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Homogenisation of sulphide inclusions within diamonds: A new approach to diamond inclusion geochemistry

机译:钻石内硫化物夹杂物的均质化:钻石包容性地球化学的一种新方法

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摘要

Base metal sulphide (BMS) inclusions in diamonds provide a unique insight into the chalcophile and highly siderophile element composition of the mantle. Entombed within their diamond hosts, these provide a more robust (closed system) sample, from which to determine the trace element, Re-Os and S-isotopic compositions of the mantle than mantle xenoliths or orogenic peridotites, as they are shielded from alteration during ascent to the Earth’s crust and subsequent surface weathering. However, at temperatures below 1100 °C some BMS inclusions undergo subsolidus re-equilibration from an original monosulphide solid solution (Mss) and this causes fractionation of the major and trace elements within the inclusions. Thus to study the subjects noted above, current techniques require the entire BMS inclusion to be extracted for analyses. Unfortunately, ‘flaking’ of inclusions during break-out is a frequent occurrence and hence the risk of accidentally under-sampling a portion of the BMS inclusion is inherent in current practices. This loss may have significant implications for Re-Os isotope analyses where incomplete sampling of a Re-rich phase, such as chalcopyrite that typically occurs at the outer margins of BMS inclusions, may induce significant bias in the Re-Os and 187Os/188Os measurements and resulting model and isochron ages.ududWe have developed a method for the homogenisation of BMS inclusions in diamond prior to their break-out from the host stone. Diamonds are heated to 1100 °C and then quenched to chemically homogenise any sulphide inclusions for both major and trace elements. Using X-ray Computed Microtomography (µCT) we determine the shape and spatial setting of multiple inclusions within a host stone and crucially show that the volume of a BMS inclusion is the same both before and after homogenisation. We show that the homogenisation process significantly reduces the inherent variability of in situ analysis when compared with unhomogenised BMS, thereby widening the scope for multiple methods for quantitative analysis, even on ‘flakes’ of single BMS inclusions. Finally we show that the trace elements present in peridotite (P-type) and eclogitic (E-type) BMS are distinct, with P-type diamonds having systematically higher total platinum-group element (particularly Os, Ir, Ru) and Te and As concentrations. These distinctions suggest that the PGE and semi-metal budgets of mantle-derived partial melts will be significantly dependent upon the type(s) and proportions of sulphides present in the mantle source.
机译:钻石中的贱金属硫化物(BMS)夹杂物提供了对地幔中嗜硫菌和高度嗜铁菌元素组成的独特见解。与地幔异种岩或造山橄榄岩相比,它们被包裹在其钻石宿主中,提供了更坚固(封闭的系统)样本,从中可以确定地幔中的痕量元素,Re-Os和S同位素组成,因为它们不受地幔蚀变的影响。上升到地壳和随后的表面风化作用。但是,在低于1100°C的温度下,某些BMS夹杂物会从原始的单硫化物固溶体(Mss)进行亚固相线再平衡,这会导致夹杂物中的主要和微量元素分馏。因此,为了研究上面提到的主题,当前的技术要求提取整个BMS包含的内容进行分析。不幸的是,在破裂过程中夹杂物的“剥落”现象经常发生,因此,当前BMS夹杂物意外取样不足的风险是固有的。这种损失可能会对Re-Os同位素分析产生重大影响,因为Re-Os相的不完全采样(例如通常发生在BMS夹杂物外围的黄铜矿)可能会在Re-Os和187Os / 188Os测量中引起显着偏差。 ud ud我们已经开发出一种方法,可以在钻石中的BMS夹杂物从主石中分离出来之前对其进行均质化。将钻石加热到1100°C,然后淬火以化学均化所有主要元素和痕量元素的硫化物夹杂物。使用X射线计算机断层扫描(µCT),我们可以确定宿主石中多个夹杂物的形状和空间设置,并至关重要地表明,均质化前后,BMS夹杂物的体积均相同。我们显示,与未均质的BMS相比,均质化过程显着降低了原位分析的固有变异性,从而扩大了多种定量分析方法的范围,即使是单个BMS夹杂物的“薄片”也是如此。最后,我们发现橄榄岩(P型)和辉闪岩(E型)BMS中存在的痕量元素是截然不同的,P型钻石具有系统地较高的总铂族元素(特别是Os,Ir,Ru)和Te和作为浓度。这些区别表明,地幔衍生的部分熔体的PGE和半金属预算将明显取决于地幔源中存在的硫化物的类型和比例。

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