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1.
论文给出了中国浙江火山岩区金矿床中黄铁矿的微量元素、形态和物理性质找矿标型特征.例如.(在许多)浙江火山岩区重要金-银矿床中黄铁矿相对富含铅、锌、钼、锡、砷、锑、铋而贫钴,镍、硒、碲:并且S/Se、Ag/Au、Pb/Ni、Se/Te、(As+sb+Bi)/(Se+Te)比值较高,Co/Nj、Ag/Pb、Ag/Zn、Cu/Zn和(Co+Ni)/(Pb+Zn)比值较低,再如含金黄铁矿比不含金黄铁矿的反射率低.总之,黄铁矿的标型性研究对于寻找金矿具有重大的理论意义和实际意义. 相似文献
2.
烧锅营子金矿床的黄铁矿形成于早、中、晚3期,是主要的矿石矿物和载金矿物,其中以中期黄铁矿为最主要的载金者.黄铁矿的化学成分为:TFe43.34%~45.52%,S46.58%~48.86%,与标准黄铁矿相比显示亏铁、亏硫特点.黄铁矿内含丰富的微量元素,有Au、Ag、As、Sb、Bi、Cu、Zn、Pb、Co、Ni、W、Mo、Se等.其中Au、Ag、Cu、Pb、Zn、Bi含量较高,而As、Sb低,Se极低.其Au/Ag(多大于0.5)、(Cu+Pb+Zn)/(Co+Ni+As)(4.26)、Co/Ni(>> 1)比值表明其属中温岩浆热液矿床. 相似文献
3.
为探讨黑龙江省东宁县金厂特大型金矿床角砾筒型和蚀变岩(石英脉)型两种矿化类型的关系,系统采集样品,利用LA-ICPMS方法对4个成矿阶段黄铁矿微量元素进行了原位点分析和面扫描。结果表明,金厂金矿黄铁矿富含As、Co、Ni、Cu、Pb、Zn、Au、Ag、Sb、Se、Te、Bi,含少量W、Mo、Sn。两种类型金矿化,从第一成矿阶段到第四成矿阶段,黄铁矿微量金属元素成分及其变化具有相对一致的脉动演化规律,总体表现为从高Co、Ni低As向高As低Co、Ni演化,Au、Ag、Cu、Pb、Zn集中在第二、第三成矿阶段。研究认为,金厂金矿区不同矿化类型、不同金矿体属同一斑岩系统、不同空间位置产物;黄铁矿中As、Au+Ag、Cu、Pb+Zn含量,微量元素总量以及成分环带发育情况是评价金(多金属)矿化强度、伴生成矿元素以及富矿部位的有效指标。LA-ICPMS方法对黄铁矿微量元素的面扫描能高效经济地识别不同阶段黄铁矿,并简单量化其微量元素变化特征。 相似文献
4.
浙江弄坑金银矿区黄铁矿成分标型研究 总被引：1，自引：0，他引：1
为确定弄坑矿区金银矿化成因类型及对该矿区深部矿化远景进行预测,应用找矿矿物学方法研究了浙江武义弄坑金银矿区黄铁矿成分及其特征比值（如S/Fe、Fe/（S＋As）、Co/Ni、S/Se、Se/Te、Au/Ag）、S、Pb同位素特征,分析了黄铁矿成分的成因标型及找矿标型,为该矿化区矿化成因类型的确定提供可靠性的矿物学依据.同时,利用黄铁矿微量元素的三角形图解对本矿区深部矿化远景进行了预测.结论显示,该区金银矿化属浅成低温火山热液成因类型,在矿化区的深部地段可望找到富的金银矿化体. 相似文献
5.
