Cobalt‐Bearing Grunerite in the Metamorphosed Banded Iron Formation in Orissa,India

Banded iron formation (BIF) comprising high grade iron ore are exposed in Gorumahisani‐Sulaipat‐Badampahar belt in the east of North Orissa Craton, India. The ores are multiply deformed and metamorphosed to amphibolite facies. The mineral assemblage in the BIF comprises grunerite, magnetite/martite/goethite and quartz. Relict carbonate phases are sometimes noticed within thick iron mesobands. Grunerite crystals exhibit needles to fibrous lamellae and platy form or often sheaf‐like aggregates in linear and radial arrangement. Accicular grunerite also occur within intergranular space of magnetite/martite. Grunerite needles/accicules show higher reflectivity in chert mesoband and matching reflectance with that of adjacent magnetite/martite in iron mesoband. Some grunerite lamellae sinter into micron size magnetite platelets. This grunerite has high ferrous oxide and cobalt oxide content but is low in Mg‐ and Mn‐oxide compared to the ones, reported from BIFs, of Western Australia, Nigeria, France, USA and Quebec. The protolith of this BIF is considered to be carbonate containing sediments, with high concentrations of Fe and Si but lower contents of cobalt and chromium ± Mg, Mn and Ni. During submarine weathering quartz, sheet silicate (greenalite) and Fe‐Co‐Cr (Mg‐Mn‐Ni)‐carbonate solid solution were formed. At the outset of the regional metamorphic episode grunerite, euhedral magnetite and recrystalized quartz were developed. Magnetite was grown at the expense of carbonate and later martitized under post‐metamorphic conditions. With the increasing grade of metamorphism greenalite transformed to grunerite.     

Genetic modelling for banded iron-formation of the Hamersley Group, Pilbara Craton, Western Australia

The banded iron-formation (BIF) of the Hamersley Group, Pilbara Craton, Western Australia, particularly from the well studied Dales Gorge Member, is unique in its lateral stratigraphic and petrological continuity throughout an area exceeding 60,000 km², enabling reasonable estimates for the annual input of components to the depository. In the model of this paper, varying supply of materials for the medley of mesoband types, particularly of iron and silica in the oxide BIF, can be accommodated by the interaction of two major oceanic supply systems: (1) surface currents and (2) convective upwelling from mid-oceanic ridge (MOR) or hot-spot activity, both modified by varied input of pyrochastic material. (1) The surface currents were saturated in silica and carried minimal iron due to photic precipitation, but were periodically recharged by storm mixing. Precipitation from them gave rise to the banded chert-rich horizons, including the varves, whose regular and finely laminated iron/silica distribution resulted from seasonal meteorological influences. (2) Precipitation from convection driven upwelling of high iron solution from MOR or hot-spot activity periodically overwhelmed the delicate seasonal patterns of (1) to produce the iron-dominated mesobands. A wide range of intermediate mesoband types resulted where the deep water supply was modified by varied MOR activity, or by partial blocking of upwelling waters by surface currents (such as by the present El Niño). During these periods of oxide-dominated BIF, silica was deposited from saturated solution mainly by evaporative concentration, and iron by oxidation due to photolysis and photosynthetically produced oxygen.Superimposed on these supply differences was the varying effect of fine aluminous ash from dominantly northern distal volcanic sources, changing the meteorological and depositional conditions. Occasional input of extremely fi ash during BIF precipitation produced mesoband (cm) scale variations involving increased carbonate-silicate precipitation. Sustained volcanic periods resulted in S-macroband deposition (chert-carbonate-silicate BIF, with shale), gradually returning to the dominant hematite-magnetite-chert BIF as the volcanic input waned. During volcanic periods, the normally high capacity of sunlight to precipitate ferric iron directly by photolytic oxidation of ferrous iron, and by photosynthetic production of oxygen, was modified by turbidity in the atmosphere (aerosols and dust) and in the water (colloids from reactive ash). S Surface-precipitated ferric hydroxyoxide redissolved in the presence of decaying organic matter in the subphotic zone, augmenting the iron content of the zone. Precursor ferrous carbonates and silicates were precipitated when the iron concentration of this sub-photic zone exceeded their respective solubilities. During volcanism, the increased availability of nutrients, particularly phosphorus, to surface waters increased the organic contribution despite lower light values, leading to an almost total absence of ferric iron oxides in the S macrobands (i.e. no magnetite or hematite). Cooling of warm, silica-saturated sea-water during these periods of “olcanic winter” increased the ratio of precipitation of silica to iron, which, however, was still controlled by seasonal conditions. Intermediate concentrations of organic matter, insufficient to totally convert the ferric compounds either during precipitation or diagenesis, resulted in overgrowths of magnetite on hematite, and eventually in the substantial conversion of hematite to magnetite, where higher temperatures were achieved during low-grade regional metamorphism.Changes in sea-level to explain facies changes in BIF are not required in this model, but are not excluded. The preferred conditions are for a very low oxygen to anoxic atmosphere, a much higher level of MOR activity than at present, the presence of photosynthetic plankton, the absence of si silica-secreting organisms, and a deep sea-water temperature higher than 20°C. However, none of these conditions is essential to the model.A narrow carbonate bank is postulated for part of the Fortescue River Valley area during Marra Mamba Iron Formation times (basal Hamersley Group), with BIF precipitation on either side. The reef is postulated to have grown northward becoming a major shallow-water carbonate platform on the Pilbara continent during upper Marra Mamba Iron Formation and Wittenoom Dolomite times, but ceased to play an important role in subsequent periods.     

