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1.
何明友 《矿床地质》1997,16(2):181-188
利用热力学方法计算了西秦岭铀矿床含矿热液中铀的迁移形式。结果表明,从含矿热液早阶段到主成矿作用发生之前,热液中的铀主要以「UO2(CO3)^0」形式迁移;在晚阶段残余热液中,铀的迁移形式改变为「UO2(SO4)^0」为主。铀迁移形式改变的原因与大气降水中SO^2-4离子的大量带入有关,表明含矿热液来自深部而非大气降水。  相似文献   

2.
王贵  王伟  王刚  李涛  刘涛 《西北地质》2021,(2):157-165
红石泉矿床在中国是最为典型的伟晶岩型铀矿床.近几年,通过系统工作,发现红石泉矿床具有多期次铀成矿的特点,不同成矿期形成了不同的矿石、铀矿物和蚀变特征.分别对不同铀成矿作用的拆分研究发现,在中条晚期花岗质岩浆演化到后期形成了富含晶质铀矿的浅肉红色伟晶花岗岩矿石,基本无蚀变,矿体集中于伟晶花岗岩体核部;在海西期含矿热液沿伟...  相似文献   

3.
核桃坝矿床是著名的沽源-红山子铀成矿带上新近勘查突破的重要铀矿床之一。为恢复成矿过程、划分成矿阶段和探讨矿床成因,本文开展了系统的矿相学和成矿年代学研究,以期为区内铀矿勘查和找矿突破提供理论支持。矿相学研究表明,矿床矿石矿物以铀石为主,成矿作用可划分为早期钠长石化交代阶段、早期热液成矿阶段、晚期热液成矿阶段和成矿后阶段四个阶段。核桃坝矿床属于碱交代型(钠交代)热液铀矿床。沥青铀矿U-Pb同位素表观年龄、电子探针化学年龄以及等时线年龄综合研究显示,矿床形成时代应在99. 1Ma左右,是晚白垩世成矿作用的产物。核桃坝矿床可能是富铀岩体在碱交代作用后形成流体(富铀含硅酸成矿流体)在外部条件改变的情况下沉淀成矿。因此,矿体的定位与富铀岩体关系密切,富铀岩体附近的开放空间(断裂构造、层间破碎带等)是重要的找矿方向。  相似文献   

4.
湘赣边区NNE向走滑断裂-流体-铀成矿动力学分析   总被引:7,自引:0,他引:7  
李紫金  傅昭仁 《现代地质》1998,12(4):522-531
以湘赣边区NNE向走滑断裂系统构造解析及其演化和动力学分析为主线,结合含矿流体的运动学过程研究,进行热液铀成矿动力学分析,以探讨成矿作用的动力来源、作用机制和演化过程。  相似文献   

5.
摩洛哥受西非克拉通、大西洋和阿尔卑斯造山带三大构造域的联合作用,其构造历史久远,太古宙至新元古代早期西非克拉通的构造演化、泛非期构造岩浆活动、早古生代克拉通边缘的裂解与海西造山,以及中新生代构造活动在该区均有反应。受这种构造背景的控制,摩洛哥的矿床分布具有一定的时空规律,太古宙克拉通基底、伊比鲁利亚期岩基及泛非期构造带均有银、铁、铀、钽、铌、金、铜和稀土等矿产出露,加里东期有沉积型铁矿床产出,海西期有重要的VMS型铅-锌-铜矿床和矽卡岩型矿床产出,阿尔卑斯期有磷矿、MVT型铅-锌矿和重晶石矿等产出。沉积成矿作用、岩浆热液成矿作用及构造热液成矿作用在摩洛哥都有显著体现,最主要的矿产类型为磷酸盐矿、银矿、MVT型铅-锌矿及重晶石矿。  相似文献   

6.
从构造演化—岩浆作用—成矿流体系统将火山岩-花岗岩型铀矿作为统一体开展成矿作用研究。在总结华南热液型铀矿成矿地质特征的基础上,根据区域铀时空分布特征,结合成矿溶液的氢、氧同位素组成,从动力学过程阐述了成矿物质来源,并进而分析了成矿流体演化及成矿作用过程。认为早寒武世富铀地层是华南热液型铀矿最本质的铀物质来源,成矿流体是岩浆水和降水混合的产物,岩浆作用形成了成矿物质的"汇"区,燕山期伸展或向伸展过渡的地球动力学背景下的岩浆作用,促成了成矿热液系统的形成、演化及成矿作用的发生,随着岩浆作用物质-能量场的减弱,华南热液型铀矿成矿作用终止。  相似文献   

