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11.
By us considered as Albo-Aptian in age and generated through halokinetic processes, the Bosmendiette breccias have been recently interpreted as Selandian (Palaeocene) globigerine-bearing sediments deposited in sub-marine canyons within a deep trough crossing the Pyrenees, from the Mediterranean Sea to the Atlantic Ocean. These breccias are really azoic in their lower part and contain a scarce microfauna including radolarians and benthic foraminifera at the top of the formation. They are unconformably covered by the Urgo-Aptian limestones and marls and indicate, under opening marine conditions, Lower Cretaceous collapse movements and northward sliding of the Jurassic slumped cover, related to the growth of the Béloscare–Apoura diapir. To cite this article: J. Canérot et al., C. R. Geoscience 336 (2004).  相似文献   
12.
西藏东部隐爆角砾岩特征及其含矿性   总被引:1,自引:0,他引:1       下载免费PDF全文
西藏东部发育大量与喜马拉雅期斑岩密切共生的隐爆角砾岩筒(脉)。隐爆角砾岩大都遭受强烈的矿化蚀变,其中的成矿元素金、银、汞等强烈富集。包裹体和同位素的资料证实爆破流体是一种与岩浆有成因联系的、介于岩浆与岩浆期后成矿热液之间的过渡性高温流体。  相似文献   
13.
湖南常宁县康家湾铅锌金矿硅化角砾岩岩石地球化学特征   总被引:8,自引:0,他引:8  
许德如  刘静  陈广浩 《地质科学》2002,37(3):356-364
湖南常宁县康家湾铅锌金矿床硅化角砾岩带由未硅化角砾岩—极弱硅化角砾岩—硅化角砾岩—强硅化角砾岩(似硅质岩)组成,产于侏罗系与下伏二叠系间的不整合面附近,角砾成份复杂,充填物和胶结物类型多样。随着硅化程度的加强,硅化角砾岩带SiO2含量变化大,最高可达95.34%,而Al2O3、MgO、FeO、K2O、Na2O、CaO、CO2和P2O5含量特别是MgO、CaO、CO2和P2O5含量明显降低,且K2O>Na2O,TiO2的含量显著偏低。硅化角砾岩带LREE/HREE比值为1.95~4.93,Ce(δCe=0.44~0.81)和Eu(δEu=0.58~0.89)均为弱负异常,属轻稀土富集型,但随硅化程度增高稀土元素含量显著减少:未硅化和弱硅化角砾岩稀土元素总量较高,为(176.82~318.93)×10-10,与当冲组泥质岩配分曲线相似;硅化强烈的角砾岩稀土元素总量低,为(7.71~65.95)×10-10,与下伏栖霞组灰岩稀土元素配分曲线极为相似。结合微量元素F、Ba、Cl、Cr、Ni、Sr、V研究结果及硅化角砾岩带自底部至顶部特有的下粗上细的韵律性层理构造,认为康家湾铅锌金矿床硅化角砾岩带是在地台体制向地洼体制转变期的大地构造环境下,由于地壳快速隆升,二叠纪灰岩、泥质岩、石英砂岩等岩石剥蚀,在古河流环境下搬运、沉积形成的。此  相似文献   
14.
