吉林省桦甸地区太古宙花岗质片麻岩的侵位与变形研究     

周永胜  林强 《吉林地质》1997,16(1):33-41

根据岩石组合，分布，接触，包裹关系以及结构和构造，吉林省桦甸地区太古宙花岗质林岩为角闪英云闪长质片麻岩类和黑云母花岗闪长质片麻岩类，角闪英云闪长质片麻岩类为变形前侵入体，黑云母花岗闪长质片麻岩类为同变形侵入体，两类花岗质片麻岩的侵位是晚太古宙近东西向构造变形相伴生的岩浆活动事件。  相似文献   

北秦岭德河黑云二长花岗片麻岩体的成岩时代--TIMS和SHRIMP锆石U-Pb同位素年代学   总被引：17，自引：6，他引：17  

陈志宏陆松年  李怀坤宋彪李惠民  相振群 《地质通报》2004,23(2):136-141

德河黑云母二长花岗片麻岩体侵位于秦岭造山带北秦岭前寒武纪变质岩系内,遭受了强烈的变形作用改造,具有典型S型花岗岩的矿物组成特征。TIMS和SHRIMP法锆石U-Pb同位素年龄测定结果分别为(964.4±5.2)Ma和(943±18)Ma,两者在误差范围内是一致的。鉴于SHRIMP法锆石微区测年具有更好的代表性,建议以(943±18)Ma代表德河黑云母二长花岗片麻岩的侵位时代。  相似文献   

晚太古代Sanukite（赞岐岩）与地球早期演化   总被引：9，自引：12，他引：9  

张旗王焰  钱青翟明国  金惟浚王元龙　简平 《岩石学报》2004,20(6):1355-1362

Shirey and Hanson(1984)将某些太古代的高镁闪长岩套称为sanukite(赞岐岩),类似于日本中新世(11～15Ma)Setouchi火山岩带的高镁安山岩。Sanukitoids由闪长岩-二长闪长岩-花岗闪长岩组成,不同于TTC岩套(奥长花岗岩-英云闪长岩-花岗闪长岩)。Sanukitoids具有下列地球化学特征:富Mg,Mg~#>0.60,Ni和Cr>100μg/g,Sr和Ba>500μg/g,LREE富集(大于球粒陨石100倍),无Eu异常。高镁安山岩在太古代很少见,而其相应的侵入岩高镁闪长岩或sanukitoids,虽然数量也很少,但却是各地晚太古代地体中随处可见的。Sanukitoids的原始岩浆是交代的地幔楔部分熔融形成的,随后可能经历了广泛的分离结晶作用。TTC和sanukitoids岩套可以相伴产出,二者均与板片熔融有关,TTG与其直接有关,sanukitoids可能与其间接有关。全球Sanukitoids主要集中在晚太古代时期,可能暗示板块的消减作用在～3.0Ga以后才起了重要的作用。  相似文献   

Stable staurolite–cordierite assemblages in K‐poor metapelitic schists in Aston and Hospitalet gneiss domes of the central Pyrenees (France,Andorra)          下载免费PDF全文

J. E. Mezger  J‐L. Régnier 《Journal of Metamorphic Geology》2016,34(2):167-190

Staurolite–cordierite assemblages are common in mica schists of the Aston and Hospitalet gneiss domes of the central Axial Zone, Pyrenees (France, Andorra). Within a 200 m wide zone, staurolite, cordierite and andalusite porphyroblasts contain inclusion trails that preserve the same stage of development of a crenulation cleavage, strongly suggesting that all three phases are contemporaneous. Their syntectonic growth occurred during a short period at the beginning of the formation of the dominant schistosity (S₂) of the domes. Staurolite and cordierite touching each other further indicates an equilibrium relationship. Whole‐rock analyses show that some staurolite–cordierite schists are depleted in K₂O compared to post‐Archean shales (PAAS) and amphibolite facies pelites. Analysis of the st‐crd paragenesis in K‐poor schists without muscovite using KFMASH and MnNCKFMASH petrogentic grids, pseudosections and AFM compatibility diagrams predicts stable conditions at pressures of ~3.5 kbar at 575 °C. For metapelites with intermediate X_Mg values (0.7 >  X_Mg >0.48) a ‘muscovite‐out window’ exists from 550–650 °C at 3.5 kbar in the KFMASH system. Conventional thermobarometry (GB‐GASP, AvT‐AvP) and petrogenetic grids show an isobaric P–T path to peak temperatures of ~650 °C, supported by the presence of sillimanite‐K‐feldspar gneiss and migmatites. LP‐HT metamorphism in the Aston dome is related to early Carboniferous (c. 339 Ma) granitic intrusions into the dome core. As metamorphism is directly linked with the formation of the main S₂ schistosity, the temporal relations demonstrated in this study conflict with previous studies which constrained LP‐HT metamorphism and the development of flat‐lying schistosity to the late Carboniferous (315–305 Ma) – at least in the eastern Axial Zone.  相似文献   

