曾家垅含锡矿物特征及地质意义

作者通过对曾家垅含锡矿物特征及赋存状态的分析认为，曾家垅含锡独立矿物以锡石为主，次为马来亚石及黄锡矿。在华南锡成矿带中，马来亚石的矿物组合在曾家垅锡矿床中首次发现，读矿物组合在岩浆期后不同的成矿阶段各具特色。矽卡岩晚期高温氧化物阶段和石英硫化物阶段早期是锡石、马来亚石的主要成矿期，所晶出的大量锡石构成了曾家垅锡矿床的主体。     

Characteristics of fluid inclusions and metallogenic mechanism of the Longshang skarn type tin polymetallic deposit in eastern Hunan Province,ChinaSCIEI北大核心CSCD

矽卡岩型锡矿是全球重要的锡金属来源,但是锡石沉淀成矿机制仍存在较大的争议。垄上矽卡岩型锡矿床位于湘东锡田锡多金属矿田中部,是南岭钨锡成矿带内矽卡岩型锡矿的典型代表。本文在野外考察、矿石矿相学、流体包裹体岩相学研究的基础上,采用流体包裹体组合法对垄上矽卡岩矿床不同矿化阶段代表矿物中的流体包裹体进行了详细研究。结果显示,垄上矽卡岩型多金属矿床成矿阶段可划分为矽卡岩阶段、退化蚀变阶段、云英岩-氧化物阶段、石英硫化物阶段以及萤石碳酸盐化等5个阶段,其中,锡石主要形成于云英岩-氧化物阶段。与锡石密切共生的石英中发育流体包裹体类型主要为富液相、富气相两相水溶液包裹体,含液相CO_(2)三相水溶液包裹体和纯CO_(2)型包裹体。流体温度和盐度具有较大的变化范围(200-400℃和2%-9%NaCleqv),指示流体在降温过程中经历了显著的不混溶。与硫化物共生的石英中主要为富液相两相水溶液包裹体,温度和盐度主要集中在190-261℃和3%-7%NaCleqv,指示流体冷却过程同时经历了流体混合。本次研究提出锡田矽卡岩型矿床中流体不混溶是导致云英岩-氧化物阶段锡石沉淀成矿的主要机制,而流体冷却和混合是导致硫化物沉淀的主要原因。     

矽卡岩锡矿石中锡的赋存状态与锡物相

锡矿物约有六十种,含锡矿物约有二十种。胶态锡是化学物相的概念,是指能溶于１∶３的硫酸中的各类矿物中的锡。它不是某一矿物物相。木锡石、胶状锡石均为锡石的一种,水锡石则是研究得不很清楚的一种矿物。硅酸盐矿物和磁铁矿中都存在类质同象态锡。根据锡矿物和含锡矿物的特性,将矽卡岩锡矿石中的锡分成氧化物相、硫化物相、水锡石相、硅酸锡相四个化学物相,它们各有相对应的矿物,新的化学物相方法利于指导选冶生产。     

柿竹园矽卡岩型钨锡钼铋矿床成矿实验研究

在世界各大锡矿区中普遍存在矽卡岩型锡矿床和锡石硫化物矿床共生的现象,且前者靠近花岗岩接触带,后者产出于矽卡岩之外的大理岩或大理岩化灰岩中。为探讨这一成矿机制,笔者模拟了柿竹园锡矿的形成条件,进行了实验研究。实验表明,在高温矽卡岩阶段成矿溶液中的锡大部分被石榴石等造岩矿物所捕获,或生成锡的钙硅酸盐矿物马来亚石,只有在相当于晚期矽卡岩阶段或石英硫化物阶段的温度条件下,溶液中的锡才以锡石形式晶出,出现锡石-石英-硫化物组合。由此,笔者认为温度是控制这类矿床的主要因素。     

