湖南锡田岩体的岩浆混合成因:岩相学､岩石地球化学和U-Pb 年龄证据   总被引：2，自引：0，他引：2       下载免费PDF全文

陈迪陈焰明  马爱军刘伟刘耀荣  倪艳军 《中国地质》2014,41(1):61-78

南岭中段的锡田岩体燕山期岩石以斑状黑云母二长花岗岩为主,岩体中广泛发育暗色微粒包体?暗色微粒包体为岩浆结构,大多数具有塑性外形,发育淬冷边?反向脉,存在多种不平衡结构和矿物组合,如钾长石环斑?石英眼斑?针状磷灰石等,显示岩浆混合特征?岩石地球化学方面,暗色微粒包体具有比寄主岩贫硅?贫碱,富K?Fe?Mg?Ca?Ti 特征;暗色微粒包体及寄主岩富集轻稀土元素(LREE/HREE=2.6~8.8),具有中-强的铕负异常(δEu=0.09~0.74)以及具有相似的稀土元素配分曲线和微量元素蛛网图;在主要氧化物含量Harker 图解中投点多呈直线变异趋势,反映了两者具有密切的亲缘关系,利用共分母和不共分母图解进行判别,暗色微粒包体与寄主岩具岩浆混合特征,在MgO-TFeO判别图解中也指示包体为岩浆混合成因?上述岩相学和元素地球化学特征表明暗色微粒包体是基性岩浆侵入到酸性岩浆中淬冷形成的,指示锡田岩体存在两种岩浆的混合作用?通过LA-ICP-MS锆石U-Pb 定年,得到寄主岩形成年龄(150.04±0.52)Ma,暗色包体形成年龄(145.09±0.63)Ma,二者年龄在测试误差范围内一致,显示岩浆混合作用发生的时间大致为晚侏罗世?  相似文献   

云南会泽HZT 型铅锌矿床蚀变白云岩特征及岩石-地球化学找矿标志   总被引：2，自引：1，他引：1       下载免费PDF全文

文德潇  韩润生吴鹏 贺皎皎 《中国地质》2014,41(1):235-245

蚀变白云岩是会泽超大型铅锌矿床的赋矿围岩。通过矿区调研和近矿围岩典型剖面精细测量,矿区蚀变中-粗晶白云岩从颜色上可分为4种类型:肉红中粗晶白云岩、米黄色针孔状粗晶白云岩、灰白孔洞状粗晶白云岩、纯白色粗晶白云岩;前三者与矿体产出关系密切,从远矿到近矿依次为:肉红中粗晶白云岩→米黄色针孔状粗晶白云岩→灰白孔洞状粗晶白云岩→铅锌矿石;总结了3个带主要矿物组合、组构特征,认为3个带在白云石重结晶程度、显微构造、黄铁矿、晶洞充填物及裂隙等具明显差异,据此可作为辨识赋矿白云岩的重要标志。同时,对比了摆佐组白云岩(矿化粗晶白云岩、粗晶白云岩、白云石化灰岩)主量元素变化特征,分析了近矿蚀变白云岩主量元素及其比值与矿体距离的相关性,以及CaO与其他主量元素相关性,确定了热液蚀变参数有SiO2、MgO/CaO、K2O/CaO、Al2O3/TFe等,为找矿预测提供理论依据。  相似文献   

若尔盖铀矿田热液矿物微量元素地球化学特征   总被引：1，自引：0，他引：1  

胡旭刚  陈友良  张成江  赵剑波 《四川地质学报》2014,(2):286-289

通过研究若尔盖铀矿田与铀成矿作用密切的热液矿物—方解石、石英、黄铁矿等的微量元素地球化学特征表明,方解石、石英、黄铁矿具有相似的微量元素组成,相对富含Sr、Zr、Ba、Zn、U、Ni、Cr等元素,说明形成方解石、石英和黄铁矿的流体来源相同。相关性分析表明,方解石、石英中成矿元素U与Zr、Ta、Co、Ni等深源元素显著正相关,反映若尔盖铀矿田的成矿流体应当来源于深部。  相似文献   

Selection of Less Biased Threshold Angles for SAM Classification Using the Real Value–Area Fractal Technique     

Hadi Shahriari  Hojjatollah Ranjbar  Mehdi Honarmand  Emmanuel John M. Carranza 《Resource Geology》2014,64(4):301-315

