Do Magnetite Layers In Algoma-Type Banded Iron Formations (BIF) Preserve Their Primary Geochemical Signature? A Case Study of Samples From Three Archean BIF-Hosted Gold Deposits Blandine Gourcerol, Daniel Kontak, Phillips Thurston, Quentin Duparc
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Blandine Gourcerol, Daniel Kontak, Phillips Thurston, Quentin Duparc. Do Magnetite Layers In Algoma-Type Banded Iron Formations (BIF) Preserve Their Primary Geochemical Signature? A Case Study of Samples From Three Archean BIF-Hosted Gold Deposits. The Canadian Mineralogist, Min- eralogical Association of Canada, 2016, 54 (3), pp.605-624. 10.3749/canmin.1500090. hal-02267547
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The Canadian Mineralogist Vol. 54, pp. 1-21 (2016) DOI: 10.3749/canmin.1500090
DO MAGNETITE LAYERS IN ALGOMA-TYPE BANDED IRON FORMATIONS (BIF) PRESERVE THEIR PRIMARY GEOCHEMICAL SIGNATURE? A CASE STUDY OF SAMPLES FROM THREE ARCHEAN BIF-HOSTED GOLD DEPOSITS
§ BLANDINE GOURCEROL ,DANIEL J. KONTAK, AND PHILLIPS C. THURSTON Mineral Exploration Research Centre, Laurentian University, Sudbury, Ontario, Canada P3E 2C6
QUENTIN DUPARC UniversiteduQu´ ebec´ a` Chicoutimi, Chicoutimi G7H 2B1, Quebec,´ Canada
ABSTRACT
The geochemistry of chert layers in Algoma-type banded iron formations (BIF) has been used to constrain the depositional setting of the BIFs, as rare earth element (REE) and yttrium (Y) systematics are a function of their chemical environment of formation. In contrast, the chemistry of the interbedded oxide-rich layers (i.e., magnetite) has not been analyzed for this purpose because of the presumed potential effects related to diagenetic changes during conversion from primary iron-bearing mineralogy to magnetite. Here, we explore the validity of this latter hypothesis by examining the results of LA-ICP-MS analysis of iron-oxide layers at three Canadian BIF-hosted gold deposits (i.e., Meadowbank, Meliadine, Musselwhite) to assess whether the primary REEþY systematics of the oxide layers are preserved and, if so, what are the implications. The results indicate that, regardless of their diagenetic, later metamorphic, and hydrothermal histories, the chemistry of the iron oxides retains a primary signal in all cases with the following indicated: (1) interaction of the primary Fe-oxyhydroxide phases with seawater, as reflected by heavy REE enrichment relative to light REE depletion that is coupled with variable La and Y enrichment; and (2) some input of moderate-temperature (.250 8C) hydrothermal vent fluids, as suggested by positive Eu anomalies. The chemical data are also used to evaluate currently used classification diagrams for ore deposits based on magnetite chemistry. Our new data indicate that the fields for magnetite geochemistry in BIF are too restricted or lead to misclassification of samples. In the case of the latter, it may be that interaction of fluids with the immediate substrate influences the chemical signature of samples. Therefore, caution is suggested in using these diagrams where hydrothermal fluids are involved in magnetite formation.
Keywords: magnetite, banded iron formation, geochemistry, hydrothermal, seawater.