湖南金船塘锡铋矿床矿物化学特征及其地质意义

金船塘锡铋矿床是东坡矿田内一以锡铋为主的大型矽卡岩型多金属矿床,迄今为止对其矽卡岩矿物学特征的系统研究较少。本文以金船塘锡铋矿床主要矽卡岩矿物为研究对象,利用电子探针技术对该矿矽卡岩矿物学特征进行了研究。电子探针分析结果表明:金船塘锡铋矿床的矽卡岩中的石榴子石主要为钙铝榴石-钙铁榴石系列,含少量的锰铝榴石,辉石为透辉石-钙铁辉石系列,角闪石主要为铁镁钙闪石,其次为钙镁闪石、阳起石和透闪石,表明该区的矽卡岩为钙质矽卡岩,含少量的锰质矽卡岩。同时,根据矽卡岩矿物学特征的研究,笔者进一步探讨了该矿床锡石的沉淀机制:早期矽卡岩阶段的氧逸度较高,Sn主要以Sn4+的形式替代Fe3+存在于石榴子石中,而在晚期矽卡岩阶段由于氧逸度的降低,Sn主要以Sn2+的形式呈氯的络合物在流体中迁移,由于流体的温度、盐度、pH和氧逸度的变化,Sn2+被氧化成Sn4+,导致锡石沉淀。     

锡同位素研究进展及其在矿床学中的应用展望

锡同位素是一种新兴的非传统稳定同位素,其在考古学及天体化学中的运用显示出非常大的示踪潜力和价值,然而目前其在地质学(尤其是矿床学)中的研究和应用前景缺乏系统介绍.本文总结分析了世界上目前所发表的主要天然及人工样品的锡同位素数据,发现天然样品中锡同位素组成有较大差异,其中玻璃陨石最富重锡(其δ122/118 Sn值可达2.53‰),而黝锡矿(黄锡矿)最富轻锡(其δ120/116Sn值可达-1.71‰).其中,含锡矿物(如锡石和黝锡矿)中的锡同位素组成变化范围要远远大于全岩样品.地幔及地壳来源的不同岩性或地质体的全岩锡同位素组成有明显差别;锡同位素在一定条件下可以发生分馏,且分馏程度可能远远大于锡同位素的初始值差异.锡石锡同位素对成矿环境非常敏感,其形成时的流体成分、化学反应速率以及物化条件(如温度、盐度、氧逸度、pH值等)等因素均能影响其锡同位素的组成.深部流体(如岩浆来源)结晶的锡石富重锡,而浅部流体(如地层流体)的加入将使锡石富轻锡,因此锡石的锡同位素具有判别不同矿床成因类型的潜力.展望未来,锡同位素的研究有望在以下三方面取得突破:①各地球圈层锡同位素储库数据的精确测定;②矿物原位微区锡同位素的准确快速分析;③热液矿床锡同位素分馏机制的建立.聚焦岩浆-热液演化过程中含锡矿物的锡同位素组成变化,有望揭示含锡流体性质及物化环境,从成矿流体来源、演化、沉淀等角度探讨成矿过程中锡同位素分馏的控制因素及其示踪机制,建立复杂锡成矿系统中的锡同位素演化模型.系统的锡同位素研究可为深入认识多类型锡矿化的"源"、"运""储"过程提供新的思路,为判别有争议锡矿床的成因类型及成矿物质来源提供关键的锡同位素证据,进而为研究大规模锡多金属成矿作用提供全新的视角,具有重要的理论价值及现实意义.     

广西花山花岗岩云英岩化分带与锡成矿过程的矿物学研究

云英岩脉型锡矿是广西花山花岗岩的主要矿化类型之一。花山花岗岩是氧化型花岗岩,岩体中的锡主要以Sn4+ 的形式,赋存于黑云母、角闪石、榍石、金红石、钛铁矿和锡石等含锡矿物中。通过矿物学研究发现,云英岩化过程是：经充 分分异和演化形成的残余岩浆流体与中细粒黑云母花岗岩相互作用。首先,黑云母等原生含锡矿物中的锡在岩浆流体的作 用下被淋滤出,进入流体或次生矿物相,如金红石、白云母等,发生初步富集;其次,在蚀变后期,成矿流体使早先沉淀 的含锡矿物发生重溶,锡溶解进入成矿流体再次富集。锡在流体中与丰富的F- ,Cl - 等络阴离子结合成稳定的配合物运移, 随着云英岩化加深,流体的pH值升高、温度降低、络阴离子浓度降低,流体中配合物的稳定性降低发生沉淀形成锡矿化     

