内蒙古得尔布干成矿带铅锌银矿两期叠加成矿的矿物学证据--以乌尔根矿为例     

魏灿坤  温守钦  杨天瑶  杨红章  张光亮  李建源  谢伟  闫莹灿  张帅 《矿物学报》2020,(2):201-212

内蒙古额尔古纳市乌尔根铅锌银矿是得尔布干成矿带上具有代表性的浅成中低温热液型铅锌银矿之一。显微镜下观察、电子探针分析结果等矿物学证据证明,该矿床存在2期成矿作用。其中早期火山热液形成的金属硫化物普遍受应力作用的改造,并广泛被晚期形成的矿物交代,典型矿物是不含乳滴状黄铜矿的闪锌矿,具有高含量Fe、Mn和低含量Cu的特征;晚期次火山(隐爆角砾岩)热液形成的金属硫化物占大多数,常交代早期形成的矿物并与其交生在一起,典型矿物是含固溶体乳滴黄铜矿的闪锌矿,并且具有中等含量Fe、Mn和高含量Cu的特征。在次火山热液期的晚阶段残余热液还形成了较为纯净的呈棕黄色-无色透明的纯净闪锌矿,具有高含量Zn,低含量Fe、Mn、Cu的特征。结合前人测定的研究区火山岩和矿石矿物定年结果以及火山岩主量元素组成数据,推测早期火山热液成矿与中基性塔木兰沟组火山岩关系密切,而晚期次火山(隐爆角砾岩)热液属于满克头鄂博组的(中)酸性岩浆热液的产物。隐爆角砾岩热液富含Cu元素且为成矿提供了主要物质来源,是研究区寻找除铅锌之外其他矿种的重要线索。  相似文献   

自然重砂成因矿物学特征及找矿指示作用     

董国臣  李胜荣  申俊峰  董朋生  李华伟  殷国栋  汤家辉 《地学前缘》2020,27(5):171-178

自然重砂是地质体经自然风化、剥蚀、搬运、沉积等地质作用而分离出的单矿物(或矿物组合)。自然重砂矿物晶体由于仍然保留有许多矿物成因信息,包括颜色、形态、化学成分、物理性质和矿物组合等特征,因此常用于追溯源区地质体或者找矿勘查。这种方法被认为是一种经济实用的找矿方法——自然重砂测量。本文基于全国自然重砂找矿的数据资料,系统梳理了自然重砂的矿物类型、出现频率及其分布等特点,分析了自然重砂的矿物组合和成因矿物学特征,研究了自然重砂矿物的源区烙印、搬运距离及标型指示矿物组合特征,探讨了自然重砂成因矿物学研究意义及其找矿应用前景。自然重砂矿物的颜色、形态及内部结构依然保留着明确的成因矿物学信息:其颜色和晶体形态具有继承性而与其源区母体联系起来,体现源区母体的特性;其矿物组成可分出残余原生重矿物(包括造岩矿物、副矿物、矿石矿物等)和新生重砂矿物两个部分,如赤铜矿、孔雀石等反映着源区岩性体的成分或者赋存状态特征,其矿物组合也在很大程度上继承原生共生矿物而体现诸如有无矿化等意义;重砂颗粒的磨圆度、边界光滑性等表面特征反映搬运距离,有利于明确响应源区母体或者物源,而具有良好的找矿指示意义。  相似文献   

