喜马拉雅中段高压麻粒岩变质作用、地球化学与年代学   总被引：2，自引：7，他引：2  

季建清  钟大赉宋彪朱美妃  温大任 《岩石学报》2004,20(5):1283-1300

研究的高压麻粒岩发现于西藏亚东以北约40公里的(Zherger-La)、出露在藏南拆离系(STDS)主构造面下盘的高喜马拉雅结晶岩系中,是继喜马拉雅东西构造结的Nanga Barbat、Namjag Barwa和喜马拉雅中段Khatra & Marina地区、定结地区发现的榴辉岩或高压麻粒岩之后,在青藏高原上新近发现的高压麻粒岩.该麻粒岩呈岩片被包裹于花岗质片麻岩中.麻粒岩记录了两期变质作用,早期矿物组合为Grt+Cpx+Pl+Qz,属麻粒岩相变质产物,矿物成分分析显示早期矿物组合达到了平衡,并且没有表现成分扩散;后期矿物组合为Hbl+Pl+Bio或Opx+Pl,指示了较高温但相对压力较低的麻粒岩相退变变质作用,矿物成分分析和结构显示了退变作用没有达到变质平衡.显微结构可以观察到多组变质反应Grt+Cpx+Qtz=Opx+Pl,Grt+Qtz=Opx+Pl,Grt+Cpx+L=Hbl+Pl+Bio+Mt,和Cpx+L=Hbl+Mt.根据矿物平衡关系,利用Grt-Cpx温度计和Grt-Cpx-Pl-Qz压力计估算的早期变质作用温压为T=780～850℃,P=12～15kbar,相对应的地温梯度16℃～18℃/km.借用Hbl-Pl温度计和A1tot in Hbl压力计估算的晚期变质作用温压为T=730～760℃;P=4～6kbar,相当的地温梯度为38℃～50℃/km.变质作用P-T演化呈等温降压轨迹,指示麻粒岩地体从增厚(或俯冲)地壳到减薄增温(或部分熔融)地壳,进而被快速剥露地表的构造过程.初步的地球化学结果表明高压麻粒岩原岩可能相当于大陆拉斑玄武岩.麻粒岩锆石SHRIMP年代学有两组相对集中的年龄分别为98±5 Ma(5 spots)和17.0±0.3 Ma(13 spots).高压麻粒岩的两期变质作用的温度都在700℃以上,略高于锆石U-Pb同位素体系计时封闭温度,推断17 Ma是高压麻粒岩变质后发生折返,随高喜马拉雅结晶岩系剥露冷却的年龄;98.4Ma的测年结果被推测是高压麻粒岩原岩形成的年龄.在喜马拉雅山,高压麻粒岩记录了类似增厚地壳到减薄地壳的转变一方面可能是地壳深部作用机制的转变,另一方面,这种机制与喜马拉雅南坡巨大的降雨量和去顶作用有密切关系,意义重大.  相似文献   

安徽铜陵新桥铜-硫-铁-金矿床中石英闪长岩和辉绿岩锆石SHRIMP年代学及其意义   总被引：48，自引：3，他引：48       下载免费PDF全文

王彦斌刘敦一  蒙义峰曾普胜杨竹森  田世洪 《中国地质》2004,31(2):169-173

对安徽铜陵新桥铜-硫-铁-金矿床区内的石英闪长岩和辉绿岩中的锆石分别进行了SHRIMP精确定年研究,石英闪长岩中锆石206Pb/238U年龄为(140.4±2.2)Ma,辉绿岩中锆石的年龄较复杂,其中发现了元古代锆石颗粒,其锆石207Pb/206Pb年龄为(2261±14)Ma,(1612±8)Ma,(919±12)Ma,(831±17)Ma。另外还有一组早古生代年龄的锆石,锆石206Pb/238U年龄为(443±13)Ma。以上这些新资料说明该区可能存在元古代基底的信息,且燕山期岩浆活动对本区成矿具有重要意义。  相似文献   

湖北新春花岗岩类锆石SHRIMP年龄:大别山造山带内弱变质—未变质晋宁期花岗岩类的发现     

薛怀民  刘敦一  董树文  简平  刘晓春 《地质学报》2004,78(1)