浙东南怀溪铜金矿床黄铁矿标型特征及其地质意义 总被引：3，自引：0，他引：3
黄铁矿标型特征在各类矿床研究中提供丰富的矿床成因信息及有效的深部找矿信息。怀溪矿床为浙东南政和-大埔大断裂和长乐-南澳大断裂间坳陷区内典型的热液脉状充填型Cu-Au多金属矿床,其黄铁矿具亏Fe和S的特点,ω(Fe)/ω(S+As)平均值为0.881,介于0.863与0.926之间,表明该矿床为中浅成中温热液矿床。黄铁矿ω(Co)/ω(Ni)比值主要介于1～5,显示怀溪Cu-Au矿床成矿流体主要为岩浆热液。黄铁矿硫同位素δ34S值为-2.14‰～+4.14‰(n=8),极差为6.28‰,平均值为+1.67‰,硫源部分来自深源岩浆。黄铁矿热电系数、微量元素综合比值Φ和As、Cu含量、As+Ag+Hg、Cu+Pb+Zn、Co+Ni微量元素组合自地表向深部均显示减小→增大→减小的变化规律。结合前人的研究成果,在深入研究黄铁矿标型特征的基础上认为该矿床深部具有一定的找矿前景。 相似文献
6.
文中给出了一个包含两大类五亚类八个型式的金矿床成矿模式图。浙江省火山岩区金矿的找矿标志有:矿床产出条件、围岩蚀变、同位素组成、包裹体、矿物共生组合、矿物组构及其标型特征。例如,该火山岩区重要金矿床的黄铁矿中,相对富含Pb、Zn、Mo、Sn、As,Sb和Bi,而贫Co、Ni、Se和Te;并且S/se、Ag/Au、Pb/Ni、Se/Te和(As+Sb+Bi)/(Se+Te)比值较高,Co/Ni、Ag/Pb、Ag/Zn、Cu/Zn和(Co+Ni)/(Pb+Zn)比值较低。Ⅰ、Ⅵ、Ⅶ式金银矿床中闪锌矿的化学成分富Fe、Mn,贫Cd、Hg;尤其贫Ge、Ga、Tl而富Au、Ag、Sn、Bi;晶体结构αo值约为5.4167～5.4191A。闪锌矿比重较低(d<4.05)、反射率(R)较高(高于纯闪锌矿0.24～1.61％),并且只有一个红外吸收峰(310～313cm~(-1))的特点。 相似文献
7.
重点研究了贵州遵义中南村和湖南张家界三岔镍-钼多金属矿床的黄铁矿,矿床成因为热水喷流沉积型。黄铁矿样品S/Fe比值的平均值为2.0093~2.048,成分特征均属于铁亏损型,说明其形成温度低。Co/Ni变化范围为0.077~4.5,均值为2.197,据Co/Ni的比值可以判断本区的黄铁矿主要为热液成因,矿化物质来源为热水喷流体系内的热液。成分图解标型显示,黑色岩系中高ω(Co+Ni)/ω(Fe)的黄铁矿和高ω(As+Se+Te)/ω(S)的黄铁矿均大量出现,可能与热水喷流沉积的温差变化范围较大有关,而并非正常沉积的产物。S/Se比值为950.8~1059.9,说明生成环境均一程度较高,而且海水温度比较高。由中南村镍-钼矿床的Se/Te值也能判明其为热液成因。关于黄铁矿的研究对本区镍-钼矿床的寻找有重要意义。 相似文献
8.
重点研究了贵州遵义中南村和湖南张家界三岔镍-钼多金属矿床的黄铁矿,矿床成因为热水喷流沉积型.黄铁矿样品S/Fe比值的平均值为2.0093-2.048,成分特征均属于铁亏损型,说明其形成温度低.Co/Ni变化范围为0.077~4.5,均值为2.197.据Co/Ni的比值可以判断本区的黄铁矿主要为热液成因,矿化物质来源为热水喷流体系内的热液.成分图解标型显示,黑色岩系中高ω(Co+Ni)/ω(Fe)的黄铁矿和高ω(As+Se+Te)/ω(S)的黄铁矿均大量出现,可能与热水喷流沉积的温差变化范围较大有关.而并非正常沉积的产物.S/Se比值为950.8-1059.9,说明生成环境均一程度较高,而且海水温度比较高.由中南村镍-钼矿床的Se/Te值也能判明其为热液成因.关于黄铁矿的研究对本区镍-钼矿床的寻找有重要意义. 相似文献
9.
