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1.
闪锌矿是自然界常见的重要金属矿物,含有很多种杂质元素,其中Fe、Cd是闪锌矿最常见,也是最重要的杂质元素。普遍认为,闪锌矿中的Cd、Fe是类质同象取代了Zn。但是,笔者研究发现闪锌矿的Cd与Zn往往成正相关,与Fe呈负消长。说明闪锌矿的Cd类质同象置换主要不是Zn,而是Fe。而且,闪锌矿Cd与Fe的相关性随其颜色的改变而变化。深色闪锌矿的Cd与Fe呈负相关,褐色闪锌矿Cd与Fe既有负消长关系,又有正消长关系。浅色闪锌矿的Cd与Fe呈正相关的数量大增。暗色闪锌矿多形成于高温,Fe具有强烈置换Zn能力。随着形成温度下降,Fe交代Zn的能力不仅逐渐减弱,而且,闪锌矿晶格的Fe变得不稳定,而被释放出来,主要由Cd替代。浅色闪锌矿形成于低温,矿液结晶的后期。矿液中的Zn可能不能满足闪锌矿结晶对Zn的需求,就由离子参数相似的Cd2+和Fe2+替代。致使闪锌矿的Cd与Fe呈正相关,Cd和Fe与Zn负消长。 相似文献
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加勒比海小安德列斯岛弧Kick’emJenny海底火山岩的斜长石成分环带:示踪大洋岛弧岩浆房的演化 总被引：1，自引：0，他引：1
我们对采自于加勒比海地区小安德列斯岛弧(Lesser Antilles Arc)Kick’em Jenny(KEJ)海底火山玄武岩中的斜长石斑晶进行了矿物形态和成分分析。利用电子探针(EMPA)和LA-ICP-MS测定了具有环带结构的斜长石斑晶中主量元素的空间分布,同时也利用LA-ICP-MS分析了斜长石中Sr的分布。结果表明,在不同的矿物斑晶中,元素含量均表现出和环带结构相联系的空间分布变化。斜长石斑晶中最主要的结构为韵律环带以及熔蚀结构,所测定的矿物边缘都存在An值从由内向外迅速降低的致密韵律环带,可能反映了快速结晶时的不平衡;而晶体内部的稀疏韵律环带结构是由岩浆填充或对流活动导致的。部分斜长石的熔蚀层An值由内向外升高,反映了高Ca岩浆填充的过程。这说明斜长石斑晶的矿物形态和元素环带可以用来制约俯冲带海底火山岩浆从源区上升到岩浆房再到喷发的复杂过程,包括岩浆演化、熔体多次填充、熔体与结晶矿物之间的反应、以及矿物再熔融等。这对于理解海底火山的喷发以及岛弧岩浆岩的演化有重要意义。 相似文献
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本文利用电子探针和背散射电子成像技术系统地研究了新疆阿尔泰可可托海3号伟晶岩脉各结构带中的铝铁矿族矿物。研究表明,本区伟晶岩脉中铌铁矿族矿物主要为铌锰矿-钽锰矿。成分特征显示从岩脉边部带到核部,Ta/(Nb Ta)比值呈近垂向演化,但Mn/(Fe Mn)比值没有明显变化。另一方面,铌铁矿族矿物在早期正岩浆阶段(Ⅰ-Ⅳ带)的成分变化非常局限,而在晚期的岩浆-热液过渡阶段(Ⅴ-Ⅶ带)的成分变化非常大。背散射电子成像技术观察还表明本区铌铁矿族矿物在正岩浆阶段没有环带构造特征,而在岩浆-热液过渡阶段有明显的环带构造特征,而且随着伟晶岩固结过程的进行,环带构造主要沿着渐变环带构造→韵律环带构造→交代构造的趋势变化。研究认为,本区铌铁矿族矿物在不同结构带的成分变化和在单颗粒中的环带构造是热液流体参与铌铁矿族矿物结晶的反应,环带构造的类型主要是由热液流体参与结晶的程度所控制。 相似文献
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冀西北姚家庄存在一套晚三叠世的超镁铁岩-正长岩杂岩体,岩体内发育具有环带特征的单斜辉石。辉石的环带有两种:简单环带和复杂环带。简单环带一般为正环带,辉石核部的MgO和Cr2O3含量高,Si O2、Fe O和Na2O含量低;边部的主要氧化物含量与核部刚好相反。简单正环带可以分为两类,其中核边接触带平滑、由核到边化学成分具有渐变特征的正环带辉石可能是岩浆在分离结晶或地壳混染过程中形成。而核边接触带有熔蚀结构、由核到边化学成分突变的正环带辉石可能是早期结晶的辉石颗粒受到晚期低镁岩浆的溶蚀改造而成的。复杂环带具有核-幔-边结构,其中,核部低镁高铁、幔部高镁低铁、边部与核部相似,但其Mg#更低,这些特征暗示了岩浆混合作用的存在,形成辉石核部的母岩浆可能来自富集的岩石圈地幔,幔部高Mg#的特征指示了软流圈地幔物质的贡献,其边部低Mg#的特征则指示了地壳物质的加入。具有韵律环带的复杂辉石是在岩浆多期侵入的过程中形成的。辉石环带的组成特征表明,姚家庄杂岩体是由岩浆多期侵位形成的,后期侵入的岩浆与前期就位的岩浆不断反应,形成了具有多种不同环带特征的辉石,并最终形成了空间上由外到内依次为辉石岩、辉石正长岩和正长岩的环状杂岩体。结合前人的研究成果,推测形成姚家庄岩体的岩浆主要来源于富集的岩石圈地幔,并由少量地壳组分和软流圈物质的贡献。 相似文献
