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李春来 《矿物岩石地球化学通报》1997,(3)
玻璃陨石的成因争论及可能的彗星撞击模型李春来（中国科学院地球化学研究所，贵阳５５０００２）关键词玻璃陨石成因彗星撞击事件玻璃陨石是一种棕黑色或浅绿色的天然玻璃，一般为厘米级大小的块状，表面多具空气动力学熔蚀刻痕。长期的研究证明，玻璃陨石在化学和结构特... 相似文献
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岩浆Cu-Ni-PGE矿床研究现状及发展趋势 总被引：4，自引：0，他引：4
从全球视野分析研究了世界岩浆铜镍硫化物矿床的大地构造分布和成岩成矿类型,特别是通过上世纪末新发现的加拿大Voisey′s Bay矿床与俄罗斯Noril′sk等世界级矿床特征的对比研究,突出强调了大火成岩省(LIPs)对大规模岩浆硫化物矿床形成的意义,从更加宏观的角度审视了世界级岩浆硫化物矿床形成的地质背景和岩浆作用条件,为中国金川等岩浆Cu-Ni-PGE硫化物矿床的深入研究提供了参照背景。评述分析了当代岩浆硫化物矿床成矿研究中,幔源岩浆中硫化物液相不混溶(熔离)的演化轨迹,对岩浆萃取地壳中的硫改变硫化物饱和度促成不混溶作用发生的可能性和条件进行了探讨,进一步讨论了岩浆演化过程中,亲铜元素(Ni、Cu、Co、Pt和Pd等)进入硫化物液相成为金属硫化物或先期进入先结晶的橄榄石、辉石矿物成为氧化物的物理化学行为,并通过加拿大Sudbury陨石撞击构造成因矿床复合热液对硫化物矿体形成贡献的讨论,提出了热液作用对岩浆硫化物矿床成矿的可能贡献。分析判断了中国岩浆Cu-Ni-PGE硫化物矿床的成矿特点和金川超大型岩浆Cu-Ni-PGE矿床外围的找矿潜力。 相似文献
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前言矿床的开发已有七千多年的历史,但直到16世纪中叶,才提出有关矿床成因的某些观点。一百年后,Descartes(1644)认为矿床物质来自地球深部,这成为后来铜、镍来自地幔的始祖。 19世纪中期,法国著名地质学家Elie de Beaumont(1847)认识到镁铁、超镁铁岩中铬、镍、铂等矿床的分结现象。1893年发现了萨德伯里铜镍矿床。此后人们普遍重视镁铁超镁铁岩有关铜镍硫化物矿床的研究。20世纪初,(1929)提出硫化铜镍矿床的 相似文献
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引言岩浆硫化物矿石中铂族元素的浓度显示一个值得注意的数值范围,从一个矿床到另一个矿床可以有数量级的变化。例如Merensky层(布什维尔德杂岩体)的矿石,硫化物少于2(重量％),仅为萨德伯里矿石的1/15到1/20,而Pt和Pd的总量却是典型萨德拍里矿床的10 相似文献
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吉林省岩浆铜镍硫化物矿床地质特征及成矿模式 总被引：3，自引：0，他引：3
吉林省是我国岩浆铜镍硫化物矿床的矿化集中区之一.本文总结了该省基性、超基性岩体及铜镍矿床赋存的大地构造环境,阐明了深断裂对岩体和矿床的控制作用,岩体及矿床地质特征,以及矿床成因、成矿作用和成矿模式. 相似文献
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东天山香山铜镍矿区构造特征与成岩成矿 总被引：4，自引：1，他引：4
香山铜镍矿床属典型的岩浆型铜镍硫化物矿床，产于东天山东段黄山-镜儿泉铜镍成矿带中，矿床形成主要受岩浆作用和构造作用控制．岩浆作用为矿床的形成提供了物质来源及成矿元素的熔离富集，构造作用为成矿物质提供了上侵通道和容矿空间．矿区断裂构造以韧性剪切带为主，具多级构造组合特点，共划分出4级构造层次，各级构造与成岩成矿有密切关系．I级构造控制基性。超基性岩带的分布；Ⅱ级构造控制基性—超基性岩体群的分布；Ⅲ级构造控制基性—超基性岩体或矿体的形态、产状；Ⅳ级构造控制岩相带或矿体的产出． 相似文献
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矿床是一种复杂系统,而成矿作用则是一种复杂的动力学过程。矿床成因的基本问题归根结底是成矿作用动力学问题（於崇文,1994）。成矿作用动力学研究成矿作用的速率、机制和过程。构造动力是成矿的基本因素之一,不同构造动力体制产生不同的成矿系统（翟裕生,2002）。常见的构造动力学体制有七种类型：伸展拉伸、挤压收缩、走滑、隆升、沉降、大型韧性剪切和大型陨石撞击（翟裕生,2003）。胶东金矿与中生代岩浆作用关系密切,对于指导区域找矿研究岩浆的隆起意义重大（吕古贤,2016）,控矿断裂和蚀变岩都是岩浆成岩之后的产物。胶东地区长期处于大陆边缘,构造成岩成矿作用过程表现出复杂性和多样性（邓军,1999）,研究构造性质与金矿的关系,认为胶东金矿是花岗岩和变质岩之间剪切拆离滑脱破碎岩带受岩浆期后热液交代蚀变的产物（吕古贤,2013）。岩浆期后的热液交代岩浆岩蚀变成矿,控制蚀变岩的断裂破碎岩以及断裂对成矿的控制作用一直是研究的重点。 相似文献
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The 1850 Ma Sudbury Igneous Complex (SIC), considered to be a composite melt sheet of a major meteorite impact, has been deformed into an oval-shaped basin known as the Sudbury Structure. This paper explores to what extent this deformation has been communicated to the surrounding Archean basement around the northern margin of the SIC.Paleomagnetism of 2450 Ma Matachewan dykes and 1850 Ma impact breccia along a traverse, about 100 km-long and normal to strike of the contact between the SIC and the basement, suggests that the basement beneath the NW corner of the Sudbury Structure has been tilted to the SE within about 10 km of the contact. At this distance a possible fault separates the tilted region from one that shows no evidence of tilting. Petrographically the dykes out to a distance of about 50 km distant from the SIC are altered to upper greenschist facies of metamorphism with a fibrous amphibole replacing pyroxene and with loss of primary texture that characterizes less altered Matachewan dykes at distances greater than 50 km. The direction of magnetization found in the altered Matachewan dykes is an overprint which is probably associated with regional metamorphism related to orogenesis, or possibly with thermo-chemical alteration associated with SIC emplacement. The direction of the component is compatible with an age of about 1.8 to 1.9 Ga suggesting that the Penokean orogen is the most likely cause, if not the impact event. The paleomagnetism of the breccias, together with shatter cone orientation data, suggests that within 10 km of the SIC/basement contact, basement tilting to the southeast increases towards the SIC. 相似文献