The Duocaima carbonate-hosted Pb-Zn deposit is a newly found large deposit in the southern area of Qinghai Province.In this paper, the characteristics, genesis, significance to Pb-Zn mineralization of the widely developed breccias, and the ore-forming process have been carefully studied based on geological documentation of drilling holes, microscopic observations of petrography and microstructure and some stable isotope measurements.Based on the compositions of the clast and matrix, the breccias can be classified into three types: limestone clasts cemented by marl; limestone clasts with fine-grained calcareous materials; and limestone clasts cemented by hydrothermal calcite.The mineralization in the first type of breccia is weak, whereas it is strong in the latter two types of breccias.According to the locations of occurrence and structural characteristics of the breccias along with the relationship between the breccias and mineralization, part of the limestone clasts that are cemented by marl and outcrop in the contact zone between the Wudaoliang Formation(Nw) and the underlying Jiushidaoban Formation(Pj) are attributed to synsedimentary fault-genetic breccia, whereas the last of the limestone clasts that are cemented by marl and developed in the Jiushidaoban Formation(Pj) are attributed to the breccia generated by karst cave collapse; the limestone clasts with fine-grained calcareous materials and the limestone clasts cemented by hydrothermal calcite are attributed to breccia formed by hydrothermal dissolution.The breccia formed by karst collapse had consistently evolved for a long period of time, while the breccias with other origins were formed around the period of mineralization(i.e., about or slightly later than 20–16 Ma).The breccia generated by karst cave collapse and hydrothermal dissolution are somewhat related; the formation of the breccia from karst cave collapse provided open space for the later mineralization and reaction between hydrothermal fluids and host rocks, and the subsequent strong dissolution by hydrothermal fluids transformed some of the breccia formed earlier by karst cave collapse.Meanwhile, carbonate host rocks with breccias and brecciaed mineralization can be a potential sign of Mississippi Valley Type(MVT) deposits and important indicators for regional mineral exploration.The δ13CV-PDB, δ18OVSMOW, and 87Sr/86 Sr values of hydrothermal calcite in the Duocaima deposit range from 4.3‰ to 7.1‰, 14.9‰ to 20.1‰, and 0.707494 to 0.708185, respectively; the δ13CV-PDB, δ18OV-SMOW, and 87Sr/86 Sr values of the host limestones of the Jiushidaoban Formation range from 3.6‰ to 5.3‰, 18.0‰ to 20.5‰, and 0.707372 to 0.707945, respectively.The δ13CV-PDB and 87Sr/86 Sr values of hydrothermal calcite and limestone are similar, indicating single sources of C and Sr in this deposit, with the likely source being the limestone of the Jiushidaoban Formation.The minor scattering of the δ18OV-SMOW values suggests that different O isotope fluids underwent the isotope exchange reaction.The C-O-Sr isotope characteristics indicate that the host limestones experienced a dissolution and precipitation process during mineralization, which is beneficial to improving the porosity of host rocks and promoting the precipitation of metal sulfides.The δ34SV-CDT value of the breccia-type mineralization sulfides ranges from-30.4‰ to-0.3‰; that is, the δ34SV-CDT value is negative with considerable variation, illustrating that during the breccia-type mineralization process, the bacteriogenic reduction of sulfates provided the vast majority of sulfur, whereas the thermochemical reduction of sulfates was relatively unimportant.The brecciation that occurred as a result of karst cave collapse was mainly generated by the dissolution of groundwater; however, the brecciation related to hydrothermal dissolution and mineralization processes were caused by mixing of different fluids.  相似文献   
15.
Keilite (Fe>0.5,Mg<0.5)S, the iron-dominant cubic analog of niningerite, (Mg>0.5,Fe<0.5)S, occurs in enstatite chondrites [Shimizu, M., Yoshida, H., Mandarino, J.A., 2002. The new mineral species keilite, (Fe,Mg)S, the iron-dominant analog of niningerite. Can. Mineral. 40, 1687–1692]. I find that keilite occurs only in enstatite chondrite impact-melt rocks and impact-melt breccias. Based on the phase relations in the system MgS–MnS–CaS–FeS [Skinner, B.J., Luce, F.D., 1971. Solid solutions of the type (Ca,Mg,Mn,Fe)S and their use as geothermometers for the enstatite chondrites. Am. Mineral. 56, 1269–1296], I conclude that keilite formed from niningerite or alabandite (Mn>0.5,Fe<0.5)S by reaction with troilite (FeS) at elevated temperatures of well above 500 °C (the lowest equilibration temperature of keilite), but it is likely that the maximum temperatures during melting experienced by keilite-bearing impact-melt rocks and impact-melt breccias were considerably higher, perhaps >1500 °C, as indicted by the occurrence of euhedral enstatite that formed from a melt [McCoy, T.J., Dickinson, T.L., Lofgren, G.E., 1999. Partial melting of the Indarch (EH4) meteorite: a textural, chemical, and phase relations view of melting and melt migration. Meteorit. Planet. Sci. 34, 735–746]. Based on the classifications of the keilite-bearing meteorites as impact-melt rocks and impact-melt breccias and my own textural observations, I conclude that this elevated temperature was reached as a result of impact and not internal heating and melting, followed by fast cooling, thus, quenching in keilite. Enstatite chondrite impact-melt rocks and impact-melt breccias that do not contain keilite may have been more deeply buried after impact and, hence, cooled slowly and were annealed so that FeS exsolved from keilite, concomitant with the formation of niningerite, alabandite or various (Mn,Mg,Fe) mixed sulfides.  相似文献   
16.
