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1.
鞠东阳  庞润连  李瑞  杜蔚 《岩石学报》2022,38(4):1025-1042
月球岩浆洋结晶形成的初始月球内部结构是其后续演化过程的开端,其结晶过程受月球岩浆洋的初始深度和物质组成这两个参数的制约。由于缺少直接来自月球深部的岩石样品,目前关于月球岩浆洋演化过程的探讨主要依赖实验和计算模拟手段。岩浆洋模型中形成的月壳厚度是否与探测结果一致是月球岩浆洋演化模型合理性的重要约束。最新的GRAIL(Gravity Recovery and Interior Laboratory)探测数据推算月壳厚度为34~43km,低于阿波罗时期认为的约70km,这对已有的月球岩浆洋演化模型提出了挑战。本文采用并修正FXMOTR程序包,针对月球岩浆洋在不同的初始深度和物质组成情况下的结晶过程,进行了一系列热力学计算模拟。通过量化月球岩浆洋的初始深度和物质组成对月壳厚度的影响,结合关于月球内部微量元素分配的研究结果,对比了月球岩浆洋结晶后期的残余熔体与原始克里普组分(urKREEP)的成分。本文的模拟结果显示,一个全月幔熔融且初始成分为月球初始上月幔组成(LPUM)的岩浆洋将在其深部结晶2.5%石榴子石,形成的月壳厚度符合GRAIL的约束,并且结晶出了合适的urKREEP成分。在此模型的基础上获取了月球初始的内部成分和密度结构,并对后期月幔翻转(Overturn)的程度进行了探讨。  相似文献   

2.
月球角砾岩是月球陨石的代表性样品,含有多来源的岩屑,是揭示月球内-外动力演化历史的重要窗口。本文对Bechar 003、NWA 13788和NWA 11110月球陨石中的岩屑开展了岩相学、矿物学及地球化学分析,通过岩相、矿物成分、全岩主微量元素等岩石地化综合分析,旨在厘清这3块样品中岩屑的类型、来源与成因机制。结果表明,3块陨石内部的斜长辉长质冲击熔融岩屑、微斑熔融角砾岩屑、以及辉长质斜长岩屑的初始物质由均是月海玄武岩与月球高地岩石的混合物,不同初始物质成分的岩屑表明月表经历了冲击事件,并且冲击事件发生在月表的不同位置,冲击事件造成月球高地岩石与月海玄武岩或非月海溅射物的混合。  相似文献   

3.
王梦玺  陈炳龙  焦建刚 《岩石学报》2018,34(8):2223-2244
坡北杂岩体位于塔里木板块东北缘北山裂谷带,主要由橄榄岩相、单辉辉石岩相、二辉岩相、辉长岩相、苏长岩相和辉长苏长岩相组成。坡一岩体中硫化物矿体赋存于超镁铁质岩中,而坡东岩体中硫化物矿体赋存于辉长苏长岩相中。坡一和坡东岩体不同岩相中单斜辉石的MgO和CaO含量、斜长石的An值和SiO_2含量连续变化且呈负相关,说明二者可能是同一原始岩浆分离结晶的产物。根据前人计算的原始岩浆成分,我们利用MELTS软件模拟了坡北杂岩体的分离结晶过程。结果表明矿物结晶顺序为:橄榄石→橄榄石+单斜辉石→橄榄石+单斜辉石+斜长石→单斜辉石+斜长石+斜方辉石,与岩相观察一致。坡北杂岩体原始岩浆经过20%分离结晶达到S饱和而发生早期硫化物熔离,形成坡一岩体中矿体。因此,在利用具有最高Fo值(90.9mol%)的橄榄石成分进行的模拟中,坡一岩体早期结晶的纯橄榄岩中橄榄石成分与分离结晶趋势线一致,而斜长橄榄岩中橄榄石成分低于趋势线,可能形成于早期硫化物熔离之后。随后岩浆中S再一次不饱和,但坡一岩体橄榄单辉辉石岩和辉长岩中橄榄石Fo和Ni含量在分离结晶趋势线之下,同时坡东岩体不含矿岩石中铂族元素总量主要在8.9×10~(-9)~29.0×10~(-9)之间,且相对于Ni和Cu明显亏损,说明在岩浆分离结晶晚期再次发生硫化物熔离,而且可能是地壳混染引起的,并形成了坡东岩体中的硫化物矿体。坡东岩体橄榄二辉岩和橄榄辉长苏长岩中橄榄石Fo值(74.5mol%~81.0mol%)较低,但变化范围较大,且Fo和Ni呈负相关关系,这可能是由于橄榄石和硫化物熔体在不平衡状态下发生成分交换造成的。坡北杂岩体超镁铁质岩石中单斜辉石Ti O2含量为0.21%~0.83%,阳离子中呈四次配位的Al(AlZ)为0.8mol%~7.8mol%,与裂谷环境堆晶岩中单斜辉石成分相似。因此,坡北杂岩体可能形成于和塔里木二叠纪地幔柱活动相关的裂谷环境。然而,超镁铁质岩石全岩Nd同位素指示其来源于亏损地幔,并不是地幔柱物质熔融的直接产物。纯橄榄岩和异剥橄榄岩La/Sm,Sm/Yb和La/Yb比值指示其源区为尖晶石二辉橄榄岩地幔。因此,坡北杂岩体源区应为浅部以尖晶石二辉橄榄岩为主的亏损岩石圈地幔,地幔柱在源区部分熔融过程中提供了大量的热。  相似文献   