7.
新疆哈图-包古图金铜矿集区锆石年龄及成矿特点   总被引:10,自引:4,他引:6  
申萍  沈远超  潘成泽  潘鸿迪  代华五  孟磊 《岩石学报》2010,26(10):2875-2893
晚古生代,新疆西准噶尔地区发生了强烈的构造-岩浆活动和广泛的金、铜成矿作用,形成了哈图-包古图大型金铜矿集区。锆石SHRIMP U-Pb年龄测量表明,含矿闪长岩体形成于312.3±2.2Ma~332.0±2.8Ma,矿集区岩浆活动及其成矿作用发生在石炭纪。哈图-包古图矿集区成矿作用有4个显著特点:(1)地幔流体活动强烈;(2)构造应力转化快速;(3)拉斑系列和钙碱性系列岩浆成矿;(4)多种矿化类型集中发育等。哈图-包古图矿集区发育石英脉型-蚀变岩型金矿床、斑岩型铜矿床和同期的石英脉型-蚀变岩型金矿床以及热液脉型铜金矿床的成矿系列。  相似文献   

8.
鹿井矿田铀成矿地质特征及找矿潜力分析   总被引:1,自引:0,他引:1  
对鹿井矿田以往的勘查成果进行了系统梳理,认为鹿井矿田是构造-岩浆作用导致的铀成矿物质汇聚区,燕山晚期岩浆热液及基性脉体热液促成了汇聚区内成矿物质的再迁移及成矿作用的发生;矿田内现有矿床的空间分布特征是剥蚀作用的结果;控矿因素本质上是地球化学障;铀成矿壳层分析表明矿田仍具较大的找矿潜力,现有矿床的近外围地区、以酸性矿石为主的矿床深部及红层覆盖区均值得开展新一轮勘查工作。  相似文献   

9.
黎心远  赵元艺 《地质学报》2018,92(2):244-262
黑龙江三矿沟-庄乎河地区位于多宝山成矿带北侧,区内构造-岩浆-热液活动复杂,主要发育有三矿沟矽卡岩型矿床及庄乎河热液脉型矿床。本文选择三矿沟-庄乎河地区的岩浆岩主体为对象开展年代学、岩石学及元素地球化学等综合研究,系统厘定两个时期的岩浆岩,包括海西期庄乎河流纹岩(288~294 Ma)、庄乎河花岗斑岩(297~303Ma),燕山期三矿沟花岗闪长岩(172~179Ma)和庄乎河矿区石英闪长岩(165~176Ma)。三矿沟-庄乎河地区的成(含)矿岩浆岩均具有高硅、高铝及富碱的I型花岗岩特征,富集Rb、Sr、Ba、K等大离子亲石元素,亏损Nb、Ta、Ti等高场强元素,轻重稀土元素分馏明显,δEu亏损等特征。本次研究认为研究区与成矿作用有关的构造背景为活动大陆边缘,三矿沟-庄乎河地区在海西期受到古亚洲洋俯冲作用形成庄乎河花岗斑岩及流纹岩,而燕山期三矿沟花岗闪长岩和庄乎河石英闪长岩则与成矿富集作用有关,且两区矿床成矿作用与燕山期古太平洋俯冲作用密切相关。  相似文献   

10.
湖南双峰紫云山隆起区金矿成矿机制探讨   总被引:3,自引:0,他引:3  
戚学祥 《黄金地质》1998,4(1):50-56
湖南双紫云山隆起区金矿受剥离断层控制,矿质主要来源于岩浆热液。成矿作用过程中,剥离断层带深部和浅部分别形成深部含矿岩浆热液循环系统和地下水热液循环系统,两热液系统在空间上的交汇处矿质沉淀、富集形成金矿化体。  相似文献   

11.
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.
13.
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   

14.
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   

15.
从榴辉岩与围岩的关系论苏鲁榴辉岩的形成与折返   总被引:4,自引:1,他引:4       下载免费PDF全文
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.
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  
陈银生 《世界地质》1999,18(1):54-59
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   

18.
19.
We first re-examined the apparent polar wander curves for stable Eurasia and Africa since the Triassic. These curves were then combined together with curves of North and South America according to the kinematics of the Atlantic ocean and a synthetic polar wander curve was given. Then, most of the paleomagnetic results from the Tethys mobile belt, from the Atlantic to the Pamirs, were analysed.Several groups of plates, microplates and blocks can be seen. First, relatively stable regions like Maghreb and Sicily, which have not moved much. Then we have a group formed by Iberia, Sardinia, Italy and, to a lesser extent, Corsica and the Western and Central Alps. For these blocks, movements are anticlockwise rotations chiefly driven by the anticlockwise rotation of Africa, but they are sometimes stronger.To the east, a major change takes place. The north of the Aegean Sea and the Ionian zone are clockwise rotated and these rotations are recent: Oligocene-Miocene for the first part, Pliocene to the present for the second part.A major problem arises in Turkey, Caucasus and Iran. Paleomagnetic results indicate a position far to the south of Eurasia, and, at the same time, geological evidence is in favour of a position close to Eurasia. We discuss these discrepancies.  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   

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