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101.
Lunar geochemistry as told by lunar meteorites 总被引:7,自引:0,他引:7
About 36 lunar meteorites have been found in cold and hot deserts since the first one was found in 1979 in Antarctica. All are random samples ejected from unknown locations on the Moon by meteoroid impacts. Lithologically and compositionally there are three extreme types: (1) brecciated anorthosites with high Al2O3 (26–31%), low FeO (3–6%), and low incompatible elements (e.g., <1 μg/g Th), (2) basalts and brecciated basalts with high FeO (18–22%), moderately low Al2O3 (8–10%) and incompatible elements (0.4–2.1 μg/g Th), and (3) an impact-melt breccia of noritic composition (16% Al2O3, 11% FeO) with very high concentrations of incompatible elements (33 μg/g Th), a lithology that is identified as KREEP on the basis of its similarity to Apollo samples of that designation. Several meteorites are polymict breccias of intermediate composition because they contain both anorthosite and basalt. Despite the large range in compositions, a variety of compositional parameters together distinguish lunar meteorites from terrestrial materials. Compositional and petrographic data for lunar meteorites, when combined with mineralogical and compositional data obtained from orbiting spacecraft in the 1990s, suggest that Apollo samples identified with the magnesian (Mg-rich) suite of nonmare rocks (norite, troctolite, dunite, alkali anorthosite, and KREEP) are all products of a small, geochemically anomalous (noritic, high Th) region of crust known as the Procellarum KREEP Terrane and are not, as generally assumed, indigenous to the vast expanse of typical feldspathic crust known as the Feldspathic Highlands Terrane. Magnesian-suite rocks such as those of the Apollo collection do not occur as clasts in the feldspathic lunar meteorites. The misconception is a consequence of four historical factors: (1) the Moon has long been viewed as simply bimodal in geology, mare or highlands, (2) one of the last, large basin-forming bolides impacted in the Procellarum KREEP Terrane, dispersing Th-rich material, (3) although it was not known at the time, the Apollo missions all landed in or near the anomalous Procellarum KREEP Terrane and collected many Th-rich samples formed therein, and (4) the Apollo samples were interpreted and models for lunar crust formation developed without recognition of the anomaly because global data provided by orbiting missions and lunar meteorites were obtained only years later. 相似文献
102.
ZENG Qiaosong WANG Jincao CHEN Guanghao 《大地构造与成矿学(英文版)》2005,29(2):93-106
1 Introduction Hydrofracturing is possibly an important fracture behavior within the whole lithospheric crust, many geologists have noticed and carried out study on hydrofracturing in the fluid-rock systems (e.g., Phillips, 1972; Sibson, 1986; Fyfe, 1987; Svyatoslav and Kirill, 1993; Cox, 1995; Nakashima and Toriumi, 1996; James et al., 2000; Agust et al., 2002). Hydrofracturing phenomena are universally existent in the active structural belts, nonlinear tension vein systems in metamorphi… 相似文献
103.
广东湛江陨击混杂堆积层的发现及其意义 总被引:1,自引:0,他引:1
通过野外地质调查和取样分析,首次在广东湛江地区中更新统早期的北海组地层中发现了一层罕见的陨击混杂堆积层,它是陨击作用下的特殊产物,是北海组含砾砂、粘土质砂在陨击高温作用下烧结、抛射堆积而形成的。陨击混杂堆积层主要分布在湛江坡头的部分地区,有的出露地表,有的为第四系所覆盖,厚度大约为0·1~4m。陨击混杂堆积层中共生玻璃陨石(雷公墨)。陨击混杂堆积层中的击变岩砾石与原岩相比较,Si O2的含量明显减少,Fe2O3的含量明显增加,其他化学成分及含量与原岩近于一致。陨击混杂堆积层的发现可能对澳大利亚—东南亚微玻璃陨石场陨击源坑的寻找和探讨该期玻璃陨石和微玻璃陨石与靶岩之间的关系有重要意义。 相似文献
104.
祁雨沟含金角砾岩筒中的冰长石-方解石组合及其矿床地质意义 总被引:6,自引:0,他引:6
通过野外地质、岩相学、拉曼光谱和电子探针分析,对祁雨沟2号和4号含金角砾岩筒中冰长石-方解石蚀变矿物组合特征进行了描述。含金角砾岩筒成矿作用分为两期:面状矿化和脉状矿化。面状矿化的蚀变主要有阳起石化、绿色黑云母化、绿泥石化、冰长石化、硅化、绿帘石化、黄铁矿化、碳酸盐化和少量的绢云母化。脉状矿化蚀变为硅化、绢云母化和少量的碳酸盐化。通过对角砾岩筒的蚀变与成矿作用关系研究,认为冰长石-方解石蚀变与含金角砾岩金成矿作用是同期,从而确定祁雨沟含金角砾岩筒是一个典型的低硫型浅成低温热液型金矿床。 相似文献
105.
