were prepared using ISOPLOT 2.49 (Ludwig, 2001b).
| SHRIMP U-Pb Results |
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Zircons analyzed from the host metavolcanic rock (Fig. 7A-D) comprise euhedral whole grains with relatively well defined crystal faces and terminations (Fig. 7A), subhedral to rounded grains (Fig. 7C-D), and rounded zircon fragments with no clear internal structure (Fig. 7B). Cathodoluminescence is moderate to strong, and almost all grains within these samples display relatively clear, concentric, euhedral, oscillatory zoning patterns.
A total of 13 spots were analyzed in nine zircon grains (Table 3). Only three concordant analyses from two grains (C.1-1, C.1-2, C.6-1) possibly define the rock age (2748 ± 34 Ma, MSWD = 2.7; Fig. 8), with two discordant analyses from another grain (D.2-1, D.2-2) giving similar 207Pb/206Pb ages. Among the other data, two are unquestionably inherited, 207Pb/206Pb ages of ~2865 Ma (C.2-1, D.1-1), consistent with previously reported ages for the Xingu Complex (e.g., Machado et al., 1991). The remaining data are all >25 percent discordant, except for C3.1, which has an anomalously young 207Pb/206Pb age of 2003 ± 9 Ma (Fig. 7B) and may be a reset age.
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Zircons analyzed from mounts B36A and B21D comprise euhedral whole grains and fragments with well-defined crystal faces and terminations (Fig. 7F-H). Moderately to well-rounded grains are noted (Fig. 7E, I), with one grain displaying an irregular, fragmented morphology (Fig. 7J). Cathodoluminescence is strong, and almost all grains display clear concentric euhedral zoning patterns. A few grains have extremely bright CL, especially along rims and within cores. Several grains have more complex and irregular zoning patterns, particularly in the central regions. There are clear structural discontinuities between core regions and rim zones in several grains (e.g., Fig. 7E, F, H), indicating xenocrystic cores (e.g., structurally discordant patterns in their central regions, overgrown by more systematic and concentric, zoned zircon rims; Fig. 7E). This was confirmed by the SHRIMP analyses.
A total of 39 spots were analyzed from 32 grains, but no consistent date emerged from the data set. Approximately half of the analyses, mostly from grains with higher U or high 204Pb, are >5 percent discordant (Table 4). The remaining 20 concordant analyses from 19 grains yielded 207Pb/206Pb ages that range between 3050 ± 9 and 2653 ± 48 Ma. It is evident from CL imaging (Fig. 7E) that the SHRIMP analysis that gave an age of 3050 ± 9 Ma was partially placed on an older core. All analyzed grains display corrosion textures, indicating that zircons were not in equilibrium with the host magma, and are likely inherited. Analyses B21D.2-1 and B21D.2-2 gave ages of 2691 ± 52 and 2653 ± 48 Ma, respectively, and correspond to the irregular grain depicted in Figure 7J. This grain is the youngest concordant zircon analyzed. Therefore, the maximum age of host dike intrusion is ~2670 Ma.
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| Strontium Isotope Composition of Carbonate Minerals |
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The 87Sr/86Sr ratios of the Igarapé Bahia carbonates are highly radiogenic and indicate crustal derivation (Table 6). These values are inconsistent with the isotopic composition of seawater at ~2.575 Ga (Veizer and Compston, 1976) and with the initial 87Sr/86Sr ratios of the Grão Pará metavolcanic rocks (0.7057 ± 0.0010) determined by Gibbs et al. (1986). This evidence clearly precludes seawater as a major component of the hydrothermal system, as would be expected if the deposits were syngenetic (e.g., VHMS model of Ferreira Filho, 1985; Almada, 1998). The wide range of highly radiogenic 87Sr/86Sr ratios (0.7140.755) of the Igarapé Bahia carbonate minerals suggests multiple crustal sources, consistent with an epigenetic magmatic-hydrothermal origin (Fig. 11). Hydrothermal calcite and tourmaline from the Salobo deposit have similar 87Sr/86Sr ratios (Mellito, 1998), suggesting that highly radiogenic strontium signatures are common to Fe oxide Cu-Au deposits of the Carajás belt.
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| Model for the Igarapé Bahia Fe Oxide Cu-Au-(U-REE) Mineralization |
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The positive correlation between REE, P, Au, and Cu, and textural evidence of chalcopyrite in equilibrium with REE minerals in the mineralized breccias (Fig. 9), supports the suggestion that monazite is genetically related to the precipitation of copper and gold in the Igarapé Bahia deposit. Thus, the in situ dating of monazite, from the matrix of ore-bearing magnetite breccias, constrains the age of ore formation. The SHRIMP 207Pb/206Pb age of 2575 ± 12 Ma of hydrothermal monazite indicates that the mineralization occurred ~175 m.y. after accumulation of the host volcano-sedimentary sequence. The data obtained from zircon xenocrysts recovered from the diabase indicate a maximum 207Pb/206Pb age of ~2670 Ma for dike emplacement, consistent with field evidence and the SHRIMP ages of the ore and host rocks (Fig. 12).
