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1.
白云鄂博的钾-钡长石系列与钡交代作用   总被引:3,自引:0,他引:3       下载免费PDF全文
在内蒙古白云鄂博铌-稀土-铁矿床的顶板围岩——钾交代岩中发现大量含钡的钾微斜长石,其钡长石(Cn)分子含量变化于5.5~13.8mol%Cn之间,构成钾钡长石系列矿物.Cn含量高者则形成钡冰长石并与含Cn较低的钾微斜长石构成环带构造.本文根据钾钡长石系列矿物的显微构造、化学成分及其矿物组合特点确定了在本区普遍发育的另一种热液变代作用——钡交代作用.  相似文献   

2.
钡长石(BaO·Al2O3·2SiO2)的熔点1770℃,热膨胀系数较低,因此具有良好的耐急冷急热性。以单斜钡长石为基材的陶瓷其应用前景广阔。钡长石在自然界分布极少,工业上用量大,就要进行人工合成。国外合成钡长石一般用碳酸钡(或硫酸钡)和经过洗涤的高岭土为原料。我们利用贵州高岭土和重晶石为原料由固相反应进行人工合成钡长石的试验研究。1 原料分析我们对贵州省内不同类型、不同地区高岭土和重晶石的试样进行了化学、差热、热重、X射线衍射等分析研究,从而弄清了原料的化学成分、矿物组成和结晶程度等[1]。从…  相似文献   

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X射线荧光分析技术在毒重石-钡解石-钡白云石型钡矿的勘查和评价中能有效地圈定矿体,划分富,中,贫矿石和非矿石的回归预测方程为BaO=0.5614-3.127×10^-5It,划分矿与非矿的荧光强度值界限为It=24350,贫矿与中等矿的边界限为It=29.467,中等矿与富矿的边界为It=33000,岩石中测量的X射线荧光强度值曲线变化幅度小,形态平缓稳定,可以用X射线荧光分析法测制地质-地球化学  相似文献   

5.
四川庙子毒重石-钡解石-钡白云石型钡矿床的成因   总被引:10,自引:1,他引:9  
庙子钡矿床是属于海底喷流热水沉积型毒重石 -钡解石 -钡白云石矿床。典型的海底喷流岩组合为毒重石岩 硅岩 硅质板岩 碳质板岩 灰岩 ,典型的海底喷流岩构造有角砾状、网脉状、气孔状、块状、层纹状、条带状等。钡矿石的主要组分为毒重石、钡解石、钡白云石。矿石的形成还与成岩早期有机质、细菌活动有着密切的关系。含矿岩系的岩石化学、微量元素、稀土元素地球化学特征表明硅岩、毒重石岩是在低能、缺氧、强还原条件下海底喷流热水沉积形成。钡矿形成环境为早寒武世麦地坪期扬子地台北部的陆棚边缘滞留盆地  相似文献   

6.
南秦岭大型钡成矿带,钡矿物种类丰富。通过对南秦岭钡成矿带钡矿床中矿石和矿化围岩的电子探针研究,结合前人研究成果,发现南秦岭大型钡成矿带中钡主要以重晶石、毒重石、钡解石、菱钡镁石、钡长石、汉江石、安康矿、钡冰长石、钒云母等形式存在;硫化物以黄铁矿为主,并含有少量的针镍矿、闪锌矿、硫钒铜矿、蓝辉铜矿、斑铜矿。此外,还发现少量钒钛氧化物。在研究钡矿物化学组成的基础上,对毒重石、钡解石、菱钡镁石、钡长石、钡冰长石等钡矿物的成因进行了探讨。  相似文献   

7.
韩善楚  胡凯  曹剑 《地质论评》2013,59(6):1143-1149
华南早寒武世黑色岩系重晶石矿床是全球著名的沉积型层状矿床。本文报道了我们最近的一项新发现,在该区天柱大河边重晶石矿床中首次发现了环带钡冰长石,环带的外带BaO含量1653%~1786%,K2O含量777%~819%,相比而言,核部BaO含量1204%~1421%,K2O含量860%~979%。结合成矿地质背景和已有工作报道,讨论了这一新发现的地质意义。认为这种环带钡冰长石的出现,反映了重晶石成矿受到热水作用影响,且其形成过程中经历了不同期富钡流体的影响,成矿可能属于一种热水、断控、幕式、渐进的过程,这不仅进一步揭示了矿床的热水(液)喷流沉积成因,而且加深了对成矿过程的刻画。该认识还可供全球沉积型重晶石矿床成因研究时类比参考。  相似文献   