西昆仑普鲁新生代火山岩的矿物化学特征及其对岩浆演化过程的约束   总被引：2，自引：0，他引：2  

张招崇  肖序常  王军  王永  LUO Zhao-hua 《矿物学报》2005,25(3):237-248

对西昆仑普鲁新生代火山岩的矿物学进行了系统的研究。结果表明：该地区火山岩主要由橄榄石、单斜辉石和斜长石组成,并有少量的斜方辉石、黑云母、角闪石、碱性长石和铁钛氧化物。其矿物学特征指示了岩浆的性质有点类似于碱性岩浆,但与典型的碱性玄武岩又有明显的区别,属于橄榄安粗岩系列。利用橄榄石-熔体平衡原理估算了进入高位岩浆房中的熔体的MgO含量约为6．2％,Mg^#为0．57,说明其不是地幔熔融形成的原始岩浆,而是经历了深部岩浆房的分离结晶过程。由单斜辉石估算的高位岩浆房的深度约7～9km。岩浆在高位岩浆房中发生了较长时间的强烈分离结晶作用,分离结晶相主要为橄榄石、单斜辉石和斜长石以及少量的斜方辉石、黑云母、角闪石、碱性长石和铁钛氧化物。不同时期形成的铁钛氧化物指示了分离结晶过程由相对高温高氧逸度向相对低温低氧逸度演化。与此相对照的是岩浆在深部岩浆房中可能只发生了橄榄石和辉石等铁镁矿物的分离结晶作用,且分异作用时间较短。深部岩浆房可能存在于岩石圈地幔或壳幔过渡带中,岩浆由深部岩浆房上升到高位岩浆房中的过程是近绝热的,从浅部岩浆房到地表是快速上升的过程。  相似文献   

Characteristics of magnetic and non-magnetic lag in the Cobar area, NSW     

S. Alipour  D.R. Cohen  A.C. Dunlop 《Journal of Geochemical Exploration》1997,58(1):15-28

Geochemical patterns from two lag anomalies in the Cobar region of central New South Wales are described. The region is semi-arid, deeply weathered and some areas are covered by variable thicknesses of aeolian and alluvial transported overburden.Lag morphology and mineralogy are related to landform. In erosional landforms the surface is covered by lag, which is composed of coarse fragments derived locally from bedrock and displays varying degrees of ferruginization, together with a range of secondary pisoids. In depositional landforms the lag is less abundant and contains more pisoids. Deflation by sheetwash may lead to lag being partially buried by alluvium. In a large proportion of pisoid lag, hematite and goethite have been converted to maghemite, allowing ready separation into magnetic and non-magnetic fractions. The non-magnetic fraction is dominated by the lithic lag whereas the magnetic fraction is dominated by pisoid lag.The magnetic and non-magnetic components of the 2–11 mm lag fraction, milled to < 75 μm and subjected to HF-HNO₃-HClO₄ attack, give rise to distinct geochemical patterns at targets related to a variant of the Cobar style of Pb-Zn mineralization with variable silicification and to Zn mineralization in a swarm of quartz and carbonate veinlets. The patterns are influenced by metal source, lag type, surface chemical conditions and landtbrm. Differences in the correlation between metal contents in the magnetic and non-magnetic lag components, and between trace elements and Fe. indicate variable loss of Cu and Zn from the magnetic lag at some targets but retention of Pb. The presence of a readily cxtractable base metal component in the lag has implications for detecting anomalies in transported cover in the region.  相似文献   

黑龙江省三矿沟夕卡岩型铁铜矿床矿物学特征及成矿物理化学条件   总被引：1，自引：0，他引：1  

邓轲  陈衍景  张成  许强伟  朱雪峰 《地学前缘》2018,25(5):167-182

黑龙江三矿沟铁铜矿床位于大兴安岭北段多宝山矿集区,矿体产于燕山期侵入岩与奥陶系多宝山组大理岩接触带的夕卡岩内。根据矿物共生组合及交代关系,确定热液成矿过程包括夕卡岩阶段、退夕卡岩阶段和石英硫化物阶段。铁矿化主要发生在退夕卡岩阶段,形成磁铁矿、镜铁矿等铁氧化物,呈浸染状、条带状、块状产于钙铁榴石夕卡岩中。铜矿化主要发生在石英硫化物阶段,形成黄铜矿、斑铜矿等硫化物,交代早期矿物。电子探针分析等研究表明,三矿沟铁铜矿床发育钙质夕卡岩矿物组合,其石榴子石主要为钙铝榴石和钙铁榴石,辉石为透辉石钙铁辉石系列,角闪石属于钙角闪石系列,绿泥石属于I型三八面体富铁绿泥石。石榴子石有3种类型：早期自形粗粒的钙铝榴石(Grt-Ia)和钙铁榴石(Grt-Ib),以及晚期呈脉状产出的钙铁榴石(Grt-Ⅱ)。夕卡岩阶段成矿流体具有高温、弱酸性、高氧逸度的特征;退夕卡岩阶段流体温度降低,pH升高,形成大量铁氧化物;石英硫化物阶段流体温度和氧逸度降低,金属硫化物沉淀。  相似文献   

