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1.
Individual ores of 37 specimens and five mill concentrates were analyzed chemically, and anomalous indium contents were detected in the tin‐polymetallic veins of the Dajing mine. The indium contents are heterogenously distributed (0.5–296 ppm In), and are low generally in the ores of the East Block. Indium is mainly correlated with copper, partly with zinc in the Dajing deposits, implying that the element is substituted in copper and zinc sulfides and sulfosalts. The total indium content is expected as >768 tons, which is lower than a previous estimation of this mine. The whole tonnage of the southern part of the Da Hinggang Mountains is >1200 tons In, which is the second largest in China after the tin‐polymetallic deposits in the southern China.  相似文献   

2.
Tin‐polymetallic base metal deposits of Miocene age in the Eastern Cordillera in Bolivia were studied by ICP/MS and EPMA for major and minor elements, paying an attention to indium concentration of the ore deposits. The highest indium content and 1000 In/Zn ratio of individual ore deposits are 5,740 ppm and 22.2 for the Potosi deposits, 2,730 ppm and 7.4 for Bolivar deposit, 2,510 ppm and 17.5 for Siete Suyos–Animas deposits, and 1,290 ppm and 3.3 for San Vicente deposit. The same content and ratio of composite samples of the studied deposits are up to 292 ppm and 4.0 for Potosi deposits, 3,080 ppm and 11.3 for Huari Huari deposit, 100 ppm and 0.3 for Tuntoco deposit, 152 ppm and 1.8 for Porco deposit, 103 ppm and 59.2 for Animas deposit, and 1,160 ppm and 3.7 for Pirquitas deposit. Those of zinc concentrates are as follows: 1,080 ppm and 2.1 at San Lorenzo; 584 ppm and 1.7 at Bolivar; 499 ppm and 1.23 at Porco; 449 ppm and 1.21 at Reserva, and 213 ppm and 0.61 at Colquiri deposit. Indium occurs mostly in dark colored sphalerite and that of the Potosi deposit was found to have one of the highest concentrations, containing up to 1.27 wt% In. Petrukite was discovered in the Potosi deposit, and indium minerals are expected to occur in the Huari Huari deposit and others with the high 1000 In/Zn ratios. The indium contents of the zinc concentrates and composite samples were applied to the produced and remaining ores, then the total amounts of indium in the Bolivian tin‐polymetallic base metal deposits are speculated to be more than 12,000 tons In, which is bigger than that of South China (11,000 tons) and the Japanese Islands (9,000 tons). Sphalerites of the Potosi deposit have one of the highest ranges of indium, similarly to those of the San Vicente deposit. Both the San Vicente and Potosi deposits are rich in silver, implying significance of both silver‐polymetallic and tin‐polymetallic environments for the concentration of trace amounts of indium.  相似文献   

3.
The occurrence of fluorite deposits in Japan is limited in the provinces characterized by tin and tungsten mineralization within Southwest Japan. The deposits were formed near acidic igneous rocks of Cretaceous to Tertiary age. The ores in limestone are generally associated with skarn and metallic ore minerals such as cassiterite, scheelite and chalcopyrite. Granitic rocks in the provinces are the ilmenite-series (Ishihara, 1977) having enhanced fluorine contents and high initial strontium ratios. A reducing condition of the ilmenite-series granitic magma may have been more favorable for the concentration of fluorine in the residual magma because of the crystallization of relatively Fe-rich mafic minerals. Presence of thick crust bearing carbonaceous matter at the site of magmatism could have involved in the enrichment of fluorine as well as the reducing condition.  相似文献   

4.
火山-侵入杂岩带的成岩-成矿专属性   总被引：8，自引：0，他引：8  
岳书仓  徐晓春 《地学前缘》1999,6(2):305-313
成岩成矿关系问题,特别是成矿作用与岩浆活动的专属性问题,一直是矿床学研究中的重要课题。粤东地区热液脉状锡、钨（多金属）矿床产于中生代花岗质火山岩、次火山岩和侵入岩组成的火山侵入杂岩带中,成岩年龄与成矿年龄一致,但矿床地质、矿床矿物流体包裹体和同位素地球化学没有相对标准来区分这些来源于岩浆作用不同阶段、不同产出状态岩浆岩的成矿物质特征,使得人们对于区内矿床成因的认识不一。文中运用稀土元素地球化学方法,着重探讨和对比了矿床矿石、蚀变岩石及与成矿有关的岩浆岩的稀土元素特征和配分型式,并进一步根据在不同压力条件下Ｃｌ－在熔体和热液间的分配系数实验数据和不同压力条件下热液与相应熔体平衡时的稀土元素分配系数实验结果,分别计算了厚婆坳锡矿床和莲花山钨矿床与矿区有关岩浆岩熔体平衡的热液中的稀土元素浓度并制出配分型式,再与矿床矿石及矿石矿物稀土元素配分型式比较,从而确定成矿与侵入阶段的花岗岩岩浆活动关系密切。区内矿床为岩浆热液矿床。研究结果表明,稀土元素作为热液流体来源的示踪剂能有效地确定火山侵入杂岩带的成岩成矿专属性。  相似文献   

