Yuzhou Zhuo·Yong Huang·Jinwei Li·Wei Gao·Jinxiang Li
Abstract Mercury mines in Guizhou province are the main base of mercury production and the most important resource base in China.The San-Dan mercury belt in Guizhou province contains a series of important mercury deposits.However,the source of metallogenic materials and the properties of metallogenic fluid of these mercury deposits have long been a controversial issue.In this study,we used cathode luminescence techniques to distinguish different stages of dolomite and calcite,laser ablation inductively coupled plasma mass spectrometry to analyze the trace elements,and stable isotope mass spectrometry techniques to analyze C—O isotopes compositions of dolomite and calcite in the Sixiangchang mercury deposit in San-Dan mercury belt.We also measured the sulfur isotope composition of cinnabar.Our study showed that dolomite can be divided into two stages,the lumpy dolomite associated with cinnabar in Dol 1 stage and dolomite vein in Dol 2 stage,which is associated with Cal 2 stage calcite vein.With the progress of mineralization,Al,As,Mo,Sb,and Sr elements were gradually enriched in the ore-forming fluid.The rare earth element(REE)partition curve of Dol 1 stage dolomite showed a trend of light REE enrichment.Cal 2 stage calcite and Dol 2 stage dolomite exhibited a flat-type REE partition curve,and Dol 2 stage dolomite showed a strong negative anomaly for Eu.δ13C of carbonate mineral variation ranges from-6.89 to-2.16%,while δ18O variation ranges from 13.80 to 23.09%,and the δ34S variation range of cinnabar is 16.51—24.28%.Carbonate mineral trace elements and C—O isotopes compositions suggested that early ore-forming fluid was reduced,and late ore-forming fluid was oxidized.The oreforming fluid of the Sixiangchang mercury deposit is a mixture of deep crustal fluid and meteoric water in deep thermal circulation, and involved in the oxidation of organic matter.The cinnabar δ34S results showed that sulfur mainly came from seawater sulfate with the participation of microbial reduction.Sulfur is sedimentary in origin and was derived mainly from the host-rock strata.
Keywords Trace elements·Carbon and oxygen isotopes·Sulfur isotope·Calcite and dolomite·Youjiang Basin
The distribution of mercury resource is extremely uneven,with three-quarters of global mercury production comes from five major mercury mining zones(Rytuba 2003).The Almaden mercury belt of central Spain alone accounts for one-third of the world's mercury production(Saupe 1990).There are many genetic types of mercury deposit.Rytuba(2003)suggested that mercury mine could be divided into three types: silica-carbonate, hot-spring, and Almaden.China is rich in mercury resource,and mercury deposits are distributed throughout the country.Guizhou province is the most abundant province of mercury resources in China(He 1990).In Guizhou province,the San-Dan mercury ore belt is the most important mercury ore belt.It is located in the northeast of the Guizhou province.San-Dan mercury ore belt is an important area of mercury and an important part of the large area of low-temperature mineralization in southwest China(Yan et al.1989).
As a kind of unique mineralization type, mercury deposits in southwest China have their own distinct geochemical characteristics.Carbonate is the main host-rock and the ore deposit is obviously strata-bound(Cambrian,Ordovician).The metallogenic age is Yanshanian,and the cause has nothing to do with magmatic rocks such as the difference between the other types of mercury(Wang and Wen 2015).Therefore,research of the mercury deposit in southwest China has high significance(Yan et al.1989).However,the source of metallogenic materials and the properties of ore-forming fluid have long been a controversial issue.Some scholars researched C and O isotopes of calcite,Pb and S isotopes of sulfide,and their result suggested that the ore-forming fluid of the mercury mine was related to the hydrocarbon brine containing organic matter in the ancient reservoir(Bao et al.1999;Shi 1991;Li et al.2002;Wang and Gao 2017).Yan et al.(1989)through field geological observation and mercury concentration test in host-rock suggested that the mercury mainly comes from the host-rock.However,previous studies mainly focused on the study of field geology,and ignored the division of metallogenic stage. The studies did not have detailed mineralogical research,and published data of isotopes and trace elements were very few.
