共查询到20条相似文献，搜索用时 312 毫秒
1.
甲玛铜多金属矿床是冈底斯成矿带东段具有重大经济价值及科学研究意义的超大型斑岩- 矽卡岩矿床,完整地保存了矽卡岩矿床形成和演化的重要信息。前人研究多集中于矽卡岩的水平分带,而对于矽卡岩矿物垂直分带以及其与金属矿化的耦合关系等方面研究薄弱。本文重点对甲玛3000 m科学深钻中矽卡岩矿体进行了精细的矿物学研究,系统揭示了矽卡岩矿体的矿物学空间分带特征以及与金属矿化的耦合关系。结果表明,矽卡岩从浅部至深部具有清晰的分带现象,即矽卡岩化角岩→透辉石石榴子石矽卡岩→硅灰石石榴子石矽卡岩→石榴子石硅灰石矽卡岩→透辉石石榴子石矽卡岩→石榴子石硅灰石矽卡岩→矽卡岩化大理岩→硅灰石石榴子石矽卡岩→透辉石石榴子石矽卡岩→硅灰石石榴子石矽卡岩→矽卡岩化大理岩→硅灰石石榴子石矽卡岩→透辉石石榴子石矽卡岩→内矽卡岩（含石榴子石花岗闪长斑岩）。金属矿物组合从浅部向深部,变化为辉钼矿±黄铜矿→斑铜矿+黄铜矿±辉铜矿±硫铋铜矿±辉钼矿→辉钼矿±黄铜矿,对应成矿元素变化为Mo±Cu±Au±Ag→Cu（Mo）±Au±Ag→Mo±Cu±Au±Ag。研究表明,侵入岩及围岩的空间位置、构造环境、多期次热液流体叠加是控制矽卡岩矿物分带的重要因素。同时,矿物学特征表明,矽卡岩中高品位金的富集与斑铜矿等铜硫化物密切相关,也可能与多期次流体叠加和富金岩浆源区有关。 相似文献
2.
西藏甲玛铜多金属矿床地质地球化学特征及成因浅析 总被引：6，自引：0，他引：6
甲玛铜多金属矿床是冈底斯成矿带内产出的超大型矿床,其铜、钼、铅+锌、伴生金、伴生银资源量均达到大型及以上规模,该矿床也是成矿系列理论指导实践取得找矿突破的典型矿床。矿区的矽卡岩型主矿体呈层状、厚板状产于下白垩统林布宗组砂板岩、角岩(矿体顶板)与上侏罗统多底沟组灰岩、大理岩(矿体底板)的层间因推覆-滑覆构造引起的扩容空间内,矿体走向延长超过3000m,倾向延伸超过2200m,最大真厚度达250m。除了矽卡岩型铜多金属矿体是主要矿体类型外,矿区角岩型钼铜矿体与斑岩型钼铜矿体已经初具规模。角岩型矿体主要呈筒状分布于0～40线矽卡岩型矿体上部的角岩中,平面面积约0.8km2,矿体垂向最大延伸超过800m;斑岩型矿体已初见端倪,基本位于矽卡岩型矿体下部,但也有部分穿切矽卡岩型矿体。矿床中矿石的主要构造特征为浸染-细脉状,结构特征以热液交代作用形成的结构为主。矿石中主要的矿石矿物包括黄铜矿、斑铜矿、辉钼矿、黝铜矿和辉铜矿等,脉石矿石以矽卡岩矿物和石英为主。通过不同类型矿石中辉钼矿的Re-Os同位素测年,甲玛铜多金属矿床的形成时代介于18～10Ma之间,与青藏高原后碰撞伸展阶段成矿作用有关。稀土元素地球化学特征表明甲玛矿区矽卡岩是由斑岩结晶分异过程中分泌出的岩浆热液交代大理岩而形成。文章通过对甲玛铜多金属矿床地质、地球化学特征的详细分析和讨论,提出该矿床成因是与斑岩成矿作用有关的斑岩-矽卡岩-角岩型矿床。 相似文献
3.
4.