西澳大利亚州铁矿分布规律及矿床成因分析

西澳大利亚州铁矿资源主要分布在北部皮尔巴拉和南部的伊尔岗两个太古宙克拉通。皮尔巴拉克拉通BIF型铁矿在汤姆普赖斯山、恰那和布鲁克曼的矿石矿物组合为假象赤铁矿一微板状赤铁矿,马拉曼巴的为赤铁矿一针铁矿,CID型铁矿在罗布河和杨迪矿石类型主要为褐铁矿;伊尔岗克拉通BIF型铁矿在库里阿诺的矿石矿物组合为针铁矿一假象赤铁,比温和曼迪尕的为磁铁矿±假象赤铁矿和针铁矿±赤铁矿。BIF型铁矿为浅生一变质成矿,而CID型铁矿则是先前形成的BIF经侵蚀、搬运、沉积和埋藏作用形成。     

便携式X射线荧光元素分析仪的应用

利用NITON XL3t 500型便携式X射线荧光光谱仪,选择云南会泽县金牛厂铅锌矿区进行样品分析条件试验.试验中分别对实验室分析与X射线荧光光谱仪分析结果,以及不同湿度条件下分析结果进行了对比研究,确定了最佳的应用条件.结果表明,实验室分析与X射线荧光光谱仪分析结果相近,但湿度因素会降低元素含量.所以应用便携式X荧光光谱仪进行试验不失为一种方便快捷和行之有效的方法.     

非洲锰矿床成因类型、地质特征及表生富集作用

[研究目的]非洲锰矿资源丰富,储量3.1亿t、资源量6.6亿t排名在世界上均列第一,加强非洲锰矿床的研究和认识对推动锰矿找矿工作具有重要的指导意义.[研究方法]通过对重要成矿带典型矿床的解剖总结了非洲锰矿床的成因类型、地质特征.[研究结果]非洲锰矿成因类型主要有前寒武系条带状铁建造(BIF)型、海相沉积型、陆相(三角洲...     

电感耦合等离子体法测定灰岩中的钙镁钾钠铝钛铁锰

灰岩样品的主要成分为碳酸钙,而镁、钾、钠、铝、钛、铁、锰的含量非常低,测试的灵敏度要求很高。该文采用一次溶矿电感耦合等离子体法直接测试灰岩中的镁、钾、钠、铝、钛、铁、锰。实验表明：在5％的盐酸介质中测试镁、钾、钠、铝、钛、铁、锰能取得很好的效果。通过测试国家标准样品,与国家标准值相比较,分析结果基本一致,准确度和精密度均令人满意,镁、钾、钠、铝、钛、铁、锰元素的相对标准偏差≤0．07％。钙元素的标准偏差≤0．15％。     

无机多元素现代仪器分析技术

本文重点介绍地质领域目前广泛应用的无机多元素现代仪器分析技术,包括电感耦合等离子体原子发射光谱(ICP-AES)、电感耦合等离子体质谱(ICP-MS)、X射线荧光光谱(XRF)、原子吸收光谱(AAS)、原子荧光光谱(AFS)、电子探针分析技术和共享平台的建立、激光剥蚀等离子体质谱(LA-ICP-MS)微区原位分析技术以...     