In recent years,with the development of microanalysis technology,there have been a lot of studies on the geochemical study of pyrite and quartz in Carlin-type gold deposit(Hu and Zhou 2012;Hu et al.2017;Su et al.2009, 2018). However, these analytical techniques are rarely used in the study of mercury deposit.In this study,we use laser ablation inductively coupled plasma mass spectrometry(LA-ICP-MS)technique in conjunction with textural studies utilizing the cathode luminescence(CL)technique to measure the trace elements of calcite and dolomite in different mineralization stage of Sixiangchang deposit in the San-Dan metallogenic belt.We measured δ13C and δ18O in different stages of calcite and dolomite,and measured δ34S of cinnabar.The goal of this study is to document the sources and properties of the ore-forming fluid of the Sixiangchang mercury deposit,and trace the source of S element.Our new data provide evidence of the properties and sources of ore-forming fluid.
The San-Dan metallogenic belt is located in the northeast margin of Youjiang basin,Southwest China(Fig.1).This metallogenic belt resides at the junction of Yangtze craton and the South China fold belt(Huang and Du 1993).The Sixiangchang mercury deposit is located in the middle of the San-Dan metallogenic belt(Fig.1)(Huang and Du 1993),which is in the northeastern margin of the Youjiang basin.The Youjiang basin is bound to the northeast by the Shuicheng-Ziyun-Bama fault,southwest by the Mile-Shizong fault and Nanpanjiang fault,and to the southeast by the Youjiang fault,which separates the Youjiang basin from the Cathaysia block(Su et al.2008,2012,2018).The San-Dan metallogenic belt is 150 km long and 20—30 km wide, which have Sixiangchang, Shuiyinchang, Hongfachang,Jiaoli and other dozens of mineral deposits(Lei et al.2012).Many mineral deposits have been exhausted.The main strata exposed in this area are the Cambrian basement,and Paleozoic and Triassic strata(Fig.1).The lithology of Cambrian basement is mainly blastopsammite and siliceous rock.Paleozoic and Triassic strata lithology is limestone,sandstone,siltstone,shale,and dolomite(Hu et al.2002).The age of Rb—Sr in the whole rock of Carlintype gold deposit tested by Jia et al.(1993)in Danzhai Hongfachang was 400 and 114 Ma.Wang et al.(2015)researched the Sm—Nd isotopes of calcite in Danzhai Jiaoli mercury deposit,and obtained the isochronic age was 129±20 Ma.They suggested that the deposit was formed in the late Yanshanian Period.Magmatic activity in this area is very weak.Granite plutons with ages varying from Triassic(or Indosinian)to Jurassic-Cretaceous(or Yanshanian)are present at the southwest margin of Youjiang Basin(Hu et al.2002,2017;Hu and Zhou 2012).Variscan and Indosinian diabase are deposited in the southeast of the basin(Du et al.2013).Variscan and Indosinian mafic dyke are deposited in the part of the basin(Du et al.2013)(Fig.1).
The Sixiangchang mercury deposit is located at the passive edge of the Yangtze plate,southeast of Guizhou province,and contains Sandu-Danzhai mercury,antimony,gold and arsenic polymetallic mineralization(Xie et al.2014).The main element of the Sixiangchang deposit is mercury,and the auxiliary element is gold,in which the average grade of gold is 7.19 g/t(Huang and Du 1993).
