Lithological and compositional diversity of diamond substrates beneath the Koidu kimberlite reveals addition of subducted sediments

IF 3.5 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Contributions to Mineralogy and Petrology Pub Date : 2024-10-04 DOI:10.1007/s00410-024-02176-3
Mei Yan Lai, Thomas Stachel, Matthew F. Hardman, D. Graham Pearson, Jeff W. Harris, Richard A. Stern, Stephen E. Haggerty
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Abstract

Six diamond-bearing eclogite xenoliths with oceanic crust protoliths and 370 mineral inclusions in 104 diamonds recovered from the Koidu kimberlite complex in Sierra Leone provide insight into the lithological and compositional diversity of the lithospheric mantle beneath the West African Craton. Diamond formation beneath Koidu is predominantly associated with eclogitic substrates that originated from subduction and high-pressure metamorphism of oceanic crust, as indicated by a dominance of eclogitic (78%) over peridotitic (17%) and mixed paragenesis diamonds (5%). Peridotitic diamonds contain olivine inclusions with very high Mg# (92.2–94.7; median = 94.2), indicative of derivation from dunite or harzburgite protoliths. Moreover, a peridotitic spinel with Cr# = 50.9 suggests that it equilibrated with orthopyroxene-free dunite. 44% of Koidu diamonds contain coesite, of which some coexist with omphacite, eclogitic garnet, and/or kyanite. Most analysed eclogitic garnet inclusions have extremely high δ18O values ( ≥ + 9.9‰) and occur with clinopyroxene inclusions that have very high jadeite components (~ 70 mol%). These high jadeite components are a close match to clinopyroxenes in high-pressure metapelites, which have a phase assemblage that includes coesite and kyanite. Our data suggest that the eclogitic mineral inclusions in most Koidu diamonds have oceanic basalt protoliths that were mingled with pelagic sediments, which may have increased δ18O values to levels much higher than observed for other eclogites at Koidu and shifted the originally basaltic bulk compositions closer to that of pelites. Most eclogitic mineral inclusions in Koidu diamonds have elemental compositions not observed for Koidu eclogite xenoliths, which have clear oceanic crust protolith (oceanic lavas and cumulates) signatures without significant crustal sediment contamination. These findings suggest the subduction of distinct packages of oceanic crust into the Koidu lithospheric mantle through time.

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科伊杜金伯利岩下金刚石基质的岩性和成分多样性揭示了俯冲沉积物的加入
从塞拉利昂科伊杜金伯利岩群发掘的 104 颗钻石中的 6 颗含钻石的埃克洛杰特异长岩与洋壳原岩和 370 颗矿物包裹体,使人们对西非克拉通下面岩石圈地幔的岩性和成分多样性有了深入的了解。科伊杜地下金刚石的形成主要与蜕屑岩基质有关,蜕屑岩基质源于大洋地壳的俯冲和高压变质作用,蜕屑岩金刚石(78%)比橄榄岩金刚石(17%)和混合成因金刚石(5%)占优势。橄榄石型金刚石含有镁含量极高的橄榄石包裹体(92.2-94.7;中位数=94.2),表明其原石来自云英岩或哈氏岩。此外,Cr# = 50.9 的橄榄石尖晶石表明,它与不含正长石的白云石平衡。44% 的科伊杜金刚石含有共闪石,其中一些与闪长岩、斜长石榴辉岩和/或闪长岩共存。大多数经分析的斜长石榴石包裹体都具有极高的δ18O 值(≥ + 9.9‰),并且与菱辉石包裹体一起出现,这些包裹体具有极高的翡翠成分(约 70 摩尔%)。这些高翡翠成分与高压偏闪长岩中的挛辉石非常相似,后者的相组合包括薏苡岩和闪长岩。我们的数据表明,大多数科伊杜钻石中的夕闪岩矿物包裹体具有海洋玄武岩原岩,它们与远洋沉积物混杂在一起,这可能使δ18O值增加到比在科伊杜的其他夕闪岩中观察到的高得多的水平,并使原本的玄武岩体成分更接近于远洋沉积物。科伊杜金刚石中的大多数蚀变质矿物包裹体的元素组成是在科伊杜蚀变质异长岩中观察不到的,这些异长岩具有明显的大洋壳原岩(大洋熔岩和积岩)特征,没有明显的地壳沉积物污染。这些发现表明,随着时间的推移,不同的大洋地壳包潜入了科伊杜岩石圈地幔。
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来源期刊
Contributions to Mineralogy and Petrology
Contributions to Mineralogy and Petrology 地学-地球化学与地球物理
CiteScore
6.50
自引率
5.70%
发文量
94
审稿时长
1.7 months
期刊介绍: Contributions to Mineralogy and Petrology is an international journal that accepts high quality research papers in the fields of igneous and metamorphic petrology, geochemistry and mineralogy. Topics of interest include: major element, trace element and isotope geochemistry, geochronology, experimental petrology, igneous and metamorphic petrology, mineralogy, major and trace element mineral chemistry and thermodynamic modeling of petrologic and geochemical processes.
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