苏丹东部地区BIF型铁矿和CID型铁矿的发现及其找矿意义

在苏丹东部地区新元古代地层中,新发现的BIF铁矿是与火山岩密切相关的Algoma型铁矿,矿石品位TFe 37.78%,对进一步研究努比亚地盾的形成时代和古地理环境有一定的参考意义。苏丹79区块发现的含铁石英砂岩,呈北东向带状分布, 角度不整合于努比亚地盾之上,通过与西澳CID型铁矿对比,存在交错层理和底砾岩等明显的再生沉积特征,矿石品位TFe 31.91%～39.33%;通过对BIF型铁矿、CID型铁矿和努比亚杂砂岩三者部分元素及氧化物含量的分析对比,以及控矿地质因素分析, CID型铁矿是由BIF铁矿风化剥蚀后搬运沉积于附近古河道内;苏丹努比亚地盾区CID型铁矿的发现,为今后找矿工作提供了新目标,具有十分重要的找矿意义。     

X射线荧光光谱-X射线衍射-红外光谱联用技术鉴别锰矿与锰冶炼渣

鉴别锰矿与锰冶炼渣对于锰矿进口贸易和环境保护具有重要意义,由于锰冶炼渣与一些锰矿具有相似的元素组成,都含有锰和硅铝镁钙等杂质元素,仅从元素含量的高低无法准确将其鉴别。本文按国别收集我国主要进口锰矿及不同工艺的主要锰冶炼渣作为研究样品,应用X射线荧光光谱、X射线衍射及傅里叶变换红外光谱技术相结合,建立了锰矿与锰冶炼渣的鉴别方法。在元素组成上,锰冶炼渣的硅含量较高,水淬渣和空气冷却渣的钙含量较高。在物相上,锰矿的特征物相包括软锰矿、氧化锰、方锰矿、菱锰矿等;而锰冶炼渣因为经过冶炼的过程存在硅酸铁、锰橄榄石等特征峰,从而对样品属性进行鉴别。红外光谱显示,锰矿在600~400 cm~(-1)范围内有两个强吸收带,并单独或者同时在1420 cm~(-1)处有特征吸收峰;而锰冶炼渣在960 cm~(-1)左右有宽强吸收峰。本法建立了锰矿的物相谱图库及锰冶炼渣的物相特征,并充分利用红外光谱技术作了有力佐证,确定了锰矿及其冶炼渣的主要区别点。     

Genesis of superimposed hypogene and supergene Fe orebodies in BIF at the Madoonga deposit, Yilgarn Craton, Western Australia

