青海同仁县江里沟斑岩-矽卡岩型铜钨钼矿床辉钼矿Re-Os同位素年龄及其成矿意义     

张涛  张德会  杨兵  张辉  喻晓 《地质学报》2015,89(2):355-364

西秦岭同德—泽库多金属成矿带是青海省重要的矿产集中区之一,位于西秦岭北缘斑岩-矽卡岩型铜、钼、金成矿带的最西端。江里沟矿床是该区的重要组成部分,为一个典型的斑岩型-矽卡岩型铜钨钼矿床。本文利用Re-Os同位素定年方法对江里沟铜钨钼矿床进行了成矿时代测定,获得了5件样品辉钼矿的Re-Os同位素模式年龄范围为219.5±3.1~222.2±4.0Ma,等时线年龄为224.3±7.3Ma。矿区二长花岗岩SHRIMP锆石UPb年龄测定结果表明岩石存在两个期次结晶年龄232±4Ma和214±4Ma,矿区花岗岩可能是两个期次岩浆活动的产物。根据斑岩型矿床矿化晚于成矿母岩的特征,认为江里沟矿床成矿时代属晚三叠世,与矿区232Ma期次的岩浆侵入活动关系密切,成矿晚于成岩约8Ma,成矿与成岩时代基本一致,是西秦岭印支期构造-岩浆活动的产物。本次研究可以大致确定岗察复式岩体周边矿床成矿时限为243.8~214Ma,与区域西秦岭—东昆仑三叠纪构造岩浆作用和成矿时代一致,构成西秦岭北缘斑岩-矽卡岩型铜-钼-金成矿系统的一部分。  相似文献   

Re–Os and U–Pb Geochronology of Porphyry and Skarn Types Copper Deposits in Jilin Province,NE China          下载免费PDF全文

Yong Zhang  Shu–Wen Xing  Quan–Heng Song  Yan Wang  Zheng–Tao Yu  Xiao–Hui Du  Yu–Bo Ma  Zeng–Jie Zhang 《Resource Geology》2015,65(4):394-404

Jilin Province in NE China lies on the eastern edge of the Xing–Meng Orogenic Belt. Mineral exploration in this area has resulted in the discovery of numerous large, medium, and small sized Cu, Mo, Au, and Co deposits. To better understand the formation and distribution of both the porphyry and skarn types Cu deposits of the region, we examined the geological characteristics of the deposits and applied zircon U–Pb and molybdenite Re–Os isotope dating to constrain the age of the mineralization. The Binghugou Cu deposit yields a zircon U–Pb age for quartz diorite of 128.1 ± 1.6 Ma; the Chang'anpu Cu deposit yields a zircon U–Pb age for granite porphyry of 117.0 ± 1.4 Ma; the Ermi Cu deposit yields a zircon U–Pb age for granite porphyry of 96.8 ± 1.1 Ma; the Tongshan Cu deposit yields molybdenite Re–Os model ages of 128.7 to 130.2 Ma, an isochron age of 129.0 ± 1.6 Ma, and a weighted mean model age of 129.2 ± 0.7 Ma; and the Tianhexing Cu deposit yields molybdenite Re–Os model ages of 113.9 to 115.2 Ma, an isochron age of 114.7 ± 1.2 Ma, and a weighted mean model age of 114.7 ± 0.7 Ma. The new ages, combined with existing geochronology data, show that intense porphyry and skarn types Cu mineralization was coeval with Cretaceous magmatism. The geotectonic processes responsible for the genesis of the Cu mineralization were probably related to lithospheric thinning. By analyzing the accumulated molybdenite Re–Os, zircon U–Pb, and Ar–Ar ages for NE China, it is concluded that the Cu deposits formed during multiple events coinciding with periods of magmatic activity. We have identified five phases of mineralization: early Paleozoic (~476 Ma), late Paleozoic (286.5–273.6 Ma), early Mesozoic (~228.7 Ma), Jurassic (194.8–137.1 Ma), and Cretaceous (131.2–96.8 Ma). Although Cu deposits formed during each phase, most of the Cu mineralization occurred during the Cretaceous.  相似文献   

基于ETM~+数据和GIS技术的缅甸铜金矿成矿预测     

独文惠  王功文  陈永清  郭娜娜  郝应龙  冯源 《地质通报》2015,34(4):786-791

在利用遥感数据和地理信息系统(GIS)技术的矿产资源勘查与评价中,矿化蚀变信息提取和构造信息提取起着至关重要的作用。以缅甸铜金矿为例,利用ETM+遥感图像,采用比值法、阈值分割和主成分分析(PCA)提取羟基蚀变信息;利用数字高程模型和遥感数据提取与铜金矿化有关的线环构造,结合地质资料和上述信息,利用证据权和分形方法进行整合,确定该研究区的成矿远景区。结果发现,已知铜金矿均分布于成矿靶区中,综合信息可为下一步的矿产资源勘探工作提供决策依据。  相似文献   

