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1.
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2.
Trace elements and rare earth elements (REE) of the sulfide minerals were determined by inductively-coupled plasma mass spectrometry. The results indicate that V, Cu, Sn, Ga, Cd, In, and Se are concentrated in sphalerite, Sb, As, Ge, and Tl are concentrated in galena, and almost all trace elements in pyrite are low. The Ga and Cd contents in the light-yellow sphalerites are higher than that in the brown and the black sphalerites. The contents of Ge, Tl, In, and Se in brown sphalerites are higher than that in light-yellow sphalerites and black sphalerites. It shows that REE concentrations are higher in pyrite than in sphalerite, and galena. In sphalerites, the REE concentration decreases from light-yellow sphalerites, brown sphalerites, to black sphalerites. The ratios of Ga/In are more than 10, and Co/Ni are less than 1 in the studied sphalerites and pyrites, respectively, indicating that the genesis of the Tianqiao Pb–Zn ore deposit might belong to sedimentary-reformed genesis associated with hydrothermal genesis. The relationship between LnGa and LnIn in sphalerite, and between LnBi and LnSb in galena, indicates that the Tianqiao Pb–Zn ore deposit might belong to sedimentary-reformed genesis. Based on the chondrite-normalized REE patterns, δEu is a negative anomaly (0.13–0.88), and δCe does not show obvious anomaly (0.88–1.31); all the samples have low total REE concentrations (<3 ppm) and a wide range of light rare earth element/high rare earth element ratios (1.12–12.35). These results indicate that the ore-forming fluids occur under a reducing environment. Comparison REE compositions and parameters of sphalerites, galenas, pyrites, ores, altered dolostone rocks, strata carbonates, and the pyrite from Lower Carboniferous Datang Formation showed that the ore-forming fluids might come from polycomponent systems, that is, different chronostratigraphic units could make an important contribution to the ore-forming fluids. Combined with the tectonic setting and previous isotopic geochemistry evidence, we conclude that the ore-deposit genesis is hydrothermal, sedimentary reformed, with multisources characteristics of ore-forming fluids.  相似文献   

3.
Optical cathodoluminescence microscopy (CLM) can provide very useful information both on mineral zoning formed during crystal growth and on variations in chemical composition of sphalerites which is reflected by their visible colors. Gem quality sphalerite crystals associated with dolomite, calcite and fluorite having 3 different visible colors - green, honey and brown - were studied to compare their mineral chemistry and CL characteristics. Electron microprobe analyses indicated essentially no significant differences in terms of major components. Although the common CL-quencher ferrous iron contents of all three were lower than 0.25 wt %, none of the sphalerites cathodoluminescenced: two (brown and honey) were non-CL, the green sphalerite showed very week CL in faint brown color. Other trace elements that were analyzed include Fe, Cd, Mn, Ag, Hg, In, Bi, Cu, Ge, and Ga. Fe, Cd, Ga and Cu were relatively higher than the others. Most significant differences with respect to the common trace elements include honey colored sphalerites are essentially Fe- and Cd-poor but rich in Ga, green sphalerites are Fe- and Cd- rich but poor in all the others, and brown sphalerites are rich in Cd. No conclusive relation between non-CL behavior of all three sphalerites and their trace element chemistry was established, however; low quantities of common CL activators in sphalerite crystal structures such as Mn, Cu, and In were the main cause of the non-CL behavior.  相似文献   

4.
The Eskay Creek, British Columbia, Canada, is a polymetallic, gold- and silver-rich, volcanic-hosted, massive sulfide deposit. The ore in the deposit is divided into subzones distinguished by mineralogy, texture, grade and metallurgical characteristics. This study presents the results of a mineralogical examination of three composite field samples, with emphasis on the chemistry of sphalerite. Sphalerite is associated with variable amounts of Hg-tetrahedrite and cinnabar, and an array of sulfides, sulphosalts and non-opaque minerals. Electron micro probe analyses of sphalerite in the three composite samples reveal wide variations in compositions. The Hg content in sphalerite in the three samples varies between 0.08 and 16.35 wt%, whereas the Fe content ranges from 0.33 to 2.29 wt%. The chemical formula of the sphalerite shows the compositional range (Zn0.89–0.98Hg0.01–0.09.Fe0.005–0.02)S. Sphalerite exhibits an almost perfect substitution of Hg and Zn, as shown by the negative covariance between them. Sphalerite with the highest Hg contents tends to have the lowest Fe concentrations. The highest Hg contents in sphalerite are recorded in the samples with the highest bulk Hg concentrations and with the highest cinnabar contents.

