印度东部Singhbhum克拉通1.77 Ga白云岩岩脉中Fe-Ni-Cu (Co)硫化物和Fe-Ti氧化物矿物的成因

A. Dey, S. Mondal
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引用次数: 2

摘要

在印度东部的Singhbhum克拉通中,白云岩岩脉群广泛分布于新太古代至古元古代,形成于地壳稳定之后。这些岩脉群的分布方向为NE-SW ~ NNE-SSW、NW-SE ~ WNW-ESE、东西走向和南北走向。在印度奥里萨邦Satkosia地区取样了向西西北东向的c. 1.77 Ga Pipilia堤防群。辉石、斜长石、Fe-Ti氧化物矿物的模态比例、粒度和结构在走向上存在明显差异。有些地方原生硅酸盐蚀变为角闪孔、绿泥石和绢云母的次生水化矿物组合。原生硅酸盐为斜辉石(辉石- mg# = 65.7-82.6;En37-48Fs11-17Wo36-41),正辉石(斜钙辉石- Mg# = 68.5-78;En63-70Fs20-29Wo4-5)和斜长石(An11-39Ab44-82Or1-7), Fe-Ti氧化物为钛磁铁矿(FeO, 34.38-39.50 wt%;Fe2O3, 48.26-56.21 wt%;TiO2, 5.05-9.60 wt%)和钛铁矿(FeO, 40.75-43.79 wt%;Fe2O3, 3.54-10.03 wt%;TiO2, 47.82-50.87 wt%)。采用双辉石测温法得到平衡温度范围为1065 ~ 978℃,共存钛磁铁矿对在氧逸度(fO2)条件NNO + 0.3 ~ FMQ−1.03下的平衡温度范围为731.39 ~ 573.37℃。岩脉在铁钛氧化物和硅酸盐的间隙处含有浸染的硫化物。硫化物矿物主要有黄铁矿、黄铜矿和钒锡矿;黄铁矿-钒锡岩组合与次生硅酸盐矿物伴生。黄铁矿颗粒含有不同浓度的Co (0.01-5.70 wt%)和Ni (0.02-1.95 wt%)。共存的钒锡石含有Co (2.42-10.44 wt%)、Ni (26.40-47.88 wt%)和Fe (7.32-26.55 wt%)。结构、硫化物-硅酸盐组合以及黄铁矿-钒锡石组合等低金属硫硫化物的存在表明,从高温不混相硫化物中分离出来的原生铁镍硫化物(磁黄铁矿-镍黄铁矿)受到晚期岩浆/热液活动的修饰。在全球范围内已发现了大量沉积于古元古代超镁铁质-基性侵入体中的含硫化物矿床,Singhbhum克拉通c. 1.77 Ga Pipilia岩脉群中铁镍硫化物的出现增加了该克拉通在印度东部的勘探潜力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Origin of Fe–Ni–Cu (Co) sulfide and Fe–Ti oxide minerals in the c. 1.77 Ga dolerite dyke, Singhbhum Craton (eastern India)
Abstract Dolerite dyke swarms are widespread within the Singhbhum Craton (eastern India) that emplaced from the Neoarchean to Paleoproterozoic era just after the stabilization of crust before c. 3 Ga. These dyke swarms are oriented in NE–SW to NNE–SSW, NW–SE to WNW–ESE, east–west and north–south directions. The WNW–ESE-trending c. 1.77 Ga Pipilia dyke swarm is sampled from the Satkosia area of Orissa state. The dyke shows a noticeable disparity in terms of the modal proportion and grain size of pyroxenes, plagioclase, Fe–Ti oxide minerals and texture across the trend. In places the primary silicates are altered to secondary hydrated mineral assemblages of amphibole, chlorite and sericite. The primary silicates are clinopyroxene (augite – Mg# = 65.7–82.6; En37–48Fs11–17Wo36–41), orthopyroxene (clinoenstatite – Mg# = 68.5–78; En63–70Fs20–29Wo4–5) and plagioclase (An11–39Ab44–82Or1–7) and the Fe–Ti oxides are titanomagnetite (FeO, 34.38–39.50 wt%; Fe2O3, 48.26–56.21 wt%; TiO2, 5.05–9.60 wt%) and ilmenite (FeO, 40.75–43.79 wt%; Fe2O3, 3.54–10.03 wt%; TiO2, 47.82–50.87 wt%). Application of two-pyroxene thermometry yields an equilibration temperature range of 1065–978°C, and coexisting titanomagnetite–ilmenite pairs reveal 731.39–573.37°C under the oxygen fugacity (fO2) condition NNO + 0.3 to FMQ − 1.03. The dyke contains disseminated sulfides at the interstices of Fe–Ti oxides and silicates. Major sulfide minerals are pyrite, chalcopyrite and vaesite; pyrite–vaesite assemblages occur in association with secondary silicate minerals. Pyrite grains contain variable concentrations of Co (0.01–5.70 wt%) and Ni (0.02–1.95 wt%). Coexisting vaesite contains Co (2.42–10.44 wt%), Ni (26.40–47.88 wt%) and Fe (7.32–26.55 wt%). Texture, sulfide–silicate assemblage and the presence of low metal/S sulfides such as the pyrite–vaesite assemblage indicate that primary Fe–Ni sulfides (pyrrhotite–pentlandite) that segregated from immiscible sulfide liquid at high temperature are modified by late magmatic/hydrothermal fluid activities. Numerous sulfide-bearing deposits hosted in ultramafic–mafic intrusions of Paleoproterozoic age have been recorded globally and the occurrence of Fe–Ni sulfides in the c. 1.77 Ga Pipilia dyke swarm in the Singhbhum Craton enhances the exploration potential of this craton in eastern India.
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