内蒙古黄岗锡铁矿床夕卡岩矿物学特征及其成矿指示意义   总被引：5，自引：1，他引：4       下载免费PDF全文

周振华  刘宏伟  常帼雄  吕林素  李涛  杨永军  张瑞军  纪显合 《岩石矿物学杂志》2011,30(1):97-112

为进一步查明黄岗锡铁矿矿床成因、夕卡岩矿物成分与金属矿化类型之间的联系,利用电子探针对研究区主要夕卡岩矿物的化学成分进行了详细的分析。测试结果表明,成矿早期石榴石的端员组分以钙铁榴石为主,主成矿期石榴石的端员组分以钙铝榴石为主;辉石端员组分变化较大,主要为透辉石和钙铁辉石。石榴石和辉石的矿物组分分别为Adr28.69～96.44Grs2.00～67.38(Prp+Sps)0.67～5.69和Di11.8～94.12Hd4.08～81.28Jo1.79～20.02,其较大的成分变化特征反映出夕卡岩不是在一个完全封闭的平衡条件下形成的。角闪石大多为镁铁钙角闪石,个别属于铁角闪石,成分变化较大的原因可能是由于氧化还原条件改变导致不同程度的AlⅥSi←→(Na,K)的置换作用,属于一种固相线下的转变。角闪石中四次配位的Si、Al及六次配位的Al、Ti和A位置的阳离子数变化范围很大,可能是由于接触交代作用过程中岩浆的成分差异或结晶时的物理化学条件改变所引起的。富锰的辉石夕卡岩是岩浆流体顺层间破碎带渗滤交代形成的,富锰辉石可作为本区寻找Sn、Cu、Zn等多金属的找矿标志,外接触带夕卡岩和其附近的大理岩中是多金属成矿的有利部位。  相似文献   

乳腺炎症及增生症病灶中钙化的矿物学研究     

熊翠娥  王长秋  鲁安怀  李艳  梅放  柳剑英 《岩石矿物学杂志》2011,30(6):1014-1020

选取9例乳腺炎症、7例乳腺增生的钙化样品,利用光学显微镜(OM)、环境扫描电镜(ESEM)、微区X射线衍射(μ-XRD)等矿物学分析方法对样品进行了原位形貌观察、分离后结构及成分的测试分析,探讨了病灶中钙化的矿物学特征及其组成成分和形成机制。研究结果表明,发生在炎症病灶中的钙化主要类型是脂肪坏死后的钙化,其发生和死亡的脂肪细胞和周围病变后期修复性Ⅲ型胶原有直接关系。增生症中的钙化主要有发生在扩张的导管内和在束状深度交联胶原中的坏死型钙化,扩张的导管边缘处Ⅳ型胶原和大片变性Ⅲ型胶原为钙化提供了成核位点,继而参与无机矿物的形成过程,最后形成较为致密的钙化。乳腺炎症和增生症中的钙化的主要成分均为碳羟磷灰石。  相似文献   

A Systematic Spectroscopic Study of Four Apollo Lunar Soils     

凌宗成  Bradley L Jolliff 《中国地质大学学报(英文版)》2011,(5)

A systematic spectroscopic study including Raman,Mid-IR,NIR,and VIS-NIR,is used to investigate four endmember lunar soils.Apollo soils(<45 μm) 14163,15271,67511,and 71501 were selected as endmembers to study,based on their soil chemistry,maturity against space weathering,and the sampling locations.These endmembers include an anorthositic highlands soil(67511),a low-Ti basaltic soil(15271) ,a high-Ti basaltic soil(71501),and a mafic,KREEPy,impact-melt-rich soil(14163) .We used a laser Raman point-counting pr...  相似文献   

