安徽省绩溪黑云母二长花岗岩中高铁铁橄榄石大斑晶的研究

高铁铁橄揽石大斑晶产在安徽省绩溪县黑云母二长花岗岩中.岩石呈细粒花岗结 构，矿物成分为条纹长石、更长石、石英和黑云母。大斑晶最大粒径可达5em，其中含有微小的 磁铁矿自形晶，呈浸染状或断续脉状.在表生条件下，高铁铁橄榄石局部氧化成褐铁矿.大斑晶 的外形、颜色和光泽等酷似黑钨矿. 大斑晶形成于上地慢高温高压条件下，先从花岗岩浆中结晶出铁橄榄石的高压变晶，岩浆沿 深断裂向上部运移过程中，随着氧分压的增加而氧化成高铁铁橄榄石.     

丹东地区花岗岩类岩石中碱性长石斑晶成因初探

丹东地区两套中生代花岗岩系中许多岩体都含碱性长石斑晶。这些斑晶具有许多相似的性质,它们呈自形晶,粒度大,具卡氏双晶。其中斜长石、黑云母等包裹体平行斑晶的生长面而呈环状排列。通常核部附近的包裹物为斜长石,而石英反被包裹在斑晶的边缘。斑晶中Ab、An和钡的含量也较基质碱性长石高。由二长石温度计计算的斑晶生成温度为700℃左右。X—光衍射数据表明,斑晶主要为中间微外长石,少量为正长石和微斜长石,这些都说明了斑晶乃岩浆结晶产物。根据实验资料,还讨论了斑晶的结晶过程,并认为斑晶的晶出反映了岩浆高水压力的特点。     

6210矿田二云母花岗岩白云母化与铀成矿的关系

6210矿田小斑状二云母花岗岩为产铀花岗岩。经研究属地壳重熔型花岗岩。钾长石和石英呈斑晶出现,具纺锤状、眼球状,呈定向分布。二云母花岗岩乃是一种白云母化的黑云母花岗岩,岩体上部是二云母花岗岩,至700—1000m 深部逐渐过渡为白云母化极弱的黑云母花岗岩。二云母花岗岩的二氧化硅比黑云母花岗岩略高。石英及钾长石含量较多,斜长石号码偏     

高铁铁橄榄石的新研究——兼论铁橄榄石的氧化作用

本文综合应用微束分析技术,包括扫描电镜、电子探针、电子显微镜和激光喇曼探针等多种分析技术,对国内外许多学者感兴趣的高铁铁橄榄石进行了系统深入的研究,发现高铁铁橄榄石通常是铁橄榄石和一系列氧化程度不等的氧化铁橄榄石及其他一些氧化产物的总和,并对高铁铁橄榄石和铁橄榄石的氧化作用提出了一些新认识:(1)铁橄榄石在其形成后至少受到两次蚀变;(2)铁橄榄石氧化的最终产物是玻璃;(3)原先关于高铁铁橄榄石的结构分析、反相畴、超结构和假双晶等问题尚待进一步研究;(4)将高铁铁橄榄石看成是新矿物实属疑问。     

高铁铁橄榄石热处理产物的研究

1976年以来,先后在我国辽宁省莱河及河北省迁西县发现了高铁铁橄榄石,它们的化学通式为Fe~(3 )Fe_2~(3 )(SiO_4)_2;产在辽宁省莱河的高铁铁橄榄石曾被命名为莱河矿。作者曾用穆斯鲍尔效应研究过这种矿物。本文的目的是用X射线、红外光谱及穆斯鲍尔谱研究采自河北省的高铁铁橄榄石的热处理产物,探讨它在氧化和还原条件下的变化,这对阐明该矿物的成因和演化将是有益的。 河北省高铁铁橄榄石产在一种特殊的英榴易溶岩中,它与石英、石榴石、易溶石、磁铁矿和石墨共生,在光片和薄片中可以看到它交代易溶石,而被磁铁矿切穿。石榴石又往往包裹上述矿物。本研究所用的高铁铁橄榄石的化学成分为:SiO_231.96,Fe_2O_335.31,Al_2O_3     