A new locality of palygorskite-rich clay from the southeastern Yucatán: a potential material source for environmental applications     

Mark P. S. Krekeler  Lance E. Kearns 《Environmental Geology》2009,58(4):715-726

A palygorskite unit was discovered in a road cut of undifferentiated Tertiary limestone between the villages of El Pariso and San Roman (18°49.309N, 88°37.861W) in the southeastern Yucatán Peninsula, Mexico. This is the southern most locality of a clay-rich sedimentary unit reported in the literature for the Tertiary carbonates of the Yucatán Peninsula. This occurrence indicates a much wider range of palygorskite-rich clay deposition than previously recognized. The lithology is 99% clay and 1% sand to silt size diagenetic quartz grains. The clay consists of approximately 85% palygorskite, 15% montmorillonite and trace amounts of titanium oxides. EDS analyses on palygorskite are largely consistent with sedimentary palygorskites from other coastal marine settings, however palygorskite has a low total Fe content (average = 0.40 wt% expressed as Fe₂O₃) compared to many other sedimentary palygorskites. Montmorillonite chemical compositions are typical and compared to the palygorskite have substantially higher Fe₂O₃ concentrations (average = 3.90 wt%). The low percentage of coarse grains in the lithology combined with a high proportion of palygorskite and lack of detrimental trace minerals suggest the deposit is of industrial grade; however, it has limited reserves (6,000 m³). The unit could be potentially used in a wide array of environmental applications which are needed in the region including liners for landfills and constructed wetlands. The unit is in a geographic location which would serve the expanding economy of the region. This resource has the potential to have great impact on the quality of the local environment and the economy of a region under great environmental threat.  相似文献   

A reanalysis of the Apollo light scattering observations, and implications for lunar exospheric dust     

David A. Glenar  Timothy J. Stubbs  James E. McCoy  Richard R. Vondrak 《Planetary and Space Science》2011,59(14):1695-1707

Conspicuous excess brightness, exceeding that expected from coronal and zodiacal light (CZL), was observed above the lunar horizon in the Apollo 15 coronal photographic sequence acquired immediately after orbital sunset (surface sunrise). This excess brightness systematically faded as the Command Module moved farther into shadow, eventually becoming indistinguishable from the CZL background. These observations have previously been attributed to scattering by ultrafine dust grains (radius ∼0.1 microns) in the lunar exosphere, and used to obtain coarse estimates of dust concentration at several altitudes and an order-of-magnitude estimate of ∼10⁻⁹ g cm⁻² for the column mass of dust near the terminator, collectively referred to as model “0”.We have reanalyzed the Apollo 15 orbital sunset sequence by incorporating the known sightline geometries in a Mie-scattering simulation code, and then inverting the measured intensities to retrieve exospheric dust concentration as a function of altitude and distance from the terminator. Results are presented in terms of monodisperse (single grain size) dust distributions. For a grain radius of 0.10 microns, our retrieved dust concentration near the terminator (∼0.010 cm⁻³) is in agreement with model “0” at z=10 km, as is the dust column mass (∼3–6×10⁻¹⁰ g cm⁻²), but the present results indicate generally larger dust scale heights, and much lower concentrations near 1 km (<0.08 cm⁻³ vs. a few times 0.1 cm⁻³ for model “0"). The concentration of dust at high altitudes (z>50 km) is virtually unconstrained by the measurements. The dust exosphere extends into shadow a distance somewhere between 100 and 200 km from the terminator, depending on the uncertain contribution of CZL to the total brightness. These refined estimates of the distribution and concentration of exospheric dust above the lunar sunrise terminator should place new and more rigorous constraints on exospheric dust transport models, as well as provide valuable support for upcoming missions such as the Lunar Atmosphere and Dust Environment Explorer (LADEE).  相似文献   

Mitigation of lunar dust adhesion by surface modification   总被引：2，自引：0，他引：2  

Adrienne Dove  Genevieve Devaud  Xu Wang  Mark Crowder  Anna Lawitzke  Christina Haley 《Planetary and Space Science》2011,59(14):1784-1790

