青山洞金矿床成因及找矿模型探讨     

唐卫国 《矿产与地质》2009,23(5):426-430

青山洞金矿位于湖南西南部的雪峰弧形构造成矿带上,是该成矿区带近年来新发现的重要金矿床。通过对青山洞金矿床地质特征的研究,分析其矿床成因类型属构造岩浆＋变质热液并以充填交代方式形成的韧脆性剪切带型金矿床,具硫化物-自然金矿石建造,工业类型为破碎蚀变岩型。并初步总结了成矿模式并建立了找矿模型,为寻找同类型金矿提供参考和指导。  相似文献   

河北省丰宁县茶棚银矿地质、地球物理特征及找矿意义     

郭长华  高明  张翔军  高州  孟令革  高雄  李会凯 《矿产与地质》2009,23(5):462-468

茶棚银矿位于河北省北部坝上草原向山区过渡地带,风成砂覆盖严重,示矿标志不明显,地表找矿难度大;地表矿体断续出露,而深部银矿体主要以隐伏矿体的形式赋存于近南北向展布的构造破碎带中,数量明显增多、品位变富、厚度变大;在这种特殊的景观地质特征下,利用激电中梯扫面,可发现厚覆盖状态下构造矿化蚀变带,利用EH4连续导电率测量可厘定矿化蚀变带的规模、产状并可提供隐爆角砾岩体等深部控矿地质信息,利用可控源音频大地电磁测深的中低阻陡变带和中阻带,特别是陡变带中的转折部位（形态呈耳状部位）可具体定位银矿体的赋存空间。  相似文献   

阿曼Daleel油田下白垩统Shuaiba组上段走滑正断裂带裂缝分布定量评价   总被引：1，自引：1，他引：0  

周文  邓虎成  赵国良  杨宇  谢润成 《矿物岩石》2009,29(4)

在对阿曼Daleel油田下白垩统Shuaiba组上段的岩芯及成像测井裂缝特征进行分析的基础上,利用过断层的水平井成像测井资料,开展对断层两侧的裂缝发育情况研究,分析认为裂缝发育密度与离断层的距离相关,提出裂缝成因主要受区内走滑正断层所控制.研究建立的3类不同规模的走滑正断层带裂缝密度分布函数,实现了对阿曼Daleel油田下白垩统Shuaiba组上段断裂带裂缝分布的定量评价.  相似文献   

Records of Indosinian Orogenesis in Lhasa Terrane, Tibet     

Li Huaqi  Xu Zhiqin  Yang Jingsui  Cai Zhihui  Chen Songyong  Tang Zemin 《中国地质大学学报(英文版)》2009,20(2)

Based on the deformation characteristics of the ductile shear zones in Sumdo (松多) Group, the quartz fabric by EBSD (electron backscatter diffraction), the data of muscovite 40Ar-39Ar geochronology (220-230 Ma) from ductile shear zones and the zircon SHRIMP U-Pb chronology (190 Ma) of granites in Snmdo region, Lhasa (拉萨) terrane is thought to have experienced an important Indosinian orogenic event at 220-230 Ma, which caused the closure of the paleo-Tethys Ocean along the tectonic zone of eclogite and the collision between northern part and southern part of the Lhasa terrane. The zircon SHRIMP U-Pb chronology of 190 Ma for biotite adamellite, with the distributing characteristics of the granite massif intruding in Sumdo Group, indicates that the biotite adamellitc should be the late orogenic or post-orogenic granite resulting from the lndosinian orogenesis. The discovery of Indosinian orogenic belt in Lhasa terrane expansed the southern boundary of lndosinian orogenic belt in Qinghai (青海)-Tibet plateau to Lhasa terrane from Qiangtang (羌塘) terrane, which changed the understanding about the distribution of Indosinian orogenic belt in Qinghai-Tibet plateau and extended the "T" type lndosinian orogenic belt in China. The study is very important for the formation and distribution of paleo-Tethys Ocean in Tibet. The ancient terrane framework and evolution of Qinghai-Tibet plateau need further research.  相似文献   