蕲春花岗质杂岩体包括斑状二长花岗岩和花岗岩两部分,它们之间在化学性质上存在着很大的差异,前者表现为高Al_2O_3(15.73％)、相对高CaO(2.46％)、Na_2O含量明显高于K_2O(Na_2O/K_2O=1.27),尤以强烈亏损重稀土元素和极强的轻、重稀土元素分馏程度[(La/Yb)_N=46.8]为特征而类似于太古宙高Al_2O_3的TTG岩石。而后者则以较低的Al_2O_3含量(14.05％)、贫CaO(0.82％)、K_2O含量明显高于Na_2O(Na_2O/K_2O=0.81)为特征,轻、重稀土元素的分馏程度[(La/Yb)_N=10.89]也较片麻状二长花岗岩中弱得多。两类岩石中锆石的U-PbSHRIMP年龄分别为824.6±17.6 Ma和784±20 Ma,该时代与大别山造山带内花岗片麻岩的原岩形成年龄类似。大别山造山带内弱变质-未变质晋宁期花岗岩的出现表明扬子板块印支期向北俯冲时,该花岗质杂岩处于俯冲板片的后缘,可代表造山带内扬子基底的原地露头。而岩体周围的高压变质杂岩应是折返上来的无根构造岩片,大别山造山带内高压-超高压变质杂岩的出露不是整体性抬升剥蚀的结果。  相似文献   

Tracing the protolith, UHP metamorphism, and exhumation ages of orthogneiss from the SW Sulu terrane (eastern China): SHRIMP U–Pb dating of mineral inclusion-bearing zircons     

Fulai Liu  Zhiqin Xu  Huaimin Xue 《Lithos》2004,78(4):411-429

Orthogneisses are the major country rocks hosting eclogites in the Sulu UHP terrane, eastern China. All of the analyzed orthogneiss cores from the main drilling hole of the Chinese Continental Scientific Drilling Project (CCSD-MH) have similar major and trace element compositions and a granite protolith. These rocks have relatively high LREE/HREE ratios, strong negative Eu anomalies (Eu/Eu*=0.20–0.39), and negative Ba anomalies (Ba/Ba*=0.25–0.64). Coesite and coesite-bearing UHP mineral assemblages are common inclusions in zircons separated from orthogneiss, paragneiss, amphibolite, and (retrograded) eclogite of the CCSD-MH. This suggests that the eclogite, together with its country rocks, experienced in situ ultrahigh-pressure (UHP) metamorphism. Laser Raman spectroscopy and cathodoluminescence (CL) images show that zircons from the orthogneisses are zoned and that they have distinct mineral inclusions in the different zones. Most zircons retain early magmatic cores with abundant low-pressure mineral inclusions, which are mantled with metamorphic zircon-containing inclusions of coesite and other UHP minerals. The outermost rims on these grains contain low-pressure mineral inclusions, such as quartz and albite. SHRIMP U–Pb dating of the zoned zircons gives three discrete and meaningful groups of ages: Proterozoic ages for the protolith, 227±2 Ma for the coesite-bearing mantles, and 209±3 Ma for the amphibolite facies retrograde rims. The widespread occurrence of UHP mineral inclusions in zircons from the Sulu metamorphic belt dated at about 227 Ma suggests that voluminous continental crust experienced late Triassic subduction to depths of at least 120 km and perhaps more than 200 km. Eighteen million years later, the terrane was rapidly exhumed to midcrustal levels, and the UHP rocks were overprinted by amphibolite facies metamorphism. The exhumation rate deduced from the zircon age data and previously obtained metamorphic P–T data is estimated to be 5.6–11.0 km/Ma. Such rapid exhumation of the Sulu UHP terrane may be due to the buoyancy forces produced by subduction of low-density continental material into the deep mantle.  相似文献   

Timing of Magma Mixing in the Gangdisě Magmatic Belt during the India-Asia Collision： Zircon SHRIMP U-Pb Dating     

MO Xuanxue  DONG Guochen  ZHAO Zhidan  GUO Tieying  WANG Liangliang  CHEN Tao 《《地质学报》英文版》2005,79(1):66-76