西藏墨竹工卡县甲玛矿区筒状矿体的发现及其地质意义 总被引：5，自引：3，他引：2
甲玛铜多金属矿床是冈底斯成矿带内与斑岩成矿作用有关的斑岩-矽卡岩型矿床。通过对甲玛矿区16号、32号勘探线剖面上主成矿元素以及其他常微量元素矿化分布规律的分析,指出在16线ZK1620～ZK1618之间存在筒状钼铜矿体,其角岩中矿体最大厚度491.38 m,铜平均品位0.21%,钼平均品位0.046%,矿化中心位于ZK1616附近;同时,在林布宗组与多底沟组层间构造带中产出巨厚的矽卡岩型铜钼（金银）多金属矿体,矿体厚度最大达252.2 m,铜平均品位0.75%,钼平均品位0.10%,金平均品位0.24 g/t,银平均品位12.26 g/t。在32线ZK3212～ZK3220范围内也存在筒状钼铜矿体,角岩型矿体最大厚度826 m,铜平均品位0.24%,钼平均品位0.054%,矿化中心位于ZK3216附近;角岩矿体下部为矽卡岩型铜钼（金银）多金属矿体,矿体最厚处超过127.9 m,铜平均品位0.72%,钼平均品位0.053%,金平均品位0.11g/t,银平均品位7.02 g/t。研究表明,甲玛铜多金属矿存在一个以ZK1616～ZK3216一带为矿化中心的筒状矿体（角岩+矽卡岩型矿体）,在筒状矿体的深部可能存在隐伏含矿斑岩体。 相似文献
5.
青藏高原甲玛斑岩成矿系统首例3000 m科学深钻的初步认识 总被引：2，自引：2，他引：0
青藏高原碰撞造山带中复杂的地质结构、深部矿产资源潜力和高效的勘查评价技术体系一直是地质学家关注的焦点,也是亟需攻克的重要科学难题.受国家重点研发计划-深地专项资助,在冈底斯成矿带甲玛斑岩成矿系统实施首个3000 m科学深钻.通过多次研讨和反复论证,确定科学施工位置、角度以及施工工艺.历时488天的施工,完成了科学深钻,总进尺3003.33 m.该科学深钻直接揭示甲玛超大型斑岩成矿系统3000 m以浅的地质信息:浅部为角岩型铜钼矿体、中部为矽卡岩型铜多金属矿体、深部为斑岩型钼铜矿体以及核部蚀变与矿化均不发育的无矿核.角岩中主要为细脉浸染状的黄铜矿、辉钼矿化,并发育黑云母化和弱绿泥石化蚀变.矽卡岩中从上到下具有清晰的分带结构,即石榴子石绿泥石角岩、绿泥石石榴子石角岩、透辉石石榴子石矽卡岩、石榴子石矽卡岩、石榴子石硅灰石矽卡岩、硅灰石矽卡岩、矽卡岩化大理岩.矿化主要为浸染状的斑铜矿、黄铜矿、辉钼矿.深部斑岩为复式岩体,主要为二长花岗斑岩,侵位较早,后被花岗闪长斑岩、石英闪长玢岩等以岩脉的形式穿切侵位.花岗闪长斑岩与矽卡岩关系最为密切.多相的复式斑岩体也揭示了甲玛斑岩成矿系统的无矿核.根据现有工业指标,科学深钻共计探获21层矿体,累计厚度583.46 m,以铜、钼矿化为主,局部发育钨矿化,同时伴生金、银矿化.甲玛科学深钻首次直接揭示青藏高原3000 m以浅的地质信息和斑岩成矿系统结构,为青藏高原地质结构研究提了科学样品,也为深部资源探测和勘查技术体系研究提供了关键支撑.后续将针对其开展详细的地球化学分析、地球物理测井、高光谱测量以及指针矿物分析等研究,并结合地表勘查评价成果,建立3000 m以浅的多元信息综合勘查评价模型,进而定位预测深部矿产资源,实现增储示范. 相似文献
6.
