峨眉山大火成岩省太和花岗岩的成因及构造意义   总被引：5，自引：0，他引：5  

钟宏  徐桂文  朱维光  胡瑞忠  何德锋 《矿物岩石地球化学通报》2009,28(2):99-110

攀西地区的太和花岗质岩体和赋存超大型钒钛磁铁矿矿床的辉长岩体在空间上共生,成因上均与峨眉山地幔柱头的上升密切相关.太和花岗质岩体主要由超碱质花岗岩和石英正长岩及少量正长岩组成;富含高场强元素并具高Ga/Al值(3.74～5.63),显示典型A型花岗岩的特征.花岗岩、正长岩和辉长岩的Nb/Ta和Zr/Hf值与洋岛玄武岩(OIB)的相应比值近似.花岗质岩石具较低的87Sr/86Sr初始值(0.7025～0.7049)和正的εNd(t)值(1.9～3.5),与辉长岩的值相近[(87Sr/86Sr)i =0.7049～0.7052; εNd(t) =2.4～3.3].太和花岗质岩体的εNd(t)为正值,显示地幔柱来源的底侵玄武质岩浆对其形成起主要作用.辉长质和花岗质岩石具相似的钕同位素组成,表明其母岩浆来自于同一源区.我们认为太和花岗质侵入体主要由底侵于下地壳的玄武质岩浆分异出的花岗质熔体侵位及随后经结晶分异而形成.因此,晚古生代时幔源岩浆底侵造成的地壳增生在峨眉山大火成岩省中表现极为显著.  相似文献   

北京白查A型花岗岩的地球化学特征及其成因与构造指示意义   总被引：17，自引：6，他引：11  

汪洋 《岩石学报》2009,25(1):13-24

位于北京昌平区的年龄为127Ma的白查岩体是一个晶洞过碱性花岗岩岩株,其侵位于燕山造山带西段的八达岭岩基中。白查岩体具有高硅、Zr、Ga、Pb、HFSE和REE含量,高Fe/Mg和Ga/Al比值,强烈亏损Ca、Sr、Eu,具有亏损放射性成因Pb同位素的特征。白查岩体属于Dall’Agnol和Oliveira (2007)定义的典型的还原型A型花岗岩,其地球化学特征与燕山带中生代晚期的后石湖山(山海关)和窟窿山A型花岗岩非常相似。白查花岗岩起源于华北克拉通下地壳镁铁质源岩在相对贫水、高温、低氧逸度条件下的低程度部分熔融。综合区域地质背景和该岩体的成岩机制判断,白查花岗岩的形成标志燕山西段造山崩塌阶段的到来。除浙江东南瑶坑过碱性花岗岩外,白查岩体是具有A1型花岗岩元素地球化学特征但并非形成于非造山大地构造背景的过碱性花岗岩的又一个实例。  相似文献   

越南西北部Posen花岗岩锆石U-Pb年龄和Hf同位素组成特征   总被引：2，自引：2，他引：0  

HIEU PhamTrung  陈福坤  祝禧艳  王伟  NGUYEN ThiBichThuy  BUI MinhTam  NGUYEN QuangLuat 《岩石学报》2009,25(12):3141-3152

本文报道出露于越南西北部的Posen花岗岩岩体锆石U-Pb年龄和Hf同位素组成特征,讨论岩石成因和该地区新元古代岩浆作用的大地构造意义.分析3个花岗岩样品获得723Ma至760Ma的锆石U-Pb年龄,表明花岗岩形成于新元古代.该花岗岩的锆石Hf同位素组成有较大的变化范围,ε_(Hf)(t)值变化范围为-16.1至+3.4,单阶段Hf模式年龄为1186～1945Ma,暗示Posen花岗岩有着复杂的源区物源组成.在误差范围内,锆石两阶段Hf同位素模式年龄值主要集中在2.0～2.1Ga,与两阶段Nd同位素模式年龄值2.1～2.2Ga一致,说明花岗岩体主要由古元古代地壳物质部分熔融形成的.部分锆石颗粒具有正ε_(Hf)(t)值,可能指示花岗岩岩浆形成过程中存在壳-幔混合相互作用.在越南西北部发育新元古代岩浆作用可能与扬子板块广泛发育的、伴随Rodinia超大陆裂解过程的岩浆活动存在成因的联系,也揭示越南西北部地体可能与扬子板块具有亲缘关系,因此,可以推断马江断裂带应该代表印支板块和华南板块之间的古特提斯缝合带在越南西北部的延伸.  相似文献   