俄罗斯远东岗仁地体金铜矿床地质、地球化学特征及其LA-ICP-MS锆石U-Pb年龄     

张国宾  杨言辰  Khomich V G  叶松青  李海洋  王林  郝明  王庆双 《地质通报》2015,34(4):618-629

岗仁地体位于额尔古纳超地体北部边缘,蒙古—鄂霍茨克构造带南部,该区分布着大量的大型、超大型金矿床,这些矿床在成因上与中酸性侵入岩和浅成次火山岩关系密切。岩石地球化学研究表明,花岗闪长岩-闪长岩组合明显富集大离子亲石元素、不相容元素和轻稀土元素,亏损高场强元素和重稀土元素。球粒陨石标准化稀土配分模式为轻稀土元素富集、重稀土元素亏损的右倾型,具有微弱的负Eu异常或基本无Eu异常,无Ce异常,元素地球化学性质反映出花岗闪长岩-闪长岩组岩浆具有壳幔混合的特征,且形成于大陆边缘的火山弧环境。LA-ICP-MS锆石U-Pb测年结果揭示,皮奥涅尔金银矿床含矿闪长玢岩的206Pb/238U年龄加权平均值为113.8±2.0Ma,博尔古利坎铜金钼矿床赋矿二长闪长斑岩的206Pb/238U年龄加权平均值为112.7±2.8Ma,与皮奥涅尔金银矿床和博尔古利坎铜金钼矿床成矿有关的奥列佳花岗闪长岩体的年龄分别为117.2±1.3Ma和117.0±3.6Ma。由此可知,皮奥涅尔金银矿床和博尔古利坎铜金钼矿床形成于燕山早期,与中国黑龙江地区三道湾子金矿、东安金矿等金矿床形成时代一致。  相似文献   

川北早寒武世碳酸盐岩台缘斜坡沉积特征及变形构造形成机制探讨   总被引：2，自引：2，他引：0       下载免费PDF全文

沈骋  谭秀成  李凌  施开兰  苏成鹏  连承波  黎虹玮  肖笛 《古地理学报》2015,17(3):321-334

基于对川北米仓山西部旺苍县鼓城乡唐家河下寒武统仙女洞组露头剖面的观察与镜下分析发现,仙女洞组下段由生物碎屑泥晶灰岩(L)、粉砂质泥岩(M)、似瘤状砾屑灰岩(L')、角砾灰岩(R)、藻凝块灰岩(A)和含生屑钙质砂岩(S)组合而成,其以角砾灰岩、似瘤状砾屑灰岩和藻凝块灰岩为特征,且发育异地岩块和滑塌变形构造。进一步分析认为:L-M岩石组合为正常的斜坡环境低能沉积;L'-R岩石组合中的角砾灰岩为上斜坡生物灰泥丘崩坍滑动至下部而形成的,似瘤状砾屑灰岩可能是由于L-M岩石组合快速沉积导致沉积物失稳滑动变形、上斜坡生物灰泥丘崩落角砾致使的差异压实和滑动、以及后期物质成分差异引起的压溶作用等共同作用的结果,从而使灰质层发生破碎并被泥质包围形成断续的砾屑状,甚至轻微的位移,进而形成条带特征不明显的杂乱变形构造;微生物岩(Mb)组合为上斜坡的灰泥丘沉积;S-M岩石组合为斜坡上部的浊流沉积。根据上述分析结果建立米仓山西部仙女洞组碳酸盐岩台缘斜坡沉积模式,表明仙女洞组沉积早期米仓山西部存在台缘斜坡相沉积。  相似文献   

青藏高原北部巴颜喀拉山群英安质沉凝灰岩LA-ICP-MS锆石U-Pb年龄     

张耀玲  胡道功  吴珍汉  郝爽  刘嘉麒 《地质通报》2015,34(5):809-814

应用激光烧蚀多接收器电感耦合等离子体质谱仪(LA-ICP-MS)方法,对青藏高原北部卡巴纽尔多湖西牙扎康塞一带巴颜喀拉山群碎屑岩系英安质沉凝灰岩夹层中的锆石进行了U-Pb同位素测定。研究结果表明,除1个继承锆石206Pb/238U年龄为419±3Ma外,其余20个岩浆锆石的206Pb/238U年龄变化于242~254Ma之间,其中7个测点的206Pb/238U年龄加权平均值为244±2Ma(MSWD=1.3),代表了火山岩的喷发年龄,说明该地区巴颜喀拉山群形成于中三叠世早期,而非传统认为的晚三叠世。该套地层时代的确定,为进一步研究巴颜喀拉山群的物质组成与形成时代提供了新的证据。  相似文献   

The inner solar system cratering record and the evolution of impactor populations   总被引：1，自引：0，他引：1  

Robert G.Strom  Renu Malhotra  Zhi-Yong Xiao  Takashi Ito  Fumi Yoshida  Lillian R Ostrach 《天文和天体物理学研究(英文版)》2015,(3):407-434