新疆阿尔泰金矿带主要金矿类型、成矿规律及成矿预测   总被引：7，自引：0，他引：7  

沈远超  申萍  曾庆栋  刘铁兵  李光明 《地质与勘探》2004,40(5):1-5

新疆阿尔泰金矿带金矿分布广泛,主要类型有火山晚期热液型金矿床、与韧性剪切带有关的金矿床.对不同类型金矿床基本成矿特征进行了研究,探讨了不同类型金矿床的控矿作用,在此基础上总结了阿尔泰金矿带主要金矿类型的成矿规律,对主要金矿深部进行了成矿预测,发现并圈出了矿床深部的矿化异常.  相似文献   

广西丹池成矿带构造特征及其控矿作用   总被引：26，自引：2，他引：24  

蔡明海  梁婷  吴德成  黄惠民 《地质与勘探》2004,40(6):5-10

丹池成矿带是我国锡多金属矿业的重要基地和超大型大厂锡多金属矿床的产出地,通过构造地质调查,在成矿带内识别出两套不同的变形构造样式和构造组合,它们分别对应于印支期挤压变形和燕山中-晚期伸展.在此基础上对控制成矿带、矿田及矿床的构造特征进行了分析,总结了带内矿床定位的两类构造组合形式.  相似文献   

新疆库车地区秋里塔格构造带成因分析   总被引：14，自引：4，他引：10       下载免费PDF全文

齐英敏  苗继军  马全天  吴建国  张国伟  叶林  李毓丰  桑洪 《地质科学》2004,39(4):561-570

秋里塔格构造带位于库车前陆逆冲带前锋,区域构造位置介于库车坳陷三叠-侏罗系烃源岩生排烃中心与塔北前缘隆起带之间,第三系广泛分布两套膏盐岩层,发育多套储盖组合和复杂的构造样式,石油地质条件非常优越.本文在分析3个区带的变形特征基础上,探讨了盐上层和盐下层的构造成因,认为盐上层的构造成因与盐层的流动性有关,西段变形比东段强烈;盐下层构造成因东、西差异较大,东段与盐层的塑性变形无关,西段则受其影响.  相似文献   

新疆西部苏盖特构造带构造特征及勘探前景   总被引：4，自引：4，他引：0       下载免费PDF全文

吴超  尚新璐  陈军  王晓云 《地质科学》2004,39(4):571-579

苏盖特构造带位于新疆昆仑山弧形推覆体前缘.本文通过研究苏盖特构造带的构造特征,确定了地震反射层的地质属性,认为苏盖特构造带由表层推覆体及下部下第三系-二叠系之间的地层经过3次重复形成的叠瓦状推覆体构成.苏盖特构造带活动始于上新世阿图什组沉积期,定型于更新世.通过研究西昆仑逆冲推覆体及已钻探井的地表油源、储层特征及储盖组合,认为苏盖特构造带具有两套好的油源即石炭-二叠系及侏罗系油源,两套好的储集层即白垩系和下第三系储层,相应地,发育两套储盖组合,具有良好的圈闭及运聚条件,是有利的勘探目标区.  相似文献   

EURONEAR—Recovery, follow-up and discovery of NEAs and MBAs using large field 1–2 m telescopes     

O. Vaduvescu  M. Birlan  A. Tudorica  A. Sonka  F.N. Pozo  A.D. Barr  D.J. Asher  J. Licandro  J.L. Ortiz  E. Unda-Sanzana  M. Popescu  A. Nedelcu  D. Dumitru  R. Toma  I. Comsa  C. Vancea  D. Vidican  C. Opriseanu  T. Badescu  M. Badea  M. Constantinescu 《Planetary and Space Science》2011,59(13):1632-1646

