首页> 外文OA文献 >Thermal State, Thickness, and Composition of the Lithospheric Mantle beneath the Upper Muna Kimberlite Field (Siberian Craton) Constrained by Clinopyroxene Xenocrysts and Comparison with Daldyn and Mirny Fields
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Thermal State, Thickness, and Composition of the Lithospheric Mantle beneath the Upper Muna Kimberlite Field (Siberian Craton) Constrained by Clinopyroxene Xenocrysts and Comparison with Daldyn and Mirny Fields

机译:上部Muna Kimberlite领域(西伯利亚Craton)下岩石架的热状态,厚度和组成由Clinopyroxene XenoCrysts约束并与Daldyn和Mirny领域的比较

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摘要

To gain better insight into the thermal state and composition of the lithospheric mantle beneath the Upper Muna kimberlite field (Siberian craton), a suite of 323 clinopyroxene xenocrysts and 10 mantle xenoliths from the Komsomolskaya-Magnitnaya (KM) pipe have been studied. We selected 188 clinopyroxene grains suitable for precise pressure (P)-temperature (T) estimation using single-clinopyroxene thermobarometry. The majority of P-T points lie along a narrow, elongated field in P-T space with a cluster of high-T and high-P points above 1300 °C, which deviates from the main P-T trend. The latter points may record a thermal event associated with kimberlite magmatism (a “stepped” or “kinked” geotherm). In order to eliminate these factors, the steady-state mantle paleogeotherm for the KM pipe at the time of initiation of kimberlite magmatism (Late Devonian–Early Carboniferous) was constrained by numerical fitting of P-T points below T = 1200 °C. The obtained mantle paleogeotherm is similar to the one from the nearby Novinka pipe, corresponding to a ~34–35 mW/m2 surface heat flux, 225–230 km lithospheric thickness, and 110–120 thick “diamond window” for the Upper Muna field. Coarse peridotite xenoliths are consistent in their P-T estimates with the steady-state mantle paleogeotherm derived from clinopyroxene xenocrysts, whereas porphyroclastic ones plot within the cluster of high-T and high-P clinopyroxene xenocrysts. Discrimination using Cr2O3 demonstrates that peridotitic clinopyroxene xenocrysts are prevalent (89%) among all studied 323 xenocrysts, suggesting that the Upper Muna mantle is predominantly composed of peridotites. Clinopyroxene-poor or -free peridotitic rocks such as harzburgites and dunites may be evident at depths of 140–180 km in the Upper Muna mantle. Judging solely from the thermal considerations and the thickness of the lithosphere, the KM and Novinka pipes should have excellent diamond potential. However, all pipes in the Upper Muna field have low diamond grades (<0.9, in carats/ton), although the lithosphere thickness is almost similar to the values obtained for the high-grade Udachnaya and Mir pipes from the Daldyn and Mirny fields, respectively. Therefore, other factors have affected the diamond grade of the Upper Muna kimberlite field.
机译:为了更好地洞察上市上部Muna Kimberlite领域(西伯利亚CRATON)下方的岩石罩的热状态和组成,已经研究了一系列323个Clinopoyroxene XenoCrysts和来自Komsomolskaya-Magnitnaya(KM)管道的10个披风Xenoliths。我们选择了188个临床,适用于精确的压力(P) - 使用单冠状曲烯热量测量法(T)估计。大多数P-T点沿着P-T空间中的一个狭窄的细长场,具有高于1300°C以上的高T和高p点,这偏离了主要的P-T趋势。后一点可以记录与金伯拉特岩浆岩浆相关的热事件(“阶梯式”或“扭结的”地热)。为了消除这些因素,在Kimberlite Magmatism发起时的KM管的稳态地幔古地热量(晚德蒙基 - 早期的石炭系)受到低于T = 1200℃以下的数值拟合的限制。所获得的地幔古地热与附近的新内膜管道相似,对应于〜34-35 mw / m 2的表面热通量,225-230公里的岩石尺寸,110-120厚的“钻窗”为上部Muna田野。粗糙恒星XenoLiths在其P-T估计中与源自临床卵烯烯酯衍生的稳态地幔古地热量一致,而高T和高P临床杂交簇内的卟啉型脉冲曲线。使用Cr2O3的歧视证明,偏异性Clinoceoxene XenoCrysts在所有研究的323个邻烯烯中普遍存在(89%),表明上部Muna Mantle主要由恒星组成。狭窄的贫民岩石或诸如Harzburgites和Dunites的贫困性岩石可能在Upe Muna Mantle的深度为140-180公里处看到。仅从热考虑和岩石圈的厚度来判断,KM和NOVINKA管道应该具有优异的钻石潜力。然而,上部MUNA领域的所有管道都有低金刚石等级(克拉/吨中的<0.9),尽管岩石圈厚度几乎类似于来自Daldyn和Mirny领域的高档Udachnaya和MiR管道所获得的值,分别。因此,其他因素影响了上部Muna金伯利石领域的钻石等级。

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