宽甸环斑花岗岩的同化混染成因

环斑花岗岩是发育于前寒武纪的一种特殊岩石。本文从环斑花岗岩的地质学、岩石学及矿物学等方面讨论了宽甸元古宙环斑花岗岩的成因,认为环斑花岗岩是由分异出石英二长岩的富钾质残余岩浆在深部同化围岩(类似盖县组的矽线石榴黑云斜长片麻岩及黑云母变粒岩等岩石)形成的含大量围岩捕虏晶的晶粥状岩浆,经侵位结晶而成。环斑长石的斜长石外壳是来自围岩的捕虏晶,它通过流动、吸附作用附着于钾长石巨晶的周围,构成环斑结构。     

松辽盆地营城组中基性火山岩成岩作用:矿物晶出序列、杏仁体充填和储层效应

利用露头和钻井资料,通过显微镜观测、化学分析和电子探针分析,研究营城组中基性火山岩的矿物晶出系列和杏仁体充填及其储层效应。本区中基性火山岩包括玄武岩、安山岩、玄武安山岩、粗面玄武岩、玄武粗安岩和粗安岩。斑晶矿物的晶出顺序为:橄榄石最早并几乎全部蚀变为蛇纹石、伊丁石和磁铁矿,仅保留橄榄石假象;辉石被斜长石包含或与之交生,说明辉石晶出有的略早于斜长石、有的与之同时。基质呈间隐间粒结构,为比斑晶偏酸性/碱性的板条状微晶长石堆积搭成格架、内充填玻璃质及微晶粒状矿物(橄榄石、辉石和磁铁矿)。基质结晶晚于斑晶,晶出序列为微晶粒状矿物→微晶长石→玻璃质。有单成分和复成分两种杏仁体。单成分者主要见硅质和钙质,具结晶世代性,为后生流体沉淀充填形成,可作为储层变差或非储层的标志。复成分杏仁体是原生火山玻璃固态下水合与蚀变作用的结果:包括蛇纹石/绿泥石-火山玻璃、石英-方解石-皂石/方解石和石英-绿泥石-方解石等组合类型,通常可作为储层改善或有效性增加的标志。中基性火山玻璃蚀变分为四个阶段:新鲜火山玻璃(折光率1.57)→水合火山玻璃(折光率降至1.53)→橙玄玻璃(铁镁质微晶矿物集合体)→新生矿物(石英、方解石、蛇纹石、绿泥石、皂石);由火山玻璃变为新生矿物的体积减小或孔隙增加效应为7%～10%。     

新疆西准噶尔宝贝金矿矿床地质和流体包裹体特征

<正>宝贝金矿位于新疆西准噶尔地区东南部,与哈图金矿同属于哈图-萨尔托海金成矿带。矿区出露地层为下石炭统太勒古拉组(C1t),岩性主要为中酸性的晶屑凝灰岩和凝灰质粉砂岩;侵入岩主要为似斑状花岗岩岩体。矿区主要发育NNE向断裂和SN向、EW向、NE向和NW向构造裂隙。宝贝金矿似斑状花岗岩岩体和围岩中均有矿化发育。似斑状花岗岩由钾长石、斜长石、石英和少量褐色黑云母组成,斑晶以石英和长石为主,发育绢云母化、角岩化和弱绿泥石化蚀变。岩体显示出很好的Cu、     

某地含水晶伟晶岩的地质、矿物及地球化学特点

一、地质概况某地含水晶伟晶兴产于海西晚期黑云母花岗岩中。岩体侵入于下二迭统火山-沉积岩系中,呈岩株状产出,平面形状沿北东方向略为伸长,出露面积约80平方公里(图1),为碱性花岗岩(表1、2)。     

DaG476火星陨石的岩相学和矿物学研究

Dar al Gani 476(简称DaG 476)是1998年在利比亚撒哈拉沙漠中发现的第13块火星陨石.它属于含橄榄石斑晶的橄玻无球粒陨石[1,2],具典型火成分异结构,辉石和长石具典型的玄武结构,橄榄石以斑晶形式镶嵌于玄武岩中,副矿物主要有氧化物、硫化物和磷酸盐等.根据背散射电子像获得的矿物模式丰度(%,vol)为:辉石61,橄榄石22,熔长石12,冲击熔融包2,铬铁矿和钛铁矿等氧化物2,陨硫铁1,磷酸盐1,以及沙漠风化作用产生的碳酸盐1.     

