云南怒江河流沉积物碎屑锆石LA-ICP-MS U-Pb年龄和Hf同位素组成及其地质意义

采用LA-MC-ICP-MS测定技术,对怒江河流沉积物中的碎屑锆石进行了U-Pb和Lu-Hf同位素测定。结果显示,碎屑锆石U-Pb年龄可分为6个组段:50~74Ma、84~235Ma、275~413Ma、451~569Ma、657~1429Ma和1602~3436Ma,其中最主要的年龄组段为50~74Ma和84~235Ma。50~74Ma的年龄段为新特提斯洋从俯冲到碰撞闭合的阶段,约65Ma的年龄峰值可能是印度大陆与欧亚大陆主体碰撞的远程地质记录。84~235Ma年龄段代表了中特提斯洋演化阶段,年龄峰值约为110Ma,可能指示羌塘地块与拉萨地块的碰撞拼接此时已经完成,通过U-Pb年龄分布对比,羌塘地块几乎没有给怒江河流沉积物提供物质。怒江河流沉积物中碎屑锆石的εHf(t)值介于-18.7~+11.7之间,模式年龄分布于0.65~4.05Ga之间,其中中生代碎屑锆石的εHf(t)值分布于-16.4~+2.9之间,与中拉萨地块有密切的亲缘性,同时含有少量北拉萨地块的特征。因此,怒江河流沉积物代表了中拉萨地块与北拉萨地块的特征。     

西藏拉萨地块过铝质花岗岩中继承锆石的物源区示踪及其古地理意义

富含继承锆石的过铝质花岗岩一般来源于富铝质岩石(如变泥质岩)的部分熔融,因而分析这些继承锆石的U-Pb年龄可以像分析沉积岩碎屑锆石的U-Pb年龄一样,提供过铝质花岗岩源区物质中碎屑沉积物物源区的丰富信息。本文报道了中部拉萨地块早侏罗世过铝质花岗岩的全岩地球化学和锆石U-Pb年代学数据,结合拉萨地块已有二叠纪和晚三叠世过铝质花岗岩的继承锆石年代学数据,总结了目前已有的拉萨地块过铝质花岗岩的继承锆石U-Pb年龄特征(共199个谐和测点)。这些过铝质花岗岩属强过铝质S型花岗岩,其中的继承锆石定义了1250~1100Ma(峰值1181±14Ma)和550~450Ma(峰值494±7Ma)2个最突出的年龄群,分别可比于拉萨地块古生代沉积岩的碎屑锆石年龄峰值(约1170Ma)和寒武纪火山岩的侵位时代,明显不同于西羌塘、安多和特提斯喜马拉雅新元古代-古生代沉积岩中的碎屑锆石年龄频谱。拉萨地块过铝质花岗岩中约1181Ma的继承锆石,可能与拉萨地块古生代沉积岩中的同期碎屑锆石一样,都来自澳大利亚南西部Albany-Fraser造山带和东南极Wilkes等地,而约494的继承锆石,既可能来自澳大利亚西部,也可能来自拉萨地块本地。本文提供了拉萨地块与澳大利亚大陆北缘具有古地理联系的过铝质花岗岩继承锆石U-Pb年龄证据。拉萨地块的研究实践表明,采用过铝质花岗岩继承锆石和古生代沉积岩碎屑锆石相结合的锆石U-Pb年代学方法,可为重建冈瓦纳大陆北缘其它微陆块的古地理和构造岩浆演化提供重要约束。     

西藏革吉地区沙木罗组碎屑锆石年代学研究:物源及其对班公湖-怒江特提斯洋西段闭合时限的制约

班公湖-怒江特提斯洋盆的闭合时限对理解班公湖-怒江结合带的构造演化意义重大。本文采用碎屑锆石年代学的方法,分析了班公湖-怒江结合带西段革吉地区沙木罗组下段与沙木罗组上段的物源特征及差异,为班公湖-怒江特提斯洋盆西段的闭合时间提供了新的证据。研究结果表明沙木罗组下段碎屑锆石年龄分布于2586±26Ma～130±1. 5Ma之间,显示出1个主峰年龄约165Ma,1个次峰年龄约240Ma。碎屑锆石年龄分6个组别,集中在2600～2400Ma、2000～1900Ma、1000～840Ma、500～400Ma、340～200Ma和200～130Ma,分别与新太古代克拉通汇聚事件、哥伦比亚超大陆相关的构造热事件、新元古代构造热事件、冈瓦纳大陆边缘安第斯型造山作用的岩浆活动事件、龙木错-双湖结合带岩浆活动事件和班公湖-怒江特提斯洋盆俯冲消减的岩浆活动事件一一对应。沙木罗组上段碎屑锆石年龄分布于2558±22Ma～101±1. 0Ma之间,显示出1个主峰年龄约107Ma,2个次峰年龄分别约226Ma、150Ma。碎屑锆石年龄集中分布于1个年龄组为122～101Ma,记录了班公湖-怒江特提斯洋盆俯冲消减的岩浆活动。通过与潜在源区的年龄谱峰进行对比,沙木罗组下段物源区与南羌塘地块有良好的亲缘性,表明其沉积物物源主要为南羌塘地块,其中南羌塘岩浆弧可能为其主要贡献者。沙木罗组上段物源区与南羌塘地块和北拉萨地块均具有良好的亲缘性,其沉积物物源具有双源性,分别来源于南羌塘岩浆弧和北拉萨岩浆弧。沙木罗组下段和上段沉积物物源的差异性暗示它们形成的沉积环境和物源区不同。对比分析沙木罗组下段和上段岩石学、碎屑锆石形态学等特征,也揭示了类似的差异性。结合其他相关地质资料,认为班公湖-怒江特提斯洋盆在革吉地区的主体闭合时间约115～110Ma,其代表性岩浆事件为南羌塘地块和北拉萨地块的早白垩世岩浆弧,沙木罗组为班公湖-怒江特提斯洋盆由俯冲消减到闭合过程中的沉积产物。     

