胶东英格庄金矿床地质地球化学特征

英格庄金矿床是胶东牟平-乳山金矿成矿带重要的石英脉型金矿床之一,其产出和分布严格受NNE向断裂控制,围岩以古老变质岩和昆嵛山花岗岩为主,金矿物主要以晶隙金形式赋存于黄铁矿-脉石晶体之间。通过成矿流体包裹体地球化学研究可知:均一温度变化有3个峰值(155℃～165℃、205℃～215℃和245℃～265℃);该矿床包裹体盐度w(NaCl)较低(17.17(),在1.05(～17.17(之间变化,应属于低盐度流体;据其成矿压力21.3～58.8MPa,进一步求得的该矿床主要成矿深度为0.83～2.31km,为中浅成矿床;依据包裹体成分测试结果可知,矿床流体属K+-Na+-SO24-Cl-型。氢氧同位素显示其成矿流体主要来源于岩浆水和变质水,并有一定的大气降水混入。     

内蒙古中西部钼多金属矿床地质特征及其动力学背景

本文首次对内蒙古中西部白乃庙铜-钼-金矿床、大苏计钼矿床、西沙德盖钼矿床、柳坝沟金-钼矿床、哈达门沟金-钼矿床、查干花钼-钨矿床和流沙山钼-金矿床的产出环境、地质特征、成因类型和时空分布特点进行了简要总结,对成矿作用与构造-岩浆活动的关系进行了概略性论述。柳坝沟、哈达门沟和白乃庙矿床均在前寒武纪变质岩地层中产出,大苏计、查干花、西沙德盖和流沙山矿床直接产于海西-印支期中酸性侵入岩中,尽管上述矿床在产出环境和地理位置上存在有一定差别,但是它们均与花岗岩类侵入岩体(或岩脉)具有密切的空间分布关系,属与中酸性侵入岩有关的钼多金属矿床。另外,根据矿床(点)的空间分布特点,可划分出5个钼多金属矿化集中区:即大苏计-明星沟钼矿化集中区、白乃庙-谷那乌苏铜-钼-金矿化集中区、哈达门沟-沙德盖金-钼矿化集中区、马尼图-查干花钼-铋-钨矿化集中区和流沙山-黑鹰山钼-金-铁矿化集中区。研究结果表明,成矿作用与板块消减、碰撞和缝合过程中所诱发的构造-岩浆事件密切相关,是地壳特定演化阶段构造-岩浆活动的产物。     

关于南天山碰撞造山时代的讨论

南天山是天山山脉的一支,是中亚型造山带的典型代表,它经历了复杂的增生—碰撞过程。关于古南天山洋最终闭合—碰撞造山(碰撞事件)发生的时间一直存在不同的认识,争论由来已久。综合分析南天山造山带的构造、地层、古生物、岩石、地球化学和同位素年代学等方面的资料,特别是对放射虫、蛇绿岩、蓝片岩、火山弧及前陆盆地沉积等地质事实的研究,我们认为,南天山碰撞造山作用起始于二叠纪末—三叠纪初。     

兰州地区新近纪地层的沉积相与古环境记录

兰州地区位于黄土和青藏高原的过渡带,其第三纪地层对研究风尘沉积发育和青藏高原隆升都有着特殊的意义。本研究以0.25 m为间距对厚度210 m的兰州皋兰山剖面的新近纪地层采集样品901个,在实验室对试验样品进行前处理后对其进行了粒度、磁化率和色度测试。用粒度分布函数的方法分离了沉积物的各成因组分,确定了风成组分和水成组分在全剖面沉积物中所占的百分比。结合色度和磁化率的实验结果分析表明,皋兰山剖面地层以风尘沉积为主,其间夹有河流相沉积的约15层砂岩。古环境的恢复表明,兰州地区从至少约7 Ma开始,沉积地层经历了由河湖相向风尘沉积转变,气候干旱化开始,与黄土高原风尘序列堆积底界8～7 Ma基本一致。6～5.2 Ma构造稳定,是比较开阔的平原环境,并且气候条件比较湿热;5.2～3.5 Ma间构造波动比较频繁,形成了间隔性的河流相砂岩沉积,而在气候表现为干冷;自3.5 Ma开始,兰州地区发生相对构造沉陷,五泉砾岩层的发育是对青藏运动A幕的具体响应。     

