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1.
Chengbiao Leng Yuhui Wang Xingchun Zhang Jianfeng Gao Wei Zhang Xinying Xu 《中国地球化学学报》2018,37(1):47-59
The Kukaazi Pb–Zn–Cu–W polymetallic deposit, located in the Western Kunlun orogenic belt, is a newly discovered skarn-type deposit. Ore bodies mainly occur in the forms of lenses and veins along beddings of the Mesoproterozoic metamorphic rocks. Three ore blocks, KI, KII, and KIII, have been outlined in different parts of the Kukaazi deposit in terms of mineral assemblages. The KI ore block is mainly composed of chalcopyrite, scheelite, pyrrhotite, sphalerite, galena and minor pyrite, arsenopyrite, and molybdenite, whereas the other two ore blocks are made up of galena, sphalerite, magnetite and minor arsenopyrite and pyrite. In this study, we obtained a molybdenite isochron Re–Os age of 450.5 ± 6.4 Ma (2σ, MSWD = 0.057) and a scheelite Sm–Nd isochron age of 426 ± 59 Ma (2σ, MSWD = 0.49) for the KI ore block. They are broadly comparable to the ages of granitoid in the region. Scheelite grains from the KI ore block contain high abundances of rare earth elements (REE, 42.0–95.7 ppm) and are enriched in light REE compared to heavy REE, with negative Eu anomalies (δEu = 0.13–0.55). They display similar REE patterns and Sm/Nd ratios to those of the coeval granitoids in the region. Moreover, they also have similar Sr and Nd isotopes [87Sr/86Sr = 0.7107–0.7118; εNd(t) = ?4.1 to ?4.0] to those of such granitoids, implying that the tungsten-bearing fluids in the Kukaazi deposit probably originate from the granitic magmas. Our results first defined that the Early Paleozoic granitoids could lead to economic Mo–W–(Cu) mineralization at some favorable districts in the Western Kunlun orogenic belt and could be prospecting exploration targets. 相似文献
2.
拉尔玛金矿的生物成矿作用 总被引：1，自引：0，他引：1
位于甘、川两省交界处的拉尔玛金矿床,赋存于下寒武统太阳顶群,矿区内岩浆活动不强烈,矿床中断裂构造较发育,矿石矿物种类较齐全。矿石中的生物有机地球化学特征表明其为细菌和低等藻类生物体衍生的生物标志物和遗传特征,证明了太阳顶群中的有机质起源于菌藻类生物。矿石中的金属矿物生物组构有生物有机胶体组构和矿交代生物组构,说明生物成矿作用经历了直接成矿和间接成矿,即两轮聚矿作用,菌藻生物的第一轮聚金主要形成矿源层,生物的两轮聚金结果,形成此矿床。 相似文献
3.
从1981年开始,北京天文台开展了发射线星系的物端稜镜巡天。用60/90cm Schmidt望远镜加5.°3的物端稜镜在敏化的ⅢaJ底片上可以得到亮于16~m的星系光谱像。本文公布了第一批巡天结果:在覆盖天区约220平方度的12张底片上证认出50个发射线天体,47个河外星系(其中3个可能是新的Seyfert星系),3个行星状星云(其中一个N2242以前被当作河外星系)。文中给出了这些天体的名称、坐标、星等及光谱结构分类等资料,并比较系统地讨论了发射线星系的证认及光谱结构分类。我们还将本巡天的结果与其他天文台的结果作了比较。这些天体的证认图见图版Ⅰ—Ⅱ。 相似文献
4.
大洋钻探与西太平洋构造 总被引：3，自引：0，他引：3
菲律宾海的深海钻探证了弧间扩张和残留弧形模式。小笠原－马里亚纳弧前区的钻探表明，俯冲带初生时伴着海底扩张，形成了异常宽阔的火山活动带。有许多出上蛇绿岩形成于俯冲带初生时的海底扩张环境。日本海的钻探揭示了日本边缘盆地的打开和关闭，新近形成的日本海东缘板边界对华北地区的构造有重要制约作用，中国东海和南海占有独特的构造位置，布置大洋钻探意义重大。文章还强调了中国地质学家从全球地质学的观点研究问题（而不仅 相似文献
5.
论文根据磁浮交通道岔梁的结构及受力特点,通过建立合理的瞬态动力学数值模型,把列车作为高速运行的荷载动态作用于道岔梁上。采用瞬态拟动力学方法模拟钢结构梁动力响应特性。研究了道岔梁上关键点位置相应的振幅、反应加速度及其时效特性。通过计算比较精确地获得工程实际中最为关注的梁的最大振动位移和加速度。研究成果可为高速磁浮实际工程设计提供借鉴。 相似文献
6.
GNSS系统的定位精度和可靠性在很大程度上依赖于观测到的卫星数量和几何图形分布.在城市、露天矿区和峡谷等地区,由于可观测卫星数少,单一系统的定位精度往往难以满足要求,GNSS多星座组合是解决问题的一个有效措施.选取雅砻江卡拉电站滑坡监测网中的一个监测点,利用实测的COMPASS星历和GPS卫星星历,从可见卫星数目及GDOP值两个角度,对GPS、COMPASS单星座系统以及其组合系统变形测量性能进行了对比分析.实验表明GPS和COMPASS组合系统能够有效改善变形监测精度. 相似文献
7.