8.
张珩  卜国光 《地质实验室》1995,11(6):343-346
以碳粉、氯化钠为缓冲剂消除基体的影响,选择钐作为内标元素,本法简单快速、Br和Sr的相对标准偏差分别为5.4%和5.1%,已成功地应用于化探样品中钡和锶的定量测定。  相似文献   

9.
矾山杂岩体多元长石的成分、结构及其研究意义   总被引:1,自引:0,他引:1  
华北早中生代矾山钾质碱性超镁铁岩-正长岩杂岩体由3个岩相带组成,本文在不同相带矿物学系统研究的基础上,重点对该区不同期次钾长石的组分和结构进行了详细的研究,其结果反映杂岩体总的具有富钾的特点,但各岩相带长石成分的差异则显示出不同期次岩浆成分上的不同。通过对长石的微量元素的进一步研究,本文首次确认了矾山地区钡冰长石和锶钡冰长石的存在。通过对不同阶段长石锶钡含量的比较研究,揭示了本区存在多次富钡流体的交代作用。该项研究对揭示本区岩石成因及其岩浆演化具有重要意义。岩浆晚期锶、钡元素的明显提高暗示:该区早中生代作为岩浆源区的岩石圈地幔有不断富集的趋势。  相似文献   

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11.
Multiphase solid inclusions in minerals formed at ultra-high-pressure (UHP) provide evidence for the presence of fluids during deep subduction. This study focuses on barian mica, which is a common phase in multiphase solid inclusions enclosed in garnet from mantle-derived UHP garnet peridotites in the Saxothuringian basement of the northern Bohemian Massif. The documented compositional variability and substitution trends provide constraints on crystallization medium of the barian mica and allow making inferences on its source. Barian mica in the multiphase solid inclusions belongs to trioctahedral micas and represents a solid solution of phlogopite KMg3(Si3Al)O10(OH)2, kinoshitalite BaMg3(Al2Si2)O10(OH)2 and ferrokinoshitalite BaFe3(Al2Si2)O10(OH)2. In addition to Ba (0.24–0.67 apfu), mica is significantly enriched in Mg (XMg ~ 0.85 to 0.95), Cr (0.03–0.43 apfu) and Cl (0.04–0.34 apfu). The substitution vector involving Ba in the I-site which describes the observed chemical variability can be expressed as BaFeIVAlClK?1Mg?1Si?1(OH)?1. A minor amount of Cr and VIAl enters octahedral sites following a substitution vector VI(Cr,Al)2VI(Mg,Fe)?3 towards chromphyllite and muscovite. As demonstrated by variable Ba and Cl contents positively correlating with Fe, barian mica composition is partly controlled by its crystal structure. Textural evidence shows that barian mica, together with other minerals in multiphase solid inclusions, crystallized from fluids trapped during garnet growth. The unusual chemical composition of mica reflects the mixing of two distinct sources: (1) an internal source, i.e. the host peridotite and its garnet, providing Mg, Fe, Al, Cr, and (2) an external source, represented by crustal-derived subduction-zone fluids supplying Ba, K and Cl. At UHP–UHT conditions recorded by the associated diamond-bearing metasediments (c. 1100 °C and 4.5 GPa) located above the second critical point in the pelitic system, the produced subduction-zone fluids transporting the elements into the overlying mantle wedge had a solute-rich composition with properties of a hydrous melt. The occurrence of barian mica with a specific chemistry in barium-poor mantle rocks demonstrates the importance of its thorough chemical characterization.  相似文献   

12.
Whole-rock compositions of muscovite-bearing amphibolite, trondhjemite, pegmatite and quartz-muscovite rocks from Sierra del Convento and La Corea mélanges (eastern Cuba), as well as mineralogy, record complex circulation of Ba-rich fluids and melts in the subduction environment. Partial melting of fluid-fluxed, MORB-derived amphibolite produced trondhjemite magmas that crystallized at depth, in some cases evolving into pegmatites. Qtz-Ms rocks probably crystallized from primary fluids derived from subducted sediments. All these rocks have elevated concentrations of large-ion lithophile elements, especially Ba (up to 11,810 ppm), presumably released from slab sediments by fluids and/or melts. Fluid–rock interaction produced crystallization of phengite in parental amphibolites. The phengite crystallized in all types of rocks is rich in Ba, with concentric zoning, characterized by Ba-rich cores and Ba-poor rims, indicating a compatible behaviour of Ba in the studied systems. Zoning in phengite is governed primarily by the celadonite (tschermak) exchange vector ((Mg,Fe)Si-(Al)-2), with more moderate contributions of the celsian (BaAl-(KSi)-1) and paragonite (NaK-1) exchange vectors. Late remobilization of Ba at relatively low temperature formed retrograde celsian. The compatible behaviour of Ba in the studied rocks strengthens the importance of the stability of phengite for the transfer of LIL elements from the subduction to the volcanic arc environments.  相似文献   

