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Article

Skarn Formation and Zn–Cu Mineralization in the Dachang Sn Polymetallic Ore Field, Guangxi: Insights from Skarn Rock Assemblage and Geochemistry

1
School of Earth Science and Resources, Chang’an University, Xi’an 710054, China
2
Laboratory of Mineralization and Dynamics, Chang’an University, Xi’an 710054, China
3
MNR Key Laboratory of Metallogeny and Mineral Assessment, Institute of Mineral Resources, Chinese Academy of Geological Sciences, Beijing 100037, China
4
Northwest Bureau of China Metallurgical Geology Bureau, Xi’an 710119, China
5
Guangxi 215 Geological Team Co., Ltd., Liuzhou 545002, China
*
Authors to whom correspondence should be addressed.
Minerals 2024, 14(2), 193; https://doi.org/10.3390/min14020193
Submission received: 11 January 2024 / Revised: 8 February 2024 / Accepted: 10 February 2024 / Published: 12 February 2024

Abstract

:
The Dachang is a world-class, super-giant Sn polymetallic ore field mainly composed of Zn–Cu ore bodies proximal to the granitic pluton and Sn polymetallic ore bodies distal to the granitic pluton. In this study, we used petrographic studies and major and trace element geochemistry with calc-silicates from the Zn–Cu ore bodies to constrain the physicochemical conditions of hydrothermal fluids during skarn rock formation and the evolution of ore-forming elements. Two skarn stages were identified based on petrographic observations: Prograde skarn rocks (Stage I), containing garnet, vesuvianite, pyroxene, wollastonite, and retrograde skarn rocks (Stage II), containing axinite, actinolite, epidote, and chlorite. The retrograde skarn rocks are closely associated with mineralization. The geochemical results show that the garnets in the Dachang ore field belong to the grossular–andradite solid solution, in which the early generation of garnet is mainly composed of grossular (average Gro72And25), while the later generation of garnet is mainly composed of andradite (average Gro39And59); the vesuvianites are Al-rich vesuvianites; the pyroxenes form a diopside–hedenbergite solid solution with a composition of Di3–86Hd14–96; the axinites are mainly composed of ferroaxinite; and the actinolites are Fe-actinolite. The mineral assemblage of the skarn rocks indicates that the ore-forming fluid was in a relatively reduced state in the early prograde skarn stage. As the ore-forming fluid evolved, the oxygen fugacity of the ore-forming fluid increased. During the final skarn stage, the ore-forming fluid changed from a relatively oxidized state to a reduced state. The skarn rocks have evolved from early Al-rich to late Fe-rich characteristics, indicating that the early ore-forming fluid was mainly magmatic exsolution fluid, which may mainly reflect the characteristics of magmatic fluids, and the late Fe-rich characteristics of the skarn rocks may indicate that the late hydrothermal fluid was strongly influenced by country rocks. Trace element analyses showed that the Sn content decreased from the prograde skarn stage to the retrograde skarn stage, indicating that Sn mineralization was not achieved by activating and extracting Sn from prograde skarn rocks by hydrothermal fluids. The significant enrichment of Sn in the magmatic hydrothermal fluid is a necessary condition for Sn mineralization. There are various volatile-rich minerals such as axinite, vesuvianite, fluorite, and tourmaline in the Dachang ore field, indicating that the ore-forming fluid contained extensive volatiles B and F, which may be the fundamental reason for the large-scale mineralization of the Dachang ore field.

1. Introduction

Skarn deposits are one of the most important ore types in the Earth’s crust and have been mined for a variety of metals, such as Cu, Fe, Mo, Zn, W, Sn, and Au, and mainly occur at the contact zone between intermediate–acidic intrusions and carbonate rocks. The interactions between the hydrothermal fluids and the country rocks have produced a sequence of skarn rocks that record the migration directions of the hydrothermal fluids and the evolution of mineralization during the formation of the skarn deposits. They are an ideal model for studying element migration in hydrothermal fluids [1,2,3,4,5].
The Dachang in Guangxi is a world-class, super-giant Sn polymetallic ore field, mainly composed of Zn–Cu ore bodies proximal to the granitic pluton and Sn polymetallic ore bodies distal to the granitic pluton, with Sn reserves of over 1 million tons (average grade 1%) and Zn reserves of 4.5 million tons (average grade 4%), accompanied by Cu, Pb, Sb, As, In, and Ge [6]. The Zn–Cu ore bodies mainly occur in the central part of the ore field and the deep part of Changpo–Tongkeng adjacent to the granitic pluton. The Sn polymetallic ore bodies mainly occur in the western and eastern parts of the ore field distal to the granitic pluton. Numerous isotopic geochronology studies have shown that the mineralization ages of the Sn polymetallic and Zn–Cu ore bodies were consistent with the emplacement age of the Longxianggai granitic pluton [7,8,9,10,11,12,13,14]. Previous researchers have carried out extensive studies here, but the focus of previous work has mainly been on the genesis of deposits, emplacement ages of granitic pluton, metallogenic age and isotopic studies, etc. [7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22,23,24]. However, mineralogical research, especially systematic studies of skarn rock petrography and geochemistry, is still relatively weak, which restricts the improvement of deposit models and in-depth understanding of skarn mineralization.
Based on previous studies, detailed petrographic observations and major element analyses were carried out on prograde skarn rocks (garnet, wollastonite, vesuvianite, pyroxene) and retrograde skarn rocks (axinite, actinolite, epidote), and representative skarn minerals (garnet, axinite) from different stages were selected for trace element analyses to constrain the physicochemical conditions of the hydrothermal fluids during skarn rock formation and the evolution of ore-forming elements.

2. Geological Setting

The Dachang ore field is located in the central part of the important non-ferrous metal mineralization belt in China, the Danchi metallogenic belt, at the junction of the Paleo-Tethys tectonic domain and the Pacific tectonic domain (Figure 1). The outcropping strata in the study area are mainly composed of Devonian mudstone, marl, and siliceous rocks, with a small amount of Carboniferous limestone. Among them, the Devonian strata are the main host rocks of the deposit [15,22]. The lithology, from bottom to top, is as follows: Black mudstone, shale and reef limestone in the lower part of the middle Devonian Nabiao Formation ( D 2 2 nb); thick stratiform limestone, black mudstone and shale of the Luofu Formation ( D 2 2 l) in the upper part of the middle Devonian, with locally lenticular carbonaceous pitch; banded siliceous rocks with calcareous nodules of the Liujiang Formation ( D 3 1 l) in the lower part of the upper Devonian; limestone of the Wuzhishan Formation ( D 3 2 w) in the middle part of the upper Devonian, which can be further divided into four sublayers from bottom to top: thick-striped limestone ( D 3 2 wa), thin-striped limestone ( D 3 2 wb), small lenticular limestone ( D 3 2 wc) and large lenticular limestone ( D 3 2 wd); carbonate rocks and shale of the Tongchejiang Formation ( D 3 3 t) in the upper part of the upper Devonian; and quartz sandstone, mudstone and carbonaceous shale of the Simen Formation (C1s) in the lower Carboniferous (Figure 2).
The structures in the ore field are mainly composed of the NW-trending Danchi and Dachang faults and anticlines, overlain by the later NE- and SN-trending folds, faults, and fractures [6].
Magmatic activity in the Dachang ore field is relatively active, and granitic plutons are less exposed on the surface and mainly occur as concealed plutons. The Longxianggai granitic pluton is the main magmatic intrusion in the study area, which crops out in the central part of the Dachang ore field, and it extends westward to the Changpo–Tongkeng deposit in the deep part [7]. The granitic pluton is mainly composed of medium- to coarse-grained biotite granite, fine-grained granite, and porphyritic biotite granite, with a gradual spatial transition relationship. The zircon U–Pb isotopic chronology of the Longxianggai granitic pluton ranges from 96.6 to 88.8 Ma [7,10,14,18]. In the eastern and western parts of the Changpo–Tongkeng, SN-trending granite porphyry and diorite porphyrite dikes intruded between 91.0 and 85.8 Ma [14,18].
The Dachang ore field is divided into three zones surrounding the Longxianggai granite. The western zone is represented by the Changpo–Tongkeng and Bali–Longtoushan Sn polymetallic deposits, while the central zone mainly includes the Lamo Zn–Cu and Chashan W-Sb deposits. There are some small- and medium-sized Sn polymetallic deposits in the eastern zone (such as Dafulou, Huile, and Kangma).

3. Geology of the Deposit

The Sn polymetallic deposit is the largest and most representative deposit in the Dachang ore field, mainly consisting of stratiform and vein-shaped ore bodies. The ore minerals are mainly composed of cassiterite, pyrite, sphalerite, pyrrhotite, arsenopyrite, and jamesonite, with complex mineral assemblages. The gangue minerals are quartz, calcite, and tourmaline.
The size of the W-Sb deposit is smaller than that of the Zn–Cu and Sn polymetallic deposits, which mainly consist of vein-shaped ore bodies. The mineral assemblages are simple and consist mainly of stibnite, wolframite, and scheelite. The gangue minerals are calcite, fluorite, and quartz.
The skarn Zn–Cu deposit mainly consists of the Lamo Zn–Cu deposit in the central part of the Dachang ore field and the lower part of the Changpo–Tongkeng deposit in the western part adjacent to the granitic pluton (Figure 3).

