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81.
热液矿床石英铅同位素组成及其地质意义 总被引:1,自引:0,他引:1
作者以若尔盖铀矿床为例,研究了含矿热液形成的石英脉石英的铅同位素组成,并将其作为联系母源铅同位素组成的桥梁,判别铀的来源。结果表明,矿床中石英铅同位素组成与含矿黄铁矿和中酸性构造-岩浆成因的花岗岩铅同位素组成具线性演化关系。由此提出含矿热液中的铀来自中酸性构造-岩浆岩而不是地层岩石的新见解,同时提出利用热液石英铅同位素组成判别非放射性矿床成矿元素来源的可能性。 相似文献
82.
The aim of this study was to analyse the hydrogeologic role of siliciclastic deposits and marly‐clayey‐calcareous successions within the carbonate Apennine chain (southern Italy). The study was carried out along the northern part of the Matese carbonate massif through (1) the hydraulic characterization of siliciclastic rocks in a test site, by means of Lugeon tests, and (2) the identification of the groundwater flow system discharging at an important spring located within a marly‐clayey‐calcareous succession in a second test site, by means of isotopic investigations. The results showed that the investigated siliciclastic deposits and marly‐clayey‐calcareous successions may allow significant groundwater discharge from carbonate aquifers. Thus, they do not everywhere behave as aquitard, contrary to the previous model. Instead, groundwater flows through the upper part of these successions, where stress release fracturing enhanced rock permeability in the near‐surface bedrock. Thus, these successions may locally be a new groundwater source within the southern Apennine chain. Copyright © 2009 John Wiley & Sons, Ltd. 相似文献
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84.
玲珑矿田含有两种类型金矿床,一是蚀变岩型金矿床,二是石英脉型金矿床。该文重点研究玲珑金矿田西山矿区石英脉型金矿床中流体包裹体的特征。石英脉型金矿床分布在玲珑帚状构造之中,含金石英脉受"帚状构造"的断裂和节理控制,有300余条。流体包裹体显微观察研究表明,玲珑石英脉型金矿新鲜花岗岩和钾化花岗岩主要含有H2O包裹体,其次有少量H2O-CO2包裹体;(黄铁)绢英岩通常含较粗粒石英集合体,石英中有丰富的H2O,特别是H2O-CO2包裹体;金矿体(含金石英脉)含有明显数量的H2O-CO2包裹体;特别是存在较大的三相H2O-CO2包裹体。不同期次(世代)石英中H2O和H2O-CO2包裹体的大小、形态、相对含量和丰度变化较大。 相似文献
85.
铜井式铜金矿(包括铜井铜金矿、金场铜金矿)是鲁西地区发现和开采最早、矿化最普遍的矽卡岩型铜金矿。该文通过矿床的He-Ar同位素测试分析,并结合前人的H,O,S,C稳定同位素分析和年代学测试结果,对铜井式铜金矿成因及成矿机制进行探讨。研究认为,铜井式金矿主要形成于燕山晚期(128~121Ma),黄铁矿中流体包裹体的~(3 )He/~(4 )He值为0.112 9~0.120 9R/Ra,高于地壳物质值,低于典型地幔物质值;~(40 )Ar/~(36 )Ar=364.1~458.0,高于大气值,低于地幔值,成矿流体中存在来源于地壳的放射成因Ar;~(4 )He/~(40 )Ar=1.16~3.433,平均2.296 5,略高于地幔值(1.36~2.23),低于典型地壳值(6.4),表明成矿流体中存在地幔He,Ar;同时有地壳He,Ar加入。综上认为,矿床成矿物质和流体具有深源特征,应来自地幔或下地壳,金成矿主要是与燕山晚期浅成—超浅成中酸性侵入岩有关,这些侵入体在侵位过程中与古生代碳酸盐岩地层发生接触交代作用,形成矽卡岩型铜金矿床。 相似文献
86.
