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151.
稀土元素(REE)作为"三稀资源"之一,是中国重要的战略性矿产资源,碳酸岩型稀土矿床是世界稀土的主要来源.成矿碳酸岩的岩浆演化以及稀土元素的富集和分异机理一直是碳酸岩型稀土矿床研究的热点和难点,国内外学者对碳酸岩的岩浆起源、岩浆演化过程中稀土元素富集与分异的机理进行了大量的研究与探讨,但仍存在较多的争议,限制了碳酸岩型稀土元素成矿理论的发展及国内外碳酸岩型稀土矿床的找矿勘查工作.文章重点对稀土成矿碳酸岩的起源、岩浆演化过程及在此过程中REE的富集与分异行为进行了详细的文献调研和评述,同时,基于笔者在冕宁牦牛坪稀土矿床前期的研究工作和最新发现,认为碳酸岩中普遍存在矿物学分带,它是岩浆演化过程的最佳记录,是不同成分矿物结晶分异作用的体现.对牦牛坪稀土矿床碳酸岩的矿物学分带特征及其中的熔体、熔流体和流体包裹体进行了初步描述与探讨,以期为研究碳酸岩的岩浆演化、岩浆-流体转化过程及稀土元素的富集与分异机理提供新的思路,促使对稀土碳酸岩矿物学分带及其对REE富集与分异的研究引起更多的关注和重视.  相似文献   
152.
四川木里耳泽岩溶型金矿床形成条件和成矿机制   总被引:1,自引:0,他引:1       下载免费PDF全文
郑明华  阳正熙 《地质科学》1995,30(4):363-373
四川本里耳泽金-菱铁矿建造矿床,赋存于上二叠统海相碳酸盐岩层中,矿化受古岩溶的严格控制,组成矿石的基本矿物为菱铁矿,金不均匀地分布于菱铁矿矿体内。成矿溶液来自加热的循环地下水。成矿过程分为早阶段和中-晚阶段。成矿温度为156-210℃,成矿深度小于1km.成矿物质主要来自地层。成矿热液呈碱性和弱还原性,贫硫,含中等盐度。矿床形成时的地质构造环境较稳定。这是我国仅见的一种特殊金矿类型。  相似文献   
153.
贵州中三叠统烂泥沟金矿有机质的初步研究   总被引:2,自引:0,他引:2       下载免费PDF全文
李忠  刘铁兵 《地质科学》1995,30(3):283-290
烂泥沟金矿是以浊积岩为容矿岩石的微细浸染型金矿。有机岩石学分析表明,矿石与围岩中干酪根类型无明显差别,同属腐泥-腐植型。与围岩相比,矿石中干酪根成熟度(R0=2.74%-3.06%)和含金性(6.15-24.8μg/g)均较高;干酪根总含金量在全岩中所占的比例是围岩高于矿石。氯仿沥青“A”的检测说明,矿石样品中可溶性有机质形成于强还原和高盐度环境,沥青质和含硫有机化合物发育。研究认为,干酪根含金性与碳的活化有关;不饱和的有机基因对金的动一定转换可能具有重要意义。  相似文献   
154.
安徽冬瓜山铜矿床的地球化学特征   总被引:5,自引:2,他引:5  
冬瓜山铜矿床发育上部层状矿体和下部浸染状—脉状矿体,地球化学特征呈现出明显的垂向变化和二元结构性。从下部浸染状—脉状矿化岩石到上部层状块状矿石,CaO、MgO、Fe2O3、FeO、Cu、Au、Zn、Ag、As等含量和δ18O、δ12C值总体逐渐增高,SiO2、Al2O3、TiO2、K2O、Na2O、Pb、Hg、Sb、Mo、REE等含量和流体包裹体温度379·3℃→135·0℃及δ34S值总体逐渐降低。硬石膏δ34S值为 14·8‰~ 20·5‰,黄铁矿δ34S值为 2·7‰~ 7·9‰,含矿硅质岩δ18O为 12·0‰,含铜矿石中菱铁矿δ18O平均值为 13·97‰。地质地球化学特征反映冬瓜山铜矿床为海底热水喷流沉积成因。  相似文献   
155.
