Significance of apatite REE depletion and monazite inclusions in the brecciated Se–Chahun iron oxide–apatite deposit, Bafq district, Iran: Insights from paragenesis and geochemistry
Research Highlights
► Apatite metasomatism occurs due to fluid over-pressuring immediately prior to brecciation. ► Apatite metasomatism is the first consequence of a shift to K-rich fluids in the system. ► The genetic affinity of the apatites is still recognisable on a Y–Sr classification diagram despite significant removal of LREE. ► Apatite first formed at 510 ± 8 Ma, at the end of or after regional sodic granite intrusion in the BMP. ► Pre-brecciation metasomatism leached the margins of magnetite crystals of Ti and Al.
Introduction
The iron oxide-(Cu–Au) deposit style (IOCG) is consistently associated with rare earth element (REE) enrichment, and consequently it is an ideal venue to study hydrothermal REE behavior during and following the emplacement of REE-bearing minerals. One of the most REE-enriched IOCG varieties are the Kiruna-type deposits (Hitzman et al., 1992, Hitzman, 2000), also recently referred to as “IOA” (iron oxide–apatite; Williams, 2010), or P-rich iron oxide deposits (Groves et al., 2010). The classic IOA districts (Kiruna (Sweden), Bafq Mineral Province (BMP; Iran), Chilean Iron Belt, El Laco (Chile)) are attributed to Andean margin processes, and are physically and temporally distinct (with some important exceptions) from economic IOCG mineralization that occurs in some of these regions (Groves et al., 2010). They consist of massive to brecciated, high temperature, magnetite–fluorapatite–calc–silicate bodies that may transgress or be transitional to regional alteration aprons of albite–actinolite ± K-feldpsar ± phyllic alteration. They show a common association with evolved felsic intrusions, although the nature of the relationship between intrusions and IOA deposits is an area of substantial argument (Parak, 1975, Hildebrand, 1986, Nyström and Henriquez, 1994, Frietsch and Perdahl, 1995, Barton and Johnson, 1996, Barton and Johnson, 2004, Treloar and Colley, 1996, Broman et al., 1999, Hitzman, 2000, Sillitoe and Burrows, 2002, Williams et al., 2005).
The question of a genetic relationship between IOA and economic IOCG deposits is important to understand for exploration models. A link is supported by the fact that some REE-rich IOCG deposits contain textural evidence of an early IOA stage (e.g., Gawler Province, South Australia: Olympic Dam (Oreskes and Einaudi, 1990) and Oak Dam (Davidson et al., 2007); Carajas district: Sossego deposit (Monteiro et al., 2008)). In most IOCG and IOA deposits, REE enrichment is strongly tied to the formation of P minerals, although allanite, and REE carbonates such as bastnaesite and parisite are also important at some sites (e.g., Olympic Dam; Oreskes and Einaudi, 1990). In an example that illustrates some of the complexity in the P-REE relationship, in the Kiruna district, Edfelt (2007) found that REE compositions of IOCG-associated apatite differ from that of IOA apatite. These aspects reinforce the need to better understand the relationship between REE and P-minerals in the iron oxide-associated clan of Groves et al. (2010).
IOA deposits, with their high formation temperatures, are a logical place to explore the P-REE relationship. Apatites from these deposits typically contain 2000–6000 ppm REE (Bafq province apatites contain up to 1.75 wt.% REE; Daliran, 2002), and are strongly LREE-enriched, with moderate to strong negative Eu anomalies (Parak, 1975, Frietsch, 1982, Frietsch and Perdahl, 1995). They contrast with the flat REE patterns of anorthosite-related apatites in ‘Nelsonites’ (apatite–magnetite bodies, e.g., Darling and Florence, 1995). The combined use of back scattered electron imaging (BSE) and LA-ICPMS-based analysis has more recently revealed that apatite can be subject to significant post-depositional REE leaching (Roedder et al., 1987, Harlov et al., 2002), so that it is important to evaluate this possibility before making comparisons to well known apatite end-members (e.g., Belousova et al., 2002). Where REE leaching has occurred in IOA apatite, it is common to observe monazite, and/or xenotime inclusions within the leached zone, or attached to the margins of the leached apatite, and/or within the adjacent calc–silicate-dominated matrix (Harlov et al., 2002, Torab and Lehmann, 2007, Stosch et al., 2010). Experimental studies prove that these monazite and xenotime inclusions typically nucleate after internal redistribution of the apatite REE by a Na–Ca-poor fluid (Harlov and Förster, 2003, Harlov et al., 2005). While this may occur as a part of the typically extensive hydrothermal history of IOA deposits, it may also accompany hydrous metamorphism (Darling and Florence, 1995, Harlov et al., 2002, Edfelt, 2007). Stosch et al. (2010) have used U–Pb dates from apatite-hosted monazite inclusions to contend that the REE redistribution in apatite may even occur during hydrothermal overprinting tens to hundreds of millions of years after IOA formation. Thus it is now uncertain whether apatite REE depletion and consequent formation of monazite inclusions has paragenetic significance within IOA formation models.