The oldest strata in this area composed of the Proterozoic Xiajiang group,which is distributed in the eastern part of the mining area(Li et al.2013)(Fig.2).Xiajiang group lithology is mainly blastopsammite and sandy slate.The Sinian strata also distributed in the eastern part of the deposit,and the lithology is mainly carbonaceous shale,dolomite,and sandy slate.Cambrian strata are the main ore-bearing host-rock of the deposit,in which the lower and middle Cambrian lithology is mainly dolomite and limestone,and the upper Cambrian lithology is clay shale,carbonaceous shale,and limestone.The upper CambrianYangjiawan formation is the main ore-bearing strata.The Ordovician strata are mostly missing due to tectonic activity and the lithology of the remaining strata is mainly bioclastic limestone and dolomite.Silurian strata are distributed in the western side of the mining area(Fig.2),with a lithology of sandstone and limestone.Devonian strata are also distributed in the western side of the deposit,and the lithology is dolomite,limestone,and quartz sandstone(Yan et al.1989).The ore minerals in the Sixiangchang mercury deposit are mainly composed of
cinnabar,pyrite,natural mercury,and stibnite(Figs.3f,d,4c,i),and the gangue minerals are mainly quartz,calcite,and dolomite(Figs.3a,c,4a,f).The alteration of the hostrock primarily includes silicification(Fig.4f),pyritization(Fig.4c),and dolomitization(Fig.4e).There is strong tectonic activity in the mining area,which belongs to the multi-twist structure of the different grades of the neocathaysian system(Lei et al.2012).Faults,folds,and other structural phenomena in the area are complex and changeable,with the multi-character structure being the most developed and the meridional structural movement as the main structure(Fig.2)(Huang and Du 1993).There is no magmatic rock outcrop in the mining area.

Fig.2 Geological map of the Sixiangchang mercury deposi.Modified from Huang and Du(1993)
Our samples for experimental analyze are from outcrops and ores in the mine pits of Sixiangchang mercury deposit.Twenty-seven samples were used for trace elements and isotopes analysis.The main lithology of the samples is sandstone,siltstone,and calcareous siltstone(Table 2).The carbonate mineral in the samples was lumpy and veined.The cinnabar in the samples is intergrowth with calcite and dolomite(Fig.3).Six rock slice samples were used for the analysis of carbonate mineral trace elements.The trace elements of calcite and dolomite were analyzed on rock slice by the LA-ICP-MS method.Sixteen samples were used for carbonate mineral δ13C and δ18O analysis.Seventeen cinnabar samples were used for the analysis of δ34S.The carbonate mineral and cinnabar was crushed to 40—60 mesh and rinsed with ultrapure water.The impurity will be removed,so that the mineral purity of more than 99%,then dry the samples and grind the pure carbonate mineral and cinnabar in an agate mortar until it is less than 200 mesh.Finally,analyzed δ13C,δ18O and δ34S of these carbonate mineral and cinnabar samples.
The cathode luminescence was conducted at the State Key Laboratory of Ore Deposit Geochemistry(SKLODG)of the Institute of Geochemistry,Chinese Academy of Sciences (IGCAS) in Guiyang, China, using a Reliotron luminoscope(produced by America Relion industries use).The luminoscope was operated with an accelerating voltage of 5 kV,a current of 500 μA,and a vacuum degree of 80—90 mTorr(Wei et al.2015).

Fig.3 The hand specimens of calcite and dolomite at different stages collected from Sixiangchang mercury deposit.a Carbonaceous clay rock sample with disseminated cinnabar and Dol 1 stage dolomite.b Sandstone sample with disseminated cinnabar and Dol 1 stage dolomite.c Carbonaceous clay rock sample with symbiosis cinnabar and Cal 2 stage calcite vein.d Carbonaceous siltstone sample with Dol 1 stage dolomite and natural mercury.e Silty clay sample with Dol 2 stage dolomite vein associated with cinnabar.f Carbonaceous clay sample with Dol 2 stage dolomite vein associated with cinnabar

Fig.4 The microscopic mineral photos(with a Leica DM 2500 P microscope)of calcite and dolomite at different stages collected from Sixiangchang mercury deposit.a Cal 2 stage calcite vein associated with cinnabar is embedded in quartz vein.b Quartz vein contains veined cinnabar.c Cinnabar,pyrite,and quartz symbiosis.d Dol 1 stage dolomite fractures are filled with fine cinnabar.e Cinnabar is disseminated in the Dol 1 stage dolomite.f Quartz and cinnabar grains are encapsulated and encased.g Cinnabar particles and bitumen embedded in quartz particles.h Dol 2 stage dolomite vein contain fine cinnabar.i Cinnabar and stibnite are symbiotic.Qz quartz,Cal calcite,Cnb cinnabar,Dol dolomite,Snt stibnite
Calcite trace elements were analyzed at the SKLODG of the IGCAS.Laser sampling was performed using a GeoLas Pro 193 nm ArF excimer laser(produced by Germany Coherent).An Agilent 7500×ICP-MS instrument(produced by Agilent)was used to acquire ion-signal intensities.Helium was applied as a carrier gas which was mixed with Argon via a T-connector before entering the ICP-MS.Each analysis incorporated a background acquisition of approximately 30 s(gas blank)followed by 50 s of data acquisition from the sample.