The Madoonga iron ore body hosted by banded iron formation (BIF) in the Weld Range greenstone belt of Western Australia is a blend of four genetically and compositionally distinct types of high-grade (>55 wt% Fe) iron ore that includes: (1) hypogene magnetite–talc veins, (2) hypogene specular hematite–quartz veins, (3) supergene goethite–hematite, and (4) supergene-modified, goethite–hematite-rich detrital ores. The spatial coincidence of these different ore types is a major factor controlling the overall size of the Madoonga ore body, but results in a compositionally heterogeneous ore deposit. Hypogene magnetite–talc veins that are up to 3 m thick and 50 m long formed within mylonite and shear zones located along the limbs of isoclinal, recumbent F₁ folds. Relative to least-altered BIF, the magnetite–talc veins are enriched in Fe₂O_3(total), P₂O₅, MgO, Sc, Ga, Al₂O₃, Cl, and Zr; and depleted in SiO₂ and MnO₂. Mafic igneous countryrocks located within 10 m of the northern contact of the mineralised BIF display the replacement of primary igneous amphibole and plagioclase, and metamorphic chlorite by hypogene ferroan chlorite, talc, and magnetite. Later-forming, hypogene specular hematite–quartz veins and their associated alteration halos partly replace magnetite–talc veins in BIF and formed during, to shortly after, the F₂-folding and tilting of the Weld Range tectono-stratigraphy. Supergene goethite–hematite ore zones that are up to 150 m wide, 400 m long, and extend to depths of 300 m replace least-altered BIF and existing hypogene alteration zones. The supergene ore zones formed as a result of the circulation of surface oxidised fluids through late NNW- to NNE-trending, subvertical brittle faults. Flat-lying, supergene goethite–hematite-altered, detrital sediments are concentrated in a paleo-topographic depression along the southern side of the main ENE-trending ridge at Madoonga. Iron ore deposits of the Weld Range greenstone belt record remarkably similar deformation histories, overprinting hypogene alteration events, and high-grade Fe ore types to other Fe ore deposits in the wider Yilgarn Craton (e.g. Koolyanobbing and Windarling deposits) despite these Fe camps being presently located more than 400 km apart and in different tectono-stratigraphic domains. Rather than the existence of a synchronous, Yilgarn-wide, Fe mineralisation event affecting BIF throughout the Yilgarn, it is more likely that these geographically isolated Fe ore districts experienced similar tectonic histories, whereby hypogene fluids were sourced from commonly available fluid reservoirs (e.g. metamorphic, magmatic, or both) and channelled along evolving structures during progressive deformation, resulting in several generations of Fe ore.     

Oxygen Isotope Study of Paleoproterozoic Banded Iron Formation, Hamersley Basin, Western Australia

A submillimeter‐scale variation of δ¹⁸O in quartz was identified in chert and Fe‐oxide mesobands of the Brockman Iron Formation, Western Australia, using an in situ CO₂‐laser fluorination technique. The total range of variation is 11.2–23.0‰, with >5‰ variations within a single mesoband of approximately 2 cm thickness. These data contradict most previous works, which have suggested that banded iron formations are isotopically homogeneous. The present sample was obtained outside of the iron mining area, and as such is considered to have been less altered by the hydrothermal event recently shown to be responsible for the formation of the iron ore. The data suggest that the largest Paleoproterozoic banded iron formations may have formed not in a stable, quiescent sea, but instead as a result of increased influx of iron‐ and silica‐rich solutions during periods of increased magmatism and submarine hydrothermal activity in a rift basin environment.     

冀东柞栏杖子BIF地球化学特征、形成时代及其地质意义

冀东地区柞栏杖子BIF出露于绿片岩相—低角闪岩相朱杖子岩群变质岩中。铁矿石主要由石英和磁铁矿组成,还含有少量透闪石和黑云母。主量元素主要为Si O2、Fe2O3和Fe O,其次为少量的Ca O和Mg O。较低的Al2O3含量、极低的Ti O2含量和高场强元素(HFSE)暗示,铁矿石中陆源碎屑物质含量很低。铁矿石的稀土元素含量较低,稀土元素配分模式特征为轻稀土元素相对亏损、重稀土元素相对富集。较明显的Eu正异常、轻微的Y正异常及较高的Y/Ho值的稀土元素特征,类似于高温热液和海水的混合热液,暗示成矿物质主要来自于海水和高温热液。对柞栏杖子BIF矿体夹层黑云斜长变粒岩进行SHRIMP锆石U-Pb定年,207Pb/206Pb年龄加权平均值为2572±8Ma(MSWD=5.8),可代表柞栏杖子BIF的形成年龄。综合前人研究,认为冀东地区变质级别不同的BIF物质来源相同、形成年代相近,BIF的变质可能和2500Ma左右华北克拉通东部陆块发生的地幔岩浆底侵事件有关。     

Genesis history of iron ore from Mesoarchean BIF at the Wodgina mine,Western Australia