5.
陈程  赵太平 《矿床地质》2021,40(2):206-220
铟作为支撑新兴高科技产业发展的关键金属,主要应用于电子工业、半导体、焊料合金及航空航天等领域,对国家安全和经济发展至关重要.当前铟的重要来源是与花岗质岩浆有关的锡多金属矿床,其中铟的富集程度远超其他类型矿床.文章在简要概括铟矿床类型的基础上,探讨了铟在岩浆-热液系统各演化阶段的富集过程以及锡、铟同步富集的原因.在岩浆演化过程中,如果有黑云母、角闪石等铟的主要载体矿物发生分离结晶,铟的成矿潜力便会被大大削弱.当铟进入成矿流体后,铟的氯化物、氟化物和氢氧化物对铟的搬运有重要作用,流体的温度、pH值以及金属配体的种类和浓度是控制铟迁移和沉淀的重要因素.而当铟从流体中沉淀时,因四次配位的In3+与贱金属硫化物(闪锌矿、黄铜矿、黝铜矿等矿物)中四次配位的金属离子更相似,造成大量的铟以类质同象替换的方式进入硫化物而与锡发生分离;沉淀后的含铟矿物在后期地质过程中可能经历铟的重新活化、迁移和扩散等过程,导致铟再次富集.铟的富集过程与锡有关,这可能是由于铟和锡具有相似的地球化学性质,二者在表生环境中活动性弱,会滞留在经历化学风化的富黏土的沉积岩中,这样的沉积岩经变质作用会形成大量的云母类矿物,而黑云母作为铟和锡的共同载体,其在高温条件下发生分解可能是导致铟和锡在矿床中同步富集的根本原因.此外,新近在一些贫锡岩浆热液矿床中发现铟也能够超常富集,其机理尚不清楚.加强表生环境中锡与铟预富集过程的研究以及贫锡矿床中铟富集机制的研究,对查明铟-锡共生、分离机制和完善铟成矿理论至关重要.  相似文献   

6.
Abstract: Plutonic rocks of the Coastal Batholith of Peru were evaluated in terms of the granitoid-series classification using the bulk ferric/ferrous ratio from the literature and new measurements of magnetic susceptibility. The batholith is largely composed of magnetite-series plutonic rocks; the magnetite series make up 85% by number of chemical analyses (n=130) and 80% by measurement of magnetic susceptibility (n=210). The ilmenite-series rocks are mostly found in the felsic facies of the batholith. Asymmetrical distribution of magnetic susceptibility is not clear as in the Japanese Islands and Peninsular Range Batholith, but the magnetic susceptibility may decreases continentward (i. e., Peninsular Range type).
The Cordillera Blanca Batholith and stocks are also composed of mainly magnetite series plutonic rocks, but ilmenite-series rocks may be more predominant than in the Coastal Batholith, which is also indicated by the presence of Sn and W mineralizations.  相似文献   

7.
广西大厂锡矿铟的地球化学特征及成因机制初探   总被引：13，自引：3，他引：10  
广西大厂锡矿位于江南古陆西南缘,桂西北海西-印支期被动陆缘裂谷盆地北部的断裂凹陷盆地中,是中国重要的、以锡为主的有色金属矿床。它主要由长坡-铜坑和高峰矿床、拉么矿床、大福楼矿床和亢马矿床等组成,其铟资源量约6 000 t。文章在对长坡-铜坑矿床、高峰矿床以及拉么矿床不同类型围岩（包括花岗岩质岩石）、矿石以及不同矿床类型中矿石矿物（硫化物和氧化物）中的In、Cu、Cd、Sn、Fe、Zn等微量元素分析的基础上,结合不同类型矿床、不同矿物组合中硫化物的微量元素电子探针测试以及硫同位素分析结果,初步认为大厂锡矿岩浆源区是富铟的,在正常的沉积岩中不存在铟的初始富集;In主要赋存于闪锌矿中,与层状和块状的矿体关系密切。在成矿作用过程中,In的分布和富集对矿物组合和矿石类型具有明显的选择性。大厂铟矿的形成是富铟的岩浆源区重融产生含铟岩浆,在岩浆侵位冷却过程中,由岩浆结晶所产生的流体携带In、Cu、Fe、Zn、Sn等成矿元素从岩浆中出溶,形成含In的成矿流体。水-岩反应以及在大气降水来源流体的参与下,导致In、Cu、Fe、Zn、Sn等从成矿流体中沉淀、富集成矿。  相似文献   