3.1. Lamo Zn–Cu Deposit

The Lamo Zn–Cu deposit is located at the contact zone between the outcrop of the Longxianggai granite and the upper Devonian striped limestone and small lenticular limestone in the central part of the Dachang ore field. It consists of gently dipping stratiform-like ore bodies and steeply dipping vein-shaped ore bodies. Among them, the gently dipping stratiform-like ore bodies are the main industrial ore bodies. The stratiform-like ore bodies are conformable with the host rock, with a strike of NNW, dipping NE, and the dip angle is relatively gentle, which mainly includes the No. 0, No. 1, and No. 3 ore bodies. The No. 0 ore body is the largest, with a strike length of 1365 m and an average thickness of 3.81 m. The No. 1 ore body extends for 130 m along strike and 4.32 m in depth. The No. 3 ore body extends for 80 to 160 m along strike, with an average thickness of 10.33 m. The vein-shaped ore bodies crop out in the cutting layer, with a strike of 15° to 25° and a dip of 285° to 295°. The dip angle is relatively steep, and mineralization is mainly characterized by filling and metasomatism along fractures, mainly including the No. 11, No. 12, No. 13, and No. 14 ore bodies. The ore bodies are large in size and stable in extension [25].

3.2. Lower Part of the Changpo–Tongkeng Deposit

The Zn–Cu ore bodies crop in the contact zone between the concealed Longxianggai granitic pluton and the calcareous mudstone and marl of the middle Devonian Luofu Formation ( D 2 2 l). There are three roughly parallel stratiform ore bodies, No. 94, No. 95, and No. 96 (Figure 4), with ore bodies striking 58° to 65° and dipping 328° to 335° [16]. The No. 94 ore body extends for 140 to 400 m along strike and 0.52 to 20 m in depth. The No. 95 ore body extends for 1500 m along strike and 0.66 to 31.76 m in depth. The No. 96 ore body has a strike length of 2235 m and an average thickness of 8.74 m.
The mineral assemblage of the Zn–Cu ore bodies includes sphalerite, chalcopyrite, arsenopyrite, pyrrhotite, and pyrite, while the gangue minerals are mainly calc-silicates, fluorite, calcite, quartz, and tourmaline. Massive and disseminated structures predominate, forming zoning, subhedral–anhedral and exsolution textures.
The host rock proximal to the granitic pluton has undergone thermal metamorphism to form marble and hornfels and metasomatism to form skarns. Skarnization is closely related to mineralization and is a prospecting indicator. Based on mineralogical characteristics and mineral assemblages, the skarn can be divided into two stages. The prograde skarn stage (stage I) is dominated by garnet, vesuvianite, pyroxene, and wollastonite, while the retrograde skarn stage (stage II) is dominated by axinite, actinolite, epidote, chlorite, and other hydrated silicate minerals. The retrograde skarn stage is intimately related to mineralization.
Based on the spatial distribution, occurrence characteristics, and mineral assemblages, the skarn Zn–Cu mineralization can be divided into two stages and four sub-stages (Figure 5). These stages include the skarn stage and the sulfide stage.

4. Sampling and Analytical Methods

The samples used for analysis were collected from the host rocks of the Zn–Cu ore bodies. Based on field geological surveys and microscopic observations, typical skarn rocks (garnet, vesuvianite, wollastonite, pyroxene, actinolite, axinite, and epidote) were selected for electron probe microanalysis (EPMA). The prograde skarn rock garnet and the retrograde skarn rock axinite were selected for laser ablation inductively coupled plasma mass spectrometry (LA-ICP–MS) trace element analysis. All sample analyses were completed at the Laboratory of Mineralization and Dynamics, Chang’an University.
Major element analyses were carried out on an EPMA (JXA-iHP200F) with an acceleration voltage of 15 kV, a beam current of 10 nA, and a beam spot diameter of 1 µm. In this work, the natural minerals albite, forsterite, corundum, K-feldspar, apatite, chromite, fayalite, and cassiterite were used as standards for Na, Mg, Al, K, P, Cr, Fe, and Sn, respectively. The natural mineral wollastonite was used as a standard for Si and Ca, and pyrophanite was used for Mn and Ti. Nickel oxide was used as the standard for Ni. Here, the element concentrations were calculated using the CitZAF interelement correction model [26].
Trace element quantification was performed by an Agilent 7900 quadrupole ICP–MS coupled with an ESL 193HE excimer laser ablation system. He (flow rate 0.5 L/min) was used as the carrier gas, and Ar (flow rate 0.8 L/min) as the make-up gas, with a beam diameter of 35 µm, a laser repetition rate of 11 HZ, and an energy fluence of 6.4 J/cm2. Each analysis included a background measurement for 25 s, followed by 40 s of data acquisition. The NIST SRM 610 silicate glass standard was used for external calibration. Here, one complete assay cycle contained a sequence of 2 spot analyses of NIST SRM 610, 6 to 10 spot analyses of unknown samples, and 2 spot analyses of NIST SRM 610. All data were collected in time-resolved analysis (TRA) mode, and data reduction was performed using “Stalquant”, an in-house data reduction software developed by the Günther group at ETH [27]. Quantification was performed using Si as the internal standard element or via matrix normalization (100 wt% oxides) [28].

5. Results

5.1. Petrographic Characteristics and EPMA Analysis Results

5.1.1. Garnet

Garnet coexists with vesuvianite and metasomatized the muddy-rich zone in the original rock. It is the earliest-formed and dominant skarn mineral, cut by vesuvianite-calcite veins and pyroxene-calcite veins, and replaced by later-formed pyroxene, epidote, and calcite. The garnet in the hand specimen shows a light brownish-red color (Figure 6a–c), with an euhedral–subhedral texture and grain sizes ranging from 0.6 to 5 mm. Under plane-polarized light, the garnet is colorless to light brown. Based on hand specimens and microscopic observations, the garnet can be divided into two generations: An early generation (Grt I) and a late generation (Grt II). Grt I displays a euhedral–subhedral dodecahedral texture, homogeneous or local abnormal extinction, and a lack of well-developed zoning. It is often intergrown with wollastonite, vesuvianite and pyroxene (Figure 6e,j,k). The surface of Grt I is relatively rough and has a dissolution texture; some surfaces can be seen to have been replaced by calcite and epidote, which may be a superposition of later hydrothermal alteration. Grt II is associated with sulfides or cuts through Grt I in a vein-like pattern (Figure 6f,g) with a euhedral–subhedral texture and obvious heterogeneity. Grt II showed well-developed zoning. Part of Grt II contains fine-grained pyroxene.
The EPMA results for two generations of garnets were published by He et al. [24]. The SiO2 and CaO contents in the garnets show limited variation, ranging from 36.04 to 39.31 wt% and 33.62 to 35.84 wt%, respectively. Compared to Grt II, Grt I is rich in Al2O3 (10.47 to 19.08 wt%) and deplete in FeO (4.97 to 15.54 wt%). Grt II is relatively rich in FeO (14.10 to 18.67 wt%) and deplete in Al2O3 (7.91 to 11.53 wt%), with low content of TiO2 and MnO. The data (based on 12 oxygen atoms) show that the garnet from the Dachang ore field belongs to the grossular–andradite solid solution series (Gro29–82And12–69); Grt I is Al-rich and dominated by grossular, while Grt II is Fe-rich and dominated by andradite (Figure 7a).

5.1.2. Vesuvianite

The vesuvianite content of the skarn rocks is relatively high and is seen in the field as a gray-green radiated aggregate coexisting with garnet (Figure 6c), formed in the prograde skarn stage. Under plane-polarized light, the vesuvianite is colorless with granular, columnar, and radial particles (Figure 6h,i) and considerable variation in particle size. The cross-section of the vesuvianite is square, and discontinuous stripes and bands are seen in the vertical section. The interference color is grayish-white, with an abnormal interference color of grayish-yellow. Vesuvianite coexists with garnet in euhedral granules, while epidote in irregularly granular filled between garnet and vesuvianite.
The EPMA analysis results for the vesuvianite are shown in Table 1, and the SiO2 content ranges from 35.23 to 36.76 wt% (avg. 36.06 wt%); CaO ranges from 34.88 to 37.12 wt% (avg. 35.94 wt%); Al2O3 ranges from 11.90 to 15.28 wt% (avg. 13.24 wt%); TFeO ranges from 4.11 to 6.72 wt% (avg. 5.77 wt%); MgO ranges from 2.65 to 3.12 wt% (avg. 2.84 wt%); TiO2 ranges from 0.14 to 0.23 wt% (avg. 0.18 wt%); and Cr2O3 ranges from 0.04 to 1.48 wt% (avg. 0.29 wt%). The contents of MnO, Na2O, K2O, NiO, and P2O5 are relatively low. A small amount of SnO2 (0 to 0.02 wt%) is also detected in the vesuvianite. The vesuvianite classification diagram shows that the vesuvianite in the Dachang ore field is an Al-rich vesuvianite (Figure 7c).

