安徽女山单斜辉石巨晶的地球化学   总被引：14，自引：0，他引：14  

陈道公  夏群科 《矿物学报》1997,17(3):260-269

本文研究了安徽女山14个单斜辉石巨晶。它们属于铝普通辉石、透辉石和铁钠造辉石。主要元素、稀土和微量元素及同位素特征表明：它们是同一碱性玄武岩浆在幔源条件下不同程度结晶分异的产物，相对于寄主岩均属捕虏晶，可能自中生代即已开始形成。  相似文献   

碱性玄武岩中的某些巨晶单斜辉石──Ⅱ:穆斯堡尔谱──兼论单斜辉石的异常穆斯堡尔谱和铁结构态的测定     

章礼明  傅平秋  张恩林 《矿物学报》1996,(1)

本文对辽宁宽甸碱性玄武岩中巨晶单斜辉石进行穆斯堡尔谱研究。应用晶体结构研究结果较合理地解释了单斜辉石的异常穆斯堡尔谱。结合XRD讨论了单斜辉石中Fe结构态的测定以及穆斯堡尔谱的可应用性。巨晶应结晶于相当氧化的环境。  相似文献   

河北汉诺坝玄武岩中深源包体和巨晶分布的动力学机理          下载免费PDF全文

袁万明  冯家麟 《岩石矿物学杂志》1993,12(1):12-19

汉诺坝碱性玄武岩是深源包体和巨晶的主要寄主岩,同时,也有不含包体的碱性玄武岩和含包体的拉斑玄武岩。本文基于理论计算,探讨了包体和巨晶分布的动力学机理。  相似文献   

中国东部新生代玄武岩中单斜辉石巨晶的主要特征及成因信息   总被引：7，自引：1，他引：7  

邱家骧  廖群安 《岩石矿物学杂志》1987,6(1):56-64

作者通过对我国东部新生代玄武岩中巨晶Cpx的109个样品的化学成分的统计、计算及投影,研究了Cpx巨晶的产状、物性及矿物化学的主要特征,并对其成因信息提出了自己的看法。Cpx巨晶的成分以A1_2O_3、A1~(v1)较高而Ti、Mg'中等为特征。但在“反应边”中,A1_2O_3、Na_2O、A1、A1~(v1)则明显降低。我国巨晶以普通辉石为主,而透辉石、次透辉石及顽透辉石少见。国内不同地区的Cpx巨晶成分也略有不同:华南区巨晶的Wo较高而A1_2O_3较低;华北区Fs、A1_2O_3较高;而东北区En较高而A1_2O_3中等。有关Cpx巨晶的成因信息,作者的观点是:(1)巨晶Cpx是寄主玄武岩浆在上地幔中结晶的产物,而不是地幔解体的捕虏晶。(2)我国巨晶Cpx的结晶温度是1021—1209℃,压力为1.4—3.2GPa,所以,Cpx巨晶的结晶深度为48—104Km。(3)我国东部新生代玄武岩均产于大陆板块内部,以碱性玄武岩成分为主,而拉斑玄武岩较少。  相似文献   

我国东部若干地区新生代玄武岩中长石巨晶的特征及成因   总被引：2，自引：0，他引：2  

邱家骧  刘蒙华 《矿物学报》1987,(1)

本文汇集了中国东部新生代玄武岩中76个长石巨晶的化学成分,并与53个国外长石巨品进行了对比。文中对长石巨晶的产状、物理性质、矿物化学及微量元素进行了研究,并对国际上关于长石巨晶五个有争议的问题进行了讨论。作者同时也提出了自己的观点。  相似文献   

辉石巨晶中的硫化物及其成因   总被引：8，自引：1，他引：8  

黄婉康  A.R.Basu 《矿物学报》1987,(2)

我国一些地区玄武岩辉石巨晶中的硫化物球泡(0.02-0.05mm)呈点阵式、散布式、定向带状或微裂隙羽状分布。硫化矿物组合是磁黄铁矿-镍黄铁矿-黄铜矿,其中以磁黄铁矿为主(～90％)。根据硫化物的规则排布以及高温矿物组合推测点阵式、散布式硫化物形成于地幔。是由溶解了～1％S的硅酸盐熔体在减压上升过程中析出过饱和的硫所致。  相似文献   

Thermoelastic model of minerals: application to Al2O3     

J. Hama  K. Suito 《Physics and Chemistry of Minerals》2001,28(4):258-267

 A thermoelastic model for calculating the high-pressure and high-temperature properties of isotropic solids is presented by extending the formalism by Thomsen and combining the resulting one with the Vinet model for static lattice and the Debye model for lattice vibration. Applying it to polycrystalline corundum, we have shown that the calculated values of entropy and heat capacity at constant pressure are in agreement with literature values to 2325 K at zero pressure and that the calculated values of thermal expansivity agree reasonably with experimental data to 1100 K at zero pressure. The model reproduces experimental data of sound velocities v _p and v _s of compressional and shear waves to 1825 K at zero pressure and those to 62 GPa at room temperature, and it reproduces also experimental shock-wave equation of state to 150 GPa. The velocity correlation (∂ln v _s /∂ln v _p ) _S was found to have weak pressure and temperature dependences and the results under lower mantle conditions are compared with those of magnesian and calcium silicate perovskites and magnesiowüstite, and the PREM values of the Earth's lower mantle. Received: 12 February 2000 / Accepted: 15 July 2000  相似文献   