The trace elements tested in this experiment include Li,Be,B,Na,Mg,Al,Si,P,K,Sc,Ti,V,Cr,Mn,Fe,Co,Ni,Cu,Zn,Ga,Ge,As,Rb,Sr,Y,Zr,Nb,Mo,Ag,Cd,Sn,Sb,Cs,Ba,Hf,Ta,Au,Pb,Th,U and REE.If the concentrations of analyzed elements are <0.1 μg/g, we considered the analyzed results unreliable.Element concentration was calibrated against multiple-standard reference materials(NIST 610,NIST 612)(Jochum et al.2015)combined with carbonate reference material MACS-3 as internal standardization.The parameters of the reference material are shown in the literature(Chen et al.2011;Jochum et al.2012).The laser ablation frequency was 5 Hz,the laser beam spot was 44 μm.A set of standard samples was tested after 10 sample points finished,with an analysis error of less than 10%.Off-line selection and integration of background and analyte signals,and timedrift correction and quantitative calibration were performed by ICPMSDataCal(Liu et al.2008,2010).
4.4.1 C-O isotopes analysis of calcite and dolomite
Calcite and dolomite carbon and oxygen stable isotopes were conducted at the SKLODG of the IGCAS.Carbon and oxygen stable isotopes were carried out with a ThermoFisher MAT 253 mass spectrometer (produced by America ThermoFisher).The samples were reacted with 100%concentrated H3PO4in a vacuum at 72°C for 12 h.The released CO2was analyzed for carbon and oxygen isotopes.Isotopic data are reported in%relative to the Peer Dee Belemnite(PDB)for carbon and oxygen.The following standards were used for internal calibration standards:GBW04416(calcite,δ13CPDB=1.61%,δ18-OPDB=-11.59%),GBW04405(calcite,δ13CPDB=0.57%, δ18OPDB=-8.49 %), NBS18 (calcite, δ13CPDB-=-5.01%,δ18OPDB=-23.2%)and L-SVEC(lithiumcarbonate, δ13CPDB=-46.6 %, δ18OPDB=-26.7%).The analytical precision at 2σ for δ13C and δ18O are±0.2 and±2.0%,respectively(Zhou et al.2017).The δ13C and δ18O test results are shown in Table 1.The values of δ18OSMOW(Vienna Standard Mean Ocean Water)were calculated based on the equation of Friedman and O'Neil(1977),where δ18OSMOW=1.03086×δ18OPDB+30.86.
4.4.2 S isotope analyze of cinnabar
The sulfur isotope of cinnabar was analyzed at the SKLODG of the IGCAS.Cinnabar with a purity of greater than 99%was selected and ground to 200 mesh in agate mortars.A sample in a foil package was put into a small bottle before testing.Sulfides were combusted with copper oxide under vacuum at 1000°C to produce SO2which was used for the gas mass spectrometer measurements(Robinson and Kusakabe 1975).The cinnabar δ34S was analyzed with the ThermoFisher MAT253 stable isotope mass spectrometer.Isotopic data were reported as δ34S relative to IAEA-S-1(δ34SVCDT=-0.30%),IAEA-S-2(δ34SVCDT=22.62 %) and IAEA-S-3 (δ34SVCDT-=-32.49%)standards for sulfur(Zhou et al.2017).The relative error at 2σ was better than 0.1%.The sulfur isotope test results are shown in Table 2.
