山东昌乐新生代碱性玄武岩中的巨晶单斜辉石成因研究

山东昌乐新生代碱性玄武岩中除斑晶单斜辉石和基质单斜辉石外,还发育大量巨晶单斜辉石和同源斜方辉石捕掳晶。巨晶单斜辉石与玄武岩间发育复杂和简单两种类型的反应边。复杂反应边往往发育在颗粒较大的巨晶单斜辉石外围。复杂反应边可分为4个带：内部带、过渡带、外部带和边缘带,其中,内部带、过渡带和外部带均由具不同结构特征的单斜辉石＋熔体＋金属氧化物构成,边缘带为不含熔体和金属氧化物的干净的单斜辉石;内部带的单斜辉石具梳状构造,过渡带的单斜辉石具细密筛孔构造,外部带为具似砂钟构造的筛孔状单斜辉石。反应边中单斜辉石、熔体及金属氧化物的成分显示,只有内部带受到单斜辉石巨晶的影响,其余带均受玄武岩浆的制约。简单反应边往往发育在颗粒较小的巨晶单斜辉石外围。简单反应边仅发育不含熔体和金属氧化物的干净的单斜辉石。巨晶单斜辉石的反应边是巨晶与玄武岩浆间温度差造成的。在与玄武岩浆反应的过程中,大颗粒的单斜辉石巨晶需要较长的时间与玄武岩浆达到温度平衡,从而有足够的时间发育包含4个带的复杂反应边;反之,由于缺乏足够的反应时间,小颗粒单斜辉石巨晶的外围只发育不含熔体和金属氧化物的简单反应边。同源斜方辉石捕掳晶的成分与地幔二辉橄榄岩包体中的斜方辉石类似,其边部发育类似于Bowen反应（1956）形成的单斜辉石环边。在单斜辉石Al^IV-Al^VI图解上,巨晶单斜辉石、二辉橄榄岩包体中的单斜辉石以及部分单斜辉石斑晶的核部,均位于较高压力的“麻粒岩和玄武岩中包体”区域,反应边中单斜辉石、基质单斜辉石以及绝大部分斑晶单斜辉石位于“火成岩”区域,说明部分斑晶单斜辉石核部来源于地幔二辉橄榄岩,属于捕掳晶。结合单斜辉石结晶压力的估算,笔者认为巨晶单斜辉石的成因模式为：来自软流圈的碱质基性熔体上侵到地幔岩石圈下部,结晶形成单斜辉石巨晶,后来该熔体携带巨晶单斜辉石与来自上地幔岩石圈、夹带大量二辉橄榄岩包体以及斜方辉石（和单斜辉石）捕掳晶的玄武岩浆混合,巨晶单斜辉石随混合后的碱性玄武岩浆上升、喷出地表。     

华北晚中生代和新生代玄武岩中单斜辉石巨晶来源及其对寄主岩岩浆过程的制约:以莒南和鹤壁为例

本文对华北克拉通晚中生代和新生代碱性玄武质岩石中的单斜辉石巨晶进行了主、微量元素和Sr-Nd同位素的综合研究,发现晚中生代和新生代单斜辉石巨晶存在明显的主、微量元素和同位素组成上的差异.新生代单斜辉石巨晶有Al-普通辉石和次透辉石两类;而中生代单斜辉石巨晶只有Al-普通辉石.新生代单斜辉石SiO2含量高、REE配分型式为上凸型、LILE和放射性元素含量高,并具有比寄主碱性玄武岩更亏损的Sr和Nd同位素组成;而中生代单斜辉石SiO2含量低、REE配分型式为LREE富集型、LILE和部分HFSE以及放射性元素含量低,并具有比寄主碱性玄武岩稍富集的Sr和Nd同位素组成;巨晶的结构、矿物成分和地球化学特征,以及Mg-Fe在熔体与单斜辉石间的分配状况皆说明,新生代碱性玄武岩中单斜辉石巨晶是碱性玄武岩浆在高压下结晶的,因此二者是同源的;而中生代单斜辉石巨晶是被寄主岩浆偶然捕获的捕虏晶,是不同源的.华北新生代单斜辉石巨晶存在于碱性玄武岩和拉斑玄武岩中,它们具有比寄主碱性玄武岩更亏损的Sr和Nd同位素组成,说明即使是碱性玄武岩也不能完全代表软流圈来源的原始岩浆,其在上升过程中或多或少存在同位素组成富集的物质的混入.同时,拉斑玄武岩不是碱性玄武质岩浆直接结晶分异的产物,亦不是完全由部分熔融程度的不同造成的.拉斑玄武岩中存在岩石圈地幔物质的贡献或是岩浆房内碱性玄武质岩浆受地壳混染作用的结果.     