东海芝麻坊的红刚玉石榴岩   总被引：2，自引：0，他引：2  

樊祺诚  严奉林 《岩石学报》1992,8(3):291-295,T001

  相似文献   

High-precision analysis of carbon isotopic composition for individual CO2 inclusions via Raman spectroscopy to reveal the multiple-stages evolution of CO2- bearing fluids and melts     

《地学前缘(英文版)》2023,14(3):101528

The carbon isotopic composition of CO₂ inclusions trapped in minerals reflects the origin and evolution of CO₂-bearing fluids and melts, and records the multiple-stages carbon geodynamic cycle, as CO₂ took part in various geological processes widely. However, the practical method for determination isotope composition of individual CO₂ inclusion is still lacking. Developing a microanalytical technique with spatial resolution in micrometers to precisely determinate the δ¹³C value of individual CO₂ inclusion, will make it possible to analyze a tiny portion of a zoning mineral crystal, distinguish the differences in micro-scale, and possible to find many useful information that could not be obtained with the bulk extraction and analysis techniques. In this study, we systematically collected Raman spectra of CO₂ standards with different δ¹³C values (?34.9 ‰ to 3.58 ‰) at 32.0 °C and from ～7.0 MPa to 120.0 MPa, and developed a new procedure to precisely determinate the δ¹³C value of individual CO₂ inclusion. We investigated the relationship among the Raman peak intensity ratio, δ¹³C value, and CO₂ density, and established a calibration model with high accuracy (0.5 ‰?1.5 ‰), sufficient for geological application to distinguish different source of CO₂ with varying δ¹³CO₂. As a demonstration, we measured the δ¹³C values and the density of CO₂ inclusions in the growth zones of alkali basalt-hosted corundum megacrysts from Changle, Shandong Province. We found the significant differences of density and δ¹³C between the CO₂ inclusions in the core of corundum and those inclusions in the outer growth zones, the δ¹³C value decreases from core to rim with decreasing density: δ¹³C values are from ?7.5 ‰ to ?9.2 ‰ for the inclusions in the core, indicating the corundum core was crystallized from mantle-derived magmas; from ?13.5 ‰ to ?18.5 ‰ for CO₂ inclusions in zone 1 and from ?16.5 ‰ to –22.0 ‰ for inclusions in zone 2, indicating the outer zones of corundum grew in a low δ¹³C value environment, resulted from an infilling of low δ¹³C value fluid and/or degassing of the ascending basaltic magma.  相似文献   

Geochemical and oxygen isotope signatures of mantle corundum megacrysts from the Mbuji-Mayi kimberlite,Democratic Republic of Congo,and the Changle alkali basalt,China     

《Comptes Rendus Geoscience》2015,347(1):24-34

Oxygen isotope signatures of ruby and sapphire megacrysts, combined with trace-element analysis, from the Mbuji-Mayi kimberlite, Democratic Republic of Congo, and the Changle alkali basalt, China, provide clues to specify their origin in the deep Earth. At Mbuji-Mayi, pink sapphires have δ¹⁸O values in the range 4.3 to 5.4‰ (N = 10) with a mean of 4.9 ± 0.4‰, and rubies from 5.5 to 5.6‰ (N = 3). The Ga/Mg ratio of pink sapphires is between 1.9 and 3.9, and in rubies, between 0.6 and 2.6. The blue or yellow sapphires from Changle have δ¹⁸O values from 4.6 to 5.2 ‰, with a mean of 4.9 ± 0.2‰ (N = 9). The Ga/Mg ratio is between 5.7 and 11.3. The homogenous isotopic composition of ruby suggests a derivation from upper mantle xenoliths (garnet lherzolite, pyroxenite) or metagabbros and/or lower crustal garnet clinopyroxenite eclogite-type xenoliths included in kimberlites. Data from the pink sapphires from Mbuji-Mayi suggest a mantle origin, but different probable protoliths: either subducted oceanic protolith transformed into eclogite with δ¹⁸O values buffered to the mantle value, or clinopyroxenite protoliths in peridotite. The Changle sapphires have a mantle O-isotope signature. They probably formed in syenitic magmas produced by low degree partial melting of a spinel lherzolite source. The kimberlite and the alkali basalt acted as gem conveyors from the upper mantle up to the surface.  相似文献