5.1.3. Pyroxene

Pyroxene, which is a green irregular granule in the outcrop, is of low abundance compared with garnet and vesuvianite. Under plane-polarized light, it is colorless to green, while under cross-polarized light, the interference color is relatively high, reaching blue-green to orange-yellow, with developed cleavage (Figure 6j). Under the microscope, pyroxene is seen to occur as irregular grains filling interstices between vesuvianite and garnet, accompanied by wollastonite. It can also be seen that the pyroxene replaced garnet, which indicated that it formed slightly after the garnet and vesuvianite.
The EPMA results (Table 2) show that the pyroxene in the Dachang ore field belongs to the diopside–hedenbergite solid solution (Figure 7d). The SiO2 content in the diopside is 52.00 to 55.03 wt%, CaO is 24.81 to 26.48 wt%, TFeO is 4.37 to 6.73 wt%, and MgO is 13.58 to 15.27 wt%; the contents of SiO2 in the hedenbergite are 47.28 to 50.87 wt%, CaO are 22.65 to 24.60 wt%, TFeO are 17.98 to 28.16 wt%, and MgO are 0.44 to 6.54 wt%. The contents of MnO, Cr2O3, Na2O, Al2O3, TiO2, K2O, NiO, and P2O5 in the pyroxene are relatively low. A small amount of SnO2 (0 to 0.27 wt%) is also detected in the pyroxene.
The data (based on 6 oxygen atoms) show that the main end member of the pyroxene is hedenbergite (Hd), with a variation range of 13.82 to 95.54% (avg. 66.86%); the second end member is diopside (Di), with a variation range of 2.69 to 85.67% (avg. 30.85%); it also contains a small amount of johannsenite (Jo) with a content of <6%, belonging to the diopside–hedenbergite solid solution (Di3–86Hd14–96Jo0.5–6).

5.1.4. Wollastonite

Wollastonite is one of the important minerals in the prograde skarn stage, and hand specimens are gray-white to pale red, long-prismatic, and radiated (Figure 6d), with a glassy luster. Under plane-polarized light, it is colorless, the interference color is gray to orange under cross-polarized light, and it coexists with pyroxene, garnet, and vesuvianite (Figure 6k). In some calcareous siliceous rocks, limestones, and marlstones, wollastonite is scattered in long-prismatic, radiated, and agglomerate.
The chemical composition of wollastonite is relatively simple, mainly consisting of SiO2 and CaO. The EPMA results are shown in Table 3, with SiO2 contents ranging from 49.71 to 51.92 wt% (avg. 50.81 wt%), CaO contents ranging from 46.32 to 49.98 wt% (avg. 48.42 wt%), and small amounts of NiO, TFeO, and Na2O. The calculation shows that the end member component of the wollastonite is mainly wollastonite (Wo), with a range of 99.07 to 99.84% (avg. 99.52%), while the contents of enstatite (En), ferrosilite (Fs), and aegirine (Ac) are less than 1%. A small amount of SnO2 (0 to 0.06 wt%) is also detected in wollastonite.

5.1.5. Axinite

Axinite is a hydrated silicate mineral of the retrograde skarn stage, with reddish brown and euhedral grains. Axinite coexists mainly with carbonates and is one of the end products of the skarn stage. It cuts and replaces garnet, pyroxene, and epidote. Axinite is intimately related to ore minerals produced by the ore-forming fluids; arsenopyrite and sphalerite can be seen coexisting with it in the axinite hornfels. Therefore, the axinite is formed during the late stage of skarnization and the early stage of mineralization, which is a transitional period. Under plane-polarized light, the axinite is wedge-shaped or plate-prismatic (Figure 6m–o), colorless or pale yellow, and interference colors not exceeding yellow, sometimes with weak abnormal interference colors.
The EPMA results for axinite are listed in Table 4, with SiO2 contents ranging from 41.59 to 43.29 wt% (avg. 42.33 wt%), Al2O3 contents ranging from 16.42 to 18.25 wt% (avg. 17.39 wt%), CaO contents ranging from 18.49 to 20.17 wt% (avg. 19.60 wt%), FeO contents ranging from 5.01 to 9.99 wt% (avg. 7.64 wt%), MnO contents ranging from 1.31 to 7.64 wt% (avg. 4.48 wt%), and B2O3 contents ranging from 5.98 to 6.19 wt% (avg. 6.10 wt%, B2O3 content calculated based on 32(O, OH) cation). The axinite in the Dachang ore field is mainly ferroaxinite (Figure 7b).

5.1.6. Actinolite

Actinolite is a common mineral of the retrograde skarn stage and is an important hydrated silicate mineral in the Dachang ore field. It often coexists with hydrated silicate minerals such as chlorite and epidote and metasomatized prograde skarn rocks and is closely related to mineralization. Under plane-polarized light, it appeared as a green fibrous and radiated aggregate (Figure 6q,r) with significant pleochromism and interference color ranging from the top of level I to the middle of level II.
The EPMA results for actinolite are listed in Table 5, with the SiO2 content ranging from 49.05 to 55.92 wt% (avg. 51.53 wt%); the TFeO content ranging from 23.27 to 28.66 wt% (avg. 26.41 wt%); the CaO content ranging from 10.16 to 12.93 wt% (avg. 11.83 wt%); the MgO content ranging from 4.67 to 7.11 wt% (avg. 5.59 wt%); the Al2O3 content ranging from 1.77 to 3.59 wt% (avg. 2.40 wt%). The contents of TiO2, MnO, Na2O, K2O, and Cr2O5 are relatively low, and a small amount of SnO2 (0 to 0.10 wt%) is also detected in the actinolite. The Mg/(Mg + Fe2+) ratio of the actinolite ranged from 0.23 to 0.34, indicating that it was mainly an Fe-actinolite (Figure 7e).

5.1.7. Epidote

Retrograde skarn stage minerals such as epidote and actinolite are replaced by anhydrous silicate minerals formed during the prograde skarn stage and are intimately related to mineralization. The epidote occurs as small and mostly irregular grains between the garnet, pyroxene, and vesuvianite (Figure 6p). Under plane-polarized light, the epidote is green to yellow-green granular and columnar shaped with bright but uneven interference colors.
The EPMA results showed that the main element components of the epidote are SiO2, Al2O3, CaO, and FeO (Table 6), with SiO2 contents ranging from 36.15 to 39.09 wt% (avg. 37.65 wt%); Al2O3 contents ranging from 20.91 to 25.12 wt% (avg. 22.93 wt%); CaO contents ranging from 23.17 to 24.85 wt% (avg. 23.91 wt%); and TFeO contents ranging from 9.57 to 12.55 wt% (avg. 11.26 wt%). The contents of MgO, TiO2, MnO, Na2O, K2O, and Cr2O5 are relatively low. A small amount of SnO2 (0 to 0.05 wt%) is also detected in the epidote.

5.2. LA-ICP–MS Analysis Results

In this study, prograde skarn rock garnet and retrograde skarn rock axinite were selected for LA-ICP–MS trace element analysis.

5.2.1. Garnet

The trace element analysis results for garnet were published by He et al. [24]. The results showed that both generations of garnets are depleted in large ion lithophile elements (LILEs) such as Rb, Cs, Ba, and K compared to the primitive mantle [35]. The Hf content ranges from 0.62 to 2.48 ppm; Zr ranges from 15.54 to 101.13 ppm; Nb ranges from 0.45 to 7.96 ppm; Ta ranges from 0.02 to 0.83 ppm; Th ranges from 0 to 0.76 ppm; and U ranges from 0 to 0.84 ppm.
All garnets contain ore-forming elements such as W, Sn, As, In, Ge, and Ga, and apart from Ga, the content of other ore-forming elements is lower in Grt I than in Grt II. The W content ranges from 0.17 to 12.8 ppm; Sn ranges from 340 to 4137 ppm; As ranges from 0 to 6.3 ppm; In ranges from 1.8 to 46.8 ppm; Ge ranges from 2.6 to 23.6 ppm; and Ga ranges from 20.3 to 43.0 ppm.
All garnets show characteristics of heavy rare earth element (HREE) enrichment and light rare earth element depletion (LREE; Figure 8), compared to the chondrite. The total rare earth element (ΣREE) content varies from 6.02 to 59.30 ppm; the ΣLREE/ΣHREE ratio varies from 0.01 to 0.67, with obvious negative to slightly negative Eu anomalies (δEu = 0.18–0.94). The ΣREE content and the ΣLREE/ΣHREE ratio are lower in Grt I than in Grt II, while δEu is higher than in Grt II.

5.2.2. Axinite

The trace element contents of the axinite are listed in Table 7. The ΣREE content of sample 1511-20-4 is 200.42 ppm, which is significantly higher than that of other axinites. It is speculated that this analysis point may contain REE-rich mineral inclusions and will not be discussed further. Axinite is depleted in LILEs compared to the primitive mantle [36], with contents of elements such as Rb, Cs, Ba, and K below detection limits. The axinite contains 12.2–33.6 ppm Sr, 0–2.4 ppm Nb, and 0.08–39.4 ppm Zr.
The axinite contains ore-forming elements such as Sn, As, In, Ge, and Ga. The content of Sn in the axinite ranges from 31.6 to 706 ppm, As ranges from 0.82 to 8.9 ppm, Ge ranges from 2.8 to 8.4 ppm, Ga ranges from 11.0 to 28.3 ppm, and In ranges from 0.30 to 8.9 ppm.
The chondrite-normalized REE pattern of the axinite shows a significant fractionation of light and heavy rare earth elements (Figure 8), with ΣLREE/ΣHREE ratios ranging from 0.10 to 0.97 (with a point value of 1.54) and significantly negative Eu anomalies (δEu = 0.00–0.70, avg. 0.28). The ΣREE content ranges from 0.44 to 19.55 ppm.