本文依据相关元素的分配和地球化学理论,讨论了各种热液成因黄铁矿中的Co、Ni、As、Sb、Cu、Pb、Zn、Au、Ag、Mn、Te、Se含量和Fe/S、Co/Ni、Pb/Zn、Au/Ag比率及其在时间上和空间上的变化趋向,并得出黄铁矿的化学成分在探索矿床成因、划分成矿阶段、研究矿床分带和矿化评价等方面具一定意义的结论。 相似文献
10.
不同成因类型矿化中黄铁矿微量元素地球化学记录——以广东大宝山多金属矿床为例 总被引：3，自引：0，他引：3
位于南岭成矿带的大宝山多金属矿床发育W-Mo-Cu-Pb-Zn多金属矿化,主要由斑岩W-Mo矿化、矽卡岩Mo-W矿化和矿床成因存在争议的层状似层状硫化物矿化3种类型组成,在这3类矿化中广泛发育黄铁矿。本文通过电子探针面扫描分析和LA-ICP-MS点分析,调查了3种类型矿化中黄铁矿的微量元素含量特征和元素Co、Ni、As的赋存状态。电子探针面扫描分析表明,除了层状似层状硫化物矿化中的黄铁矿具弱的As不均匀分布外,其余两类矿化中黄铁矿的微量元素分布均匀,无明显环带构造;LA-ICP-MS分析表明3类矿化中黄铁矿的微量元素含量很低,但在误差范围内依然体现出明显差异,斑岩矿化中的微量元素Co、Ni、As和Se主要以类质同像替代存在,而Cu、Zn、Sn、Sb则分别以黄铜矿、闪锌矿、锡石和辉锑矿的微细粒矿物包裹体形式赋存;矽卡岩矿化中的黄铁矿富集Co、Ni、As、Se、Mo和微量的Cu和Zn;Ni和Ag则在层状似层状硫化物矿化中的黄铁矿中相对富集。研究结果表明大宝山多金属矿床中的黄铁矿微量元素特征一方面可以用于研究黄铁矿中微量元素的赋存状态,另一方面可以用于指示成矿过程中的物理化学条件和示踪区域成矿物质来源,厘定成矿过程。矿床成因存在争议的层状似层状矿化经历了泥盆纪海底火山喷发,在断陷盆地处形成的矿胚受到燕山期深源物质和多期次成矿流体的叠加改造。 相似文献
11.
七宝山金铜多金属矿区的钓鱼台硫铁矿床、金线头金铜矿床以及七宝山铅锌矿床,其矿化类型分别为似层状浸染型、隐爆角砾岩型、裂控热液脉型,黄铁矿是三类矿化中最发育的金属硫化物矿物。通过对3个矿床黄铁矿产状,晶体形态,主、微量元素的nS与nFe实际原子个数比图解(nS/nFe=1.985~2.066)、δFe与δS特征图解(δFe/δS=±5%)、δFe/δS-As图解、(Fe+S)-As图解、Co/Ni特征图解(Co/Ni=1.2~11;Co/Ni=2~27;0.7~18)、Co-Ni-As特征图解以及微量元素相关性[Se-Sb(0.528)、Se-Zn(0.371)、Zn-Sb(0.642)、Pb-Te(0.463)]等研究,得知3个矿床黄铁矿均受岩浆热液的影响,其成矿物质和岩浆作用密切相关,表明3类矿化黄铁矿均为与七宝山次火山杂岩体有关的中温热液型矿床。 相似文献
12.
