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681.
蔡玉曼  曹磊 《岩矿测试》2007,26(3):225-229232
通过对榴辉岩中金红石物相二氧化钛含量重复测定,建立数学模型,分析了测量过程的不确定度主要来源于样品制备的不确定度、标准物质引入的不确定度、曲线拟合中产生的不确定度.以及重复试验的不确定度。当二氧化钛平均含量为3.75%时,评定其扩展不确定度为0.16%。  相似文献   
682.
拉萨地块榴辉岩样品中的锆石SHRIMP U-Pb年龄值为(242.4±15.2)~(291.9±12.8)Ma,平均261.7Ma±5.3Ma。所有锆石均含有大量的包裹体,主要分布在锆石核部。最常见的矿物包裹体是石榴子石,其次为石英、磷灰石、金红石和绿辉石,可见角闪石、榍石、多硅白云母和钠长石。包裹体具3种组合:榴辉岩相(Grt Omp Rt Phe)、角闪岩相(Amp Spn Ab)和不确定相(Qtz Ap)。锆石中的矿物包裹体与岩石中对应矿物的成分相同。包裹体集中在锆石核部和榴辉岩相矿物的大量出现表明锆石生长发生于变质峰期或峰期之后不久。锆石的Th/U比值均很低,具变质成因锆石的典型特征。区域地质资料对比表明,榴辉岩的原岩可能形成于石炭纪—二叠纪早期,是古特提斯洋盆裂解的产物。  相似文献   
683.
The North China craton (NCC) is distinctively dif-ferent from other Archean craton around the world due to violent construction-magmatic activity, ore deposi-tion and basin formation process and the deep dynam-ics could be probably related with lithospher…  相似文献   
684.
低温榴辉岩中石榴子石的成分分带:快速抬升的证据   总被引:2,自引:4,他引:2  
对南大别黄镇冷榴辉岩中——颗石榴子石进行了详细的电子探针工作,对其特殊的成分分带,建立了扩散模型并进行数值模拟,结果得到4.5mm/a的快速抬升速率。该结果表明黄镇榴辉岩曾经历了一个快速的抬升过程。  相似文献   
685.
成岩成矿深度的构造校正测算方法,是从测算压力中先消除掉构造附加静水压力之后再计算上覆岩石厚度,即成岩成矿深度的方法。该方法基于对地壳岩石处于固体应力状态的认识之上,采用弹性固体模型代替静止流体模型,对“上覆岩石重力在数值上等同于该点所承受的静水压力”这一通常的认识提出了不同见解,比沿袭至今单纯用压力/比重(或密度)方法得出深度更符合于实际情况。本文介绍了该方法的理论基础和野外地质研究方法——开展变形岩相形迹填图,在室内利用三维变形和古差应力测量,根据样品所处构造部位和性质,选择不同的参数换算成矿时差应力的众值。以胶东玲珑——焦家式金矿床为例,求得成矿深度仅3.5km或更浅,进而提出更深部位存在深部金矿富集带的预测意见。胶东几个大型金矿深部第二富集带已揭露的勘探资料证实这一认识比较符合实际情况。用这一方法测算出大别超高压带含柯石英榴辉岩形成深度仅32km多,而不是用压力/比重方法估算的100多公里,这为大别造山带的构造格局和演化历史的研究提出新的途径和方法。  相似文献   
686.
苏北踢球山榴辉岩演化的同位素年代学证据   总被引:1,自引:0,他引:1  
采用Sm Nd同位素定年方法 ,测得江苏北部新沂地区踢球山三个榴辉岩岩体时代为 :2 2 1.6± 8.4Ma ,2 13.6± 9.2Ma和 2 16 .6± 8.1Ma;εNd(t)分别为 - 2 .9,- 2 .9和 - 3.0。采用Rb Sr定年方法得到其中一个榴辉岩的年龄为 2 0 1± 2 1Ma ;87Sr/ 86Sr =0 .70 5 35± 37。Sm Md年龄被看作为踢球山超高压变质之后板块折返过程中的高压榴辉岩相重结晶阶段年龄。Rb Sr年龄反映了踢球山榴辉岩体的板块折返过程中的角闪岩相退变质阶段开始年龄。为中朝板块与扬子板块碰撞时代主要发生在晚三叠世的观点提供了依据  相似文献   
687.
The eclogite gravels, which were found in the Mesozoic Fenghuangtai and Maotanchang formations on the northern margin of the Dabie orogenic belt, are rich in K2O(1.21%),∑REE (278μg/g) ,and LILE(such as Rb, Ba, K, Th, etc.) , with high (La/Yb)N ratios(14.4),on the basis of the analyses of major elements, rare-earth elements (REE) and trace elements. Their enrichment in LILE, notable Nb-Ta depletion through, and depletion in HFSE relative to REE in comparison with the primitive mantle and N-MORB indicate that the protoliths of the eclogite gravels were formed in an island-arc setting. According to the Th-Hf-Ta discrimination diagram, the protoliths of the eclogite gravels are characterized by volcanic arc basalts.Trace element data indicate that the subducted marine sediments were assimilated in the magma chamber, resulting in the enrichment of LILE in the protoliths. Therefore, the protoliths of the eclogite gravels are considered to have been formed in an inland-arc setting, indicating that there had developed a paleo-inland arc before Triassic collision between the North and South China blocks in the Dabie orogenic belt. There is a marked difference between the eclogite gravels and the eclogites developed along the Dabie orngenic belt, solely based on their geochemical data,especially REE. Therefore, the eclogite gravels may not be derived from eclogite terrains preserved in the Dabie orogenic belt.  相似文献   
688.