中国东部新生代玄武岩中巨晶矿物的地球化学

本文对安徽女山、河北汉诺坝和广东普宁碱性玄武岩中的单斜辉石和角闪石巨晶进行了主要元素、稀土元素、微量元天和Ｓｒ＿Ｎｄ同位素的综合分析。数据显示产出于３个研究区的单斜辉石巨晶有３类：Ａｌ普通辉石、透辉石和Ｆｅ＿Ｎａ透辉石。普宁地区的角闪石巨晶乃世界上罕见的绿钙闪石巨晶。女山和普宁的单斜辉石和角闪石巨晶是碱性玄武岩浆在幔源高压下的结晶产物；汉诺坝的单斜辉石巨晶既可以是碱性玄武岩浆又可以是拉斑玄武岩浆的高压结晶体。所有巨晶相对于寄主岩者属于偶然捕掳晶。巨晶的形成符合“流动结晶模式”。它们与共存的橄榄岩色体无成因     

滇东南马关巨晶单斜辉石原位Sr同位素特征及其含水性

对滇东南马关火山爆砾岩筒以及玄武岩中的单斜辉石巨晶进行了主量元素、微量元素、原位Sr同位素以及含水性研究,结果显示,单斜辉石巨晶均为铝质普通辉石,Mg#与Al、Fe、Ti呈负相关,与Ca呈正相关;稀土元素总量不高,HREE及LREE亏损,而MREE相对富集,大离子亲石元素均出现明显亏损,高场强元素Nb、Zr出现亏损而Hf略富集,Nb、Ta与Zr、Hf分馏明显,Rb、Ba的变化范围较大。原位Sr同位素87Sr/86Sr值为0. 703 92～0. 705 06,巨晶单斜辉石来源于上地幔,形成于同一母岩浆,与寄主玄武岩同源,为源岩浆在高压下的结晶产物。运用显微红外-傅里叶变换红外光谱仪(Micro-FTIR)分析测试了单斜辉石巨晶的水含量,结果显示OH吸收峰位于3 700～2 800cm-1,含水量赋值范围为318×10-6～693×10-6,水含量稍富于女山及汉诺坝地区的单斜辉石巨晶,也高于马关地区幔源橄榄岩包体中的单斜辉石结构水含量,暗示该区上地幔岩石圈具高含水性,这同时证实了俯冲洋壳在研究区的活动。新近纪到达地幔过渡带的西太平洋洋壳俯冲发生转向东撤,此时新特提斯洋洋壳正在NE向俯冲,是马关地区深部地幔富水的主因,到达软流圈(或地幔过渡带)的新特提斯洋俯冲洋壳导致该区地幔熔融,岩浆随之而生。     

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

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。     

中国东部几个地区新生代玄武岩中单斜辉石—熔体平衡温压—兼论幔源包体的成因

以中国东部宽甸、汉诺坝和明溪含有幔源包体的新生代玄武岩中的单斜辉石斑（巨）晶为研究对象,采用最新的单斜辉石－熔体平衡温压计对单斜辉石斑（巨）晶－熔体进行了平衡温压计算。结果表明,碱性玄武岩中的单斜辉石斑晶结晶温度和压力高于共生的亚碱性玄武岩中的单斜辉石斑晶,单斜辉石巨晶的结晶温度和压力高于单斜辉石斑晶。这说明碱性玄武岩的形成深度大于亚碱性玄武岩,单斜辉石巨晶是更高压力下的结晶产物,单斜辉石斑晶在岩浆上升的不同深度均有晶出。回归分析表明,尽管携带幔源包体的玄武岩浆上升速度较快,但并不是绝热上升。单斜辉石斑（巨）晶的结晶温压条件与同一地点幔源包体平衡温压条件的对比表明,单斜辉石巨晶和碱性玄武岩中的部分单斜辉石斑（巨）晶的结晶温压大于幔源包体的平衡温压,表明了包体寄主岩浆的来源深度大于包体的深度。因此,幔源包体是寄主岩浆上升途中捕虏的上地幔碎块,而非寄主岩浆形成源区的残留体。     

