冈底斯中段岗讲斑岩铜钼矿床锆石U-Pb和辉钼矿Re-Os年代学及其地质意义

岗讲铜钼矿床是西藏冈底斯成矿带中段典型的斑岩型矿床,岗讲矿床成岩成矿时代、岩浆演化过程及其与成岩成矿关系尚不明确,利用LA-ICP-MS锆石U-Pb定年方法对岗讲矿区主要岩体二长花岗斑岩、花岗闪长斑岩和英云闪长玢岩成岩时代进行研究,获得锆石U-Pb年龄加权平均值分别为16.6±0.3 Ma (MSWD=0.94,n=10)、16.1±0.2 Ma (MSWD=1.07,n=12)、14.4±0.4 Ma (MSWD=1.12,n=7);同时采用辉钼矿Re-Os同位素测年方法首次对岗讲矿床石英硫化物脉中的辉钼矿进行定年,获得12件辉钼矿Re-Os同位素模式年龄集中于13.24±0.20 Ma~13.55±0.22 Ma,加权平均年龄为13.4±0.1 Ma (MSWD=0.65),等时线年龄为13.6±1.6 Ma (MSWD=1.2).结果表明:(1) 岗讲矿区复式岩体侵入序列为含巨斑黑云二长花岗岩-二长花岗斑岩-花岗闪长斑岩-流纹斑岩 (深部定名为英云闪长玢岩),成岩时限为16.6~14.4 Ma,成矿时代为13.4 Ma左右,成岩成矿是一个连续的岩浆演化过程;(2) 辉钼矿中Re含量为155.4~171.1 μg/g,均值为162.9 μg/g,指示其成矿物质中有幔源成分的加入;(3) 矿床产出于中新世印度-亚洲大陆碰撞后伸展构造环境.      

西藏邦铺钼铜矿区花岗斑岩成岩年龄研究

邦铺钼铜矿床是发育于冈底斯成矿带的大型斑岩型钼铜矿床,矿区内岩浆岩发育,(二长)花岗斑岩为成矿母岩。利用斑岩中锆石离子探针U-Pb法和全岩Rb-Sr法测定邦铺含矿斑岩的年龄,以确定含矿斑岩的形成时代。花岗斑岩中锆石SHRIMP U-Pb法测定其年龄为14.2 Ma±0.2 Ma(MSWD=0.79);二长花岗斑岩中锆石SHRIMP U-Pb法测试值为13.9 Ma±0.3 Ma(MSWD=3.05);全岩Rb-Sr等时线年龄为13.88 Ma±0.38 Ma(MSWD=1.7)。因此14.2 Ma~3.9 Ma年龄值可以作为邦铺矿区含矿斑岩体的结晶年龄。     

福建紫金山矿田罗卜岭铜钼矿化斑岩锆石LA-ICP- MS U-Pb年龄及成矿岩浆高氧化特征研究

罗卜岭斑岩铜钼矿床是紫金山Cu-Au-Mo浅成低温-斑岩矿田内新近发现的大型斑岩铜钼矿床,本文在岩芯及光薄片系统观察的基础上,分析了矿化斑岩锆石LA-ICP-MS U-Pb年龄及锆石Ce4/Ce3+比值.罗卜岭赋矿斑岩体可分为两期,早期为角闪黑云母花岗闪长斑岩及黑云母花岗闪长斑岩,晚期为黑云母花岗闪长斑岩.早期角闪黑云母花岗闪长斑岩和黑云母花岗闪长斑岩锆石LA-ICP-MS U-Pb年龄分别为103.7±1.2Ma,MSWD=0.33和103.0±0.9Ma,MSWD=1.00;晚期黑云母花岗闪长斑岩锆石LA-ICP-MS U-Pb年龄为97.6±2.1Ma,MSWD=6.00.罗卜岭成矿斑岩基质普遍发育硬石膏,两期成矿斑岩锆石都具较高的Ce4 +/Ce3平均值,在630 ～770之间,高于区内非成矿花岗岩锆石的Ce4+/Ce3+平均值(182 ～577),显示罗卜岭斑岩矿床成矿岩浆具有高氧逸度的特征.据罗卜岭斑岩矿床的形成时代、高氧逸度岩浆特征,结合华南地区中生代构造背景,我们初步认为罗卜岭斑岩矿床的形成可能和中生代古太平洋向北西西方向俯冲有关.     

