湖北通城透锂长石伟晶岩中锂辉石的发现   总被引：1，自引：0，他引：1  

张玉玉  张如柏 《矿物岩石》2008,28(3)

湖北通城伟晶岩体是我国唯一的以透锂长石为主要锂矿物的锂伟晶岩,而在该伟晶岩中发现首次与透锂长石成因密切相关的锂辉石,该锂辉石呈灰白色一白色,强玻璃光泽,比重为3.12,硬度为6.5～7.0,有平行f轴的纵纹,正交偏光下为二轴晶,负光性.在常温下测得其3个光学主轴的参数为:N8=1.675,Np=1.667,Nm=1.669,N8-Np=0.008.2V=60°.锂辉石样品的化学成份w(B)为:Li2O 7.61%,Al2O3 27.72%,SiO263.30%,K20 0.03%.Na2O 0.19%,CaO 0.05%,MgO 0.11%,FeO 0.21%,MnO0.35%,H2O 0.30%,HzOˉ0.52%,总计100.39%.锂辉石样品的X射线数据为:2.791(100),2.917(52),4.250(61),6.109(51),2.863(16)和4.445(16)与标准锂辉石相吻合.  相似文献   

福建南平花岗伟晶岩中钾长石的矿物学研究     

杨岳清  王文瑛  林国新  朱锦煌  陈成湖 《福建地质》2003,22(1):1-12

钾长石是南平伟晶岩中分布广泛的一种造岩矿物，它的结晶作用几乎贯穿于伟晶岩形成－演化过程的所有阶段。通过对不同类型伟晶岩和同一类型伟晶岩中不同世代钾长石的产出条件、物理性质、矿物粉晶X光衍射、化学成分等方面研究，发现钾长石在伟晶岩中的分布有明显的规律性。这不仅深化了对南平伟晶岩形成机制的了解，而且对钾长石的综合利用也有重要意义。  相似文献   

岩浆-流体过渡和阿尔泰三号伟晶岩脉之成因   总被引：13，自引：0，他引：13  

卢焕章  王中刚  李院生 《矿物学报》1996,16(1):1-7,T002

本文对新疆阿尔泰可可托海的三号伟晶岩形成的物理化学条件、特别是流体-熔融包裹体进行了研究，证明岩浆的确可以分出热液，对于三号伟晶岩脉来说，这种热液组分主要是NaCl－CO2－H2O流体。  相似文献   

Mafic Pegmatites Intruding Oceanic Plateau Gabbros and Ultramafic Cumulates from Bolivar, Colombia: Evidence for a 'Wet' Mantle Plume?     

KERR  ANDREW C.; TARNEY  JOHN; KEMPTON  PAMELA D.; PRINGLE  MALCOLM; NIVIA  ALVARO 《Journal of Petrology》2004,45(9):1877-1906

The fault-bounded Bolívar Ultramafic Complex (BUC) onthe eastern fringes of the Western Cordillera of Colombia wastectonically accreted onto the western coast of South Americain the late Cretaceous–early Tertiary, along with pillowbasalts of the Caribbean–Colombian Oceanic Plateau (CCOP).The complex consists of a lower sequence of ultramafic cumulates,successively overlain by layered and isotropic gabbroic rocks.The gabbros grade into, and are intruded by, mafic pegmatitesthat consist of large magnesiohornblende and plagioclase crystals.These pegmatites yield a weighted mean ⁴⁰Ar–³⁹Ar step-heatingage of 90·5 ± 0·9 Ma and thus coincidewith the timing of peak CCOP volcanism. The chemistry of theBUC is not consistent with a subduction-related origin. However,the similarity in Sr–Nd–Pb–Hf isotopes betweenthe CCOP and the BUC, in conjunction with their indistinguishableages, suggests that the BUC is an integral part of the plume-derivedCCOP. The parental magmas of the Bolívar complex wereprobably hydrous picrites that underwent 20–30% crystallization.The residual magmas from this fractionation contained  相似文献   