赣杭构造带相山火山侵入杂岩的岩浆演化特征——来自斜长石和黑云母的化学成分研究

黑云母、斜长石等矿物可作为寄主岩石的岩浆演化的指示剂。本文借助电子探针微区分析技术,通过对赣杭构造带中相山盆地火山侵入杂岩中这些矿物的化学组成进行定量分析发现:碎斑熔岩、花岗斑岩及石英二长斑岩的斜长石环带不明显,并且主要是中长石;石英二长斑岩中黑云母矿物成分为镁质黑云母和铁质黑云母,化学成分更为接近研究区镁铁质微粒包体中黑云母的成分,而碎斑熔岩及花岗斑岩中黑云母的镁含量较低。结合黑云母、斜长石矿物的化学特征及前人的工作研究,相山碎斑熔岩和花岗斑岩的物质来源主要是壳源,没有明显地幔物质的加入,而石英二长斑岩有一定量的地幔物质的加入,并且这个地幔物质的加入发生在石英二长斑岩的黑云母开始结晶之前。     

广西栗木矿田花岗岩体地球化学特征制约因素及其动力学背景

对栗木矿田3个花岗岩体进行了岩石主量元素、微量元素的地球化学研究和分析,岩石化学成分具高铝高硅碱特征,属于高钾钙碱性岩系列;微量元素总量明显偏低,Eu强烈亏损,以富含Li、Rb贫Sr、Ba为特征,花岗岩浆分异度高或岩浆发生过充分的结晶分异作用;推断花岗质岩浆熔出后源区残留相为石榴石+斜长石+钾长石±角闪石±黑云母等组成的麻粒岩相,具深源的特征,在中高—高压条件下部分熔融形成的,同时,受氧逸度(f O 2)较低、水活度(αH 2 O)较低、水逸度(f H 2 O)较高的制约因素影响.通过对华南地区岩石圈深部动力学背景分析,认为岩石圈减薄合理地解释了本区栗木花岗岩体的形成机制.     

新疆喀拉萨依含锡花岗岩体地质特征及成岩成矿机制

通过对大量实际资料的分析认为,喀拉萨依含锡花岗岩体形成于造山期后阶段,年龄300Ma左右,岩体中出露的肉红色和灰白色黑云母钾长花岗岩由强分异岩浆先后侵入形成,二者具同源演化关系;原始岩浆为上地壳变碎屑质沉积岩部分熔融形成的黑云母二长花岗质岩浆;发育于岩体边部的云英岩型锡矿化同岩浆期后富含氟的高温气液流体作用有关。     

Concentric zoning in the Tunk Lake pluton,coastal Maine

The Tunk Lake pluton of coastal Maine, USA is a concentrically zoned granitic body that grades from an outer hypersolvus granite into subsolvus rapakivi granite, and then into subsolvus non-rapakivi granite, with gradational contacts between these zones. The pluton is partially surrounded by a zone of basaltic and gabbroic enclaves, interpreted as quenched magmatic droplets and mushes, respectively, as well as gabbroic xenoliths, all hosted by high-silica granite. The granite is zoned in terms of mineral assemblage, mineral composition, zircon crystallization temperature, and major and trace element concentration, from the present-day rim (interpreted as being closer to the base of the chamber) to the core (interpreted as being closer to the upper portions of the chamber). The ferromagnesian mineral assemblage systematically changes from augite and hornblende with augite cores in the outermost hypersolvus granite to hornblende, to hornblende and biotite, and finally, to biotite only in the subsolvus granite core of the pluton. Sparse fine-grained basaltic enclaves that are most common in the outermost zone of the pluton suggest that basaltic magma was present in the lower portions of the magma chamber at the same time that the upper portions of the magma chamber were occupied by a granitic crystal mush. However, the slight variations in initial Nd isotopic ratio in granites from different zones of the pluton suggest that contamination of the granitic melt by basaltic melt played little role in generating the compositional gradation of the pluton. The zone of basaltic and gabbroic chilled magmatic enclaves, and gabbroic xenoliths, hosted by high-silica granite, that partially surround the pluton is interpreted as mafic layers at the base of the pluton that were disrupted by invading late-stage high-silica magma. These mafic layers are likely to have consisted of basaltic lava layers and basalt that chilled against granitic magma to produce coarse-grained gabbroic mush. Basaltic and gabbroic magmatic enclaves and gabbroic xenoliths are hornblende-bearing, suggesting that their parent melts were relatively hydrous. The water-rich nature of the underplating mafic magmas may have prevented extensive invasion of the granitic magma by these magmas, owing to the much greater viscosity of the granitic magma than the mafic magmas in the temperature range over which magma interaction could have occurred.     