The carbonate minerals in the Sixiangchang mercury deposit are dolomite and calcite,but primarily dolomite.According to hand specimens and microscopic mineral assemblage observations, dolomite is divided into two stages,Dol 1 stage and Dol 2 stage,and calcite is characterized as Cal 2 stage.Dol 1 stage dolomite is primarily in the form of milky clumps and is distributed in the hostrock in an infective form with cinnabar(Figs.3a,b,4d).Dol 1 stage dolomite glows a bright red under cathode luminescence(Fig.5b,c),and dark in the area with high Fe concentration(Fig.5a,points 1 and 4).Dol 2 stage dolomite has milky white veins with cinnabar(Fig.3e,f).Dol 2 stage dolomite glows dark under cathode luminescence(Fig.5e).Cal 2 stage calcite is mainly in the form of milky white rough veins and infective with cinnabar(Figs.3c,4a).Cal 2 stage calcite vein glows bright red under cathode luminescence(Fig.5a,d).The detailed sequence of mineral symbiosis is shown in Fig.6.

Table 1 Carbon and oxygen isotopes compositions and calculated temperatures of carbonate mineral in Sixiangchang mercury deposit

Table 2 Sulfur isotope composition of cinnabar in Sixiangchang mercury deposit
The concentrations of Cu, Mn and Sn in calcite and dolomite in the Sxiangchang Hg deposit have small variation ranges than Fe,Sb and Sr(Fig.7).The elements with the highest concentrations in calcite and dolomite are Fe,Mg, Mn, Na,Si, Sr, and Al, with the concentrations ranging from tens to thousands of ppm(Fig.7).The concentrations of Cu,Mo,Zn,As,Sb,Sn range from below the detection limit to tens of ppm.The concentrations of Sr and As in calcite are higher than dolomite,which indicates that these two elements are more likely to enter calcite.

Fig.5 The cathode luminescence photos of calcite and dolomite at different stages collected from Sixiangchang mercury deposit.(Mn,Fe)represent the concentrations of Mn and Fe of calcite and dolomite,the concentration unit is μg/g.a Cal 2 stage calcite glows bright red under cathode luminescence,symbiotic with Dol 1 stage dolomite,which glows dark red under the same luminescence.a,b are the cathode luminescence photos of the sample SXC-9(Fig.3a).b The red glow of Dol 1 stage dolomite.c Dol 1 stage dolomite glows bright red under cathode luminescence and glows dark red in local areas.c Cathode luminescence photo of the sample SXC-18(Fig.3b).d The bright red glow of Cal 2 stage calcite.d Cathode luminescence photo of the sample SXC-5(Fig.3c).e The bright red and dark red interphase of Dol 2 stage dolomite.e Cathode luminescence photo of the sample SXC-1(Fig.3f).From this cathode luminescence photo,we can see that the area of the bright red cathode light calcite tends to have a higher content of Mn and a lower content of Fe,and areas with a dark red cathode light tend to have lower levels of Mn and higher levels of Fe.f The bright red glow of Dol 2 stage dolomite.f Cathode luminescence photo of the sample SXC-23(Fig.3e).Cathode luminescence photos of SXC-9-1-2,SXC-18-3,SXC-5-1 and SXC-23-2 are similar with the photos of SXC-9-1-1,SXC-18-2,SXC-5-2 and SXC-23-1 respectively,so we didn't show them in the text

Fig.6 Generalized alteration and ore mineral paragenesis of the Sixiangchang mercury deposit

Fig.7 Box diagram of characteristic trace elements of different stages of calcite and dolomite in Sixiangchang mercury deposit.Cal 2 is representative of Cal 2 stage calcite,Dol 1 is representative of Dol 1 stage dolomite,Dol 2 is representative of Dol 2 stage dolomite
The REE distribution forms of calcite and dolomite in Sixiangchang mercury deposit are flat and light REE enrichment(Fig.8).The Cal 2 stage calcite exhibits a flattype(Fig.8c)REE partition curve with the ΣREE concentration varies from 16.27 ppm to 132.33 ppm.Dol 1 stage dolomite exhibits light REE enrichment(Figs.8a,b),and the ΣREE concentration varies from 4.43 to 289.07 ppm.The REE of the Dol 2 stage dolomite are distributed in a flat pattern with a strong Eu negative anomaly(Fig.8d—f),and the ΣREE concentration varies from 2.45 to 301.62 ppm.

