Fluids, Metals, and Mineral/Ore DepositsView this Special Issue
The Fe-Zn Isotopic Characteristics and Fractionation Models: Implications for the Genesis of the Zhaxikang Sb-Pb-Zn-Ag Deposit in Southern Tibet
The genesis of the Zhaxikang Sb-Pb-Zn-Ag deposit remains controversial. Three different geological environments have been proposed to model mineralization: a hot spring, a magmatic-hydrothermal fluid, and a sedimentary exhalative (SEDEX) overprinted by a hot spring. Here, we present the electron probe microanalysis (EPMA) and Fe-Zn isotopic data (microsampled) of four samples from the first pulse of mineralization that show annular textures to constrain ore genesis. The Zn/Cd ratios from the EPMA data of sphalerite range from 296 to 399 and overlap the range of exhalative systems. The δ56Fe values of Mn-Fe carbonate and δ66Zn values of sphalerite gradually decrease from early to late stages in three samples. A combination of the EPMA and isotopic data shows the Fe-Zn contents also have different correlations with δ66Zn values in sphalerite from these samples. Rayleigh distillation models this isotope and concentration data with the cause of fractionation related to vapour-liquid partitioning and mineral precipitation. In order to verify this Rayleigh distillation model, we combine our Fe-Zn isotopic data with those from previous studies to establish 12 Fe-Zn isotopic fractionation models. These fractionation models indicate the δ56Fei and δ66Zni values (initial Fe-Zn isotopic compositions) of the ore-forming system are in the range of − and , respectively. To conclude, the EPMA data, Fe-Zn isotopic characteristics, and fractionation models support the SEDEX model for the first pulse of mineralization.
To date, the Zhaxikang Sb-Pb-Zn-Ag deposit is the only super large deposit that has been identified within the North Himalayan Polymetallic Metallogenic Belt (NHMB). Although basic research including the geology, petrography, geochronology, and geochemistry studies has been conducted (e.g., [1, 2]), the genesis of this deposit is still debated due to the complicated mineralogy and the presence of multiple stages of mineralization. The main viewpoints involve a hot spring [3, 4], two magmatic-hydrothermal fluids [5, 6], and a SEDEX overprinted by hot spring  genetic models. However, most of these genetic models are based on the S, C, O, H, and Si isotopic evidence, which cannot absolutely trace the metal source.
The traditional light stable C, H, O, S, and N isotopes have been widely used to constrain fluid evolution and metal sources in ore deposit studies (e.g., [8, 9]). However, the evidences for metal source from these elements are always indirect and putative as they are not the metallogenic elements themselves . For instance, these elements usually have different characteristics with the changing of tectonic settings, and sometimes they may even have different sources from the metallogenic elements . However, the nontraditional transition metal stable isotopes (e.g., Fe, Zn, Cu, Cd, Mg, Cr, Sn, and Mo) are more precise tracers for the metal sources and ore-forming processes in metallogenic systems [10, 12, 13]. The development of Multicollector-Inductively Coupled Plasma Mass Spectrometer (MC-ICP-MS) technology has greatly improved the precision of isotopic analyses [14, 15], which results in the wide application of the nontraditional transition metal stable isotopes in economic geology studies (e.g., [16, 17]).
The Fe-Zn isotopes are two of the most representative isotopes applied in ore deposit studies. For example, Mason et al.  and Wilkinson et al.  both identified that the δ66Zn values of minerals precipitating from the same hydrothermal fluid become heavier over time by studying the Zn isotopic fractionation of the Alexandrinka volcanic hosted massive sulfide (VHMS) type deposit in Russia and Midlands Irish-type deposit in Ireland, respectively. The gradual increasing δ66Zn values both from early to late stages and from south to north within the Red Dog ore district in Alaska record the temporal-spatial evolution of the ore-forming fluid and constrain the SEDEX genesis with a single Zn source . In addition, Fe isotopic studies of skarn Cu−Au±Fe deposits in South China excluded the possibility that Fe originated from sedimentary strata [21, 22]. These Fe isotopes matched the igneous source rocks and mineralization, and the δ56Fe values of sulfides gradually increase both from early to late stages and away from the ore-related igneous rocks. Wang et al. [21, 22] also revealed that the Fe isotopes fractionate during fluid exsolution and that the ore-forming fluid is enriched in light isotopes relative to ore-related igneous rocks. To the contrary, Wawryk and Foden  investigated the Fe-isotope fractionation in the Renison Sn-W deposit in Australia and discovered that Fe isotopic compositions of pyrite (), chalcopyrite (), and magnetite () are isotopically heavier than Renison granite () and thus hypothesized that a magmatic-hydrothermal fluid exsolved from an isotopically heavy reduced magma could deposit isotopically heavy ore minerals whereas oxidized magmas crystallise magmatic magnetite could result in an isotopically lighter melt and fluid. These studies demonstrate the potential of Fe-Zn isotopes to trace the metal source and provide insights into ore-forming evolution.
With regard to the Zhaxikang deposit, Duan et al.  have investigated the Zn isotope of sphalerite, galena, Fe-Mn carbonates, and igneous rocks and speculated that the δ66Zn values of the hydrothermal fluid are 0.39 ± 0.10. This value is consistent with those of basement rocks (average value of 0.36 ± 0.03) and Fe-Mn carbonates (average value of 0.27 ± 0.15), which is identified as the evidence for the magmatic origin. Meanwhile, the contribution of regional sedimentary rocks is conjectured by the Zn-Pb-S isotopes: the Zn isotopic variation range of sulfides () is larger than basement rocks (); the radiogenic Pb isotopic compositions of sulfides (e.g., 206Pb/204Pb = 18.727~19.896) is higher than regional igneous rocks (206Pb/204Pb = 18.4~19.2); the δ34S values of sulfides () are lighter than regional sedimentary wall rocks () but higher than mantle value (0 ± 2). However, the Zn isotopic fractionation during the fluid exsolution and leaching process [27, 28] has been ignored in Duan et al. . In addition, Wang et al.  also studied the Fe-Zn isotopes of the pyrite, sphalerite, and Mn-Fe carbonate in Zhaxikang deposit, which successfully constrained the two pulses of mineralization by the temporally increasing δ56Fe and decreasing δ66Zn values recorded in the deposit that coincided with an increase in alteration. The Fe-Zn isotopic research also demonstrated the magmatic-hydrothermal fluid origin of the second pulse of mineralization by the heavier δ56Fe values of stage 3 pyrite and excluded the possibility that slate is the metal source by the similar δ66Zn values of slate and sphalerite. Nevertheless, the attempt to trace the metal source of the first pulse of mineralization failed in Wang et al. . In this study, we present the Fe-Zn isotopic values and variations within four annular polished section samples from Zhaxikang deposit to provide more credible evidence for the primary and earlier stages of ore genesis.