The compositional variations of sphalerite are important because they can be used in mapping ore forming fluids and indicate possible temporal variations. Second, determination of the compositional variation of the sphalerite in the mine has metallurgical implications because the mineral is an important Zn source. The mineralogical data indicate that non-physical processes (e.g. pyrometallurgy) must be used to separate Hg from Zn concentrates, with direct environmental implications, that is, release of metals, such as Hg, into the environment during mining and processing.  相似文献   


5.
The C. S. A. Mine is located near Cobar, central New South Wales. The copper-zinc-lead ores occur in Early Devonian rocks of the Cobar Super-Group. Lower greenschist (slate-grade) metamorphism has developed elongate lenticular ore systems parallel to the extension (down-dip) lineation in cleavage. FeS contents of sphalerites coexisting with pyrite and pyrrhotite outside and inside pressure shadows indicate much higher pressures (7.7 to 9.0 kbar) than those inferred from stratigraphic reasoning and the low metamorphic grade. The homogeneous distribution of Fe in sphalerites suggests equilibration with pyrite-pyrrhotite; and concentrations of Co and Ni in iron sulphides, and Mn, Cd and Cu in sphalerite are too low to have influenced phase relations in the FeS-ZnS pseudobinary system. The anomalously high pressures are therefore ascribed to reequilibration of sphalerite compositions with a monoclinic pyrrhotite-pyrite buffer. The FeS contents of the reequilibrated sphalerites apparently reflect the differing mean stress domains that exist outside and inside pressure shadows. This suggests that reequilibration occurred under the same stress distribution as produced the original pressure shadows, and implies FeS dissolution during the decay of the cleavage-producing structuro-metamorphic event. The commonly observed scatter of sphalerite compositions in low grade assemblages appears to record micro-scale mean stress domains, and thereby testifies to the pressure sensitivity of the mole percent FeS contents.  相似文献   

6.
Abstract: The gold deposit at Ashanti occurs in the Proterozoic Birimian formation of Ghana. Two main ore types mined from the deposit are gold-bearing quartz veins, and gold-sulfide disseminations in metasediments and metavolcanics. The main sulfide minerals in the gold-sulfide disseminated ores are arsenopyrite, pyrite and pyrrhotite, and to a very minor extent, sphalerite and tetrahedrite. Carbonate alteration and sericitization are prominent in the metavolcanics and the metasediments, respectively. In the quartz veins, pyrite and arsenopyrite commonly occur in small amounts, but gold mostly occurs in contact with tetrahedrite, chalcopyrite, galena, aurostibite, and sphalerite. Pyrrhotite is absent in the quartz veins.
Microprobe studies indicate that As content of homogeneous arsenopyrite grains ranges from 27. 0 to 31. 7 atm%, and gives mineralization temperatures from 170 to 430°C, although mostly from 300 to 400°C. Chlorite geothermometry using temperature dependence of substitution of Al for Si in the tetrahedral site gives formation temeratures of 330 to 400°C, comparable to the arsenopyrite temperatures. Applying sphalerite–pyrite–pyrrhotite geobarometry to sphalerite with FeS contents from 13. 6 to 12. 5 mol%, the pressure was estimated to be in a range from 5. 9 to 7. 0 kb at the stage of elevated temperatures.
Mineralogical observations, especially absence of pyrrhotite in the quartz veins, together with microprobe data for gold and associated minerals suggest that the fluids having ascended through fissures in the Ashanti deposit were reduced by the reaction with carbonaceous materials in the metasediments during the declining stage of the regional metamorphism.  相似文献   