4.
冀北小张家口基性-超基性杂岩体主要由辉石岩和次要的纯橄岩组成,并含有方辉橄榄岩透镜状捕掳体.岩石学和元素地球化学数据表明,辉石岩和纯橄岩可能是堆晶成因,而方辉橄榄岩可能是来自地幔源区的地幔岩捕掳体(抽取玄武质熔体之后的难熔残余).辉石岩和纯橄岩都表现出相当富集的Nd-Sr同位素特征,εND (t)=-2~10,ISr=0.7045~0.7081,表明它们的母岩浆来自富集的岩石圈地幔的部分熔融.化学成分和同位素成分一致表明,母岩浆在以橄榄石和辉石为主的分离结晶过程中,遭受下地壳不同程度的混染.辉石岩受显著混染,不能代表岩石圈地幔的同位素成分;而纯橄岩是最初的分离结晶体,仅受轻微下地壳混染,可近似反应岩石圈地幔源区的同位素成分.小张家口岩体的形成可能与古亚洲洋的缝合(240~250Ma)有关.  相似文献   

5.
大别杂岩内角闪质岩石的稀土元素特征及其成因   总被引:1,自引:0,他引:1  
大别杂岩内角闪质岩石呈透镜状或似层状产出,由10种不同岩类构成。根据稀土元素特征,可把角闪质岩石分为轻稀土富集型和平坦型两大类。稀土元素的定量模拟表明,它们是由上地幔石榴二辉橄榄岩经20%的部分熔融和35—56%的橄榄石(TH1型)和14—20%的橄榄石和单斜辉石(TH2型)的分离结晶形成的。  相似文献   

6.
胶东东部中生代中酸性花岗杂岩形成机理   总被引:2,自引:0,他引:2  
出露在胶东东部地区的中生代中酸性花岗花岩,普遍含有大量的细粒闪长岩类包体,对主体岩石和包体岩石的地质学、岩相学、地球化学以及同位素等方面的综合研究,证实这些主岩是中生代壳幔分层熔融形成的同生壳源岩浆和幔泊岩浆发生混合作用形成混合岩浆,然后通过分离结晶作用形成花岗杂财的不同类型。  相似文献   

7.
辽东硼矿的成矿机制及成矿模式   总被引:7,自引:0,他引:7  
为了解辽东硼矿的成矿机制及建立成矿模式, 分析了含硼岩系、镁质容矿岩石、区域变质作用及混合岩化作用、构造等四大控矿因素, 发现含硼岩系具富硼特征, 容矿岩石具富镁特点并可成为硼质的沉淀剂, 含硼岩系中硼在区域变质和混合岩化过程中得到进一步活化形成含硼热液, 含硼热液在有利的构造空间交代镁质岩石即可形成镁硼酸盐型硼矿.含硼岩系、镁质容矿岩石是硼矿形成的物质基础, 区域变质及混合岩化作用、构造活动是硼矿形成的必要条件.辽东硼矿成矿模式为原始火山-沉积初始富集和部分熔融含硼热液交代镁质岩石.   相似文献   

8.
白垩纪华北克拉通岩石圈经历了巨大的减薄事件,但减薄过程及机制仍存在较大争论。早白垩世的西石门杂岩体是华北克拉通东部与岩石圈减薄相关的重要杂岩体。根据西石门杂岩体形成时代和岩石结构特征将其划分为两套岩石组合。早期岩套由二长闪长岩-二长岩-正长岩系列组成,具等粒结构,形成时代约为135. 6Ma,岩石地球化学成分为SiO_2=51. 72%~68. 56%、MgO=0. 17%~4. 88%,少部分样品表现出C型埃达克岩的特征;晚期岩套由斑状二长岩-斑状正长岩系列组成,具似斑状结构,形成时代约为125. 3Ma,岩石地球化学成分为SiO_2=57. 00%~67. 51%、MgO=0. 61%~3. 37%,其中还存在大量年龄约2500Ma的继承锆石。两套侵入岩均为高钾钙碱性系列但早期岩套多具埃达克质岩特征,晚期岩套岩石中锆石具有更负的ε_(Hf)(t),显示其具有更多的壳源物质组成。角闪石温度计、压力计显示,早期岩套的定位环境为T=883. 66℃、P=194. 95MPa,相当于7. 36km深处;晚期岩套的定位环境为T=642. 34℃、P=26. 81MPa,相当于1. 01km深处。从135. 6Ma至125. 3Ma,地壳快速抬升了约6. 35km。研究认为,在约135. 6Ma时陆内岩浆作用开始影响研究区,软流圈地幔上涌促使地壳物质熔融、混合形成了早期岩套,同时大规模的岩浆活动及地壳褶皱变形导致陆壳加厚。之后岩石圈地幔发生拆沉作用,地壳快速抬升。在约125. 3Ma后,软流圈地幔继续上涌,回弹的陆壳开始发生大规模的熔融形成了晚期岩套。据此认为拆沉作用是中生代华北克拉通岩石圈减薄的主要机制。  相似文献   