腾冲—梁河地区原生锡矿床类型及成矿机理

腾冲-梁河地区锡矿床是富亲石元素地壳在板块会聚碰撞作用下与再生花岗岩浆活动有关的地球化学旋回中形成的。成矿期前的富集,发生于花岗岩上升侵位、分异演化过程中。由于早期硅酸盐结晶不相容,锡及相关元素逐渐向花岗岩演化序列晚阶段聚集,最终富集于残浆中。残浆在高蒸气压驱动下,向岩基顶部或近侧围岩压力释放带侵位,发生减压沸腾。含矿气-液流体与硅酸盐分离,在非平衡结晶分异条件下,锡及相关元素进入流体相,形成岩浆期后成矿流体。岩浆期后含矿气-液锡的沉淀富集机理决定于成矿流体活动的物理化学场性质。构造封闭岩体内,矿石沉淀富集作用主要由对同源母岩早期晶出的矿物碱交代作用和流体温度压力改变引起的热化学参数变化所形成,产出含锡(钨)-稀有金属变花岗岩型和内云英岩型矿床。构造开放岩体外.成矿流体迁移到长英质围岩断裂-裂隙带中,矿石沉淀富集受减压沸腾和气-液、酸-碱分离作用的制约,并有异源组分加入,产出锡石外云英岩型、富硫化物锡石-石英型矿床。富碳酸盐沉积围岩的物理化学场是以与异源物质交代平衡为主要沉淀富集机理。除接触交代矽卡岩中有部分钙硅酸盐含锡外,随成矿流体与碳酸盐平衡交代进程中流体物理化学条件下的变化,可发生一系列多阶段矿物共生组合,主要有:云英岩化矽卡岩型,含锡硼镁铁矿磁铁矿型,锡石-多金属硫化物型,含锡硫盐-方解石型。在梁河丝光坪尚产出一种以高、低温矿物共生为特点的锡石-木锡石-蛋白石绢英岩型浅成高温热液锡矿床。     

内蒙古大井锡多金属矿床锡矿物特征

大井锡多金属矿床含锡矿物为锡石和黄锡矿,产于3个成矿阶段和5种矿石类型中.从早到晚,即韧性变形阶段→锡石-毒砂-石英阶段→锡石-硫化物阶段(或黄铜矿-黄铁矿阶段),主要含锡矿物锡石的化学成分,表现出SnO2逐渐升高而FeO、TiO2、Nb2O5、Ta2O5和In2O5依次跳跃式递减的特征,同时NiO和Ga2O5趋于升高.与一般脉状锡矿床相比,早阶段锡石富Ta而晚阶段锡石富Ti、Fe,表明早期的锡石更接近花岗质岩浆源特征而晚期锡石则明显具层控性质.锡石的组分变化特征与各阶段(内)从早到晚成矿温度递减有关.另一含锡矿物黄锡矿含As、Zn较高,仅出现于锡石-硫化物阶段,并在温度为220℃～320℃、硫逸度为10-10.04×105～10-13.44×105Pa的特定区间内淀出.两个阶段锡石的稀土元素特征分别与矿区次火山岩和林西组地层一致,表明早期锡石-毒砂-石英阶段中的锡主要来自次火山岩(如英安斑岩),而晚期锡石-硫化物阶段中的锡可能主要来自林西组围岩(如粉砂岩).     

