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新特提斯缝合带中的铬铁矿带是全球最重要的豆荚状铬铁矿成矿带之一,尤其是新特提斯缝合带中段,即穆斯林巴赫-科希斯坦-雅鲁藏布江一带,自东向西发育罗布莎、马拉坎德、穆斯林巴赫等若干大型铬铁矿床。本文系统总结和梳理新特提斯缝合带中段蛇绿岩的时空分布特征以及典型豆荚状铬铁矿的矿床特征、赋存规律和控矿因素。研究表明,蛇绿岩形成时代主体为中侏罗世—晚白垩世,自东向西大致呈逐渐变新的趋势,构造侵位的时代相近,为古新世—始新世;马拉坎德、瓦济里斯坦、穆斯林巴赫及贝拉铬铁矿,与罗布莎矿床相似,均属于富铬型铬铁矿,产于SSZ相关构造背景下,显示良好的岩相分带,具有良好的成矿条件;提出下一步找矿方向是针对成矿条件优越的蛇绿岩,解析层序剖面,识别纯橄岩与方辉橄榄岩的岩相分带,确定有利赋矿岩相。 相似文献
2.
在萨尔托海高铝型铬铁矿中发现20余种矿物,包括金刚石、单质铬、自然铁和单质硅等自然元素类;碳化物碳硅石;铁镍、铁镍铬合金等金属合金;方铁矿、金红石、赤铁矿、磁铁矿、钛铁矿、石英和铬尖晶石等氧化物类;方铅矿、闪锌矿、针镍矿、赫硫镍矿和毒砂等硫化物类;镁橄榄石、顽火辉石、透辉石、蛇纹石、锆石和长石等硅酸岩类。这些超高压、强还原性和壳源矿物与俄罗斯极地乌拉尔以及西藏罗布莎铬铁矿可以对比,暗示萨尔托海高铝铬铁矿和高铬铬铁矿一样,可能存在深部地幔成矿阶段。深部地幔矿物以及浅部壳源矿物的发现,暗示萨尔托海铬铁矿的形成可能经历了深部地幔预富集和浅部再造富集成矿两个阶段。 相似文献
3.
豆荚状铬铁矿豆状结构成因机制探讨--以遵化地区豆荚状铬铁矿为例 总被引：5，自引：0，他引：5
豆荚状铬铁矿是蛇绿岩套地幔构造岩中特征的矿产 ,其矿石发育丰富的岩浆 -变形结构构造类型 ,对认识大洋上地幔成因及其成矿过程具有重要意义。对遵化新太古代豆荚状铬铁矿的深入研究 ,发现它们发育了丰富的岩浆结构 (豆状结构、豆壳状结构等 ) ,还保留了大量凝缩标志和旋转特征。对比分析其各种特征结构发现豆状结构是由浸染状结构逐步演化形成的 ,并且旋转和凝缩是形成豆状结构的主要机理。豆荚状铬铁矿以其独特而稳定的物理化学特性 ,记录了大洋地幔深部岩浆活动(特别是扩张中心原始岩浆活动 )以及大洋岩石圈运动过程。因此 ,研究其成因机制能够为研究大洋上地幔动力学机制提供重要线索 相似文献
4.
从西藏雅鲁藏布江蛇绿岩带的罗布莎蛇绿岩的铬铁矿中，发现一个由70-80种奇异矿物组成的地幔矿物群，其中包括一种成分特殊的尖晶石类矿物。该种尖晶石呈包裹体分布在毒砂中，28粒该矿物的平均化学成分：Na2O 1.58％，MgO7．52％，Al2O3 36．59％，SiO2 44．45％，FeO 8．72％，并含少量CaO和TiO2。经激光拉曼谱仪测试，一部分颗粒具有Franclinite（锌铁尖晶石ZnFe2O4）拉曼谱。根据尖晶石结构和化学成分，可以得出两种分子式：（Mg0．52Na0．14Fe0.32Al0.74）1.72（Si2.00Al1.20）3.20O8和（Mg0.52Na0.14Fe0.32Si0.50）1.48相（Si1.50Al1.94）3．44O8。两种分子式都表明阳离子Si呈六配位占据尖晶石八面体晶格位置。Si离子呈六配位的硅酸盐。实验证明具有超高压性质，来自相当于过渡带400-670km的深部。表明西藏雅鲁藏布江蛇绿岩（古大洋岩石圈）的岩浆活动达到过渡带。可能是地幔柱活动将硅尖晶石类等超高压矿物搬运到上地幔浅部的。 相似文献
5.