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藏北戈木错渐新世碱性钾质火山岩中单斜辉石斑晶普遍出现正环带、反环带和韵律环带结构,多具有"绿核辉石"的结构特征。通过矿物电子探针测得"绿核辉石"的核部有高Mg#和低Mg#两种不同成分,两者都不同程度发育有筛孔状熔蚀结构,环带结构主要发育在辉石的幔部到边部,与绿色核部存在明显的成分间断,幔部环带结构的成分变化范围相对较窄。"绿核辉石"的成分和结构特征反映了同源碱性钾质岩浆在壳内岩浆房中发生了岩浆补给-混合作用,复杂的环带结构记录了混合岩浆的结晶过程。 相似文献
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《地球化学》2015,(4)
青海省祁漫塔格-都兰成矿带是以铁铜多金属为主的成矿带,其矿产丰富但研究程度较低。双庆铁矿床是该成矿带上的典型矿床,目前尚未对其金属硫化物开展地球化学研究。本文运用电子探针测试手段,分析金属硫化物地球化学特征,结合闪锌矿标型特征研究,以期为矿床中金属硫化物生成环境提供指示意义。基于金属硫化物的电子探针分析结果,通过计算其标准化学式可知,其平均化学式的S元素比例逐渐减弱,表明对应矿物生成的还原环境在逐渐减弱。闪锌矿的Zn/Fe比值、Zn/Cd比值及闪锌矿地质温度计结果表明属于中-高温型闪锌矿。再结合闪锌矿流体包裹体均一温度测试结果,证实与中-高温型闪锌矿吻合。 相似文献
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青藏米巴勒地区中新世钠质方沸石(霞石)响岩中单斜辉石环带研究:对岩浆-构造演化的启示 总被引：5，自引：3，他引：2
在拉萨地块中部米巴勒地区产出的中新世钠质方沸石(霞石)响岩中的单斜辉石发育大量环带结构,环带结构包括正环带、反环带和韵律环带。其中正环带结构从核部到边部Mg#、MgO、Cr2O3呈逐渐降低趋势,而FeO、Na2O、Al2O3、TiO2呈逐渐升高的趋势,它反映了岩浆正常结晶的历史。反环带结构中Mg#、MgO、Cr2O3从核部到边部呈升高的趋势,FeO、Na2O、Al2O3的含量总体上呈降低趋势,本文认为响岩中单斜辉石的这种环带结构是受到了和它共存的钾质-超钾质火山岩岩浆混合或混染所致,两种岩石应是各自独立的母岩浆的结晶产物。具韵律环带结构的单斜辉石从核部到边部出现成分规律性波动,Na2O、Al2O3、TiO2、Cr2O3含量的变化在正反环带的范围内,Mg#值的变化范围较小,在正环带斑晶和基质的范围内,它是岩浆多次混合作用的结果。该地区钠质过碱性岩的出现可能指示青藏高原在这套火山岩喷发时(13~12Ma),构造体制发生了显著的改变,进入到一个典型的陆内伸展阶段。 相似文献
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月壤颗粒微观环带的太空风化成因 总被引：2，自引：0，他引：2
太空风化是迄今31亿年以来影响月球表面物质演化过程的主要因素,主要包括陨石、微陨石的轰击,太阳风粒子的注入,太阳/银河宇宙射线的辐射以及周期性的加热作用等。通过深入剖析太阳风粒子的注入与溅射、微陨石轰击的蒸发与沉积、宇宙射线辐射的辐射损伤等过程的作用机理,探讨了不同太空风化过程对矿物颗粒环带厚度、化学组成、晶体结构等特征的影响,认为微陨石轰击与太阳风注入是形成月壤颗粒微观环带的主导因素,宇宙射线辐射与周期性加热的影响可忽略不计。进一步结合非晶质环带、富内含物环带、多环环带以及小泡环带等月壤颗粒主要环带的基本特征,在总结和对比分析各类型环带的厚度、结构以及化学组成特征基础上,对不同类型环带的成因进行初步推断,认为非晶质环带、小泡环带以及多环环带的内层环带具有太阳风作用特征,而富内含物环带、多环环带的外层环带则具有微陨石轰击的成因特征。根据目前单纯依靠环带的化学组成分析解释环带成因存在的不足,指出了通过补充分析矿物晶体结构在模拟太空风化实验过程中的变化特征来研究环带成因的新思路。 相似文献
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闪锌矿是在热液型金属矿床中最常见的金属矿物之一。世界各地已经有很多关于描述闪锌矿化学成分的文献。电子探针显微分析仪在闪锌矿的分类中,被认为是一种鉴定闪锌矿中主要元素,微量元素含量的很有用的技术工具。闪锌矿中FeS组分的含量被建议作为判断成矿过程中硫逸度的灵敏标志,并获得成功的应用。当闪锌矿与六方晶系的磁黄铁矿,黄铁矿共生的时候,其内部FeS组分的含量还是一种很有用的地质压力计。 相似文献
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Trace Elements and Rare Earth Elements of Sulfide Minerals in the Tianqiao Pb-Zn Ore Deposit, Guizhou Province, China 总被引：2，自引：0，他引：2
ZHOU Jiaxi HUANG Zhilong ZHOU Guofu LI Xiaobiao DING Wei BAO Guangping 《《地质学报》英文版》2011,85(1):189-199