13.
Unusual ultrapotassic dikes were recently found on the Kvalöya Island in Northern Norway. The dikes crosscutting granites 1.8 Ga in age are 0.1–1.0 m thick and consist of phlogopite phenocrysts in a fine-grained groundmass of K-magnesioarfvedsonite, orthoclase, apatite, and secondary chlorite. According to the composition of the rock-forming minerals (4.5–6.0 wt % K2O and 0.7–3.5 wt % TiO2 in magnesioarfved-sonite, 1.6–3.6 wt % FeO in orthoclase, 9.2–10.7 wt % Al2O3 and 2.1–2.6 wt % TiO2 in phlogopite) and its bulk chemical composition (K/Na = 2.3–2.9, K/Al = 1.0–1.2, (Na + K)/Al = 1.4–1.7, Mg# V = 65–73, (La/Yb) n = 100–140, 3.2–4.0 wt % TiO2, 0.55–1.47 wt % BaO, 2.5–3.0 wt % P2O5, 2650–3000 ppm Zr, 900–1260 ppm REE total, 2300–2500 ppm Sr), the rock corresponds to lamproite of the transitional type. The unique chemical composition of the rock resulted in uncommon Ti-Ba-P accessory mineralization, including baotite Ba4(Ti,Nb)8Si4O28Cl (up to 5 vol %), Sr-apatite (5–7 vol %), and previously unknown Na-Mg-Ba phosphate. Baotite forms anhedral elongated and isometric grains 10–500 μm in size. It is characterized by low Nb (0.03–0.05 f.c.); admixtures of K (0.04–0.12 f.c.) and Sr (0.04–0.07) replacing Ba and Fe (0.01–0.03 f.c.); and Al (0.03–0.04 f.c.) substituting Ti. Euhedral elongated zonal apatite crystals are extremely enriched in SrO (8–12 wt %) and REE2O3 + Y2O3 (6–9 wt %) in the marginal zone. Na-Mg-Ba phosphate occurs as prismatic grains 10–100 μm in size. The atomic ratio of its major cations Na: Mg: Ba: P ~ 2: 1: 1: 2 corresponds to the conventional formula Na2MgBa(PO4)2; the mineral contains Sr, Mn, Fe, Ca, Si, and Al admixtures.  相似文献   

14.
The paper presents mineralogical and geochemical data on clinkers and paralavas and on conditions under which they were formed at the Nyalga combustion metamorphic complex, which was recently discovered in Central Mongolia. Mineral and phase assemblages of the CM rocks do not have analogues in the world. The clinkers contain pyrogenically modified mudstone relics, acid silicate glass, partly molten quartz and feldspar grains, and newly formed indialite microlites (phenocrysts) with a ferroindialite marginal zone. In the paralava melts, spinel microlites with broadly varying Fe concentrations and anorthite–bytownite were the first to crystallize, and were followed by phenocrysts of Al-clinopyroxene ± melilite and Mg–Fe olivine. The next minerals to crystallize were Ca-fayalite, kirschsteinite, pyrrhotite, minerals of the rhönite–kuratite series, K–Ba feldspars (celsian, hyalophane, and Ba-orthoclase, Fe3+-hercynite ± (native iron, wüstite, Al-magnetite, and fresnoite), nepheline ± (kalsilite), and later calcite, siderite, barite, celestine, and gypsum. The paralavas contain rare minerals of the rhönite–kuratite series, a new end-member of the rhönite subgroup Ca4Fe 8 2+ Fe 4 3+ O4 [Si8Al4O36], a tobermorite-like mineral Ca5Si5(Al,Fe)(OH)O16 · 5H2O, and high- Ba F-rich mica (K,Ba)(Mg,Fe)3(Al,Si)4O10F2. The paralavas host quenched relics of microemulsions of immiscible residual silicate melts with broadly varying Si, Al, Fe, Ca, K, Ba, and Sr concentrations, sulfide and calcitic melts, and water-rich silicate–iron ± (Mn) fluid media. The clinkers were formed less than 2 Ma ago in various parts of the Choir–Nyalga basin by melting Early Cretaceous mudstones with bulk composition varies from dacitic to andesitic. The pyrogenic transformations of the mudstones were nearly isochemical, except only for volatile components. The CM melt rocks of basaltic andesitic composition were formed via melting carbonate–silicate sediments at temperatures above 1450°C. The Ca- and Fe-enriched and silicaundersaturated paralavas crystallized near the surface at temperatures higher than 900–1100°C and oxygen fugacity \(f_{O_2 }\) between the IW and QFM buffers. In local melting domains of the carbonate–silicate sedimentary rocks and in isolations of the residual melts among the paralava matrix the fluid pressure was higher than the atmospheric one. The bulk composition, mineral and phase assemblages of CM rocks of the Nyalga complex are very diverse (dacitic, andesitic, basaltic andesitic, basaltic, and silica-undersaturated mafic) because the melts crystallized under unequilibrated conditions and were derived by the complete or partial melting of clayey and carbonate–silicate sediments during natural coal fires.  相似文献   