《Ore Geology Reviews》2011,43(1):32-46
Hydrothermal pyrite contains significant amounts of minor and trace elements including As, Pb, Sb, Bi, Cu, Co, Ni, Zn, Au, Ag, Se and Te, which can be incorporated into nanoparticles (NPs). NP-bearing pyrite is most common in hydrothermal ore deposits that contain a wide range of trace elements, especially deposits that formed at low temperatures. In this study, we have characterized the chemical composition and structure of these NPs and their host pyrite with high-resolution transmission electron microscopy (HRTEM), selected area electron diffraction (SAED), high-angle annular dark-field scanning transmission electron microscopy (HAADF-STEM), analytical electron microscopy (AEM), and electron microprobe analysis (EMPA). Pyrite containing the NPs comes from two types of common low-temperature deposits, Carlin-type (Lone Tree, Screamer, Deep Star (Nevada, USA)), and epithermal (Pueblo Viejo (Dominican Republic) and Porgera (Papua New-Guinea)).EMPA analyses of the pyrite show maximum concentrations of As (11.2), Ni (3.04), Cu (2.99), Sb (2.24), Pb (0.99), Co (0.58), Se (0.2), Au (0.19), Hg (0.19), Ag (0.16), Zn (0.04), and Te (0.04) (in wt.%). Three types of pyrite have been investigated: “pure” or “barren” pyrite, Cu-rich pyrite and As-rich pyrite. Arsenic in pyrite from Carlin-type deposits and the Porgera epithermal deposit is negatively correlated with S, whereas some (colloform) pyrite from Pueblo Viejo shows a negative correlation between As + Cu and Fe. HRTEM observations and SAED patterns confirm that almost all NPs are crystalline and that their size varies from 5 to 100 nm (except for NPs of galena, which have diameters of up to 500 nm). NPs can be divided into three groups on the basis of their chemical composition: (i) native metals: Au, Ag, Ag–Au (electrum); (ii) sulfides and sulfosalts: PbS (galena), HgS (cinnabar), Pb–Sb–S, Ag–Pb–S, Pb–Ag–Sb–S, Pb–Sb–Bi–Ag–Te–S, Pb–Te–Sb–Au–Ag–Bi–S, Cu–Fe–S NPs, and Au–Ag–As–Ni–S; and (iii) Fe-bearing NPs: Fe–As–Ag–Ni–S, Fe–As–Sb–Pb–Ni–Au–S, all of which are in a matrix of distorted and polycrystalline pyrite. TEM-EDX spectra collected from the NPs and pyrite matrix document preferential partitioning of trace metals including Pb, Bi, Sb, Au, Ag, Ni, Te, and As into the NPs. The NPs formed due to exsolution from the pyrite matrix, most commonly for NPs less than 10 nm in size, and direct precipitation from the hydrothermal fluid and deposition into the growing pyrite, most commonly for those > 20 nm in size. NPs containing numerous heavy metals are likely to be found in pyrite and/or other sulfides in various hydrothermal, diagenetic and groundwater systems dominated by reducing conditions. 相似文献
13.
山西堡子湾金矿床黄铁矿标型特征 总被引：6，自引：1，他引：6
从成因矿物学及找矿矿物学观点出发，系统研究了堡子湾金矿床黄铁矿的产状，形态，化学成分，热电性质和热爆特征，该矿床黄铁矿富含Co,Ni,As,Ag,Au与W，Cu,Hg,Ag，As，Bi,Ni,Co,Pb相关性较好，构成特征元素组合，与通常认为的与火山－次火山热液有关的明矾石－高岭土型浅成中低温热液型金矿床特征元素及其组合基本一致。黄铁矿空穴型导电性与明矾，石－高岭土型浅成中低温热液型金矿床特征元素圾其组合基本一致。黄铁矿空穴型导电性与As,Au正相关，与Co，Ni呈明显的负相关，P型和N型导电性是由As/(Co Ni)值决定的。利用黄铁矿热电性及热爆特征空间分带与赋矿空间的对应关系进行成矿预测，效果明显。 相似文献
14.
本文依据21件黄铁矿样品的电子探针成分分析数据,讨论了Au,Ag,Fe,Co,Ni,S,As,Sb,Cu,Te,Sn,Se等13个元素在黄铁矿中的含量和S/Fe,As/Sb比值在时间和空间上的变化规律。对矿体上的黄铁矿单晶体进行的能谱扫描电镜成分分析,Fe,S,As等成分在黄铁矿内部呈环带状分布,由晶体中心向边缘,它们的含量呈脉动式变化,反映成矿热液活动频繁。 相似文献
15.