沱沱河地区多才玛铅锌矿晶屑熔结凝灰岩锆石SHRIMP年龄及岩石地球化学特征

多才玛铅锌矿是近年来沱沱河地区发现的一处超大型铅锌矿床,位于青藏高原东北部的东羌塘地块。恶劣的气候条件以及矿床发现时间晚,造成该地区地质研究程度极低。笔者重点对容矿围岩之一的晶屑熔结凝灰岩进行了SHRIMP锆石U-Pb测年和岩石化学成分分析。研究表明,晶屑熔结凝灰岩中锆石呈自形-半自形,发育典型的岩浆锆石振荡生长环带,Th/U值较高(0.39~0.69),为典型的岩浆锆石。测得晶屑熔结凝灰岩U-Pb加权平均年龄为(254.0±2.9)Ma,MSWD=1.9;谐和年龄值为(254.0±3)Ma,MSWD=1.9,属海西末期。岩石化学成分表现为高硅过铝、贫钙和镁,明显富集Rb、Th、U等大离子亲石元素,强烈亏损P、Ti、Nb、Ta等高场强元素,富集LREE,Nb/Ta值(7.78~8.29)等特征表现为壳源岩浆和弧火山岩特征。综合分析认为,254Ma±时期本区处于深俯冲消减阶段。     

辽宁鞍山地区东山杂岩带3.3～3.1Ga期间的岩浆作用——锆石SHRIMP U-Pb定年

报道了鞍山地区东山杂岩带奥长花岗岩和二长花岗岩的锆石SHRIMP U-Pb年龄。中粗粒奥长花岗岩中岩浆锆石的年龄为3329Ma±22Ma（MSWD=9.6）,存在年龄为3687~3784Ma的残余锆石。细粒奥长花岗岩和二长花岗岩中岩浆锆石的年龄分别为3141Ma±8Ma（MSWD=1.5）和3142Ma±5Ma（MSWD=0.35）。表明约3.3Ga和3.1Ga是鞍山地区2个重要的地壳演化阶段。     

黑龙江鹿鸣钼矿区花岗质杂岩锆石U-Pb年龄、Hf同位素、辉钼矿Re-Os年龄及其地质意义

鹿鸣超大型钼矿(钼金属量89万吨,平均品位0.084%)产于小兴安岭-张广才岭成矿带北段,矿体呈细脉浸染状赋存于二长花岗斑岩和二长花岗岩体内,围岩蚀变有钾化、绢云母化、硅化、绿泥石化、碳酸盐化等,矿化类型主要为斑岩型矿化。鹿鸣矿区含矿岩体二长花岗斑岩和二长花岗岩的锆石U-Pb定年、Hf同位素及辉钼矿Re-Os同位素定年研究表明:二长花岗岩和二长花岗斑岩锆石的U-Pb年龄分别为186.8±2.1Ma和183.2±1.9Ma,形成于燕山早期,二长花岗斑岩晚于二长花岗岩。6个样品辉钼矿Re-Os等时线年龄为176.7±4.4Ma(MSWD=0.92),Re含量变化于30×10-6~49×10-6。二长花岗岩的锆石εHf(t)值变化于1.1~3.8,Hf单阶段模式年龄为729Ma,两阶段模式年龄为1055Ma;二长花岗斑岩的锆石εHf(t)值变化于0.4~5.9,Hf单阶段模式年龄为741Ma,两阶段模式年龄为1075Ma。研究表明成矿与二长花岗斑岩有关,并且二长花岗岩和二长花岗斑岩岩浆为中新元古代新生的地壳物质熔融的产物,成岩成矿作用与古太平洋板块俯冲作用(或佳木斯与松嫩地块的拼合)有关。     

藏东玉龙斑岩铜矿带扎拉尕含矿斑岩体锆石U-Pb年龄及其地质意义

玉龙斑岩铜矿带扎拉尕斑岩铜钼矿床位于玉龙斑岩铜矿带中北部,赋矿岩体侵入下二叠统火山岩及三叠系砂泥岩中,主要由早阶段为二长花岗斑岩及晚阶段正长花岗斑岩组成。分析了早阶段二长花岗斑岩及晚阶段正长花岗斑岩锆石 LA-ICP-MS U-Pb 年龄。早阶段二长花岗斑岩该年龄为（38.5±0.2） Ma, MSWD=1.12,晚阶段正长花岗斑岩该年龄为（38.5±0.2） Ma, MSWD=1.08,早阶段和晚阶段含矿斑岩体锆石U-Pb 年龄完全一致。这表明早晚两阶段成矿岩体是在很短的时间间隔内形成的。扎拉尕赋矿斑岩体形成年龄为（38.5±0.2） Ma。据扎拉尕斑岩矿床形成时代及藏东地区在始新世至渐新世地质构造背景,提出扎拉尕斑岩矿床和玉龙斑岩铜矿带的形成与印度板块-欧亚板块碰撞在藏东地区形成的走滑构造活动诱发的岩浆活动有关,为陆陆碰撞走滑构造环境的斑岩矿床。     