湖南宝山铅锌矿西部矿带银的工艺矿物学研究   总被引：3，自引：3，他引：0  

彭艳华  彭光菊  贾利攀  周卫宁 《岩矿测试》2013,32(5):729-737

湖南宝山铅锌矿西部矿区为中低温热液裂隙充填交代型铅锌银矿床。本文对该矿带银的工艺矿物学进行系统研究,利用多种现代分析技术手段,查明矿石中银的主要矿物种类、赋存状态和工艺特征。化学分析结果确定矿石中银的平均品位为156.6×10^-6;地质小样化学分析统计显示银含量在空间上呈现上部高、下部低,平面上北西和南西部较北东和南东高的特征;白云岩型、砂岩型、灰岩型、角砾岩型矿石的银平均含量分别为595.78×10^-6、247.97×10^-6、195.83×10^-6、169.73×10^-6,白云岩型矿石的银含量最高,角砾岩矿石的银含量最低;银与方铅矿关系密切,银和铅二者的含量总体表现出良好的趋同性,据此可预测高品位的铅矿石的银含量高。对光片进行显微镜下鉴定、扫描电镜以及电子探针分析,确定矿区的金属矿物主要是方铅矿、闪锌矿、黄铜矿和黄铁矿,初步查明矿石中的银矿物主要是银黝铜矿,其次是含银砷黝铜矿和含银方铅矿;该矿床银的存在形式主要有两种:一种是以独立矿物——银黝铜矿形式存在,这部分银含量为10.179%~13.579%,银的平均含量为12.061%;另一种是赋存于方铅矿中,这部分银含量为0.011%~0.127%,银的平均含量为0.069%。经银的物相分析、单矿物银含量分析和平衡配分计算,揭示银黝铜矿虽然含有较高品位的银,但因矿物含量较少,银的平衡配分低;方铅矿的银含量不高,但由于矿物含量高,平衡配分率达到84.78%,因此成为银的主要载体矿物。筛析实验也发现银与铅有较好的趋同性,进一步印证了银的主要载体矿物是方铅矿,并且银在细粒级中含量偏高。本研究提出,在选矿过程中要提高银的回收率,应重视细粒级中主金属元素铅、锌的回收。  相似文献   

西藏嘎拉勒铜金矿床地质特征及矽卡岩矿物学特征研究   总被引：2，自引：0，他引：2  

张志  陈毓川  唐菊兴  何林  姚晓峰  杨毅  胡正华  王红星  宋俊龙 《矿床地质》2013,32(5):915-931

嘎拉勒铜金矿床位于班公湖-怒江缝合带西段,是该带上新近发现的十分重要的矽卡岩(斑岩)型铜金矿床,其金资源量已达大型以上规模。矿区内出露地层有白垩系朗久组及捷嘎组,并发育大量燕山期中酸性侵入岩。矿体主要产于灰白色花岗闪长岩与白云岩或白云质大理岩的接触带矽卡岩内。矽卡岩主要呈层状、似层状、港湾状及不规则状等产出;矽卡岩矿物主要为橄榄石、蛇纹石、辉石、金云母、透闪石、绿帘石、水镁石等;靠近内接触带可见石榴子石;金属矿物主要有磁铁矿、自然金、黄铜矿、斑铜矿、辉铜矿、辉钼矿等。电子探针分析表明,矿区内矽卡岩矿物中的橄榄石主要为镁橄榄石,辉石主要为透辉石,云母主要为金云母,由此构成的矽卡岩矿物组合为典型的镁质矽卡岩;与之伴生的钙质矽卡岩矿物石榴子石主要为钙铁榴石。矿区中的矽卡岩在空间上具有较好的分带性,其表现为从内接触带至外接触带经历了镁橄榄石-透辉石相至金云母-透闪石相的渐变过渡演化,表明矿区矽卡岩具有从高温至低温的矿物组合演化序列;与矽卡岩分带相伴随的矿化分带,表现为深部的铜(钼)矿化过渡到浅部的铜金矿化。矿区最新勘查成果显示,在深部已发现少量斑岩型矿化,显示存在统一的矽卡岩-斑岩成矿系统的可能性,深部找矿潜力较大。  相似文献   