Song Xuexin 《Mineralium Deposita》1984,19(2):95-104
The Fankou Pb-Zn deposit occurs in the Middle-Upper Devonian and Lower Carboniferous carbonate and argillaceous carbonate formations. In principle, the deposit can be classified as a carbonate-hosted strate-bound deposit. Representative sphalerite, galena, and pyrite separates from Fankou have been analysed. For the purpose of comparison a literature survey on minor elements of other districts have been carried out. The comparison of determined data with the quoted data shows that the Fankou sphalerites are rich in Ga, Ge and Ag, but poor in Se and Te; the Fankou galenas are rich in Ag, Hg, Sb and As, but poor in Se, Te, Tl and Bi; the Fankou pyrites are rich in As, Cd and In, but poor in Se, Te, Co and Ni. Zn/Cd and Se/S×10–4 ratios for sphalerites, Sb/Ag, Sb/Bi and Se/S×10–4 ratios for galenas and Co/Ni ratios for pyrites from Fankou and other districts have been calculated. Ga-Ge-Ag atomic ratios in sphalerites, Sb-Bi-Ag atomic ratios in galenas and Co-Ni relations in pyrites have been plotted. The average value (311) of Zn/Cd ratios for sphalerites from Fankou is similar to values of sphalerites from Gaobanhe, Heqing, Accesa and Broken Hill. The average Sb/Ag ratio (0.74) and the Sb-Bi-Ag atomic ratios in Fankou galenas are similar to those in the syngenetic galena from the British Island. The Ga-Ge-Ag atomic ratios for Fankou sphalerites are similar to those for the syngenetic sphalerites and Gorno sphalerites. The average Co/Ni ratio (1.1) for micro to fine-grained pyrites from Fankou laminated-bedded pyrite ore is similar to that (0.8) for the sedimentary pyrites from other districts. As to the fine to medium-grained pyrites from Fankou massive pyritic ores, their higher Co/Ni ratios (1.6–1.8) may relate to the fact that more Ni is lost than Co, during the reformation or recrystallization. Sphalerite, galena and pyrite from Fankou all are rather poor in Se and have very low values of Se/S×10–4, so they may bear no genetic relation to volcanism. To sum up, the following conclusions can be reached: (1) The Fankou deposit possesses some syngenetic features. (2) Evidently it differs from skarn type, hydrothermal type, and volcanogenic type deposits. (3) Surely it is a reformed sedimentary Pb-Zn deposit. 相似文献
16.
粤北大宝山铜多金属矿床一直存在燕山期岩浆热液成因和海西期火山喷流成因之争,争议的焦点在于块状、似层状硫化物矿体的成因。本文在全面开展矿区地质调查和钻探查证的基础上,对块状、似层状和脉状硫化物矿石中的黄铁矿和磁黄铁矿开展EPMA和LA-ICP-MS原位分析。测试结果表明,不同产状黄铁矿的平均分子式相似,分别为FeS_(1.98)、FeS_(1.99)和FeS_(1.98),似层状和脉状硫化物中磁黄铁矿的平均化学式为Fe_(0.886)S和Fe_(0.874)S,属形成温度相对较低单斜磁黄铁矿。与花岗岩岩浆热液标型黄铁矿相比,不同产状的黄铁矿和磁黄铁矿中Co、Ni、Mn、Se和Ge等元素以类质同象形式赋存,它们含量较低但稳定,Cu、Pb、Zn、Ag、Bi和Tl及Ga主要以微细矿物子晶形式存在,其含量丰富,但变化明显。从块状、似层状到脉状硫化物矿体,黄铁矿和磁黄铁矿中Co、Zn和Se的含量及Co/Ni值降低,而Cu、Pb、Ag、Bi等元素的含量明显升高。结合矿区次英安斑岩的产状和含矿性特征表明,大宝山矿床块状、似层状和脉状硫化物矿体都是次英安斑岩深部岩浆房产出的含矿流体在不同赋矿环境中的产物。 相似文献
17.