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The epigenetic nature of the Igarapé Bahia Cu-Au mineralization is supported by field evidence that includes the presence of fragments of rocks from both the lower and upper unit in the mineralized breccias (Fig. 3C) and the presence of chalcopyrite-rich veins and nodules in the upper unit (Fig. 3A-B). The circular shape of the cluster of breccia bodies (Fig. 2B) is similar to that of ring complexes associated with the intrusion of alkaline magmas.
Chlorite thermometry of the mineralized breccia, determined by Tallarico et al. (2000), indicates relatively high temperatures (313°375°C), consistent with the fluid inclusion data of Ribeiro (1989) and Lindenmayer et al. (1998), which indicate the presence of a high-temperature (150°430°C) group of high-salinity (up to 40% NaCl equiv) inclusions. Assuming that the fluids depositing magnetite and gold were similar to those postulated for other magnetite-rich Cu-Au systems (e.g., Davidson and Large, 1994; Skirrow and Walshe, 2002), copper and gold transport was most likely by chloride complexing, which could also explain the high REE concentrations (e.g., Gieré, 1996).
The stable isotope data of Oliveira et al. (1998) and Tazava (1999), from calcite and siderite in the matrix of mineralized breccias and crosscutting veins from the Igarapé Bahia deposit, yield a narrow range of negative
13C values (9.3 to 5.8
) and a relatively wide range of
18O values (0.79.4
; Fig. 13). The negative
13C values are consistent with a homogeneous deep-seated carbon source from which carbonate minerals were precipitated within a limited pH range. The wider range of
18O values may be the result of mixing or overprinting of deep-seated solutions (high
18O) with meteoric fluids (low
18O). Additional evidence for the latter is provided by a second, low-temperature (100°150°C) group of low-salinity (~10% NaCl equiv) inclusions identified in the studies of Ribeiro (1989) and Lindenmayer et al. (1998).
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| Discussion |
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Iron-oxide Cu-Au-(U-REE) deposits have been recognized as a distinctive ore deposit type during the last decade (Hitzman et al., 1992; Oreskes and Hitzman, 1993). Representative examples of this group include the Olympic Dam deposit with resources of 2,000 Mt at 1.6 percent Cu and 0.6 g/t Au (Roberts and Hudson, 1983; Reeve et al., 1990; Hitzman et al., 1992; Cross et al., 1993; Oreskes and Hitzman, 1993) and the Ernest Henry deposit with resources of 167 Mt at 1.1 percent Cu and 0.5 g/t Au (Williams, 1998). These structurally controlled epigenetic deposits share a number of common features such as (1) high tonnage (>100 Mt) and low copper (<2.0 %) and gold (<0.8 g/t) grades, (2) abundance of magnetite and/or hematite, (3) oxidized and S-poor ore paragenesis (chalcopyrite, bornite, and/or chalcocite), (4) low SiO2 content of the ore, and (5) a metal association of Fe-Cu-Au with anomalous low REE, U, P, and F (Hitzman et al., 1992; Oreskes and Hitzman, 1993; Williams, 1998; Groves and Vielreicher, 2001). Mineralization at all deposits involved high-temperature (200°600°C) ore fluids that were extremely saline (as much as 50 wt % NaCl equiv), acid, and oxidizing, and carried metals as Cl complexes (Hitzman et al., 1992; Oreskes and Hitzman, 1993; Davidson and Large, 1994), with involvement also of relatively low temperature and less saline fluids (Oreskes and Einaudi, 1992; Oreskes and Hitzman, 1993; Gow et al., 1994; Haynes et al., 1995; Barton and Johnson, 1996). The styles of hydrothermal alteration, the ore mineralogy and geochemistry, and the strontium isotope data presented here, together with previous stable isotope and fluid inclusion data, strongly support the classification of Igarapé Bahia as a member of the world-class Olympic Dam-type Fe oxide Cu-Au-(U-REE) deposit group, as previously argued by several authors (Oliveira et al., 1998; Tallarico et al., 1998; Soares et al., 1999; Tazava, 1999). The SHRIMP 207Pb/206Pb age of 2575 ± 12 Ma for hydrothermal monazite from the matrix of mineralized breccia clearly defines Igarapé Bahia as an Archean example of the deposit group.
Several other Cu-Au deposits of the Carajás belt, such as Salobo (2576 ± 9 Ma; Requia et al., 2003), Sossego, and Cristalino, share a number of characteristics with the Igarapé Bahia, such as (1) intense Fe metasomatism resulting in the formation of grunerite, fayalite, and/or Fe oxides (magnetite and/or hematite); (2) intense carbonate alteration; (3) sulfur-poor ore paragenesis (chalcopyrite and bornite); (4) absence of quartz due to silica dissolution; (5) extreme low REE enrichment; and (6) enrichment in U and Co. The similarities between these deposits and Igarapé Bahia indicate that they might also be genetically related to the intrusion of Archean (ca. 2.57 Ga) Estrela-type alkaline granites or deeper, associated, but unexposed, alkaline intrusions in the Carajás belt.
| Acknowledgments |
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May 1, 2002; October 20, 2004
May 1, 2002; October 20, 2004
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D. I. Groves, R. M. Vielreicher, R. J. Goldfarb, and K. C. Condie Controls on the heterogeneous distribution of mineral deposits through time Geological Society, London, Special Publications, January 1, 2005; 248(1): 71 - 101. [Abstract] [PDF] |
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