K-Ar Ages of Granitic Magmatism and Related Pegmatite Formation at the Umanotani-Shiroyama Mine, Shimane Prefecture, SW Japan and Their Bearings on Cooling History     

Shouji Kihara    Kenichi Hoshino    Makoto Watanabe    Hirotsugu Nishido  Shunso Ishihara 《Resource Geology》2005,55(2):123-129

Abstract. The Umanotani-Shiroyama pegmatite deposits, the largest producer of K-feldspar and quartz in Japan, are of typical granitic pegmatite. Ilmenite-series biotite granite and granite porphyry, hosting the ore deposits, and biotites separated from these rocks yielded K-Ar ages ranging from 89.0 to 81.4 Ma and 95.2 to 93.7 Ma, respectively. Muscovite and K-feldspar separated from the ore zone yielded K-Ar ages with the range of 96.2 to 93.1 Ma and 87.3 to 80.7 Ma, respectively. Muscovites from quartz-muscovite veins in the ore zone and in the granite porphyry yielded K-Ar ages of 90.4 and 76.3 Ma, respectively. K-feldspar is much younger in age than coexisting muscovite. It is noted that the K-Ar ages of biotite separates and the whole-rock ages are identical to those of muscovite and K-feldspar in the ore zone, respectively. These time relations, as well as field occurrence, indicate that the formation of the pegmatite deposits at the Umanotani-Shiroyama mine is closely related in space and time to a series of granitic magmatism of ilmenite-series nature. Using closure temperatures of the K-Ar system for biotite and K-feldspar (microcline), cooling rate of the pegmatite deposits is estimated to be about 82C/m.y. at the beginning, but slowed down to about 15C/m.y. in the later period.  相似文献   

利用LA-ICP-MS在16 μm和10 μm激光束斑条件下测定独居石U-Th-Pb年龄     

汪双双  韩延兵  李艳广  魏小燕  靳梦琪  程秀花 《岩矿测试》2016,35(4):349-357

我国锂钾主要矿产资源大多分布在西部偏远地区,其勘查找矿或综合利用迫切需要现场快速分析技术的支持。本文介绍了自行开发的便携式Li-K分析仪的主要性能及其在锂辉石中锂的分析应用。Li-K分析仪是一种基于大气压的液体阴极辉光放电光谱仪,以待测液体为放电阴极,实现样品中Li、K等元素的原子化和激发。该仪器以光纤传导CCD光谱仪作为检测器,其波长范围为345～1015 nm,分辨率3 nm;以Li 670.78 nm和K 769.90 nm分析谱线,在最佳仪器工作条件下测定Li、K的精密度（RSD,n=14）均低于2%,检出限为0.03 μg/mL,检测范围0.1～10 μg/mL。研究表明,不同酸度和酸的类型对谱线强度影响较大,且存在显著的样品基体效应,标准曲线法分析锂辉石中Li的结果偏差高达267%;而标准加入法可克服基体效应的影响,获得与ICP-OES一致性较好的分析结果,为现场开展固体样品中Li的测定奠定了基础。  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   

青藏高原拉萨地块西部念青唐古拉岩群的地球化学特征及构造意义   总被引：1，自引：0，他引：1  

吴勇  马绪宣  张志平  焦世文  段凯  董瀚  王小伟  马涛  李鹏举  梁志勇  曹勇刚  孔垂鹏  马亮 《地质学报》2016,90(11):3081-3098