Our contribution describes the geology and geochemistry (with emphasis on REE, U and Th) of an IOA deposit, Se–Chahun, from the BMP, Central Iran. The deposit has received little previous attention, but is economically important, and is of interest in the context of the above brief review of REE-P relationships in IOA deposits, because it provides new information on the timing of apatite metasomatism within an IOA paragenesis, and in particular its relationship to brecciation. Our samples were collected from mined outcrops and from drillcore, and were analyzed using transmitted light microscopy, BSE imaging, mineral liberation analysis (MLA), electron microprobe analysis (EMPA), and laser ablation-inductively coupled plasma-mass spectrometry (LA-ICPMS) techniques. Numerous samples were used to construct the paragenesis, and our detailed geochemistry was undertaken on 6 of these.
Section snippets
Geological setting of the Bafq Mining District
The BMP is surrounded by fold-and-thrust belts, within the Alpine–Himalayan orogenic system of western Asia. The terrane is divided into three major crustal domains, from east to west: the Lut Block, Tabas Block and the Yazd Block (Alavi, 1991). The Tabas and Yazd blocks are separated by a nearly 600 km long, 80 km wide, arcuate and structurally complex belt (Kashmar-Kerman Tectonic Zone) composed of variably deformed and fault-bound supracrustal rocks (Ramezani and Tucker, 2003). The latter
Magnetite
Magnetite (Fig. 5A–D) grain size tends to be bimodal, with one mode averaging 200 μm diameter (up to 1 mm) with a typically more euhedral form (Fig. 5C), whereas the second mode averages 100 μm, and is more typically anhedral. All primary magnetite crystals have cores rich in distinct ilmenite lamellae parallel to the {111} plane (Fig. 5B), but Ti mapping shows that the natural magnetite rims are characterized by a ~ 50 μm wide, smaller scale, speckled ilmenite exsolution texture (Fig. 6A).
EMPA
Mineral analyses were carried out using a SX-100 CAMECA EMPA at the Central Science Laboratory, University of Tasmania. The wavelength dispersive technique was employed. Detection limits for the rare earth elements were 300–1000 ppm. Concentrations of Tb, Ho, Er, and Lu in monazite were routinely measured but their concentrations were below detection limits. The concentrations of U and Pb also were below detection limits (230 and 80 ppm, respectively). Analyses of apatite were performed at 15 kV
Significance of apatite–monazite textures and chemistry
The Se–Chahun IOA ore bodies have the same massive to brecciated textures, high temperature calc–silicate–albite haloes, and LREE-rich geochemical signatures as those of classic Swedish IOA deposits (Hildebrand, 1986, Nyström and Henriquez, 1994, Frietsch and Perdahl, 1995, Belousova et al., 2002, Harlov et al., 2002). The other Bafq district magnetite–apatite deposits also share these features (for instance, Esfordi, Chador-Malu, Choghart; Förster and Jafarzadeh, 1994, Daliran, 2002, Jami et
Conclusion
Extensive Na-rich fluid circulation produced large-scale sodic alteration (albitization) in a mixed volcano-sedimentary sequence intruded by sodic granitoids (525 ± 7 Ma). This regional alteration was followed by deposit-related Na–Ca alteration and magnetite–apatite mineralization at 510 ± 8 Ma at Se–Chahun. Main-stage apatite formation was succeeded by a change in fluid chemistry to co-existing CO2 and K–Cl-rich fluids (the latter requires analytical confirmation), which was followed by
Acknowledgments
The authors express their gratitude to the managers of the ICIOC (Iranian Central Iron Ore Co.) and Se–Chahun mine for access to the deposit, sampling and support during field work. We feel particularly indebted to Mr. Abdol-Hossein Dehghani Firoozabadi for his invaluable orientation in the field. We wish to thank Dr. Karsten Goemann who assisted with the electron-microprobe and scanning electronic microscopy studies. Simon Stephens is thanked for providing thin and polish sections. Professor
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