铜锡复合成矿研究进展与展望

铜与锡具有不同的地球化学性质,然而铜锡共生或复合成矿现象在世界主要铜、锡成矿带中比较常见,如中国的右江、南岭(湘南)、大兴安岭南段(内蒙东部)、葡萄牙伊比利亚、秘鲁安第斯、英格兰德文郡、德国厄尔士山、日本西南、俄罗斯远东、加拿大新不伦瑞克等成矿带均为铜锡复合矿床的集中产区。铜锡复合矿床主要为岩浆热液矿床,以矽卡岩型、脉状矿床为主,兼有火山热液沉积型、斑岩型及云英岩型等。铜矿体的主要矿石矿物为黄铜矿,兼有斑铜矿、黝铜矿、辉铜矿等;锡矿体的主要矿石矿物为锡石,兼有黝锡矿。铜锡复合矿床的成矿物质来源(尤其是铜、锡成矿元素的来源是否具有一致性)尚有不少争议,锡普遍被认为是岩浆来源,而铜的来源具有多样性。成矿流体演化过程中的氧化还原环境的改变及流体的混合是导致铜锡复合成矿的主要原因。目前对于铜锡复合成矿的研究,主要是从矿床的年代学、单矿物(黄铜矿、锡石)微量元素及传统同位素地球化学、流体包裹体等方面入手,但对厘定铜锡复合成矿过程的作用有限。铜锡复合矿床的成因及勘查模型的建立具有重要的理论价值及现实意义。本文提出未来研究可以从多种非传统稳定同位素(例如Cu、Sn、W、Zn同位素)的联合示踪探索、成...     

Tin-carrier minerals in metaluminous granites of the western Nanling Range (southern China): Constraints on processes of tin mineralization in oxidized granites

Huashan, Guposhan and Qitianling are three similar and representative metaluminous A-type tin granites in the western Nanling Range, China. They all have a high oxidization state with magnetite as the dominant Fe–Ti oxide. This study presents an understanding of systematic mineralogy of Sn-bearing minerals (biotite, titanite, magnetite and cassiterite) in the three granites. Biotite has an annite composition and both electron-microprobe and LA-ICP-MS analyses indicate trace amounts of tin in biotite (approximately 100–20 ppm). Chloritization of biotite is accompanied by formation of Sn-rich rutile and cassiterite. Titanite has a long history of crystallization from the early-magmatic stage through the late-magmatic stage to the hydrothermal stage. Owing to its solid-solution relationship with malayaite (CaSnSiO₅), titanite always contains tin to various extents. Early-magmatic titanite contains about 0.5 wt.% SnO₂, while the late-magmatic titanite is markedly enriched in tin (on average 14.8 and 3.4 SnO₂ in titanite from the Qitianling and Huashan granites, respectively). Magnetite grains typically display a trellis structure with ilmenite lamellae, where microinclusions of cassiterite (<1 μm in size) are present. This is likely consistent with features of the “oxy-exsolution” process of Sn-bearing titanomagnetite precursor. Cassiterite may be observed as late-magmatic phase, but most commonly appears as an alteration product of other primary minerals. All tin-bearing minerals in the three granites record a complete process of tin mineralization in granite. The features of tin in primary biotite, titanite and magnetite reflect an initial enrichment during the early stage of magmatic crystallization of the Huashan, Guposhan and Qitianling granites. Association of interstitial Sn-titanite and cassiterite suggests further tin enrichment related to fractional crystallization of granitic magmas. Fluids and alteration of primary minerals play an important role in the leaching, concentration and transportation of Sn during hydrothermal processes, which favors vein-type Sn mineralization.     