7.
胡雄伟 《地球学报》1991,12(1):91-100
电子探针研究表明江西大吉山矿床二云母花岗岩和白云母花岗岩中副矿物闪锌矿为富镉闪锌矿(Cd,4.34—19.89％,wt％,下同),铁含量低(Fe,1.03—4.24),尤以具W、Be、Ta、Nb矿化的白云母花岗岩中闪锌矿镉含量为高,并随岩体由下到上(标高的增大)而增高。矿物中Cd+Fe与Zn之间存在良好的线性负相关关系,指示了主要类质同象替代发生在Cd、Fe与Zn之间。矿物中可能存在不等位替代现象和四面体空位。富镉闪锌矿晶胞参数为0.54250—0.54440nm,随矿物中Cd含量的增加而增大。对照表明,当矿物中镉含量特别高时,Skinner(1961)晶胞参数计算公式估计值偏大,需作重新修正。最后,文章对富镉闪锌矿的成因意义进行了讨论。  相似文献   

8.
广东天堂铜铅锌多金属矿床Rb-Sr等时线年龄及其地质意义   总被引：19，自引：7，他引：12  
文章选取8件闪锌矿、3件方铅矿和1件黄铁矿样品,采用Rb-Sr等时线定年方法测定天堂铜铅锌多金属矿床的成矿时代.获得闪锌矿等时线年龄为(98.1±1.6) Ma,闪锌矿+方铅矿等时线年龄为(99±2)Ma,闪锌矿+方铅矿+黄铁矿等时线年龄为(98.2±1.3) Ma,闪锌矿+黄铁矿等时线年龄为(97.87±0.96) Ma,方铅矿+黄铁矿等时线年龄为(98.6±4.2) Ma.Rb-Sr定年结果表明,天堂铜铅锌多金属矿床的成矿时代为98 Ma左右,矿床形成于晚白垩世早期,可能与135Ma之后太平洋板块的运动方向发生转向,使得中国大陆包括华南板块在内均处于持续伸展阶段有关.硫化物矿石Rb-Sr所得的Sr同位素初始比(87Sr/86Sr)i平均值为0.7117,小于陆源硅酸盐的值(0.720),高于地幔Sr的初始值0.707,结合笔者对该矿床所做的S、Pb等同位素组成特征研究,显示成矿物质来源于壳幔混合.研究表明,利用特定矿床的主要矿石矿物,采用Rb-Sr等时线定年方法通过共生矿物组合和单矿物相互约束,可以有效地确定成矿时代,这对了解矿床的成矿背景等具有一定的指示意义.  相似文献   

9.
本文采集了我国19个产地的天然闪锌矿进行矿物学和光催化性能研究。样品皆为立方Zn S结构,化学成分变化较大,其中Fe对闪锌矿中Zn的替代范围为0.235%~14.826%(质量分数,下同),Cd对闪锌矿中Zn的替代范围为0.133%~1.576%。闪锌矿中Fe含量由低到高,导致颜色由浅变深直至呈黑色,半导体禁带宽度由大变小,估算获得天然闪锌矿的禁带宽度范围为3.18~2.28 e V,明显低于纯Zn S禁带宽度3.68 e V,光催化响应均在可见光范围。验证光催化实验结果表明含Fe较低、含Cd较高的天然闪锌矿可见光催化还原降解甲基橙的效果较佳,如可见光下1 g/L闪锌矿样品(含铁4.262%,含镉1.576%)对30 mg/L甲基橙催化反应4 h后的脱色降解率达到82.11%。天然闪锌矿中Fe含量影响着禁带宽度和光响应范围,Cd含量影响着光催化性能,为高附加值开发利用贱金属资源天然闪锌矿提供了科学依据。  相似文献   