新疆包古图金矿四矿区L7号脉中的特殊矿物组合及其成矿意义   总被引：3，自引：3，他引：0  

郑波  张晋国  陈刚  朱永峰 《矿床地质》2013,32(6):1117-1138

包古图金矿四矿区L7号脉由浅部的自然砷-石英脉型矿石和深部的辉锑矿-石英脉型矿石组成。矿脉中含罕见的As、Sb矿物,如paakkonenite（Sb₂AsS₂）、自然砷、自然锑、方锑金矿、硫锑金银矿（Au₃Ag₄Sb₁₀S₁₂）等。热液过程划分为5个阶段：黄铁矿-毒砂阶段（Ⅰ）,围岩中形成大量的毒砂和黄铁矿并伴随较强硅化;粗粒石英阶段（Ⅱ）,形成沿围岩壁或围岩角砾的梳状石英;Au-As-Sb矿化阶段（Ⅲ）,形成辉锑矿-自然锑-自然砷-paakkonenite-银金矿-自然金-方锑金矿-硫锑金银矿-辉锑银矿-银锌黝铜矿-斜方砷铁矿-硫铜锑矿-石英;晚期Sb矿化阶段（Ⅳ）,形成与粒状方解石共生的辉锑矿、自然锑和paakkonenite;方解石阶段（Ⅴ）,形成穿切矿体和围岩的方解石（-石英）细脉。辉锑矿和斜方砷铁矿交代毒砂,自然金、方锑金矿、paakkonenite和自然砷交代辉锑矿。辉锑矿的结晶主要受温度和还原S含量的控制,自然砷、自然锑的结晶主要受氧逸度和温度控制。As、Sb分别以自然砷、辉锑矿和自然锑形式存在,同时消耗大量H₂S,流体进入张性空间后也释放H₂S,导致硫逸度急剧降低,含Au络合物失稳而成矿。  相似文献   

The origin of tin deposits in the Mount Wells region,Pine Creek Geosyncline,Northern Territory     

M. Ahmad 《Australian Journal of Earth Sciences》2013,60(5):427-443

Tabular steeply dipping cassiterite‐bearing lodes in the Mount Wells region are hosted by lower greenschist fades metasediment of the Pine Creek Geosyncline within the contact aureole of late orogenic granitoids. The latter are predominantly I‐type, but S‐type phases are developed near the sediment‐granitoid contact.

Quartz, cassiterite, pyrite, arsenopyrite, chalcopyrite and pyrrhotite are the main minerals. Two types of lodes are present: (i) Sn‐quartz lodes containing 5–10 vol% sulphide minerals; and (ii) Sn‐sulphide lodes containing ～ 70 vol% sulphide minerals. At the surface, the former appear as normal quartz veins and the latter as hematite‐quartz breccia resulting from the collapse of original sulphide‐rich lodes as a consequence of volume reduction due to oxidation and leaching.

Two stages of quartz veining are recognized in both types of lodes. Cassiterite is present in stage I while stage II is composed of barren quartz with minor pyrite. Late stage III carbonate veinlets are present in Sn‐sulphide lodes. The lode‐wallrock contact is sharp with weak alteration effects confined to the fringe of the lodes. The alteration minerals include sericite, quartz, tourmaline, chlorite, pyrite and minor K‐feldspar.

Four types of fluid inclusions are present in vein quartz and cassiterite: Type A (CO₂ ± H₂O ± CH₄); Type B (H₂O+～ 20% vapour); Type C (H₂O+ < 15% vapour) and Type D (H₂O+ < 15% vapour + NaCl). Early ‘primary’ inclusions represented by Types A and B are present in stage I only and have a well‐defined temperature mode at ～300°C and a salinity range of 1–20 wt% eq NaCl. Types C and D inclusions are ‘secondary’ in stage I and primary in stage II and have a temperature mode at 120–160°C and salinities from about 1 to more than 26 wt% eq NaCl. Variable H₂O‐CO₂ ratios of Type A inclusions and homogenization in CO₂ or H₂O phase at near identical temperature indicate entrapment at the H₂O‐CO₂ solvus and define a pressure of ～ 100 MPa. The melting sequence of frozen inclusions suggests that the ore fluids were mainly H₂O‐CO₂‐CH₄‐Na‐Ca‐Cl brines. This is also confirmed by Raman Laser Spectrometry.

Oxygen and sulphur isotope data are consistent with a magmatic origin of the ore fluids. The δD values are up to 20%0 higher than those expected for magmatic fluids and probably resulted from interaction of the latter with the carbonaceous strata. This interpretation is supported by δ¹³C data on the fluid inclusion CO₂.

Fluid inclusions, stable isotope and mineralogical data are used to approximate the physico‐chemical parameters of the ore fluids which are as follows: T 300°C, m Cl～2, fO₂ ～ 10^‐35, mSS ～ 0.01, Sn ～ 1 ppm, Cu ～ 1 ppm and pH ～ 5.5.

