Recent Data on the Isotope–Geochemical Composition of Kimberlites in the TSNIGRI-Arkhangelskaya Pipe, Arkhangelsk Diamondiferous Province (Northern East European Platform)

IF 0.7 4区 地球科学 Q4 GEOSCIENCES, MULTIDISCIPLINARY
E. V. Agasheva, L. V. Zyryanova, A. M. Agashev, N. G. Soloshenko, N. P. Pokhilenko
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Abstract

Recent data on the bulk and isotopic (Sr, Nd) composition of kimberlites from the low-diamondiferous TsNIGRI–Arkhangelskaya pipe, located in the Kepino field of the Arkhangelsk diamondiferous province, are presented. It is shown that the kimberlites belong to the moderate titanium type of kimberlites of the province and differ significantly from the previously studied kimberlites of the Kepino field in the lower concentrations of TiO2, Ba, high field strength, and light rare earth elements. Among all the kimberlites of the province, the kimberlites from the TsNIGRI–Arkhangelskaya pipe have the most radiogenic Sr composition (87Sr/86Sr t from 0.7068 to 0.7089), which may be related to a combination of several factors. It has been established that the kimberlites from the pipe are represented by two varieties, having differences both in the concentrations of major and trace elements and in the Sr and Nd isotopic composition. The Nd isotopic composition (εNd from 0 to –0.6) for type-I kimberlites indicates their enriched source in the lithospheric mantle. The type-II kimberlites have a less radiogenic Nd composition (εNd from –3.5 to –4.9), which is interpreted ambiguously: their formation from an even more ancient enriched source inside the lithospheric mantle compared to type-I kimberlites cannot be excluded.

Abstract Image

关于阿尔汉格尔斯克(北东欧地台)金刚石矿床 TSNIGRI-Arkhangelskaya 矿管中金伯利岩同位素地球化学成分的最新数据
摘要 本文介绍了位于阿尔汉格尔斯克金刚石矿区克皮诺矿田的低菱锰矿TsNIGRI-Arkhangelskaya矿管金伯利岩的块状成分和同位素(Sr、Nd)成分的最新数据。研究表明,这些金伯利岩属于该省的中等钛型金伯利岩,与之前研究过的克皮诺矿田金伯利岩在二氧化钛、钡、高场强和轻稀土元素含量方面有很大不同。在该省的所有金伯利岩中,来自 TsNIGRI-Arkhangelskaya 管道的金伯利岩的放射性 Sr 成分最高(87Sr/86Sr t 从 0.7068 到 0.7089),这可能与多种因素的综合作用有关。已经确定,来自该管道的金伯利岩有两个品种,在主要元素和微量元素的浓度以及硒和钕的同位素组成方面都存在差异。I 型金伯利岩的钕同位素组成(εNd 从 0 到 -0.6)表明其富源于岩石圈地幔。II型金伯利岩的钕同位素组成(εNd从-3.5到-4.9)的辐射性较低,对其解释含糊不清:与I型金伯利岩相比,不能排除它们是由岩石圈地幔内更古老的富集源形成的。
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来源期刊
Doklady Earth Sciences
Doklady Earth Sciences 地学-地球科学综合
CiteScore
1.40
自引率
22.20%
发文量
138
审稿时长
3-6 weeks
期刊介绍: Doklady Earth Sciences is a journal that publishes new research in Earth science of great significance. Initially the journal was a forum of the Russian Academy of Science and published only best contributions from Russia. Now the journal welcomes submissions from any country in the English or Russian language. Every manuscript must be recommended by Russian or foreign members of the Russian Academy of Sciences.
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