拉萨—羌塘地体碰撞时限:来自班公湖—怒江缝合带中段多尼组沉积的约束

早白垩世多尼组沿西藏北部班公湖—怒江缝合带沿线广泛分布,其沉积环境、碎屑组成和沉积物源等记录了班公湖—怒江特提斯洋闭合后拉萨—羌塘地体碰撞的演化历史。班戈地区多尼组以角度不整合于侏罗纪海相复理石之上,主要由砾岩、砂岩、粉砂岩、泥岩及少量安山岩夹层组成。砂岩中普遍发育槽状、板状、楔状交错层理,泥岩中可见泥裂,砾岩多为透镜状并发育叠瓦状构造,指示其形成于河流—三角洲沉积,且总体呈现出向上变粗的沉积组合序列。对多尼组中安山岩夹层样品进行LA?ICP?MS锆石U?Pb定年,获得206U/238Pb加权平均年龄为114 ± 0.4 Ma。对砾岩中砾石成分和砂岩碎屑组成的统计分析结果显示,多尼组沉积组合中的碎屑组成主要来自蛇绿岩、中酸性岩浆岩、沉积岩和少量变质岩。砂岩重砂矿物组合和古水流分析结果表明,多尼组的沉积物源主要来自其南北两侧的拉萨和羌塘地体以及其下伏蛇绿岩。综合区域地质资料,班戈地区早白垩世多尼组是班公湖—怒江特提斯洋闭合过程中拉萨—羌塘地体碰撞背景下沉积作用的产物。     

澜沧江河流沉积物碎屑锆石U-Pb年龄、Hf同位素组成及其地质意义

为研究澜沧江沉积物的物质来源及相邻地块的地壳生长和演化规律,利用LA-MC-ICP-MS分析技术,对澜沧江河流沉积物碎屑锆石进行了U-Pb年龄和Hf同位素研究。结果表明：锆石U-Pb年龄主要有5个年龄段,分别是＜177 Ma、201~418 Ma、428~544 Ma、581~1189 Ma和1406~2533 Ma,主要峰值为260 Ma、788 Ma、1 827 Ma和2 474 Ma。其年龄分布特征与北羌塘地块的年龄分布非常一致,说明澜沧江沉积物主要来源于北羌塘地块;结合Hf同位素分析结果,能够反映源区北羌塘地块的形成与演化历史。新太古代-中元古代是北羌塘地块从亏损地幔物质增生的地壳持续生长阶段,它们构成现今北羌塘地块全部地壳物质的78%以上,此后直到0.64 Ga,北羌塘地块的地壳增生作用基本结束。     

班公湖- 怒江缝合带同碰撞海沟盆地砂岩物源分析及其大地构造意义

同碰撞海沟沉积可为重建板块缝合带大地构造演化、约束陆块初始碰撞时间提供重要信息。本文对班公湖-怒江缝合带西段的改则县亚多组和日土县多仁组进行了沉积学、岩相学、碎屑锆石年代学、重矿物研究。沉积学分析表明,多仁组、亚多组沉积于海底扇环境。最年轻的碎屑锆石年龄限制了最早沉积时代为晚侏罗世。多仁组、亚多组砂岩Q：F：L分别为52：4：44、32：8：60,均以丰富的沉积岩和酸性火成岩岩屑及少量的变质岩屑为特征;重矿物以磷灰石、锆石、电气石等稳定重矿物为主。多仁组和亚多组具有相似的碎屑锆石年龄分布模式,主峰分布在350～200 Ma、550～450 Ma、900～750 Ma、1900～1800 Ma、2550～2450 Ma范围内。这些数据表明,亚多组、多仁组碎屑物质来源于沉积区北侧的班公湖-怒江缝合带增生杂岩及南羌塘岩浆岩。多仁组、亚多组出现的大量沉积岩岩屑,表明物源区经历了广泛的构造缩短作用,导致沉积岩和同期岩浆岩被剥蚀,因此多仁组、亚多组是拉萨-羌塘同碰撞的产物。据此推断,沿班公湖-怒江缝合带改则-日土区域拉萨-羌塘初始碰撞发生在晚侏罗世多仁组、亚多组沉积之前。     