We report on the follow-up and recovery of 100 program NEAs, PHAs and VIs using the ESO/MPG 2.2 m, Swope 1 m and INT 2.5 m telescopes equipped with large field cameras. The 127 fields observed during 11 nights covered 29 square degrees. Using these data, we present the incidental survey work which includes 558 known MBAs and 628 unknown moving objects mostly consistent with MBAs from which 58 objects became official discoveries. We planned the runs using six criteria and four servers which focus mostly on faint and poorly observed objects in need of confirmation, follow-up and recovery. We followed 62 faint NEAs within one month after discovery and we recovered 10 faint NEAs having big uncertainties at their second or later opposition. Using the INT we eliminated four PHA candidates and VIs. We observed in total 1286 moving objects and we reported more than 10,000 positions. All data were reduced by the members of our network in a team effort, and reported promptly to the MPC. The positions of the program NEAs were published in 27 MPC and MPEC references and used to improve their orbits. The O−C residuals for known MBAs and program NEAs are smallest for the ESO/MPG and Swope and about four times larger for the INT whose field is more distorted. For the astrometric reduction, the UCAC-2 catalog is recommended instead of USNO-B1. The incidental survey allowed us to study statistics of the MBA and NEA populations observable today with 1–2 m facilities. We calculate preliminary orbits for all unknown objects, classifying them as official discoveries, later identifications and unknown outstanding objects. The orbital elements a, e, i calculated by FIND_ORB software for the official discoveries and later identified objects are very similar with the published elements which take into account longer observational arcs; thus preliminary orbits were used in statistics for the whole unknown dataset. We present a basic model which can be used to distinguish between MBAs and potential NEAs in any sky survey. Based on three evaluation methods, most of our unknown objects are consistent with MBAs, while up to 16 unknown objects could represent NEO candidates and four represent our best NEO candidates. We assessed the observability of the unknown MBA and NEA populations using 1 and 2 m surveys. Employing a 1 m facility, one can observe today fewer unknown objects than known MBAs and very few new NEOs. Using a 2 m facility, a slightly larger number of unknown than known asteroids could be detected in the main belt. Between 0.1 and 0.8 new NEO candidates per square degree could be discovered using a 2 m telescope.  相似文献   

Mafic dykes derived from Early Cretaceous depleted mantle beneath the Dabie orogenic belt: implications for changing lithosphere mantle beneath Eastern China     

Ling Chen  Chang Q. Ma  Jin Y. Zhang  Roger Mason  Chao Zhang 《Geological Journal》2011,46(4):333-343

SHRIMP zircon U–Pb geochronological, elemental and Sr–Nd isotopic data from Early Cretaceous mafic dykes in North Dabie orogenic belt elucidate a change of Mesozoic lithospheric mantle in eastern China. The dykes are predominantly dolerite with the major mineral assemblage clinopyroxene + hornblende + plagioclase and yield a SHRIMP zircon U–Pb age of 111.6 ± 5.3 Ma. They have a narrow range of SiO₂ from 46.16% to 49.78%, and relative low concentrations of K₂O (1.07−2.62%), Na₂O (2.45−3.54%), Al₂O₃ (13.04−14.07%), and P₂O₅ (0.42−0.55%) but relatively high concentration of MgO (5.94–6.61%) with Mg^# 52–54. All the samples are characterized by enrichment of large ion lithophile elements (LILE, e.g., Ba, Th) and high field strength elements (HFSE, e.g., Nb, Ti). (⁸⁷Sr/⁸⁶Sr)_i ratios from 0.704 to 0.705, ε_Nd values from 3.36 to 4.33 and mantle‐depletion Nd model ages (T_2DM) in the range 0.56–0.64 Ga indicate that the magma of the Baiyashan mafic dykes was derived from a young depleted mantle source. This finding is different from previous research on mafic dykes in the age range 120–138 Ma that revealed enrichment of LILE and depletion of HFSE, high initial Sr isotopic ratios and negative ε_Nd, value which represents an old enriched mantle source. Ours is the first report of the existence of Early Cretaceous depleted mantle in eastern China and it implies that changing of enriched mantle to depleted mantle occurred at ca. 112 Ma, associated with back‐arc extension which resulted from the subduction of the Palaeo‐Pacific Plate towards the Asian Continent. Copyright © 2010 John Wiley & Sons, Ltd.  相似文献