2. Geological Setting
2.1. Regional Geology
The NHMB is in the eastern section of the North Himalayan Tectonic Belt (NH), in the Himalayan terrane. From north to south, the Himalayan terrane is divided into four tectonic belts: the North Himalayan Tethys Sedimentary Fold Belt (the North Himalayan Tectonic Belt; NH), the High Himalayan Crystalline Rock Belt (HH), the Low Himalayan Fold Belt (LH), and the Sub-Himalayan Tectonic Belt (SH; Figure 1(a)) [29–31]. These belts are separated by four nearly EW-trending faults, including the South Tibet Detachment System (STDS), the Main Central Thrust (MCT), the Main Boundary Thrust (MBT), and the Main Frontal Thrust (MFT; Figure 1(a)) [24, 32]. The NH, composed of a set of Palaeozoic marine sedimentary sequences that formed in a passive continental margin environment within northern India , is located between the Indus-Yarlung Zangbo Suture Zone (IYZS) and the HH (Figure 1(a)).
The sedimentary sequence in the NH records Late Precambrian to Devonian prerift, Carboniferous to Early Jurassic syn-rift and Middle Jurassic to Cretaceous passive continental margin sediments (Figure 1(b)) [66–68]. These sediments crop out in an EW and NWW trend and are predominated by the Precambrian Laguigangri Group and a series of Upper Triassic, Jurassic, Lower Cretaceous, and Quaternary sediments. The Laguigangri Group crops out in the core of the Yelaxiangbo dome and is composed of schist, gneiss, and migmatite units (Figure 1(b)). A set of Late Triassic-Early Cretaceous flysch formations deposit in neritic-bathyal environments and crop out across the NH. This set of formations are dominated by turbidite deposits and host the majority of the Au-Sb-Pb-Zn-Ag deposits in the NH. The lithology of these Late Triassic-Early Cretaceous flysch formations is weak-metamorphic slate that is intercalated with metamorphosed fine-grained sandstone, argillaceous limestone, micrite, and siliceous rock that is intercalated with volcanic rocks . Some quaternary sediments also occur in the central and southern area of the NH, which are composed of gravel, sand gravel, sandy loam, clay, and ice boulder.
The EW-trending and NS-trending faults, both with the several episodes of motion, are present in the NH. The EW-trending faults, controlling the distribution of intermediate-acid magmatic rocks and ore deposits in the NH , are older and cover a larger area than the NS-trending faults. The representative EW-trending faults include the Lazi-Qiongduojiang, Rongbu-Gudui, and Luozha faults as well as the STDS and numerous metamorphic core complexes (Figure 1(b)). A series of rifts that formed from 25 Ma to present are associated with these faults [29, 69–71], mainly including the Sangri-Cuona, Yadong-Gulu, Shenzha-Xietongmen, and Dangreyongcuo-Gucuo rift zones from east to west . In addition, the NS-trending faults that are considered as the result of east-west extension of the Qinghai-Tibet Plateau [73, 74] also formed during this period especially from 18 to 4 Ma [75, 76]. These NS-trending faults are also the important ore-controlling structures in the NH .
Magmatism in the NH primarily includes the Mesozoic and Cenozoic magmatism. The Mesozoic magmatism generated multiple suites of mafic-intermediate igneous rocks between the Late Triassic and the Early Cretaceous, including basaltic volcanic interlayers, dyke swarms, and subvolcanic dykes. According to the previous geochronological data, the SHRIMP U-Pb ages of the basic dyke swarms from different area in the NH are 134.9 ± 1.8 Ma, 135.5 ± 2.1 Ma , and 138.0 ± 3.5 Ma , respectively. The SHRIMP U-Pb age of the gabbro is 155.8 Ma . Tong et al. , Pan et al. , and Zhong et al.  regarded these basic dyke swarms as the result of late-stage massive expansion of Neo-Tethys Ocean under the structural environment of the Himalaya passive continental margin intensive stretching and breaking-off, lithosphere extension-thinning, and asthenosphere upwelling. On the contrary, Zhu et al.  and Qiu et al.  suggested that these basic dyke swarms are the result of interaction between mantle plume and lithospheric mantle material and form in the continental-rift environment. The Cenozoic magmatism is characterized by the formation of monzogranite, leucogranite, diorite, porphyritic diorite, and aplite units [84, 85]. These Cenozoic intermediate-acidic intrusive masses are distributed along the EW-trending faults and in the core of Ranba, Kangma, and Yelaxiangbo dome in the form of batholith, laccolith, and dykes (Figure 1(b)). This phenomenon is considered to be the result of crustal thickening  related to the collision of the India Plate and the Eurasia Plate during the postcollision stage (25 to 0 Ma) [87, 88].
The NHMB contains many Sb, Au, Sb-Au, Pb-Zn, and Sb-Pb-Zn-Ag deposits, and the Zhaxikang Sb-Pb-Zn-Ag, the Mazhala Au-Sb, the Chalapu Au, the Bangbu Au, the Shalagang Sb, the Cheqiongzhuobu Sb deposits are representative (Figure 1(b)) [7, 25]. The geneses and metallogenic age of these deposits are controversial due to the limited research, the genetic models mainly include the SEDEX overprinted by hot spring, carlin and carlin-like, hot spring, subvolcanic magmatic-hydrothermal fluid, and orogenic types .
2.2. Ore Deposit Geology
The Zhaxikang Sb-Pb-Zn-Ag deposit is located ~48 km west from Longzi County Town within the southeastern Yangzuoyong-Nariyong composite syncline in the NH (Figure 1(b)). This deposit has a reserve of 1.268 Mt Pb-Zn with a 3.66% average Zn grade and a 2.45% average Pb grade, 0.138 Mt Sb with an average grade of 1.08%, 1800 t Ag with an average of 99.55 g/t, 3.9 t associated Au, 361 t associated Ga, and 20 Mt Mn-Fe carbonate ores with an average grade of 42% for Fe + Mn , which makes it the largest deposit within the NHMB. The majority of mineralization in the orefield is hosted by the Lower Jurassic Ridang formation that consists of epimetamorphic marine clastic rocks. This formation, dipping shallowly to the north and striking eastwest, is divided into five lithologic sections (Figure 2(a)). A few Upper Jurassic Weimei formations composed of fine-grained metamorphic quartzose sandstone, silty slate, and calcarenite as well as Quaternary sediments distributed along valleys also crop out in the orefield (Figure 2(a)) .
