布拜图对PACMANUS热液区Si-Fe-Mn-羟基氧化物沉淀条件的指示

Utilizing Si, Fe and Mn concentrations within the end-member PACMANUS hydrothermal fluid, Si-Fe-MnH_2 O Pourbaix diagrams were constructed at 300°C and 25°C. The Pourbaix diagrams show that the main Si, Fe and Mn oxides species precipitating from the hydrothermal fluid were Si O_2, Fe(OH)_3, Fe_3(OH)_8, Mn_3O_4, and Mn_2O_3 at 25°C. During mixing of hydrothermal fluid with seawater, Si O_2 precipitated earlier than FeMn-oxyhydroxides because of the lower stability boundary. Then Fe(OH)_2 precipitated first, followed by Fe_3(OH)_8 and Fe(OH)_3, and last, small amounts of Mn_3O_4 and Mn_2O_3 precipitated. Fe(OH)_3 was readily deposited in alkaline solution with little influence by Eh. There were many Si-Fe-Mn-concentric particles in the polished sections of the massive precipitates collected from PACMANUS. In the concentric nucleus and ellipsoid, Si oxides precipitated first before the hydrothermal fluid had mixed with seawater. In the concentric nucleus, after the precipitation of Si oxides, the increase of p H and Eh promoted the precipitation of Mn oxides around the Si oxides. In the large ellipsoid, the precipitation of Fe was divided into two periods. In the early period, increase of p H value of hydrothermal fluid produced by low-temperature convection and an input of a small volume of seawater promoted a small amount of Fe(OH)_3 to precipitate in the Si-rich core. In the late period, after complete mixing with seawater and the resultant fluid was close to neutral or slightly alkaline in p H, Fe(OH)_3 was easily precipitated from the solution and distributed around the Si-rich core.     

东太平洋海隆深海热液区沉积物古菌多样性分析

采用PCR-RFLP方法对东太平洋海隆深海热液区3个站位沉积物中的古菌多样性进行了初步研究.结果显示,从古菌16S rRNA基因文库中随机挑取的296个阳性克隆分属奇古菌门（Thaumarchaeota,47.64%）、广古菌门（Euryarchaeota,44.93%）、泉古菌门（Crenarchaeota,6.77%）和未分类古菌（0.68%）,其中优势菌群为奇古菌门的亚硝化侏儒菌属（Nitrosopumilus,35.47%）和广古菌门的热原体纲（Thermoplasmata,27.03%）,DHVE3、DHVE5、DHVE6、MBGB和MBGE类群在沉积物样品中也均有发现.另外,3个站位沉积物中古菌类群组成存在差异,S5-TVG1站位样品文库的97个古菌克隆分属奇古菌门（49.48%）、广古菌门（49.48%）和泉古菌门（1.03%）,S14-TVG10站位样品文库的103个古菌克隆由奇古菌门（84.47%）和广古菌门（15.53%）组成,S16-TVG12站位样品文库的96个古菌克隆包括广古菌门（71.88%）、泉古菌门（19.79%）、奇古菌门（6.25%）和未分类古菌（2.08%）.研究结果表明,东太平洋海隆深海热液区沉积物中古菌多样性丰富,存在着许多新的古菌菌群;不同站位古菌菌群结构以及多样性存在差异,这与其所处环境的热液活动密切相关.     

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

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.     

Calcium,Na, K and Mg Concentrations in Seawater by Inductively Coupled Plasma‐Atomic Emission Spectrometry: Applications to IAPSO Seawater Reference Material,Hydrothermal Fluids and Synthetic Seawater Solutions

We report a measurement procedure to determine simultaneously the major cation concentrations (Na, Ca, K and Mg) of seawater‐derived solutions by inductively coupled plasma‐atomic emission spectrometry. The best results were obtained when the IAPSO (‘standard’) seawater reference material was diluted by thirty times with Milli‐Q^® water. We obtained an average reference value r_K (the ratio of the mass fraction of potassium to that of chlorine, i.e., (g kg^?1)/(g kg^?1)) for IAPSO seawater of 0.0205 ± 0.0006 (2.9% RSD), not significantly different from 0.0206 ± 0.0005 (2.4% RSD) for seawater composition reported in the literature. The measured Na, Ca and Mg concentrations correspond to r_Na, r_Ca and r_Mg values of 0.5406 ± 0.0026 (0.5% RSD), 0.02192 ± 0.00048 (2.2% RSD) and 0.06830 ± 0.00047 (0.7% RSD), respectively, in line with previous values measured by wet‐chemistry and atomic absorption spectrophotometry or wet‐chemical titration. Our measurement procedure was used successfully on synthetic seawater solutions and high‐temperature hydrothermal fluids.     