Fig.8 Chondrite-normalized rare earth element(REE)patterns of different stages of calcite and dolomite in the Sixiangchang mercury deposit.Sample/chondrite of Y axis means the ratio of rare earth elements in samples to those in C1 carbonaceous chondrite.a Chondrite-normalized REE pattern of the sample of SXC-9.SXC-9-1 represents the first cathode luminescence field of sample SXC-9.SXC-9-1-1 represents the first test point of the first cathode luminescence field of sample SXC-9(Fig.5a).The rare earth partition numbers in other figures are similar to this.b Chondrite-normalized REE pattern of the sample of SXC-9.c Chondrite-normalized REE pattern of the sample of SXC-5.d Chondritenormalized REE pattern of the sample of SXC-1.e Chondrite-normalized REE pattern of the sample of SXC-23.f Chondrite-normalized REE pattern of the sample of SXC-23
In our study,we selected 15 dolomite samples and 1 calcite sample for carbon and oxygen isotope analysis.The δ13C(%V-PDB)is in the range of-4.21 ~-2.16%in Dol 1 stage dolomite,-6.89 ~-2.27%in Dol 2 stage dolomite,and-6.13%in Cal 2 stage calcite(Table 1).The δ18O(%S-MOW)is in the range of 13.80—21.27%in Dol 1 stage dolomite, 15.77—23.09% in Dol 2 stage dolomite,and 18.93%in Cal 2 stage calcite.According to the calcite-carbon dioxide conversion formula:1000 lnα=2.962-11.346×103/T+5.358×106/T2-0.388×109/T3(T=0—3727°C) (Chacko et al.1991)and the calcite fluid inclusion temperature data,the calcite carbon isotope can be converted into the fluid carbon dioxide carbon isotope value.1000 ln α=δ13CCaCO3-δ13CCO2,T representative Kelvin temperature.The Dol 1 stage dolomite formation temperature is 200°C,and the Dol 2 stage dolomite and Cal 2 stage calcite fluid inclusion homogenization temperatures are 150°C(Table 1).Calcite fluid inclusion homogenization temperature data are shown in the literature(Huang and Du 1993;Li et al.2002,2013;Li and Zhou 1988).The δ13C value of carbon dioxide is calculated to be in the range of-3.46 ~-1.42%in Dol 1 stage dolomite,-7.84 ~-3.22%in Dol 2 stage dolomite,and-7.08%in Cal 2 stage calcite.According to the calcite-fluid oxygen isotope conversion formula:1000 ln α=2.78×106/T2-3.39 (T=0—500°C)(O'Neil et al.1969),and calcite fluid inclusion homogenization temperature data.The calcite oxygen isotope can be converted into the fluid oxygen isotopic value.1000 ln α=δ18OCaCO3-δ18OH2O,T representative Kelvin temperature.The calculated result is as follows:the δ18O value of fluid oxygen to be in the range of 4.77—12.25%in Dol 1 stage dolomite,3.63—10.96%in Dol 2 stage dolomite,and-6.08%in Cal 2 stage calcite.