MIL090036是一块在南极新发现的月球陨石,属于斜长岩质月球角砾岩。本文对这块陨石开展了详细的岩石学、矿物学特征观察与研究。MIL090036月球陨石具有典型的碎屑结构。碎屑包括岩屑、矿屑和玻屑。岩屑类型有斜长岩岩屑、辉长质斜长岩岩屑、辉长岩岩屑、风化角砾岩岩屑、橄长岩岩屑、微斑熔融角砾岩岩屑、复合角砾岩岩屑等;矿屑有辉石、斜长石、橄榄石、钛铁矿等;玻屑主要为长石质。基质由玻璃质、重结晶的细粒矿物和矿屑胶结组成。辉长岩岩屑中的斜长石(An81-83)和斜长岩中的斜长石(An88-93)较其他碎屑中的斜长石(An90-98)贫钙。岩屑、矿屑和长石质玻屑中的辉石相对贫铁(Fs 12-35Wo3-44 En22-79),而含玻璃质的辉长岩岩屑中的辉石(Fs37-65Wo10-29 En21-49)与基质中的辉石(Fs18-69Wo3-45 En14-50)相对富铁。辉长岩质斜长岩中辉石成分变化范围最小(Fs24-27Wo7-14 En59-69)。矿屑橄榄石和分布于基质中的橄榄石铁镁含量(Fo57-79)相对岩屑中的橄榄石(Fo67-77) 变化范围大。橄榄石Fe/Mn比值为47-83(平均76)、辉石Fe/Mn比值为76-112(平均73),都与月球橄榄石和月球辉石一致。岩石结构、矿物模式组合和化学成分等特征表明MIL090036是来自Apollo和Luna采样范围外的样品。对MIL090036的矿物学、岩石学和化学成分的进一步研究将能够丰富我们对月表物质组成和演化的认识。  相似文献   
17.
中浅成含矿岩浆的隐爆作用机制与两相分离流动   总被引:2,自引:0,他引:2  
本文首次从物理上讨论了隐爆作用的具体机制,指出隐爆作用的本质是由超压导致相变而发生的一种快速物理反应。分析表明,岩浆上侵至低围压的中浅层环境→气水组分分离并产生气泡→后续岩浆提供高压力梯度而导致超压,即为隐爆作用得以发生的充要条件。模拟实验表明,在隐爆发生的瞬间,岩浆中的多相组分因密度差而发生分离流动,围岩则在爆轰冲击下局部碎裂并气、液化,从而使相关的热液活动及多种成矿作用得以进行,由此形成相应的隐爆角砾岩系列及其矿床组合.  相似文献   
18.
流体参与下的岩石破裂机制及其分形特征   总被引:1,自引:0,他引:1  
流体参与下的岩石破裂机制一般分为爆发作用、流化作用和液压致裂等,其分维值大小一般遵循爆发作用→流化作用→液压致裂.通过对凤凰山铜矿II号矿体不同地段的角砾岩进行分形统计分析,判明其属于液压致裂角砾岩,验证了分维值的大小与致裂能量之间的正相关关系.  相似文献   
19.
云南金顶超大型铅锌矿床沥青Re-Os法测年及地质意义   总被引:6,自引:3,他引:3  
油气藏与金属矿床在世界许多沉积盆地内共存,油气成藏与金属成矿的动力学关系备受关注。云南兰坪金顶产有中国目前最大铅锌矿床,也是世界上唯一陆相沉积岩容矿、且形成于新生代的超大型铅锌矿床。矿床中常见沥青、重油等有机质,它们的形成早于或晚于铅锌硫化物成矿存在明显分歧,限制了对油气成藏与铅锌成矿关系的认识。本文针对金顶超大型矿区以古新统云龙组含砾砂岩和砂砾岩为主岩铅锌矿石中沥青,开展了Re-Os法同位素测年,获得68±5Ma的等时线年龄(MSWD=9.2,n=6),指示金顶古油气成藏形成于古新世,先于铅锌硫化物大规模成矿;烃类物质具有通过热化学还原硫酸盐提供铅锌成矿所需硫化氢的客观条件;油气成藏与铅锌成矿在云南金顶矿区很可能是一个先后发生的连续地质过程,成藏为成矿奠基,成矿伴随着油气藏的破坏。  相似文献   
20.
烟筒桥子金矿床是以隐爆角砾岩筒型矿化为主体的金矿床,以矿区3号矿体为主要对象,通过对该矿体岩、矿石微量元素的地球化学分析,探讨了该类矿体地球化学特征。结果表明,在所分析的12种元素中,Au与Ag、Bi、Pb和Zn元素具有相似的富集趋势。这些元素的的富集规律可用于隐爆角砾岩体中金矿体的找矿标志之一。  相似文献   
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