河南东沟钼矿花岗斑岩成因: 岩石地球化学、锆石U-Pb年代学及Sr-Nd-Hf同位素制约   总被引：16，自引：8，他引：8  

戴宝章  蒋少涌  王孝磊 《岩石学报》2009,25(11):2889-2901

本研究对东沟超大型钼矿床的成矿母岩-东沟花岗斑岩开展了系统的年代学、岩石地球化学及Sr-Nd-Hf同位素分析工作.LA-ICP-MS锆石U-Pb定年结果表明,东沟花岗斑岩成岩年龄为114～117Ma,与已有的成矿年龄(116±2Ma,Re-Os法)一致,证实了东沟钼矿为一斑岩型矿床.详细的岩石地球化学分析显示东沟花岗斑岩岩体与区域上太山庙大型花岗岩基为同源演化关系,它们均为弱过铝质,具有富Si、富K、富Rb、Th、U等大离子亲石元素、富Nb、Ta、Zr、Hf等高场强元素,贫Fe、Mg、Ca,贫Sr、Ba,Ga/Al比值较高等地球化学特征,属铝质A型花岗岩,形成于伸展构造体制,东沟岩体是母岩浆经历了强烈结晶分异高度演化的产物;东沟岩体Nd同位素组成为0.51166～0.51182,ε_(Nd)(t))值在-17.3～-14.3之间,锆石的ε_(Hf)(t)值变化较大,由-3.4至-18.7,另有一颗年龄为1715Ma的捕获锆石的ε_(Hf)(t)值为-2.4,Nd、Hf模式年龄分别为1.5～1.8Ga与1.3～1.7Ga.我们认为东沟岩体的岩浆源区以古老地壳物质为主,但也有少量幔源组分参入,并且幔源物质的加入及很高的岩浆演化程度可能对东沟钼矿的成岩成矿过程具有重要作用.  相似文献   

龙王(石童)A型花岗岩地球化学特征及其地球动力学意义   总被引：11，自引：0，他引：11  

包志伟  王强  资锋  唐功建  杜凤军  白国典 《地球化学》2009,38(6)

龙王花岗岩岩体产于华北克拉通南缘,岩石类型主要为黑云母钾长花岗岩,局部见有霓辉石花岗岩。岩体高硅(SiO2=72.17%～76.82%)、富碱(K2O+Na2O=8.28%～10.22%,K2O/Na2O>1),碱性指数AI(agpaitic index)=0.84～0.95,分异指数DI=95～97,铝指数ASI(aluminium saturation index)=0.96～1.13。含铁指数高(FeO/(FeO+Mg)=0.90～0.99),岩石为准铝质至弱过铝质、碱性—碱钙性、铁质A型花岗岩。岩石富集大离子亲石元素,稀土元素含量很高(854～1572μg/g);高场强元素(Nb、Ta、Zr、Hf)的富集程度明显低于大离子亲石元素,因此在微量元素蛛网图上呈相对亏损特征;岩石显著亏损Ba、Sr、Ti、Pb;εNd(t)=-4.5～-7.2,Nd模式年龄为2.3～2.5Ga。εHf(t)=-1.11～-5.26,模式年龄tHf1=2.1～2.3Ga,tHf2=2.4～2.6Ga。黑云母钾长花岗岩中的锆石主要为无色透明柱状晶体,CL图像多数显示清晰的岩浆成因的韵律环带结构,锆石LA-ICPMSU-Pb年龄为...  相似文献   