In this experiment,we selected 17 cinnabar samples for sulfur isotope analysis,in which cinnabar was symbiotic with calcite and dolomite. The range of δ34S is 12.08—24.28%(Table 2).For one cinnabar sample with symbiotic host-rock,δ34S is 12.08%.While for other samples,δ34S are mainly above 20.00%.
In our study,we find that in dolomite,the area that glows bright red tends to have a higher content of Mn and a lower content of Fe(Fig.5e,points 2 and 3),and the area that glows dark red tends to have a lower content of Mn and a higher content of Fe(Fig.5e,points 1 and 4).The average concentrations of Al,As,Mo,Sb,and Sr in Dol 1 stage dolomite are lower than Dol 2 stage dolomite.This indicates that the fluid enriched these elements more in the late metallogenic period.The average concentrations of As,Cu,Si,Sn,and Sr in Cal 2 stage calcite are higher than Dol 1 and Dol 2 stages of dolomite.This indicates that these elements are easier access to calcite.
REEs are of particular interest in geoscience due to their use as chemical tracers of natural processes.As a result of their systematic electron configuration, they exhibit relatively similar chemical behavior. Their gradually varying ionic size,however,leads to distinct REE concentration patterns stemming from their aqueous complexation and their varying ability to incorporate into and/or adsorb onto solid phases(Mo¨ller et al.1991,2003;Mo¨ller 1997,2002).
In our study,the Dol 1 stage massive dolomite partition curve exhibits light REE enrichment.This REE distribution is the same as that of the host-rock(Zhuo et al.unpublished data).The Dol 2 stage dolomite vein and Cal 2 stage calcite vein symbiosis with cinnabar partition curve show a flattype(Fig.8c—f).In the Dol 2 stage dolomite,there is a strongly Eu negative anomaly(Fig.8d,e).The type of the REE partition curve indicates that the ore-forming fluid in Dol 1 stage dolomite is closer to the characteristics of the host-rock and the reaction degree between the fluid and host-rock in the early mineralization stage is greater than late mineralization stage.The negative anomaly of Eu indicates the late ore-forming fluid is oxidized.The Dol 2 stage dolomite and Cal 2 stage calcite are both veinshaped,and their REE distributions are both flat.Dol 2 stage dolomite shows an obvious Eu negative anomaly.These phenomena indicate that in the late metallogenic period,the fluid is more concentrated in heavy REE,and the metallogenic environment is more oxidized.
The carbon and oxygen isotopes composition of calcite and dolomite of hydrothermal ore deposits can provide important constraints on the origin of mineralizing fluids,alteration temperature,and size of a hydrothermal system(Zheng and Hoefs 1993).In our study,the δ18O values were in the range of 13.80—21.27%and 15.77—23.09%for Dol 1 and Dol 2 stage dolomite,and 4.77—12.25%and 3.63—10.96%for converted fluid δ18O values,respectively(Table 1).This indicates that the H2O of the mineralization fluid of the Sixiangchang mercury deposit is mainly from the dissolution of marine carbonate and mixes with H2O of sedimentary organic matter decarboxylation(Fig.9).The δ13C values ranged from-4.21 to-2.16%and-6.89 to-2.27%for Dol 1 and Dol 2 stage dolomite,and-3.46 to-1.42%and-7.84 to-3.22%for converted fluid δ13C of carbon dioxide,respectively.This indicates that the mineralization of CO2mainly comes from mantle degassing and sedimentary organic matter decarboxylation (Fig.9). Therefore, δ13C and δ18O of calcite and dolomite indicate that the ore-forming fluid is mainly dominated by the dissolution of marine carbonate and the decarboxylation of sedimentary organic matter.

