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Mineralogy, geochemistry and the origin of high-phosphorus oolitic iron ores of Aswan, Egypt

机译:埃及阿斯旺的矿物学,地球化学和高磷橄榄岩铁矿石的起源

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The Coniacian-Santonian high-phosphorus oolitic iron ore at Aswan area is one of the major iron ore deposits in Egypt. However, there are no reports on its geochemistry, which includes trace and rare earth elements evaluation. Texture, mineralogy and origin of phosphorus that represents the main impurity in these ore deposits have not been discussed in previous studies. In this investigation, iron ores from three localities were subjected to petrographic, mineralogical and geochemical analyses. The Aswan oolitic iron ores consist of uniform size ooids with snowball-like texture and tangentially arranged laminae of hematite and chamosite. The ores also possess detrital quartz, apatite and fine-grained ferruginous chamosite groundmass. In addition to Fe2O3, the studied iron ores show relatively high contents of SiO2 and Al2O3 due to the abundance of quartz and chamosite. P2O5 ranges from 0.3 to 3.4 wt.% showing strong positive correlation with CaO and suggesting the occurrence of P mainly as apatite. X-ray diffraction analysis confirmed the occurrence of this apatite as hydroxyapatite. Under the optical microscope and scanning electron microscope, hydroxyapatite occurred as massive and structureless grains of undefined outlines and variable size (5-150 mu m) inside the ooids and/or in the ferruginous groundmass. Among trace elements, V, Ba, Sr, Co, Zr, Y, Ni, Zn, and Cu occurred in relatively high concentrations (62-240 ppm) in comparison to other trace elements. Most of these trace elements exhibit positive correlations with SiO2, Al2O3, and TiO2 suggesting their occurrence in the detrital fraction which includes the clay minerals. Sigma REE ranges between 129.5 and 617 ppm with strong positive correlations with P2O5 indicating the occurrence of REE in the apatite. Chondrite-normalized REE patterns showed LREE enrichment over HREE ((La/Yb)(N) = 2.3-5.4) and negative Eu anomalies (Eu/Eu* = 0.75-0.89). The oolitic texture of the studied ores forms as direct precipitation of iron-rich minerals from sea water in open space near the sediment-water interface by accretion of FeO, SiO2, and Al2O3 around suspended solid particles such as quartz and parts of broken ooliths. The fairly uniform size of the ooids reflects sorting due to the current action. The geochemistry of major and trace elements in the ores reflects their hydrogenous origin. The oolitic iron ores of the Timsha Formation represent a transgressive phase of the Tethys into southern Egypt during the Coniacian-Santonian between the non-marine Turonian Abu Agag and Santonian-Campanian Um Barmil formations. The abundance of detrital quartz, positive correlations between trace elements and TiO2 and Al2O3 , and the abundance mudstone intervals within the iron ores supports the detrital source of Fe. This prediction is due to the weathering of adjacent land masses from Cambrian to late Cretaceous. The texture of the apatite and the REE patterns, which occurs entirely in the apatite, exhibits a pattern similar to those in the granite, thus suggesting a detrital origin of the hydroxyapatite that was probably derived from the Precambrian igneous rocks.
机译:阿斯旺地区的柯尼西亚—桑顿高磷橄榄岩铁矿石是埃及主要的铁矿床之一。但是,尚无有关其地球化学的报道,其中包括痕量和稀土元素的评估。先前的研究尚未讨论过代表这些矿床主要杂质的质地,矿物学和磷的来源。在这项调查中,对三个地区的铁矿石进行了岩石学,矿物学和地球化学分析。阿斯旺软铁矿石由大小均一的,呈雪球状纹理,切向排列的赤铁矿和硅铁矿薄片组成。矿石还具有碎屑石英,磷灰石和细粒铁质辉绿岩质地层。除Fe2O3外,由于石英和硅铁矿的含量高,所研究的铁矿石还显示出较高的SiO2和Al2O3含量。 P 2 O 5的范围为0.3至3.4wt。%,与CaO显示出强烈的正相关,表明P的存在主要是磷灰石。 X射线衍射分析证实该磷灰石以羟基磷灰石的形式存在。在光学显微镜和扫描电子显微镜下,羟基磷灰石以无定形轮廓的块状和无结构的晶粒形式出现,在椭圆形内部和/或在铁质磨削块内尺寸可变(5-150μm)。与其他痕量元素相比,痕量元素中的V,Ba,Sr,Co,Zr,Y,Ni,Zn和Cu的浓度较高(62-240 ppm)。这些微量元素大多数与SiO2,Al2O3和TiO2呈正相关,表明它们存在于包括粘土矿物在内的碎屑中。 Sigma REE在129.5至617 ppm之间,与P2O5呈强正相关,表明磷灰石中存在REE。球粒陨石标准化的REE模式显示LREE高于HREE((La / Yb)(N)= 2.3-5.4)和负Eu异常(Eu / Eu * = 0.75-0.89)。所研究矿石的橄榄质地是通过在悬浮固体颗粒(如石英)和碎卵石的部分附近堆积FeO,SiO2和Al2O3,从沉积物-水界面附近的开放空间中的海水中直接沉淀出富含铁的矿物。卵石的大小相当均匀,反映了由于当前动作而产生的排序。矿石中主要和微量元素的地球化学反映了它们的氢成因。 Timsha组的鲕状铁矿石代表了在非海洋Turonian Abu Agag和Santonian-Campanian Um Barmil组之间的Coniacian-Santonian时期,特提斯进入埃及南部的海侵阶段。碎屑石英的丰度,微量元素与TiO2和Al2O3之间的正相关性以及铁矿石中的丰富泥岩间隔支持了Fe的碎屑源。这种预测是由于从寒武纪到白垩纪晚期的邻近陆地风化。磷灰石的质地和REE模式(完全出现在磷灰石中)表现出与花岗岩相似的模式,因此表明羟基磷灰石的碎屑起源可能源自前寒武纪火成岩。

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