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…

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。     

华北晚中生代和新生代玄武岩中单斜辉石巨晶来源及其对寄主岩岩浆过程的制约

玄武岩中的"巨晶",因矿物颗粒粗大而得名,通常是指那些相对于玄武岩斑晶,形成深度较大即结晶于较高压力环境,个体粗大的单矿物晶体.因此,通常用高压巨晶来描述玄武岩中这些个体粗大的单矿物晶体(鄂莫岚和赵大升,1987),如单斜辉石巨晶、透长石/歪长石巨晶、石榴子石巨晶、锆石巨晶和蓝宝石等,其中以单斜辉石巨晶最为常见.华北克拉通中部中生代岩石圈地幔的性质:     

碱性玄武岩中巨晶辉石的出溶结构

人们在研究玄武岩浆的起源和演化时,对碱性玄武岩中的巨晶辉石产生了越来越大的兴趣。这些巨晶辉石具下列特点:个体大;常与来自上地幔的橄榄岩包体伴生;其氧化铝含量,特别是Al(?)的含量远高于寄主玄武岩中的辉石斑晶和橄榄岩包体中的单斜辉石;与寄主     

延边明月沟盆地中生代火山岩深源捕虏体和捕虏晶的发现及矿物化学

在延边地区明月沟盆地中侏罗世屯田营组火山岩中发现含有较多的辉石岩捕虏体及单斜辉石和角闪石捕虏晶。单斜辉石相对富含Al2O3、FeO和TiO2,与中国东部新生代玄武岩中单斜辉石巨晶的成分相当。角闪石巨晶的成分明显不同于地幔橄榄岩包体中的韭闪石。从矿物化学所获得的温度-压力计算结果表明：岩浆来源应位于壳幔过渡带。     

Constitution Water in Mantle-derived Megacryst and Xenolith Pyroxene of an Ultrabasic Pipe in Anyuan, Jiangxi

This paper studies the hydrous facies of mantle-derived megacryst clinopyroxenes and pyroxenes of xeno-liths of pyroxenolite and spinel peridotite as well as garnet pyroxenolite in a kimberlitic lamprophyre pipe in Anyuan, Jiangxi, by Fourier Transform Infrared (FTIR). It explores the relationship between the water content of pyroxene on the one hand and its composition and source depths on the other hand. All the samples contain constitution water. Spectra of the clinopyroxene are dominated by two groups of bands: 3607-3630 cm-1 and 3522-3542 cm-1. Spectra of the orthopy-roxene are dominated by three groups of bands: 3410-3424 cm-1,3510-3516 cm-1 and 3560-3595 cm-1. The water content of the clinopyroxenes has a positive correlation with their FeO and Al2O3 contents. The source depths of mantle-derived clinopyroxene megacrysts, pyroxenolite, spinel peritotite and garnet pyroxenelite increase gradually in order. The Al2O3 and water contents of four pyroxenes have similar correlation with the source depth     

Petrologic implications of trace element variation in clinopyroxene megacrysts from the Nógrád volcanic province, north Hungary: a study by laser ablation microprobe-inductively coupled plasma-mass spectrometry

