西藏谢通门县德新铅锌矿地质特征及找矿标志   总被引：1，自引：0，他引：1  

王育良  苏会平  张凯  李革委 《陕西地质》2010,28(2):40-46

德新铅锌矿位于西藏自治区谢通门县,地处西藏冈底斯Cu、Mo、Pb、Zn、Au、Fe成矿带中段。矿体主要赋存于岩浆岩与第三系火山岩的接触带,地层、岩浆岩控制了矿体的总体展布方向和空间位置。早期东西向构造对成矿起了导矿作用,晚期近南北向、北西、北东向构造是主要的容矿、储矿构造。属标准的地层、构造、岩浆岩＂三位一体＂的成矿模式。矿床成因可能属火山隐爆角砾岩型。本文提出了区内8条找矿标志。  相似文献   

月面环境与月壤特性研究的主要问题探讨   总被引：6，自引：0，他引：6  

王世杰  李雄耀  唐红  李阳 《地球化学》2010,39(1):73-81

月面环境与月壤特性是月球探测和月球科学研究的重要基础,对它们的研究一直在不断加深,本文对月球表面地形地貌、热环境以及月壤特性三个方面的研究现状进行了总结,初步分析了这三个方面研究目前存在的一些主要问题：（1）地形地貌对月球定量遥感的影响以及南极艾特肯（SPA）盆地等地貌单元的年代学划分和成因演化;（2）月面热辐射、月表物理温度和热流等月面热环境特征的进一步探测和全面分析,以及其对地球反照率变化的响应;（3）月壤形成演化过程及空间风化作用,月球极区氢富集机制和水冰探测,以及月球资源开发利用。  相似文献   

徽县银洞子金矿床地质特征与控矿因素分析          下载免费PDF全文

石素娟 《甘肃地质》2014,23(3):56-60

银洞子金矿床位于甘肃徽县东南部,属多因素沉积再造型矿床。矿床受EW向F1断裂及次级构造控制,金矿化与下石炭统下岩组凝灰岩、凝灰质灰岩、不纯的薄层灰岩及其构造角砾岩有关,在金矿化区常见中基性—中酸性小岩体（枝）分布。金矿化赋存在通过此岩组断裂中。与金矿化关系密切的围岩蚀变主要是硅化、黄铁矿化、褐铁矿化、碳酸盐化等。  相似文献   

黑龙江争光金矿床隐爆角砾岩特征及其地质意义   总被引：2，自引：0，他引：2  

高荣臻 《地质与勘探》2014,50(5):874-883

黑龙江争光金矿床位于大兴安岭东北缘的多宝山矿集区,矿体主要呈脉状产于燕山期闪长岩体与中奥陶统多宝山组的内外接触带上,受断裂构造控制明显。在野外地质调查过程中,发现了3个隐爆角砾岩体（J-1、J-2、J-3）,角砾岩体从中心向外侧有较显著的岩石类型分带,中心为热液隐爆角砾岩,向外角砾增大,逐渐过渡为震碎角砾岩。根据胶结物的不同和穿插关系可将其分为四期,最早期为硅质胶结,中期为绿泥石胶结,其次为矿质胶结,最后为灰黑色安山质胶结,其中第二期和第三期隐爆作用与矿化关系密切。通过对隐爆角砾岩地质特征的研究,结果表明在Ⅱ号矿带绿泥石胶结隐爆角砾岩体深部具有寻找与矿质胶结隐爆角砾岩有关金铜矿化体的潜力,这对争光金矿床深部及外围找矿具有一定的指导意义。  相似文献   

Morphological differentiation characteristics and classification criteria of lunar surface relief amplitude     

DENG Jiayin  CHENG Weiming  LIU Qiangyi  JIAO Yimeng  LIU Jianzhong 《地理学报(英文版)》2022,32(11):2365-2378