6. Discussion

6.1. Redox Conditions of the Ore-Forming Fluids

Different redox conditions often produce different skarn rocks, so the mineral assemblages and chemical compositions of skarn rocks can be used to constrain the redox conditions of the ore-forming fluids [3,4,36,37,38,39]. The contents and chemical compositions of garnet have significant implications for the redox conditions of ore-forming fluids [3,39]. When the oxygen fugacity of the fluid was high, the skarn rocks had a relatively high Fe3+/Fe2+ ratio, and andradite was formed. However, when the oxygen fugacity of the fluid was low, the skarn rocks had a relatively high Fe2+/Fe3+ ratio, and grossular was formed [40,41,42,43,44,45,46]. Based on the temperature–logfO2 diagram for stable skarn rocks and sulfide assemblages at different stages summarized by Meinert et al. [5], we proposed an evolution process for the redox conditions of ore-forming fluids at the skarn stage.
The earliest mineral formed during the skarn stage of the Dachang ore field was grossular, indicating that the early ore-forming fluid during the skarn stage was relatively reduced [24]; with the evolution of the ore-forming fluid, considerable andradite, pyroxene, and wollastonite were formed, indicating an increase in the oxygen fugacity of the ore-forming fluid in the later stage. In the final skarn stage, garnet and pyroxene were replaced by Fe-actinolite, chlorite, and quartz, indicating that the ore-forming conditions changed from relatively oxidized to reduced (Figure 9). Subsequently, many sulfides precipitated under the relatively reduced conditions [1,5]. The δEu of fluorite coexisting with the Zn–Cu ore bodies is 0.16–0.87 (avg. 0.41, unpublished data), also indicating that the ore-forming fluid is under reducing conditions.

6.2. Lithological Control during the Formation of Skarn Rocks

The Zn–Cu ore bodies in the Dachang ore field were intimately related to the retrograde skarn stage. Mineralization mainly occurred in the limestone, black mudstone, and shale of the middle Devonian Luofu Formation ( D 2 2 l) and the limestone of the upper Devonian Wuzhishan Formation ( D 3 2 w). The early generation garnet was mainly composed of grossular; the vesuvianites are Al-rich vesuvianites; the late generation garnet is mainly composed of andradite; the pyroxenes formed a diopside–hedenbergite solid solution; the axinites are mainly ferroaxinites; and the actinolites are Fe-actinolites, indicating that the skarn rocks gradually evolved from early Al-rich to late Fe-rich characteristics. After analyzing the Longxianggai granitic pluton, Liang [6] pointed out that the granitic pluton had a high Al content and was depleted in Fe, indicating that the early ore-forming fluid was mainly composed of magmatic exsolution fluids, and the skarn rocks may mainly reflect the characteristics of the magmatic fluids. After analyzing the geochemistry of the Devonian strata in the Dachang ore field, Han et al. [47] noted that the middle Devonian Luofu Formation ( D 2 2 l) and the upper Devonian Wuzhishan Formation ( D 3 2 w) in this area contained widely distributed spotted, nodular, striped, and banded fine-grained pyrite, and the content of Fe2+ was higher than that of Fe3+. The ratio of Fe3+/(Fe3+ + Fe2+) was typically lower than 0.3%. The late stage of the Fe-rich skarn rocks may indicate that the late ore-forming fluid was strongly influenced by the country rock.

6.3. Implications of Mineralization

EPMA results of the calc-silicates in the Dachang ore field show that all skarn contain a small amount of the ore-forming element Sn. The end-member components of the pyroxene are relatively similar to those of the vast majority of skarn-type Sn deposits worldwide [5]. According to the classification proposed by Sanero and Gottardi [48], the axinite in the Dachang ore field is mainly ferroaxinite (Figure 6b). Qian [49] and Hu et al. [50] analyzed axinite from the Gejiu and Furong Sn deposits and noted that the axinite in these two deposits was also mainly composed of ferroaxinite.

6.3.1. Migration of Ore-Forming Elements during the Evolution of Hydrothermal Fluids

LA-ICP–MS analysis showed that neither the garnet nor the axinite contained Cu, and Zn was not detected in the axinite. We collected the trace element contents of the Longxianggai granitic pluton and the vesuvianite in the Dachang ore field and plotted them (Figure 10). From Longxianggai granitic pluton → garnet → vesuvianite → axinite, the content of ore-forming elements Sn and In first increased and then decreased, with the highest content in garnet; the content of W and As decreased; the content of Zn was relatively low in Longxianggai granitic pluton and garnet, but significantly increased in vesuvianite; and the content of Ga and Ge in skarn rocks did not change significantly.
Sn in garnet is very high; the contents of Sn are 2378 ppm in garnet, 688 ppm in vesuvianite [51] and 281 ppm in axinite. From the prograde skarn stage to the retrograde skarn stage, the Sn content gradually decreased, indicating that the Sn mineralization was not the remobilization of Sn from prograde skarn rocks by hydrothermal fluid. The significant enrichment of Sn in the magmatic hydrothermal fluid is a necessary condition for Sn mineralization. This conclusion is consistent with that drawn by Chen et al. [52] after studying the Furong skarn-type Sn deposit.

6.3.2. Influence of the Volatile on Mineralization

The widely developed minerals such as vesuvianite, axinite, fluorite, and tourmaline in the Dachang ore field indicate that the ore-forming fluid contained large amounts of volatiles F and B. Zhao et al. [53] analyzed the trace elements and B isotopes of tourmaline in the Longxianggai granitic pluton and the Dachang ore field and noted that the ore-forming fluid and volatile B were mainly from magmatic hydrothermal fluids.
Volatiles play a significant role in magma evolution and mineralization. During the partial melting process in the source region, volatiles B and F lowered the solidus temperature of Sn-bearing minerals, facilitating the partial melting of Sn-bearing minerals [54,55]. During magma evolution, the enrichment in B increased the solubility of fluid in the magma system and increased fluid content [56]. F broke the bridging oxygen bonds in the melt, reduced the viscosity of the melt, and to some extent increased the diffusion of the ore-forming elements in the melt, thereby increasing the solubilities of the ore-forming elements in the melt. The presence of volatiles may have prolonged the magma evolution process and allowed the enrichment of incompatible elements, such as Sn, in the residual magma. During the dissolution of magmatic hydrothermal fluids, volatiles facilitated further enrichment of the ore-forming elements in the hydrothermal fluid and may have formed complexes with Sn(BF4)2 [57], allowing long-distance migration of the ore-forming elements in the hydrothermal fluid [58,59,60,61,62]. The widely distributed volatiles F and B in the ore-forming fluid may be one of the reasons for the large scale of metal deposition and mineralization in the Dachang ore field and also one of the reasons for the formation of Zn–Cu ore bodies proximal to the granitic pluton and Sn polymetallic ore bodies distal to the granitic pluton in the Dachang ore field.

7. Conclusions

(1) Based on the mineral assemblages and chemical composition characteristics of the skarn rocks in the Dachang ore field, the early ore-forming fluid in the skarn stage was in a relatively reduced state; as the ore-forming fluid evolved, the oxygen fugacity of the ore-forming fluid in the later stage increased; in the final skarn stage, the ore-forming conditions changed from a relatively oxidized state to a relatively reduced state, and sulfides were precipitated.
(2) The skarn rocks in the Dachang ore field evolved from early Al-rich to late Fe-rich characteristics, indicating that the early hydrothermal fluids were mainly magmatic exsolution fluids, and the skarn rocks may mainly reflect the characteristics of the magmatic fluids. The late stage of Fe-rich skarn rocks may indicate that the late hydrothermal fluids were strongly influenced by the country rock.
(3) From the prograde skarn stage to the retrograde skarn stage, the Sn content gradually decreased, indicating that the Sn mineralization was not due to the remobilization of Sn from prograde skarn rocks by hydrothermal fluid. The significant enrichment of Sn in the magmatic hydrothermal fluid was a necessary condition for Sn mineralization.
(4) The widely developed minerals such as vesuvianite, axinite, fluorite, and tourmaline in the Dachang ore field indicate that the ore-forming fluid contained large amounts of volatiles F and B. This may be the vital reason for the large-scale mineralization of the Dachang ore field and one of the reasons for the formation of Zn–Cu ore bodies proximal to the granitic pluton and Sn polymetallic ore bodies distal to the granitic pluton in the Dachang ore field.

Author Contributions

Conceptualization, L.H. and T.L.; methodology, L.H.; software, J.Z.; investigation, B.L.; writing—original draft preparation, L.H. and T.L.; writing—review and editing, L.H., T.L. and D.W.; funding acquisition, T.L. All authors have read and agreed to the published version of the manuscript.

Funding

This study is financially supported by the China Geological Survey granted to T. Liang (Grant Number: DD20221695-43, DD20190379).

Data Availability Statement

Data are contained within the article.

Acknowledgments

We would like to thank Minwu Liu and Xijuan Tan from Chang’ an University. We also thank the editors and three anonymous reviewers for their editorial handling and constructive comments on this manuscript.

Conflicts of Interest

Author Jianxin Zhang was employed by the company Northwest Bureau of China Metallurgical Geology Bureau, and author Bosheng Liu was employed by the company Guangxi 215 Geological Team Co., Ltd. The remaining authors declare that the research was conducted in the absence of any commercial or financial relationships that could be construed as a potential conflict of interest.

