http://www.sciencedirect.com/science/article/pii/S1674987111000764   总被引：1，自引：0，他引：1  

Guoxiang Chi  Chunji Xue  Hairuo Qing  Wei Xue  Jiangwei Zhang  Yunqiang Sun 《地学前缘(英文版)》2012,3(1):73-84

The Jinding Zn-Pb deposit has been generally considered to have formed from circulating basinal fluids in a relatively passive way,with fluid flow being controlled by structures and sedimentary facies,similar to many other sediments-hosted base metal deposits.However,several recent studies have revealed the presence of sand injection structures,intrusive breccias,and hydraulic fractures in the open pit of the Jinding deposit and suggested that the deposit was formed from explosive release of overpres-sured fluids.This study reports new observations of fluid overpressure-related structures from underground workings(Paomaping and Fengzishan).which show clearer crosscutting relationships than in the open pit.The observed structures include:I) sand(±rock fragment) dikes injecting into fractures in solidified rocks:2) sand(±rock fragment) bodies intruding into unconsolidated or semi-consolidated sediments;3) disintegrated semi-consolidated sand bodies;and 4) veins and breccias formed from hydraulic fracturing of solidified rocks followed by cementation of hydrothermal minerals.The development of ore minerals(sphalerite) in the cement of the various clastic injection and hydraulic fractures indicate that these structures were formed at the same time as mineralization.The development of hydraulic fractures and breccias with random orientation indicates small differential stress during mineralization,which is different from the stress field with strong horizontal shortening prior to mineralization. Fluid flow velocity may have been up to more than 11 m/s based on calculations from the size of the fragments in the clastic dikes.The clastic injection and hydraulic fracturing structures are interpreted to have formed from explosive release of overpressured fluids,which may have been related to either magmatic intrusions at depth or seismic activities that episodically tapped an overpressured fluid reservoir.Because the clastic injection and hydraulic structures are genetically linked with the mineralizing fluid source,they can be used as a guide for mineral exploration.  相似文献   

激发极化法在冰湖沟金矿区找矿中的应用     

刘涛  李凯春  李国辉 《吉林地质》2011,30(1):81-84

冰湖沟金矿区岩浆活动频繁、构造较为发育,区内有Ⅴ号角砾岩等赋矿岩体.角砾岩体矿化规模大,离矿体越近,矿化蚀变越强.标本测定表明,角砾岩体矿化蚀变后极化率显著增大,因此本区具有开展激电找矿工作的物性基础.在该区开展的激电工作成果得到了钻孔验证,指导了该区的地质找矿工作.  相似文献   

云南武定迤纳厂铁铜矿岩浆角砾岩LA-ICP-MS 锆石U-Pb年龄及其意义   总被引：5，自引：1，他引：4  

侯林  丁俊  邓军  廖震文  彭惠娟 《地质通报》2013,32(4):580-588

康滇地区是中国西南地区重要的元古宙铁铜成矿带.该地区元古宙昆阳群中串珠状分布岩浆角砾岩,周边分布大量铁铜矿床.选取武定迤纳厂东方红矿段穿插斜切入迤纳厂组的岩浆角砾岩,挑选胶结物中的岩浆锆石进行LA-ICP-MS测年,得到复合岩浆锆石内核207pb/206pb年龄为2193Ma±8Ma,代表深部围岩原生锆石年龄;岩浆锆石或复合岩浆锆石边缘环带207Pb/206Pb年龄为1739Ma±13Ma,代表岩浆侵位年龄;下交点年龄为980Ma±11Ma,代表变质年龄.结合相关资料判断,迤纳厂组与上昆阳群、大红山群、河口群均为1.7Ga左右昆阳板内裂谷拉张、岩浆侵位/喷发的同时异相产物.这对在滇中地区昆阳裂谷中,元古宙地层内的岩浆角砾岩周边寻找IOCG(IRON-OXIDE-COPPER-GOLD,铁氧化物-铜-金)型铁铜矿具有重要的启示.  相似文献   