Trace elements and rare earth elements (REE) of the sulfide minerals were determined by inductively-coupled plasma mass spectrometry. The results indicate that V, Cu, Sn, Ga, Cd, In, and Se are concentrated in sphalerite, Sb, As, Ge, and Tl are concentrated in galena, and almost all trace elements in pyrite are low. The Ga and Cd contents in the light-yellow sphalerites are higher than that in the brown and the black sphalerites. The contents of Ge, Tl, In, and Se in brown sphalerites are higher than that in light-yellow sphalerites and black sphalerites. It shows that REE concentrations are higher in pyrite than in sphalerite, and galena. In sphalerites, the REE concentration decreases from light-yellow sphalerites, brown sphalerites, to black sphalerites. The ratios of Ga/In are more than 10, and Co/Ni are less than 1 in the studied sphalerites and pyrites, respectively, indicating that the genesis of the Tianqiao Pb–Zn ore deposit might belong to sedimentary-reformed genesis associated with hydrothermal genesis. The relationship between LnGa and LnIn in sphalerite, and between LnBi and LnSb in galena, indicates that the Tianqiao Pb–Zn ore deposit might belong to sedimentary-reformed genesis. Based on the chondrite-normalized REE patterns, δEu is a negative anomaly (0.13–0.88), and δCe does not show obvious anomaly (0.88–1.31); all the samples have low total REE concentrations (<3 ppm) and a wide range of light rare earth element/high rare earth element ratios (1.12–12.35). These results indicate that the ore-forming fluids occur under a reducing environment. Comparison REE compositions and parameters of sphalerites, galenas, pyrites, ores, altered dolostone rocks, strata carbonates, and the pyrite from Lower Carboniferous Datang Formation showed that the ore-forming fluids might come from polycomponent systems, that is, different chronostratigraphic units could make an important contribution to the ore-forming fluids. Combined with the tectonic setting and previous isotopic geochemistry evidence, we conclude that the ore-deposit genesis is hydrothermal, sedimentary reformed, with multisources characteristics of ore-forming fluids. 相似文献