Sedimentary pyrites in black shales contain abundant trace elements that provide information on the chemistry of the seawater at the time of sedimentation. This study focuses on the Barney Creek Formation (~ 1640 Ma) in the McArthur Basin in the Northern Territory of Australia, which is host to one of the world's largest SEDEX Zn-Pb-Ag deposits, and several smaller deposits. Fine-grained sedimentary pyrite has been sampled from three drill holes through the Barney Creek Formation at various distances from SEDEX mineralisation. Samples were selected through the stratigraphy of each hole and analysed by LA-ICPMS for a suite of 14 trace elements. The data show that sedimentary pyrite at the base of the Barney Creek Formation, closest (within 1 km) to SEDEX mineralisation, is strongly enriched in Zn and Tl by one to two orders of magnitude compared to the global average for sedimentary pyrite. In contrast sedimentary pyrite from the hole furthest from SEDEX mineralisation (~ 60 km) contains mean Zn and Tl values equal to, or less than, the global average. Based on the three drill hole pyrite data sets it is concluded that trace elements that are contributed to the basin during hydrothermal exhalation, and adsorbed into contemporaneous sedimentary pyrite, are principally Zn, Tl, Cu, Pb, Ag and As. In contrast, trace elements that are adsorbed into sedimentary pyrite from background seawater are principally Mo, Ni, Co, Se and As. These differences have enabled the development of a SEDEX fertility diagram for sedimentary basins, based on the composition of sedimentary pyrite, that distinguish high Zn, but barren shales, from high zinc SEDEX-related shales. In parallel with the increase in Zn and Tl in sedimentary pyrite approaching mineralisation there is a decrease in Ni, Co and Mo. This means that the ratios Zn/Ni and Tl/Co are particularly good pyrite vectors to SEDEX mineralisation in the McArthur Basin, varying over 4 to 6 orders of magnitude from barren shales to mineralised shales. It is speculated that the reason for the reverse relationship between Ni, Co and Zn, Tl may be caused by hydrothermal exhalations into the water column that effect the ion-exchange pyrite surface complexation processes that alter the uptake of these elements into sedimentary pyrite.Another important conclusion of this study is that hydrothermal exhalations into a sedimentary basin may affect the redox sensitive trace element chemistry of sedimentary pyrite and therefore the trace element chemistry of pyritic black shales. Nickel, Co and Mo all decrease in proximity to hydrothermal vents that form SEDEX deposits, whereas Zn, Tl and Pb increase. Selenium and bismuth are the only redox sensitive trace elements that appear to be unaffected by hydrothermal activity in the McArthur Basin. This has implications on how trace element concentrations of black shales and pyrite are used to reflect past global ocean chemistry. 相似文献
18.
浙江遂昌治岭头金矿床黄铁矿的化学成分标型研究 总被引：12，自引：2，他引：10
对遂昌治岭头金矿床 3个矿段 (东矿段、中矿段、西矿段 )的黄铁矿进行了化学成分标型特征的研究。指出黄铁矿中铁、硫主元素的含量 ,钴、镍含量及比值 ,硒、碲含量及比值均为本矿床的成因系沉积后经热液叠加提供了比较可靠的依据。黄铁矿中的 w( Cu) /w( Zn)、w ( Ag) /w ( Zn)、w ( Pb) /w ( Zn)值为本矿床提供了成矿信息 ,认为西矿段见矿部位矿体向下延伸要大于中矿段 ,指出了进一步找矿的前景。 相似文献
19.
Trace element distribution,Co:Ni ratios and genesis of the big cadia iron-copper deposit,new south wales,australia 总被引：9，自引：0，他引：9
Analyses of pyrite, chalcopyrite and magnetite from the volcanic-hosted Big Cadia stratabound iron-copper deposit in Central Western New South Wales show considerable variation in the minor elements Mn, Ba, Ag, Pb, Zn, Cd, Se, Co and Ni. The preferential concentration of Co and Cd in pyrite, Zn and Ag in chalcopyrite and Mn in magnetite can be attributed to variations in activities of the ions in the hydrothermal fluid at the time of crystallisation of the mineral phases, or in cases such as the concentration of Co in pyrite, dependent on compatible electronic spin states between Co2+ and Fe2+. Trace element concentrations, especially Co and Ni contents and Co:Ni ratios in pyrite (average Co:Ni ratio=17.1) support a volcanic exhalative origin of mineralisation at Big Cadia. Differences in trace element composition such as higher Ni contents in pyrite in contrast with other volcanic-hosted ores may reflect the more basic character of volcanic rocks underlying the Big Cadia deposit. 相似文献