粤北大宝山矿区船肚岩体和大宝山花岗斑岩锆石LA-ICP-MS U-Pb年龄及多阶段成矿分析

粤北大宝山矿床矿区出露船肚和大宝山矿化岩体。本文分析了两个岩体矿物组成特征和锆石LA-ICP-MS U-Pb年龄。船肚岩体为似斑状结构,块状构造,主要由似斑状花岗岩、似斑状二长花岗岩及似斑状花岗闪长岩等组成,和云英岩型及矽卡岩型Mo-W矿化紧密共生。大宝山岩体为斑状结构,块状构造,主要由碱长花岗斑岩、普通花岗斑岩、二长花岗斑岩及花岗闪长斑岩组成,矿物组成和船肚岩体的基本相同,和细脉浸染状Mo-W矿化紧密共生。船肚似斑状二长花岗岩和大宝山二长花岗斑岩锆石LA-ICP-MS U-Pb年龄分别为162.1±1.6 Ma,MSWD=2.72和165.8±2.0 Ma,MSWD=1.38。据船肚和大宝山岩体矿物组成基本相同、岩石结构不同及两者锆石Th/U比值不同和U-Pb年龄存在约4 Ma左右时差,提出大宝山矿区在燕山期发生了两阶段岩浆成矿事件,第一阶段岩浆成矿事件发生在166 Ma左右,形成大宝山斑岩型矿床,第二阶段岩浆成矿的形成时间约为162 Ma左右,形成船肚似斑状二长花岗岩及与岩体紧密共生的矽卡岩型和云英岩型矿化;大宝山斑岩体和船肚似斑状岩体是同一岩浆房两次脉动侵入形成的。     

南岭诸广山北体复式花岗岩锆石SHRIMP U-Pb年龄及多期岩浆活动

诸广山复式花岗岩基位于湘、赣、粤三省交界处,是南岭花岗岩的重要组成部分,由南体和北体组成,出露面积大于5000 km2,形成于加里东期、印支期、燕山期3个时代。通过对诸广山北体3期花岗岩锆石SHRIMP U-Pb定年,结果表明,加里东期花岗闪长岩锆石SHRIMP U-Pb年龄为(414.5±4.5)Ma(n=13,MSWD=0.52)、(417.3±4.8)Ma(n=12,MSWD=0.84),形成于晚志留世末。印支期黑云母二长花岗岩锆石SHRIMP U-Pb年龄(207.5±2.7)Ma(n=10,MSWD=1.6),形成于晚三叠世末。燕山期二云母二长花岗岩锆石SHRIMP U-Pb年龄(148.2±1.7)Ma(n=13,MSWD=0.93),形成于晚侏罗世。该成果为南岭地区构造-岩浆演化及成矿作用研究,提供了重要的花岗岩年代学依据。     

云南马厂箐岩体(似)斑状花岗岩锆石LA-ICP-MS U-Pb年龄及地质意义

应用LA-ICP-MS对马厂箐岩体中(似)斑状花岗岩的锆石进行了U-Pb定年和微量元素分析。在CL图像上,(似)斑状花岗岩中锆石均发育有典型的振荡环带,锆石的稀土元素配分模式表现为亏损轻稀土,富集重稀土,具有强烈正Ce异常和中度负Eu异常,且呈现出较高的Th/U比值等特征,表明所测锆石均为典型的岩浆锆石。马厂箐岩体(似)斑状花岗岩锆石U-Pb加权平均年龄为(33.78±0.21)Ma(MSWD=0.71),累计概率统计得到正长斑岩锆石U-Th-Pb年龄为(35.6±0.3)Ma、花岗斑岩锆石U-Th-Pb年龄为(35.0±0.2)Ma,宝兴厂矿段铜钼矿辉钼矿Re-Os等时线年龄分别为(35.8±1.6)Ma和(33.9±1.1)Ma,乱硐山矿段接触交代型金矿白云母40Ar/39Ar年龄为(35.25±0.36)Ma,人头箐—金厂箐矿段热液脉型金成矿白云母40Ar/39Ar年龄为(35.35±0.32)Ma,反映斑岩型铜钼矿化、接触交代型金矿化和热液脉型金矿化为同一个构造-岩浆-热液成矿系统的产物,Ⅱ期(33～37Ma)正长斑岩+二长斑岩+花岗斑岩+(似)斑状花岗岩岩性组合是成矿的地质体,为成矿提供了物质、流体和热动力条件,这期斑岩-热液-成矿系统的持续时间约为4Ma,铜、钼、金的成矿主要发生在Ⅱ期岩浆活动的早-中期。     

Unity of the national and the international in the socio-cultural development of the peoples of the USSR

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.     

Deviation of the major axis of the inertia ellipsoid of the Moon from the direction toward the Earth

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″.     

Global repeating events in the history of the Earth and the motion of the Sun in the Galaxy

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.     

摩擦桩基桩土间极限摩阻力取值问题探讨

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。     

从榴辉岩与围岩的关系论苏鲁榴辉岩的形成与折返

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。     

某高速公路下伏煤矿采空区稳定性分析

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。      

On the consistency of proposed models for the Pyrenees with the structure of the eastern parts of the belt

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.     

Paleomagnetic implications on the evolution of the tethys belt from the atlantic ocean to the pamirs since the triassic

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.