江西省花山洞钨矿花岗岩锆石U Pb定年及其地质意义

花山洞钨矿是在江西省西北部新近发现的与花岗岩有关的钨矿床,为了确定矿区花岗岩的物质来源,形成过程以及构造背景环境,探讨成岩与成矿作用之间的关系。利用地球化学方法分析了与花山洞钨矿密切相关的花岗岩的地球化学特征,采用LA ICP MS锆石U Pb定年的方法测定了花岗岩的形成时代。岩石地球化学表明,花岗岩具有较高的w(SiO2)(6823%~7378%)含量;全碱含量w(Na2O+ K2O)为593%~7%;富Na,K2O/Na2O为038~086,小于1;w(Al2O3)为1441%~1581%,A/CNK均大于11,为过铝质岩石。富集Rb、Tu、U、La、Nd等大离子亲石元素,亏损Ba、Nb、Ti、Sr、P等元素,具大陆地壳的特征;稀土总含量较低,基本无δCe异常。稀土配分型式总体向右倾斜,为典型的‘I’型花岗岩特征;轻稀土斜率较大,分异较为明显,重稀土较为平缓,分异不明显。花岗岩锆石U Pb测年结果为(807±8)Ma,与前人测得的辉钼矿Re Os年龄极为接近,故花岗岩应该为成矿岩体。结合区域资料,综合分析可知,矿区花岗岩应主要来源于地壳物质,有部分地幔物质的加入;其可能形成于大陆边缘弧环境。花山洞钨矿床成矿年龄略晚于矿区花岗岩,表明成矿作用是花岗岩分异演化的结果,是晋宁期岩浆活动的产物。     

山东郭城牧牛山二长花岗岩的岩石成因:地球化学和锆石U—Pb年代学制约

山东胶莱盆地东北缘郭城牧牛山二长花岗岩的锆石LA--ICP--MS U--Pb年代学及岩石地球化学特征表明,牧牛山花岗岩为古元古代(2 138±15 Ma)岩浆侵入产物,是一套钾玄岩系列岩石,A/CNK为1.07~1.13。稀土配分曲线表现为右倾模式,轻稀土和重稀土分异明显,Eu/Eu*值为0.59~0.71。蛛网图表明明显富集大离子亲石元素(Rb、K),相对亏损高场强元素(Th、U、Nb、Ta、Ti、P)。岩石10 000 Ga/Al值(2.73~2.85),为A型花岗岩。岩石的Mg~#值为12~28,Nd/Th值为1.62~1.96,Rb/Sr值为4.70~9.71,显示壳源特征。综合分析认为,古元古代胶辽地块向西俯冲引发幔源岩浆底侵,导致地壳物质部分熔融形成牧牛山花岗岩。     

西秦岭熊山沟岩体地球化学及构造环境分析

在区域地质调查及综合研究的基础上,对位于西秦岭天水东南部地区的原百花岩体进行了详细的岩石学、岩石地球化学、岩体接触关系、同位素年龄研究,从中解体出熊山沟岩体,并初步了解了该岩体的岩浆活动规律。熊山沟岩体早期岩石类型为斜长花岗岩,岩石化学成分K2O含量较低,K2O∕Na2O比值为0.33～0.42;晚期岩石类型为二长花岗岩,岩石相对富集K2O,K2O∕Na2O比值为1.01～1.43,岩石属拉斑-钙碱性系列;微量元素富集Th、Hf、Nb、Zr等元素;稀土元素以富集轻稀土,无铕负异常或铕负异常不明显为主要特征;氧同位素值较低（δ^18O为＋3.32‰）,岩石具Ⅰ型花岗岩的特征,岩浆来源于下地壳物质,形成于大陆弧构造环境。     

桂北融水地区钾镁煌斑岩Ar- Ar年代学、地球化学特征及其构造意义

桂北地区发育较多的钾镁煌斑岩脉,可能为该区近源金刚石重砂矿的母岩,对于其形成时代一直是长期争议悬而未决的重要地质问题。本文研究表明,融水地区金云钾镁煌斑岩的金云母(斑晶、基质) 40 Ar- 39 Ar冷却封闭年龄为203~204 Ma,表明其形成于晚三叠世。岩石SiO 2为55. 68%~56. 85%,高钾(K 2O/Na 2O=1. 87~3. 06)、高Mg # (71. 90~73. 20)、轻稀土富集、重稀土相对亏损,轻重稀土分异明显,Eu略亏损,富集大离子亲石元素,亏损高场强元素,地球化学特征表明其来源于俯冲流体交代的富集地幔特征。上述研究表明,扬子克拉通东南缘桂北地区中生代岩石圈地幔为经历俯冲流体交代的富集地幔,并于晚三叠世经历了重要的岩石圈伸展减薄构造事件,其形成可能与古太平洋板块平板式俯冲有关。     

