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栾川西沟铅-锌-银矿是与中元古界官道口群碳酸盐岩、上元古界栾川群碎屑岩-碳酸盐岩沉积建造有关层状铅-锌-银矿.通过对成矿地质背景、矿床地质特征及成矿物质来源的研究,其结果认为,该层状铅-锌-银矿床在地层同沉积时形成了矿源层和部分硫化物,之后经历了二个成矿期:(1)中-低温热液期,它使得矿源层进一步发展成矿,并对其进行了叠加改造;(2)风化期,该期对已形成的矿体作了轻微的改造,形成小部分氧化矿体.从成矿条件、成矿物质来源及同位素特征来看,该矿床属于热水沉积-叠加改造型层控矿床. 相似文献
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豫西南铅锌多金属矿控矿条件及找矿方向 总被引:11,自引:1,他引:11
豫西南地区是中国中部重要的多金属成矿远景区。对区内成矿地质条件和典型矿床特征进行了总结,认为①与官道口群碳酸盐岩和栾川群碎屑岩一碳酸盐岩沉积建造有关的层状铅锌银矿床、②与燕山期花岗(斑)岩有关的铅锌银(铜)矿床、③与古生界海相火山一碎屑岩建造有关的锌铜(铅、银、金)矿床是今后调查的3种主要矿床类型,并圈定出12处找矿远景较好的矿集区(矿化集中区)为重点工作地区,为下一步找矿勘查工作部署提供了依据。 相似文献
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卢氏-栾川地区位于河南省西南部,属华北地层大区,跨越晋冀鲁豫地层区和秦祁昆地层区,分别属华熊地层小区和秦祁昆地层区南部、北部,主要分布地层为太古宙太华岩群,中元古界熊耳群、高山河组、官道口群,新元古界栾川群。矿产以铅、锌、钼、钨、银为主,著名的南泥湖矿田即位于本区,是我国重要的钨钼铅锌银多金属成矿区。 相似文献
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河南栾川杨树凹-百炉沟MVT铅锌矿带地质特征 总被引:7,自引:4,他引:7
河南栾川地区马圈-百炉沟铅锌矿带位于华北陆块南缘中-新元古代被动大陆边缘中的浅海台地相碳酸盐岩环境,矿化以铅锌(银)为主,矿床赋存于官道口群中的三个古含水层系统(基本上是由下部含(透)水的碎屑岩(砂岩)与上覆相对不透水的碳酸盐岩组成)中,矿体形态比较简单,富矿段多赋存于多组构造交汇部位,硅化、角砾岩化、白云岩化、滑石化是矿区最主要的围岩蚀变。矿床地质特征可与北美Missouri地区的MVT矿床对比,成因属密西西比河谷型(MVT)。研究表明,位于龙家园组、冯家湾组中的含水层是最重要的找矿层位,角砾岩化、白云岩化、滑石化等是主要的找矿标志,沿马圈~竹园沟一百炉沟推覆断层北侧(官道口群)地区是寻找MVT型铅锌银矿床最主要的远景区。 相似文献
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河南栾川地区是我国著名斑岩钼矿集区,近年铅锌矿勘查取得重要进展,但对铅锌矿成因认识分歧颇多。研究表明,栾川地区铅锌矿产在燕山期斑岩钼矿床外围,矿区地层为中元古界官道口群和新元古界栾川群碳酸盐岩-碎屑岩沉积变质建造,地层中侵入有晋宁期辉长岩、正长岩和燕山期酸性斑岩,铅锌矿呈脉状或透镜状,发育3种类型:受燕山期斑岩与元古界钙质地层接触带控制的夕卡岩型铅锌矿、受北西西向层间断裂构造控制的脉状铅锌矿和受北东或近南北向张-张扭性断裂控制的脉状铅锌矿。铅锌矿石中硫化物δ~(34)S_(V-CDT)为近零的正值(骆驼山0.37‰~4.20‰、赤土店-0.32‰~8.30‰、百炉沟-1.20‰~10.90‰、冷水北沟0.70‰~12.10‰),岩浆来源硫特征明显;夕卡岩型铅锌硫化物的δ~(34)S_(V-CDT)与本地斑岩型钼矿石中硫化物的δ~(34)S_(V-CDT)(1.24‰~3.30‰)极为相近,脉状铅锌硫化物的δ~(34)S_(V-CDT)与斑岩型钼矿石中硫化物重合,但有地层中硫(δ~(34)S_(V-CDT)为12.43‰~18.63‰)的影响。总体上δ~(34)S_(黄铁矿)>δ~(34)S_(闪锌矿)>δ~(34)S_(方铅矿),指示矿石中主要硫化物矿物硫同位素分馏基本达到平衡,赤土店铅锌矿石中共生方铅矿与闪锌矿的硫同位素温度计指示硫化物矿物沉淀温度较高(388.29℃)。河南栾川地区铅锌矿主体应为受燕山期构造-岩浆作用控制的中高温热液铅锌矿床。 相似文献
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赤土店铅锌矿床位于华北陆块南缘豫西南泥湖超大型钼钨多金属矿集区东南部,矿体呈脉状、似层状产于新元古界栾川群煤窑沟组碎屑岩-碳酸盐岩夹石煤层沉积建造中。闪锌矿ICP-MS微量元素分析结果表明,赤土店矿床闪锌矿,以富含In、Ga、Sn、Cd和As等微量元素,而亏损Cu、Ni、Tl和Co等元素为特征,形成于中低温环境。总体上该矿床闪锌矿微量元素含量组成特征与层控-岩浆热液叠加改造型铅锌矿床类似,暗示其具有相似的成因联系。闪锌矿稀土元素特征显示出两种配分模式,从早期弱正Eu异常到晚期明显的负Eu异常,而且稀土元素总量有所增加,轻重稀土分馏增强。这种变化反映了成矿流体可能由一个相对还原环境向相对氧化环境的转变,为岩浆热液叠加改造的结果。 相似文献
