首页> 外文期刊>Journal of Geochemical Exploration: Journal of the Association of Exploration Geochemists >Detection of concealed Cu-Zn massive sulfide mineralization below eolian sand and a calcrete cover in the eastern part of the Namaqua Metamorphic Province, South Africa
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Detection of concealed Cu-Zn massive sulfide mineralization below eolian sand and a calcrete cover in the eastern part of the Namaqua Metamorphic Province, South Africa

机译:在南非那马夸变质省东部发现风成砂和钙质覆盖物下的隐蔽的Cu-Zn块状硫化物矿化

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The regolith studied here is located at the defunct Areachap mine and the newly discovered Kantienpan Cu-Zn volcanic-hosted massive sulfide (VHMS) deposit, located in the Areachap Group of the eastern part of Mesoproterozoic Namaqua Metamorphic Province. This area is highly prospective for further VHMS discoveries. Paleo and recent weathering of the upper most parts of massive sulfide deposits led to the formation of a gossan zone. Due to semi-arid climatic conditions during the late Cretaceous, affecting the African Land surface, the lowermost units of the Kalahari Group and the underlying floor rocks were calcretized. An approximately 6 m thick calcrete layer formed above the gossan zone and this was later covered by eolian Kalahari sand. Samples were collected from the eolian sand cover in the study areas to determine the best analytical method that would enable recognition of the concealed ore deposits and detect the widest secondary dispersion halo. Mobile metal ions from the finest fraction of the eolian sand samples (<75 μm) were extracted with a NH4EDTA (EDTA) solution. The solution was analysed for Cu, Zn, Pb and Mn by inductively coupled plasma mass spectrometry (ICP-MS). The same grainsize fraction of the original samples was also analysed for comparison purposes by means of X-ray fluorescence (XRF). Results indicate that the ore zone in both areas may be recognized by both partial and total analyses of the eolian sand samples collected, although the calcrete layer, below the sand cover, acts as a partial geochemical barrier. The recognition of the ore zone depends on the regolith forming processes and the thickness of the eolian sand cover. In the Areachap area, with a relatively thick sand cover (in excess of 1 m) above the calcrete layer, the detectable geochemical halo is related to the distribution of the mobile metal ions, and partial extraction (EDTA solution) results define a larger dispersion halo than that, that could be detected by total analysis (XRF). Whereas, in the Kantienpan area with a very thin sand cover (<50 cm) dispersion appears to be related more to the secondary redistribution of gossaniferous clasts released by recent weathering out of the calcrete, than to dispersion of mobile metal ions on the surface of sand particles. In this area, the XRF results reveal a wider dispersion of the elements of interest.
机译:此处研究的长石位于已灭绝的Areachap矿山和新发现的Kantienpan铜锌火山岩质块状硫化物(VHMS)矿床,位于中生代纳马夸变质省东部的Areachap组。该领域对于进一步发现VHMS具有很高的前景。大量硫化物矿床最上部的古风化和最近的风化导致形成了戈桑地带。由于白垩纪晚期的半干旱气候条件,影响了非洲陆地表面,因此将卡拉哈里群的最低层单元和下伏的地基石化了。戈桑地区上方形成了一个约6 m厚的钙质层,随后被风成的喀拉哈里沙漠砂覆盖。从研究区域的风沙覆盖层中收集样品,以确定最佳的分析方法,该方法将能够识别隐藏的矿床并检测最宽的二次弥散晕。用NH4EDTA(EDTA)溶液提取风沙样品中最细部分(<75μm)中的活动金属离子。通过电感耦合等离子体质谱法(ICP-MS)分析溶液中的Cu,Zn,Pb和Mn。为了进行比较,还通过X射线荧光(XRF)分析了原始样品中相同粒度的部分。结果表明,尽管对风积砂样品进行了部分和全部分析,但两个区域的矿石区均可被识别,尽管砂覆盖层下方的钙凝层是部分地球化学屏障。矿石区的识别取决于重碎屑的形成过程和风积砂层的厚度。在Areachap地区,在砂砾层上方有相对较厚的砂层(超过1 m),可检测到的地球化学晕与移动金属离子的分布有关,部分萃取(EDTA溶液)的结果定义了较大的分散度晕,那么可以通过总分析(XRF)进行检测。相比之下,在坎蒂恩潘地区,沙层非常薄(<50厘米),分散似乎与因近期风化作用从碎石中释放出的碎屑岩屑的二次再分布有关,而不是与活动金属离子在水面的分散有关。沙粒。在该区域,XRF结果显示了感兴趣元素的更广泛分散。

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