中祁连西段野马山岩基年代学、地球化学特征及地质意义

野马山岩基位于中祁连地块西段,由早期岩体(花岗闪长岩、斑状二长花岗岩)和晚期岩体(二长花岗岩)组成,二者呈侵入接触。LA-ICPMS锆石U-Pb定年表明,早期岩体侵位时代为中奥陶世((469.0±1.3)Ma),晚期岩体侵位时代为晚奥陶世((450.0±1.0)Ma)。早期岩体Si O2=59.8%~64.2%,K2O/Na2O1,且A/NKC=0.8~1.0,为准铝质岩石;微量元素相对富集Rb、U、Th和亏损Ba、Nb、Ta、Sr、P、Ti;稀土总量为97.7×10-6~185×10-6,且(La/Yb)N=5.57~12.47,LREE/HREE=7.7~11.3,具轻重稀土分馏明显,轻稀土富集,弱Eu负异常(δEu=0.66~0.89)特征。晚期岩体Si O2=69.8%~76.5%、K2O/Na2O=1.2~1.7、A/NKC=1.0~1.1,属弱过铝质花岗岩;稀土总量为78.97×10-6~244.92×10-6,轻重稀土分馏不明显((La/Yb)N=1.90~5.72),强Eu负异常(δEu=0.11~0.24)。岩石地球化学特征表明,野马山岩基早期岩体为I型花岗岩,形成于俯冲环境,晚期岩体为高分异的I型花岗岩,形成于后碰撞环境。结合岩体产出的区域构造位置及区域地质演化,认为早古生代北祁连洋发生了双向俯冲,野马山岩基为其向南俯冲碰撞的产物。     

新疆博格达东缘色皮口地区晚石炭世裂谷火山岩地球化学、锆石U-Pb年代学及Hf同位素研究

新疆色皮口地区位于博格达造山带东段北部,区域内的上石炭统柳树沟组火山岩为玄武岩-玄武安山岩、角斑岩-石英角斑岩和流纹岩,组成双峰式火山岩建造。岩石SiO 2含量为48.07%~77.62%,赖特碱度率(AR)为1.35~4.7,Na2O+K2O含量为3.74%~9.02%,K2O/Na2O值为0.04~1.04,为低钾高钠钙碱性-碱性岩石。玄武岩、玄武安山岩TiO 2=0.86%~1.7%,较高的Al、低Mg,以及低K2O/TiO 2和K2O/P2O5比值(分别为0.13~1.81、0.36~6.00),反映了在岩浆演化过程中发生了不明显的分离结晶作用。玄武岩、玄武安山岩、角斑岩不相容元素K、Rb、Th、Ba强富集,高场强元素Nb、Ta、Zr、Hf无富集,Ti亏损不明显,玄武岩(Th/Nb)N值为1.36~6.55,Nb/La值为0.29~0.44,具有较低的Nb/Zr比值(0.03~0.05)。由玄武岩到石英角斑岩,稀土元素组成略右倾平行曲线簇,倾斜度(轻重稀土分异度)略增大,铕负异常趋于明显(δEu=0.81~1.17)。流纹岩不相容元素K、Rb、Th、Ba富集,高场强元素Nb、Ta、Zr、Hf富集,流纹岩稀土总量增高,轻重稀土分异增大,明显铕负异常(δEu=0.27~0.50),显示后期较强的岩浆分异作用。石英角斑岩的锆石LA-ICP-MS U-Pb定年结果为314.9±1.2Ma(n=16,MSWD=0.4,Th/U比值在0.56~1.21之间),这表明石英角斑岩形成时代为晚石炭世。石英角斑岩中锆石的176Hf/177Hf比值均分布在0.282897~0.283097之间,并具有较高的正εHf值(11~18),平均值为14,Hf的模式年龄tDM2介于180~628Ma。所有锆石的176Hf/177Hf比值和εHf值位于亏损地幔演化线与下地壳之间,并靠近亏损地幔演化线。上述特点反映晚石炭世火山岩形成于板内裂谷环境,下部玄武岩与角斑岩-石英角斑岩具有同源特征,暗示岩浆源区来源于亏损地幔,并受地壳混染。     