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《矿物学报》2013,(Z1)
Optical cathodoluminescence microscopy (CLM) can provide very useful information both on mineral zoning formed during crystal growth and on variations in chemical composition of sphalerites which is reflected by their visible colors. Gem quality sphalerite crystals associated with dolomite, calcite and fluorite having 3 different visible colors - green, honey and brown - were studied to compare their mineral chemistry and CL characteristics. Electron microprobe analyses indicated essentially no significant differences in terms of major components. Although the common CL-quencher ferrous iron contents of all three were lower than 0.25 wt %, none of the sphalerites cathodoluminescenced: two (brown and honey) were non-CL, the green sphalerite showed very week CL in faint brown color. Other trace elements that were analyzed include Fe, Cd, Mn, Ag, Hg, In, Bi, Cu, Ge, and Ga. Fe, Cd, Ga and Cu were relatively higher than the others. Most significant differences with respect to the common trace elements include honey colored sphalerites are essentially Fe- and Cd-poor but rich in Ga, green sphalerites are Fe- and Cd- rich but poor in all the others, and brown sphalerites are rich in Cd. No conclusive relation between non-CL behavior of all three sphalerites and their trace element chemistry was established, however; low quantities of common CL activators in sphalerite crystal structures such as Mn, Cu, and In were the main cause of the non-CL behavior. 相似文献
13.
西藏罗布莎豆荚状铬铁矿中发现超高压矿物柯石英 总被引：18，自引：0，他引：18
在西藏雅鲁藏布江蛇绿岩带东段的罗布莎豆荚状铬铁矿床中发现典型的超高压矿物柯石英和蓝晶石, 二者呈针柱状交生, 产在一个以TiFe合金成分为主的颗粒(0.7mm× 0.5mm大小) 的最外部.该颗粒从内到外由4层矿物组成, 分别为TiFe合金主体、2 0~ 70 μm宽的自然钛、约10 μm宽的TiSi合金及30~ 5 0 μm宽的柯石英和蓝晶石为主的硅酸岩和氧化物层.主体矿物为高Ti低Fe的TiFe合金, 内部出现由细粒状低Ti高Fe的TiFe合金和自然钛组成的蠕英结构.最外层由柯石英和蓝晶石组成的格架中分布细粒的Si金红石和Ti-Mg -K -Na -Ca氧化物.初步认为TiFe合金从深部高温高压环境往浅部上升过程中, 内部发生局部熔融, 分解出自然Ti, 并在其边部与其他硅酸岩矿物或熔体发生反应, 形成柯石英和蓝晶石.这一过程可能发生在洋脊拉张环境, 由于地幔柱的上涌, 将深部的豆荚状铬铁矿带到浅部, 使得其中包裹的一些高温高压环境下稳定的矿物变得不稳定, 发生熔融和交代反应, 形成新的不平衡的矿物组合.罗布莎柯石英的这种不寻常产出特征说明是在减压过程中形成, 不同于造山带中常见的由板块俯冲增压过程中形成的柯石英 相似文献
14.