Clinopyroxene megacrysts in alkali basalts are an important source of information about the evolution of magmatic systems at depth. In this study, we have undertaken a detailed examination of the trace element contents in a suite of megacrysts from 2.5 Ma old alkali basalts in the Nógrád volcanic province of Hungary and Slovakia. The megacrysts range in composition from Mg-rich and in equilibrium with their host magmas, to those that are Fe-rich and must have evolved in more fractionated magmas. The conditions of crystallization of these megacrysts, as calculated from the Al^VI/Al^IV ratios, suggests they all formed at about 30 km, or the crust–mantle boundary in this area. Using the most magnesian megacrysts and compositions of the host lavas, we have calculated the partition coefficients for a range of trace elements. However, the trace element contents in the megacrysts show a systematic variation with major element composition. Moreover, the rate of increase or change in the trace element concentrations is not consistent with models involving constant or steady state partition coefficients. Using a series of assumptions and models, we hypothesize that the partition coefficients between clinopyroxene and melt change substantially during the magmatic evolution of the system. This change is not constant for each element group, with the high field strength elements showing the most substantial increases. Electrostatic charge balance may have been the most important factor in controlling the mineral/melt partitioning.     

Andesine megacrysts in alkali basalts from Japan

Andesine megacrysts up to 3 cm in size occur sporadically in certain alkali basalts and allied mafic rocks in southwestern Japan. They are sometimes accompanied by megacrysts of mafic minerals and ultramafic and mafic inclusions. Nine andesines have been chemically analysed.From the petrography and chemistry and the results of high pressure experimental work, it is suggested that andesine megacrysts crystallized from alkali basalt magma under dry conditions at a depth of about 30 to 60 km.     

K-feldspar megacrysts in granites — Phenocrysts,not porphyroblasts

K-feldspar megacrysts in granitoid plutons have been interpreted as either phenocrysts or porphyroblasts. Most of the microstructural, mineralogical and chemical evidence (e.g., shape, alignment, concentration, Ba content, zoning, inclusions, and twinning) favours a phenocryst origin. The main features that have been used to support a porphyroblast origin are occurrence of megacrysts: (1) across aplite vein boundaries, (2) in country rocks, and (3) in or across boundaries of microgranitoid enclaves (mafic inclusions). However, these features can be explained by the phenocryst hypothesis. In particular, megacrysts in microgranitoid enclaves can be explained by growth or mixing in magma before a globule of that magma or a fragment of the resulting igneous rock was incorporated as an enclave. All available evidence favours or is consistent with a phenocryst origin for K-feldspar megacrysts in granitoid rocks and their enclaves.The large size of the megacrysts is evidently due to nucleation difficulties for K-feldspar in granitic melts. Though K-feldspar is commonly the last mineral to begin crystallizing in granitic magmas, abundant melt is still present at that stage, allowing sufficient space for the megacrysts to grow. The reason for the common lack of megacrysts in volcanic rocks may be that the phenocrysts do not grow large enough to be called “megacrysts” until the magma contains such a high proportion of crystals that it cannot erupt.     

Amphibole megacrysts as a probe into the deep plumbing system of Merapi volcano,Central Java,Indonesia

Amphibole has been discussed to potentially represent an important phase during early chemical evolution of arc magmas, but is not commonly observed in eruptive arc rocks. Here, we present an in-depth study of metastable calcic amphibole megacrysts in basaltic andesites of Merapi volcano, Indonesia. Radiogenic Sr and Nd isotope compositions of the amphibole megacrysts overlap with the host rock range, indicating that they represent antecrysts to the host magmas rather than xenocrysts. Amphibole-based barometry suggests that the megacrysts crystallised at pressures of >500 MPa, i.e., in the mid- to lower crust beneath Merapi. Rare-earth element concentrations, in turn, require the absence of magmatic garnet in the Merapi feeding system and, therefore, place an uppermost limit for the pressure of amphibole crystallisation at ca. 800 MPa. The host magmas of the megacrysts seem to have fractionated significant amounts of amphibole and/or clinopyroxene, because of their low Dy/Yb ratios relative to the estimated compositions of the parent magmas to the megacrysts. The megacrysts’ parent magmas at depth may thus have evolved by amphibole fractionation, in line with apparently coupled variations of trace element ratios in the megacrysts, such as e.g., decreasing Zr/Hf with Dy/Yb. Moreover, the Th/U ratios of the amphibole megacrysts decrease with increasing Dy/Yb and are lower than Th/U ratios in the basaltic andesite host rocks. Uranium in the megacrysts’ parent magmas, therefore, may have occurred predominantly in the tetravalent state, suggesting that magmatic fO₂ in the Merapi plumbing system increased from below the FMQ buffer in the mid-to-lower crust to 0.6–2.2 log units above it in the near surface environment. In addition, some of the amphibole megacrysts experienced dehydrogenation (H₂ loss) and/or dehydration (H₂O loss), as recorded by their variable H₂O contents and D/H and Fe³⁺/Fe²⁺ ratios, and the release of these volatile species into the shallow plumbing system may facilitate Merapi’s often erratic eruptive behaviour.     