Lunar landforms are the results of geological and geomorphic processes on the lunar surface. It is very important to identify the types of lunar landforms. Geomorphology is the scientific study of the origin and evolution of morphological landforms on planetary surfaces. Elevation and relief amplitude are the most commonly used geomorphic indices in geomorphological classification studies. Previous studies have determined the elevation classification criteria of the lunar surface. In this paper, we focus on the classification criteria of the topographic relief amplitude of the lunar surface. To estimate the optimal window for calculating the relief amplitude of the lunar surface, we use the mean change-point method based on LOLA (Lunar Orbiter Laser Altimeter) Digital Elevation Model (DEM) data and SLDEM2015 DEM data combining observations from LOLA and SELenological and Engineering Explorer Terrain Camera (SELENE TC). The classification criterion of the lunar surface relief amplitude is then determined according to the statistical analysis of basic lunar landforms. Taking the topographic relief amplitudes of 100 m, 200 m, 300 m, 700 m, 1500 m and 2500 m as thresholds, the lunar surface is divided into seven geomorphic types, including minor microrelief plains (< 100 m), minor microrelief platforms [100 m, 200 m), microrelief landforms [200 m, 300 m), small relief landforms [300 m, 700 m), medium relief landforms [700 m, 1500 m), large relief landforms [1500 m, 2500 m) and extremely large relief landforms (≥ 2500 m). The minor microrelief plains are mainly distributed in the maria and the basalt filled floors of craters and basins, while the minor microrelief platforms are mainly in the transition regions between the maria and highlands. The microrelief landforms are mainly located in regions with relatively high topography, such as wrinkle ridges and sinuous rilles in the mare. The small relief landforms are mainly scattered in the central peak and floor fractures of craters. The medium relief landforms are mainly distributed in the transition regions between crater floors and crater walls, between crater walls and crater rims, between basin floors and basin walls, and between basin walls and basin rims. Large and extremely large relief landforms are mainly found along crater walls and basin walls. The classification criteria determination for assessing lunar surface relief amplitude described in this paper can provide important references for the construction of digital lunar surface geomorphology classification schemes.  相似文献   

嫦娥3号巡视探测器桅杆的转动角度误差检校     

张烁  徐亚明  刘少创  贾阳  薛博  马友青 《测绘科学》2014,39(9)

嫦娥3号巡视探测器桅杆的展开机构、偏航机构和俯仰机构在转动过程中存在系统性的偏差,这些误差影响了巡视探测器导航定位、地形恢复和路径规划的精度.针对这一问题,文章提出了一种间接平差模型,通过真实数据试验证明该方法能够用于对嫦娥3号巡视探测器桅杆的转动角度误差进行检校,并且具有很高的精度和稳定性.  相似文献   

Weak stability boundary trajectories for the deployment of lunar spacecraft constellations     

Christian Circi  Paolo Teofilatto 《Celestial Mechanics and Dynamical Astronomy》2006,95(1-4):371-390

Suitable lunar constellation coverage can be obtained by separating the satellites in inclinations and node angles. It is shown in the paper that a relevant saving of velocity variation ΔV can be achieved using weak stability boundary trajectories. The weakly stable dynamics of such transfers allows the separation of the satellites from the nominal orbit to the required orbit planes with a small amount of ΔV. This paper also shows that only one different set of orbital parameters at Moon can be reached with the same ΔV manoeuvre starting from a nominal trajectory and ending at a fixed periselenium altitude. In fact, such a feature is proved to be common to other simpler dynamical systems, such as the two- and three-body problems.  相似文献   

Thermal equilibration of the Earth following a giant impact     

Tilman Spohn  G. Schubert 《Geophysical Journal International》1991,107(1):163-170

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月球重力场对绕月低轨卫星的长期影响     

HUANG Yong HU Xiaogong HUANG Cheng 《中国科学院上海天文台年刊》2005,(1):14-21

从解析形式出发,利用月球重力场模型JGL165P1,分析了月球重力场(带谐项)对绕月低轨卫星的长期影响。为了减少计算误差,保证计算精度,在分析解中使用循环公式来计算倾角函数。结果指出对于一个高度为100km的极月轨道卫星,冻结轨道存在的可能性不大,但是当轨道倾角在i=90°附近或者高度再高一些,则有可能存在冻结轨道;对于100km高的初始圆轨道,卫星在无控的情况下半年内将会坠落到月球表面,如果高度增加到200km,则不进行轨道控制也不会坠落到月面上。利用仿真软件GEODYN解算出来的结果证实了上述结论。  相似文献   

用LLR资料解算日月轨道根数     

白金明  金文敬 《天文学报》1994,35(4):424-433

本文推导了激光测月资料归算中测距对地月系轨道根数的偏导数，并对所得偏导数进行了精度估计，利用这些偏导数和１９８８年至１９９２年全球激光测月资料解算了日月轨道根数，得到了比较理想的结果。  相似文献