Chuanwei Zhu Hanjie Wen Yuxu Zhang Zhilong Huang Christophe Cloquet Béatrice Luais Tao Yang 《地学前缘(英文版)》2021,12(6):162-170
The Sichuan-Yunnan-Guizhou(SYG)Zn-Pb metallogenic zone in SW China contains＞400 carbonate-hosted hydrothermal Zn-Pb deposits.Some of these,such as the Huize,Tianbaoshan,and Daliangzi deposits,are super-large deposits with significant reserves of Cd,Ge,and Ag.However,the sources of these metals remain controversial.This study investigated the Cd isotopic geochemistry of the Huize deposit,the largest Zn-Pb deposit in the SYG area.Sphalerites formed at three stages in the deposit have different colors:black or dark brown(Stage Ⅰ),red(Stage Ⅱ),and light-yellow(Stage Ⅲ).The δ114/110Cd values of the sphalerites are in the order Stage Ⅲ＜Stage Ⅰ＜Stage Ⅱ.Kinetic isotopic fractionation is likely the key factor causing the lower δ114/110Cd values in the early formed Stage Ⅰ sphalerites than in later-formed Stage Ⅱ sphalerites,with cooling of ore-forming fluids being responsible for the still lower values of the Stage Ⅲ sphalerites.In galena,the δ114/110Cd values are inversely correlated with Cd contents and tend to be higher in high-Zn galena.We speculate that Cd isotopic fractionation was significant during the precipitation of sphalerite and galena,with light Cd isotopes being enriched in galena rather than sphalerite.Comparison of the Cd isotopic signatures and Zn/Cd ratios of different endmembers suggests that the δ114/110Cd values and Zn/Cd ratios of sphalerite from the Huize deposit,as well as other large-scale deposits from the SYG area,are lie in those range of Emeishan basalts and sedimentary rocks and the mean δ114/110Cd values of these deposits show good negative correlation with 1/Cd,suggesting that the ore-forming materials of these deposits were derived from the mixing of Emeishan basalts and sed-imentary rocks.This study demonstrates that Cd isotopes can be useful proxies in elucidating ore genesis in large Zn-Pb deposits. 相似文献
15.
《International Geology Review》2012,54(9):1388-1395
A consistent, relatively rapid decrease in FeS molecular content of sphalerites at decreasing depth is recognizable in upper parts of this structurally controlled Pb-Zn ore deposit, as an expression of tectonic calm and continuity of the productive stages of the mineralization. Elsewhere, in the depths, abrupt changes in quantity of isomorphous iron in sphalerites, within a relatively short depth-span, signify intensive movements during deposition of the ore. Wherever the structures are bent and healed by early quartz sufficiently to retard circulation of the solutions and to promote their cooling, variations in the FeS content of sphalerite at different depths may be related to thermal “knickpoints” of the ascending solutions. Nonetheless, FeS molecular content of sphalerites is no clue to the temperature of their crystallization. There is no relationship between the depth at which sphalerite was formed and the isomorphous Cd or Mn in crystal structures of the mineral. — V.P. Sokoloff. 相似文献
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17.
Song Xuexin 《Mineralium Deposita》1984,19(2):95-104
The Fankou Pb-Zn deposit occurs in the Middle-Upper Devonian and Lower Carboniferous carbonate and argillaceous carbonate formations. In principle, the deposit can be classified as a carbonate-hosted strate-bound deposit. Representative sphalerite, galena, and pyrite separates from Fankou have been analysed. For the purpose of comparison a literature survey on minor elements of other districts have been carried out. The comparison of determined data with the quoted data shows that the Fankou sphalerites are rich in Ga, Ge and Ag, but poor in Se and Te; the Fankou galenas are rich in Ag, Hg, Sb and As, but poor in Se, Te, Tl and Bi; the Fankou pyrites are rich in As, Cd and In, but poor in Se, Te, Co and Ni. Zn/Cd and Se/S×10–4 ratios for sphalerites, Sb/Ag, Sb/Bi and Se/S×10–4 ratios for galenas and Co/Ni ratios for pyrites from Fankou and other districts have been calculated. Ga-Ge-Ag atomic ratios in sphalerites, Sb-Bi-Ag atomic ratios in galenas and Co-Ni relations in pyrites have been plotted. The average value (311) of Zn/Cd ratios for sphalerites from Fankou is similar to values of sphalerites from Gaobanhe, Heqing, Accesa and Broken Hill. The average Sb/Ag ratio (0.74) and the Sb-Bi-Ag atomic ratios in Fankou galenas are similar to those in the syngenetic galena from the British Island. The Ga-Ge-Ag atomic ratios for Fankou sphalerites are similar to those for the syngenetic sphalerites and Gorno sphalerites. The average Co/Ni ratio (1.1) for micro to fine-grained pyrites from Fankou laminated-bedded pyrite ore is similar to that (0.8) for the sedimentary pyrites from other districts. As to the fine to medium-grained pyrites from Fankou massive pyritic ores, their higher Co/Ni ratios (1.6–1.8) may relate to the fact that more Ni is lost than Co, during the reformation or recrystallization. Sphalerite, galena and pyrite from Fankou all are rather poor in Se and have very low values of Se/S×10–4, so they may bear no genetic relation to volcanism. To sum up, the following conclusions can be reached: (1) The Fankou deposit possesses some syngenetic features. (2) Evidently it differs from skarn type, hydrothermal type, and volcanogenic type deposits. (3) Surely it is a reformed sedimentary Pb-Zn deposit. 相似文献
18.