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关于加拿大Sudbury构造的成因,现在的学者大多认同其形成于陨石撞击。为了找到更加强有力的证据,文中对取自Sudbury冲击角砾岩中的锆石进行了研究。Sudbury冲击角砾岩是Sudbury构造的特殊现象,采用扫描电镜、结合拉曼光谱方法从角砾岩的锆石中发现了显微构造和相变的证据。所观察到的显微构造呈一系列面状构造(planar microstructure),在3个方向上平行展布,并相互剪切。Sudbury角砾岩锆石的典型Raman谱线中,除锆石的几个峰外,在640cm-1和817cm-1也可见两个峰,并可分别与铁橄榄石和一种ZrO2相匹配。该ZrO2相的谱线也不同于典型的斜锆石,却与López等合成的一种含有0.5%(质量分数)TiO2的ZrO2相非常相似。这些证据显示,一些锆石的颗粒边缘发生了如下反应:ZrSiO4+2FeOZrO2+Fe2SiO4,并已变成了一种ZrO2相和铁橄榄石(fayalite)。这些显微构造和相变特征都能够说明Sudbury角砾岩受到过高压冲击,并进一步支持Sudbury构造的陨石撞击成因。 相似文献
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《International Geology Review》2012,54(12):1079-1102
In the past few years, meteoritic and cometary impacts have emerged as a major geological agent in the construction and evolution of planetary surfaces. Formation of complex central ring, peak ring and multiring craters involves excavation and melting of large volumes of crustal material. High-resolution geophysical mapping measuring gravity, magnetics, and topography of the Moon and Mars have recently provided information on the subsurface structure of large basins and aided in identifying buried giant craters. The terrestrial crater record has been significantly erased by tectonic, magmatic, and erosion processes and only a small proportion of impact structures remain. Record of multiring craters is limited to three examples: Vredefort, Sudbury and Chicxulub. Deep geophysical surveys and geochemical and isotopic studies of those craters provide means to evaluate the influence of large impacts on the lithospheric and crustal evolution by providing estimates of excavation depth and volume, amounts of material fragmented, ejected, vaporized and melted, and effects on the crustal stratigraphy and crustal thickness. Analyses on the melt from Vredefort, Sudbury, and Chicxulub indicate andesitic composition derived from lower-crustal material. The melt formed inside the lower transient cavity from lower crustal material that was then redistributed and emplaced in upper-crustal levels, resulting in crustal redistribution. Crystalline basement clasts fragmented and incorporated into the breccias show varying degrees of alteration but no significant thermal effects. Ejecta were deposited locally within the crater region and ballistic material and fine ejecta are globally distributed on the planetary surface. Impacts influence the crust–mantle boundary, with Moho uplift. Material from the mantle was not incorporated into the melt and impact breccias, indicating that the excavation cavities were confined to the lower crust. This is also apparently the case for the giant basins on the Moon, including the 2500 km diameter South Pole-Aitken Basin. Considering the numbers of large multiring basins, possible flux of large impacts, and effects on target surfaces, crustal scale redistribution of material during those large impacts has played a major role in the evolution of planetary surfaces. 相似文献
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A. Deutsch R. A. F. Grieve M. Avermann L. Bischoff P. Brockmeyer D. Buhl R. Lakomy V. Müller-Mohr M. Ostermann D. Stöffler 《International Journal of Earth Sciences》1995,84(4):697-709
The occurrence of shock metamorphic features substantiates an impact origin for the 1.85 Ga old Sudbury Structure, but this has not been universally accepted. Recent improvements in knowledge of large-scale impact processes, combined with new petrographic, geochemical, geophysical (LITHOPROBE) and structural data, allow the Sudbury Structure to be interpreted as a multi-ring impact structure. The structure consists of the following lithologies: Sudbury Breccia —dike breccias occurring up to 80 km from the Sudbury Igneous Complex (SIC); Footwall rocks and Footwall Breccia — brecciated, shocked