We review previously published and newly obtained crater size-frequency distributions in the inner solar system. These data indicate that the Moon and the terrestrial planets have been bombarded by two populations of objects. Population 1,dominating at early times, had nearly the same size distribution as the present-day asteroid belt, and produced heavily cratered surfaces with a complex, multi-sloped crater size-frequency distribution. Population 2, dominating since about 3.8–3.7 Gyr,had the same size distribution as near-Earth objects(NEOs) and a much lower impact flux, and produced a crater size distribution characterized by a differential –3single-slope power law in the crater diameter range 0.02 km to 100 km. Taken together with the results from a large body of work on age-dating of lunar and meteorite samples and theoretical work in solar system dynamics, a plausible interpretation of these data is as follows. The NEO population is the source of Population 2 and it has been in near-steady state over the past ～ 3.7–3.8 Gyr; these objects are derived from the main asteroid belt by size-dependent non-gravitational effects that favor the ejection of smaller asteroids. However, Population 1 was composed of main belt asteroids ejected from their source region in a size-independent manner, possibly by means of gravitational resonance sweeping during orbit migration of giant planets;this caused the so-called Late Heavy Bombardment(LHB). The LHB began some time before ～3.9 Gyr, peaked and declined rapidly over the next ～ 100 to 300 Myr,and possibly more slowly from about 3.8–3.7 Gyr to ～2 Gyr. A third crater population(Population S) consisted of secondary impact craters that can dominate the cratering record at small diameters.  相似文献   

Machine Learning-based Weather Support for the 2022 Winter Olympics     

Jiangjiang XIA  Haochen LI  Yanyan KANG  Chen YU  Lei JI  Lve WU  Xiao LOU  Guangxiang ZHU  Zaiwen Wang  Zhongwei YAN  Lizhi WANG  Jiang ZHU  Pingwen ZHANG  Min CHEN  Yingxin ZHANG  Lihao GAO  Jiarui HAN 《大气科学进展》2020,37(9):927-932

正1.A key support for the 2022 Winter Olympics The XXIV Olympic Winter Games are scheduled to take place from 4 to 22 February 2022, followed by the Paralympic Games from 4 to 13 March, in Beijing and towns in the neighboring Hebei Province, China. Weather plays an extremely important role in the outcome of the games (Chen et al., 2018). It can not only cause a difference between a medal or not, but affect the safety of athletes. Success of the Winter Olympics will greatly depend on weather conditions at the outdoor competition venues, dealing with many weather elements including the snow surface temperature, apparent tem-  相似文献   

Specific Relationship between the Surface Air Temperature and the Area of the Terra Nova Bay Polynya,Antarctica   总被引：1，自引：0，他引：1  

Yifan DING  Xiao CHENG  Xichen LI  Mohammed SHOKR  Jiawei YUAN  Qinghua YANG  Fengming HUI 《大气科学进展》2020,37(5):532-544

Antarctic polynyas play an important role in regional atmosphere?ice?ocean interactions and are considered to help generate the global deep ocean conveyer belt.Polynyas therefore have a potential impact on the Earth’s climate in terms of the production of sea ice and high-salinity shelf water.In this study,we investigated the relationship between the area of the Terra Nova Bay polynya and the air temperature as well as the eastward and northward wind based on the ERA5 and ERAInterim reanalysis datasets and observations from automatic weather stations during the polar night.We examined the correlation between each factor and the polynya area under different temperature conditions.Previous studies have focused more on the effect of winds on the polynya,but the relationship between air temperature and the polynya area has not been fully investigated.Our study shows,eliminating the influence of winds,lower air temperature has a stronger positive correlation with the polynya area.The results show that the relationship between the polynya area and air temperature is more likely to be interactively influenced.As temperature drops,the relationship of the polynya area with air temperature becomes closer with increasing correlation coefficients.In the low temperature conditions,the correlation coefficients of the polynya area with air temperature are above 0.5,larger than that with the wind speed.  相似文献   

Seasonal and Sub-Seasonal Circulation Anomalies Associated with Persistent Rainy Days in 2018/2019 Winter in Shanghai,China     

Wei Wang  Fei Xin  Xiao Pan  Ying Zhang  Tim Li 《Acta Meteorologica Sinica》2020,34(2):304-314

Shanghai experienced the longest rainy days in 2018/2019 winter since 1988. The physical cause of such an unusual climate condition was investigated through the diagnosis of observational data. From a seasonal perspective, a long persistent rainy winter was often associated with an El Niño condition in the equatorial Pacific. This abnormal oceanic condition induces a remote teleconnection pattern with pronounced low-level southerly anomalies over East China. The wind anomalies transported moisture from tropical oceans and caused persistent rainfall in East Asia. Meanwhile, the local rainfall time series exhibited a strong quasi-biweekly oscillation (QBWO). Three persistent rainy events were identified in the 2018/2019 winter and they all occurred during the active phase of the QBWO. The first two events were associated with a low pressure anomaly west of Shanghai. Southerly anomalies associated with the low pressure system advected high mean moisture into central eastern China, leading to the persistent rainfall there. The third event was associated with a high pressure anomaly in lower troposphere to the east of Shanghai, which induced anomalous southerlies to its west, favoring the occurrence of rainfall in Shanghai. The result suggests the importance of high-frequency variability in affecting seasonal rainfall anomalies.  相似文献