大兴安岭西坡银都赋矿岩体LA-ICP-MS锆石U-Pb定年及其成因意义

银都矿床位于内蒙古大兴安岭西坡,为受断裂控制的银多金属矿床。该矿床的岩体主要为石英闪长岩。该岩体中的锆石分为岩浆锆石和热液锆石两类:岩浆锆石无色透明,自形长柱状,具有典型的振荡环带特征;而热液锆石呈浅褐色,半透明—不透明,等轴状,其暗色增生边明显切过了核部岩浆锆石结构。热液锆石相对岩浆锆石具有低Th/U和LREE,高Hf和HREE的特征。银都岩体岩浆锆石的206Pb/238 U加权平均年龄为(451.8±7.8)Ma,属加里东期,为岩体的结晶年龄;热液锆石的206 Pb/238 U加权平均年龄为(337.0±7.7)Ma,属中石炭世,代表了热液作用的年龄。热液锆石年龄表明,该区在337Ma左右经历了一次强烈的热液作用,该期热液作用可能与该区造山峰期的变质作用有关。本区的地质特征和流体包裹体特征表明,本区银矿的形成很可能与这期热液活动密切相关。     

赣南白面石铀矿田成因再认识

赣南白面石铀矿田经上世纪60~80年代勘查,发现和探明了白面石、龙坑、双坑、马荠塘4个铀矿床和黄泥湖铀矿点,成为中国重要的铀资源基地。该矿田产于EW向南岭铀成矿带东段的白面石沉积-火山盆地内。该盆地的基底为印支期白面石花岗岩体;盖层为中侏罗统菖蒲组。盖层的底部为第一层砂岩,其上由基性-酸性双峰式火山岩组合与5层碎屑岩夹层组成。铀矿主要赋存在盖层底部的第一层砂岩中,其次是产在第一层玄武岩与第一层砂岩的接触带,有少量产在基底花岗岩顶部的风化壳中。关于该铀矿田的成因,有砂岩型沉积说、同生沉积后生富集说、成岩成矿热液叠加说、岩浆热液说,等等。为了厘定矿床成因类型,以确立今后的找矿方向,笔者对该矿田的资料进行了重新整理,应用Minesight软件选择典型的白面石铀矿床建立了三维地质模型,并收集了最新的同位素定年和岩石地球化学分析资料。研究表明,白面石铀矿田存在2次成矿（160~156 Ma和99~86 Ma）,其主成矿作用与第一层玄武岩的覆盖,在空间上相伴（铀矿体主要赋存于第一层砂岩及其与玄武岩的接触带）、时间上相近（成矿时间为160~156 Ma,玄武岩成岩时间为173 Ma）、成生上相关（矿化具有明显的中-低温热液蚀变）,为火山热盖成因类型,后期又有大量脉体活动,在岩脉两侧的砂岩层内又有热液型铀矿化叠加,从而形成了火山热盖及热液叠加的复成因矿床。该矿田的成矿条件是：富铀的基底,砂岩的沉积,洼沟的地形,岩浆的热盖,脉岩的入侵。     

再论甘肃镜铁山铁矿成因

甘肃“镜铁山”铁矿位于北祁连山加里东褶皱带西段,因铁矿规模大、类型特殊,并同时赋存一个中型铜矿而倍受关注。有关矿床成因各家意见不一,有“火山热液沉积”说,“变质沉积”说,“海底喷气沉积”说,“Sedex型”等,但均认为铁矿属沉积矿产。笔者近期在野外工作期间,在与成矿关系密切的黑色千枚岩中发现了钙质千枚岩捕掳体,证明黑色千枚岩为火成岩,所采矿石、围岩样品的地球化学性质也显示出火成岩特征,因局部地段黑色千枚岩与铁矿成过渡关系,并结合前人所测成矿温度在280℃至340℃之间等证据,综合分析认为镜铁山铁矿可能不是沉积成因,而是与中、基性岩有关的热液变质铁矿。     

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

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。     

热液矿床中萤石的稀土元素地球化学及其地质意义

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。     

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

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.