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Figure 1. Location diagram of Dachang ore field (a) and distribution of deposits in Dachang ore field (b) (modified after [15]).
Figure 1. Location diagram of Dachang ore field (a) and distribution of deposits in Dachang ore field (b) (modified after [15]).
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Figure 2. Stratigraphic column of the Dachang oer field (modified after [8]).
Figure 2. Stratigraphic column of the Dachang oer field (modified after [8]).
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Figure 3. Profile of the Sn polymetallic ore bodies and Zn–Cu ore bodies distribution in the Dachang ore field (modified after [20]).
Figure 3. Profile of the Sn polymetallic ore bodies and Zn–Cu ore bodies distribution in the Dachang ore field (modified after [20]).
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Figure 4. Characteristics of mineral assemblages in Zn–Cu ore bodies. (a) Zn–Cu ore bodies and garnet bands along layers, (b) contact relationship between skarn rocks and granitic pluton, (c) the retrograde skarn stage is intimately related to mineralization.
Figure 4. Characteristics of mineral assemblages in Zn–Cu ore bodies. (a) Zn–Cu ore bodies and garnet bands along layers, (b) contact relationship between skarn rocks and granitic pluton, (c) the retrograde skarn stage is intimately related to mineralization.
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Figure 5. Paragenesis of the mineral assemblages showing the mineralized sequence of Zn–Cu ore bodies.
Figure 5. Paragenesis of the mineral assemblages showing the mineralized sequence of Zn–Cu ore bodies.
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Figure 6. Skarn mineral characteristics of Dachang ore field. (a) Sphalerite and garnet formed along strata, (b) skarn formation along strata, (c) vesuvianite intergrown with garnet, (d) wollastonite with radiated aggregate, (e) Grt I presents euhedral–subhedral grains with a rough surface, (f) Grt I cut by vein Grt II, (g) Grt II surrounded by sphalerite, (h) the interference color of vesuvianite is grayish-white, (i) vesuvianite with a radiated aggregate, (j) pyroxene included in garnet in an irregular granular form, (k) wollastonite intergrown with garnet, (l) long-prismatic wollastonite in carbonaceous siliceous rocks, (m) axinite surrounded by sphalerite, (n) plate-prismatic axinite, (o) axinite surrounded by calcite, (p) green granular epidote surrounded by actinolite, (q) actinolite with fibrous associated with calcite, and (r) actinolite coexisting with sphalerite. Mineral abbreviations: Grt—garnet, Ves—vesuvianite, Wo—wollastonite, Sp—sphalerite, Ep—epidote, Cpx—clinopyroxene, Ax—axinite, Cc—calcite, Act—actinolite.
Figure 6. Skarn mineral characteristics of Dachang ore field. (a) Sphalerite and garnet formed along strata, (b) skarn formation along strata, (c) vesuvianite intergrown with garnet, (d) wollastonite with radiated aggregate, (e) Grt I presents euhedral–subhedral grains with a rough surface, (f) Grt I cut by vein Grt II, (g) Grt II surrounded by sphalerite, (h) the interference color of vesuvianite is grayish-white, (i) vesuvianite with a radiated aggregate, (j) pyroxene included in garnet in an irregular granular form, (k) wollastonite intergrown with garnet, (l) long-prismatic wollastonite in carbonaceous siliceous rocks, (m) axinite surrounded by sphalerite, (n) plate-prismatic axinite, (o) axinite surrounded by calcite, (p) green granular epidote surrounded by actinolite, (q) actinolite with fibrous associated with calcite, and (r) actinolite coexisting with sphalerite. Mineral abbreviations: Grt—garnet, Ves—vesuvianite, Wo—wollastonite, Sp—sphalerite, Ep—epidote, Cpx—clinopyroxene, Ax—axinite, Cc—calcite, Act—actinolite.
Minerals 14 00193 g006
Figure 7. (a) Diagram of end members of garnet (after [29]), (b) diagram for classification of axinite (after [30]), (c) diagram for classification of vesuvianite (after [31,32]), (d) diagram of end members of clinopyroxene (after [5]), (e) diagram for classification of amphibole (after [33]), and (f) distribution of octahedral Al and Fe for epidotes (after [34]) from Dachang ore field. Mineral abbreviations: And—andradite, Gro—grossular, Spe—spessartine, Pyr—pyrope, Alm—almandine, Jo—johannsonite, Di—diopside, Hd—hedenbergite.
Figure 7. (a) Diagram of end members of garnet (after [29]), (b) diagram for classification of axinite (after [30]), (c) diagram for classification of vesuvianite (after [31,32]), (d) diagram of end members of clinopyroxene (after [5]), (e) diagram for classification of amphibole (after [33]), and (f) distribution of octahedral Al and Fe for epidotes (after [34]) from Dachang ore field. Mineral abbreviations: And—andradite, Gro—grossular, Spe—spessartine, Pyr—pyrope, Alm—almandine, Jo—johannsonite, Di—diopside, Hd—hedenbergite.
Minerals 14 00193 g007
Figure 8. Chondrite-normalized REE patterns of garnets and axinites (normalization values after [35]).
Figure 8. Chondrite-normalized REE patterns of garnets and axinites (normalization values after [35]).
Minerals 14 00193 g008
Figure 9. Temperature–log oxygen fugacity diagram, showing the stability fields of major skarn silicate, oxide, and sulfide minerals (Modified from [5]). Mineral abbreviations: Ad = andradite, Amp = amphibole, Cc = calcite, Fe–Act = ferro–actinolite, Gp = graphite, Hd = hedenbergite, Hm = hematite, Mt = magnetite, Po = pyrrhotite, Py = pyrite, Pyx = pytoxcnc, Qz = quartz, Wo = wollastonite. The red arrow shows the direction of evolution.
Figure 9. Temperature–log oxygen fugacity diagram, showing the stability fields of major skarn silicate, oxide, and sulfide minerals (Modified from [5]). Mineral abbreviations: Ad = andradite, Amp = amphibole, Cc = calcite, Fe–Act = ferro–actinolite, Gp = graphite, Hd = hedenbergite, Hm = hematite, Mt = magnetite, Po = pyrrhotite, Py = pyrite, Pyx = pytoxcnc, Qz = quartz, Wo = wollastonite. The red arrow shows the direction of evolution.