The tectono‐metamorphic evolution of the very low‐grade hangingwall constrains two‐stage gneiss dome formation in the Montagne Noire (Southern France)          下载免费PDF全文

M. P. Doublier  S. Potel  K. Wemmer 《Journal of Metamorphic Geology》2015,33(1):71-89

The Montagne Noire in the southernmost French Massif Central is made of an ENE‐elongated gneiss dome flanked by Palaeozoic sedimentary rocks. The tectonic evolution of the gneiss dome has generated controversy for more than half a century. As a result, a multitude of models have been proposed that invoke various tectonic regimes and exhumation mechanisms. Most of these models are based on data from the gneiss dome itself. Here, new constraints on the dome evolution are provided based on a combination of very low‐grade petrology, K–Ar geochronology, field mapping and structural analysis of the Palaeozoic western Mont Peyroux and Faugères units, which constitute part of the southern hangingwall of the dome. It is shown that southward‐directed Variscan nappe‐thrusting (D₁) and a related medium‐P metamorphism (M₁) are only preserved in the area furthest away from the gneiss dome. The regionally dominant pervasive tectono‐metamorphic event D₂/M₂ largely transposes D₁ structures, comprises a higher metamorphic thermal gradient than M₁ (transition low‐P and medium‐P metamorphic facies series) and affected the rocks between c. 309 and 300 Ma, post‐dating D₁/M₁ by more than 20 Ma. D₂‐related fabrics are refolded by D₃, which in its turn, is followed by dextral‐normal shearing along the basal shear zone of both units at c. 297 Ma. In the western Mont Peyroux and Faugères units, D₂/M₂ is largely synchronous with shearing along the southern dome margin between c. 311 and 303 Ma, facilitating the emplacement of the gneiss dome into the upper crust. D₂/M₂ also overlaps in time with granitic magmatism and migmatization in the Zone Axiale between c. 314 and 306 Ma, and a related low‐P/high‐T metamorphism at c. 308 Ma. The shearing that accompanied the exhumation of the dome therefore was synchronous with a peak in temperature expressed by migmatization and intrusion of melts within the dome, and also with the peak of metamorphism in the hangingwall. Both, the intensity of D₂ fabrics and the M₂ metamorphic grade within the hangingwall, decrease away from the gneiss dome, with grades ranging from the anchizone–epizone boundary to the diagenetic zone. The related zonation of the pre‐D₃ metamorphic field gradients paralleled the dome. These observations indicate that D₂/M₂ is controlled by the exhumation of the Zone Axiale, and suggest a coherent kinematic between the different crustal levels at some time during D₂/M₂. Based on integration of these findings with regional geological constraints, a two‐stage exhumation of the gneiss dome is proposed: during a first stage between c. 316 and 300 Ma dome emplacement into the upper crust was controlled by dextral shear zones arranged in a pull‐apart‐like geometry. The second stage from 300 Ma onwards was characterized by northeast to northward extension, with exhumation accommodated by north‐dipping detachments and hangingwall basin formation along the northeastern dome margin.  相似文献   

Impact of gneissic layering and localized incipient melting upon melt flow during experimental deformation of migmatites     