The accuracy of classification of the Spectral Angle Mapping (SAM) is warranted by choosing the appropriate threshold angles, which are normally defined by the user. Trial‐and‐error and statistical methods are commonly applied to determine threshold angles. In this paper, we discuss a real value–area (RV–A) technique based on the established concentration–area (C–A) fractal model to determine less biased threshold angles for SAM classification of multispectral images. Short wave infrared (SWIR) bands of the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) images were used over and around the Sar Cheshmeh porphyry Cu deposit and Seridune porphyry Cu prospect. Reference spectra from the known hydrothermal alteration zones in each study area were chosen for producing respective rule images. Segmentation of each rule image resulted in a RV–A curve. Hydrothermal alteration mapping based on threshold values of each RV–A curve showed that the first break in each curve is practical for selection of optimum threshold angles. The hydrothermal alteration maps of the study areas were evaluated by field and laboratory studies including X–ray diffraction analysis, spectral analysis, and thin section study of rock samples. The accuracy of the SAM classification was evaluated by using an error matrix. Overall accuracies of 80.62% and 75.45% were acquired in the Sar Cheshmeh and Seridune areas, respectively. We also used different threshold angles obtained by some statistical techniques to evaluate the efficiency of the proposed RV–A technique. Threshold angles provided by statistical techniques could not enhance the hydrothermal alteration zones around the known deposits, as good as threshold angles obtained by the RV–A technique. Since no arbitrary parameter is defined by the user in the application of the RV‐A technique, its application prevents introduction of human bias to the selection of optimum threshold angle for SAM classification.  相似文献   

热液矿床中萤石的稀土元素地球化学及其地质意义     

孙海瑞  黄智龙  周家喜  冷成彪  甘婷 《岩石矿物学杂志》2014,33(1):185-193

萤石是许多热液矿床中重要的脉石矿物,其稀土元素含量及相关参数（如∑REE、LREE/HREE、Eu/Eu^*、Ce/Ce^*、Y/La、Tb/Ca-Tb/La图解等）,能为揭示成矿流体性质、来源与演化,建立成矿模式,评价区域成矿潜力等提供重要信息。然而,随着微区分析技术的日趋成熟,原位实测数据显示,萤石中微量元素（包括稀土元素）的分配在显微尺度上可能具有不均一性,致使依据萤石溶液法获得的稀土元素含量所反映地质信息的可靠性受到质疑。因此,在应用萤石稀土元素地球化学探讨相关地质问题前,有必要加强萤石微观结构的观察和配套的流体包裹体以及相关同位素组成分析。本文在综述萤石稀土元素地球化学研究基础上,初步探讨了影响萤石稀土元素不均一分配的主要机制,以期为萤石稀土元素在热液矿床成因研究中的应用提供借鉴。  相似文献   

阿尔泰南缘可可托海地区二厂房岩体LA-ICP-MS锆石U-Pb年代学、岩石成因及其地质意义     

张亚峰  蔺新望  郭岐明  吕军利  赵端昌  王星  王旭 《岩石矿物学杂志》2014,33(1):13-28

对出露于阿尔泰造山带南缘可可托海地区二厂房岩体中的黑云母花岗闪长岩进行了LA-ICP-MS锆石U-Pb定年和岩石地球化学分析。结果显示,锆石的²⁰⁶Pb/²³⁸U年龄加权平均值为398.0±3.5 Ma（MSWD=1.3）,表明该岩体形成于早中泥盆世。岩体的SiO₂含量介于65.40%～69.31%之间,里特曼指数值为1.27～1.65,A/CNK值为0.92～1.02,属中钾、钙碱性、准铝质岩石。具有富集Cs、Rb、Th、U等大离子亲石元素和轻稀土元素,相对亏损重稀土元素和Nb、Ta、Zr、Hf等高场强元素,负Eu异常明显（δEu=0.48～0.65）的岛弧岩浆岩特征。结合区域地质资料,认为二厂房岩体形成于陆缘弧构造环境,是在古亚洲洋俯冲过程中,幔源的基性岩浆底侵下地壳后使之熔融并发生了岩浆混合作用的产物。  相似文献   