Minerals 14 00193 g009
Figure 10. Trace element compositions of skarn rocks and granite by LA-ICP–MS. (Vesuvianite from [48]; granite from [6,11,18]).
Figure 10. Trace element compositions of skarn rocks and granite by LA-ICP–MS. (Vesuvianite from [48]; granite from [6,11,18]).
Minerals 14 00193 g010
Table 1. Major element compositions (wt%) of the vesuviante.
Table 1. Major element compositions (wt%) of the vesuviante.
Sample Na2OK2OFeOMgOP2O5MnOAl2O3CaONiOSiO2TiO2Cr2O3SnO2TotalNaFeMgMnAlCaSiTiCr
LM-21X
(N = 5)
MAX0.06 0.01 6.11 3.01 0.03 0.14 13.24 36.31 0.03 36.22 0.23 0.24 0.01 94.32 0.03 1.38 1.19 0.03 4.15 10.32 9.73 0.05 0.05
MIN0.01 0.00 5.69 2.65 0.00 0.04 11.90 35.40 0.00 35.23 0.14 0.04 0.00 92.78 0.01 1.27 1.07 0.01 3.77 10.11 9.43 0.03 0.01
AVG0.03 0.01 5.96 2.85 0.01 0.08 12.79 35.73 0.01 35.65 0.17 0.11 0.01 93.41 0.02 1.34 1.14 0.02 4.03 10.25 9.54 0.04 0.02
LM-15X
(N = 4)
MAX0.06 0.02 6.72 3.12 0.08 0.21 15.28 37.12 0.01 36.76 0.21 1.48 0.02 97.11 0.03 1.47 1.22 0.05 4.60 10.16 9.62 0.04 0.31
MIN0.02 0.00 4.11 2.70 0.01 0.10 12.31 34.88 0.00 35.97 0.16 0.09 0.00 94.27 0.01 0.90 1.05 0.02 3.80 9.80 9.37 0.03 0.02
AVG0.04 0.01 5.29 2.82 0.05 0.16 13.94 35.91 0.00 36.37 0.18 0.66 0.01 95.44 0.02 1.15 1.10 0.04 4.28 10.02 9.48 0.04 0.14
590-1X
(N = 4)
MAX0.04 0.01 6.11 2.88 0.02 0.10 13.36 36.47 0.01 36.64 0.19 0.26 0.01 95.48 0.02 1.34 1.12 0.02 4.12 10.25 9.60 0.04 0.06
MIN0.03 0.00 5.95 2.80 0.01 0.07 12.92 36.08 0.00 35.84 0.16 0.06 0.00 94.22 0.02 1.31 1.11 0.02 3.99 10.20 9.51 0.03 0.01
AVG0.04 0.00 6.01 2.85 0.02 0.09 13.12 36.25 0.01 36.25 0.18 0.15 0.01 94.96 0.02 1.32 1.12 0.02 4.07 10.22 9.54 0.04 0.03
Number of ions based on 38 oxygen atoms.
Table 2. Major element compositions (wt%) of the pyroxene.
Table 2. Major element compositions (wt%) of the pyroxene.
Sample SiO2TiO2Al2O3Cr2O3FeOMnOMgOCaONa2OK2ONiOSnO2P2O5TotalSiFe3+Fe2+MnMgCaJoDiHd
976-500.53 (N = 3)MAX55.03 0.06 0.39 0.11 5.84 0.28 15.27 25.74 0.17 0.03 0.03 0.02 0.02 100.36 2.01 0.04 0.15 0.01 0.83 1.03 0.90 85.67 18.64
MIN52.96 0.01 0.16 0.05 4.37 0.15 14.17 24.81 0.05 0.01 0.01 0.02 0.02 99.13 1.98 0.00 0.13 0.00 0.79 0.97 0.50 80.86 13.82
AVG53.81 0.04 0.26 0.07 5.27 0.20 14.60 25.39 0.10 0.02 0.02 0.02 0.02 99.78 1.99 0.03 0.14 0.00 0.81 1.01 0.63 82.62 16.74
LM-4X
(N = 4)
MAX53.53 0.03 0.22 0.05 6.73 0.34 14.82 26.48 0.09 0.02 0.03 0.00 0.04 100.50 2.00 0.16 0.21 0.01 0.83 1.06 1.03 82.31 21.35
MIN52.00 0.01 0.09 0.02 5.11 0.17 13.58 25.07 0.02 0.02 0.01 0.00 0.03 98.44 1.94 0.00 0.04 0.01 0.77 1.02 0.55 78.10 16.76
AVG52.93 0.02 0.14 0.04 6.03 0.27 14.07 25.79 0.05 0.02 0.02 0.00 0.04 99.37 1.99 0.04 0.15 0.01 0.79 1.04 0.87 80.00 19.13
590-7
(N = 4)
MAX50.35 0.01 0.27 0.07 23.51 0.85 4.94 24.04 0.14 0.01 0.04 0.00 0.01 100.83 2.00 0.10 0.79 0.03 0.29 1.02 2.81 29.42 81.72
MIN47.99 0.01 0.13 0.05 20.49 0.57 2.63 22.65 0.07 0.01 0.03 0.00 0.01 98.86 1.96 0.00 0.63 0.02 0.16 0.99 2.01 16.28 68.21
AVG49.18 0.01 0.20 0.06 22.34 0.72 3.69 23.37 0.10 0.01 0.04 0.00 0.01 99.68 1.99 0.04 0.71 0.03 0.22 1.01 2.46 22.17 75.38
590-21
(N = 4)
MAX50.79 0.03 0.05 0.05 23.15 1.33 4.46 24.60 0.09 0.02 0.03 0.04 0.02 100.91 2.01 0.01 0.78 0.05 0.26 1.04 4.68 27.65 80.76
MIN49.29 0.01 0.04 0.04 19.76 1.04 2.35 23.73 0.03 0.02 0.01 0.01 0.01 99.51 2.00 0.00 0.65 0.03 0.14 1.02 3.65 14.55 68.70
AVG50.07 0.02 0.04 0.04 21.63 1.19 3.31 24.02 0.06 0.02 0.02 0.03 0.01 100.42 2.00 0.01 0.72 0.04 0.20 1.03 4.19 20.51 75.31
590-26
(N = 5)
MAX51.32 0.06 0.32 1.06 21.74 0.42 6.54 24.02 0.17 0.01 0.04 0.02 0.04 101.10 2.01 0.10 0.71 0.01 0.39 1.02 1.48 37.57 74.94
MIN49.16 0.03 0.07 0.03 18.49 0.29 3.83 23.17 0.06 0.01 0.01 0.02 0.02 99.30 1.96 0.00 0.53 0.01 0.23 0.97 1.02 23.58 61.29
AVG50.03 0.05 0.20 0.38 19.89 0.34 5.20 23.69 0.11 0.01 0.03 0.02 0.03 99.90 1.99 0.03 0.63 0.01 0.31 1.01 1.17 31.35 67.48
530-6
(N = 4)
MAX49.62 0.02 0.57 0.08 28.16 0.63 3.03 23.27 0.10 0.01 0.00 0.27 0.03 100.55 2.01 0.11 0.86 0.02 0.18 1.03 2.26 19.27 95.54
MIN47.28 0.01 0.08 0.02 21.95 0.51 0.44 23.08 0.04 0.01 0.00 0.12 0.02 99.12 1.95 0.00 0.75 0.02 0.03 1.00 1.78 2.69 78.47
AVG48.73 0.02 0.30 0.05 25.18 0.55 1.66 23.19 0.07 0.01 0.00 0.20 0.02 99.85 1.99 0.03 0.83 0.02 0.10 1.02 1.95 10.38 87.67
530-14
(N = 5)
MAX50.08 0.02 0.68 0.07 25.61 0.61 4.00 24.16 0.13 0.06 0.06 0.15 0.02 100.88 2.02 0.06 0.87 0.02 0.24 1.03 2.14 24.68 91.42
MIN48.50 0.01 0.14 0.03 21.18 0.34 1.16 23.10 0.08 0.03 0.01 0.02 0.01 99.41 1.98 0.00 0.68 0.01 0.07 1.00 1.23 7.35 73.18
AVG49.46 0.02 0.39 0.05 23.74 0.50 2.40 23.51 0.10 0.04 0.04 0.09 0.02 100.33 1.99 0.02 0.78 0.02 0.14 1.02 1.79 14.94 83.27
LM-7X
(N = 4)
MAX49.71 0.02 0.21 0.07 24.41 1.24 2.25 23.76 0.25 0.05 0.04 0.04 0.02 100.67 2.01 0.04 0.82 0.04 0.14 1.04 4.51 14.22 86.61
MIN48.79 0.01 0.09 0.05 23.25 0.99 1.39 23.36 0.07 0.04 0.03 0.04 0.02 99.52 1.99 0.00 0.76 0.03 0.08 1.02 3.52 8.88 82.04
AVG49.11 0.02 0.16 0.06 23.96 1.09 1.81 23.53 0.17 0.05 0.03 0.04 0.02 100.01 2.00 0.02 0.79 0.04 0.11 1.03 3.94 11.39 84.68
LM-14X
(N = 3)
MAX50.87 0.02 0.36 0.09 21.73 0.40 6.30 24.36 0.13 0.01 0.02 0.10 0.04 100.89 2.01 0.07 0.72 0.01 0.37 1.04 1.39 38.28 74.04
MIN49.18 0.02 0.07 0.04 17.98 0.23 4.07 23.57 0.07 0.01 0.01 0.02 0.01 98.86 1.97 0.00 0.52 0.01 0.24 1.00 0.81 24.65 60.91
AVG49.81 0.02 0.20 0.07 20.04 0.34 5.10 23.93 0.11 0.01 0.02 0.06 0.03 99.67 1.99 0.04 0.62 0.01 0.30 1.02 1.17 30.89 67.94
LM-21X
(N = 4)
MAX50.38 0.02 0.11 0.06 21.90 1.03 5.16 24.58 0.09 0.02 0.06 0.01 0.02 100.45 2.01 0.02 0.73 0.03 0.31 1.05 3.65 31.78 76.71
MIN49.82 0.01 0.05 0.01 18.76 0.48 3.14 23.37 0.05 0.02 0.03 0.01 0.01 99.22 1.99 0.00 0.60 0.02 0.19 1.00 1.65 19.64 64.70
AVG50.05 0.01 0.08 0.03 20.30 0.84 4.25 24.10 0.07 0.02 0.05 0.01 0.02 99.76 2.00 0.01 0.67 0.03 0.25 1.03 2.97 26.35 70.68
LM-22X
(N = 4)