《Journal of Structural Geology》2016

In this study, we test experimentally the role of compositional layering as a key parameter for controlling melt flow in a natural migmatite during coaxial deformation. We performed in – situ pure-shear experiments on two natural gneisses. The first gneiss is weakly foliated with minerals homogenously distributed. The second gneiss shows a pronounced compositional layering of alternating quartz – feldspar – rich and biotite – muscovite – rich layers. Experimental conditions were selected to obtain homogeneous melt distribution in the homogeneous gneiss and heterogeneous melt distribution in the layered gneiss. Initial melt distribution is not modified by deformation in experiments on the homogeneous gneiss, implying that melting products did not migrate from their initiation sites. In contrast, melt flowed in shear zones or in inter-boudin positions during experimental deformation of the heterogeneous gneiss. These experiments attest to the strong influence of initial gneissic layering on melting pattern, melt segregation and flow during deformation of partially molten rocks.  相似文献   

全球冥古宙的研究进展和存在问题   总被引：1，自引：0，他引：1  

沈其韩  耿元生  宋会侠 《地质学报》2016,90(9):2083-2099

冥古宙是地球上最老的一个地质历史时期,由于缺少可靠的岩石记录一直没有得到国际地学界的重视和承认,到2004年才在建议的国际地层表中使用了冥古宙这一术语,定义从地球形成到出现地球最老岩石这段地球历史。但冥古宙与太古宙没有明确的地质界线,一些研究者提出了不同的年代界线(3.85Ga,4.0Ga,4.03Ga),目前还存在较大分歧。目前已知残存的冥古宙岩石只有两处,一处是加拿大的阿卡斯塔片麻岩(Acasta gneiss)中两个英云闪长岩和一个变质花岗闪长岩。前者锆石U-Pb年龄为4002±4Ma和4012±6Ma,后者为4031±1Ma。另一处是东南极索尼山(Mount Sones)的麻粒岩相英云闪长质片麻岩,已获得U-Pb年龄为3927±10Ma。世界上最老的表壳岩(≥3870Ma)出露在格陵兰。冥古宙年代久远,地球形成最初的600~700Ma的初始岩石经历了陨石撞击、地壳再循环、重熔等改造,甚至再循环到地幔,几乎已经消失殆尽。目前主要以年轻岩石中的碎屑锆石或继承锆石作为桥梁,来追索这些古老锆石原来母岩的类型、特征及成因。3800Ma的碎屑锆石已在全球十多个地区发现,而以西澳伊尔岗克拉通的杰克山最多最全,从3800Ma到4404Ma都有,在3840Ma,3900~3920Ma,4000~4200Ma,4260~4300Ma和4404Ma显示峰值,其中以3900~4200Ma最为发育,4404Ma是目前世界公认的最老碎屑锆石。此外在北美克拉通、南非克拉通、华北克拉通等古老克拉通以及一些年轻造山带中都发现有冥古宙的碎屑锆石,这些锆石是追索冥古宙地质事件的重要桥梁。通过对冥古宙碎屑锆石的研究提出了很多值得重视和进一步研究的课题和内容。包括早期地壳的性质,一些锆石具有与太古宙之后岩浆锆石特征相似的环带结构,因此这些碎屑锆石的母岩大部分被认为相当花岗质,来自老地壳的重熔。冥古宙碎屑锆石的Hf同位素等综合分析表明这些碎屑锆石来源于中性熔岩的结晶,或许表明早期地壳具有中性成分特征。冥古宙锆石的成因也是一个重要的课题,根据锆石中钛的含量、锆石Ti饱和温度计计算的温度以及锆石的一些结构特征,有的研究者提出冥古宙相当一部分碎屑锆石是陨石撞击导致的岩石熔融结晶产生的,是追溯地球早期撞击事件的重要手段。在4300Ma的碎屑锆石中包裹有金刚石和石墨晶体,前者表明锆石的母岩曾处于高压条件,而后者石墨的碳同位素接近有机碳,有人认为可能为生命起源的迹象。多个地区的碎屑锆石的边部Th/U比值低,U-Pb年龄为4000Ma左右,属于变质作用的产物,表明当时地壳已具有一定厚度。冥古宙碎屑锆石的研究提出了很多重要的问题,但是由于资料有限,有些认识还存在矛盾,还需要获得更多实际资料,才能对冥古宙的地质事件过程取得更可靠的科学认识。因此今后应加强可能赋存古老碎屑锆石地区的寻找,并发现更多古老碎屑锆石。对现有的古老碎屑锆石加强综合研究以及各地区的对比研究。  相似文献   