新疆霍什布拉克铅锌矿床微量元素地球化学     

李志丹  薛春纪  董新丰  王思程  张岩 《岩石矿物学杂志》2014,33(3):540-550

霍什布拉克铅锌矿床是新疆西南天山地区晚古生代碳酸盐岩容矿的重要矿床。本文采用高精度电感耦合等离子质谱(ICP-MS)对主要矿石矿物(黄铁矿、方铅矿、闪锌矿)和热液脉石矿物方解石进行了微量元素地球化学研究。研究表明,黄铁矿、方铅矿、闪锌矿、方解石具有较为相似的稀土元素特征,Eu正异常明显,弱负或弱正Ce异常指示成矿流体最初由相对氧化的条件演化为还原条件。与霍什布拉克岩体、容矿围岩的稀土元素组成进行对比后发现,硫化物及热液方解石稀土元素配分曲线部分与重结晶泥晶灰岩重合,结合前人同位素地球化学研究,认为容矿坦盖塔尔组碳酸盐岩为成矿提供了必要的成矿物质及成矿流体组分。Ga/In值显示闪锌矿为低温成矿;硫化物明显富集LREE,Hf/Sm、Nb/La和Th/La值小于1,显示铅锌成矿过程中成矿流体主体以富Cl为特征;Y/Ho、Zr/Hf和Nb/Ta值变化范围相对较小,表明成矿期流体性质相对较为稳定,基本未混入外来流体。  相似文献   

热液金矿床围岩蚀变特征及其与金矿化的关系   总被引：1，自引：0，他引：1  

黄诚  张德会  和成忠 《物探与化探》2014,(2):278-283,288

热液金矿床总是伴随着围岩蚀变,研究围岩蚀变对金矿勘查具有重要意义。总结不同类型热液金矿发现,与热液金矿密切相关的围岩蚀变主要有硅化、钾长石化、钠长石化、碳酸盐化、绿泥石化、绢英岩化等;重点分析讨论了硅化、钾长石化、钠长石化、碳酸盐化的特征、形成机理及其与金矿化之间密切关联的内在原因,同时也对热液金矿蚀变的分带性进行了讨论。  相似文献   

Geochemistry of mafic rocks and melt inclusions and their implications for the heat source of the 14.0°S hydrothermal field,South Mid-Atlantic Ridge     

Bing Li  Xuefa Shi  Yaomin Yang  Jun Ye  Jingjing Gao  Wenqin Zheng 《中国地球化学学报》2014,33(4):325-335

Fresh rocks sampled from the 14.0°S hydrothermal field of the South Atlantic Ridge can be divided into two categories： olivine-gabbro and basalt. The olivine-gabbro is composed mainly of three types of minerals： olivine, clinopyroxene and plagioclase, while a multitude of melt inclusions occur in the plagioclase phenocrysts of the basalts. We analyzed the whole-rock, major and trace elements contents of the basaks, the mineral chemistry of phenocrysts and melt inclusions in the basalts, and the mineral chemistry of olivine-clinopyroxene-plagioclase in the olivine-gabbro, then simulated magma evolution within the crust using the COMAGMAT program. The whole-rock geochemistry shows that all the basalts exhibit typical N-MORB characteristics. In addition, the mineral chemistry characteristics of the olivine-gabbro （low-Fo olivine, low-Mg# clinopyroxene, high-TiO2 clinopyroxene, low-An plagioclase）, show that strong magma differentiation occurred within the crust. Nevertheless, significant discrepancies between those minerals and phenocrysts in the basalts （high-Fo olivine, high-An plagioclase） reflect the heterogeneity of magma differentiation. High Mg# （-~0.72） melt inclusions isobaric partial crystallization simulations suggest that the magma differentiation occurred at the depth shallower than 13.03 km below the seafloor, and both the vertical differentiation column shows distinct discrepancies from that of a steady-state magma chamber. Instead, a series of independent magma intrusions probably occurred within the crust, and their corresponding crystallized bodies, as the primary high-temperature thermal anomalies within the off-axis crust, probably act as the heat source for the development of the 14.0°S hydrothermal system.  相似文献   

Preparation and Characterization of a New Layered Double Hydroxide, Mg–Fe–Ce     

LIU Zhiqi  LI Lijuan  CHEN Yunf  ZHANG Yanling 《《地质学报》英文版》2014,88(Z1):354-355

正1 Introduction In the present paper,MgCl2·6H2O,FeCl3·6H2O,and CeCl3·6H2O were used as raw materials in the precipitationhydrothermal method to synthesize MgF eC e hydrotalcite.The effects of the Fe:Ce molar ratio on the composition,crystal structure,and thermal stability of hydrotalcite are examined.Energy-dispersive X-ray spectroscopy(EDS),X-  相似文献