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Ferro-manganese nodules from the Kara Sea: Mineralogy, geochemistry and genesis

机译:来自卡拉海的铁锰结节:矿物学,地球化学和创世纪

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Sixteen ferromanganese nodules collected from a large area in the Kara Sea were studied by optical and scanning electron microscopy, X-ray powder diffraction, X-ray fluorescence analysis, inductively coupled plasma mass spectrometry, and electron microprobe analysis. The geological setting, chemical and mineralogical features suggest that Fe-Mn concretions of the Kara Sea mainly were formed by diagenetic process, while hydrogenetic process is secondary if present. The studied nodules are characterized by the alternation of Mn- and Fe-P-enriched laminae. The Fe-P-rich laminae are almost completely composed of an amorphous phase under X-ray. We consider that the phosphatization process did not occur during formation of the Fe-Mn crusts and nodules from the Kara Sea. Several Mn-bearing phases are present in the studied samples (buserite-1, birnessite and X-ray amorphous phase). All studied nodules have similar contents of the main chemical elements. In all cases, the samples are depleted in light REE, enriched in heavy REE, and have negative Ce and Y anomalies. Our data indicate that diagenetic crusts and nodules differ significantly in terms of chemical composition from other types of Fe-Mn concretions. Based on their Co, Ni, Cu, Ce, Zr and Mo contents, we could differentiate diagenetic concretions from hydrogenetic and hydrothermal (both high and low-temperature) concretions.
机译:通过光学和扫描电子显微镜,X射线粉衍射,X射线荧光分析,电感耦合等离子体质谱和电子微探测分析,研究了从卡拉海大面积收集的十六叶锰喃的结节。地质环境,化学和矿物学特征表明,卡拉海的Fe-Mn凝固主要是通过成岩过程形成的,而氢化过程是次要的,如果存在。所研究的结节的特征在于Mn-和Fe-P富含薄层的交替。 Fe-P-富含薄层的薄膜几乎完全由X射线下的非晶相组成。我们认为在从卡拉海形成Fe-Mn壳体和结节期间没有发生磷化过程。研究样品(Buserite-1,Birnerneryite和X射线非晶相)存在几个Mn轴承阶段。所有研究的结节都有类似的主要化学元素的内容物。在所有情况下,样品在轻质ree中耗尽,富含重的ree,并且具有负ce和y异常。我们的数据表明,在来自其他类型的Fe-Mn凝集的化学成分方面,成岩壳和结节显着差异。基于它们的CO,Ni,Cu,Ce,Zr和Mo含量,我们可以区分氢化和水热(高温)凝结的成岩凝集。

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