crater floor materials, in part thermally metamorphosed by the overlying SIC; Sublayer and Offset Dikes, Main Mass of the SIC and Basal Member of the Onaping Formation (OF) — geochemically heterogeneous coherent impact melt complex ranging from inclusion-rich basal unit through a dominantly inclusion-free to a capping inclusion-rich impact melt rock; Grey Member of OF — melt-rich impact breccia (suevite); Green Member of OF — thin layer of fall back ejecta; Black Member of OF — reworked and redeposited breccia material; Onwatin and Chelmsford Formations — post-impact sediments. Observational and analytical data support an integrated step-by-step impact model for the genesis of these units. Analysis of the present spatial distribution of various impact-related lithologies and shock metamorphic effects result in an estimated original rim-to-rim diameter of the final crater of 200 or even 280 km for the Sudbury Structure, prior to tectonic thrusting and deformation during the Penokean orogeny. 相似文献
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加拿大萨德伯里奈恩( Nairn) 铜多金属矿
地球化学特征及意义 总被引：1，自引：0，他引：1
[摘 要] 加拿大奈恩(Nairn)工作区位于萨德伯里(Sudbury)镍铜矿集区南西方向约50 km,工作区
内的矿化类型可划分两类:淤产于辉长岩中的铜镍矿化和于产于石英角砾岩中的铜矿化。两种矿石的
微量元素和稀土元素特征较为相似, 高场强元素中富集Th-Zr-Hf 而相对亏损Nb-Ta 等,大离子亲石元
素中富集Rb-U-Pb 而相对亏损Ba-P-Ti 等,稀土元素相对富集轻稀土,轻稀土元素分馏程度明显,而重
稀土元素分馏程度不明显,铈异常不明显,而铕异常变化较大,总体上表现为负异常。上述特征暗示其
物质来源可能相似,结合其矿物组合和本区围岩特征来看, 铜镍矿石主要与中-基性岩浆有关,而石英
角砾岩的铜矿化主要与后期的岩浆热液有关,表明两种矿化类型主要与本区岩浆的结晶分异作用有关,
早期的高温铜镍硫化物随辉长岩中硅酸盐矿物的结晶而后生成,晚期的含矿热液沿构造产生的断层破
碎带迁移并最终充填在构造裂隙中。从奈恩矿区成矿特征来看,本区辉长岩墙与上伏围岩的接触部位,
特别是构造发育或相互交汇处将为最有利的成矿部位。 相似文献
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On the track of the elusive Sudbury impact: geochemical evidence for a chondrite or comet bolide 
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下载免费PDF全文 Siderophile and lithophile trace element data for 69 samples from the Sudbury impact crater fill (Onaping Formation) and quartz diorite offset dikes help constrain the sources of the established moderately elevated platinum group element signature associated with the impact structure. The siderophile element distribution of the crater fill requires contributions from bulk continental crust, mafic rocks and a chondritic component. A mantle component is absent, but the involvement of mid to lower crust is implied. After considering post‐impact hydrothermal alteration, melt heterogeneity and mafic target admixture, the projectile elemental ratios were determined on a more robust data subset. Chondrite discrimination diagrams of these ratios identify an ordinary or enstatite chondrite as the most probable source of meteoritic material in the Sudbury crater fill. However, the relative and absolute siderophile element distributions within the impact structure as well as bolide size models are congruent with the bolide being a comet that had a chondritic refractory component. 相似文献
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Geologic marks related to extraterrestrial impact events, such as impact split gravels, impact brecciate layers, impact dikes, microirghizites, microtektites, especially meteoritic residues, were discovered on the boundary between Sinian/Cambrian at Tianmenshan of Western Hunan, which may possibly demonstrate that an extraterrestrial impact event has ever occurred there on the S/C boundary. 相似文献
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天门山震旦/寒武系界线上地外撞击事件痕迹 总被引：2，自引：0，他引：2
从湘西北天门山震旦—寒武系界线上发现的冲击砾裂、冲击角砾、冲击岩脉、微球粒撞击玻粒(microirghi-zites)、微球粒玻璃陨石(microtektites),特别是陨石碎屑残迹现象,可能表明:在震旦—寒武系界线上曾经发生过地外撞击的事件。 相似文献
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Györgyi Tuba Ferenc Molnár Doreen E. Ames Attila Péntek David H. Watkinson Peter C. Jones 《Mineralium Deposita》2014,49(1):7-47