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豫西白术沟组的构造位态及时代问题 总被引:1,自引:0,他引:1
白术沟组以其独特的岩石物理特性而卷入到推覆构造带的特殊部位,本文研究了白术沟组的三种构造位态,确定其主要呈第一种构造位态广泛分布于推覆体内部某次一级逆冲滑脱断层的下部,其上覆逆冲岩席由震旦系栾川群及中元古界官道口群构成,下伏地层为下古生界陶湾群。前人将白术沟组置于栾川群的底部层位,笔者对此提出异议,认为以含磷,铀为特征的白术沟组碳质毛枚岩层实与我省北部华北地台区早寒武世辛集组底部含磷铀的碳泥质层为 相似文献
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马圈一带出露的主要地层为上元古界栾川群和中元古界官道口群 ,是Pb、Zn、Ag的主要含矿地层。燕山期花岗岩在空间上与矿化关系密切。矿体主要受北西向断裂控制 ,常分布在北西、北东向断裂构造交汇部位。根据地球化学特征、矿产分布规律和找矿标志 ,划分出百炉沟西凹—东凹—磨沟、百炉沟—黄花北沟—杨树凹等两个一级和银窝沟—大石渣沟—小石渣沟、板岔沟等两个二级找矿预测区。 相似文献
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河南省栾川县西沟铅锌银矿床单矿物铷-锶同位素组成特征 总被引:9,自引:7,他引:2
河南栾川西沟铅锌银矿床位于华北克拉通南缘栾川断裂北侧,为赋存于中-晚元古代浅变质碳酸盐建造中的层控矿床,被认为是晚元古代的热水沉积型矿床.从成矿早阶段至晚阶段,矿物共生组合依次为;细粒黄铁矿、粗粒黄铁矿-闪锌矿-白云石-石英组合、多金属硫化物-白云石-石英组合、黄铁矿-石英-碳酸盐组合.本文对其矿石硫化物和黑云母进行了单颗粒矿物Rb-Sr同位素分析和研究.1件赋矿钙质二云片岩样品的5个黑云母颗粒样品给出Rb-Sr等时线年龄为366.0±10Ma,代表赋矿围岩的区域变质年龄.由于黄铁矿-碳酸盐细脉切穿了钙质二云片岩的片理,闪锌矿细脉切穿大理岩条带,矿体未遭受区域变质作用,可推断矿化发生于366Ma之后.考虑到区域内的构造变形事件和大规模花岗岩类侵入和成矿作用的年龄数据集中在156~134Ma,峰值在138 Ma左右,认为西沟铅锌银矿床形成于晚侏罗世-早白垩世.5件成矿早阶段细粒黄铁矿具有较低的I_(Sr-138Ma0值(按138Ma计算的锶同位素初始比值),变化范围为0.7100~0.7151,平均0.7127,该值略高于晚侏罗-早白垩斑岩类和花岗岩基,明显低于太古代太华群变质基底、中元古代熊耳群安山质火山盖层和中-晚元古代栾川群和官道口群的片岩地层,但与赋矿围岩栾川群大理岩地层接近,表明碳酸盐地层变质脱水和晚侏罗-早白垩岩浆岩均有可能为早阶段成矿提供成矿流体.相比之下,主成矿阶段硫化物则更加富含放射成因锶;14个主成矿阶段粗粒黄铁矿测点的I_(Sr-138Ma)值范围为0.7152~0.7344,平均0.7247,13个闪锌矿测点的I_(Sr-138Ma)值范围为0.7108~0.7398,平均0.7283,这些硫化物I_(Sr-138Ma)值接近于或低于太古宙太华群、中元古代熊耳群和中-晚元古代官道口群和栾川群,表明这些地层的锶都有可能混入成矿流体.因此,上述研究表明成矿早阶段流体主要为壳源岩石的变质脱水流体或燕山期岩浆热液,而在主成矿阶段,通过水岩相互作用与浅源循环的大气水或建造水的混入,浅部盖层栾川群地层的成分较多地加入了成矿系统. 相似文献
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通过对粤东地区地层和岩石中成矿元素含量和区域地质背景的分析,认为粤东地区铜铅-锌-银成矿作用与燕山期的构造-岩浆作用关系密切,成矿物质中银-铜-锌以下地壳来源为主,铅则以上地壳及沉积地层来源为主。 相似文献
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The Paleoproterozoic McArthur Basin (McArthur Group) of northern Australia hosts world-class sedimentary ‘exhalative’ (SEDEX) McArthur type Zn–Pb deposits, which are largely hosted within a sequence of 1.64 Ga pyritic carbonaceous shales deposited in an extensional rift setting. A well-known example of these is McArthur River (or Here's Your Chance [HYC] Zn–Pb–Ag deposit). The ~ 1.78 Ga McDermott and ~ 1.73 Ga Wollogorang formations (Tawallah Group) both contain carbonaceous shales deposited in similar environments. Our observations suggest the carbonaceous facies of the Wollogorang Formation were