西藏甲玛矿区铅锌矿体成因研究及其找矿意义 总被引：1，自引：0，他引：1
西藏甲玛铜多金属矿床是近年来在冈底斯成矿带取得找矿突破的超大型矿床之一。本文通过甲玛铜多金属矿床与典
型喷流沉积矿床的对比研究,指出甲玛铜多金属矿床成因是与斑岩成矿作用有关的斑岩-矽卡岩型矿床,由产于斑岩中的
钼（铜）矿体、产于矽卡岩中的铜多金属矿体、产于角岩中的钼铜矿体以及外围独立金矿体构成了完整的甲玛斑岩成矿系
统。甲玛矿床同典型喷流沉积矿床的主要区别在于：①地质特征：岩浆热液不仅在林布宗组与多底沟组扩容空间内可形成
层状矽卡岩,而且在林布宗组的泥质灰岩夹层中也可形成小规模、透镜状、囊状矽卡岩;矿区不存在喷流岩,前人认为的
喷流岩实际上是矽卡岩化角岩;矿床的主成矿年龄为14~16Ma,成矿与中新世冈底斯碰撞造山带发生拆沉、大规模的地壳
伸展作用及大规模斑岩体侵位有关;矽卡岩铜多金属矿体不存在喷流沉积矿床所特有的二元结构,矽卡岩顶部与顶板围岩
之间为渐变过渡关系;粗粒结构的矽卡岩亦是岩浆热液长时间补给而使矿物自形生长的结果。②地球化学特征：元素地球
化学特征方面成矿元素组合以Cu,Mo,Au,Ag为主,少量Pb,Zn;多底沟组灰岩中Mn相对于区域背景含量为负异常;甲玛铅
锌矿体的Zn/ （Pb+Zn）比值较低,主要集中在0~0.1和0.2~0.45两个区间内;矿床的矿化分带表现出：由岩体中心向四周Mo
→Cu+Mo→Cu→Pb+Zn,为典型的斑岩铜钼矿成矿系统的矿化分带。同位素地球化学特征方面硫同位素比值主要呈负值且
变化范围很窄,而硅同位素比值则以正值为特征。此外,文章建议在念青唐古拉具有类似甲玛矿区成矿地质条件地区,以
岩浆热液矿床成因为指导,建立依据浅边部铅锌矿（化）体,向深部（中心）追索铜钼矿体或钨矿体的找矿模型。 相似文献
7.
西藏甲玛铜多金属矿床深部斑岩矿体找矿突破及其意义 总被引：7，自引：0，他引：7
甲玛铜多金属矿是西藏冈底斯成矿带中东段勘查程度最高、成矿元素与矿体类型复杂的超大型斑岩-矽卡岩型矿床。通过4年多、近350 个钻孔的验证,不仅实现了矽卡岩矿体的找矿突破,同时在0-40线深部发现了产于二长花岗斑岩与石英闪长玢岩中的斑岩钼（铜）矿体,建立了“四位一体”的找矿勘查模式。斑岩矿体赋存标高一般处于4 600 m以下,矿体走向NW-SE,倾向NE,近直立,矿体垂向延伸大于350 m;斑岩矿石以发育细脉-浸染状、网脉状构造为特征;矿石中的矿石矿物主要为黄铜矿与辉钼矿,少见斑铜矿;脉石矿物主要为石英。初步查明:与铜矿化有关的含矿岩体主要为偏中性的石英闪长玢岩,蚀变以典型的细粒热液黑云母交代角闪石斑晶和基质而成的黑云母化蚀变为主;与钼矿化有关的含矿岩体主要为二长花岗斑岩,蚀变以硅化为主,次为绿帘石化、泥化和钾化。斑岩体与碳酸盐岩接触带常产出厚度超过200 m的巨厚矽卡岩矿体,且在岩体一侧有内矽卡岩产出。甲玛深部斑岩矿体的发现不仅证实了“斑岩-矽卡岩型”的矿床成因观点,而且完善了甲玛矿床成矿模式与勘查模型。 相似文献
8.