冀东黑云母片麻岩在1GPa压力下脱水熔融实验

报道冀东黑云母片麻岩在1GPa压力下脱水熔融实验的相关系。其固相线温度为812℃,黑云母消失的温度为837℃,角闪石消失的温度为887℃,在862℃时开始形成斜方辉石和单斜辉石。实验表明,在温度812-950℃范围内形成水不饱和的花岗质岩浆,数量为20%-30%,而留下的难熔残余是斜方辉石+单斜辉石+石榴石+斜长石+石英±角闪石,后者与麻粒岩相岩石的矿物组合相符合,暗示下地壳岩石经生成花岗质熔浆的熔融事件后,留下的将是麻粒岩相岩石。     

法国中央高原Margeride花岗岩中黑云母岩的起源探讨

法国中央高原Ｍａｒｇｅｒｉｄｅ花岗岩暗色相中包含的Ａｎｃｅ和Ｖａｚｅｉｌｌｅｓ黑云母岩，大小达数十米，分别含有４０％和９０％以上的黑云母及少量的磷灰石、锆石、斜长石或钾长石，且发现有变质岩包体。野外观察可见，黑云母岩与其上覆花岗岩呈逐渐过渡关系，而其下部界限则很分明；它的面状及线状结构与相邻花岗岩的一致。矿物成分显示，各矿物（黑云母、斜长石、磷灰石）的化学成分与相邻花岗岩中相同矿物的相似或相同。由     

A Review of the Nature of Magmatism in Central Anatolia during the Mesozoic Post-Collisional Period

Magmatism in central Anatolia is characterized by petrographically and chemically distinct granitic and syenitic rocks. The granitic magmatism comprises C-type (crustal-derived) and H-type (hybrid) monzogranites and monzonites. Garnet-bearing C-type leucogranites represent the oldest magmatic phase, but younger hornblende ± biotite ± K-feldspar H-type plutons dominate the geology of the Central Anatolian Crystalline Complex (CACC). These typically include mafic microgranular enclaves. The granitic magmatism predates syenitic intrusions, among which quartz-bearing syenites were emplaced prior to feldspathoid-bearing ones.

The nature of magmatism in central Anatolia varies through time from peraluminous to metaluminous to alkaline. These different magma types reflect distinct stages of postcollisional magmatism, in which interaction between crust and mantle varied considerably. The C-type granites of the early stages of postcollisional magmatism were likely derived by partial melting of the lower continental crust induced by mafic magma underplating as a result of lithospheric delamination. The H-type granites and syenites of the mature and advanced stages of postcollisional magmatism indicate a significant contribution from mande-derived magma within a continuous or episodic extensional tectonic regime.     

Abundance and distribution of tungsten in the Afu Younger Granite Complex of central Nigeria

Geochemcial distribution of tungsten in the granitic rocks of Afu Younger Granite Complex of Central Nigeria, indicates that the average tungsten content (168 ppm) of the rocks is significantly higher than any reported average abundance for granitic rocks. However, significant contrast between the rock phases is obtained only in the Igo biotite granite which is directly connected with tungsten lode mineralization.The close spatial relationship between tungsten mineralization and the Igo biotite granite suggests that the ore forming fluids were probably derived from the residual fraction of the granitic magma. Greisenization is intimately associated with mineralization and it is suggested that they both had a common process of formation.     

Petrology of rapakivi granites in Salmi massif

Crystallization of rapakivi is accompanied by a progressive decrease in the alkali content of the high-temperature granitic magma and by the concurrent increase in its iron content, during the crystallization of potassium feldspar which is followed by the crystallization of biotite. The pressure is not high enough to permit a simultaneous crystallization of potassium feldspar, as e. g. of albite. The potassium feldspar-biotite sequence is upset by Mg, in the ovoid varieties of rapakivi in which the potassium feldspar crystallization is arrested, short of its completion, by the crystallization of Mg biotite. – IGR Staff.