deposited under mostly euxinic conditions, with periodically-high concentrations of sedimentary pyrite deposition. The carbonaceous shales in the older McDermott Formation contain considerably less early pyrite, reflecting a mostly sulfide-poor, anoxic depositional environment. Localized fault-bound sub-basins likely facilitated lateral facies variations, which is evident from synsedimentary breccias.The presence of evaporitic oxidized facies within the McDermott and Wollogorang formations, alongside evidence for synsedimentary brecciation in reduced shales are favourable criteria for SEDEX-style base metal deposition. Both formations overlie volcanic units, which could have been sources of base metals. Detailed X-ray petrography, new geochemical data and sulfur isotope data from historical drill cores indicate multiple horizons of stratiform and sediment breccia-hosted base metal sulfide within carbonaceous shale units, with high-grade Zn concentrations. A close association between sphalerite and ferromanganean dolomite alteration draws comparisons with younger SEDEX mineralization at HYC. Additionally, SEDEX alteration indices, used demonstrably as a vector to the younger orebodies, indicate the sedimentary rocks analyzed in this study are marginally below the ore window when compared to the overlying mineralized stratigraphy.Our data imply that localized active circulation of metalliferous brines occurred in the Tawallah Group basin. High-grade sulfide deposition in reduced facies alteration may represent distal expressions of larger SEDEX-style deposits. Furthermore, abundant pyrite and high molybdenum in the Wollogorang Formation suggest the global oceanic sulfate concentration was sufficient by ~ 1.73 Ga to engender intermittent but strong bottom-water euxinia during shale deposition, thus providing a robust chemical trap for base metal sulfide mineralization. 相似文献
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白云鄂博群黑色岩系微量元素地球化学特征及地质意义 总被引:3,自引:1,他引:3
白云鄂博群位于华北地台北缘,是一套中—新元古代裂谷沉积的产物。尖山组和比鲁特组是其中主要的黑色岩系。对以上两组中的碳质页岩和板岩的Au、Ag、As、Ba、Co、Cu、Hg、Mn、Mo、Ni、P、Pb、V、Zn、U、B、Sb等微量元素和稀土元素进行了较为详细的研究。通过元素含量特征、w(V)/w(V+Ni)、w(Zn)-w(Co)-w(Ni)三元图、稀土配分曲线、w(Ce)/w(La)、Ce和Eu异常、w(La)/w(Yb)-w(Ce)/w(La)和w(La)/w(Yb)-w(ΣREE)图解等方法对其沉积环境特征进行了探讨。微量元素含量分析显示白云鄂博群黑色岩系以富亲铜元素和亲石元素、贫亲铁元素为特征,其中富集Hg、B、As、Mn、Sb、Au、Ag、Pb、P、Ba、U、Mo等多种元素;较高的w(B)反映了黑色岩系沉积于盐度较高的水体中;高的w(V)/w(V+Ni)、w(Ce)/w(La)反映了黑色岩系形成于缺氧的沉积环境中;黑色岩系中Hg、Sb、Ba的富集和w(Zn)-w(Co)-w(Ni)图解中投点大部分靠近热水沉积区域指示了黑色岩系中有热水沉积物的参与;稀土元素配分模式、Ce和Eu异常及w(La)/w(Yb)-w(ΣREE)和w(La)/w(Yb)-w(Ce)/w(La)图解投点在两岩组中的不同特点表明尖山组沉积物以陆源沉积为主,有少量热水沉积物参与;而比鲁特组中热水沉积组分所占比例较大,形成时海水较深。 相似文献