西藏甲玛铜多金属矿床矽卡岩中辉钼矿铼-锇同位素定年及其成矿意义 总被引：36，自引：1，他引：35
西藏甲玛铜多金属矿床中辉钼矿是主要的矿石矿物,普遍发育,产出于不同的矿石类型(角岩型、矽卡岩型、斑岩型)矿石中。辉钼矿大多分布于裂隙、节理面上和石英脉或不同岩性岩石中。矽卡岩型矿石中辉钼矿呈微细粒浸染状、团斑状、脉状等,直接分布于矽卡岩中或矽卡岩中后期的石英脉中。采集西藏甲玛铜多金属矿床矽卡岩型矿石中不同产状的辉钼矿,进行铼-锇同位素测年,得到等时线年龄为(15.34±0.10)Ma,模式年龄变化于(15.21±0.22)Ma～(15.50±0.22)Ma,说明甲玛的辉钼矿成矿年龄集中在15Ma左右。结合前人的年代学研究成果,认为甲玛铜多金属矿成矿时代与冈底斯斑岩铜矿带斑岩铜矿的成矿年龄相近,可以否定甲玛铜多金属矿海底喷流沉积成矿成因的观点,为甲玛铜多金属矿的成矿成因和斑岩-矽卡岩型矿体的深部找矿提供了理论依据。 相似文献
9.
西藏甲玛斑岩成矿系统中厚大矽卡岩矿体控矿因素研究 总被引：11，自引：2，他引：9
西藏甲玛斑岩矿床是冈底斯成矿带上具有重大经济意义和科学研究意义的超大型矿床,近年来,取得了重大的找矿突破,现已累计查明和控制铜金属资源储量超过700万吨,共伴生钼、铅+锌、金、银资源储量均达到大型以上规模。笔者在充分收集、整理甲玛矿床最新勘查、研究成果的基础上,对矿区386个钻孔样品化学分析数据进行了系统梳理和分析,按一般工业指标边界品位圈定矽卡岩型铜钼矿体、矽卡岩型铅锌矿体,对厚大矽卡岩型矿体在平面上、剖面上的分布及产出特征进行了全面、系统的分析。研究发现,甲玛矿区厚大矽卡岩矿体主要分布于3个区域:1矿区中部斑岩接触带;2矿区南部铜山滑覆体内;3矿区北西部牛马塘一带。对于不同部位的厚大矿体,其控矿因素各不相同,按主要制约因素,可以概括为:岩体接触带控矿、滑覆体构造控矿和背斜核部构造控矿。文章通过对矿区厚大矽卡岩矿体控矿因素的探讨,建立了相应的岩浆-构造控矿模式,对于完善甲玛斑岩成矿系统模型及矿山开采具有重大意义。 相似文献
10.
矿区出露地层为震旦一寒武系浅变质岩。钼矿床与燕山期高氟、高锂的细粒少斑黑云母花岗岩和花岗斑岩存在密切的空间、时间关系,钼矿化赋存在岩体的内外接触带,包括含辉钼矿萤石石英脉,含辉钼矿的裂隙脉和蚀变岩石（云英岩化）内浸染状产出的钼矿化,含辉钼矿的萤石石英脉是受NEE-SWW向和近SN向裂隙带控制,构成矿床的富矿体,矿区内的富矿作用为钾长石化、黑云母化、云英岩化、萤石化、硅化、绢云母化和绿泥石化,其中,与钼矿化关系密切的蚀变作用是黑云母化、云英岩化、萤石化和硅化。 相似文献
11.
Guboglo M. N. 《GeoJournal》1980,4(1):53-58
International unity is becoming ever stronger in this country owing to an increasing similarity in the development of the cultural environment. This comprises the provision of all the country's republics with a sufficient number of schools, theatres, and other institutions and cultural information media in accordance with the needs of the population. An important part is played by the rise in ‘the general educational level, as well as the level of professional qualifications and skills. Among all the Soviet nations and nationalities, this rise being more rapid among formerly backward peoples. Prominent among the factors of internationalization is the progressive development of the nationalities’ cultural resources, while professional culture is being increasingly brought within the reach of the masses.The implementation of the nationalities policy promotes the all-round development of all Soviet nations and nationalities, their drawing together, the upsurge of the individual capabilities of every Soviet citizen. 相似文献
12.
Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth
B. P. Kondratyev 《Astronomy Reports》2017,61(8):709-714
It is known from observations that the center of mass of the Moon does not coincide with the geometric center of its figure, and the line connecting these two centers is not aligned with the direction toward the center of the Earth, instead deviating toward the Southeast. This stationary deviation of the axis of the inertia ellipsoid of the Moon to the South of the direction toward the Earth is analyzed. A system of five linear differential equations describing the physical libration of the Moon in latitude is considered, and these equations are derived using a new vector method taking into account perturbations from the Earth and partly from the Sun. The characteristic equation of this system is obtained, and all five oscillation frequencies are found. Special attention is paid to the fifth (zero) frequency, for which the solution of the latitude libration equations are stationary and represents a previously unknown additional motion of the rotational axis of theMoon in a cone with a small opening angle. In contrast to the astronomical precession of the Earth, the rotation of the angular-velocity vector is in the positive direction (counter-clockwise), with the period T 3 = 27.32 days. On this basis, this phenomenon has been named “quasi-precession.” This quasi-precession leads to a stationary inclination of the major axis of the inertia ellipsoid of theMoon to the South (for an observer on Earth), making it possible to explain one component of the observed deviation of the center of mass of the Moon from the direction toward the Earth. The opening angle of the quasiprecession cone is approximately 0.834″. 相似文献
13.
14.
Chronological analyses of correlations between certain global repeating events (mass extinctions of marine organisms, meteorite impacts, and flashes in the frequency of geomagnetic reversals) during the Phanerozoic Eon and the motion of the solar system in the Galaxy are presented for five rotationally symmetrical models for the regular Galactic gravitational field. Thirteen of sixteen mass-extinction events can be described by a repetition interval of 183±3 million years. This is in agreement with the anomalistic period (interval between two subsequent passages of the Sun through the apocenter of its Galactic orbit) in the model of Allen and Martos. The positions of the minima and maxima in Gaussian functions approximating the frequency distribution for geomagnetic reversals also agree with the times of passage of the Sun through the apocenter and pericenter, respectively, of its Galactic orbit in this model. The maximum in the distribution of the deviations of the dates of mass extinctions from the nearest dates of impacts of large, crater-forming bodies is close to zero, providing evidence that many such events are correlated. As a rule, extinctions follow impact events. The impacts of large bodies have occurred most often when the solar system passes through the Galactic plane, while mass extinctions occur more often at some distance from the Galactic plane (about 40 pc). As a rule, intervals of increases in the frequency of geomagnetic reversals coincide with dates of impacts of large bodies. At the same time, these intervals do not show a clear correlation with the dates of mass extinctions. The intensity of mass extinctions, like the energy released by impacts, is consistently higher in periods when the Sun is moving from the apocenter toward the pericenter of its orbit, than when it is moving from the pericenter toward the apocenter. Thus, there is evidence for a variety of relationships between repeating global events in the Phanerozoic and the motion of the Sun in the Galaxy. Long-period variations in the frequency of geomagnetic reversals are correlated with the orbital motion of the Sun, and increases in the frequency of geomagnetic reversals are correlated with impacts. Mass extinctions are correlated with the impacts of large bodies, whose motions may have been perturbed by clouds of interstellar material concentrated toward the Galactic plane and by the shock front associated with the Perseus spiral arm, through which the solar system passes. The velocity of the Sun relative to the spiral pattern is estimated. 相似文献
15.