8.
The Saishitang–Rilonggou Ore Field (SROF), which includes the Saishitang, Tongyugou, and Rilonggou ore deposits as well as other scattered occurrences, is located in the Elashan region in Qinghai Province, and is a significant Cu–Sn ore field in NW China. These ores are hosted in stratiform skarn deposits with the main metals being Cu and Sn, as well as Zn, Pb, Au, Ag, and trace elements (e.g. Ga, Ge, Se, and In). Bulk‐rock geochemical analyses of 50 ore samples from the three deposits show that In contents in the Saishitang deposit range from 0.03 to 39 ppm (average 12.7 ppm, n = 19), with 1000 In/Zn values that vary from >0.01 to 29.83 (average 4.29). Indium contents in the Tongyugou deposit vary from 7.51 to 131 ppm (average 28.37 ppm, n = 13), with 1000 In/Zn values from 0.74 to 48 (average 17.55). Finally, indium contents in the Rilonggou deposit vary from 0.73 to 120 ppm (average 36.15 ppm, n = 18), with 1000 In/Zn values from 0.33 to 47 (average 8.52). Indium is hosted mainly in sphalerite, while some other In‐bearing minerals (e.g., roquesite, stannoidite, and stannite) are present locally within the ore field. Roquesite, which replace or fill bornite, occurs in bornite‐rich ores in the Saishitang deposit. This is the first reported Chinese locality of roquesite. Based on previously reported Zn resources, a total of 136 tons of In is calculated to be hosted in the SROF, with 30, 66, and 40 tons of In attributed to the Saishitang, Tongyugou, and Rilonggou deposits, respectively. The differences in indium contents among the deposits and their respective geological histories and characteristics suggest that the origin of indium relates to volcanogenic metallogenesis in an early Permian volcano‐sedimentary basin. Based on the evaluation of In resources, future mining operations should include the recovery of indium in the Tongyugou and Rilonggou deposits.  相似文献   

9.
Iron, tin, tungsten, copper, and polymetallic deposits are examined and the paper investigates the mineral distribution of indium in mineral deposits in central Kazakhstan. Indium is a relatively rare element; of the 18 formations examined only five revealed high concentrations of indium. Economic accumulations were discovered only in Early and Late Variscan skarnitic formations with lead-zinc, copper, and bismuth mineralizations. Among the hypogene minerals, indium was found in sulfides, and silicates. Among supergene minerals indium was found only in oxides, carbonates, and silicates. Sphalerites are the principal collector of indium. No connection between the enrichment in indium and the typomorphic peculiarities of different varieties of sphalerites could be established. In mineral deposits with higher indium concentration, a paragenetic connection of this element with tin is noticeable. Regular enrichment of sphalerites in indium would admit as most probable an isomorphous replacement of zinc and bivalent iron by indium. — A.W. Bellais  相似文献   

10.
Research on hydrogeochemistry for mineral exploration for inland Australia includes development of weathering models and extensive mine-scale and regional groundwater data. Mineral saturation indices for groundwater, activity–activity plots and reaction modelling simulate weathering of volcanic-hosted massive sulfide (VHMS) deposits in deeply weathered environments. At 10 m or more below surface, dissolved O2 is very low and other solutes such as sulfate, carbonate and nitrate are more likely oxidants. Modelling indicates that these processes differ from oxic weathering of highly eroded terrains, and provide the framework to develop robust hydrogeochemical exploration procedures in covered terrains. Sulfide weathering potentially occurs in two or more phases that effect surrounding groundwaters in differing manners. Deeper oxidative alteration of sulfides (e.g. bornite to chalcopyrite), occurring tens to hundreds of metres below surface, uses sulfate and carbonate as oxidants, causing neutral to alkaline conditions. In this zone, only pyritic massive sulfides potentially generate acidic conditions. Thus, deep sulfide-rich rocks are indicated by sulfate-depleted groundwater. Closer to the surface, sulfides are oxidised to soluble sulfates by dissolved nitrate, with much less acid production than if dissolved oxygen was the main oxidant. Thus, in shallow groundwater, sulfides are indicated by sulfate enrichment and nitrate depletion. Elements are released from sulfides and wall rocks by acid or alkaline conditions. The derived FeS (pH–Eh + Fe + Mn) and AcidS (Li + Mo + Ba + Al) indices distinguish sulfide systems through tens of metres of cover. VHMS systems are distinguished from other non-economic sulfide deposits where there is little transported cover, using various dissolved elements, including Zn, Pb and Cu. Elsewhere, ‘patchiness’ and limited aerial extent of metal signals are due to adsorption effects, that intensify with depth. Other elements such as Mn and Co have lesser diminution effects, but are less selective indicators for VHMS. There is exploration potential for elements such as Pt or Ag. These varying sulfide indicators have moderate utility, even for large-scale (～5 km spacing) sampling. Results indicate that hydrogeochemistry can add value to greenfields exploration for VHMS ore deposits in deeply weathered terrains. It is also moderately successful at indicating the presence of sulfide-rich systems (whether magmatic or hydrothermal) under >100 m cover, thus providing a rapid and cost-effective regional prospectivity tool for deeply buried terrains. Such mineral exploration tools will encourage exploration investment for more difficult regions of Australia and in other deeply weathered regions of the world.  相似文献   

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