MAX50.78 0.02 0.09 0.06 23.21 1.69 5.07 24.19 0.08 0.00 0.06 0.01 0.03 100.85 2.01 0.07 0.77 0.06 0.30 1.03 5.68 31.11 80.72
MIN49.00 0.01 0.08 0.05 19.21 0.76 2.58 23.62 0.06 0.00 0.01 0.01 0.02 99.45 1.97 0.00 0.60 0.03 0.15 1.02 2.65 16.01 66.24
AVG49.89 0.01 0.09 0.06 20.87 1.10 4.19 23.95 0.07 0.00 0.04 0.01 0.02 100.02 2.00 0.02 0.67 0.04 0.25 1.03 3.80 25.51 70.69
Number of ions based on 6 oxygen atoms. Jo—johannsenite, Di—diopside, Hd—hedenbergite.
Table 3. Major element compositions (wt%) of the wollastonite.
Table 3. Major element compositions (wt%) of the wollastonite.
Sample SiO2Al2O3Cr2O3FeOMnOMgOCaONa2OK2ONiOSnO2P2O5TotalSiCaWoEnFsAc
1511-2
(N = 4)
MAX51.53 0.00 0.05 0.10 0.02 0.03 49.62 0.05 0.03 0.01 0.04 0.04 101.46 1.98 2.04 99.68 0.09 0.19 0.19
MIN50.79 0.00 0.03 0.10 0.01 0.01 48.83 0.03 0.03 0.01 0.02 0.03 99.91 1.97 2.04 99.56 0.03 0.17 0.12
AVG51.17 0.00 0.04 0.10 0.01 0.02 49.27 0.05 0.03 0.01 0.03 0.03 100.74 1.98 2.04 99.60 0.07 0.18 0.17
1511-6
(N = 5)
MAX51.47 0.02 0.06 0.13 0.03 0.08 47.96 0.06 0.03 0.76 0.06 0.04 99.77 2.00 2.02 99.66 0.23 0.23 0.23
MIN50.26 0.01 0.04 0.07 0.01 0.03 47.36 0.01 0.01 0.23 0.01 0.02 98.84 1.99 1.99 99.35 0.09 0.16 0.05
AVG50.69 0.01 0.05 0.10 0.02 0.05 47.68 0.03 0.02 0.57 0.03 0.03 99.27 1.99 2.01 99.53 0.15 0.19 0.13
1520-870.3
(N = 6)
MAX51.60 0.01 0.06 0.18 0.03 0.09 49.73 0.09 0.01 0.06 0.06 0.04 101.68 1.98 2.06 99.61 0.25 0.33 0.33
MIN50.41 0.01 0.02 0.07 0.01 0.01 48.34 0.03 0.01 0.01 0.01 0.02 99.02 1.96 2.03 99.42 0.04 0.12 0.00
AVG51.04 0.01 0.04 0.11 0.02 0.04 49.24 0.06 0.01 0.02 0.03 0.03 100.61 1.98 2.04 99.52 0.10 0.19 0.19
1520-870.9
(N = 5)
MAX51.92 0.00 0.05 0.27 0.03 0.09 49.23 0.18 0.02 2.19 0.03 0.05 101.62 2.01 2.05 99.48 0.26 0.43 0.70
MIN49.96 0.00 0.02 0.07 0.01 0.06 46.32 0.01 0.02 0.01 0.01 0.01 98.98 1.97 1.96 99.07 0.18 0.05 0.00
AVG50.92 0.00 0.03 0.21 0.02 0.08 48.27 0.08 0.02 0.56 0.02 0.03 100.02 1.98 2.02 99.30 0.24 0.28 0.18
530-8
(N = 5)
MAX51.55 0.01 0.05 0.09 0.04 0.06 49.98 0.11 0.03 0.07 0.06 0.04 101.66 1.97 2.05 99.84 0.17 0.20 0.40
MIN49.83 0.01 0.03 0.02 0.01 0.02 48.53 0.01 0.01 0.01 0.01 0.01 98.67 1.97 2.04 99.23 0.06 0.04 0.00
AVG50.51 0.01 0.04 0.06 0.03 0.05 48.97 0.05 0.02 0.04 0.04 0.02 99.76 1.97 2.05 99.61 0.13 0.11 0.14
530-9
(N = 4)
MAX51.50 0.05 0.07 0.14 0.00 0.11 49.81 0.07 0.02 0.13 0.04 0.06 101.56 1.99 2.06 99.72 0.32 0.22 0.26
MIN49.71 0.01 0.02 0.03 0.00 0.01 48.15 0.01 0.01 0.09 0.02 0.02 98.25 1.97 2.01 99.38 0.03 0.04 0.04
AVG50.61 0.03 0.04 0.07 0.00 0.07 48.76 0.04 0.02 0.11 0.03 0.03 99.70 1.98 2.04 99.56 0.21 0.11 0.13
530-14
(N = 5)
MAX51.52 0.01 0.05 0.26 0.03 0.08 48.30 0.06 0.02 0.02 0.00 0.04 99.27 2.01 2.03 99.72 0.23 0.44 0.22
MIN50.46 0.01 0.04 0.08 0.01 0.03 47.35 0.01 0.01 0.01 0.00 0.01 98.42 1.98 1.97 99.29 0.09 0.18 0.00
AVG50.91 0.01 0.03 0.14 0.02 0.06 47.82 0.03 0.02 0.02 0.00 0.03 99.01 1.99 2.01 99.51 0.16 0.24 0.09
590-27
(N = 5)
MAX51.32 0.02 0.07 0.12 0.02 0.07 47.65 0.04 0.02 0.84 0.04 0.03 99.52 2.00 2.01 99.59 0.20 0.22 0.16
MIN50.21 0.01 0.01 0.09 0.01 0.04 47.12 0.01 0.01 0.31 0.01 0.02 98.22 1.99 1.99 99.47 0.12 0.17 0.05
AVG50.58 0.02 0.04 0.11 0.02 0.06 47.45 0.03 0.02 0.61 0.03 0.02 98.95 1.99 2.00 99.53 0.16 0.20 0.11
Number of ions based on 6 oxygen atoms. Wo—wollastonite, En—enstatite, Fs—Ferrosilite, Ac—aegirine.
Table 4. Major element compositions (wt%) of the axinite.
Table 4. Major element compositions (wt%) of the axinite.
Sample SiO2Al2O3TiO2SnO2K2OCaONa2OMgOFeOMnOCr2O3H2O *B2O3 *TotalSiAlCaMgFeMnOHB
1511-5-1
(N = 5)
MAX42.47 17.86 0.08 0.00 0.00 20.01 0.02 0.41 9.53 5.23 0.06 1.51 6.16 101.30 8.04 3.96 4.05 0.12 1.51 0.83 2.00 2.00
MIN42.04 16.93 0.01 0.00 0.00 19.62 0.01 0.09 8.13 3.86 0.02 1.48 6.07 99.70 7.97 3.79 4.00 0.02 1.28 0.62 2.00 2.00
AVG42.24 17.39 0.05 0.00 0.00 19.84 0.02 0.24 8.58 4.48 0.04 1.50 6.12 100.40 8.00 3.88 4.03 0.07 1.36 0.72 2.00 2.00
1511-5-2
(N = 5)
MAX42.43 17.64 0.10 0.15 0.03 20.17 0.00 0.86 9.99 4.84 0.11 1.50 6.13 100.40 8.04 3.93 4.08 0.24 1.58 0.78 2.00 2.00
MIN41.86 16.65 0.01 0.03 0.03 19.39 0.00 0.05 7.51 2.75 0.03 1.47 6.03 99.00 7.97 3.77 3.95 0.02 1.19 0.44 2.00 2.00
AVG42.16 17.27 0.05 0.08 0.03 19.67 0.00 0.58 8.74 3.77 0.07 1.49 6.10 99.98 8.01 3.87 4.00 0.17 1.39 0.61 2.00 2.00
1511-3-1
(N = 8)
MAX42.44 17.52 0.07 0.13 0.03 19.73 0.02 0.45 9.66 6.09 0.10 1.49 6.09 100.30 8.10 3.93 4.06 0.13 1.56 0.98 2.00 2.00
MIN41.59 16.42 0.02 0.06 0.01 19.06 0.01 0.28 5.63 3.77 0.01 1.46 5.98 98.00 7.96 3.74 3.96 0.08 0.90 0.61 2.00 2.00
AVG41.96 16.95 0.05 0.09 0.01 19.48 0.02 0.36 8.12 4.61 0.05 1.48 6.04 99.15 8.04 3.83 4.00 0.10 1.30 0.75 2.00 2.00
1511-3-2
(N = 7)
MAX42.53 17.72 0.00 0.03 0.02 19.91 0.02 0.43 8.91 6.62 0.06 1.50 6.14 100.30 8.07 3.94 4.07 0.12 1.42 1.06 2.00 2.00
MIN41.93 17.22 0.00 0.01 0.01 19.51 0.01 0.37 5.43 3.78 0.02 1.48 6.05 98.70 8.00 3.85 4.00 0.11 0.87 0.61 2.00 2.00
AVG42.22 17.33 0.00 0.02 0.01 19.75 0.01 0.39 7.30 5.12 0.04 1.49 6.09 99.76 8.03 3.88 4.02 0.11 1.16 0.83 2.00 2.00
1511-3-3
(N = 8)
MAX42.82 17.67 0.09 0.07 0.02 19.89 0.02 0.53 9.83 6.37 0.21 1.50 6.15 100.80 8.10 3.94 4.04 0.15 1.57 1.02 2.00 2.00
MIN41.89 16.77 0.02 0.04 0.01 19.26 0.01 0.24 5.72 3.57 0.02 1.48 6.07 99.50 7.99 3.76 3.89 0.07 0.91 0.58 2.00 2.00
AVG42.41 17.28 0.04 0.06 0.01 19.57 0.02 0.40 8.01 4.58 0.11 1.49 6.10 99.90 8.05 3.86 3.98 0.11 1.27 0.74 2.00 2.00
1511-20-1
(N = 4)
MAX42.73 18.09 0.03 0.03 0.03 20.05 0.01 1.29 8.95 7.64 0.02 1.51 6.18 100.10 8.06 4.00 4.03 0.36 1.40 1.23 2.00 2.00
MIN42.07 17.44 0.01 0.03 0.01 18.49 0.01 0.56 5.01 1.31 0.02 1.48 6.08 99.20 8.01 3.92 3.76 0.16 0.79 0.21 2.00 2.00
AVG42.44 17.79 0.02 0.03 0.02 19.46 0.01 0.92 7.08 4.20 0.02 1.50 6.13 99.55 8.03 3.97 3.95 0.26 1.12 0.68 2.00 2.00
1511-20-2
(N = 7)
MAX43.29 18.25 0.04 0.07 0.02 19.81 0.02 1.69 6.58 6.25 0.06 1.51 6.19 100.20 8.10 4.04 3.99 0.47 1.03 1.01 2.00 2.00
MIN42.57 17.56 0.01 0.01 0.01 19.24 0.01 0.55 5.25 3.50 0.02 1.49 6.09 99.00 8.00 3.93 3.87 0.16 0.83 0.56 2.00 2.00