Abstract  Abundant mafic microgranular enclaves (MMEs) extensively distribute in granitoids in the Gangdisê giant magmatic belt, within which the Qüxü batholith is the most typical MME‐bearing pluton. Systematic sampling for granodioritic host rock, mafic microgranular enclaves and gabbro nearby at two locations in the Qüxü batholith, and subsequent zircon SHRIMP II U‐Pb dating have been conducted. Two sets of isotopic ages for granodioritic host rock, mafic microgranular enclaves and gabbro are 50.4±1.3 Ma, 51.2±1.1 Ma, 47.0±1 Ma and 49.3±1.7 Ma, 48.9±1.1 Ma, 49.9±1.7 Ma, respectively. It thus rules out the possibilities of mafic microgranular enclaves being refractory residues after partial melting of magma source region, or being xenoliths of country rocks or later intrusions. Therefore, it is believed that the three types of rocks mentioned above likely formed in the same magmatic event, i.e., they formed by magma mixing in the Eocene (c. 50 Ma). Compositionally, granitoid host rocks incline towards acidic end member involved in magma mixing, gabbros are akin to basic end member and mafic microgranular enclaves are the incompletely mixed basic magma clots trapped in acidic magma. The isotopic dating also suggested that huge‐scale magma mixing in the Gangdisê belt took place 15–20 million years after the initiation of the India‐Asia continental collision, genetically related to the underplating of subduction‐collision‐induced basic magma at the base of the continental crust. Underplating and magma mixing were likely the main process of mass‐energy exchange between the mantle and the crust during the continental collision, and greatly contributed to the accretion of the continental crust, the evolution of the lithosphere and related mineralization beneath the portion of the Tibetan Plateau to the north of the collision zone.  相似文献   

Geochronologic Constraints on the Magmatic Underplating of the Gangdisê Belt in the India-Eurasia Collision: Evidence of SHRIMP II Zircon U-Pb Dating     

DONG Guochen  MO Xuanxue  ZHAO Zhidan  GUO Tieying  WANG Liangliang  CHEN Tao 《《地质学报》英文版》2005,(6)

  相似文献   

鞍山地区东鞍山花岗岩年代学、地球化学特征及成因研究   总被引：2，自引：1，他引：1  

朱凯  刘正宏  徐仲元  王兴安 《岩石学报》2016,32(2):590-604

鞍山地区位于华北地台东北部辽宁省,区内保留有3.8~2.5Ga连续的地质记录。对位于鞍山市南侧的东鞍山花岗岩进行了SHRIMP锆石U-Pb同位素分析、白云母Ar-Ar同位素分析及岩石地球化学分析。SHRIMP测年结果为3004±7Ma,代表岩石的形成年龄,Ar-Ar测年结果为2545±16Ma,代表岩石受到构造热事件扰动的时间。岩体地化特征为富硅(Si O2=72.95%~75.37%,平均值为74.18%)、富碱(K2O+Na2O=7.05%~8.45%)、富铝(Al2O3=12.95%~15.44%),低钙(Ca O=0.13%~0.66%)。在稀土元素配分图上,曲线呈明显的右倾趋势,且有较明显的负Eu异常,重稀土分馏不明显。在微量元素洋中脊玄武岩标准化蛛网图上可以看出,东鞍山花岗岩强烈亏损Nb、P、Sr、Ti,富集大离子亲石元素Rb、K、Nd和高场强元素Th、U。岩石地球化学特征表明东鞍山花岗岩岩浆来源为壳源,残留相可能由石榴石+辉石+角闪石+斜长石组成。将鞍山-本溪地区3个3.0Ga花岗岩(东鞍山花岗岩岩体、铁架山二长花岗岩岩体以及弓长岭片麻状花岗岩)的地球化学数据进行对比,发现三者的地球化学存在较大差异,为三个独立的岩体。三个岩体最初可能发育在一个陆块之上,然后在25.5亿年左右分离开来,最后在25亿年左右再次拼贴到一起。  相似文献   