10.
The relationship between mineralogical characteristics and isotopic composition of sulfides has not received its proper share of attention from geologists, although many references are available concerning the application of sulfur isotopes to geological problems. Located in the vicinity of the contact region between the Yangtze Platform and the South China Caledonian Folding Zone, the Huxu deposit is hosted in a structural zone in quartz-diorite-porphyrite emplaced in Jurassic volcanic rocks. Sphalerite and galena are the principal ore minerals in the deposit. (1) Sphalerite is highly variable in color and this variation can be related to its chemical composition and sulfur isotopic characters. Dark colored sphalerites are poor in Zn and Ni, rich in Pb, Cu, Fe, Ag and Au and have high δ34S values, while the opposite is true for light-colored ones. (2) δ34S of sphalerite is negatively correlated with the contents of Zn and Ni and positively correlated with the contents of Pb, Cu, Ag and Au, with the absolute values of the correlation coefficients being greater than 0.7. The above two characters suggest that the sulfur isotopic composition of sphalerite is controlled not only by the physicochemical conditions under which the mineral was formed, but also by mineralogical characteristics of the host mineral. (3) Apparent correlations exist among the constituent elements in the sphalerite. For example, Zn is negatively correlated with Cu, Pb, Fe, Ag and Au and positively correlated with Ni. (4) Sphalerites of the same color in the same hand specimen always show similar characters with respect to trace element and sulfur isotopes. (5) Two distinct trends of evolution can be recognized between Zn and Cu, Zn and Pb, Zn and Ag and between these elements on one hand and δ34S on the other, reflecting that the ore-forming solutions may have resulted from mixing of fluids of different origins. (6) Pb is uniformly distributed in sphalerite and shows positive correlations with Cu, Fe, Ag and δ34S, suggesting isomorphic substitution in the sphalerite lattice. This project was financially supported by the Open Laboratory of Ore Deposit Geochemistry, Institute of Geochemistry, Chinese Academy of Sciences.  相似文献   

11.
筲箕湾铅锌矿床位于黔西北铅锌成矿区中部,为该区铅锌矿床中的又一典型代表,其金属资源量（Pb＋Zn）超过20万t。本文利用电感耦合等离子体质谱（ICP-MS）分析了不同类型矿石中原生矿石硫化物（黄铁矿、闪锌矿和方铅矿）中分散元素含量,结果显示除Cd含量较高外,Ga、In、Se、Tl和Re的富集程度均较低。不同分散元素在硫化物中表现出不同的富集规律,表现为Ga含量在闪锌矿中最高,黄铁矿次之,方铅矿最低;方铅矿中Tl含量高于闪锌矿,黄铁矿最低;Cd在闪锌矿中含量最高,方铅矿次之,黄铁矿最低;从黄铁矿→方铅矿→闪锌矿In含量依次升高;Re含量表现出在闪锌矿中最高,黄铁矿次之,方铅矿最低;Se富集程度从黄铁矿→方铅矿→闪锌矿依次升高。Ga、In和Re在不同颜色闪锌矿中富集程度相似,而Se、Cd和Tl则相对富集在棕色闪锌矿中。统计发现闪锌矿中Zn含量与Cd、Ga含量不呈类质同象的负相关特征,而其中的Fe含量与Cd、Ga含量间表现出曲线相关或负相关特征,暗示Cd、Ga可能是通过替代先进入闪锌矿中的Fe而占据其晶格,这可能是一种新的机制。闪锌矿Ga、Cd、In含量及Ga/In、Zn/Cd比值等参数,指示筲箕湾铅锌矿床形成于中-高温条件,其矿床成因类型与沉积-改造型相似。  相似文献   

12.
闪锌矿Cd、Fe含量与矿化阶段的关系   总被引：1，自引：0，他引：1  
闪锌矿是在许多矿床中最常见的矿物.闪锌矿的Cd、Fe含量与矿化阶段关系的研究,可以推断矿液演化史和矿床形成环境变化史.对矿床评价及勘查有一定的指示意义.分析国内外200多个矿床闪锌矿Cd、Fe含量数据,有8个矿床注明了闪锌矿形成的矿化阶段.其中4个矿床早阶段产生的闪锌矿比晚阶段形成的闪锌矿富Fe、贫Cd,4个矿床早阶段结晶的闪锌矿比晚阶段形成的闪锌矿既富Fe,又富Cd.反映矿床形成的地质构造和物理化学环境,矿液来源及演化史绝然不同.  相似文献   