拉萨地块西部呈断块状沿狮泉河-申扎-嘉黎蛇绿混杂岩带附近分布的念青唐古拉岩群被认为是前寒武纪变质基底。本文对念青唐古拉岩群进行了系统的岩石学、地球化学、同位素年代学及构造地质学研究。研究结果表明片岩-片麻岩-变粒岩含十字石、石榴子石等特征变质矿物,遵循粒度分异规律,其原岩可能为来自冈瓦纳古陆核北缘中新元古代弧盆体系的活动大陆边缘浊积岩。斜长角闪岩具低硅、高铁镁、富钙的基性岩特征,其原岩为岛弧型基性火山岩。念青唐古拉岩群中的花岗伟晶岩锆石LA-ICPMS U-Pb年龄为1150±13Ma,具过铝质S型花岗岩地球化学特征,可能为中元古代(1150±13 Ma)以前就开始沉积的念青唐古拉岩群基底岩石通过部分熔融形成。与花岗伟晶岩渐变过渡接触的二云斜长片麻岩第一组变质重结晶锆石U-Pb年龄为701±15 Ma,结合十字石特征变质矿物,暗示了该地区中温高压变质作用的峰期变质,变质程度达角闪岩相;第二组热液流体锆石UPb年龄为301±8.4 Ma,可能与冈瓦纳大陆北缘古特提斯洋演化过程中的岩浆热液作用有关。  相似文献   

陕西华阳川铀多金属矿床黑云母~(40)Ar/~(39)Ar年龄及其地质意义     

何升  李子颖  惠小朝  郭建 《铀矿地质》2016,(3):159-164

笔者采用Ar-Ar测年技术,获得华阳川铀多金属矿床碳酸岩中黑云母~(40)Ar/~(39)Ar坪年龄132.58±0.70 Ma,等时线年龄133.01±0.74 Ma,含黑云母闪石硫化物伟晶岩中黑云母的~(40)Ar/~(39)Ar坪年龄93.72±2.38 Ma,等时线年龄91.49±1.97 Ma。镜下特征显示,铌钛铀矿的形成晚于碳酸岩中的黑云母及含黑云母闪石硫化物伟晶岩中的黑云母。因此,铌钛铀矿的形成时间应晚于93.72±2.38 Ma。这表明成矿带内除了已知存在三叠纪碳酸岩型Mo-Pb矿和白垩纪斑岩型Mo矿的成矿过程之外,还存在早白垩世之后的岩浆热液型U-Nb-Ti成矿过程。  相似文献   

Interaction of crustal and mantle materials,sources of trace elements during the formation and evolution of Early Paleozoic Li-rich granite-pegmatite systems in southeastern Tuva     

L.G. Kuznetsova 《Russian Geology and Geophysics》2018,59(12):1660-1678

We present new data on the age, composition, and environments of formation of granites of the Kystarys complex and the associated Li-rich rare-element pegmatites of the South Sangilen pegmatite belt including the large Tastyg lithium deposit. It has been established that they formed during the Early Paleozoic collisional orogeny in the Tuva-Mongolian massif at the Cambrian-Ordovician boundary. The granites of the Kystarys complex are moderately alkaline high-K rocks and are enriched in Zr, Nb, Y, and REE; therefore, they are classified as postcollisional, transitional to within-plate (A-type). The spodumene pegmatites of the South Sangilen pegmatite belt are similar to the above granites in age and isotopic and geochemical parameters, which suggests a paragenetic relationship between these rocks. Pegmatites form several pegmatite fields within the belt, which differ in trace-element signatures. In addition to predominant Li, Cs, and Ta, specific to all spodumene pegmatites (LCT family), pegmatites of two fields have high contents of Nb, Y, REE, and Zr, which are indicator elements of NYF family pegmatites. It has been established that the formation of spodumene pegmatites with combined LCT-NYF geochemical signatures was preceded by the intrusion of dikes of monzogabbro with the geochemical characteristics of OIB and of alkali aegirine granites and by the formation of associated metasomatites enriched in Zr, Nb, Y, and REE. Based on the geological, mineralogical, and geochemical data, we substantiate the hypothesis of the formation of Li-bearing granite-pegmatite melts from a mixed source resulted from the influence of fluids of an alkaline igneous complex of mantle genesis on the crustal protolith.  相似文献