南岭地区钨锡花岗岩的成矿矿物学：概念与实例

南岭地区的钨锡成矿作用与花岗岩岩浆活动有十分密切的关系。花岗岩的物源与成矿元素的初始富集、花岗岩的分异程度和花岗岩中流体性质与活动性集中体现了花岗岩对成矿的控制能力,即花岗岩的成矿能力。初步建立了南岭地区钨锡花岗岩的成矿矿物学研究体系。黑云母、榍石、锆石、锡石、金红石、黑钨矿、白钨矿和钨铁铌矿等是讨论的重点矿物,它们可用于判别花岗岩的成矿能力。首先以矿物晶体化学为基础,介绍了上述矿物在钨锡花岗岩中的岩相学特征、内部构造和矿物化学及其变化,并分别论证了花岗岩原始含矿性、花岗岩结晶演化和花岗岩中成矿元素活动性的矿物学标志;其次,系统对比了南岭地区三类钨锡花岗岩（准铝质含锡花岗岩、过铝质含锡花岗岩和过铝质含钨花岗岩）的成矿矿物学特征。以湖南骑田岭花岗岩复式岩体为实例,进行了芙蓉- 菜岭含锡花岗岩和新田岭含钨花岗岩的成矿矿物学对比研究。前者以黑云母、榍石为典型含锡矿物,它们在流体富集阶段,经热液蚀变作用,导致锡的淋滤和结晶富集作用;后者则以出现岩浆白钨矿和黑钨矿为特征。提出的钨锡花岗岩成矿矿物学研究体系有助于深化矿床学研究和矿床勘探工作,并将在今后工作中进一步完善。     

A combined EMPA and LA-ICP-MS study of Li-bearing mica and Sn–Ti oxide minerals from the Qiguling topaz rhyolite (Qitianling District,China): The role of fluorine in origin of tin mineralization

The Sn-rich Qiguling topaz rhyolite dike intrudes the Qitianling biotite granite of the Nanling Range in southern China; the granite hosts the large Furong Sn deposit. The rhyolite dike is typically peraluminous, volatile-enriched, and highly evolved. Whole-rock F and Sn concentrations attain 1.9 wt.% and 2700 ppm, respectively. The rhyolite consists of a fine-grained matrix formed by quartz, feldspar, mica and topaz, enclosing phenocrysts of quartz, feldspar and mica; it is locally crosscut by quartz veinlets. Lithium-bearing micas in both phenocrysts and the groundmass can be classified as primary zinnwaldite, “Mus-Ann” (intermediate member between annite and muscovite), and secondary Fe-rich muscovite. Topaz is present in the groundmass only; common fluorite occurs in the groundmass and also in a specific cassiterite, rutile and fluorite (Sn–Ti–F) assemblage. Cassiterite and rutile are the only Sn and Ti minerals; both cassiterite and Nb-rich rutile are commonly included in the phenocrysts. The Sn–Ti–F assemblage is pervasive, and contains spongy cassiterite in some cases; cassiterite also occurs in quartz veinlets which cut the groundmass. Electron microprobe and LA-ICP-MS compositions were used to study the magmatic and hydrothermal processes and the role of F in Sn mineralization. The presence of zinnwaldite and “Mus-Ann”, which are respectively representative of early and late mica crystallization during magma differentiation, also suggests a significant decrease in f(HF)/f(H₂O) of the system. Cassiterite included in the zinnwaldite phenocrysts is suggested to have crystallized from the primary magma at high temperature. Within the Sn–Ti–F aggregates, rutile crystallized as the earliest mineral, followed by fluorite and cassiterite. Spongy cassiterite containing inclusions of the groundmass minerals indicate a low viscosity of the late fluid. The cassiterite in the quartz veinlets crystallized from low-temperature hydrothermal fluids, which possibly mixed with meteoric water. In general, cassiterite precipitated during both magmatic and hydrothermal stages, and over a range of temperatures. The original fluorine and tin enrichments, f(HF)/f(H₂O) change in the residual magma, formation of Ca,Sn,F-rich immiscible fluid, decrease of the f(HF) during groundmass crystallization, and mixing of magma-derived fluids with low-saline meteoric water during the late hydrothermal stage, are all factors independently or together responsible for the Sn mineralization in the Qiguling rhyolite.     