9.
李瑞  刘建忠  庞润连  朱丹  鞠东阳  杜蔚 《岩石学报》2022,38(4):1043-1062
由于缺少直接来自月球深部的岩石样品,实验和计算模拟是认识早期月球演化过程的有效方法和手段。20世纪70年代以来,陆续开展了大量的实验岩石学和实验地球化学工作对月球岩浆洋(lunar magma ocean,LMO)演化模型进行验证和修正。但是,学界对LMO模型中的两个关键性参数,即初始物质组成和熔融深度,仍然存在不同的认识。根据月震和重力探测数据推测的平均月壳厚度的差异、月球样品含水量的研究以及新的遥感数据解译发现月表广泛分布富镁铝尖晶石(Cr#<5)等等,直接影响我们对月球初始物质组成和LMO深度以及月球深部高压矿物相的评估。本文通过整理高温高压实验岩石学和实验地球化学在研究LMO演化方面的一系列研究成果,主要聚焦以下几个科学问题:(1)月球初始物质组成中的难熔元素和挥发分含量,以及LMO深度对月壳厚度、结晶矿物的种类及含量有着决定性的影响;(2)高压矿物相石榴子石在月球深部稳定存在的可能性及其对残余岩浆中微量元素的分配行为的制约;(3)特殊类型的月球样品(包括火山玻璃、镁质岩套等)的成因机制对月球深部物质组成具有指示意义;(4)月核的不同物质组成对LMO模型的初始成分含量,特别是微量元素的限定作用。我们以最新的观测数据和月球样品的分析结果为依据,对已有的LMO演化模型进行重新评估,提出月球深部含有石榴子石的LMO演化模型的可能性,并对该方向亟需开展的工作进行探讨。  相似文献   

10.
月球的化学演化   总被引:2,自引:0,他引:2  
月球是一个发生了化学分异的星球,它由月壳、月幔±一个小的金属月核组成。大量观察事实显示月球曾经有过岩浆洋,岩浆洋的结晶分异主导了月球的化学演化。目前主流观点认为,月球是在太阳系演化的早期,至少45亿年前,一个火星大小的星球,与即将完成原始吸积的地球胚胎发生偏心撞击,造成地球的熔融,形成岩浆洋,飞溅出来的物质迅速吸积形成绕地球运动的月球,并且在月球上形成了全球规模的岩浆洋,进而发生了结晶分异。,由于月球上没有海洋和板块俯冲,岩浆洋分异是其化学演化的主要途径。月球岩浆洋的80%~85%在大撞击后的100Ma内已经固化,这可能是由于月球体积小、表面没有大气包裹所致。月球极贫水,因此在岩浆结晶过程中斜长石首先结晶。斜长石由于密度小于玄武质岩浆而漂浮在岩浆洋的表层,橄榄石等密度大的矿物则堆积在岩浆洋的底部。随着结晶分异的进行,残余岩浆不断富集不相容元素,包括K、U等放射性元素;与此同时,密度较大的钛铁矿开始结晶,造成高钛堆晶岩密度大于其下的橄榄石堆晶岩的不稳定结构,进而发生月幔翻转,引发一系列岩浆活动,进而形成月球上特有的镁质系列、碱质系列等岩石。由于月球氧逸度较低,Eu主要以+2价形式存在,因此斜长石高度富集Eu,相应地除高地斜长岩外,其他岩石均表现为Eu高度亏损的特点。与此同时,Re在低氧逸度下表现为强亲铁元素的特点,Re/Os在月球岩浆过程中不发生分异。月球的体积远小于地球,因而其演化时间远远短于地球,很多原始的分异被完整地保留下来。因此月球的化学演化是类地行星早期演化过程的“化石”,尽管与现代的地球存在较大差异,但是对于认识地球早期演化具有借鉴意义。  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.
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   

13.
14.
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   

15.
16.
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   

17.
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   

18.
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   

19.
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   

20.
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   

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