Stages in the P-T path of ascending basalt magma: An example from San Quintin,Baja California

Late Pleistocene or Recent lavas from San Quintin, Baja California are basanitoids and alkali basalts. The surface quench temperatures of the lavas average 1 005° C with log =–11.4, as deduced from the groundmass Fe-Ti oxides. Spinel lherzolite xenoliths and megacrysts of augite and andesine have been found in lava flows and cinder deposits. Using analytical data on the rocks and minerals and simple thermodynamic expressions, the pressures and temperatures of equilibration of lavas and xenoliths, megacrysts and phenocrysts have been calculated. The lavas could have been in equilibrium with lherzolite at 1 330–1 410° C and 27.5–31.6 kb, the more silica-poor liquid having the higher values. The basanitoid could have equilibrated with the megacrysts at about 10.5 kb and with phenocrysts at about 1.4 kb and 1130° C. The variation in composition of the lavas may be explained by a rising zone of melting within the mantle, the most silica-poor liquid having the deepest source. The source of the San Quintin basalts is probably related to spreading of the ocean floor in the Gulf of California.     

How late are K-feldspar megacrysts in granites?

Various petrologists have suggested that K-feldspar megacrysts grow in granites that are extensively crystallized, even at subsolidus conditions. However, experimental evidence indicates that, though K-feldspar nucleates relatively late in the crystallization history, abundant liquid is available for development of large crystals. A great deal of evidence, involving many different factors, favours a magmatic/phenocrystic origin for K-feldspar megacrysts in granites, namely simple twinning, oscillatory zoning, euhedral plagioclase inclusions, and concentric, crystallographically controlled arrangements of inclusions. In addition, abundant evidence has been presented of (1) mechanical accumulation of K-feldspar megacrysts in granites, (2) alignment of megacrysts and megacryst concentrations in magmatic flow foliations, (3) involvement of megacrysts in zones of magma mixing in granite plutons, and (4) occurrence of megacrysts in some volcanic rocks, implying that the megacrysts were suspended in enough liquid to be moved without fracturing or plastic deformation. Detailed trace element and isotopic data also indicate that megacrysts can move between coexisting felsic and more mafic magmas. Irregular overgrowths on megacrysts are consistent with continued magmatic growth after euhedral megacrystic growth ceased, the overgrowths being impeded by simultaneously crystallizing quartz and feldspar grains.     

A complex magmatic system beneath the Devès volcanic field,Massif Central,France: evidence from clinopyroxene megacrysts