Tin-bearing minerals at the Furong tin deposit,South China: Implications for tin mineralization

It remains poorly constrained whether remobilization of Sn from granites and prograde skarns plays an essential role in forming economic (skarn-type) tin mineralization. Using both electron probe microanalysis and laser ablation–inductively coupled plasma–mass spectrometry methods, in-situ Sn contents, as well as major elements, were analyzed for numerous silicates and magnetite from fresh granite, altered granite, and skarn at the large Furong Sn deposit (530,000 t Sn @ 0.8% Sn) in the Nanling Range, South China. Hornblende and biotite in fresh granite are the main Sn-bearing phases (Sn = 44–321 ppm), while plagioclase and K-feldspar are poor in Sn (< 5 ppm). In altered granite, tin is hosted mainly by hydrothermal muscovite (299–583 ppm) replacing plagioclase, but rarely by chlorite (mostly <10 ppm) replacing hornblende and biotite. In contrast, most silicates (garnet, diopside, vesuvianite, pargasite and epidote) and magnetite from tin skarn are Sn-rich (47–44,241 ppm), except for Sn-poor phlogopite and scapolite (< 10 ppm). In particular, garnet, pargasite, and epidote reach tin concentrations in the percent range. Tin generally enters the stannous silicates and magnetite through substitutions for octahedral Al^vi and Fe³⁺. Comparisons of Sn contents between magmatic and hydrothermal minerals in granite, prograde and retrograde minerals related to tin skarn indicate that remobilization of Sn from granite and prograde skarn is not a pre-requisite to form tin mineralization.     

Composition, mineral assemblages, and genesis of titanite and malayaite in skarns

The composition of minerals of the titanite-malayaite series and their mineral assemblages and genesis were examined at the Bol’shoi Kan’on deposit in Magadan oblast and at other deposits. These minerals were demonstrated to be typomorphic Sn-bearing silicates in postmagmatic bimetasomatic hypabyssal calc skarns and skarnoids in tin-bearing provinces. The series of these minerals with similar crystal structures has a miscibility gap, and the minerals are characterized by notably different Sn concentrations. Moreover, titanite may contain Al, Fe, F, and OH, whose concentrations decrease in the Sn-bearing members of the series (malayaite). These silicates were formed at many deposits after the successive transforms of skarn mineral assemblages. The early assemblages include wollastonite in calcic carbonate rocks and diopside and salite in skarnoids. The latter minerals are replaced first by hedenbergite with subordinate amounts of vesuvianite and garnet first of grossular and then andradite composition. This process was syngenetic with the formation of borosilicates (danburite, axinite, and tourmaline). Ti thereby may be accommodated in grossular and Sn in Fe-bearing silicates, mostly, in andradite. Skarns often contain both titanite and malayaite, which were produced in these rocks earlier than cassiterite. The isomorphic series of these minerals has a miscibility gap. The oreforming processes ended with the crystallization of quartz, fluorite, and rare sulfides, including stannite. The late Sn-bearing minerals at some deposits are stokesite and Mg, Fe, and Ca stannates, which crystallized during malayaite replacement by newly formed calcite-quartz aggregates. The Sn-bearing sulfides are replaced by varlamoffite during supergene processes.     

In-situ LA–ICP-MS trace elemental analyses of magnetite: The Mesozoic Tengtie skarn Fe deposit in the Nanling Range,South China