Several iron-ore deposits hosted within Mesoarchean banded iron formations (BIFs) are mined throughout the North Pilbara Craton, Western Australia. Among these, significant goethite±martite deposits (total resources >50 Mt at 55.8 wt% Fe) are distributed in the Wodgina district within 2 km of the world-class pegmatite-hosted, tantalum Wodgina deposits. In this study, we investigate the dominant controls on iron mineralisation at Wodgina and test the potential role of felsic magma-derived fluids in early alteration and upgrade of nearby BIF units. Camp-scale distribution and geochemistry of iron ore at Wodgina argue against any significant influence of identified felsic intrusions in the upgrade of BIF. Whereas, the formation of BIF-hosted goethite±martite iron ore at Wodgina involves: (i) early (ca 2950 Ma) metamorphism of BIF causing camp-scale recrystallisation of pre-existing iron oxides to form euhedral magnetite, with local enrichment to sub-economic grades (～40 wt% Fe) within or proximal to metre-wide, bedding-parallel shear zones, and (ii) later supergene lateritic enrichment of the magnetite-bearing BIF and shear zones, forming near-surface goethite±martite ore. The supergene alteration sequence includes: (i) downward progression of the oxidation front and replacement of magnetite by martite, (ii) local development of silcrete at ～40 m below the modern surface caused by the lowering of the water-table, (iii) intensive replacement of quartz by goethite, resulting in the goethite±martite ore bodies at Wodgina, and (iv) late formation of ferricrete and ochreous goethite. Goethitisation most likely took place within the hot and very wet climate that prevailed from the Paleocene to the mid-Eocene. Goethite precipitation was accompanied by the incorporation of trace elements P, Zn, As, Ni and Co, which were likely derived from supergene fluid interaction with nearby shales. Enrichment of these elements in goethite-rich ore indicates that they are potentially useful pathfinder elements for concealed ore bodies covered by trace element-depleted pedogenic silcrete and siliciclastic rocks located throughout the Wodgina mine.     

Neutron Activation Analysis, Atomic Absorption and X-Ray Fluorescence Spectrometry Review for 2003

This review for the year 2003 deals with three relatively well-established, mature, analytical techniques (neutron activation analysis, atomic absorption spectrometry and X-ray fluorescence spectrometry) that nevertheless remain very important for the characterisation of geological and environmental samples. Developments in neutron activation analysis included modification to the technique in relation to the determination of platinum-group elements, as well as consideration of sample size in ore grade estimation. A considerable body of literature was published on the application of atomic absorption spectrometry in the analysis of environmental samples. Many of these proposed technical and methodological improvements, notably in extraction procedures. X-ray fluorescence spectrometry saw developments in in situ analysis, synchrotron micro-XRF (μ-SRXRF) and a confocal X-ray set-up for 3D elemental imaging. XRF technologies were used in the analysis of geological samples, reference materials, glasses, solutes and environmental materials.     

Major element distribution in Archean banded iron formation (BIF): influence of metamorphic differentiation

The Archean (2.8 Ga) Banded Iron Formation (BIF) of the Bell Lake region of Yellowknife greenstone belt, Canada is recrystallized to metamorphic assemblages of the amphibolite facies. This BIF is characterized by centimetre‐scale Fe‐rich and Si‐rich mesobands. In the Si‐rich mesobands, thin layers of magnetite microbands are developed in a quartz matrix. The Fe‐rich mesobands are composed mainly of Ca‐amphibole (hornblende), Fe–Mg amphibole (grunerite), and magnetite. The metamorphic foliation locally cuts across the mesoband boundaries, indicating the mesobanding was formed prior to peak metamorphism. Variations in mineral modal proportions between Fe‐rich mesobands and microbands are diagnostic of depositional compositional differences between beds. Micro‐X‐ray fluorescence imaging reveals metamorphic differentiation within Fe‐rich mesobands, with segregation of Fe–Mg amphibole, and the incompatible element Mn is concentrated at the margins of the Fe‐rich mesobands during the amphibole‐forming reactions. Ti was relatively immobile during metamorphic segregation and its distribution provides a record of the original structures in the Fe‐rich mesobands.     