青藏高原片麻岩穹窿与找矿前景   总被引：4，自引：0，他引：4  

许志琴  付小方  马绪宣  戚学祥  吴婵  侯立伟  赵中宝 《地质学报》2016,90(11):2971-2981

片麻岩穹窿是研究俯冲-折返和碰撞-折返造山过程的重要窗口。已查明的大量青藏高原片麻岩穹窿(群)分布在古特提斯和新特提斯大洋俯冲-折返以及地体碰撞-折返过程中。松潘-甘孜造山带中雅江甲基卡片(麻)岩穹窿的三叠纪变质片岩的含矿伟晶岩脉中发现了超大型锂矿床,揭示片(麻)岩穹窿构造与同构造花岗岩、含矿伟晶岩脉以及大型印支滑脱带在时空和成因上有天然联系,为片麻岩穹窿的找矿前景提供了范例。  相似文献   

北京平原区地质剖面的初步建立——太古宙结晶基底和元古宙地层          下载免费PDF全文

吕金波  郑桂森  李良景  王海波  刘凯  王纯君 《中国地质》2016,(3):879-889

北京平原目前尚未建立系统的地质剖面。1867年庞培莱将北京西山分为3大系,1871年李希霍芬提出震旦系、划分12层。1922年葛利普将震旦系限定在前寒武系,1923年田奇镌将南口剖面划分为7个岩组,1934年高振西将震旦系3分(南口群、蓟县群、青白口群)。1976年乔秀夫3分青白口群(下马岭组、龙山组和景儿峪组),1980年汪长庆等将十三陵剖面分为4系12组,1991版《北京市区域地质志》将十三陵剖面分为3系12组。本文初步建立平原区地层表,详细描述太古宙结晶基底和元古宙地层剖面,在京南大兴区的榆垡(兴热-1井)和安定(兴热-2井)发现太古宙片麻岩,在京热-70井、京热-59井、京热-71井和京热-75井编录蓟县纪地层,利用亦庄小学钻孔厘定待建系下马岭组、青白口纪龙山组和景儿峪组。  相似文献   

广西大瑶山东南缘侏罗纪埃达克质花岗岩的特征、成因及构造意义     

许华  韩淑朋  钟锋运  黄启明  白晓  陈子龙 《岩石矿物学杂志》2021,40(6):1074-1092

对钦杭结合带西南段大瑶山东南缘的中晚侏罗世埃达克质花岗岩（165~153 Ma）进行了岩石学、地球化学研究,并探讨了埃达克质和TTG岩类的特征属性。岩石SiO₂含量63.76%~72.13%,总体具高Al₂O₃（Al₂O₃≥15%）、低MgO （<3%）,亏损重稀土元素（HREE）、正Eu异常或弱的负Eu异常,低Y （≤18×10^-6）和Yb （≤1.9×10^-6）,高Sr （>300×10^-6）和Sr/Y值（>20）等埃达克岩独特的地球化学特征。结合区域构造演化分析认为,该侏罗纪埃达克质花岗岩形成于陆内伸展构造背景,为大陆板内加厚（隆起区）的下地壳底部岩石部分熔融的产物,属大陆板内环境I型花岗岩。具有类似于低镁安山岩/闪长岩系列（LMA）和镁安山岩/闪长岩系列（MA）两种高压型TTG亚类的属性,为古俯冲增生带下地壳弧型岩石熔融的继承性特征,与中生代古太平洋俯冲板片熔融过程无关,属非俯冲成因的埃达克/TTG岩类。其空间上与大瑶山东南缘早古生代俯冲增生带高度重合,且与早古生代TTG侵入岩组合紧密相邻,提示它们可能源自于早古生代洋壳俯冲带或大陆边缘弧下地壳玄武质岩石的部分熔融,因而具有洋俯冲成因的特征属性。  相似文献