Fig.9 Scheme diagram of the fluid source of Sixiangchang mercury deposit.The arrows show typical isotopic trends resulting from carbonate dissolution(Dis Carb),mixture(MT),decarboxylation of organic matter(Decbx),and the oxidation of organic matter(Oxid Org)[fields of mantle reservoir according to Hoefs(1997),Deme′ny et al.(2004);sedimentary marine carbonates reservoir according to Veizer et al.(1999),typical isotopic trends according to Hu et al.(2017)]
The δ34S values of cinnabar showed a narrow range of 16.51—24.28%,excluding one sample which had a δ34S value of 12.08%(Table 2).The strong local fluid-rock interaction experienced by sulfur between the formation water and the host-rock during fluid transport can affect the cinnabar sulfur isotope composition.The δ34S values of sulfide minerals are not always equal to that of the hydrothermal fluids from which they precipitated and are controlled by the physical and chemical conditions during the transport of hydrothermal fluids and precipitation of related minerals, namely, the total sulfur composition,temperature,oxygen fugacity(fO2),pH,and ionic strength(Ohmoto 1972).In the Sixiangchang deposit area,contemporaneous (Cambrian—Ordovician) seawater sulfate δ34S is about 30%(Yan et al.1989;Chang et al.2008)(Fig.10). There are three distinct reservoirs of δ34S(Rollinson 1993):(1)mantle-derived sulfur with δ34S value of 0%±3%(Chaussidon et al.1989),(2)seawater sulfur with δ34S value of 20%today,though this value has varied in the past,and(3)strongly reduced(sedimentary)sulfur with large negative δ34S values.The δ34S we measured to be less than the contemporaneous seawater sulfate δ34S value,which is mainly related to the participation of δ32S bio-sulfur in the ore-forming fluid.Our data and these phenomena indicate that the sulfur mainly comes from the host-rock(Cambrian strata)and is deposited into the area.

Fig.10 Diagram of the cinnabar sulfur δ34S of Sixiangchang mercury deposit.Blue solid point is our δ34S data.Variation of S isotopic through geologic time diagram.Modified from Chang et al.(2008)
In summary,according to dolomite and calcite δ13C and δ18O data,carbon and oxygen of carbonate minerals in Sixiangchang mercury deposit are the dissolution of marine carbonate and the decarboxylation of sedimentary organic matter.The ore-forming fluid is mainly heated recycling groundwater that was recharged by meteoric water.This groundwater may come from the deep crustal,because the carbon isotope composition of carbon dioxide in the oreforming fluid shows the characteristics of mantle carbon isotope composition.According to the result of REE concentration,the ore-forming fluids were reduced at the early stage,and gradually became oxidized with the progress of ore-forming.The sulfur isotope result showed that the sulfur is derived mainly of seawater sulfate with the participation of microbial reduction.Sulfur is sedimentary in origin,originating primarily from the host-rock strata.
Based on our study of the cathode luminescence characteristics of different stages of calcite and dolomite,trace elements and REEs,carbon and oxygen isotopes composition,and sulfur isotope composition of cinnabar,we can draw the following conclusions.
1. The Cal 2 stage calcite and Dol 2 stage dolomite exhibited a flat-type REE partition curve,and Dol 2 dolomite showed a strong negative anomaly for Eu.The REE partition curve of Dol 1 stage dolomite showed a trend of light REE enrichment.
2. Carbon and oxygen isotopes and trace elements data of dolomite and calcite indicate that,with the progress of mineralization,Al,As,Mo,Sb,and Sr were gradually enriched in the ore-forming fluid. The early oreforming fluid was reduced,and the late ore-forming fluid was oxidized. The ore-forming fluid of the deposit was a mixture of deep crustal fluid and meteoric water in deep thermal circulation,and was involved in the oxidation of organic matter.
3. Cinnabar sulfur isotope results showed that the sulfur was primarily derived from seawater sulfate with the participation of microbial reduction.Sulfur is sedimentary in origin,derived mainly from the host-rock(Cambrian strata).
AcknowledgementsThis study was funded by the National 973 Program of China (2014CB440906) and the key project of the National Natural Science Foundation of China(41230316).We thank Dai Zhihui and Tang Yanwen for LA-ICP-MS analysis,Gu Jing for C,O and S isotopes analysis.