豆荚状铬铁矿是蛇绿岩套地幔构造岩中特征的矿产,其矿石发育丰富的岩浆活动-高温变形结构构造类型,豆荚状铬铁矿高温下仍具有稳定的物理化学特性,对认识大洋上地幔扩张、横向运移具有重要指示意义。在对遵化新太古代豆荚状铬铁矿显微构造的深入研究基础上,通过对比分析豆荚状铬铁矿结构构造特征(岩浆活动、低温变形),提出高温变形结构及其特征(拉长网孔结构、条带状、糜棱状结构等)。借鉴现代洋中脊及弧后盆地扩张的构造模型,提出华北新太古代豆荚状铬铁矿扩张中心形成后的显微构造演化序列,豆荚状铬铁矿变形机制的研究,可以提供认识早期大洋上地幔动力学过程的新线索。 相似文献
6.
Rodolfo A. TAMAYO Jr Graciano P. YUMUL Jr René C. MAURY Mireille POLVÉ Joseph COTTEN Marcel BOHN 《Resource Geology》2001,51(2):145-164
Abstract: The Antique ophiolite, located in Panay island (west‐central Philippines), corresponds to several tectonic slices within the suture zone between the Philippine Mobile Belt (PMB) and the North Palawan Block (NPB). It includes dismembered fragments of a basaltic sequence, dominantly pillow‐lavas with minor sheet flows, rare exposures of sheeted dikes, isotropic gabbros, subordinate layered mafic and ultramafic rock sequences and serpentinites. Most of the ophiolite units commonly occur as clasts and blocks within the serpentinites, which intrude the whole ophiolitic body, as well as, the basal conglomerate of the overlying Middle Miocene sedimentary formation. The volcanic rock sequence is characterized by chemical compositions ranging from transitional (T)‐MORB, normal (N)‐MORB and to chemistry intermediate between those of MORB and island arc basalt (IAB). The residual upper mantle sequence is harzburgitic and generally more depleted than the upper mantle underlying modern mid‐oceanic ridges. Calculations using whole‐rock and mineral compositions show that they can represent the residue of a fertile mantle source, which have undergone degrees of partial melting ranging from 9‐22.5 %. Some of the mantle samples display chondrite‐nor‐malized REE and extended multi‐element patterns suggesting enrichments in LREE, Rb, Sr and Zr, which are comparable to those found in fore‐arc peridotites from the Izu‐Bonin‐Mariana (IBM) arc system. The Antique ultramafic rocks also record relatively oxidizing mantle conditions (Δlog fO2 (FMQ)=0.9‐3.5). As a whole, the ophiolite probably represents an agglomeration of oceanic ridge and fore‐arc crust fragments, which were juxtaposed during the Miocene collision of the PMB and the NPB. The intrusion of the serpentinites might be either coeval or subsequent to the accretion of the oceanic crust onto the fore‐arc. Volcanogenic massive sulfide (VMS) deposits occur either in or near the contact between the pillow basalts and the overlying sediments or interbedded with the sediments. The morphology of the deposits, type of metals, ore texture and the nature of the host rocks suggest that the formation of the VMS bodies was similar to the accumulation of metals around and in the subsurface of hydrothermal vents observed in modern mid‐oceanic ridge and back‐arc basin rift settings. The podiform chromitites occur as pods and subordinate layers within totally serpentinized dunite in the residual upper mantle sequence. No large coherent chromitite deposit was found since the host dunitic rocks often occur as blocks within the serpentinites. It is difficult to evaluate the original geodynamic setting of the mineralized bodies since the chemistry of the host rocks were considerably modified by alteration during their tectonic emplacement. A preliminary conclusion for Antique is that the VMS is apparently associated with a primitive tholeiitic intermediate MORB‐IAB volcanic suite, the chemistry of which is close to the calculated composition of the liquid that coexisted with the podiform chromitites. 相似文献
7.
豆荚状铬铁矿主要赋存于地幔橄榄岩中,与方辉橄榄岩密切相关。在全球的分布与蛇绿岩带分布基本一致,但并非所有蛇绿岩体都赋存有铬铁矿,且其中赋存的铬铁矿体规模和分布都是很不规律的。我们对比研究了国内外9个含铬矿和4个不含铬矿蛇绿岩中地幔橄榄岩的地球化学组成,认为含铬矿地幔橄榄岩具有全岩低含量的CaO(<1.91%)和Al_2O_3(<1.76%)、方辉橄榄岩轻稀土元素富集,橄榄石高Fo值(>90),斜方辉石低Al_2O_3含量(<3.8%)以及副矿物铬尖晶石高Cr/Fe值(>1.5)等特征,可以作为该蛇绿岩体含矿评价的地球化学指标。通过这些指标可知豆荚状铬铁矿床是较高程度部分熔融和地幔交代作用的共同结果,结合前人提出的铬铁矿成矿模式,对铬铁矿的成矿过程有了进一步的认识。 相似文献
8.