13.
凹子岗锌矿床位于上扬子地块东缘,该矿床经历了两个成矿期:沉积成岩期和热液期,形成两种不同岩相学特征的闪锌矿。流体包裹体岩相学研究显示,存在盐水包裹体(W型)、烃类包裹体(G型)和含石盐子矿物多相包裹体(S型)。有机流体活动与成矿存在耦合关系,其中烃类包裹体(G型)赋存于白云石和自形粗粒闪锌矿中,具有黄色荧光效应,激光拉曼测试显示其成分为沥青质、CH_4、C_3H_8和H_2O;此外,沥青与闪锌矿密切共生。显微测温结果显示热液期流体包裹体均一温度集中于160~180℃,盐度集中于8%~14%NaCl_(eqv),部分可达30%NaCl_(eqv)左右。成矿流体除含有机质外,还含有NaCl、KCl、CaCl_2、MgCl_2、H_2O,为多元共存的流体体系,成矿压力为22~84 MPa。  相似文献   

14.
作为华南大面积低温成矿域的重要组成部分,川滇黔铅锌矿集区是我国重要的铅锌银等资源基地之一,同时该矿集区也是Ge、Cd、Ga和In等稀散元素的超常富集区域。毛坪矿床是该矿集区内第二大铅锌矿床,累计探明铅锌金属储量超过3Mt(Pb+Zn平均品位≥18%),锗(Ge)保有储量182t。本文以新发现的Ⅵ矿带(铅锌金属已探明储量≥60万t,Pb+Zn平均品位≥20%)为研究对象,利用LA-ICPMS对主要矿石矿物闪锌矿和黄铁矿进行了微区原位微量元素组成和Mapping分析。研究结果显示Ⅵ矿带闪锌矿普遍富集Ge(最高580×10^(-6),均值81.1×10^(-6))、Cd(最高3486×10^(-6),均值1613×10^(-6))和Ga(最高190×10^(-6),均值44.4×10^(-6));黄铁矿普遍富集Mn、As、Pb、Cu、Ag和Sb。与Ⅰ和Ⅱ号矿带闪锌矿相比,Ⅵ号矿带闪锌矿更富集Ge和Ga。闪锌矿中Fe和Pb以类质同象为主,偶见黄铁矿和方铅矿显微包体;Cu、Ge、Ag和As赋存形式主要为类质同象,替代方式为Ge^(4+)+2(Cu+,Ag+,As+)↔3Zn^(2+);Cd以类质同象方式赋存为主,替代机制为Cd^(2+)↔Zn^(2+);Ga和In可能主要以类质同象方式存在。黄铁矿中Pb和Mn主要以方铅矿和碳酸盐矿物显微包体为主;Cu、As和Sb以类质同象形式存在于黄铁矿中;Ag和Zn可能以独立矿物形式赋存;Co和Ni以类质同象方式替代Fe进入黄铁矿晶格中,替代方式为Ni^(2+)+Co^(2+)↔2Fe^(2+)。毛坪矿床新发现Ⅵ矿带硫化物相比典型MVT矿床硫化物具有不同的In和Ge含量以及Cd/Fe比值,结合矿床地质特征和其他证据,表明毛坪矿床成因类型特殊,有别于经典MVT铅锌矿床,属于川滇黔型铅锌矿床。  相似文献   

15.
The surface analytical techniques of X-ray Photoelectron Spectroscopy (XPS) and Time of Flight Secondary Ion Mass Spectroscopy (ToF-SIMS) have provided information on the type and concentration of species on the surface of sphalerite and pyrite particles in flotation concentrate and tail samples, but also on their distribution on each particle and across particles of different sizes. From this surface analytical study, a more accurate interpretation of the flotation results of sphalerite and pyrite minerals in a mixed mineral system could be made as a function of the concentrations of copper sulphate activator and xanthate collector, and particle size. In particular, it was found that sphalerite particles reporting to the concentrate are larger in size and contain less iron hydroxide on their surface than particles reporting to the tail. As for the pyrite particles, their lower recovery than the sphalerite particles is the result of a larger proportion of iron hydroxide on their surface inhibiting copper and collector adsorption.  相似文献   