矿床空间分布的分形研究及其找矿意义——以三江南段银铅锌矿床分布为例

矿床的空间分布规律对地质勘查和找矿工作具有指导作用,三江南段地区是我国重要的多金属成矿区带,因此在该地区使用现代数学理论来研究矿床的空间分布规律具有重要意义。本文在深入研究三江南段地区银铅锌成矿机理、成矿地质背景以及数盒子法(Box-counting method)的基础上采用近年来广泛使用的关联维数来研究该地区银铅锌矿床的空间分布规律。首先借助G IS技术量测了13个银铅锌矿床之间的距离,用不同的标度r及其对应的关联函数C(r)得到一点对序列(r,C(r)),然后通过在平面坐标下作出(lnr,lnC(r))的散点图,使用最小二乘法拟合直线来估算关联维数,整体拟合得到的关联维数D=0.875;分段拟合得到的关联维数D1=0.184、D2=1.00。研究结果表明三江南段地区的银铅锌矿床在空间上具有分形丛集分布的特征。依据本次研究,将该地区划分为三个银铅锌矿密集区,并就该地区找矿工作提出指导意见,同时也探讨了关联维数与盒子维数的差异。     

Définition et datation de la Formation de Venaco (Corse) : dépôt d’origine gravitaire d’âge Priabonien

Priabonian age is highlighted for the first time in Corsica in the Venaco Formation using the presence of specific microfauna (in particular some representatives of Turborotalia cerroazulensis lineage). This silicoclastic formation is mainly represented by coarse facies. It is composed of three members from south to north and from oldest towards youngest: member of Uboli, Cardo and Orsu. The sedimentologic analysis reveals a gravity depositional environment, involving different type of currents. Sedimentologic and chronologic characteristics make the Venaco Formation and the Annot Formation (p.p.) equivalent. Dating the Venaco Fm. brings confirmation that the green schist metamorphism of the Variscan batholith and the related deformation are from the pre-Priabonian period.     

内蒙古赤峰市鸭鸡山钼铜矿成矿流体特征及矿床成因

鸭鸡山钼铜矿床所处大地构造位置为蒙古—鄂霍次克造山带的温都尔庙—翁牛特旗褶皱带,该带是我国重要的有色金属成矿带之一。鸭鸡山钼铜矿床分布受控于区域EW向深断裂,矿体产于EW向主断裂F1上盘的二长花岗岩体中,严格受东西向F1断裂和北东向断裂控制。该矿床矿石自然类型为石英脉型和蚀变岩型,矿石中硫化物主要有黄铁矿、辉钼矿和黄铜矿。石英流体包裹体有气液两相、含子矿物三相和纯气相3种类型。流体盐度(w(NaCl))为2.06%～44.00%,集中在40%～44%和4%～8%;流体密度为0.85～1.25 g/cm3,集中在1.20～1.24 g/cm3和0.88～0.92 g/cm3;成矿温度为167～380℃,集中在320～360℃和200～220℃;流体盐度、密度、成矿温度在直方图上均表现为双峰特征。研究表明:成矿早阶段流体为高盐度、高密度和高温的岩浆流体,气相包裹体与含子晶三相包裹体共存,表明该阶段发生过强烈的沸腾或不混溶;成矿晚阶段为低盐度、低密度和中温的混合流体。通过等容线图解法估算成矿压力为274.7～368.5 MPa,用静岩压力梯度估算成矿深度为8.32～11.2 km。矿床成因类型为中成、中高温热液脉型...     