The Zhaxikang deposit developed extensive geological structures. A near northsouth striking fault system is prevalent in the orefield, which coexists with a group of northeast-striking faults and some folds. Engineering and geological mapping projects have identified 16 faults, the majority of which are steeply dipping normal faults associated with tensional stress and wrench faults associated with torsional stress. Faults F2, F4, F5, F6, F7, F13, F14, and F16 are the main ore-bearing faults, faults F1 and F10 are partly mineralized, fault F3 was associated with late-stage mineralization, faults F8 and F9 are wrench faults without any mineralization, and fault F12 is a nonmineralized regional fault (Figure 2(a)). The orebodies I–VI are hosted by nearly NS-striking faults and orebodies VII–IX are hosted by nearly NE-striking faults (Figure 2). Our samples in this study are all from the orebody V, which is the largest and richest one among these orebodies within the orefield and hosts more than 80% of the reserves. This orebody is >1400 m long, 1 to 30 m wide, and controlled by fault F7 (Figure 2).
The magmatism in the orefield is associated with diabase, porphyritic rhyolite, basalt, and leucogranite units as well as some granite porphyry dykes that intruded into the porphyritic rhyolite (Figure 2(a)). The diabase is identified by drillholes and footrill in the central part of the orefield as dykes that emplaced into the Jurassic Ridang Formation and has been dated by zircon U-Pb methods to ~133 Ma . The rhyolite porphyry with the zircon SHRIMP U-Pb age of ~135 Ma crops out in the western part of the orefield  and the leucogranites crop out in the southern part of the orefield over an area of <1 km2. Additionally, the basalt usually occurs near the orebody in the form of consequent layer or shear layer distributed in slate and the contact region of slate and diabase.
Various types of alteration associated with mineralization have occurred in the orefield, including (1) the silicification that is associated with Sb mineralization and generally located in fault zones in the form of quartz veins, radiating quartz, and quartz druse; (2) the carbonatization that is associated with Pb-Zn mineralization in the form of Mn-Fe carbonate veins and also formed the postmineralization calcite; (3) the chlorite alteration that is generally confined to massive and stellated aggregates of chlorite within diabase; (4) the weak sericite alteration that is associated with chlorite alteration and barren quartz; and (5) the clay alteration that developed along the edges of fracture-related crushed zones. Furthermore, the ore-forming elements display a vertical sequence that is zoned from a lowermost Zn (Pb + Ag) zone through a central Zn + Pb + Ag-(Sb) zone to an uppermost Pb + Zn + Sb + Ag zone, although no horizontal zoning is present .
2.3. Ore Paragenetic Sequence
The paragenetic sequence in the Zhaxikang deposit is divided into six stages of ore formation based on the detailed hand specimen and microscopic observations. These six stages are assigned to two clear pulses: the first pulse consists of stages 1 to 2 and is characterized by the assemblages of Mn-Fe carbonates and sulfides, and the second pulse includes stages 3 to 6 and is primarily dominated by quartz, calcite, sulfosalt minerals, and sulfides (Figure 3).
Stage 1, dominated by a Mn-Fe carbonate + sphalerite + pyrite + arsenopyrite assemblage, is the initial stage of ore formation in the Zhaxikang deposit. Majority of the fine-grained sphalerite, pyrite, and arsenopyrite are hosted by fine-grained Mn-Fe carbonate in the form of laminae (Figures 4(a)–4(c)), and a few sulfides occur within the Mn-Fe carbonates as stellated aggregates (Figure 4(d)). The fine-grained layered and colloform with synsedimentary features (Figure 4(b)). The laminae and Mn-Fe carbonates in some samples have been cut by later stage 4 quartz-boulangerite veins (Figure 4(c)) or have been affected by the stage 2 coarse-grained sphalerite (Figure 4(a)).
Stage 2 hosts majority of the Pb-Zn mineralization in the Zhaxikang deposit and comprises an assemblage of Mn-Fe carbonate + galena + sphalerite + pyrite ± arsenopyrite. The more abundant and coarser-grained sulfides are hosted by coarse-grained Mn-Fe carbonate and slate to form the banded (Figure 4(k)), net-veined (Figure 4(i)), massive (Figure 4(h)), concentric annular (Figures 4(g) and 5), and Dal Matianite (Figure 4(l)) ores. The Mn-Fe carbonate during this stage recrystallized to different degree (Figures 4(f), 4(g) and 4(i)–4(k)), some even formed the druse containing the idiomorphic columnar quartz, needle-like boulangerite, or valentinite (Figure 4(j)). We can also observe that the later sphalerite replaces the earlier pyrite containing automorphic stage 1 arsenopyrite to form a skeletal texture during this stage (Figure 4(w)). Zheng et al.  considered that the ore textures in stages 1 and 2 are similar to those of the Red Dog SEDEX-type ore district in Alaska.
Stage 3, characterized by the formation of a quartz ± calcite + pyrite + sphalerite + galena ± chalcopyrite ± arsenopyrite assemblage without Mn-Fe carbonate, is the earliest stage of the second pulse of mineralization. The massive, veined, net-veined, and brecciated sphalerite, galena, and pyrite occur in the quartz and calcite (Figures 4(l)–4(p), 4(x)), and most of the sulfides form by the modification of sulfides from earlier stages. Some chalcopyrite grains are distributed in sphalerite, galena, and pyrite as stellated aggregates (Figures 4(y) and 4(z)). Some of these sulfides have been cross-cut by the later quartz-boulangerite or quartz-calcite veins (Figure 4(o)).
Stage 4 is marked by a mineral assemblage composed of quartz + antimony-lead-silver sulfosalt minerals (Figure 4(r)) that prevailingly include boulangerite and jamesonite, as well as minor bournonite, tetrahedrite, and andorite. This stage hosts the majority of the Sb and Ag mineralization and yields the ores with relatively high average Ag grades. The minerals formed in earlier stages are replaced and cross-cut by the quartz-boulangerite veins and boulangerite of this stage (Figures 4(c) and 4(aa)). Some samples also contain quartz druse filled with needle-like boulangerite (Figure 4(q)).
Stage 5 is distinguished by the formation of a quartz + stibnite + cinnabar assemblage and hosts part of the Sb mineralization within the deposit. Elongate-radial stibnite and massive stibnite-cinnabar are hosted by quartz (Figures 4(s) and 4(t)). Some stibnite cross-cut the stage 4 boulangerite (Figure 4(aa)).
Stage 6, representing the youngest stage of mineralization in the Zhaxikang deposit, is identified by a quartz ± calcite assemblage without sulfides. The quartz-calcite veins of this stage cross-cut the earlier formed minerals (Figures 4(o) and 4(ab)). Zheng et al.  regarded the ore textures in the second pulse of mineralization as typical hot spring type metallogenic features.