东准噶尔贝勒库都克铝质A 型花岗岩 地球化学特征及锡矿化     

杨高学 《地质与勘探》2009,45(5):530-538

本文通过对新疆东准噶尔卡拉麦里地区贝勒库都克岩体的地球化学研究,初步探讨贝勒库都克A型花岗岩与锡矿的关系。研究表明贝勒库都克黑云母花岗岩具有高硅、低铝、贫钙镁、富碱的特征,FeOt/MgO值高,富集Rb、K、Th等大离子亲石元素及Zr、Hf等高场强元素,亏损Ba、Sr、Nb、Eu等元素,Eu的负异常极强,稀土元素配分模式呈平坦的V字型,属于典型的铝质A型花岗岩。该岩体含Sn普遍都比较高,已圈出8条含锡构造蚀变带,为锡的成矿物质来源和锡矿矿床学的深入探索提供了有利的证据。  相似文献   

Characterisation of the Dabla Granitoids, North Khetri Copper Belt, Rajasthan, India: Evidence of Bimodal Anorogenic Felsic Magmatism   总被引：1，自引：0，他引：1  

Naveen Chaudhri  Parampreet Kaur  Martin Okrusch  Annette Schimrosczyk 《Gondwana Research》2003,6(4):879-895

The Palaeoproterozoic Dabla granitoid pluton of the North Khetri Copper Belt is located to the east of a NNE-SSW trending lineament with numerous albite-rich intrusives, the intraplate ‘albitite line’. The Dabla pluton is essentially made up of calcic amphibole-bearing granitoids, displaying a concentric bimodal distribution of alkali-feldspar granites, comprising a microcline-albite granite and an albite-granite. The dominant rock type is pink-coloured granite, which is characterised by quartz, microcline, albite and hastingsitic hornblende, and occurs in the marginal parts of the pluton. The volumetrically subordinate albite-granite in the central part of the pluton is invariably white in colour, non-foliated and is mainly composed of quartz, albite and amphibole of actinolite to ferro-actinolite composition. The albite-granite is characterised by low K₂O (0.06-0.09%), Rb (<5 ppm) and Ba (<20 ppm), high Na₂O (7.19-7.36%) and high Na/K ratios (122.4-185.2) as compared to the granite. These rocks are not subjected to any metamorphic overprint, especially the albite-granite, which shows pristine abundances of major and trace elements. The rocks are highly evolved as reflected in their high SiO₂ (72 to 78%) contents and high DI (89.5-97) values. The Dabla granitoids are characterised by similar REE and spider patterns, displaying LREE enriched slopes, flat HREE profiles and strong negative Sr, P, Ti and Eu anomalies suggesting their comagmatic nature. Nevertheless, the granite is relatively more fractionated [(La/Yb)_N = 3.89-8.19] and show higher REE abundances (466-673 ppm) as compared to the albite-granite [(La/Yb)_N = 1.97-2.96; REE = 220-277 ppm]. Distinctive features of these rocks are their low Ca (0.21-1.53%), Mg (<0.02-0.19%), Al (11.84-12.96%) and Sr (12-46 ppm) abundances, high Zr (155-631 ppm), Y (67-156 ppm), Nb (14-91 ppm), and Ga (20-31 ppm) concentrations and high Fe*-number, high Ga/Al ratio and high agpaitic index (AI) values. These features, coupled with their ferroan, alkaline and metaluminous nature, are typical of within-plate aluminous A-type granites. The geochemical data further indicate that the Dabla magma was generated at fairly high temperature, apparently in an upper mantle region, under relatively low H₂O activities and reduced conditions and emplaced at a shallow depth in an extensional tectonic environment.  相似文献   

西秦岭中川花岗岩岩浆活动特征及地质效应   总被引：5，自引：1，他引：5       下载免费PDF全文

卢哲  权君娟  程彧  闫德飞 《甘肃地质》2003,12(2):25-30

西秦岭中川花岗岩为3期5次侵入的复式岩体,其主侵入体为印支—燕山期黑云母同碰撞S型二长花岗岩。该岩浆活动在沉积建造中形成热变质作用带和岩浆侵位构造,并产生成矿地质效应。  相似文献   

Sedimentational,structural and migmatitic history of the Archaean Dharwar tectonic province,southern India     

