Localization of High-Titanium Dolerites in Kimberlite Fields: Possible Causes and a New Criterion for Kimberlite Search

М.D. Тomshin, N. Pokhilenko, S. Gogoleva, A.L. Zemnukhov
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Abstract

––The generalized chemical composition data on the studied dolerites from the Vilyui–Markha dike swarm (Vilyui paleorift) allowed detecting geochemically anomalous areas among them. It has been found that percentage of TiO2 and a number of heavy rare-earth elements (Th, Ta, Hf, Y, Nd) in the dolerites of dikes located within the kimberlite fields show almost twofold increase compared to the normal content for these elements in the Vilyui–Markha dolerites. Similar behavior of these elements is also observed in the dolerite dikes near the Kuoika kimberlite field (the Molodo dike swarm, Olenek paleorift). It is inferred that there is a connection between the increase in abundances of titanium and rare-earth elements in the dolerites and that the latter occur within the lithosphere blocks hosting kimberlite fields. The areas of lithospheric mantle roots linked with the formation of proto-kimberlites may have had bearing on the composition of tholeiite melt both in the processes of its generation and during its ascent to the Earth’s surface, which led to its local enrichment in titanium and a number of other elements. While the processes of the alignment of the geochemical composition between the high-titanium basites and the rest of the melt beyond the contours of the lithospheric blocks with kimberlite fields were weakly pronounced, they were responsible for appearance of zones enriched in titanium. Kimberlite fields that formed before or after basite magmas intrusion overlap with placements of high-titanium dolerite dikes. Thus, high-titanium dolerites in dike swarms (belts) can be used as one of the criteria for kimberlite searches. In view of the above, two new potential zones (Tenkelyakh and Kyulenke areas) for kimberlite exploration have been identified within the Vilyui–Markha dike swarm.
金伯利岩田中高钛辉长岩的定位:金伯利岩搜索的可能原因和新标准
--所研究的维柳伊-马尔卡辉长岩群(维柳伊古漂移)中的辉长岩的一般化学成分数据有助于发现其中的地球化学异常区域。研究发现,位于金伯利岩岩场内的辉长岩中二氧化钛和一些重稀土元素(Th、Ta、Hf、Y、Nd)的含量与维柳伊-马尔卡辉长岩中这些元素的正常含量相比几乎增加了两倍。在 Kuoika 金伯利岩场附近的辉长岩中(奥利尼克古漂移区的莫洛多辉长岩群)也观察到了这些元素的类似情况。据此推断,辉绿岩中钛元素和稀土元素丰度的增加与后者出现在容纳金伯利岩场的岩石圈区块中有关。与原金伯利岩形成有关的岩石圈地幔根区域可能在托勒密岩熔体的生成过程中以及在其上升到地球表面的过程中对其成分产生了影响,从而导致其钛和其他一些元素在局部富集。虽然高钛基性岩和岩石圈块轮廓线以外的熔体与金伯利岩场之间的地球化学成分排列过程并不明显,但它们是出现钛元素富集区的原因。在玄武岩岩浆侵入之前或之后形成的金伯利岩场与高钛辉长岩岩峰的位置重叠。因此,尖晶石群(带)中的高钛辉长岩可作为寻找金伯利岩的标准之一。有鉴于此,在 Vilyui-Markha 长堤群中确定了两个新的潜在金伯利岩勘探区(Tenkelyakh 和 Kyulenke 地区)。
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