3. Sampling and Analytical Methods
The sampling points for EPMA and Fe-Zn isotopic analyses (the powders are sampled by microdrill) are all in the annular polished section samples 9-3, 9-8, ZXK-1, and ZXK-2. The specific numbers, locations, and photomicrographs of these sampling points are given in Figures 5 and 6, respectively. These four samples are all from the first pulse of mineralization, only the sample ZXK-2 has been cut by a stage 3 quartz vein (Figure 5(d)).
Chemical compositions of sulfide, Mn-Fe carbonate, and quartz were determined on a JEOL (Japan Electron Optics Laboratory) JXA-8100 electron microprobe (EMP) at the Second Institute of Oceanography, State Oceanic Administration of China. The accelerating voltage is 15 kV for Mn-Fe carbonate and quartz and 20 kV for sulfide, the beam current is 10 nA, the beam diameter is 1 μm, the secondary electronic resolution is 6 nm with the operating distance of 11 mm, and the repeat accuracy of the sample stage is within 1 nm. The standards are natural minerals and synthetic oxides as those of Sun et al. . The correction program supplied by the manufacturer is used for matrix corrections [91, 92].
3.3. Fe-Zn Isotopic Analyses
Approximately 10–50 milligrams of sample powders was placed in 15 ml Teflon jars and the solids were dissolved in 4 ml of heated ultrapure aqua regia. The solutions were dried and then Fe and Zn were purified using the BioRad MP-1 anion exchange resin using the protocol from Maréchal et al. . Yields from the columns were tested volumetrically on the ICP-OES at Pennsylvania State University and were all greater than 95%. Isotope values are reported in the traditional per mil values ().
The Fe isotopes were measured on the Neptune MC-ICP-MS at Pennsylvania State University. The instrument setup, sample introduction, and running conditions are discussed in greater detail in Yesavage et al. . Samples were diluted to a 3 ppm Fe solution which produced approximately a 10 V signal on the shoulder to the argon interference peak (56Fe and 16O). Sample intensities matched the intensity of the bracketing standard within 10%. Mass bias was corrected for by standard-sample-standard bracketing. In-house and international standards were measured throughout the sessions and yielded overlapping values of SRM-3126a δ56Fe = 0.33 ± 0.08, = 8 (accepted values δ56Fe = 0.34 ± 0.1 2σ) , and HPS-WU δ56Fe = 0.62 ± 0.11, = 8 (accepted values δ56Fe = 0.60 ± 0.07 2σ) . The samples are reported relative to the international standard IRMM-014 (δ56Fe () = ). Reported values are an average of two different measurements and the errors fall within the range 0.1 2σ of the standards.
The Zn isotopes were measured on Neptune MC-ICP-MS at Rutgers University. Correction of mass bias for Zn using Cu (NIST 976) was employed for these samples as suggested in [94–97] and the corrected values were then bracketed by the standards. The samples are reported relative to the newly developed Zn isotope standard (AA-ETH; δ66Zn () =  × 1000) and all the quoted data from previous literatures in this paper are converted relative to the AA-ETH standard (δ66) . We also compared the new standard relative to IRMM 3702 and obtained a δ66Zn = 0.03, which is within the error reported in Archer et al. . Solutions were kept at 100 ppb Cu and 150 ppb Zn which generated 63Cu = 7 V and 66Zn = 4 V. One block of 30 ratios is reported and the average error for the standard compared to itself throughout the session is 0.05 2σ.
All the EPMA data are given in Tables 1 and 2. The Mn-Fe carbonate contains 23.562~31.806 wt% Fe and 27.514~32.232 wt% Mn, with a negative correlation between Fe and Mn contents (Figure 7(a)), which indicates that the Mn-Fe carbonates form by the isomorphic substitution of Fe2+ and Mn2+ ions and have a molecular formula of (Mn0.5Fe0.5)CO3. The Fe contents are around 36 wt% for the arsenopyrite samples and 46 wt% for the pyrite samples. The sphalerite samples have 56.941~60.552 wt% Zn and 5.375~9.424 wt% Fe with a negative correlation between these two elements (Figure 7(b)).
4.2. Fe-Zn Isotopes
All the Fe-Zn isotopic data are given in Table 3. The annular polished section samples have δ56 of , with an average of −0.50 ± 1.09 (2SD, = 19), and δ66 of with an average of −0.25 ± 0.19 (2SD, = 12). The Mn-Fe carbonate and pyrite show the δ56Fe values range from −1.95 to −0.59 (average value of −0.97 ± 0.86; 2SD, = 8) and from −0.26 to 0.23 (average value of −0.07 ± 0.35; 2SD, = 9), respectively. The two arsenopyrite samples exhibit the δ56Fe values of −1.01 (ZXK-1-3; Figure 5(c)) and −0.18 (ZXK-2-2; Figure 5(d)).
In sample 9-3, the 9-3-1, 9-3-2 (Figure 6(a)), and 9-3-3 sphalerite have the δ66Zn values of −0.12, −0.23, and −0.31 with a gradually decreasing trend, the 9-3-4 and 9-3-5 Mn-Fe carbonate show the same trend with the δ56Fe values of −0.59 and −1.95, and the δ56Fe value of 9-3-7 pyrite is −0.26 (Figure 5(b)). Similarly, in sample 9-8, from 9-8-2 (−0.09; Figure 6(c)) through 9-8-5 (−0.23) to 9-8-3 (−0.35; Figure 6(d)), the δ66Zn values of sphalerite also present a gradually decreasing trend; meanwhile the δ56Fe values also decrease from −1.06 (9-8-8; Figure 6(b)) to −1.38 (9-8-9) for Mn-Fe carbonate and from 0.23 (9-8-4) to 0.09 (9-8-7) for pyrite, although the 9-8-1 sphalerite and 9-8-6 pyrite have the δ66Zn value of −0.17 and δ56Fe values of −0.26 (Figure 5(a)). In sample ZXK-1, the δ66Zn values of ZXK-1-3 (−0.18; Figures 6(f) and 6(m)) and ZXK-1-2 (−0.15; Figure 6(g)) sphalerite are almost the same and heavier than ZXK-1-1 (−0.38) sphalerite; the δ56Fe values for pyrite increase from ZXK-1-3 (−0.22) to ZXK-1-4 (0.12; Figure 6(e)) and ZXK-1-5 (−0.05); and, as for Mn-Fe carbonate, the ZXK-1-6 (−0.66) has heavier δ56Fe values than ZXK-1-7 (−0.78; Figure 5(c)). By contrast, in sample ZXK-2, the ZXK-2-1 (−0.32; Figure 6(h)) and ZXK-2-3 (−0.28; Figures 6(k) and 6(p)) sphalerite have almost the same δ66Zn values; the ZXK-2-7 (−1.06) and ZXK-2-8 (−1.04) Mn-Fe carbonate also yield approximate δ56Fe values; also the ZXK-2-5 (Figures 6(i) and 6(n)) and ZXK-2-6 pyrite show the similar δ56Fe values of −0.07 and −0.17 (Figure 5(d)).