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16.
西天山敦德铁矿床磁铁矿原位LA-ICP-MS元素分析及意义   总被引:5,自引:3,他引:2  
敦德铁矿床是天山成矿带内新近发现并勘查的一处大型海相火山岩型铁矿床。该矿床的矿石可划分为浸染状、稠密浸染状、条带状和块状4种主要类型。其中的条带状矿石包括磁铁矿_矽卡岩条带和磁铁矿_方解石条带2种亚类型。块状矿石内出现围岩或矽卡岩角砾时则构成角砾状矿石,其磁铁矿的成因无甚差异。根据野外观察和矿相显微研究,认为磁铁矿形成于早期矽卡岩阶段后的退化蚀变阶段,之后又被更晚的硫化物阶段和绿泥石_碳酸盐阶段的矿物叠加。敦德磁铁矿内主要发生了Al、Mn、Mg和Zn的类质同象置换,此外,也含有Ti、Si、Ca等次要元素以及Na、K、V、Cr、Ni、Co等多种可检测到的微量元素。磁铁矿内元素含量在空间上显示出直观的差异,由深部到浅部,Mn、Zn含量升高,Si、Ca、Na、K、Pb、Ba、Sr、Sb、Cu等含量降低。在Ti O2_Al2O3_Mg O图解、Ti O2_Al2O3_(Mg O+Mn O)图解和Ca+Al+Mn_Ti+V图解上,敦德磁铁矿的分析数据均投影于热液交代(矽卡岩)成因区域。综上认为,该矿床的磁铁矿可能为热液充填交代成因。  相似文献   

17.
扬子陆块北缘的鄂东北地区是湖北省沉积变质型锰矿集中区,发育了广水—黄陂—蕲春SEE-NWW向元古代沉积变质锰矿带,锰矿赋存于新元古界红安岩群中。本文以鹰咀山锰矿床、四方山锰矿床及孙冲锰矿床为例,分析研究其矿物学特征和地球化学特征,以便为总结该区锰矿床成矿环境及成矿物质来源提供帮助。研究表明,锰矿石矿物主要为菱锰矿、软锰矿、硬锰矿、黑锰矿、锰铝榴石等;矿石化学组分多样,Co、Ni、Zn、Sr、Ba、U等元素相对富集。锰矿石的w(Th)/w(U)、w(V)/w(Cr)值反映锰矿形成于弱氧化-还原的沉积环境;w(SiO2)/w(Al2O3)、w(Fe+Mn)/w(Ti)、w(Fe)/w(Ti)、w(Al)/w(Fe+Mn+Al)、w(Y)/w(Ho)、w(La)/w(Ce)特征值,以及w(SiO2)—w(Al2O3)图解、w(Fe)/w(Ti)—w(Al)/w(Fe+Mn+Al)图解,均反映其成矿过程中有热水物质参与。因此,鄂东北地区的沉积变质型锰矿形成于弱氧化-还原性沉积环境,有热水(液)活动参与成矿作用并提供了丰富的物质来源。  相似文献   

