Geology and mineralization of the supergiant Shimensi granitic-type W-Cu-Mo deposit (1.168 Mt) in northern Jiangxi,South China: A Review     

《China Geology》2022,5(3):510-527

The Shimensi deposit is a recently discovered W-Cu-Mo polymetallic deposit located in the Jiangnan porphyry-skarn W belt in South China. The deposit has a resource of 0.74×10⁶ t of WO₃ accompanied by 0.4×10⁶ t Cu and 28000 t Mo and other useful components like Ga, making it one of the largest W deposits in the world. This paper is aimed to reveal the ore-controlling mechanisms of the Shimensi deposit, involving the role of the ore-related granites, the tectonic background for its formation, and the metallogenesis model. The systematic geological survey suggests multi-types of alteration are developed in the deposit, mainly including greisenization, potassic-alteration, sericitization, chloritization, and silicification. Drilling engineering data and mining works indicate that the Shimensi deposit consists of two main orebodies of I and II. Therein, the W resource has reached a supergiant scale, and the accompanied Cu, Mo, Au, Bi, Ga, and some other useful components are also of economic significance. The main ore-minerals consist of scheelite, wolframite and chalcopyrite. Disseminated mineralization is the dominant type of the W-Cu-Mo polymetallic orebodies, and mainly distributes in the inner and external contact zone that between the Neoproterozoic biotite granodiorite and the Yanshanian granites. The main orebody occurs at the external contact zone, and the pegmatoid crust near the inner contact zone is an important prospecting marker of the W mineralization. Of them, the disseminated W ores within the wall rock of the Neoproterozoic biotite granodiorite is a new mineralization type identified in this paper. Combining previous geochronological and isotopic data, we propose that the mineralization of the Shimensi deposit is closely related to the intruding of the Yanshanian porphyritic biotite granite and granite porphyry. Geochemical data suggest that the biotite granodiorite is rich in Ca and had provided a large amount of Ca for the precipitation of scheelite in this area. Thus, it is a favorable wall rock type for W mineralization. The Shimensi deposit belongs to granitic-type W polymetallic deposit related to post-magmatic hydrothermal, and the ore-forming fluid was initially derived from the Yanshanian magmas.©2022 China Geology Editorial Office.  相似文献   

Chemical composition of garnet from the Xintianling skarn W deposit in southern Hunan and its geological significanceSCIEI北大核心CSCD     

郁凡  舒启海  曾庆文  马星华  牛旭东  马绍龙  李一昕  邢凯 《岩石学报》2022,38(1):78-90

新田岭矿床是南岭钨锡成矿带中的一个大型矽卡岩型钨矿床,产于骑田岭岩体东北部与石炭系碳酸盐地层的接触带位置。本文运用LA-ICP-MS技术对该矿床矽卡岩中的石榴子石进行了系统的成分分析,获得了其主量、微量和稀土元素含量。结果显示,新田岭矿床中的石榴子石属于钙铁榴石-钙铝榴石固溶体系列(And₂₄Gro₆₆ -And₇₁Gro₂₂),石榴子石的端元成分在富钙铝榴石和富钙铁榴石之间变化。稀土元素的配分模式也同时出现了左倾、Eu负异常和右倾、Eu正异常两种类型,暗示新田岭矿床石榴子石结晶过程中热液流体存在不同的氧化还原环境和水/岩比条件,这也与其晶体中是否出现振荡环带相对应。将不同矽卡岩型矿床中石榴子石的W、Sn含量进行对比显示,含W矿化的矽卡岩型矿床中石榴子石的W、Sn含量整体上显著高于不含W矿化的矿床,指示石榴子石中的W、Sn含量在一定程度上具有预测矽卡岩型矿床成W矿潜力的作用。此外,石榴子石中Fe、Eu、U等元素的含量还可以进一步区分矽卡岩W矿床中的伴生金属元素类型(包括W-Mo、W-Sn、W-Cu-...  相似文献   

Fe(Ⅱ)/针铁矿复合系统对水中橙黄G的吸附-还原脱色研究     

赵丹  肖丹玲  何广平  吴宏海 《岩石矿物学杂志》2015,34(1):97-102

系统研究了Fe(Ⅱ)/针铁矿复合系统对偶氮染料橙黄G(简称OG)的吸附-还原脱色机理,重点考察了反应条件p H值、Fe(Ⅱ)与OG摩尔比对OG还原脱色效果的影响。研究结果表明,矿物表面结合态Fe(Ⅱ)能够有效提高还原脱色反应速率;OG脱色反应非常符合准一级反应动力学方程,速率常数(k)随p H值的升高、亚铁离子吸附量的增加而显著增大;当OG初始浓度为50 mg/L、Fe(Ⅱ)与OG的摩尔比为27.0时,Fe(Ⅱ)/针铁矿复合系统对OG的去除脱色率在弱碱性条件下1 h内可达到100%。该系统对OG去除脱色的高效性是界面吸附与还原协同作用的结果。该研究可为有效应用Fe(Ⅱ)/针铁矿复合系统在缺氧环境中的污染修复提供理论指导。  相似文献   