INTRODUCTION diagenesis or by later metamorphic recrystallization to hematite, magnetite, various iron-silicates and carbon- Algoma-type banded iron formations (BIFs) are ates, and pyrite (e.g., Posth et al. 2013). The thinly bedded, chemical sedimentary rocks comprised interbedded chert layers have been shown to reflect a of alternating layers of iron-bearing minerals and primary geochemical signature that suggests precipi- chert. The iron-bearing minerals are considered to tation upon interaction of seawater and moderate- have originally precipitated as iron oxyhydroxides due to mixing of acidic to neutral, iron-rich Archean temperature hydrothermal fluids with variable amounts seawater and alkaline moderate-temperature hydro- of detrital contamination (e.g., Gourcerol et al. 2015a, thermal fluids (Shibuya et al. 2010, Gourcerol et al. b, c). An essential question in this regard, therefore, is 2015b) combined with possible photoautotrophic whether the iron-bearing minerals, despite having bacterial activity (i.e., Kappler et al. 2005, experienced multiple recrystallization events (e.g., Konhauser et al. 2005, Gourcerol et al. 2015b). These Pickard et al. 2003), retain a geochemical signature primary iron-bearing minerals are transformed during indicative of their primary environment, this being a
§ Corresponding author e-mail address: [email protected]
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combination of marine seawater and hydrothermal In this contribution, we explore the geochemistry of vent fluids. iron-oxide layers at three Archean BIF-hosted gold The compositional variability of oxide minerals deposits located in Canada: the ~4 Moz Au Meadow- (e.g., magnetite, hematite), which collectively form in bank deposit, hosted by the 2.71 Ga Woodburn Lake a wide variety of ore-forming environments (e.g., greenstone belt; the 2.8 Moz Au Meliadine gold hydrothermal versus magmatic), has been the focus of district, hosted by the 2.6 Ga Rankin Inlet greenstone many studies in recent years, in part due to advances in belt; and the ~6 Moz Au Musselwhite deposit, hosted analytical instrumentation such as the laser ablation- by the 2.9–3 Ga North Caribou greenstone belt. inductively coupled plasma-mass spectrometer (LA- Importantly, in each of these studied areas we have ICP-MS) (e.g., Grigsby 1990, Dare et al. 2012, 2014, previously characterized the chemistry of the inter- Nadoll et al. 2014). Of particular significance is that bedded chert (Fig. 1; Gourcerol et al. 2015a, b, c). several studies have demonstrated that the geochem- Also relevant is that the BIFs at each of these deposits ical signature of the oxide minerals, in particular are either intercalated with mafic to ultramafic magnetite, can be a genetic indicator of ore deposit volcanic rocks or associated interflow sedimentary environments, in part due to the ability of the rocks, which may represent different potential sources analytical method to provide the resolution necessary for the iron-rich minerals composing the Fe-oxide to distinguish various geochemical types (Dupuis & layers. Beaudoin 2011, Dare et al. 2014). As a result of these The main objective of this study is, therefore, to recent advances, it is now possible to distinguish assess the potential of using the REE þ Y systematics geochemically between hydrothermal and magmatic of magnetite bands to identify their primary geochem- ical signature, as we have done for the associated magnetite. For example, whereas hydrothermal mag- cherts (Gourcerol et al. 2015b). If this study is netite compositions may vary depending on various successful, it will provide the possibility of using the factors such as fluid composition, host rock buffering, geochemistry of magnetite from magnetite-rich bands and re-equilibration processes (Nadoll et al. 2014), to constrain the genesis of BIF units. In addition, we they are generally characterized by depletion in Ti and also use these data to assess the validity of the an elevated Ni/Cr ratio compared to their magmatic currently defined field for magnetite from BIF settings equivalent and are enriched in elements which do not in chemical classification diagrams. nominally enter the lattice of magmatic magnetite (e.g., Si and Ca). Magmatic magnetite is enriched in Ti GEOLOGICAL SETTING OF THE SELECTED BIFS with a lower Ni/Cr ratio (Dare et al. 2014). However, despite geochemical characteristics which have not The Meadowbank gold deposit been well documented, magnetite may also be The Meadowbank deposit, which has been mined precipitated by hydrogeneous processes during forma- since 2010, contains a total of about 4 Moz of gold tion of BIF, as discussed above (e.g., Kappler et al. including 1.3 Moz produced from 2010 to 2013 2005, Konhauser et al. 2005, Shibuya et al. 2010, (Janvier et al. 2015). Located in the Rae Domain of Gourcerol et al. 2015b) and may show depletion in the Churchill Province, the deposit is hosted by the compatible elements (Cr, Ni, V, Co, Zn, Ti) that are Woodburn Lake greenstone belt (ca. 2.71 Ga) which characteristic of magnetite formed from low-temper- consists of tholeiitic and komatiitic metavolcanic rocks ature environments (Dare et al. 2014). with minor calc-alkaline felsic tuffs and flows with Only a few studies have explored the REE intercalated BIF and clastic metasedimentary rocks geochemistry of iron oxides in Algoma-type BIF (Armitage et al. 1996, Sherlock et al. 2001a, b, 2004, (e.g., Pecoits et al. 2009, Angerer et al. 2012, Li et al. Hrabi et al. 2003, Pehrsson et al. 2004). The regional 2014), but in such cases, analyses of the accompanying metamorphic grade ranges from middle greenschist to chert bands are lacking. These analyses would provide amphibolite facies (Pehrsson et al. 2004) and the an internal check on geochemical concordance, that is, sequence was deformed by at least six regional-scale each providing the same chemical signature of their Archean and Paleoproterozoic deformation events environment of formation. Thus, the occurrence of (e.g., Pehrsson et al. 2013). geochemical parallelism and hence genetic processes Numerous units of oxide-, silicate-, and locally between the chemistry of magnetite and chert (i.e., sulfide-facies Algoma-type BIF have been identified LREE depletion relative to HREE, variable positive which include the West IF, Central BIF, and East BIF; La/La* and Y/Y* anomalies, positive Eu/Eu* anom- all of the BIFs are generally interlayered with the alies) has yet to be documented. The purpose of this volcanic rocks and locally with a quartzite unit paper is to present the first such data and validate this (Gourcerol et al. 2015c, Sherlock et al. 2001a, b, hypothesis. 2004).