5.1. The Fe-Zn Isotopic and Elemental Variations
Sample 9-3 with typical concentric annular texture has the gradually decreasing δ66Zn values of sphalerite and δ56Fe values of Mn-Fe carbonate from core to edge (early to late; Figure 5(b)). Similarly, sample 9-8 shows the same isotopic variation trend of pyrite, sphalerite, and Mn-Fe carbonate except the sulfides in the core (Figure 5(a)). As the core in 9-8 consists of crushed, earlier formed slate breccias and sulfides, the annular sulfides and Mn-Fe carbonate formed around the core, and thus this core is not included in the decreasing trend. In sample ZXK-1, as the laminae (ZXK-1-3; Figure 5(c)) is regarded as the earliest, the Fe-Zn isotopic values of sphalerite and Mn-Fe carbonate still present gradually decreasing trend from ZXK-1-3 (−0.18) to ZXK-1-1 (−0.38) and ZXK-1-6 (−0.66) to ZXK-1-7 (−0.78), respectively (Figure 5(c)), whereas the δ56Fe values of pyrite show the different variation, which might be related to the influence of Fe isotopic fractionation within pyrite-arsenopyrite-sphalerite mineral pair (Figures 6(f) and 6(m)). However, there is no similar decreasing Fe-Zn isotopic variation trend in sample ZXK-2, and the modification by the stage 3 quartz vein must be the main cause (Figures 5(d), 6(h)–6(l) and 6(n)–6(p)).
Previous studies [12, 62, 99] have proposed a Rayleigh distillation model to explain an increasing trend in δ66Zn values within precipitates over time for the hydrothermal fluid. This Rayleigh distillation model is as follows: the ore-forming materials derived from a single source would be subjected to kinetic Rayleigh fractionation that would lead to the early formed mineral precipitants being preferentially enriched in light isotopes, as well as residual fluids and later precipitants with heavier isotopic values, causing an increasing trend in isotopic values within precipitants over time. Several previous studies have used this distillation model to explain the Zn isotopic variation within different types of deposits (e.g., VHMS: ; Irish-type: [19, 100]; SEDEX: [20, 53]). Likewise, this Rayleigh distillation model is also applicable to the Fe isotopic variation in skarn deposits [21, 22]. However, the δ66Zn and δ56Fe values gradually decrease from early to late stages within Zhaxikang deposit, which cannot be explained by this distillation model. Another Rayleigh distillation mechanism models this decreasing trend: the metallogenic elements are transported by the ore-forming system consisting of vapour and liquid phases, and there is partitioning between vapour-liquid phases and the ratios change with the temperature decreasing. Then the minerals precipitate from the liquid phase of the ore-forming system. During this period, the vapour-liquid partitioning and mineral precipitation cause the Rayleigh fractionation, and this Rayleigh fractionation leads to the mineral precipitation being preferentially enriched in heavy isotopes relative to the ore-forming system. Thus, the isotopic values of subsequent minerals are lighter and lighter [101, 102].
This Rayleigh distillation model is supported by the following evidence: (1) The vapour-liquid partitioning and related isotopic fractionation for transition metal elements (e.g., Cu and Mo) have been confirmed by previous research in the Dahutang W-Cu-Mo ore field ; (2) minerals typically precipitate from the liquid phase; however, according to the previous literature , in unique cases the vapour phase containing metal can even directly condensate to form solid phases from high-temperature ore-forming system (e.g., VMS and volcano related system), which can demonstrate the existence of the vapour phase for metal elements. As for the Zhaxikang deposit, the theoretical calculated ore-forming temperature from Fe isotopic data is 500~800°C , and thus there should be a transitory high-temperature period, making the vapour-liquid partitioning possible; (3) the fluid inclusion data demonstrate that Mn-Fe carbonates and sulfides exist in three types of inclusions: ① gas-liquid two-phase water inclusions (W type, more than 90%), ② pure liquid inclusions (L type), and ③ pure CO2 inclusions (PG type)  from Zhaxikang deposit.
On the other hand, for sphalerite, there are positive correlations between Zn contents and δ66Zn values, with negative correlations between Fe contents and δ66Zn values in samples 9-8 (Figure 5(a)), 9-3 (Figure 5(b)), and ZXK-1 (Figure 5(c)), respectively. Moreover, plotting all the data from these three samples on a diagram together, the correlations are also good with > 0.6 (Figures 7(c) and 7(d)). Zinc and iron usually show similar geochemical behaviour as both of them are highly mobile in chloride-bearing hydrothermal fluids [23, 100]. Thus, the Zn2+ and Fe2+ ions are preferentially enriched in the liquid phase relative to the vapour phase before precipitation [23, 100], which cause the decreasing Zn contents of sphalerite over time. As the total content of Zn2+ and Fe2+ is constant in sphalerite, the Fe contents of sphalerite gradually increase with the decreasing Zn contents. These correlations further support the hypothesis that the ore-forming system is the mixture of vapour and liquid phases. In addition, the sample ZXK-2 cut by a later stage 3 quartz vein does not present the same correlations and variations, which is a new evidence for two pulses of mineralization proposed by Zheng et al.  and Wang et al. .
All of the evidence above reveals that the ore-forming elements are transported by the ore-forming system that consists of vapour and liquid phases. The vapour-liquid partitioning and mineral precipitation are the main cause of Fe-Zn isotopic and elemental variations. Afterwards, the overprint by the second pulse of mineralization has also partly modified the Fe-Zn isotopic and elemental compositions of some earlier samples (Figure 5(d)) .
5.2. The Fe-Zn Isotopic Fractionation Models for the Ore-Forming System
In order to verify the Rayleigh distillation model in Section 5.1 and obtain more information of the ore-forming system, we use the following equations to establish Fe-Zn isotopic fractionation models for the ore-forming system and mineral precipitation:, , and are the δ56Fe-δ66Zn values of momentary mineral precipitation and momentary and initial ore-forming system, respectively; , , and are the isotopic fractionation factors between ore-forming system and mineral precipitation that refer to the momentary condensation temperature , the initial temperature of ore-forming system , and , respectively; and is the fraction of remaining ore-forming system that consists of vapour and liquid phases [102, 105]. In addition, the equations for fractionation factors are approximately using ln for Fe  and ln for Zn ( is absolute temperature in K) .