曹四夭斑岩钼矿床位于内蒙古兴和县,是华北克拉通北缘最大的钼矿床。该矿床中部发育斑岩型钼矿体,外围和上部产出热液脉型铅锌金矿体。文章选取1件与斑岩钼矿化共生的绢云母样品进行了40Ar-39Ar定年,获得40Ar-39Ar坪年龄为(144.4±1.2)Ma,相应的39Ar/36Ar-40Ar/39Ar等时线年龄为(146.4±2.2)Ma(MSWD=0.31),将等时线年龄认作绢云母的Ar封闭年龄,表明曹四夭斑岩钼矿化发生在约146 Ma前。选取14件脉型铅锌矿石中的闪锌矿、黄铁矿和磁黄铁矿样品开展了Rb-Sr定年,获得4件闪锌矿的Rb-Sr等时线年龄为(145.1±3.0)Ma(MSWD=0.63);5件黄铁矿的Rb-Sr等时线年龄为(145.2±1.3)Ma(MSWD=0.53);4件闪锌矿、5件黄铁矿和1件磁黄铁矿的Rb-Sr等时线年龄为(145.3±1.0)Ma(MSWD=0.43)。硫化物Rb-Sr定年结果表明曹四夭矿床脉型铅锌矿化形成于约145 Ma前。本次绢云母40Ar-39Ar和硫化物Rb-Sr定年结果表明,曹四夭矿床斑岩型钼矿化和脉型铅锌金矿化为同期产物,两者均形成于晚侏罗世末期,属于同一个斑岩成矿系统。曹四夭矿床硫化物的w(Rb)和w(Sr)分别为0.1867×10~(-6)~1.305×10~(-6)和0.3175×10~(-6)~6.935×10~(-6),Sr同位素初始比值(87Sr/86Sr)i介于0.709 919~0.711 951之间,平均值0.710 952,结合前人获得的辉钼矿Re含量,认为曹四夭矿床的成矿物质主要来源于地壳。 相似文献
19.
塔里木盆地下奥陶统白云岩化流体来源的地球化学分析 总被引：9，自引：0，他引：9
塔里木盆地是中国重要的含油气盆地,其中奥陶系白云岩是主要储层之一,然而有关白云岩成因的问题众说纷纭,其中的关键是对于白云岩化流体性质的认识不一。元素地球化学和同位素测试分析表明,白云岩的稀土元素来源大部分继承原始灰岩,具有与海水类似的配分特征,只不过稀土元素的含量明显增高了;Sr、Ti含量和Sr/Ba比值较高,且Sr和Mn都具典型的埋藏演化特征;碳、氧同位素分布于正常海相范围内,与典型的埋藏白云岩特征类似;在局部发育一些与断裂相关的铁(锰)白云岩和鞍状白云岩,显示明显的Eu正异常,具相对较高的Fe-Mn-Ba-Si(-Zn-Pb)元素含量及Sr/Ba比值。分析结果说明塔中和塔北下奥陶统的白云岩化流体主要为正常或浓缩了的海水,白云岩形成于准同生和/或埋藏环境,局部发育与断裂相关的热液白云岩,而前人强调的大气淡水或混合水作用对白云岩的形成并不重要。 相似文献
20.
Minor elements in sphalerite and galena from Binnatal 总被引：1，自引：0，他引：1
Stefan Graeser 《Contributions to Mineralogy and Petrology》1969,24(2):156-163
The trace element contents of 23 sphalerites and galenas from Binnatal, Switzerland, have been determined. Most of these samples have been previously studied in respect to lead and sulphur isotope abundances. Coloration of sphalerites — varying from yellow to black for nearly identical iron contents — seems to be strongly influenced by the manganese content. A linear relationship between sulphur isotope composition and copper content in sphalerites was found. Trace elements in galenas show a significant inverse relationship between silver and copper. With the determination of the bismuth content, it is possible to distinguish several galena types; a similar grouping has been found by lead isotope determinations. The results of the trace analyses are discussed in connection with the occurrence of a large number of very rare and special Pb-As-sulphosalt minerals in the Binnatal dolomites. 相似文献