班公湖—怒江洋复理石沉积时代:来自改则县亚多村碎屑锆石的制约

木嘎岗日岩群是班公湖?怒江洋的洋盆沉积记录,它的时代归属对约束班公湖?怒江洋的演化具有重要意义.然而自命名以来,木嘎岗日岩群的时代一直争议较大.以班公湖?怒江缝合带中段改则县亚多村一带的木嘎岗日岩群为研究对象,对其进行岩石学和碎屑锆石年代学方面的研究.该区木嘎岗日岩群以薄层砂岩和页岩互层为主,具复理石沉积特征.砂岩碎屑锆石年代学分析结果显示,最小碎屑锆石为149 Ma,最小年龄峰值为156 Ma,指示该地区木嘎岗日岩群的时代为晚侏罗世?早白垩世.在此基础上,对班公湖?怒江缝合带中西段内不同地区木嘎岗日岩群的年龄信息进行搜集和整理,结果显示,木嘎岗日岩群的时代跨度至少为晚三叠世?早白垩世,表明班公湖?怒江洋中西段在晚三叠世?早白垩世内可能是连续演化的.      

中国西秦岭碎屑锆石U-Pb年龄及其构造意义

西秦岭是北接华北克拉通、西接祁连与柴达木、南接松潘—甘孜地块的东秦岭造山带的西延。文中研究了该区从前寒武纪到三叠纪的碎屑沉积岩。这些碎屑沉积岩中分离出的锆石由LA-ICPMS(激光剥蚀等离子体质谱)进行了U-Pb定年。全岩Nd亏损地幔模式年龄类似于扬子克拉通年龄,主要分布于1.55~1.98Ga,峰值为1.81Ga,而与华北克拉通主要为古元古代与太古宙的模式年龄形成明显的对比。泥盆系中的碎屑锆石930~730Ma的U-Pb年龄指示其与扬子克拉通具亲缘性。930~730Ma是源区地壳的强烈增长阶段。二叠系—三叠系的碎屑沉积岩主体以含老于1600Ma的碎屑锆石为特征。碎屑锆石U-Pb年龄与Sm-Nd同位素组成指示此时华北克拉通南缘的基底岩石成为二叠系—三叠系碎屑沉积岩的重要物源。扬子克拉通在三叠纪时与华北克拉通拼接。西秦岭二叠系—三叠系碎屑沉积岩含有高达50%的华北克拉通南缘的基底岩石。     

临沧地体亲缘性及南段组物源——来自泥盆纪—石炭纪南段组碎屑锆石U-Pb年龄的证据

对临沧地体泥盆纪—石炭纪南段组的沉积岩开展碎屑锆石LA-ICP-MS U-Pb定年研究结果表明,所有样品的U-Pb年龄谱存在3个主要峰值:泛非期(530~680Ma)、晚格林威尔期(900~980Ma)和早格林威尔期(1100~1300Ma)。次要峰值年龄为1550~1730Ma和2350~2630Ma,反映了物源区构造-岩浆事件的复杂性。南段组碎屑岩锆石年龄图谱明显区别于思茅地块泥盆纪—石炭纪碎屑锆石年龄图谱,临沧地块南段组碎屑锆石的年龄表明其物源来自东冈瓦纳超大陆,临沧地体应该是来自东冈瓦纳北缘的微地块,这也与其生物特征相吻合。     

拉萨地块晚古生代沉积源区转变——来自措勤地区永珠组碎屑锆石的证据

晚古生代是拉萨地块地质演化的重要转折期,一些关键地质问题存在争论,如拉萨地块来源问题。选择西藏措勤地区上石炭统永珠组为研究对象,石英砂岩中碎屑锆石U-Pb测年数据显示523Ma、920Ma两个年龄峰值。通过与拉萨地块及其周缘晚石炭世冰期之前地层碎屑锆石对比,认为拉萨地块永珠组920Ma年龄峰值更具有冈瓦纳大陆靠印度一侧的物源特征,其与南羌塘、拉萨、喜马拉雅微陆块在裂离之前具有显著的亲缘关系。而含有冰筏碎屑的拉嘎组和来姑组中包含的西澳大利亚物源信息(约1180Ma年龄峰值),暗示来自西澳大利亚的冰筏可能通过洋流作用漂移至拉萨地块而后沉积冰筏碎屑。     

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.