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FIG. 1. Photographs at different scales that illustrate the nature of the BIFs in the field, their microscopic features and traces of the laser ablation traverses. (A) Outcrop photograph of BIF at the Meadowbank gold deposit area showing the characteristic layers of chert and iron-rich layers, in this case magnetite. (B) Close up of the outcrop showing alternating layers of chert and magnetite. (C) Scanned thin section of BIF from outcrop in image which shows the chert and magnetite layers. The black solid line represents the laser ablation traverse done on the chert as part of our previous LA ICP-MS study (Gourcerol et al. 2015a, b, c), whereas the white solid line represents the line traverse done on the magnetite rich layer in this study. (D) SEM back-scattered electron image of the BIF layering showing alternating layers of chert and magnetite.
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The Meliadine gold district B, C, D) that are mainly composed of anhedral and amalgamated (i.e., polycrystalline texture of anhedral The Meliadine gold district, which is one of the and annealed crystals) magnetite with rare cryptocrys- Canada’s largest BIF-hosted gold districts, contains talline hematite that is locally overprinted by late 2.8 Moz Au in reserves as well as an indicated and euhedral magnetite grains. The iron-rich bands form inferred resource of 5.8 Moz Au (Lawley et al. 2015). millimetric to centimetric layers that are interbedded The gold district is hosted by the 2.6 to 2.7 Ga Rankin with chert layers. The Fe-oxide layers are dominated Inlet greenstone belt (Wright 1967, Aspler & by magnetite, but they may also contain variable Chiarenzelli 1996a) which lies along the boundary proportions of mineral inclusions such as quartz, between the Central and the North Western Hearne hematite, pyrite, pyrrhotite, apatite 6 chlorite, and domains of the Churchill Province (Tella et al. 2007, variable silicates (Fig. 2A, B, C, D). No specific Davis et al. 2008). The Rankin Inlet greenstone belt attention was paid to recognition of and deciphering consists of poly-deformed massive and pillowed mafic the different events responsible for the formation of volcanic rocks, felsic pyroclastic rocks and associated the Fe-oxide layers, that is, primary versus later interflow sedimentary units, gabbro sills, and oxide- recrystallization stages, as only the continuous Fe- facies BIFs; all of these units are intruded by minor oxides layers (i.e., anhedral and amalgamated magne- granite and undeformed biotite lamprophyre, as well tite phase) were selected for analysis. as late gabbro and diabase dikes of Archean and Each of the Fe-oxide layers analyzed in this study Proterozoic age. These rocks have been metamor- is located immediately adjacent to the chert layers phosed from lower greenschist to lower-middle analyzed in our earlier study (Gourcerol et al. 2015b; amphibolite facies (Carpenter 2004, Carpenter, et al. Fig. 1C, D). Polished thin sections (100 lm thick) 2005). were examined, using both transmitted and reflected light microscopy, and selected material was studied in The Musselwhite gold deposit more detail using a JEOL JSM-6400 scanning electron The Musselwhite deposit, which has been mined microscope coupled to an energy dispersive spectrom- since 1997, contains a total of about 6 Moz of gold, eter (EDS). Based on previous petrographic work, including 4 Moz produced and 1.85 Au reserves areas for analysis were selected to minimize the (Oswald et al. 2015). Located in the North Caribou presence of phases other than magnetite, including terrane