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Many metallic ore deposits of the Late Cretaceous to Early Tertiary periods are distributed in the Gyeongsang Basin. Previous and newly analyzed sulfur isotope data of 309 sulfide samples from 56 ore deposits were reviewed to discuss the genetic characteristics in relation to granitoid rocks. The metallogenic provinces of the Gyeongsang Basin are divided into the Au–Ag(–Cu–Pb–Zn) province in the western basin where the sedimentary rocks of the Shindong and Hayang groups are distributed, Pb–Zn(–Au–Ag–Cu), Cu–Pb–Zn(–Au–Ag), and Fe–W(–Mo) province in the central basin where the volcanic rocks of the Yucheon Group are dominant, and Cu(–Mo–W–Fe) province in the southeastern basin where both sedimentary rocks of the Hayang Group and Tertiary volcanic rocks are present. Average sulfur isotope compositions of the ore deposits show high tendencies ranging from 2.2 to 11.7‰ (average 5.4‰) in the Pb–Zn(–Au–Ag–Cu) province, ?0.7 to 11.5‰ (average 4.6‰) in the Cu–Pb–Zn(–Au–Ag) province, and 3.7 to 11.4‰ (average 7.5‰) in the Fe–W(–Mo) province in relation to magnetite‐series granitoids, whereas they are low in the Au–Ag(–Cu–Pb–Zn) province in relation to ilmenite‐series granitoids, ranging from ?2.9 to 5.7‰ (average 1.7‰). In the Cu(–Mo–W–Fe) province δ34S values are intermediate ranging from 0.3 to 7.7‰ (average 3.6‰) and locally high δ34S values are likely attributable to sulfur derived from the Tertiary volcanic rocks during hydrothermal alteration through faults commonly developed in this region. Magma originated by the partial melting of the 34S‐enriched oceanic plate intruded into the volcanic rocks and formed magnetite‐series granitoids in the central basin, which contributed to high δ34S values of the metallic deposits. Conversely, ilmenite‐series granitoids were formed by assimilation of sedimentary rocks rich in organic sulfur that influenced the low δ34S values of the deposits in the western and southeastern provinces. 相似文献