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大石桥菱镁矿区诸矿床已初步查明为蒸发沉积成岩-热液交代富集型,本文进一步研究热液的物质来源。该区青山怀矿床的菱镁矿及蚀变白云岩的稀土总丰度、铺和重稀土均高于未蚀变白云岩。后者的稀土型式反映沉积成因,菱镁矿和蚀变白云岩则反映热液富集交代型式,热液为混合岩化热液。自元古宙混合岩的强烈蚀变中获得稀土,并从长石中获得Eu,并与蚀变混合岩达到稀土平衡。由含碱氯化络合物搬运,在循环过程中淋滤了围岩(白云岩)的物质。菱镁矿通过品格收容和晶问沉淀捕获稀土。显示了高浓度卤水在搬运、沉淀过程中的稀土分馏。物质来源主要来自混合 相似文献
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本文叙述了辽宁省海城市牌楼镇发达菱镁矿、滑石矿矿区地层、构造、赋矿层位等控矿因素,对区内菱镁矿、滑石矿矿体特征、矿石矿物组成、矿石化学成分、质量、品级等进行了研究分析,确定该矿床成因为区域沉积变质热液交代型矿床。 相似文献
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白云鄂博矿床稀土矿物稳定同位素特征及其意义 总被引：4，自引：0，他引：4
稀土元素是白云鄂博矿床最有特色的矿产。本文在详细讨论了稀土矿物氧、碳同位素制样方法的基础上，对矿床中晚期脉、白云石型矿石、萤石型矿石中的主要稀土矿物进行了系统的氧、碳同位素分析。其中，晚期脉中的氟碳酸盐矿物的碳、氧同位素值较低，具有幔源热液结晶的特点；白云岩型矿石中氟碳铈矿δ１３Ｃ在－１．１‰～－３．４‰，δ１８Ｏ在８．６‰～１２．０‰；独居石δ１８Ｏ在５．７‰～１１．４‰，磷灰石δ１８Ｏ在６．３‰～９．４‰；萤石型矿石中氟碳铈矿δ１３Ｃ在－５．２‰～－５．８‰，δ１８Ｏ在３．６‰～５．５‰；独居石δ１８Ｏ在３．５‰～４．５‰。结合矿床地质特征分析，矿区萤石型矿石和晚期脉的形成可能与深源热液有关；而白云岩中的稀土矿化作用则表现出多源多期次的特点 相似文献
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和静县哈勒哈特菱镁矿地质特征与找矿方向 总被引：1，自引：0，他引：1
新疆和静县哈勒哈特菱镁矿,产于南天山中泥盆统萨阿尔明组下段第五岩性层中,该矿床由32个矿体组成,主要赋矿岩性为厚层白云岩夹菱镁矿透镜体、矿化白云岩及少量生物碎屑灰岩.矿石矿物为菱镁矿,脉石矿物主要为白云石.哈勒哈特菱镁矿中MgO含量为41.82％-45.87％,CaO含量为1.23％～5.54％,SiO2含量为0.24％～0.85％,矿石主要为半自形粗晶结构,块状构造.矿床成因类型是与区域变质作用有关的热液矿床.经研究对比发现,可利用矿区地层、构造、地貌和矿物标志等作为矿区和区域找矿标志. 相似文献
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早前寒武纪李老庄铁-菱镁矿床位于华北克拉通南缘安徽霍邱铁矿带中部,赋存于火山-沉积变质岩系中,矿床内同时发育条带状磁铁矿(BIF)矿体和含铁菱镁矿体。为探讨菱镁矿的成因及其与BIF成矿的关系,针对磁铁矿-菱镁矿这一特殊成矿组合,对取自矿体岩芯的样品开展了显微岩相学观察、电子探针和C、O同位素分析研究。结果显示,矿床内与磁铁矿共生的菱镁矿和含铁菱镁矿矿石中的菱镁矿单矿物均含有较高含量的铁。李老庄矿床含铁菱镁矿矿石的δ^18O约为11‰,δ^13C为-2.16‰^-1.35‰;与磁铁矿共生的菱镁矿的δ^18O为12.49‰~15.43‰,δ^13C为-10.66‰^-5.30‰;矿区白云石大理岩的δ^18O为15.2‰~16.1‰,δ^13C为-2.57^-1.91‰,δ^13C与δ^18O呈同步降低。研究认为,该矿床是在形成富镁碳酸盐岩和BIF铁矿层的基础上,经低角闪岩相变质及富铁镁流体的蚀变交代,使成矿物质在赋矿围岩构成的向斜核部叠加富集形成的沉积-热液改造型矿床。 相似文献
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湘西董家河铅锌矿地质特征及成矿物质来源探讨 总被引：2，自引：0，他引：2
湘西董家河铅锌矿区赋存于陡山沱组下部(Zd)微晶白云岩中,顶板为黑色炭质板岩,底板为南沱组冰碛层,矿体产状、矿石矿物组合、矿石组构反映成矿受沉积成岩和后期构造热液活动的双重控制,成矿温度低(130°~170℃),属典型的低温沉积改造型矿床。矿床经历了沉积成岩和后期热液改造阶段,硫、铅、碳氧同位素组成表明成矿物质主要来源于下伏地层和围岩,部分物质来源于深部基底变质岩。 相似文献
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用Y／Ho比值指示俄罗斯乌拉尔南部晶质菱镁矿矿床的成因 总被引：1，自引：1，他引：1