K. Naha  R. Srinivasan  S. Jayaram 《Journal of Earth System Science》1991,100(4):413-433

The earliest decipherable record of the Dharwar tectonic province is left in the 3.3 Ga old gneissic pebbles in some conglomerates of the Dharwar Group, in addition to the 3.3–3.4 Ga old gneisses in some areas. A sialic crust as the basement for Dharwar sedimentation is also indicated by the presence of quartz schists and quartzites throughout the Dharwar succession. Clean quartzites and orthoquartzite-carbonate association in the lower part of the Dharwar sequence point to relatively stable platform and shelf conditions. This is succeeded by sedimentation in a rapidly subsiding trough as indicated by the turbidite-volcanic rock association. Although conglomerates in some places point to an erosional surface at the contact between the gneisses and the Dharwar supracrustal rocks, extensive remobilization of the basement during the deformation of the cover rocks has largely blurred this interface. This has also resulted in accordant style and sequence of structures in the basement and cover rocks in a major part of the Dharwar tectonic province. Isoclinal folds with attendant axial planar schistosity, coaxial open folds, followed in turn by non-coaxial upright folds on axial planes striking nearly N-S, are decipherable both in the “basement” gneisses and the schistose cover rocks. The imprint of this sequence of superposed deformation is registered in some of the charnockitic terranes also, particularly in the Biligirirangan Hills, Shivasamudram and Arakalgud areas. The Closepet Granite, with alignment of feldspar megacrysts parallel to the axial planes of the latest folds in the adjacent schistose rocks, together with discrete veins of Closepet Granite affinity emplaced parallel to the axial planes of late folds in the Peninsular Gneiss enclaves, suggest that this granite is late-tectonic with reference to the last deformation in the Dharwar tectonic province. Enclaves of tonalite and migmatized amphibolite a few metres across, with a fabric athwart to and overprinted by the earliest structures traceable in the supracrustal rocks as well as in a major part of the Peninsular Gneiss, point to at least one deformation, an episode of migmatization and one metamorphic event preceding the first folding in the Dharwar sequence. This record of pre-Dharwar deformation and metamorphism is corroborated also by the pebbles of gneisses and schists in the conglomerates of the Dharwar Group. Volcanic rocks within the Dharwar succession as well as some of the components of the Peninsular Gneiss give ages of about 3.0 Ga. A still younger age of about 2.6 Ga is recorded in some volcanic rocks of the Dharwar sequence, a part of the Peninsular Gneiss, Closepet Granite and some charnockites. These, together with the 3.3 Ga old gneisses and 3.4 Ga old ages of zircons in some charnockites, furnish evidence for three major thermal events during the 700 million year history of the Archaean Dharwar tectonic province.  相似文献   

Flexural and gravity modelling of the Mérida Andes and Barinas–Apure Basin, Western Venezuela     

Luis Chacín  María I. Jcome  Carlos Izarra 《Tectonophysics》2005,405(1-4):155-167

The kinematic evolution of the Barinas–Apure Basin and the southern Mérida Andes from Lower Miocene to the Present is numerically modelled using flexural isostatic theory and geophysical and geological data. Two published regional transects are used to build up a reference section, which is then used to constrain important parameters (e.g. shortenings and sedimentary thicknesses) for the flexural modelling. To control the location of the main fault system in the flexural model earthquake information is also used. The estimated flexural elastic thickness of the South American lithosphere beneath the Barinas–Apure Basin and the Mérida Andes Range is 25 km. The value for the final total shortening is 60 km. The flexural isostatic model shows that the Andean uplift has caused the South American lithosphere subsidence and the development of the Barinas–Apure Basin.In addition, gravity modelling was used to understand deep crustal features that could not be predicted by flexural theory. Consequently, the best-fit flexural model is used to build a gravity model across the Mérida Andes and the Barinas–Apure Basin preserving the best-controlled structural features from the flexural modelling (e.g. basin wavelength and depth) and slightly changing the main bodies density values and deep crustal structures. The final gravity model is intended to be representative of the major features affecting the gravity field in the study area. The predicted morphology in the lower crustal level of the final gravity model favours the hypothesis of a present delamination or megathrust of the Maracaibo crust over the South American Shield. This process would use the Conrad discontinuity as a main detachment surface within an incipient NW dipping continental subduction.  相似文献