Francisco González-Sánchez Antoni Camprubí Eduardo González-Partida Rafael Puente-Solís Carles Canet Elena Centeno-García Viorel Atudorei 《Mineralium Deposita》2009,44(3):343-361
Northeastern Mexico hosts numerous epigenetic stratabound carbonate-hosted low-temperature hydrothermal deposits of celestine, fluorite, barite and zinc-lead, which formed by replacement of Mesozoic evaporites or carbonate rocks. Such deposits can be permissively catalogued as Mississippi Valley-type (MVT) deposits. The deposits studied in the state of Coahuila are associated with granitic and metasedimentary basement highs (horsts) marginal or central to the Mesozoic Sabinas Basin. These horsts controlled the stratigraphy of the Mesozoic basins and subsequently influenced the Laramide structural pattern. The Sabinas Basin consists of ~6,000-m-thick Jurassic to Cretaceous siliciclastic, carbonate and evaporitic series. The MVT deposits are mostly in Barremian and in Aptian-Albian to Cenomanian formations and likely formed from basinal brines that were mobilized during the Laramide orogeny, although earlier diagenetic replacement of evaporite layers (barite and celestine deposits) and lining of paleokarstic cavities in reef carbonates (Zn–Pb deposits) is observed. Fluid inclusion microthermometry and isotopic studies suggest ore formation due to mixing of basinal brines and meteoric water. Homogenization temperatures of fluid inclusions range from 45°C to 210°C; salinities range from 0 to 26 wt.% NaCl equiv., and some inclusions contain hydrocarbons or bitumen. Sulfur isotope data suggest that most of the sulfur in barite and celestine is derived from Barremian to Cenomanian evaporites. Regional geology and a compilation of metallogenic features define the new MVT province of northeastern Mexico, which comprises most of the state of Coahuila and portions of the neighboring states of Nuevo León, Durango and, perhaps extends into Zacatecas and southern Texas. This province exhibits a regional metal zonation, with celestine deposits to the south, fluorite deposits to the north and barite and Zn–Pb deposits mostly in the central part. 相似文献
87.
本文根据雷公山背斜南段的几个锑矿床的勘查资料,结合1:5万区调和相应的科研成果,总结该区锑矿床的共同特征,并对其控矿条件进行分析,认为逆冲断层、剪切带控制锑矿田的分布,“褶皱 断层”控制锑矿床分布,单条剪切带及后期脆性断层控制锑矿体的产出。 相似文献
88.
The future exploration of Mars is likely to utilize resources that can be extracted in situ. An overview of the geology of Mars has been presented and several mechanisms that could result in the formation of ore deposits have been identified. These include deposits caused by hydrothermal fluids resulting from volcanic activity, large igneous province formation and impact craters. Surface enrichment of mineral sand deposits is also discussed. Where appropriate, terrestrial analogues of these mechanisms have been discussed and supporting evidence from observations of Mars undertaken to date presented. Types of deposits that are unlikely to be found on Mars are also listed. 相似文献
89.
90.
Computer thermodynamic modeling of the transport and deposition of Sb and Au during the formation of Au-Sb deposits 总被引:1,自引:0,他引:1
A.A. Obolensky L.V. Gushchina A.S. Borisenko A.A. Borovikov P.A. Nevolko 《Russian Geology and Geophysics》2009,50(11):950-965
Using the Chiller computer program, we performed modeling of the mechanisms of the joint transport and deposition of Au and Sb from various ore-forming solutions during the formation of Au-Sb deposits. Three models are considered by the example of the Uderei Au-Sb deposit in the Yenisei Ridge: (1) simple cooling (cooling only), (2) iso-enthalpy boiling (P = f(T)), and (3) solution–rock interaction (rock titration model). The behavior of Sb(III) and Au(I) in the system Au–Sb–Fe–Cu–Pb–Zn–As–H2O–Cl–H2S–CO2 under hydrothermal conditions was studied. It is shown that both weakly alkaline (near-neutral) and reduced acidic Feaq2+-enriched low-chloride high-CO2 and high-chloride hydrothermal solutions play a crucial role in the formation of gold parageneses of Au-Sb ores. 相似文献