中国斑岩铜矿与埃达克(质)岩关系探讨 总被引：16，自引：2，他引：14
对比研究了中国26个主要斑岩铜矿的地球化学特征和年代学,结果表明其中25个矿床与埃达克(质)岩有成因联系,且多数与玄武质下地壳熔融形成的埃达克岩(C型)有关,现有数据表明土屋-延东和普朗斑岩铜矿可能与俯冲板片熔融形成的埃达克岩(O型)有关。容矿斑岩的初始锶值为0.7034～0.7090,均大于洋中脊玄武岩和亏损地幔的初始锶值,多数与EMI的初始锶值接近,推测其源区或源岩主要为玄武质下地壳,少数为洋中脊玄武岩,并受到中、上地壳不同程度的混染,这与两类埃达克岩的源区基本一致。虽然埃达克质岩浆具有形成斑岩铜矿的巨大潜力,但并非所有埃达克岩都能成矿,不同岩体需具体分析。 相似文献
8.
Visible gold in arsenian pyrite at the Shuiyindong Carlin-type gold deposit, Guizhou, China: Implications for the environment and processes of ore formation 总被引：13，自引：0，他引：13
Wenchao Su Bin Xia Hongtao Zhang Xingchun Zhang Ruizhong Hu 《Ore Geology Reviews》2008,33(3-4):667-679
Carlin-type gold deposits are best known for the scarcity of visible gold in their ores. It has long been recognized that the majority of gold is “invisible”, such that it cannot be resolved by conventional microscopy, and resides in arsenian pyrite. Shuiyindong differs in that sub-μm to μm-sized native gold is present in arsenian pyrite veinlets and disseminations. It is also the largest (55 tonnes) and highest grade (7 to 18 ppm), stratabound, Carlin-type gold deposit in Guizhou, China and has produced 5 tonnes of gold from sulfide refractory ores extracted by underground mining methods. In this study, an electron microprobe analyzer (EMPA) was used to map the spatial distribution of “invisible” gold and sub-μm to μm-size visible gold particles in arsenian pyrite in high-grade ore samples from the Shuiyindong. The samples studied are hosted in Permian bioclastic ferroan limestone of the Longtan Formation and exhibit evidence of decarbonation, silicification and sulfidation. Arsenian pyrite with detectable Au (> 400 to 3800 ppm) is disseminated in altered limestone and was deposited in two stages separated by an episode of corrosion in a veinlet.The results show that there are two populations of native gold in arsenian pyrite. One is comprised of sub-μm size gold particles (0.1 to 0.2 μm) that are occasionally present in the gold-bearing arsenian pyrite disseminated in the host rocks. This arsenian pyrite is interpreted to have been formed by sulfidation of ferroan calcite and dolomite. Another is comprised of coarser (1 to 6 μm) native gold grains present in the arsenian pyrite veinlet, either on the first stage where it has been corroded or on the second stage. The lack of fluid inclusion or other evidence of boiling and the low iron content of fluid inclusions in quartz, suggest the veinlet formed by sulfidation of another fluid containing Fe. The Fe-bearing fluid may be a depleted ore fluid that gained Fe by dissolution of ferroan limestone after H2S had been consumed. The association of the largest visible gold grains with an episode of corrosion suggests that fluids episodically became undersaturated with arsenian pyrite while remaining saturated with gold (e.g., pH decrease or an increase in the oxidation state). This may have resulted from incursion of relatively acidic or oxidized fluids that were able to dissolve arsenian pyrite and remain saturated with gold. In this case, sulfidation of iron from the host rock, was the most important depositional mechanism for Au-bearing arsenian pyrite with, or without, grains of native gold. 相似文献
9.
滇西北中甸松诺含旷斑岩的锆石SHRIMP U-Pb年龄及地质意义 总被引：8，自引：1，他引：7
位于义敦岛弧南端的中甸岛弧中广泛发育印支期斑岩及斑岩型和矽卡岩型铜矿床.松诺(或称松诺力赞)复式岩体位于东斑岩带中部,由石英闪长玢岩、黑云石英二长斑岩、闪长玢岩和含矿石英二长斑岩组成,其南部为普朗超大型斑岩铜矿床,北部为地苏嘎铜矿点.本文对含矿石英二长斑岩进行了岩相学和锆石SHRIMP U-Pb 定年研究,结果表明所有锆石颗粒自形较好且均发育规则的韵律环带,Th 含量为 180～854 μg/g,U 含量为270～709μg/g,Th/U 比值为 0.77～1.24,为典型岩浆成因锆石.获得了含矿石英二长斑岩的侵位年龄为220.9±3.5Ma(n=9,MSWD= 1.6),这与中甸岛弧洋壳俯冲造山作用的时限(210～235 Ma)相吻合. 相似文献
10.
荔枝越冬期间冠层气温与大气温度关系的初步分析 总被引：2，自引：0，他引：2
基于野外实测数据,按晴天、阴天、雨天、多云到晴等天气类型,分析2007/2008年、2008/2009年冬季荔枝果园大气温度、冠层气温与观测站大气温度的变化关系,结果表明:晴天荔枝冠层温度昼夜变化最为剧烈,多云到晴天气次之,阴天和雨天冠层大气温度变化相对平缓;果园和观测站大气温度昼夜变化同样与天气类型有关.按天气类型分别建立的观测站与荔枝冠层之间的夜间、白天和全天大气温度线性、曲线回归关系模型表明:阴天和雨天模型效果好于多云到晴、晴天天气,夜间模型好于全天和白天.这一结果对应用观测站大气温度开展荔枝寒害冻害监测有参考作用. 相似文献