Dust has been recognized as one of the greatest hazards in continued lunar exploration due to its tenacious adhesion to everything with which it comes into contact. Unfortunately, there is little known about the mechanisms of adhesion on widely varying surface types: van der Waals and electrostatic forces are the dominant forces under consideration here. Surface energy, roughness, mechanical properties and electronic properties are all known to contribute to the adhesion characteristics. An optimal solution to mitigate dust adhesion would be to identify the dominant components of the adhesive force and to reduce that force by surface modification. In this study, an ion beam process was used to modify (treat) the surfaces of three dramatically different materials spanning the range of conductor (black Kapton), semiconductor (silicon), and insulator (quartz). Adhesive forces between less than JSC-1 lunar simulants and these virgin/treated surfaces were measured in vacuum using a centrifugal force detachment method. We found that JSC-1 particles adhered less to treated silicon and quartz surfaces, correlated with a reduction in van der Waals force due to a reduced surface energy. The large reduction in adhesion for treated black Kapton is mainly due to the large decrease in the electrostatic (image) force that results from reduced contact charging. Materials in space and on the lunar surface will be directly exposed to high-energy ultraviolet radiation prior to being covered by dust, so the UV irradiation effects on surface adhesion were also examined. Both virgin and treated quartz surfaces are most affected by the UV-irradiation, showing dramatically increased adhesion.  相似文献   

Within‐colony variation in skeletal mineralogy of Adeonellopsis sp. (Cheilostomata: Bryozoa) from New Zealand     

Katherine E. Wejnert  Abigail M. Smith 《新西兰海洋与淡水研究杂志》2013,47(4):389-395

Three colonies of the erect, robust branching, cheilostome bryozoan Adeonellopsis sp. were collected from Doubtful Sound, New Zealand, to investigate within‐colony variation in carbonate mineralogy. One‐hundred‐and‐twenty‐one sections from 9 branches were found to contain mostly aragonite, with calcite ranging from 1.1 to 7.3 wt% (mean ± SD = 2.4 ± 1.2 wt%, n = 120). The magnesium (Mg) content in calcite ranged from 5.3 to 13.1 wt% magnesium carbonate (8.8 ± 1.0 wt% MgCO₃; n = 120). Calcite content decreased with increasing age proximally along the branch, indicating that secondary thickening is achieved with aragonite. In contrast, an oscillating trend in Mg content along branches suggests that seasonal or interannual environmental parameters may influence this geochemical parameter. Mineralogical variability highlights the need for multiple samples from the same colony to be measured when determining quantitative carbonate mineralogy in bryozoans. Bimineralic bryozoans such as Adeonellopsis sp. may have lower preservation potential than monomineralic bryozoans, and consequently may not survive diagenesis to become fossils. Bimineralic species may also be more vulnerable to dissolution pressure and possible ocean acidification than monomineralic calcitic taxa.  相似文献   

云南兰坪盆地北部东缘铅锌矿床喷流沉积成因的厘定———来自矿物学和硫同位素证据   总被引：1，自引：0，他引：1  

黄玉凤  曹殿华  王志军  李以科  王安建 《地质力学学报》2011,17(1):91-102

通过详细的野外地质工作和显微镜下观察,对云南兰坪盆地东北部维西—乔后断裂带上三叠统石钟山组(T₃s)中产出的铅锌矿床成因进行厘定。研究结果表明,测区内存在大量典型的同生沉积矿床标志,如:纹层构造、条纹条带构造、网脉构造、黄铁矿条带软沉积构造、黄铁矿草莓状结构、黄铁矿胶状构造、闪锌矿同心环状构造等。青甸湾矿床金属硫化物硫同位素测试结果显示,黄铁矿的δ34 S介于3.7‰ ~ 8.1‰,均值5.34‰; 闪锌矿的δ34 S介于5.2‰ ~ 10.0‰之间,均值为7.18‰; 方铅矿的δ34 S介于5.2‰ ~ 9.9‰之间,均值为7.275‰,铅锌矿床硫来源于海水硫酸根无机还原。结合矿床形成时代及大地构造背景,认为该区铅锌矿为喷流沉积作用形成。   相似文献