甘肃代家庄铅锌矿的地质特征与找矿意义   总被引:4,自引:1,他引:4  
位于甘肃宕昌县的代家庄矿床曾被认为是西成矿田铅锌找矿的重大进展,矿床产于秦岭西成盆地西北端泥盆系浅海相的富含生物化石的细碎屑岩—灰岩中。矿体不规则受NW向断裂的控制,呈角砾状分布于下部碎屑岩与上部厚层灰岩界面附近灰岩一侧。矿石的矿物共生组合为闪锌矿 方铅矿 少量黄铁矿 少量白铁矿 方解石,不含石英。硫化物发育大量的胶状、球粒状、草霉状微晶结构,部分显现出微生物化石结构特点。对代家庄与西成主要类型铅锌矿床地质地球化学特征的对比发现,二者在容矿围岩沉积环境、矿石形态、结构构造以及同位素地球化学等多方面存在明显的差异,代家庄矿床成因属于碳酸盐岩容矿的低温热液矿床,不同于西成矿田的主要SEDEX类型。主要控矿因素为灰岩—碎屑界面附近、NW向断裂等。  相似文献   
156.
The Taojiang Mn ore deposit was exploited in the early 1960s, and waste rocks were developed since then. Because the Mn ores were hosted within the metal-enriched black shales (Peng et al., 2004), the continuous mining has led to the exposure of an immense quality of black shales, which might cause serious impacts on environments. The present study deals with this environmental issue with samples from the waste rocks, and from the surrounding soils and surface water. The mineralogy of the waste rock was studied using EMPA, then a large number of elements in all waste rock, soil, and water samples were analyzed at a wide range of concentrations with high accuracy using an Elan6000 ICP-MS machine at Guangzhou Institute of Geochemistry, Chinese Academy of Sciences. The waste rock is composed mostly of black shales, with minor Mn carbonates. Both black shales and Mn carbonates of the waste rock contain many sulfide minerals, mainly pyrite, with minor galena, sphalerite, chalcopyrite, and others. The waste rocks are enriched in many metals including Sc, V, Cr, Co, Ni, Fe, Mn, Cu, Zn, Pb, Th, U, Mo, Sb, Sn, Tl, and others, and the metals are mostly hosted within the sulfides. Weathering of waste rocks might cause emission of the following metals: V, Cd, Ni, Th, U, Mo, Sb, Tl, Sc, Cr, Cu, Zn, Sn, and minor Co, and Pb. The surrounding soils are highly enriched in Cr, Co, Cu, Zn, Mn, Mo, Cd, Tl, and Pb, with the enrichment factors of 2.67.3.8, 7.26, 7.27, 8.2, 5.7, 13, and 5.4, respectively. The element ratios (Rb/Cs, Fe/Mn, Nb/Zr, Hf/Zr, and Ba/Sr) and REE distribution patterns of the soils are similar to those of the waste rocks and bedrocks.  相似文献   
157.
Dajing is a large-scale tin–polymetallic deposit that hosts the largest tin mine in North China. It is a hydrothermal vein-type deposit containing Sn, Cu, Pb, Zn, Ag, and minor components Co and In. The deposit consists of more than 690 veins hosted within Upper Permian sedimentary rocks.Three mineralization stages and six ore types are recognized with cassiterite constituting the dominant tin mineral. The SnO2 content of cassiterite increases in the sequence of mineralization stages shear-deformation→cassiterite–quartz→cassiterite–sulfide (or chalcopyrite–pyrite) stage, while the content of FeO, TiO2, Nb2O5, Ta2O5, and In2O5 tends to decrease with increases in NiO and Ga2O5. It is considered that the negative correlation between SnO2 and FeO, Nb2O5, Ta2O5, and In2O5 results from elemental substitutions. The early stage cassiterite is much richer in Ta and the later stage cassiterite is much poorer in Ti and Fe than is usual in hydrothermal vein type tin deposits. This is interpreted to indicate that the component of early stage cassiterite reflects a granitic magma source while the composition of later stage cassiterite has a more obvious strata source. The compositional variation of cassiterite corresponds to decreasing crystallization temperatures within each stage and between sequential stages with time. The characteristics of REE in cassiterite from two stages are in accord with that of subvolcanic rocks and the Linxi formation. It suggests that tin transported during the cassiterite–quartz stage may have originated from subvolcanic dikes (e.g., dacite porphyry), while in the cassiterite–sulfide stage, tin may have been derived from wallrock (e.g. siltstone) of the Upper Permian-age Linxi Formation.  相似文献   
158.