Re-Os geochronology of Cu and W-Mo deposits in the Balkhash metallogenic belt,Kazakhstan and its geological significance

<正>The Central Asian metallogenic domain(CAMD) is a multi-core metallogenic system controlled by boundary strike-slip fault systems.The Balkhash metallogenic belt in Kazakhstan,in which occur many large and super-large porphyritic Cu—Mo deposits and some quartz vein- and greisen-type W—Mo deposits,is a well-known porphyritic Cu—Mo metallogenic belt in the CAMD.In this paper 11 molybdenite samples from the western segment of the Balkhash metallogenic belt are selected for Re—Os compositional analyses and Re—Os isotopic dating.Molybdenites from the Borly porphyry Cu deposit and the three quartz vein-greisen W—Mo deposits—East Kounrad.Akshatau and Zhanet—all have relatively high Re contents(2712—2772μg/g for Borly and 2.267—31.50μg/g for the other three W—Mo deposits),and lower common Os contents(0.670—2.696 ng/g for Borly and 0.0051—0.056 ng/g for the other three).The molybdenites from the Borly porphyry Cu—Mo deposit and the East Kounrad,Zhanet,and Akshatau quartz vein- and greisen-type W—Mo deposits give average model Re—Os ages of 315.9 Ma,298.0 Ma,295.0 Ma,and 289.3 Ma respectively.Meanwhile,molybdenites from the East Kounrad,Zhanet,and Akshatau W—Mo deposits give a Re—Os isochron age of 297.9 Ma,with an MSWD value of 0.97.Re-Os dating of the molybdenites indicates that Cu—W—Mo metallogenesis in the western Balkhash metallogenic belt occurred during Late Carboniferous to Early Permian(315.9—289.3 Ma),while the porphyry Cu—Mo deposits formed at—316 Ma,and the quartz vein-greisen W—Mo deposits formed at ~298 Ma.The Re—Os model and isochron ages thus suggest that Late Carboniferous porphyry granitoid and pegmatite magmatism took place during the late Hercynian movement.Compared to the Junggar-East Tianshan porphyry Cu metallogenic belt in northwestern China,the formation of the Cu—Mo metallogenesis in the Balkhash metallogenic belt occurred between that of the Tuwu-Yandong in East Tianshan and the Baogutu porphyry Cu deposits in West Junggar. Collectively,the large-scale Late Carboniferous porphyry Cu—Mo metallogenesis in the Central Asian metallogenic domain is related to Hercynian tectono-magmatic activities.     

Shaking and splashing—A case study of far-field effects of the Mjølnir asteroid impact on depositional environments in the Barents Sea

The Mjølnir impact crater in the Norwegian Barents Sea features among the 20 largest impact craters listed in the Earth Impact Database. The impact is dated to 142 ± 2.6 Ma, corresponding closely to the Jurassic/Cretaceous boundary in the Boreal stratigraphy. Multidisciplinary studies carried out over the last three decades have suggested that the up to 40 km wide crater was created by a 1–3 km diameter impactor colliding with a shallow epicontinental sea, causing regional havoc and a regional ecological crisis that followed in its wake. Only minor evidence for the consequences of the impact for the surrounding depositional basins has been documented so far. This study describes a large submarine slump penetrated by hydrocarbon exploration well 7121/9-1, located in the southern Hammerfest Basin and approximately 350 km away from the impact site. The slump is dated by a black shale drape, which contains characteristic impact-related biotic assemblages and potential ejecta material. This precise dating enables us to associate the slump with large-scale fault movements and footwall collapse along the basin-bounding Troms-Finnmark Fault Complex, which we conclude were caused by shock waves from the Mjølnir impact and the passage of associated tsunami trains. The draping black shale is interpreted to represent significant reworking of material from the contemporary seabed by tsunamis and currents set up by the impact.     

山东福吉山铜矿构造控矿因素分析

福吉山铜矿成矿地质特点不同于山东已有的铜矿类型,属于构造热液成因类型。近SN向的平移断裂同时具有张扭性和压扭性双重力学性质,其中张扭性破碎带造就成矿空间,造成了矿体近等间距雁列式排列。受断裂构造的影响,矿区内节理、裂隙发育,为成矿热液的运移和积聚提供了良好的空间。区内沿裂隙充填形成的石英脉、褐铁矿脉、铜矿脉发育。