AVG42.86 17.95 0.03 0.03 0.02 19.45 0.01 1.50 5.87 4.26 0.04 1.51 6.17 99.61 8.05 3.97 3.91 0.42 0.92 0.68 2.00 2.00
* H2O and B2O3 content and number of ions based on 32(O, OH) cation.
Table 5. Major element compositions (wt%) of the actinolite.
Table 5. Major element compositions (wt%) of the actinolite.
Sample SiO2TiO2Al2O3Cr2O3FeOMnOMgOCaONa2OK2ONiOSnO2P2O5TotalSiAlCrFeMnMgCaNaK
LM-4X
(N = 3)
MAX55.92 0.04 2.19 1.76 26.59 0.87 5.13 11.54 0.21 0.13 0.05 0.10 0.00 99.67 8.23 0.38 0.20 3.31 0.11 1.13 1.83 0.06 0.02
MIN54.51 0.01 1.77 0.02 23.27 0.42 4.67 10.16 0.17 0.11 0.00 0.00 0.00 99.38 8.08 0.31 0.00 2.86 0.05 1.04 1.60 0.05 0.02
AVG55.11 0.02 1.97 0.89 24.79 0.72 4.94 10.67 0.19 0.12 0.03 0.06 0.00 99.51 8.17 0.34 0.10 3.07 0.09 1.09 1.69 0.05 0.02
LM-5X
(N = 3)
MAX52.64 0.06 2.48 1.37 28.66 1.07 5.52 12.37 0.28 0.21 0.06 0.07 0.01 101.58 7.85 0.44 0.16 3.58 0.14 1.24 2.00 0.08 0.04
MIN51.11 0.05 1.95 0.14 26.31 0.60 4.83 11.64 0.18 0.18 0.00 0.00 0.00 100.36 7.69 0.34 0.02 3.32 0.08 1.07 1.88 0.05 0.03
AVG51.72 0.05 2.17 0.82 27.61 0.79 5.21 12.06 0.24 0.19 0.02 0.02 0.01 100.91 7.76 0.38 0.10 3.47 0.10 1.17 1.94 0.07 0.04
LM-17X
(N = 3)
MAX50.49 0.05 3.59 0.93 28.49 0.92 5.38 12.44 0.24 0.26 0.06 0.02 0.03 100.12 7.68 0.64 0.11 3.62 0.12 1.23 2.03 0.07 0.05
MIN49.87 0.02 2.42 0.09 26.80 0.67 5.07 11.82 0.15 0.17 0.00 0.00 0.00 98.83 7.63 0.44 0.01 3.41 0.09 1.15 1.95 0.04 0.03
AVG50.17 0.03 2.89 0.38 27.49 0.78 5.23 12.08 0.20 0.20 0.03 0.01 0.01 99.50 7.66 0.52 0.04 3.51 0.10 1.19 1.98 0.06 0.04
LM-22X
(N = 3)
MAX50.10 0.08 3.51 0.62 26.61 0.90 6.24 12.93 0.24 0.26 0.01 0.05 0.01 98.54 7.69 0.64 0.08 3.41 0.12 1.43 2.14 0.07 0.05
MIN49.05 0.03 2.38 0.12 25.89 0.57 4.97 12.00 0.15 0.23 0.00 0.03 0.00 98.21 7.57 0.43 0.01 3.34 0.07 1.14 1.97 0.04 0.04
AVG49.55 0.06 2.88 0.29 26.28 0.71 5.78 12.31 0.20 0.24 0.01 0.04 0.01 98.36 7.63 0.52 0.03 3.38 0.09 1.32 2.03 0.06 0.05
1511-1
(N = 3)
MAX51.84 0.04 2.28 0.86 27.66 0.87 7.11 12.21 0.23 0.17 0.01 0.00 0.02 100.25 7.76 0.40 0.10 3.55 0.11 1.59 1.96 0.07 0.03
MIN50.47 0.04 1.99 0.06 24.76 0.73 5.72 11.58 0.16 0.15 0.00 0.00 0.00 98.77 7.72 0.36 0.01 3.10 0.09 1.31 1.91 0.05 0.03
AVG50.99 0.04 2.13 0.41 26.15 0.80 6.41 11.90 0.19 0.16 0.00 0.00 0.01 99.20 7.74 0.38 0.05 3.32 0.10 1.45 1.94 0.06 0.03
Number of ions based on 23 oxygen atoms.
Table 6. Major element compositions (wt%) of the epidote.
Table 6. Major element compositions (wt%) of the epidote.
Sample SiO2TiO2Al2O3Cr2O3FeOMnOMgOCaONa2OK2ONiOSnO2P2O5TotalSiAlFeCaHEp
1511-7 (N = 4)MAX39.09 0.11 25.12 0.06 10.33 0.25 0.04 24.85 0.00 0.01 0.04 0.03 0.05 97.39 3.18 2.42 0.70 2.16 1.00 23.30
MIN37.45 0.01 22.85 0.02 9.57 0.16 0.00 23.65 0.00 0.00 0.00 0.00 0.00 95.79 3.06 2.19 0.65 2.07 1.00 21.28
AVG38.17 0.06 23.97 0.04 9.95 0.18 0.02 24.12 0.00 0.01 0.02 0.01 0.02 96.56 3.12 2.31 0.68 2.11 1.00 22.77
1511-10 (N = 4)MAX37.28 0.12 22.98 1.06 12.55 0.14 0.03 24.35 0.03 0.01 0.04 0.05 0.07 96.54 3.12 2.27 0.88 2.20 1.00 29.87
MIN36.15 0.00 20.91 0.26 11.12 0.04 0.00 23.17 0.00 0.00 0.02 0.00 0.00 95.32 3.03 2.07 0.78 2.08 1.00 25.80
AVG36.76 0.04 22.07 0.65 12.08 0.09 0.02 23.89 0.01 0.00 0.03 0.03 0.03 95.70 3.08 2.18 0.85 2.15 1.00 28.00
590-21 (N = 3)MAX38.44 0.08 22.84 0.04 12.07 0.22 0.06 23.84 0.02 0.01 0.09 0.05 0.03 97.53 3.14 2.20 0.82 2.08 1.00 27.35
MIN37.74 0.05 22.53 0.03 11.83 0.19 0.05 23.47 0.00 0.00 0.00 0.00 0.01 96.15 3.13 2.19 0.81 2.08 1.00 26.88
AVG38.14 0.07 22.70 0.04 11.92 0.20 0.05 23.68 0.01 0.01 0.05 0.03 0.02 96.91 3.13 2.20 0.82 2.08 1.00 27.14
Number of ions based on 12.5 oxygen atoms. Ep = clinozoisite component in epidote (Fe3+/(Fe3+ + AlVI) × 100.
Table 7. Trace element compositions (ppm) of the axinite.
Table 7. Trace element compositions (ppm) of the axinite.
Sample BePScTiVCrGaGeAsSrZrNbMoInSnSbCsBaLaCePrNd
1511-3
(N = 8)
MAX26.926810.424.831984.428.33.78.914.62.00.010.290.881620.560.113.80.050.210.050.31
MIN4.42201.312.522021.016.92.80.8212.20.080.010.170.3031.60.160.050.040.010.060.010.05
AVG14.82446.217.629658.020.33.33.213.70.770.010.250.4864.80.240.081.90.020.120.020.15
1511-20
(N = 11)
MAX43.410667.415118616817.38.43.433.639.42.40.338.97760.882.03.20.561.460.302.33
MIN1.32710.5458.91095.911.05.31.215.66.60.040.113.01620.130.130.030.050.240.050.30
AVG18.63802.992.314261.613.26.62.721.918.60.540.265.74130.481.00.660.210.660.130.88
Sample SmEuGdTbDyHoErTmYbLuYHfTaWPbThUΣREELREE/HREELaN/YbNδEuδCe
1511-3
(N = 8)
MAX0.140.030.260.060.440.080.200.050.220.032.210.110.000.010.090.010.011.941.543.390.702.20
MIN0.040.010.050.010.090.020.030.010.010.010.450.010.000.010.050.010.010.440.430.000.000.74
AVG0.080.020.150.030.200.040.090.020.100.021.100.000.000.010.070.010.010.980.840.980.151.24
1511-20
(N = 11)
MAX1.260.232.220.553.941.134.270.593.760.3840.401.150.010.110.850.690.2219.550.590.190.571.31
MIN0.160.030.580.171.480.411.700.271.330.0915.100.180.010.010.200.020.019.390.100.010.270.86
AVG0.490.101.160.292.640.702.480.362.320.2424.620.510.010.060.450.200.1212.640.240.070.391.04
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He, L.; Liang, T.; Wang, D.; Zhang, J.; Liu, B. Skarn Formation and Zn–Cu Mineralization in the Dachang Sn Polymetallic Ore Field, Guangxi: Insights from Skarn Rock Assemblage and Geochemistry. Minerals 2024, 14, 193. https://doi.org/10.3390/min14020193

AMA Style

He L, Liang T, Wang D, Zhang J, Liu B. Skarn Formation and Zn–Cu Mineralization in the Dachang Sn Polymetallic Ore Field, Guangxi: Insights from Skarn Rock Assemblage and Geochemistry. Minerals. 2024; 14(2):193. https://doi.org/10.3390/min14020193

Chicago/Turabian Style

He, Lei, Ting Liang, Denghong Wang, Jianxin Zhang, and Bosheng Liu. 2024. "Skarn Formation and Zn–Cu Mineralization in the Dachang Sn Polymetallic Ore Field, Guangxi: Insights from Skarn Rock Assemblage and Geochemistry" Minerals 14, no. 2: 193. https://doi.org/10.3390/min14020193

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