The Nanling Range in South China hosts numerous world-class W–Sn deposits and some Fe deposits. The Mesozoic Tengtie Fe skarn deposit in the southern Nanling Range is contemporaneous with the regional Sn mineralization. The deposit is composed of numerous ore bodies along the contacts between the late Paleozoic or Mesozoic carbonate rocks and the Yanshanian Lianyang granitic complex. Interaction of the magma with hosting dolomitic limestone and limestone formed calcic (Ca-rich) and magnesian (Mg-rich) skarns, respectively. The Tengtie deposit has a paragenetic sequence of the prograde stage of anhydrous skarn minerals, followed by the retrograde stage of hydrous skarn minerals, and the final sulfide stage. Magnetite in the prograde and retrograde skarn stages is associated with diopside, garnet, chlorite, epidote, and phlogopite, whereas magnetite of the final stage is associated with chalcopyrite and pyrite. Massive magnetite ores crosscut by quartz and calcite veins are present mainly in the retrograde skarn stage. Laser ablation ICP-MS was used to determine trace elements of magnetite from different stages. Some magnetite grains have unusually high Ca, Na, K, and Si, possibly due to the presence of silicate mineral inclusions. Magnetite of the prograde stage has the highest Co contents, but that of the sulfide stage is extremely poor in Co which partitions in sulfides. Magnetite of magnesian skarns contains more Mg, Mn, and Al than that of calcic skarns, attributed to the interaction of the magma with compositionally different host rocks. Magnetite from calcic and magnesian skarns contains 6–185 ppm Sn and 61–1246 ppm Sn, respectively. The high Sn contents are not due to the presence of cassiterite inclusions which are not identified in magnetite. Instead, we believe that Sn resides in the magnetite structure. Regionally, intensive Mesozoic Sn mineralization in South China indicates that concurrent magmatic–hydrothermal fluids may be rich in Sn and contribute to the formation of high-Sn magnetite. Our study demonstrates that trace elements of magnetite can be a sensitive indicator for the skarn stages and wall-rock compositions, and as such, trace elemental chemistry of magnetite can be a potentially powerful fingerprint for sediment provenance and regional mineralization.     

Mineralogy, Geochemistry, and Age Constraints on the Beni Bou Ifrour Skarn Type Magnetite Deposit, Northeastern Morocco

Abstract: The Beni Bou Ifrour deposit of northeastern Morocco is a skarn type magnetite deposit. K-Ar age determination suggests that the mineralization occurred at 7.040.47 Ma. The spatial relationship between skarn and dikes of microgran-odiorite derived from the batholith of Wiksane Granodiorite, and the similarity of age (8.020.22 Ma), confirms that the Wiksane Granodiorite is the igneous rock most probably related to mineralization. The skarn is distributed asymmetrically in the limestone, and magnetite ore was developed just below the calc-silicate skarn as two parallel beds separated by 100 m of barren limestone and schist.
The mineralization can be divided into three stages. The early stage is characterized by the formation of calc-silicate minerals, mainly clinopyroxene (80–70 % diopside) and garnet (early almost pure andradite to the late 60 % andradite). The main stage is characterized by the formation of a large amount of magnetite. Epidote and quartz formed simultaneously with magnetite. Fluid temperatures exceeded 500 C during the early to main stages. Fluid with very high salinity (50–75 wt% NaCl equiv.) was responsible for the formation of the magnetite ore. The oxygen isotope composition, together with the fluid inclusion data, suggests that magmatic fluid was significant for the formation of calc-silicate skarn minerals and magnetite. Low temperature (-230C) and low salinity (-10 % NaCl equiv.) hydrothermal fluids dominated by meteoric water were responsible for the late stage quartz and calcite formation.     