Wang et al.  have calculated the ore-forming temperature (500~800°C) of the first pulse of mineralization in Zhaxikang deposit using the Fe isotopic fractionation between pyrite and Mn-Fe carbonate. Although this temperature range is a little wide, the highest temperature of such ore-forming system can reach around 500°C according to the previous ore deposit studies [6, 22, 23]; hence we regard 500°C as the initial temperature of the ore-forming system. The homogenization temperature (240°C) of the fluid inclusions  from the first pulse of mineralization in Zhaxikang deposit is considered as the momentary condensation temperature. Furthermore, for the purpose of making the fractionation models more comprehensive and exact, we also quote the Fe-Zn isotopic data of pyrite (δ56Fe: stage 1: −0.33 to −0.09; stage 2: −0.30 to 0.19; stage 3: 0.16 to 0.43), sphalerite (δ66Zn: −0.31 to 0.07), and Mn-Fe carbonate (δ56Fe: −0.80 to −0.55; δ66Zn: −0.11 to 0.04) from Wang et al. , as well as the δ66Zn values of sphalerite (−0.25 to 0.03) and Mn-Fe carbonate (−0.01) from Duan et al. . Finally, we set up 12 Fe-Zn isotopic fractionation models for pyrite, sphalerite, and Mn-Fe carbonate (Figure 8) with different δ56Fei values of 0 (mean value of magma) , −0.5, and −1, as well as δ66 values of −0.28 (the lightest value of seafloor hydrothermal fluids) , 0 (mean value of bulk earth) , and 0.23 (the mean value of deep sea water) [63, 108, 109].
These fractionation models show that the ranges for ore-forming system highly depend on the values (Figure 8). The details are as follows: the pyrite covers the ranges of (δ56Fei = 0; Figure 8(a)), (δ56Fei = −0.5; Figure 8(b)), and more than 77.7% (δ56Fei = −1; Figure 8(c)). The ranges for sphalerite are (δ66Zni = −0.28; Figure 8(d)), (δ66Zni = 0; Figure 8(e)), and (δ66Zni = 0.23; Figure 8(f)), respectively. In comparison, the Mn-Fe carbonates has the ranges of (δ56Fei = 0; Figure 8(g)), (δ56Fei = −0.5; Figure 8(h)), and (δ56Fei = −1; Figure 8(i)) for Fe isotope, as well as (δ66Zni = −0.28; Figure 8(j)), (δ66Zni = 0; Figure 8(k)), and (δ66Zni = 0.23; Figure 8(l)) for Zn isotope. All of these results suggest that the Fe-Zn isotopic data of Zhaxikang deposit fit these Rayleigh fractionation models well.
However, we need to consider the following facts in the Zhaxikang deposit: (1) the second pulse of mineralization has brought some Fe to form the stage 3 pyrite with heavier δ56Fe values () ; thus the stage 3 pyrite does not fit the fractionation models; (2) as most of the sphalerite and pyrite are paragenetic during the first pulse of mineralization (Figures 4(g), 4(i), 4(k), 5(a)–5(c) and 6(c)), especially in the earliest lamina (Figures 4(a)–4(c), 5(c), 6(f) and 6(m)), the sphalerite and pyrite should overlap on ranges; (3) in theory, the Mn-Fe carbonates would have the same range for Fe-Zn isotopes. Nonetheless, in view of the tight Zn isotopic variation range, the range for Fe isotope should cover that for Zn isotope; (4) during the earlier period, as the ore-forming system consisting of vapour and liquid phases is dominant, values in fractionation models should be large. Taking all these facts and 12 fractionation models into consideration, the δ56Fei value is supposed to be in the range of −1, and the δ66 value should be between −0.28 and 0.
5.3. Implications for the Genesis of Zhaxikang Deposit
5.3.1. Excluding the Possibility of Hot Spring Genetic Model
The hot spring model predicts that metals (e.g., Zn, Pb, Sb, Ag, and Fe) are leached from sedimentary wall rocks, which is supported by the following evidence: (1) the δ34S values of the sulfides () are similar to those of sedimentary wall rocks (); (2) the δ30Si values of quartz (−0.40) are the same as those of siliceous rocks with hot spring genesis; (3) the (−127) and δ18 values () of fluid inclusions trapped in quartz are similar to those of the south Tibetan hot spring; (4) the Pb isotopes (: 18.474~19.637; : 15.649~15.774; : 39.660~40.010) show the characteristics of radiogenic Pb; (5) the He-Ar isotopes demonstrate the contribution of crustal fluid and meteoric water [3, 4].
However, this genetic model is inconsistent with textural and Fe-Zn isotopic evidence presented here. Firstly, the primary sedimentary wall rocks in the orefield are slate. As suggested by the continuous batch experimental research of Fernandez and Borrok , the ore-forming fluid would preferentially leach out the heavy Zn isotopes. Likewise, Chen et al.  have analyzed the Zn isotopic compositions of samples from 8 hot springs, and the results show most of the hot springs have relatively constant and heavier δ66Zn values (approximately 0.42) than host rocks (−0.42 to 0.14). Therefore, if the metallogenic elements are leached from the slate by hot spring, there would be some sphalerite with heavier δ66Zn values than these slates in Zhaxikang deposit. Nevertheless, the δ66Zn values of the slate from Zhaxikang orefield range from −0.23 to 0.10 that are similar to sphalerite, especially the unmodified slate sample with the δ66Zn value of 0.10 that is even a little heavier than that of sphalerite (−0.38 to 0.07; Figure 9(b)) . As the slate has heavier Zn isotopic compositions than those of host rocks from Chen et al. , the δ66Zn values of the hot spring in Zhaxikang orefield would even be heavier than 0.42, which are much heavier than the δ66Zni values () of the fractionation models in Section 5.2. Secondly, Sharam et al.  have measured the δ56Fe values (−0.59 to −0.12) of hot springs in Juan de Fuca Ridge, which is much heavier than the δ56Fei value (−1) gained from the fractionation models. Moreover, the marine fluids usually have lighter Fe isotopic compositions (Figure 9(a)); thus the hot springs in Tibet would have heavier δ56Fe values than those of Sharam et al. .
The possibility of hot spring genesis for the first pulse of mineralization event can be excluded by Fe-Zn isotopic data. Evidence for the second pulse of mineralization is based on the fact that the Fe-Zn isotope values do not follow similar concentric patterns with the ore textures as seen in sample ZXK-2. Meanwhile, the evidence from Si-H-O isotopes demonstrates that the second pulse of mineralization may be related to hot spring. Additionally, the Fe-Zn isotopic data demonstrate that the sedimentary wall rocks have not provided significant amounts of metals, although the S-Pb isotopic data show that these wall rocks constitute some contribution for S-Pb [4, 5], whereas the similar Zn isotopic compositions of slate and sphalerite suggest that they share the same Zn origin.