位于新疆西南天山阿合奇县的布隆金矿是一个国内较少见的低温热液石英重晶石脉型金矿床,它赋存于上泥盆统细碎屑岩中,金矿体受层间缓倾斜破碎带控制。根据矿脉矿物组合及相互穿插关系,原生成矿期成矿作用可分为:①黄铁矿-石英阶段;②石英-黄铁矿-菱铁矿-重晶石阶段;③方解石-石英-重晶石阶段和④重晶石阶段。年代学研究表明,主成矿阶段(②阶段)含金石英脉RB-SR等时线年龄为258±15MA,表明成矿作用发生在晚二叠世末,与中亚南天山大规模的金成矿作用发生时期相一致。  相似文献   
159.
Abstract. Major and trace element contents are reported for Permian manganese ore and associated greenstone from the Ananai manganese deposit in the Northern Chichibu Belt, central Shikoku, Japan. The manganese deposit occurs between greenstone and red chert, or among red chert beds. Chemical compositions of manganese ore are characterized by enrichments in Mn, Ca, P, Co, Ni, Zn, Sr and Ba, and negative Ce and positive Eu anomalies relative to post-Archean average Australian Shale (PAAS). Geochemical features of the manganese ore are similar to those of modern submarine hydrother-mal manganese deposits from volcanic arc or hotspot setting. In addition, geochemical characteristics of the greenstone closely associated with the Ananai manganese deposit are analogous to those of with-in plate alkaline basalt (WPA). Consequently, the Ananai manganese deposit was most likely formed by hydrothermal activity related to hotspot volcanism in the Panthalassa Ocean during the Middle Permian. This is the first report documenting the terrestrially-exposed manganese deposit that was a submarine precipitate at hotspot.  相似文献   
160.
Great earthquakes of variable magnitude at the Cascadia subduction zone   总被引:1,自引:0,他引:1  
Comparison of histories of great earthquakes and accompanying tsunamis at eight coastal sites suggests plate-boundary ruptures of varying length, implying great earthquakes of variable magnitude at the Cascadia subduction zone. Inference of rupture length relies on degree of overlap on radiocarbon age ranges for earthquakes and tsunamis, and relative amounts of coseismic subsidence and heights of tsunamis. Written records of a tsunami in Japan provide the most conclusive evidence for rupture of much of the plate boundary during the earthquake of 26 January 1700. Cascadia stratigraphic evidence dating from about 1600 cal yr B.P., similar to that for the 1700 earthquake, implies a similarly long rupture with substantial subsidence and a high tsunami. Correlations are consistent with other long ruptures about 1350 cal yr B.P., 2500 cal yr B.P., 3400 cal yr B.P., 3800 cal yr B.P., 4400 cal yr B.P., and 4900 cal yr B.P. A rupture about 700-1100 cal yr B.P. was limited to the northern and central parts of the subduction zone, and a northern rupture about 2900 cal yr B.P. may have been similarly limited. Times of probable short ruptures in southern Cascadia include about 1100 cal yr B.P., 1700 cal yr B.P., 3200 cal yr B.P., 4200 cal yr B.P., 4600 cal yr B.P., and 4700 cal yr B.P. Rupture patterns suggest that the plate boundary in northern Cascadia usually breaks in long ruptures during the greatest earthquakes. Ruptures in southernmost Cascadia vary in length and recurrence intervals more than ruptures in northern Cascadia.  相似文献   
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