of the Superior Province, the deposit is hosted alteration, and mineral inclusions. Operating condi- by the North Caribou greenstone belt which is tions were an accelerating voltage of 20 keV, 1.005 nA dominated by mafic to ultramafic metavolcanic rocks beam current, acquisition count times of 10 s, and a of the 2973 to ,2967 Ma Opapimiskan-Markop working distance of 15 mm. The SEM-EDS was used metavolcanic assemblage, and tholeiitic basalts and to select the most suitable magnetite layers having minor felsic volcanics of the 2980 to 2982 Ma South minimal amounts of paragenetically later-stage min- Rim metavolcanic assemblage (Biczok et al. 2012, erals related to metamorphic, hydrothermal, or ore- McNicoll et al. 2013). These rocks have been forming processes, such as garnets, variable amphi- metamorphosed from lower greenschist to lower-mid boles, and sulfides. amphibolite facies (Breaks et al. 2001) and deformed Using the same protocol applied to the chert layers by three deformation events (Hall a& Rigg 1986, analyzed in Gourcerol et al.(2015a,b,c),the Breaks et al. 2001). The Opapimiskan-Markop meta- magnetite layers were analyzed with line traverses volcanic assemblage consists, from the structural base rather than spots (Fig. 2E, F) using a Resonetics to the top, of the ‘‘Lower Basalt’’ unit, the Southern RESOlution M-50 193 nm ArF excimer laser-ablation Iron Formation, ‘‘Basement Basalt’’ unit, and the system coupled to a Thermo X Series II quadrupole Northern Iron Formation (e.g., Moran 2008, Biczok ICP-MS in a two-volume Laurin Technic sample cell. et al. 2012). The nature of the BIFs is described in The instrument operated with a forward power of 1450 more detail in Gourcerol et al. (2015a). W. Gas flows were 800 ml/min for Ar, 650 ml/min for He, and 6 ml/min for N. Dwell times for elements SAMPLE DESCRIPTION,ANALYTICAL METHODS, AND analyzed were 10 ms. These conditions should 69 29 40 DATA TREATMENT minimize interferences such as Ga with Si Ar. Stage movement speed was 20 lm/s. As chert and The samples collected for the study include: (1) magnetite layers show very low concentrations of seven samples from the Meadowbank deposit (Fig. 1A, REE, spot analyses may yield data below the detection B); (2) eight samples from the Meliadine gold district; limit for many elements, therefore, line traverses of and (3) three samples from the Musselwhite deposit. polycrystalline aggregates were made using both 140 These samples represent bands of Fe-oxides (Fig. 2A, and 190 lm beam diameters with a repetition rate of
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10 Hz and an energy density of 7 J/cm2 to optimize the 1996) and a slightly negative Gd anomaly associated time-signal acquisition, representing therefore an with hydrothermal vent fluid (e.g., Allwood et al. average for each element along the analyzed traverse. 2010). Thus, as Archean seawater was influenced by However, since the line traverse method increases the hydrothermal vent fluids, the Gd anomalies are possibility of detrital contaminants, present as inclu- variable in magnitude and sign (þ versus –), sions or minerals disseminated along the traverse line, suggesting precipitation under influence of seawater the Queensland alluvial shale composite (MUQ) was and hydrothermal input. We note that the Gd used to normalize the REE þ Y values to minimize the anomalies reported and discussed in previous papers influence of any potential terrigenous input, whereas on REE þ Y systematics from BIF precipitated in trace elements were normalized to bulk continental Archean seawater (e.g., Bolhar et al. 2005, Thurston et crust (values from