18.
The Finero lherzolite is distinct amongst the tectonically emplaced slices of mantle in the Ivrea Zone (Italian Alps) for its abundant coarse phlogopite. An average composition (SiO2 39.9, TiO2 0.97, Al2O3 16.0, Cr2O3 1.16, FeO 2.73, MgO 24.5, NiO 0.16, BaO 0.31, Na2O 0.58, K2O 8.7, Rb2O 0.056, Cl 0.03, F 0.10 wt.%) is similar in Fe, Cr, Ni, Ba and F/Cl to primary-textured micas from coarse garnet-lherzolite xenoliths from S. Africa, but is higher in Ti, Na, Rb, and Al, and lower in halogens. The distinct values of Ti and Fe for five specimens of Finero peridotites demonstrate local spatial variation. The overall ranges of TiO2 (0.5–1.7) and FeO (2.3–3.6) fall within the range for secondary-textured micas in peridotite xenoliths from S. Africa. The Finero micas are lower in both K/Rb and K/Ba than the primary and secondary micas from S. Africa, and their mean values of K/Rb (110–220) and K/Ba (15–39) are lower than for almost all bulk rocks, but fit well with the ranges of 109–180 and 12–49 for the high-K lavas of the Roman region.Although all evidence is indicative rather than conclusive, the chemical properties of the Finero micas are consistent with introduction of an alkaline phase into peridotite during or before emplacement of the Finero complex from the upper mantle into the crust, and the coarse, partly-deformed textures can be explained by incomplete metamorphic equilibration during prolonged deformation. The alkaline phase is tentatively attributed to the uppermost mantle.  相似文献   

19.
Oxidation of the relatively iron sulfide-poor Dugald River zinc-lead lode in northwest Queensland and reaction of the acid solutions with carbonate has resulted in an undifferentiated gossan profile. The gossan is composed predominantly of quartz, goethite, hematite, barite, adularia, plumbian jarosite, plumbogummite and minor mica, chlorite, kaolinite and montmorillonite. Barite and adularia are formed by the breakdown of the barium feldspar hyalophane (K, Na, Ba)[(Al, Si)4O8] which occurs in the lode.Lead in the gossan is contained within the secondary minerals plumbogummite and plumbian jarosite, and in traces of anglesite and cerussite, whereas Zn occurs in the barite, secondary lead minerals and coronadite structures, and is adsorbed by iron oxides, phyllosilicates and carbonaceous matter. Only traces of zinc minerals smithsonite, goslarite and hemimorphite were detected.Use of Gresens' general metasomatic equation has enabled quantitative determination of compositional changes resulting from the oxidation of the ore. Silicon, Al, Ti and Ba are essentially immobile under the mildly acidic oxidizing conditions. In decreasing order of mobility Cd, Ca, S, Na, K, Mn, Mg, Zn, Ni and Cu, together with CO2 and Tl, have been leached from the gossan profile, while Ag, Sb, Se, As, Fe and Pb appear to have been added to the gossan, notably in a zone of solution-deposited secondary minerals where they have been concentrated, possibly as a result of leaching from the surface gossan.  相似文献   

20.
We analyzed 238U, 234U, 232Th, 230Th, and 226Ra by thermal ionization mass spectrometry (TIMS) and Ba by inductively coupled plasma optical emission spectrometry (ICP-OES) on eight Mn/Fe crusts from the Mecklenburg Bay (SW Baltic) and on one from the Bothnian Bay (N Baltic) to test the 226Raex/Ba ratio as potential geochronometer. 226Raex/Ba ratios decrease as a function of depth within the concretions in all analyzed profiles. Calculated diffusion coefficients are relatively low (∼9 · 10−7 cm2/yr for Ra and 5 · 10−7 cm2/yr for Ba) and suggest that diffusion is negligible for the Ra and Ba record. In addition, 226Raex/Ba ages are consistent and independent from the growth rate and growth direction within a crust. Thus, the decline in 226Raex/Ba ratio is most likely due to radioactive decay of 226Raex, although the influence of varying oxic conditions has still to be evaluated. 226Raex/Ba growth rates range from 0.021 to 0.0017 mm/yr and tend to be lower than those calculated and based on stratigraphic methods (1 to 0.013 mm/yr). 226Raex/Ba ages of concretions from shallow water environment (20 m depth, Mecklenburg Bay/SW Baltic) cover a time interval from 990 ± 140 yr to 4310 ± 310 yr BP corresponding to the stabilization of the sea level close to the present position about 5500 to 4500 yr ago. One sample from greater depth (70 m, Bothnian Bay-/N Baltic) showed a higher 226Raex/Ba age of 6460 ± 520 yr BP.  相似文献   

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