5.3.2. Inconsistency with the Magmatic-Hydrothermal Fluid Genetic Models
There are two genetic models for the magmatic-hydrothermal fluid genesis. In the first model, Duan et al.  considered that the genesis of Zhaxikang deposit relates to the mid-low temperature magma-related hydrothermal activity and that the metallogenic elements are mainly sourced from the mixing of basement and the sedimentary wall rocks. The evidence is mainly from the Zn-S-Pb isotopes that we mentioned in Section 1.
Duan et al.  have analyzed the δ66Zn values of the sulfides () and basement rocks (). The dominating sedimentary wall rocks in the orefield are slate (δ66Zn values: ) , which is formed by the epimetamorphism of shale and sandstone. Meanwhile, combining the data from Wang et al.  with this study, the sphalerite should have a range from −0.38 to 0.07 in Zhaxikang deposit. Both the basement and sedimentary wall rocks have heavier Zn isotopic compositions than sphalerite in Zhaxikang deposit. However, just like we discussed in Section 5.3.1, if the Zn is sourced from mixing of the basement and sedimentary wall rocks, there should be some sphalerite with heavier δ66Zn values than these rocks. This inference is also evidenced by the research of Zhou et al. : the Paleozoic carbonate host rocks and Precambrian basements are considered to be the origin of metals, and these rocks have lighter δ66Zn values (−0.52 to 0.16) than the sphalerite from the Tianqiao (−0.54 to 0.30) and Bangbangqiao (−0.21 to 0.43) deposits in the Sichuan-Yunnan-Guizhou Pb-Zn metallogenic province (Figure 9(b)). Additionally, in respect of the Fe isotope, the Schwarzwald hydrothermal vein deposit in Germany can be used as an analogy . Iron in this deposit originates from the basement consisting of granites and gneisses, as well as sedimentary rocks including shale and sandstone. The basement of Zhaxikang is composed of dolerite, quartz diorite, rhyolite porphyry, pyroclastics, and porphyritic monzogranite , and these crust-derived igneous rocks have the similar Fe isotopic composition with granites according to the data from previous studies [21–23, 28, 36–45]. Likewise, the δ56Fe values of shale and sandstone in the Schwarzwald deposit are −0.21, 0.03, and 0.22, all of which fall into the Fe isotopic variation range of shale () from Beard et al.  and Rouxel et al. . Therefore, we regard the fact that the metal-sourced rocks in these two deposits have the similar Fe isotopic compositions. And, yet, Markl et al.  suggested that fluid-rock interaction make the ore-forming fluid have the δ56Fe value of , which is heavier than the δ56Fei value (−1) of the fractionation models in Section 5.2. Furthermore, it is generally known that the equilibrium isotope fractionation is a function of temperature, with larger fractionation generated at lower temperatures . Although the temperature of ore-forming fluid (100~200°C)  in the Schwarzwald deposit is lower than that in Zhaxikang deposit (~250°C) , the lightest δ56Fe value (−1.36) of siderite from this deposit is much heavier than that of Mn-Fe carbonate (−1.95) from Zhaxikang deposit (Figure 9(a)). All of these inconsistencies from Fe-Zn isotopic data indicate that this genetic model is not appropriate for Zhaxikang deposit.
In the second genetic model, Xie et al.  suggested the mineralization in Zhaxikang deposit was genetically related to the Miocene dome-related magmatism. This magmatism generated the pegmatite and two-mica granite in the core of the regional domes (Figure 1(b); e.g., Cuonadong, Yalaxiangbo, Ranba, and Kangma), and the high-temperature ore-forming fluids were derived from magmatic melts exsolution. This hypothesis is based on the research of field geology, petrography, melt and fluid inclusions, and C−H−O isotopes: (1) the δ13 (−6.9) and (+11.8) values of rhodochrosite show the mantle origin; (2) the δ13 ( −110) and δ18 (−8.89) values, the low salinity (0.2~7.9 wt.% NaCleqv), high temperature (298~457°C), and rich CO2 content with minor CH4, N2, C2H6, C3H8, and C6H6 of the melt and fluid inclusions trapped in quartz and beryl within pegmatite indicate the magmatic origin; (3) the 40Ar-39Ar plateau age of pegmatite (18.93 ± 0.27 Ma) is similar to stage 5 quartz-pyrite-stibnite (17.9 ± 0.5 Ma).
The pegmatite and two-mica granite in the domes have the typical characteristics of S-type granite: (1) containing abundant Al-rich minerals, A/CNK: 1.07~1.24; (2) w(SiO2): , w(K2O)/w(Na2O): 1.1~1.2, w(FeO)/w(Fe + Mn): 0.64~0.76; (3) the content of corundum molecules > 1% in the CIPW standard minerals [112, 113]. Meanwhile, based on the facts that all the Fe-bearing minerals in Zhaxikang deposit are ferrous, and the magmatic-hydrothermal fluid is CO2-rich with minor CH4, N2, C2H6, C3H8, and C6H6 , and the parent magma is most likely S-type reduced magma. In consideration of the situation in the Renison Sn-W deposit that we mentioned in Section 1, the ore-forming fluid is considered to exsolve from S-type reduced magma and the sulfides have heavier Fe isotopic compositions than ore-related igneous rocks . The case in Zhaxikang deposit is contrary yet the pyrite from the first pulse of mineralization has the δ56Fe value of that is much lighter than those of granitoids (−0.08% to 0.59%) [22, 28]. Moreover, Heimann et al.  proposed that we would not expect Fe isotopic compositions of high F/Cl magmatic/hydrothermal systems to significantly deviate from the average of igneous rocks, hence as Xie et al.  considered that the Zhaxikang parent magma has high F contents, the magmatic-hydrothermal fluid in this genetic model would have the similar Fe isotopic compositions with granitoids, which is not in line with our fractionation models. Even if the parent magma in Zhaxikang orefield is oxidized-type and is similar to the magma related to I-type granitoids with δ56Fe values of in Tongling ore district (Figure 9(a)) [21, 22], it is still hard to produce so light δ56Fei value (−1). Similarity, Zn isotopic data do not support this genetic model, either. Chen et al.  studied the Zn isotopic fractionation during igneous process and suggested that the maximum Zn isotopic variation induced by high-temperature igneous processes is no larger than δ66Zn~0.10%. Besides this, Telus et al.  measured the δ66Zn values of pegmatite () and some other granitoids () and then found there is even no variation in δ66Zn values during fluid exsolution in some cases. As the granitoids in the regional domes are principally dominated by pegmatite and the magmatic fluids which have high temperature of 298~457°C , it is also hard to generate δ66Zni value between −0.28 and 0 as yielded from the Fe-Zn isotopic fractionation models. Consequently, the Fe-Zn isotopic data are also not in favor of the second genetic model.