Rudnick & Gao 2003). The MUQ al. 2012) were small to nonexistent, thus Gd anomalies composition represents a mixed bimodal felsic and are not discussed here. mafic volcanic provenance (Kamber et al. 2005), which acts as a proxy for the expected average REE þ YSYSTEMATICS terrigenous input from a typical bimodal greenstone belt into the Archean ocean (e.g., Bolhar et al. 2005, Despite some minor exceptions, the REE þ Y Thurston et al. 2012). normalized data presented in the tables (Tables 1, 2, 3) The final concentrations of elements were deter- and diagrams (Fig. 3) show relatively uniform REE þ mined using off-line calculations following the Y patterns for the magnetite layers sampled from the protocol of Longerich et al. (1996). Data were three different gold deposits (i.e., Meadowbank, processed with Iolite (Paton et al. 2011) and the NIST Meliadine, and Musselwhite) and these data are 612 glass standard was used as a primary external discussed separately below. Comparisons to other reference material (e.g., Nadoll et al. 2014); iron studies of magnetite geochemistry are discussed in concentrations were used as an internal standard for subsequent sections. calibration of the LA-ICP-MS data. In the Meadowbank area (Fig. 3A), the magnetite The elemental concentrations reported in this study bands show depletion in light REE (LREE) relative to represent the integrated signal over the length of the middle and heavy REE (HREE) with Nd/YbMUQ ¼ traverse. The element list used for each analysis 0.1–0.4 associated with slight to moderate positive La, included the 14 REEs in addition to 7Li, 9Be, 29Si, Y, and Eu anomalies (La/La* ¼ 1.4–2.7, Y/Y* 45Sc, 47Ti, 51V, 52Cr, 55Mn, 57Fe, 59Co, 60Ni, 65Cu, MUQ MUQ ¼ 1.01–1.6, Eu/Eu* ¼ 1.7–3.7) and super-chon- 66Zn, 69Ga, 75As, 85Rb, 88Sr, 90Zr, 93Nb, 95Mo, 107Ag, MUQ dritic Y/Ho values (Y/Ho ¼ 30.9–43.9). In addition, 111Cd, 115In, 118Sn, 121Sb, 133Cs, 137Ba, 178Hf, 181Ta, slight positive Ce anomalies are notable (Ce/Ce* 182W,197Au, 205Tl, 208Pb, 232Th, and 238U. In this MUQ 1.09–1.38). study, the detection limits achieved were significantly ¼ lower than the concentration of REEs in magnetite In the Meliadine gold district (Fig. 3B), most of the samples (Tables 1, 2, 3). The La, Ce, Eu, and Y magnetite layers also show depletion in the LREE anomalies were calculated [Equations (1) to (4)] relative to middle and HREE (Nd/YbMUQ¼ 0.08– 0.6) following the procedure of Lawrence & Kamber with associated slight to moderate positive La, Y, and (2006): Eu anomalies (La/La*MUQ ¼ 0.7–1.8, Y/Y*MUQ ¼ 0.9– hi1.3, Eu/Eu*MUQ ¼ 0.9–1.9) and super-chondritic to * 2 chondritic Y/Ho values (Y/Ho ¼ 24.7–34.9). In detail, ðLa=LaÞ MUQ ¼ LaMUQ= PrMUQ*ðPrMUQ=NdMUQÞ samples MEL-032 and MEL-033 yield slightly ð1Þ anomalous HREE-depleted concentrations (Nd/ YbMUQ¼ 1.4–1.9) which are also associated with * moderate positive La, Y, and Eu anomalies. Minor to ðCe=CeÞ MUQ ¼ CeMUQ= PrMUQ*ðPrMUQ=NdMUQÞ moderate positive Ce anomalies are also recognized in ð2Þ these samples (Ce/Ce*MUQ ¼ 0.9–1.2). In the Musselwhite area (Fig. 3C), magnetite layers * 2 1=3 ðEu=EuÞ MUQ ¼ EuMUQ=ðSmMUQ*TbMUQÞ ð3Þ show depletion in LREE relative to middle and HREE (Nd/YbMUQ¼ 0.3–0.5) with associated slight to * moderate positive La, Y, and Eu anomalies (La/ ðY=YÞ MUQ ¼ YMUQ=ð0:5ErMUQ*0:5HoMUQÞð4Þ La*MUQ ¼ 1.14–2.45, Y/Y*MUQ ¼ 1.2–1.6, Eu/ The Gd values in Archean iron formation are Eu*MUQ ¼ 2.1–2.8), super-chondritic Y/Ho values considered to reflect a combination of a small positive (Y/Ho ¼ 35.8–41.3), and slightly to moderately Gd anomaly associated with seawater (Bau & Dulski positive Ce anomalies (Ce/Ce*MUQ ¼ 1.1–1.3).