滇东南都龙锡锌铟多金属矿床磁铁矿矿物化学组成特征及其对成矿作用的约束

都龙锡锌铟多金属矿床位于著名的滇东南钨锡多金属成矿区之老君山矿集区,成矿与白垩纪大规模花岗岩活动关系密切,沿隐伏花岗岩接触带周边发育石榴子石、透辉-透闪石等矽卡岩蚀变和条带状(似层状)、脉状(囊状)的锡石、闪锌矿及磁铁矿、辉钼矿、黄铁黄铜矿等矿化,形成超大规模的岩浆热液-矽卡岩成矿系统。野外观测及研究发现,早期(矽卡岩期)高温阶段形成的磁铁矿可分为I阶段交代型磁铁矿(I-Mag)和II阶段充填型磁铁矿(II-Mag)两类:前者多呈囊状、条带状,与矽卡岩矿物共生;后者为脉状,与金属硫化矿物共生。利用ICP-AES、ICP-MS对两类磁铁矿进行主、微量元素测试,从I-Mag到II-Mag,Si、Ca、Mn及ΣREE、Pb、Zn、Ti含量增加,Mg及Sn、W、In、V、Cr、Ga含量减少,REE配分型式也由平缓向右倾的逐渐变化。TiO 2-Al 2 O 3-(MgO+MnO)、(Ti+V)-(Ca+Al+Mn)、Ni/Cr-Ti、(Ti+V)-Ni/(Cr+Mn)成因判别图解表明,磁铁矿属岩浆热液-矽卡岩成因类型;Ti、V与Zr、Hf、Nb、Ta,以及Y/Ho(24~3414)、Ni/Co(<2→>2)、Ti/V(<25→>25)、Hf/Zr(003~006→004~005)存在着线性关系和规律变化特征,指示两类型磁铁矿具有相同的物质来源,为同一成矿过程不同阶段的产物。而代表成矿流体REE组成的II-Mag的REE组成继承了老君山花岗岩REE配分趋势和Eu负异常特征,表明磁铁矿与白垩纪老君山花岗岩具有一致的物质来源。Cr-V、(Ti+V)-(Al+Mn)、Ga-Mg及Ga-Sn图解显示相同的成因类型和一致的线性关系,指示磁铁矿主体形成于较高氧逸度和温度(约300℃)的成矿环境下,并且从I-Mag到II-Mag,存在着氧逸度逐渐升高、温度逐渐降低的演化趋势。     

Cassiterite exsolution with ilmenite lamellae in magnetite from the Huashan metaluminous tin granite in southern China

Sn⁴⁺ is generally the dominant form of tin in magnetite-series granites as shown by the presence of cassiterite or its incorporation into Ti-bearing minerals such as biotite and titanite. Little is known about the behavior of tin in magnetite. The Huashan granite is an oxidized tin granite in the Nanling Range, southern China, where it contains magnetite as the dominant Fe oxide mineral. It is included in biotite as an early phase and also as interstitial grains spatially associated with ilmenite, cassiterite, Sn-rich titanite (SnO₂ up to 5.9?wt.%), fluorite and apatite. This association indicates that tin enrichment occurred during the late stage of magma crystallization. Ilmenite lamellae display a trellis structure consistent with features of the “oxy-exsolution” process of Sn-bearing titanomagnetite precursor. Micro-inclusions of cassiterite (<1?μm in size) are found only within ilmenite lamellae. This suggests that magnetite with cassiterite inclusions is likely an indicator mineral of oxidized tin granites. Although rare in nature, Sn-bearing magnetite from weathered granites where concentrated in stream sediments, may serve as a strategic tracer for tin exploration in granite districts and in placer deposits, in general.     

大兴安岭南段黄岗矽卡岩型铁锡多金属矿床蚀变矿化特征及其成因

大兴安岭南段黄岗铁锡多金属矿床具有明显的蚀变-矿化特征,对于研究矽卡岩型矿床的成矿过程具有重要的意义.因此对该矿床中具有代表性的蚀变矿物以及金属矿物开展电子探针研究,结果指示研究区的热液演化经历了4个阶段:在进变质矽卡岩阶段（Ⅰ）,矿物以含有钙铁榴石GrtⅠ核的钙铝榴石GrtⅡ和钙铁辉石为主;在退变质矽卡岩阶段（Ⅱ）,矿物以富铁榴石GrtⅢ、浸染状磁铁矿以及含水矿物为代表;氧化物阶段（Ⅲ）的矿物以大量磁铁矿、锡石以及少量钙铁榴石GrtⅣ和透辉石为主;在硫化物阶段（Ⅳ）,磁铁矿逐渐被硫化物交代,最后形成毒砂、黄铁矿、黄铜矿、铁闪锌矿、浅色闪锌矿-黄铜矿-方黝锡矿固溶体、锑黝铜矿等,表明黄岗铁多金属矿床的流体来源从岩浆水、交代流体最后演化为大气降水的加入,流体成分变化复杂,流体演化具体表现为温度逐渐降低,水岩比值逐渐升高,具有还原性→氧化性→还原性等特点.