It is suggested that fluids of granitic parentage interacted with the enclosing sediment and picked up CO₂, CH₄ and possibly Ca. The granitic phases became reduced due to this interaction and developed S‐type characteristics. Tin was probably partitioned into the CH₄‐bearing reduced fluids. At some stage the fluid overpressure exceeded the lithostatic lode enforcing failure of the carapace and the intruded rocks by hydraulic fracturing causing CH₄ and CO₂ loss resulting in the precipitation of the ore minerals.  相似文献   

Mineralogical and Geochemical Constraints on the Genesis of the Carbonate‐Hosted Jebel Ghozlane Pb–Zn Deposit (Nappe Zone,Northern Tunisia)     

Nejib Jemmali  Fouad Souissi  Emmanuel John M. Carranza  Torsten W. Vennemann 《Resource Geology》2013,63(1):27-41

The Pb–Zn deposit at Jebel Ghozlane, in the Nappe zone (northern Tunisia), is hosted by Triassic dolostones and Eocene limestones and is located along faults and a thrust‐sheet boundary. The sulfide mineralization of the deposit consists mainly of galena and sphalerite and occurs as vein, stockwork, breccia, dissemination and replacement ores. Three hydrothermal stages are involved in the formation of the ores: stage I is dominated by celestite‐barite, hydrothermal dolomite DII, colloform sphalerite, and galena I; stage II consist of galena II; and stage III contains calcite. Galena in the deposit yielded average ²⁰⁶Pb/²⁰⁴Pb, ²⁰⁷Pb/²⁰⁴Pb and ²⁰⁸Pb/²⁰⁴Pb ratios of 18.705, 15.667 and 38.734, respectively, suggesting a single upper crustal source reservoir for metals. Trace element data indicate the presence of Zn‐ and As‐free galena and As‐rich galena (with 0.2–0.5% As). Sphalerite contains 0.4% As, 0.7–0.9% Cd and 0.1–1.5% Fe. Microthermometric analysis of fluid inclusions in celestite shows that the deposit formed from fluids composed of heterogeneous mixtures of saline (19.5 ± 1 wt% NaCl eq.) aqueous solutions sourced from basinal brines, and gaseous CO₂‐rich phases bearing low amounts of CH₄, N₂ and/or H₂S, at temperatures of 172 ± 5°C.  相似文献   

具磷灰石假象绿松石的岩石矿物学及谱学特征     

申广耀  卢保奇  亓利剑 《上海国土资源》2013,(4):96-100

采用x射线粉晶衍射（XRD）、博里叶变换红外光谱（FTI码以及拉曼光谱等方法对安徽马鞍山具磷灰石假象的绿松石进行了研究。结果表明：其主要矿物组成为绿松石,保留了磷灰石六边形的形态特征。XRD~U试的特征谱线d值为36745～36748（111）、29008～29025（123）、34247～34293（2101、32709～32781（113）、61626～61781（011）3020130～20162（301）,与绿松石的标准衍射谱线基本致。红外光谱测试分析表明：3510～3465cm。间的谱带归属绿松石0（OH）的伸缩振动,3300～3070cm’间的谱带归属为绿松Nu（M-H。O）伸缩振动,1210-1012cm’间的谱带归属为绿松石U3口O。）ira缩振动,在838cm。附近的吸收谱带归属为绿松石6（OH）弯曲振动,655-480cm。间的谱带归属为绿松石u4（P04）弯曲振动。拉曼光谱测试分析表明：3466cm’附近的尖锐拉曼谱峰归属于绿松石（OH）基团的伸缩振动所致,宽缓的拉曼谱峰3281cm’~03078cm’归属于绿松石中水合络离子的伸缩振动,798cm’谱峰则是由于OH的弯曲振动所致。  相似文献   

实验矿物学方法研究进展     

雷洁  王金荣  赵磊 《甘肃地质》2013,22(1):90-93

基于3S技术的数字填图RGMAP区域地质调查技术实现了区域填图中数据采集的全过程信息化,其中背景图层数据参数的正确调整是数字化区调项目野外各项工作顺利开展的前提。本文根据笔者在数字填图技术应用中得切身体会,对背景图层参数不规范,比例尺不统一及路线或剖面导入后无法正常显示等常见问题的解决方法进行了较为详细的介绍。  相似文献