豆荚状铬铁矿是铬的主要来源,是中国的紧缺矿种,因此,寻找一批大型铬铁矿矿床已成为解决我国对铬铁矿长期依赖进口的途经.然而对于豆荚状铬铁矿的成因,一直以来都有较大分歧.豆荚状铬铁矿及其围岩地幔橄榄岩中大量异常地幔矿物的发现,引起了各国地质学家对豆荚状铬铁矿成因的新一轮思考.本文着重讨论近年来国内外学者对豆荚状铬铁矿研究的最新成果和进展,包括豆荚状铬铁矿的形态特征、产出规律、矿物化学、铂族元素(PGE)的分布模式,铬铁矿矿石中出现的超高压矿物,以及围岩地幔橄榄岩的演化过程等等.豆荚状铬铁矿中的铬来源于两种辉石的不一致熔融与副矿物铬尖晶石,其形成环境可能在下地幔或者是过渡带的位置.豆荚状中含铂族元素矿物呈包裹体状和裂隙状分布,铂族元素含量与铬铁矿形成过程中的S饱和程度有关,具有多期性的特征.进而初步地拟定了豆荚状铬铁矿形成过程存在四个阶段,分别为铬的来源阶段、铬尖晶石及超高压矿物的结晶阶段、铬铁矿的成矿阶段、铬铁矿的就位阶段,而每一阶段的特征还需进一步细化与翔实,并且需要对不同岩体不同产出的豆荚状铬铁矿矿床进行详细的对比研究. 相似文献
9.
Argyrios Kapsiotis Tassos A. Grammatikopoulos Basilios Tsikouras Konstantinos Hatzipanagiotou 《Resource Geology》2010,60(2):178-191
The Pindos ophiolite complex, located in the north-western part of continental Greece, hosts various podiform chromite deposits generally characterized by low platinum-group element (PGE) grades. However, a few locally enriched in PPGE + Au (up to 29.3 ppm) chromitites of refractory type are also present, mainly in the area of Korydallos (south-eastern Pindos). The present data reveal that this enrichment is strongly dependant on chromian spinel chemistry and base metal sulfide and/or base metal alloy (BMS and BMA, respectively) content in chromitites. Consequently, we used super-panning to recover PGM from the Al-rich chromitites of the Korydallos area. The concentrate of the composite chromitite sample contained 159 PGM grains, including, in decreasing order of abundance, the following major PGM phases: Pd-Cu alloys (commonly non-stoichiometric, although a few Pd-Cu alloys respond to the chemical formula PdCu4), Pd-bearing tetra-auricupride [(Au,Pd)Cu], nielsenite (PdCu3), sperrylite (PtAs2), skaergaardite (PdCu), Pd-bearing auricupride [(Au,Pd)Cu3], Pt and Pd oxides, Pt-Fe-Ni alloys, hollingworthite (RhAsS) and Pt-Cu alloys. Isomertieite (Pd11Sb2As2), zvyagintsevite (Pd3Pb), native Au, keithconnite (Pd20Te7), naldrettite (Pd2Sb) and Rh-bearing bismuthotelluride (RhBiTe, probably the Rh analogue of michenerite) constitute minor phases. The bulk of PGE-mineralization is dominated by PGM grains that range in size from 5 to 10 µm. The vast majority of the recovered PPGM are associated with secondary BMS and BMA, thus confirming that a sulphur-bearing melt played a very important role in scavenging the PGE + Au content of the silicate magma from which chromian spinel had already started to crystallize. The implemented technique has led to the recovery of more, as well as noble, PGM grains than the in situ mineralogical examination of single chromitite samples. Although, the majority of the PGM occur as free particles and in situ textural information is lost, single grain textural evidence is observed. In summary, this research provides information on the particles, grain size and associations of PGM, which are critical with respect to the petrogenesis and mineral processing. 相似文献
10.
Re-Os同位素体系为研究地幔的成分-结构-演化提供了新的地球化学示踪和定年的工具.上地幔Os同位素组成演化的球粒陨石模型是Re-Os体系用于地幔物质定年的基础, 尤其在采用Re亏损模式年龄和Os同位素代理等时线年龄时.综合了铁陨石和各类球粒陨石、地幔橄榄岩包体和蛇绿岩豆荚状铬铁矿的Re-Os同位素体系研究的近期成果, 为认识对流上地幔Os同位素组成的演化提供了制约.对河北遵化蛇绿岩豆荚状铬铁矿岩的研究, 获得新太古代(2.5 Ga)时形成豆荚状铬铁矿的对流上地幔的187Os/188Os=0.110 2, 与球粒陨石型模式的一致.文献中常用的球粒陨石模式的参数如下: 地球形成时(4.558 Ga)初始值187Os/186Os为0.095 31, 现代值分别采用碳质球粒陨石的187Os/186Os比值为0.127 0和原始上地幔(PUM)的187Os/186Os比值为0.129 6, PUM与普通球粒陨石和顽火球粒陨石的187Os/186Os比值接近. 相似文献