东天山白山钼矿区花岗岩的岩石成因:锆石U-Pb年代学、地球化学及Hf同位素约束

新疆东天山晚古生代中酸性岩浆活动广泛分布且已有较多研究成果。近年来在该区识别出印支期岩浆作用,然而研究者对其岩石成因、源区性质及相关动力学问题研究较少。白山钼矿区位于东天山康古尔-黄山韧性剪切带东段,是东天山多金属成矿带印支期斑岩型钼矿床,其矿体主要赋存于深部花岗斑岩体外接触带中。本文则对白山钼矿区深部花岗斑岩开展了岩石地球化学、锆石U-Pb年代学及Lu-Hf同位素组成研究。SIMS锆石U-Pb定年结果表明,白山花岗斑岩体大约侵位于226.8±3.2Ma。岩石地球化学结果表明,花岗斑岩具高Si O2含量(68.87%~72.82%)及全碱含量(6.85%~8.17%),铝饱和指数A/CNK为0.93~1.06,均小于1.1,为准铝质至过铝质I型花岗岩。岩石具有明显的轻重稀土分异和弱的Eu负异常,富集大离子亲石元素(K、Rb、Sr),相对亏损高场强元素(Nb、Ta、Ti、Th),具高Sr/Y和La/Yb比值的特点,显示与埃达克质岩石相似的地球化学特征。白山花岗斑岩锆石Lu-Hf同位素数据显示,其具较高的εHf(t)值(+8.0~+11.0)和较年轻的地壳模式年龄tCDM(556~758Ma)。结合岩石地球化学及同位素地球化学特征,本文认为白山花岗岩体可能来源于增厚下地壳物质的部分熔融,并可能混有幔源岩浆物质,形成于东天山碰撞造山作用之后的板内伸展阶段。     

东天山石炭纪—二叠纪花岗质侵入岩的地球化学及地质意义

东天山吐哈盆地南缘至喀拉塔格—星星峡地块,晚古生代花岗质侵入岩岩石类型主要有花岗闪长岩、二长花岗岩、石英闪长岩、石英二长闪长岩。岩石地球化学特征表明：Si O2质量分数为57.3%~77.76%,全碱（K2O＋Na2O）质量分数为4.14%~10.49%,Ca O质量分数为0.49%~6.56%,Al2O3质量分数为11.39%~14.76%,铝饱和指数（A/CNK）为0.77~1.04,属于高钾钙碱性系列—钾玄质系列的准铝质花岗岩。稀土总量较高且轻稀土富集,富集Rb、Th、U、K、Pb,而亏损Nb、Ta、Ti、P,无明显负Eu异常。区域构造背景、岩石学和地球化学特征综合分析显示,东天山石炭纪—二叠纪花岗质侵入岩,是后碰撞构造演化阶段岩浆活动的产物,主要由幔源岩浆底侵引起的地壳物质部分熔融所形成的钙碱性花岗闪长质岩浆经高度演化及分异结晶作用而成。     

冈底斯西段萨果花岗岩地球化学和年代学特征及其地质意义

萨果花岗岩位于冈底斯西段中、南亚带交界位置,主要岩石类型有二长花岗岩和花岗闪长斑岩,岩石总体上富Si,K,贫Mg,Ca,w(Si O2)=64.84%~70.1%,w(K2O)/w(Na2O)=1.21~1.75,A/CNK=0.99~1.2,w(Al2O3)介于14.48%~15.52%,属过铝质岩石,稀土总量(ΣREE)变化范围为256.1×10~(-6)~428.8×10~(-6),LREE/HREE>10,轻稀土富集,δEu=0.77~0.85,弱的铕负异常。Rb、Th和K等大离子亲石元素富集,而Ba、U和Ta等高场强元素亏损。岩石学特征表明岩石总体上具岛弧花岗岩特征,仅少数岩石显示碰撞花岗岩的特点,结合区域花岗岩浆演化和构造环境等地质背景,推断萨果花岗岩体可能形成于俯冲向同碰撞的过渡环境。二长花岗岩的LA-ICP-MS锆石U-Pb年龄为(88.6±1.5)Ma。萨果花岗岩是新特提斯洋向北俯冲的产物,表明印亚大陆碰撞起始时间晚于88.6 Ma。     

北黄海盆地花岗斑岩锆石U-Pb年代学、地球化学及其地质意义

北黄海盆地X1和X2钻井岩心揭示上侏罗统中有侵入的花岗质岩石,镜下鉴定其为花岗斑岩。对花岗斑岩进行了主量、微量和稀土元素测试分析,样品的Si O2含量介于70.22%~71.88%之间,K2O/Na2O比值介于0.95~1.68之间,A/CNK比值介于0.75~1.12之间,有高钾钙碱性、弱碱质-偏铝质性质。微量元素组成富集Rb、Th、U等元素,相对亏损Nb、Eu、Sr等元素。稀土总量较高(∑REE=50.38×10-6~162.27×10-6),轻稀土(LREE)相对富集(LREE/HREE=6.86~25.43,(La/Yb)N=10.06~57.76),具有明显的Eu负异常(?Eu=0.65~0.83)。样品的Th含量高,与Rb呈正相关性,综合主量元素特征(A/CNK1.1),判别其为I型花岗岩。LA-ICP-MS锆石U-Pb测年结果表明X1井花岗斑岩年龄为110±1 Ma,X2井花岗斑岩年龄108±1 Ma、107±1 Ma,形成于早白垩世晚期。结合区域构造背景及岩石地球化学特征认为,北黄海盆地花岗斑岩形成于板块碰撞后的伸展构造背景。     

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.     

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。      

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。     

The Importance of the Precipitation and the Susceptibility of the Slopes for the Triggering of Landslides Along the Roads

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.     

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.