Mikhail T KRUPENIN 《岩石学报》2004,20(4):803-816
乌拉尔省南部赋存有两种类型的晶质菱镁矿:1)白云岩地层中的层状矿体;2)白云质灰岩中的透镜状矿体。晶质菱镁矿矿体位于Riphean系列中下层的白云岩中,而在上层的白云岩单元中缺失。这两种类型的菱镁矿可通过矿体形态、晶体大小、石英和白云石含量不同来进行区分。第一种类型的菱镁矿储量巨大,菱镁矿呈粗粒结构,晶体粒径>10mm(最大达150mm);一般来说,矿体与白云岩围岩界限清楚,这种类型矿床以产在Riphean序列下部为特征。第二种类型的菱镁矿由于菱镁矿矿体穿插进入到白云岩围岩中,矿体很不规则,菱镁矿晶体也相对较小(1-5mm),这种类型的矿体主要产在Riphean中部层位中。这两种矿体都显示了交代成因的特征。但这两种菱镁矿矿石在一些主量元素和稀土元素的分布上具有不同的特征:与第二种类型相比,第一种菱镁矿具有较低的FeO,CaO和SiO2含量,与白云岩围岩(La／Lu>1)相比,具La／Lu<1的轻稀土亏损特征。第二种菱镁矿稀土分馏度较低,在稀土分配方面与白云岩围岩有差别。本文还特别讨论了Y／Ho值的重要性,因为该比值在菱镁矿和围岩中的类似性使得划分菱镁矿形成中的热液和成岩交代过程成为可能。因此我们认为,第一种类型菱镁矿,如具有高Y／Ho比值的Satka和Bakal矿床的形成属于沉积盆地发育过程中的早期成岩阶段;第 相似文献
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江西武山铜矿床是长江中下游地区具有代表性的叠加复合矿床之一。文章选取武山铜矿床典型剖面为研究对象,在野外地质调研和室内岩相学研究的基础上,识别出层状硫化物型、层状矽卡岩型和接触交代矽卡岩型三类矿体,及相对应的3种类型矿石。3类矿石在矿物组合、结构构造和矿物学特征等方面有明显差异,分别显示出原生沉积、叠加改造和岩浆热液成因特征。选择代表性脉石矿物和矿石矿物进行矿物化学研究,认为石榴子石是岩浆期后热液渗滤交代作用的产物,层状矽卡岩中石榴子石相对富Fe,而接触交代矽卡岩中石榴子石相对富Al;矿区内存在2类黄铁矿,即胶状黄铁矿和粒状黄铁矿,分别对应原生沉积成因和岩浆热液交代成因;磁铁矿是与矽卡岩有关的岩浆期后热液交代作用的产物,层状矽卡岩中磁铁矿相对富Mg O和Mn O,贫Al2O3,受地层影响明显,而接触交代矽卡岩中磁铁矿相对富Al2O3,贫Mg O和Mn O,受岩浆岩影响明显。武山铜矿床的形成经历了原生沉积作用、岩浆热液交代作用及叠加改造作用等复杂成矿过程。 相似文献
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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
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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
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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
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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
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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
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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
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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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Michel Westphal Mikhail L. Bazhenov Jean Paul Lauer Diamar M. Pechersky Jean-Claude Sibuet 《Tectonophysics》1986,123(1-4)
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