Clinopyroxene megacrysts and mineral aggregates with clinopyroxene occur in the volcanic deposits at Mont Briançon and Marais de Limagne, which are located in the northern part of the Devès volcanic field (Massif Central, France). The clinopyroxenes can be subdivided into five groups based upon their major and trace element chemistry. Types 1a, 1b and 1c have mg# ～0.80 and are relatively Al-rich and low in Na and Fe³⁺. Subdivision into three groups is based on differing trace element signatures. Type 2 clinopyroxenes have mg# = 0.63–0.65 and higher Na and Fe³⁺ (Fe³⁺/ΣFe > 0.4) contents and may contain apatite inclusions. A type 3 megacryst is Fe-rich (mg# = ～0.52) and has the highest Na and Fe³⁺ contents, as well as containing titanite and apatite inclusions. High Fe³⁺ contents in all clinopyroxenes investigated emphasises the need to consider Fe³⁺/Fe²⁺ when assessing the petrologic origin of such megacrysts. The large range in mg# means that the clinopyroxenes could not all have crystallised from the same melt; in fact comparison with the basanitic host lavas from the two localities reveal that nearly all of the megacrysts are xenocrystic in the strict sense. The clinopyroxenes are mostly genetically related, having crystallised from related melts within the magmatic system that had undergone various degrees of differentiation. Similarities in clinopyroxene chemistry indicate that both volcanic centres are linked to the same magmatic system at depth. Assessing the depth of crystallisation reveals that types 1a and 1b formed in the lithospheric mantle, near the asthenosphere–lithosphere boundary, whereas types 1c, 2 and 3 formed in crustal magma chambers or conduits. Eruption was induced by a pulse of Mg-rich magma from the asthenosphere that entered the existing magmatic system, entraining clinopyroxene as megacrysts at several stages of ascent, before erupting at the surface. The style of eruption at Mont Briançon (cinder cone) and Marais de Limagne (maar) is different and most likely reflects local differences in near-surface hydrology. The essentially identical variety in megacrysts at the two localities suggests that eruption must have been nearly contemporaneous.     

西伯利亚雅库特金伯利岩中四颗古老锆石巨晶的微量元素和Hf同位素特征——对区分金伯利岩中锆石巨晶的启示

金伯利岩中的锆石按照颗粒大小可以分为细粒锆石（一般小于200μm）和巨晶锆石（一般大于500μm）。前人的研究结果显示在金伯利岩中粒径较大的巨晶锆石的U-Pb体系在高温的地幔中一直保持着开放状态,直到寄主金伯利岩浆的喷发才使地幔锆石的U-Pb体系封闭,因此这些巨晶锆石是确定金伯利岩年龄的重要矿物之一。然而,近年来的研究表明,金伯利岩中还存在一些时代远老于金伯利岩年龄的锆石,也具有较大的粒径（以下称古老锆石巨晶）。它们的存在无疑影响了利用锆石U-Pb方法确定金伯利岩年龄的准确性。本文以西伯利亚雅库特（Yakutia）金伯利岩省中的四颗古老锆石巨晶为研究对象,通过形态学、年代学、微量元素和Hf同位素组成,讨论古老锆石巨晶的来源。同时,我们统计和对比了全球多个金伯利岩中能够确定金伯利岩年龄的锆石和古老锆石巨晶的形态学、U、Th含量和微量元素组成、Hf-O同位素等特征。研究结果显示,金伯利岩中的古老锆石巨晶的t_DM年龄和O同位素组成与可以用来确定金伯利岩年龄的锆石巨晶具有明显的差别。这些手段在未来的研究中可以用来区分可确定金伯利岩年龄的锆石巨晶和古老的锆石巨晶。

     

三斜水钠锰矿层间阳离子交换作用的拉曼谱学

水钠锰矿为自然界中常见的锰氧化物矿物,其离子交换作用及结构转变理解尚不深刻,矿物表征手段较为局限.为探究水钠锰矿的离子交换特性以及结构转变在拉曼光谱上的反映,利用MnSO₄和NaOH合成了三斜晶系的Na型水钠锰矿,进行了NH₄+、K+、Mg2+、Ca2+、Ba2+、Co2+、Zn2+的离子交换实验,使用ICP-OES、XRD、拉曼光谱等手段对离子交换水钠锰矿进行表征.拉曼光谱分析表明,570~585 cm-1与640~655 cm-1两个锰氧八面体伸缩振动模式的相对强度及570~585 cm-1附近拉曼峰峰位指示水钠锰矿的结构对称型;570~585 cm-1拉曼峰强度大、振动频率高指示三斜对称型.280 cm-1与500 cm-1附近的拉曼峰是层间离子种类的识别标志.水钠锰矿层间若为Na+、K+、Mg2+、Ca2+、Ba2+等碱金属、碱土金属离子,则在280 cm-1附近存在1个峰值,500 cm-1存在2个分立的峰值;其他种类的层间离子仅500 cm-1处有1个孤峰,指示层间离子排列无序.