鲜思远 《沉积与特提斯地质》1998,18(5):28-56
笔者系统研究了广西六景中泥盆统民塘组底部的硅化腕足化石,描述了31个属种,其中新属、新亚属各1个,新种20个,划分出Geranocephalus-Pentamerela(下部)动物群和Stringocephalus-Changtanela(上部)两个动物群。着重对Geranocephalus-Pentamerela动物群的特征与时代进行了讨论,其时代具浓厚的艾菲尔晚期的色彩。该动物群属老世界区的一部分,与美国内华达同期动物群有密切的亲缘关系,同时与欧洲(如德国、捷克以及乌拉尔地区)也有一定相似性,然而从种群而言,它是一个斩新的动物群。提出Geranocephalus不是Subrensel-landia与Stingocephalus之间的中间形态,而是Renselandia与Stingocephalus之间的中间形态,很可能Geranocephalus就是Stingocephalus的先躯,它代表Rensselandia向Stingocephalus演化过程中的一个重要阶段。 相似文献
106.
康家湾硅化角砾岩天然热释光特征及对找矿的指导意义 总被引:1,自引:0,他引:1
通过对康家湾Pb、Zn、Ag矿床的含矿带硅化角砾岩带进行天然热释光分析。发现其热释光特征与成矿有密切的关系,从而划分出了成矿的远景区。 相似文献
107.
新疆乌伦布拉克隐爆角烁岩筒型斑岩铜矿成矿地质特征 总被引:7,自引:0,他引:7
矿床直接产于一套浅成—超浅成或次火山侵入的花岗质潜火山杂岩中。赋矿岩石为斜长花岗岩、石英闪长岩、闪长岩及英安玢岩质隐爆角砾岩。矿石矿物有孔雀石、兰铜矿、兰辉铜矿、赤铜矿、黄铜矿、斑铜矿、黄铁矿等。矿石结构构造为交代残余结构、包含结构和星点状、细脉状、网脉状、团块状构造。围岩蚀变为硅化、赤铁矿化、碳酸盐化、绢云母化和绿泥石化。成矿温度为119℃~190℃。成矿时代为海西中晚期。隐爆角砾岩筒中石英—钾长石—黄铜矿脉的石英包裹体氢氧同位素δD为-101.7‰,δ18O为8.4‰,钾长石K—Ar法年龄为211±3Ma。 相似文献
108.
109.
德安县金家洞萤石矿床地质特征 总被引:1,自引:0,他引:1
金家洞萤石矿位于彭山背斜构造北西翼,萤石矿体赋存于中奥陶统汤山组的硅化破碎带内。受区域北东-南西向断裂构造控制,矿体具中等规模,埋藏浅、质量好。矿石类型以纯萤石型、石英-萤石型、硅化灰岩-萤石型为主,次为方解石-萤石型、方解石-石英-萤石型。矿床成因属岩浆期后低温热液充填交代型矿床,成矿作用与燕山期岩浆活动密切相关。 相似文献
110.
A. A. P. S. R. Acharyulu B. Sreenivasa Murty B. K. Bhaumik 《Journal of Earth System Science》2004,113(3):321-352
Over the years a large number of rock samples were collected by the explorationists of Atomic Minerals Directorate for Exploration
and Research (AMD), Department of Atomic Energy from Sambalpur district, Orissa, India. The variation of uranium enrichment
with various types of rock in these samples was studied with an aim to help quick reviewing of toposheets in case of newly
taken up areas, for uranium exploration. The radioelements U, Th and K determined for these samples are plotted in ternary
diagrams for classifying them as being uraniferous or thoriferous with respect to various type of rocks, keeping the total
natural content of radioelements (expressed by eUP3O8) as a parameter.
In this study it is seen that samples of quartzofeldspathic breccia type are enriched in uranium irrespective of their further
sub classification and eU3O8 content. Granites are enriched in thorium when eU3O8 < 100 ppm and are enriched in uranium when eU3O8 > 100 ppm.
A database prepared for this purpose may be useful for reviewing toposheets in future 相似文献