Chemical Characterisation of Geological Raw Materials Used in Traditional Ceramics

A wide range of natural raw materials is used in the manufacture of traditional ceramic products such as ceramic tiles, frits, glazes and pigments. The chemical composition of these raw materials needs to be strictly controlled to assure end-product quality and enable the identification of the origin of defects caused by impurities or contamination. Six types of ceramic raw materials (silica sand, clays and kaolin, feldspars and related minerals, calcium and magnesium carbonates, sodium and calcium borates, and zirconium silicates) have been analysed in this study. X-ray fluorescence (XRF), potentiometry, coulometry and atomic absorption spectrometry (AAS) were used in this chemical characterisation. A methodology has been established for characterising each studied raw material, by identifying the chemical elements to be determined, selecting the most appropriate technique and validating each measurement. The reference materials used for validation were BCS CRM 267, 313/1, 393 and 388 (BAS), GBW 03103, GBW 07404, NIST SRM 181, 201a and 1835, Euronorm CRM 782-1 and Syenite SY-2. The results showed that most of the elements present in the geological samples used as traditional ceramic raw materials could be determined by XRF. The determination of light elements, such as lithium, fluorine and boron, is more suitably conducted by ICP-AES/AAS, potentiometry or potentiometry/ICP-AES respectively. Organic and inorganic carbon could be determined by coulometry. Inorganic carbon (CO₂) could also be determined by coulometry or by thermogravimetry, if samples did not contain clay minerals. Loss on ignition was always determined by gravimetry.     

GGR Biennial Review: Atomic Absorption,Inductively Coupled Plasma-Atomic Emission Spectrometry,Neutron Activation Analysis and X-Ray Fluorescence Spectrometry Review for 2008–2009

This review describes developments major and in trace element determination using atomic absorption spectroscopy (AAS), inductively coupled plasma-atomic emission spectrometry (ICP-AES), instrumental neutron activation analysis (INAA), and X-ray fluorescence (XRF) spectrometry that were reported in 2008 and 2009. Publication levels were comparable to those of previous years, except for XRF which showed an increase in the number of articles published in the past 2 years. In terms of number of publications and impact, the most active field was AAS, while INAA was the least active. As expected for well-established and mature methods, novel developments for all four analytical techniques were relatively sparse. For AAS, the most notable publications concerned developments in sample introduction, particularly focussing on solid samples, increasing analyte sensitivity, and higher sample throughput. For ICP-AES, publication of developments in sample introduction, remediation of matrix effects and calibration continues. Compared with past years, there was a clear focus on sample preconcentration methods, but very few publications reporting new hyphenated speciation methods. For INAA, there were several publications exploring the accuracy and robustness of the method, as well as the requirements for INAA to meet criteria for a primary method of measurement. Two other related techniques, delayed neutron activation analysis, and prompt gamma activation analysis, were also described. Hyphenated XRF techniques showed interesting developments in enabling XRF and XRD analysis on the same spot, and further work characterising and calibrating three-dimensional micro-XRF shows promising results for investigating sample heterogeneity.     

X荧光分析仪在新疆某地的应用

介绍新一代X射线荧光分析仪在新疆某地的勘查应用,并采用几种方法对基体效应、湿度效应、不平度效应进行效正。该仪器可同时显示20余种元素的含量,测试结果证明,X荧光技术是一种快速、经济、有效的方法。     

X射线荧光光谱法测定土壤和沉积物中的锰

X射线荧光光谱法(XRF)是测定土壤和沉积物中锰的重要方法,具有制样简单、非破坏性测定、检测速度快等优点。目前用于建立工作曲线的土壤和沉积物标准物质的锰含量最高为2490mg/kg,采用XRF法测定受污染土壤和沉积物中的锰含量时易超出工作曲线测定范围。本文将锰标准溶液定量加入到土壤标准物质中,制备锰含量更高的校准样品,工作曲线的测定上限范围由2490mg/kg提高至3780mg/kg。该方法测定不同含量标准物质中锰含量的结果均在认定值范围内,实际样品的加标回收率为97.8%～108.3%,高含量锰的实际样品测定值与电感耦合等离子体发射光谱法测定值的相对偏差小于5.7%,相对标准偏差(RSD)小于0.4%(n=7)。实验结果表明该法测定锰含量高的土壤和沉积物的准确度和精密度良好。