Abstract For the first time, we apply different geospeedometric models to garnet zoning patterns that were obtained in this study from detailed EMP analyses for garnets from eclogites and granulite in the Dabie‐Sulu orogen. Various zonings of cation diffusion were preserved in the garnets, enabling the acquirement of average cooling rates for the high‐to ultrahigh‐pressure rocks without using geochronological approaches. The coesite‐bearing hot eclogites yield fast cooling rates of about 20 to 30°C/Ma subsequent to peak metamorphic temperatures, whereas the cold eclogite gives a relatively slow cooling rate of 8°C/Ma at its initial exhumation. A very slow cooling rate of <0.3°C/Ma is obtained for the granulite at Huangtuling, suggesting that the granulite may not be involved in the continental deep subduction.  相似文献   
689.
In the Central Orogenic Belt, China, two UHP metamorphic belts are discriminated mainly based on a detailed structural analysis of the Kanfenggou UHP metamorphic fragment exposed in the eastern Qinling orogen, and together with previous regional structural, petrological and geochronological data at the scale of the orogenic domain. The first one corresponds to the South Altun-North QaidamNorth Qinling UHP metarnorphic belt. The other is the Dabie-Sulu UHP and HP metamorphic belts. The two UHP metamorphic belts are separated by a series of tectonic slices composed by the Qiniing rock group, Danfeng rock group and Liuling or Foziling rock group etc. respectively, and are different in age of the peak UHP metamorphism and geodynamic implications for continental deep subduction and collision. Regional field and petrological relationships suggest that the Kanfenggou UHP metamorphic fragment that contains a large volume of the coesite- and microdiamond-bearing eclogite lenses is compatible with the structures recognized in the South Altun and North Qaidam UHP metamorphic fragments exposed in the western part of China, thereby forming a large UHP metamorphic belt up to 1000 km long along the orogen strike. This UHP metamorphic belt represents an intercontinental deep subduction and collision belt between the Yangtze and Sino-Korean cratons, occurred during the Paleozoic. On the other hand, the well-constrained Dabie-Sulu UHP and HP metamorphic belts occurred mainly during Triassic time (250-220 Ma), and were produced by the intracontinental deep subduction and collision within the Yangtze craton. The Kanfenggou UHP metamorphic fragment does not appear to link with the DabieSulu UHP and HP metamorphic belts along the orogen. There is no reason to assume the two UHP metamorphic belts as a single giant deep subduction and collision zone in the Central Orogenic Belt situated between the Yangtze and Sino-Korean cratons. Therefore, any dynamic model for the orogen must ac-count for the development of UHP metarnorphic rocks belonging to the separate two tectonic belts of different age and tectono-metamorphic history.  相似文献   
690.
The central part of the Carolina terrane in western South Carolina comprises a 30 to 40 km wide zone of high grade gneisses that are distinct from greenschist facies metavolcanic rocks of the Carolina slate belt (to the SE) and amphibolite facies metavolcanic and metaplutonic rocks of the Charlotte belt (to the NW). This region, termed the Silverstreet domain, is characterized by penetratively deformed felsic gneisses, granitic gneisses, and amphibolites. Mineral assemblages and textures suggest that these rocks formed under high‐pressure metamorphic conditions, ranging from eclogite facies through high‐P granulite to upper amphibolite facies. Mafic rocks occur as amphibolite dykes, as metre‐scale blocks of coarse‐grained garnet‐clinopyroxene amphibolite in felsic gneiss, and as residual boulders in deeply weathered felsic gneiss. Inferred omphacite has been replaced by a vermicular symplectite of sodic plagioclase in diopside, consistent with decompression at moderate to high temperatures and a change from eclogite to granulite facies conditions. All samples have been partially or wholly retrograded to amphibolite assemblages. We infer the following P‐T‐t history: (1) eclogite facies P‐T conditions at ≥ 1.4 GPa, 650–730 °C (2) high‐P granulite facies P‐T conditions at 1.2–1.5 GPa, 700–800 °C (3) retrograde amphibolite facies P‐T conditions at 0.9–1.2 GPa and 720–660 °C. This metamorphic evolution must predate intrusion of the 415 Ma Newberry granite and must postdate formation of the Charlotte belt and Slate belt arcs (620 to 550 Ma). Comparison with other medium temperature eclogites and high pressure granulites suggests that these assemblages are most likely to form during collisional orogenesis. Eclogite and high‐P granulite facies metamorphism in the Silverstreet domain may coincide with a ≈570–535 Ma event documented in the western Charlotte belt or to a late Ordovician‐early Silurian event. The occurrence of these high‐P assemblages within the Carolina terrane implies that, prior to this event, the western Carolina terrane (Charlotte belt) and the eastern Carolina terrane (Carolina Slate belt) formed separate terranes. The collisional event represented by these high‐pressure assemblages implies amalgamation of these formerly separate terranes into a single composite terrane prior to its accretion to Laurentia.  相似文献   
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