The Amy Lake PGE zone is a “low-sulfide-type” Cu-(Ni-)PGE mineralization in the East Range footwall of the 1.85 Ga Sudbury Igneous Complex occurring in a 100-m-wide Sudbury Breccia belt that coincides with an impact-related major fracture zone (Bay Fault zone). Detailed hydrothermal alteration mapping, fluid inclusion, trace element, and stable isotope studies revealed a complex alteration and mineralization history in a multi-source, multi-stage Sudbury-related hydrothermal system. The two major stages of syn-Sudbury hydrothermal activity are characterized by similarly high-salinity, high-temperature fluids that are (1) locally derived from footwall granophyre bodies, and typified with high Ni/Cu and PGE/S ratios and high REE contents (magmatic–hydrothermal stage), and (2) a more voluminous Cu–Ni–PGE-rich fluid flux probably originated from the Sudbury Igneous Complex/footwall contact (hydrothermal stage). The second hydrothermal flux was introduced by brittle fractures in the area and resulted in a complex zonation of alteration assemblages and mineralization governed by local footwall composition. The Sudbury-related hydrothermal event was overprinted by shear-related epidote veining and calcite–chlorite replacement, both regionally present in the Sudbury structure. Based on analogies, the most important factors involved in the formation of hydrothermal low-sulfide mineralization are proposed to be (1) accumulation of PGE-enriched fluids, (2) large-scale brittle structures as conduits to these fluids, and (3) adequate host rock composition as a chemical trap resulting in sulfide and PGM precipitation. In environments meeting these criteria, hydrothermal PGE mineralization is known to have formed not only in the Sudbury footwall but also from mafic–ultramafic intrusions associated with primary magmatic PGE from several locations around the world. 相似文献
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《International Geology Review》2012,54(2):291-325
We performed detailed field and drill core mapping of partial melting features and felsic rocks (footwall granophyres, FWGRs) representing segregated and crystallized partial melts within the contact aureole of the Sudbury Igneous Complex (SIC) in the 1.85 Ga Sudbury impact structure. Our results, derived from mapping within the North (Windy Lake, Foy, Wisner areas) and East Ranges (Skynner, Frost areas) of the structure, reveal that partial melting was widespread in both felsic and mafic footwall units up to distances of 500 m from the basal contact of the SIC. Texturally and mineralogically, significant differences exist between rocks formed by partial melting within and between localities. In general, however, melt bodies are dominated by different quartz-feldspar intergrowths (e.g. granophyric, graphic) and miarolitic cavities up to 5 cm in diameter. Major and trace element compositions of Wisner and Frost FWGRs imply that they crystallized from melts dominantly derived from partial melting of felsic Levack Gneiss and Cartier granitoid rocks, as well as from gabbroic rocks only at Frost. These results accord with our observations on in situ partial melting features and crystallized melt of microscopic scale in both felsic and mafic rocks. We conclude that partial melting occurred at a pressure of 1.5 ± 0.5 kbar and at temperatures up to 750°C in the Wisner area and up to 900°C in the Frost and Windy Lake areas. Segregations of partial melt into veins and dikes are present in all localities, and were promoted by deformation of the Sudbury structure in the Penokean orogeny as indicated by dominant strike directions. Whereas veins and dikes reflect brittle conditions during melt migration, sheared melt pods in the Sudbury breccia matrix indicate ductile conditions during their crystallization. Our results suggest a close genetic association of partial melting, melt segregation, and hydrothermal processes responsible for remobilization of Cu–Ni–PGE sulphides into and within the SIC footwall. 相似文献