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FIG. 2. Images showing typical Fe-oxide layers sampled for this study: (A) Reflected light image of a polished thin section of sample AMB-126225 showing its groundmass which consists of magnetite with minor quartz (yellowish color) and minor recrystallized magnetite 6hematite (darker grey) inclusions. (B) Back-scattered electron (BSE) image from the SEM of sample MEL-025 which illustrates a magnetite band with inclusions of minor chlorite and quartz. (C) BSE image from the SEM of sample MEL-028 which illustrates magnetite layers associated with minor inclusions of quartz and chlorite. (D)
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ADDITIONAL MAJOR AND TRACE ELEMENT DATA BIF magnetites are notably depleted in these compat- ible elements (Fig. 5), which is probably a reflection of Magnetite layer samples from the three deposits their lower solubility in these fluids (e.g., Ray & show relatively similar abundances of major and trace Webster 2007, Nadoll et al. 2012, 2014, Dare et al. elements, as indicated in Figure 4, which attests to 2014). Hence, it appears that magnetite from BIFs is their similar overall geochemistry. As expected, high characterized by lower overall abundances of the concentrations of Fe, Ti, V, Cr, Mn, Ni, and Zn occur compatible trace elements relative to high-temperature in the magnetite, whereas the relatively high Si hydrothermal magnetite (e.g., Angerer et al. 2012, concentrations, as noted in the three deposits, are Nadoll et al. 2014, Dare et al. 2014, Chen et al. 2015). attributed to the presence of quartz and other silicate In contrast to these elements, similar or higher grains present along the line traverses. The moderate normalized values are noted for Pb, Zr, Hf, Mn, Mo, concentrations of Ba and Sr detected may reflect the Nb, and Cu, which might be attributable to the high presence of feldspar, likely of metamorphic origin. solubility of Pb and contamination from ubiquitous In previous geochemical studies of magnetite, data micro- to nanometer scale inclusions (Duparc 2014) were normalized to bulk continental crust (values from such as zircon, various sulfides, and Nb-bearing oxide Rudnick & Gao 2003) in order to emphasize the grains in the magnetite layers. partitioning behavior of the trace elements between the magnetite, magma, hydrothermal fluid, and co-crys- DISCUSSION tallizing phases (Dare et al. 2014). Therefore, in order to assess and compare the trace element data from this It is now widely accepted that abundance of REE þ study to that of other magnetite studies, the data for Y and the MUQ-normalized patterns of chert bands our samples have also been normalized to bulk from Algoma-type BIFs may reflect primary geo- continental crust in multi-element variation diagrams chemical signatures inherited through precipitation in which elements are plotted in order of increasing from a mixed reservoir of seawater and moderate- compatibility with respect to magnetite (Dare et al. temperature hydrothermal vent fluids with variable 2014). Most of the major and trace elements show amounts of detrital contamination (e.g., Bau & Dulski 1996, Thurston et al. 2012, Gourcerol et al. 2015a, b, consistent patterns (Fig. 5A, B, C) with concentrations c). Below, we assess the validity of this chemical less than one times bulk continental crust. In detail, pattern, which is also present in the magnetite layers however, the magnetite samples from the Meadow- interbedded with the cherts. using the data from the bank, Meliadine, and Musselwhite deposits show three Archean Algoma-type BIFs examined in this slight to moderate relative depletions in Ti, Co, V, study. In addition, these data are then used to assess Ni, and Cr compared to magnetite of high-temperature the validity of the currently defined fields for origin (Dare et al. 2014). This latter feature is in magnetite from BIF in magnetite classification dia- general similar to the data for both whole-rock (Pecoits grams (e.g., Dupuis & Beaudoin 2011, Dare et al. et al. 2009, Angerer et al. 2012) and in situ (Dare et al. 2014). 2014, Dupuis et al. 2014, Nadoll et al. 2014) analyses of magnetites from BIFs in the literature (Fig. 5A, B, Assessing the primary geochemical signature for C). It must be noted that the composition of iron magnetite layers formations associated with gold mineralization do not differ substantially from non-mineralized iron forma- Comparison of the REE þ Y distribution patterns of tions (e.g., Gourcerol et al. 2015c, Thurston et al. metalliferous sediments (on a carbonate-free basis) 2012). Compared to the relatively high-temperature composed mainly of poorly crystalline to amorphous (i.e., .500 8C) hydrothermal magnetite samples of Fe-Mn oxyhydroxides and variable amorphous silicate Dare et al. (2014), the magnetites in this study formed phases from the Pacific Ocean (Fig. 6; Barrett & Jarvis in part from lower-temperature fluids, including a 1987, Dekov et al. 2010) and the magnetite layers in component of hydrothermal vent fluids (,250 8C). this study highlights that, other than the differences in Thus, based on the latter, it is not surprising that the the Ce anomalies between modern metalliferous