地震微裂群区与岩浆热液成矿     

王铁军 《地质找矿论丛》2013,28(4):535-539

岩浆热液矿床是在地壳浅部形成的,恰好位于浅源地震的震源深度范围.文章将地震机制中的微裂隙群区理论引入到岩浆热液矿床成矿过程中,地震组合模式中闭锁带必须在下一次断裂滑动之前破坏,所以这个带为微裂群区和它相关的震源区的核心.文章认为微裂群区理论不但揭示了孕震机制,同时也揭示了岩浆热液矿床形成过程,岩浆热液侵位与断裂形成过程中微裂群区的形成发展密切相关,成矿期矿体范围内应力场与区域应力场呈共轭关系.微裂群区即为岩浆热液矿床的矿化富集场,控矿的隐爆角砾岩带也与微裂群区密切相关.  相似文献   

Magma mingling in the Tungho area,Coastal Range of eastern Taiwan     

Yu-Ming Lai  Sheng-Rong Song  Yoshiyuki Iizuka 《Journal of Volcanology and Geothermal Research》2008

Complex rocks, consisting of different lithologic breccias and sediments in the Tungho area of the southern Coastal Range, eastern Taiwan, were formed by magmas and magma–sediment mingling. Based on field occurrences, petrography, and mineral and rock compositions, three components including mafic magma, felsic magma, and sediments can be identified. The black breccias and white breccias were consolidated from mafic and felsic magma, respectively. Isotopic composition shows these two magmas may be from the same source. Compared to the white breccias, the black breccias show clast-supported structures, higher An values in plagioclase, higher contents of MgO, CaO, and Fe₂O₃ and lower SiO₂, greater enrichment in the light rare earth elements (LREE), and depletion in the heavy rare earth elements (HREE). The white breccias show matrix-supported blocks and mingling with tuffaceous sediments to form peperite. Physical and chemical evidence shows that the characteristics of these two components (mafic and felsic magmas) are still apparent in the mingled zone. According to their petrography, mafic and felsic magmas did not have much time for mingling. White intrusive structures and black flow structures show that mingling occurred before they solidified. Finally, the occurrence of mingling between magmas and sediments suggests that the mingling has taken place at the surface and not in the magma chamber.  相似文献   

胶东地区层间滑动角砾岩型金矿成矿远景   总被引：10，自引：2，他引：8  

曾庆栋  沈远超 《地质与勘探》2000,36(6):36-39

胶东地区中生代盆地周边存在层间滑动断层,它控制了层间滑动角砾岩型金矿（如蓬家夼金矿）的产出,根据盆地的分布及矿化特征,划分了胶东地区四个层间滑动砾岩型金矿成矿远景区,蓬家夼成矿远景区、菜西远景区、牟平西部远景区、栖霞远景区,这些地区有望成为胶东地区甚至我国东部新的黄金工业基地。  相似文献   

新疆哈密坡子泉地区首次发现隐爆角砾岩筒     

白云山  彭湘萍 《新疆地质》1999,(2)

新疆哈密坡子泉地区首次发现的隐爆角砾岩筒处在塔里木板块北缘活动带卡瓦布拉克微板块之上,基底地层为前寒武系,盖层主要为石炭系,受ＮＥ向断裂带控制。隐爆角砾岩特征及产出环境相似于金伯利岩。  相似文献   

熊耳山地区内生金矿床成矿系列     

葛良胜 《地质与资源》1994,3(2):114-122

按容矿空间和控矿因素,可将熊耳山地区内生金矿床划分为角砾岩型、构造破碎带蚀变岩型、石英脉型及由不同控矿因素复合控制的复合类型等。空间上不同类型之间具有密切的共生过渡关系。太华群原岩中的金在变质热液作用下被活化迁移至有利的构造部位,发生局部富集,形成"矿胚"或"矿胚"的发展,并为后期岩浆热液再次搬运,参与成矿。燕山中晚期钙碱性岩浆岩具较大的成矿能力,是本区金矿床的主要矿源。不同类型矿床稳定同位素及包裹体特征具相似的变化特点,分析表明,成矿流体主要源自岩浆,在成矿早期和晚期,不同地区可能有不同程度的变质水或大气水加入。作者认为,区内不同类型的金矿床是在统一的大地构造环境和成矿背景中形成的,有统一的矿质和介质来源,具相同或相似的成因,以发育角砾岩型金矿床为特点,以构造破碎带蚀变岩和角砾岩型为主要矿床类型,形成一个特定的矿床组合,即熊耳山地区内生金矿床系列。  相似文献   