On the other hand, neither of these two genetic models can explain the different Fe-Zn isotopic and elemental variations in sample ZXK-2, which is considered to result from the overprint by the second pulse of mineralization. Overall, all of the Fe-Zn isotopic and elemental evidences are inconsistent with both of these magmatic-hydrothermal fluid genetic models. Nevertheless, the evidence for these two genetic models may prove that the second pulse of mineralization is related to magmatic-hydrothermal fluids.
5.3.3. Constraints on SEDEX Modified by Hydrothermal Fluid Genetic Model
Zheng et al. [7, 25] considered that the first pulse of mineralization (Pb-Zn) has the SEDEX genesis, and the second pulse of mineralization (Sb-Ag) is related to hot spring that overprints the earlier mineralization. The previous evidences are mainly as follows: (1) the evidence from ore textures and obviously late Sb mineralization compared to Pb-Zn mineralization in Section 2.3; (2) the stage 1 and 2 ores have high Mn, Fe, Ba, and B contents, Ga In (Ga/In: 1.49~4.47), Pb + Zn Cu, and host rocks are exhalative rocks and Mn-Fe carbonates; (3) the δ34S values of sphalerite and galena () are different from those of stibnite (); (4) the data from valentinite (δ30Si values: −0.4) and fluid inclusions trapped in quartz (: −142, δ18: −1.9, homogenization and freezing temperatures: 164~313°C and −3.2−0.7°C, salinity: , and density: 0.74~0.93 g/cm3) both demonstrate the Sb mineralization is related to the south Tibetan hot spring; (5) the Rb-Sr isotopic isochrone age of stage 2 sphalerite is 147.2 ± 3.2 Ma that is similar to the Jurassic sedimentary wall rocks, whereas a later stage quartz-pyrite-stibnite vein has the - plateau age of 17.9 ± 0.5 Ma.
Wen et al.  investigated several Pb-Zn deposits with different geneses in China, and the results show that the Zn/Cd ratios of sphalerite vary with different geneses: (1) high-temperature systems including the porphyry, magmatic hydrothermal, skarn, and volcanic hosted massive sulfide (VMS)-type deposits: 155~223; (2) low-temperature systems that include the Mississippi Valley-type (MVT) deposits: 17~201; (3) SEDEX-type deposits of exhalative systems: 316~368; (4) seafloor hydrothermal sulfides of exhalative systems: 211~510. According to the EPMA data, the Zn/Cd ratios of sphalerite range from 296 to 399 in Zhaxikang deposit, which overlap the range of exhalative systems and much higher than those of high-temperature and low-temperature systems.
The Fe-Zn isotopic data also conform to the SEDEX modified by hydrothermal fluid genetic model. Firstly, as discussed in Sections 5.3.1 and 5.3.2, neither the hot spring nor the magmatic-hydrothermal fluids can have the δ56Fei () and δ66Zni () values to satisfy the Fe-Zn isotopic fractionation models. However, the Fe-Zn isotopic compositions of seafloor hydrothermal fluid system covers the range of for Fe isotope and for Zn isotope according to previous studies (Figure 9) [38, 46–49, 62], which can generate the ore-forming system with δ56Fei and δ66Zni values to meet the fractionation models. Secondly, although there are large overlaps in Zn isotopic compositions among deposits with different geneses, the Zn isotopic compositions of Zhaxikang deposit is most similar to the Alexandrinka VHMS-type and Red Dog SEDEX-type deposits with marine origin, as well as obviously distinguishing from the narrow range of magmatic-hydrothermal deposits (Figure 9(b)). Thirdly, the lightest δ56Fe value in Zhaxikang deposit is −1.95, and only the minerals with marine origin (mid-oceanic ridges pyrite) or SEDEX genesis (sphalerite and pyrrhotite in Dongshengmiao SEDEX-type deposit) can have so light δ56Fe values (Figure 9(a)). Fourthly, under the conditions of high and low PH (<8), the Zn precipitated as sulfides is isotopically nearly unfractionated with respect to the parent hydrothermal fluid, whereas, under the conditions of high and high-PH (>9), negative δ66Zn values down to 0.6 can be expected in sulfides precipitated from hydrothermal fluid . In Zhaxikang deposit, would be high as there are plenty of Mn-Fe carbonates; meanwhile, owing to the facts that the modern seawater has the PH around 8 and there is more CO2 in Jurassic atmosphere than present, the Jurassic seawater would have a lower PH than modern seawater. This can well explain that the δ66Zn values of sphalerite () slightly fractionate with the ore-forming system (δ66Zni value: ). Besides these, the overprinting of earlier ores by second pulse of mineralization is not only proved by the different Fe-Zn isotopic and elemental variations in sample ZXK-2 from the other 3 samples in this research (Figure 5) but also evidenced by the temporally increasing δ56Fe and decreasing δ66Zn values recorded in this deposit that coincided with an increase in alteration . Nevertheless, further research is required to confirm whether this hydrothermal fluid is hot spring or magmatic-hydrothermal fluid.
To sum up, among the various genetic models, the Fe-Zn isotopic and EPMA evidence indicate the SEDEX modified by hydrothermal fluid genetic model is the most plausible. Our research also demonstrates that the Fe-Zn isotopes have the potential to trace the metal source and provide insights into ore-forming processes.
The EPMA and Fe-Zn isotopic data allow us to make the following conclusions:(1)The ore-forming elements are transported by the ore-forming system that is the mixture of vapour and liquid phases; the vapour-liquid partitioning and mineral precipitation are the main cause of Fe-Zn isotopic and elemental variations.(2)The Fe-Zn isotopic fractionation models demonstrate that the δ56Fei and δ66Zni values of the ore-forming system are in the range of − and −0.28~0, respectively.(3)Based on the evidence from the EPMA data, Fe-Zn isotopic characteristics, and fractionation models, the SEDEX modified by hydrothermal fluid genetic model is most plausible for the Zhaxikang deposit.(4)There are two pulses of mineralization in the Zhaxikang deposit; the overprint by the second pulse of mineralization has also partly modified the Fe-Zn isotopic and elemental compositions of some earlier samples.
Conflicts of Interest
The authors declare that they do not have any commercial or associative interest that represents conflicts of interest in connection with the submitted work.
This work was carried out while Da Wang was a visiting student at the Juniata College. The authors would like to thank Matthew Gonzalez (Pennsylvania State University) and Linda Godfrey (Rutgers University) for aid in measuring and access to the Neptune instruments. They acknowledge support from the Program for Changjiang Scholars and Innovative University Research Teams (IRT14R54, IRT1083), the Commonwealth Project from the Ministry of Land and Resources (201511015), and the Fundamental Research Funds for the Central Universities (2652015044 and 2652015354).
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