16.
A consistent, relatively rapid decrease in FeS molecular content of sphalerites at decreasing depth is recognizable in upper parts of this structurally controlled Pb-Zn ore deposit, as an expression of tectonic calm and continuity of the productive stages of the mineralization. Elsewhere, in the depths, abrupt changes in quantity of isomorphous iron in sphalerites, within a relatively short depth-span, signify intensive movements during deposition of the ore. Wherever the structures are bent and healed by early quartz sufficiently to retard circulation of the solutions and to promote their cooling, variations in the FeS content of sphalerite at different depths may be related to thermal “knickpoints” of the ascending solutions. Nonetheless, FeS molecular content of sphalerites is no clue to the temperature of their crystallization. There is no relationship between the depth at which sphalerite was formed and the isomorphous Cd or Mn in crystal structures of the mineral. — V.P. Sokoloff.  相似文献   

17.
Gold deposits at El Sid are confined to hydrothermal quartz veins which contain pyrite, arsenopyrite, sphalerite and galena. These veins occur at the contact between granite and serpentinite and extend into the serpentinite through a thick zone of graphite schist. Gold occurs in the mineralized zone either as free gold in quartz gangue or dissolved in the sulfide minerals. Ore-microscopic study revealed that Au-bearing sulfides were deposited in two successive stages with early pyrite and arsenopyrite followed by sphalerite and galena. Gold was deposited during both stages, largely intergrown with sphalerite and filling microfractures in pyrite and arsenopyrite.Spectrochemical analyses of separated pyrite, arsenopyrite, sphalerite and galena showed that these sulfides have similar average Au contents. Pyrite is relatively depleted in Ag and Te. This suggests that native gold was deposited in the early stage of mineralization. Arsenopyrite and galena show relatively high concentrations of Te. They are also respectively rich in Au and Ag. Tellurides are, thus, expected to be deposited together with arsenopyrite and galena.  相似文献   

18.
The compositions of arsenopyrite and sphalerite from five Swedish metamorphosed Cu, Zn-sulfide deposits are related to T and P, according to the methods described by Kretschmar and Scott (1976) and Scott (1973). The As/S ratio of arsenopyrite indicates an equilibrium temperature around 400°C for all the deposits studied, whereas the sphalerite barometer shows pressures between 5 and 7 kb. The mineral assemblages of the bedrocks indicate a similar temperature but a lower pressure. A constant fs2 is probably only effective over distances of millimetres or a few centimetres in the samples studied. The fs2 has always been lower in the surrounding rocks than in the ores as indicated by a higher As/S in arsenopyrite, more FeS in sphalerites and the absence of pyrite.  相似文献   

19.
闪锌矿的吸收光谱和颜色的本质   总被引：1，自引：0，他引：1  
本文采用电子吸收光谱和分子轨道（MO）－能带理论模型，系统地研究了不同颜色的闪锌矿呈色的机理和本质。闪锌矿由于其形成条件不同，所含杂质元素各异而颜色变化。黑色闪锌矿含Fe高，其颜色是由于以配位体硫为特征的非键轨道2e到Fe^2 的晶体场型轨道的电子转移在500nm产生吸收所致。只有闪锌矿含Fe低（＜1％）时，它才可具有其他颜色，黄色与受主能级Cu^ 到导带或价带到施主能级Ga^3 的电子跃迁在410nm产生吸收有关；绿色是Co^2 的晶体场跃迁^4A2→^4T2(P)在700nm附近产生的吸收峰所致；红色可能与受主能级Hg^ 到施主能级Ga^3 的电子跃迁在470nm产生宽吸收带有关。当闪锌矿的吸收光谱有其中两个吸收带叠加时，它具有过渡的颜色，如黄绿色或绿黄色、桔黄色或桔红色，主要色调取决于两个吸收带的相对强度。  相似文献   

20.
闪锌矿中杂质Fe存在形式的重新认识   总被引：5，自引：1，他引：5  
闪锌矿作为一种重要的金属硫化物已得到广泛的研究，但在对闪上矿中杂质Ｆｅ存在形式的认识上却存在许多问题。本文对不同含Ｆｅ量的天然闪锌矿测定并分析了Ｆｅ的Ｋ边ＥＸＡＦＳ谱，同时对低温光吸收谱及穆斯堡尔进行了研究。结果表明，Ｆｅ在闪锌矿中主要以六配位形式存在。  相似文献   

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