渤海海域W油田新近系明化镇组河流相砂体结构特征   总被引：1，自引：0，他引：1  

陈飞  胡光义  范廷恩  孙立春  高云峰  王晖 《地学前缘》2015,22(2):207-213

利用野外露头、现代沉积和大量岩心以及钻测井资料,以高分辨率层序地层学原理为指导,结合地震和探地雷达,分析了W油田新近系明化镇组明下段河流相层序格架和砂体结构的沉积特征,总结了砂体的发育规模特征,建立了河流相砂体的沉积模式,为海上油田开发及后期调整提供依据和指导。研究表明,渤海海域明化镇组河流相砂体结构划分为堆叠型、侧叠型和孤立型3种类型共7种样式,其中侧叠型又分为紧密型、疏散型和离散型;孤立型又分为下切侵蚀型、孤立河道和决口扇;河道砂体厚度为2.1~15m,平均6.75m;宽度为200~1 225m,平均宽度519m。决口扇砂体厚约2~3m,宽度为150~450m,平均宽度300m。河流相砂体结构受控于湖平面的变化。不同的湖平面变化下发生堆叠型、侧叠型和孤立型规律性的砂体结构变化。  相似文献   

A MERLIN survey of 4.7-GHz excited OH masers in star-forming regions     

L. Harvey-Smith  R. J. Cohen 《Monthly notices of the Royal Astronomical Society》2005,356(2):637-646

Phase-referenced observations of 13 star-forming regions in the  ²Π_1/2, J = 1/2  transition of rotationally excited OH at 4765 MHz have been carried out using MERLIN. Two of the regions were also observed at 4750 MHz and one at 4660 MHz. There were 10 maser detections at 4765 MHz and three non-detections. There were no detections at 4750 and 4660 MHz. The 4765-MHz masers have brightness temperatures of  ∼10⁷ K  at MERLIN resolution (∼50 mas). Several cases of 4765-MHz masers overlapping in position and velocity with 1720- and 1665-MHz masers are reported. There are also isolated 4765-MHz masers with peak flux densities ≥30 times that of any ground-state counterpart. Most of the 4.7-GHz maser spots are unresolved at 50-mas angular resolution, but in four of the nearest sources the maser spots are resolved, indicating a characteristic size for 4765-MHz maser regions of ∼100 au. In W3(OH) we discovered that 20 per cent of the 4765-MHz emission comes from a narrow low-brightness filament that stretches north–south for ∼1.0 arcec (∼2200 au) between two previously known 4765-MHz maser spots. The filament appears in projection against the H  ii region and has a brightness temperature of  ∼4 × 10⁵ K  . There are matching absorption features in mainline transitions of highly excited OH. The filament may trace a shock front in a rotating disc.  相似文献   

The Type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope     

Nikolai N. Chugai  Sergei I. Blinnikov  Robert J. Cumming  Peter Lundqvist  Angela Bragaglia  Alexei V. Filippenko  Douglas C. Leonard  Thomas Matheson  Jesper Sollerman 《Monthly notices of the Royal Astronomical Society》2004,352(4):1213-1231

  相似文献   

W UMa型相接双星的理论研究     

李立芳  张奉辉 《天文研究与技术》2004,1(1):1-15

本文回顾了W UMa型相接双星观测和理论研究的历史。总结了W UMa型相接双星观测特性和理论研究的成果。最后讨论了W UMa型相接双星理论模型研究中存在的问题及其解决这些问题的一些可行方法。  相似文献   

Photometric Study Of W Uma Type Binary In The Old Cluster Ngc 6791     

J.?Rukmini  P.?Vivekananda?RaoEmail author  K.?Sriram 《Astrophysics and Space Science》2005,299(2):109-116

Study of eclipsing binaries in an open cluster offer information regarding the age of the cluster in addition to the component stars. In this paper we present the analysis of a W UMa system discovered in the open cluster NGC 6791 using the Wilson–Devinney (W–D) method.  相似文献   

测量船的摇动对AIRSEA SystemⅡ的干扰分析     

于富强 《北京测绘》2012,(6):11-13

根据海洋重力测量的实际情况,结合AIRSEA SystemⅡ的结构特点,对仪器在测量中受到测量船摇动的影响进行分析,认为影响仪器观测精度的干扰因素有三类:垂直加速度、横摇与纵摇、交叉耦合效应。并对这三种干扰因素进行分析,给出了减弱干扰影响的措施,这些措施能使海洋重力测量外业获取更高的观测精度。  相似文献   

Search for VHE gamma rays from SS433/W50 with the CANGAROO-II telescope     

《Astroparticle Physics》2009,32(2):112-119

SS433, located at the center of the supernova remnant W50, is a close proximity binary system consisting of a compact star and a normal star. Jets of material are directed outwards from the vicinity of the compact star symmetrically to the east and west. Non-thermal hard X-ray emission is detected from lobes lying on both sides. Shock accelerated electrons are expected to generate VHE gamma rays through the inverse-Compton process in the lobes. Observations of the western X-ray lobe region of SS433/W50 system have been performed to detect VHE gamma rays using the 10 m CANGAROO-II telescope in August and September, 2001, and July and September, 2002. The total observation times are 85.2 h for ON source, and 80.8 h for OFF source data. No significant excess of VHE gamma rays has been found at three regions of the western X-ray lobe of SS433/W50 system. We have derived 99% confidence level upper limits to the fluxes of gamma rays and have set constraints on the strengths of the magnetic fields assuming the synchrotron/inverse-Compton model for the wide energy range of photon spectrum from radio to TeV. The derived lower limits are G for the center of the brightest X-ray emission region and G for the far end from SS433 in the western X-ray lobe. In addition, we suggest that the spot-like X-ray emission may provide a major contribution to the hardest X-ray spectrum in the lobe.  相似文献