华北克拉通大青山-集宁地区古元古代变质沉积岩的锆石氧同位素组成:SHRIMP微区原位分析   总被引：1，自引：0，他引：1  

董春艳  万渝生  龙涛  张玉海  刘建辉  马铭株  颉颃强  刘敦一 《岩石学报》2016,32(3):659-681

在已获得锆石U-Pb年龄基础上,我们首次对孔兹岩带典型出露区大青山和集宁土贵乌拉地区古元古代变质沉积岩进行了锆石SHRIMP氧同位素研究。锆石具有复杂的内部结构和年龄分布。大青山地区古元古代早期变质沉积岩4个样品碎屑锆石的δ18O为5.52‰~7.11‰,部分重结晶锆石的δ18O为7.22‰~7.90‰,变质新生锆石的δ18O为6.37‰~8.31‰。大青山地区古元古代晚期变质沉积岩2个样品的锆石O同位素组成特征与古元古代早期的类似,另外2个样品的锆石O同位素组成与之不同,碎屑锆石、部分重结晶锆石和变质新生锆石的δ18O分别为6.26‰~10.80‰、9.00‰~11.20‰和9.66‰~11.90‰。集宁土贵乌拉地区古元古代晚期超高温变质沉积岩4个样品不存在碎屑锆石,变质锆石的δ18O变化范围为11.41‰~13.57‰。主要认识如下:1)大青山地区碎屑沉积物主要来自新太古代晚期-古元古代早期成熟度不高的TTG花岗质岩石物源区,与之相比,集宁土贵乌拉地区古元古代晚期超高温岩石的变质原岩成熟度更高;2)不同类型变质沉积岩变质新生锆石的δ18O和变质新生锆石与碎屑锆石的Δ18O存在明显区别,主要反映了岩石体系和变质流体的O同位素组成不同;3)大青山地区高角闪岩相-麻粒岩相变质沉积岩,重结晶锆石的O同位素完全重置,但U-Th-Pb体系未完全重置,集宁土贵乌拉地区超高温变质沉积岩的重结晶锆石O和U-Th-Pb同位素体系都完全重置。变质作用强度不同是主要原因。  相似文献   

Zircon SHRIMP U-Pb dating of the Neogene coral reefs,Xisha Islands,South China Sea: implications for tectonic evolution     

《China Geology》2018,1(1):49-60

The Xisha Block is a minor one in the South China Sea and an important tectonic unit in the northwestern part of the region. Zircon SHRIMP U-Pb ages for three volcanic intrusive core samples from Xike-1, an exploratory well penetrating the bioherms of the Xisha Islands. The core samples are from the Miocene reef carbonate bedrock and are recognized as dark-gray biotite-hornblende gabbro, gray fine-grained biotite diorite, and gray fine-grained granite, respectively. Zircon cathodoluminescence (CL) images and trace Th, U and Pb compositions of the zircons show that these rocks are of volcanic intrusive origin. Zircon SHRIMP U-Pb dating yielded six groups of ages, ranging from 2451-1857 Ma to early Cretaceous, which indicate that the formation and evolution of the Xisha Block was affected by the evolution and closure of Neotethys Ocean, probably within its eastern extension into South China Sea. Both old, deep-sourced material, including fragments from Rodina supercontinent, and recent mantle-derived magma products contributed to the emergence and formation of the Xisha block. The SHRIMP U-Pb results also proved that this process differed from that of the Kontum massif, the Hainan Block, and the South China Block, but is similar to that of the Nansha and Zhongsha blocks. The process was associated with the effects of Yanshanian magmatism induced by subduction mechanisms of the Paleo-Pacific Plate or the reworking of the multiple magmatisms since the Early to mid-Yanshanian, possibly jointly experienced by the Xisha-Zhongsha-Nansha Block.  相似文献   

粤东鸿沟山金矿区流纹斑岩锆石SHRIMP U-Pb定年、Lu-Hf同位素组成及其地质意义     

范飞鹏  肖惠良  陈乐柱  李海立  蔡逸涛  康丛轩  朱意萍  刘建雄  邓中林  李少斌  林耿伟  周霞  肖凡 《地质论评》2018,64(1):213-226

鸿沟山矿区位于华南粤东莲花山钨矿床的中部,是近年来通过地质矿产调查新发现具有找寻金矿潜力的矿床之一。本文以与鸿沟山金等多金属矿化关系密切的流纹斑岩为研究对象,开展了锆石SHRIMP U-Pb定年、流纹斑岩和矿石岩石地球化学、锆石Lu-Hf同位素组成特征研究。获得流纹斑岩锆石206Pb/238U加权平均年龄为169.1±1.5Ma,说明岩体形成于中侏罗世。在微量元素特征方面,流纹斑岩都表现为相对亏损大离子亲石元素Ba、Sr和高强场元素Nb、P、Zr、Hf,富集大离子亲石元素Rb,高强场元素U、Ce、Sm和轻稀土元素La、Nd,流纹斑岩与矿石稀土元素特征基本相似,Eu具中等负异常,但随着矿化强度的增强稀土元素更加富集。流纹斑岩εHf(t)(-15.0~2.2)分布范围宽,二阶段模式年龄TDM2主要变化范围为0.82~0.93 Ga,表明成岩物质主要来源于新元古代古老地壳变质泥岩和变质砂岩部分熔融,并有幔源物质的加入。因此,围绕着该时间段的流纹斑岩岩体,对于找寻W、Cu、Pb、Zn、Bi、Au、稀土、稀有和稀散元素矿产具有重要意义。  相似文献