Radiolarian‐based study on the fabric and the formation process of the Early Cretaceous mélange near Zhongba,Yarlung–Tsangpo Suture Zone,southern Tibet     

Xin Li  Atsushi Matsuoka  Yalin Li  Yushuai Wei  Chengshan Wang 《Island Arc》2019,28(1)

The Yarlung–Tsangpo Suture Zone (YTSZ), as the southernmost and youngest among the sutures that subdivides the Tibetan Plateau into several east–west trending blocks, marks where the Neo‐Tethys was consumed as the Indian continent moved northward and collided against the Eurasian continent. Mélanges in the YTSZ represent the remnants of the oceanic plate through subduction and collision. Mélanges are characterized by a highly sheared volcanoclastic or siliceous mudstone matrix including blocks of chert, claystone, and basalt. Detailed radiolarian analyses are conducted on the mélange near Zhongba County. Macroscopic, mesoscopic, and microscopic observations are combined in order to elucidate the relationships among age, lithology, and structure of blocks in the mélange. Reconstructed ocean plate stratigraphy includes Lower Jurassic limestone within the chert sequence accumulated at a depth near the CCD (Unit 2), Upper Jurassic thin‐bedded chert interbedded with claystone deposited in the wide ocean basin (Unit 3), and Lower Cretaceous chert with siliceous mudstone (Units 4 and 5), representing the middle parts of ocean plate stratigraphy. The results highlight the fabric of brecciated chert on mesoscopic scale, which is thought to be due to localized overpressure. The formation of mesoscopic and microscopic block‐in‐matrix fabrics in the mélange is proposed for the chert and siliceous mudstone bearing different extents of consolidation and competence during the progressive deformation of accreted sediments at shallow‐level subduction.  相似文献   

Formation of mud clast breccias and the process of sedimentary autobrecciation in the hominin-bearing (Homo naledi) Rising Star Cave system,South Africa     

Jelle P. Wiersma  Eric M. Roberts  Paul H. G. M. Dirks 《Sedimentology》2020,67(2):897-919

Unconsolidated mud clast breccia facies in the hominin-bearing (Homo naledi) Rising Star Cave, Cradle of Humankind, South Africa, are interpreted to have formed through a process termed sedimentary autobrecciation in this study. This process, by which most of the angular mud clast breccia deposits are thought to have formed autochthonously to para-autochthonously via a combination of erosion, desiccation, diagenesis and microbial alteration of laminated mud deposits, is thought to have taken place under relatively dry (i.e. non-flooded) conditions inside the cave. Subsequently, gravitational slumping and collapse was the dominant mechanism that produced the mud clast breccia deposits, which commonly accumulate into debris aprons. The mud clast breccia is typically associated with (micro) mammal fossils and is a common facies throughout the cave system, occurring in lithified and unlithified form. This facies has not been described from other cave localities in the Cradle of Humankind. Additionally, sedimentary autobrecciation took place during the deposition of some of the fossils within the Rising Star Cave, including the abundant Homo naledi skeletal remains found in the Dinaledi Subsystem. Reworking of the mud clast breccia deposits occurs in some chambers as they slump towards floor drains, resulting in the repositioning of fossils embedded in the breccias as evidenced by cross-cutting manganese staining lines on some Homo naledi fossil remains. The formation of the unlithified mud clast breccia deposits is a slow process, with first order formation rates estimated to be ca 8 × 10⁻⁴ mm year⁻¹. The slow formation of the unlithified mud clast breccia facies sediments and lack of laminated mud facies within these deposits, indicates that conditions in the Dinaledi Chamber were probably stable and dry for at least the last ca 300 ka, meaning that this study excludes Homo naledi being actively transported by fluvial mechanisms during the time their remains entered the cave.  相似文献