位于华北和扬子两板块碰撞带中的苏鲁榴辉岩形成的温压条件不但是超高压，而且是高温。榴辉岩的PTt轨迹表明其为陆-陆磁撞俯冲带的产物。榴辉岩的区域性围岩花岗质片麻岩为新元古代同碰撞期花岗岩，榴辉岩及其他直接围岩皆呈包体存在于其中，并见新元古代花岗岩呈脉状侵入榴辉岩包体中。区域性围岩新元古代花岗岩的锆石中发现有柯石英、绿辉石等包裹体，表明新元古代花岗岩的组成物质也经受过超高压变质作用，且榴辉岩与围岩新元古代花岗岩的锆石U-Pb体系同位素年龄基本相同。但新元古代花岗岩所记录的变质作用和变形作用期次（或阶段）却少于榴辉岩。椐上述可得如下推断：超高压榴辉岩与新元古代花岗岩岩浆是同时在碰撞带底部（俯冲板块前部）形成的；榴辉岩的第一折返阶段是由新元古代花岗岩岩浆携带上升的，其第二折返阶段是和新元古代花岗岩一起由逆冲及区域性隆起而上升，遭受剥蚀。 相似文献
16.
某高速公路下伏煤矿采空区稳定性分析 总被引：10，自引：0，他引：10
在论述某高速公路下伏砦脖煤矿采空区地质、采矿和工程地质特征的基础上, 进行了稳定性数值模拟分析, 定性与定量地分析与评价了该煤矿采空区的地表变形特征及稳定性。研究结果表明: 该煤矿采空区的变形尚未完成, 对拟建的高速公路将产生很大的危害, 必须采取相应的工程治理措施。 相似文献
17.
18.
摩擦桩基桩土间极限摩阻力取值问题探讨 总被引：1，自引：0，他引：1
通过对广珠东线高速公路横沥大桥的试桩及土体的工程地质条件分析,总结出影响摩擦桩基桩土间极限摩阻力取值的一般问题以及解决问题的方法和措施。 相似文献
19.
The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads 总被引：3，自引：1，他引：2
Clemente Irigaray Francisco Lamas Rachid El Hamdouni Tomás Fernández José Chacón 《Natural Hazards》2000,21(1):65-81
In order to characterise the influence of the heavyrains on the observed landslides during the 1996–1997hydrological cycle, rainfall records for the last 100years are analysed from 104 stations in easternAndalusia. Regarding the amounts of rain recordedbetween October 1996 and March 1997 in the 104stations studied, 31 presented new all-time records;15 presented values that were 80–100% of thepre-1995 record; 49 stations, 80–50%; and 9stations, < 50%. A map has been devised of thesusceptibility of the materials through which thesouth-eastern Andalusian road network crosses,together with an inventory of the damage caused byinstability phenomena on banks and cuttings of theroad network during the winter of 1996–1997. Therelationships between the rainfall during the studyperiod, the damage caused to the road network and thesusceptibility of the materials affected are analysed.The results indicate that there is a clearcorrespondence between the rainfall recorded and thesusceptibility of the materials with the inventorieddamage. It is concluded that the widespread seriousdamage caused in early 1997 to the roads andsurrounding areas in the Alpujarra region and thecoast of the Province of Granada was mainly caused bythe extraordinarily heavy rains. However, considerablyless damage was observed where the susceptibility ofthe terrain is low, thus highlighting the extremeusefulness of terrain-susceptibility maps for riskprevention and territorial planning. 相似文献
20.
The structure of the eastern Pyrenees consists mainly of south-directed thrusts involving basement and cover rocks. An antiformal stack developed by the piling up of basement thrust sheets which outcrop in the Axial zone. These structures account for a thin-skinned thrust model rather than a vertical fault model in which the Axial zone would be essentially autochthonous, and the North-Pyrenean fault the axial plane of a fan thrust system. New data from the Eastern Pyrenees and the thin-skinned model suggest that(1) the structure east of the Pedraforca nappe is similar to that of the Central Pyrenees; (2) the cover rocks of the South-Pyrenean units and of the Axial zone-after restoration—built up a northwards-thickening prism consistent with the existence of a unique Pyrenean sedimentary basin during Mesozoic time; (3) the Axial zone is only a complex antiformal stack developed as a part of South-Pyrenean system related to the Paleogene thrusting-tectonics. The Axial zone palaeogeographic area had no special meaning during Mesozoic time. 相似文献