Reed B. Mershon, Oded Navon, Jeffrey W. Harris, Yaakov Weiss
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The nitrogen aggregation level of all the diamonds is similar, with 6–37% of the nitrogen residing in B centers, suggesting mantle residence temperatures of 1100–1200 ºC. Comparing the composition of the carbonatitic HDFs to available experimental data on melting of carbonated peridotite, we show that they can be produced by a very low degree of partial melting (< 0.1%) of mantle peridotite. In an oxidized environment, such melts are stable in most of the lithospheric mantle and the main barrier for their existence is the reduced nature of the lithosphere. With increasing temperature, the experimental melts evolve towards kimberlites. The similar trace element patterns of the HDFs and their host kimberlite also suggest derivation from similar sources. Still, the difference in the formation temperatures means that the HDFs were trapped in the lithosphere, whereas kimberlite formation requires asthenospheric conditions. 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引用次数: 0
摘要
本文报道了辽宁瓦房店14颗钻石微包裹体中高密度流体(HDFs)的主微量元素组成。本文首次详细报道了华北克拉通HDFs的主要元素和微量元素。被捕获的流体与其他地方已知的流体相似,除了具有独特的富含cl - k - ba - sr的成分,该成分也非常富含Th和轻稀土元素(ree)。一颗钻石含有典型成分的含盐HDF。其余12颗钻石呈高镁碳酸盐型HDFs,微量元素模式与瓦房店金伯利岩相似,但含量更高。所有钻石的氮聚集水平相似,6-37%的氮集中在B中心,表明地幔居住温度为1100 ~ 1200℃。通过对比碳酸化橄榄岩的组成与现有的碳酸化橄榄岩熔融实验数据,我们发现它们可以由地幔橄榄岩极低程度的部分熔融(< 0.1%)产生。在氧化环境下,这种熔体在大多数岩石圈地幔中是稳定的,它们存在的主要障碍是岩石圈的还原性质。随着温度的升高,实验熔体向金伯利岩演化。HDFs及其寄主金伯利岩相似的微量元素模式也表明其来源相似。尽管如此,形成温度的差异意味着HDFs被困在岩石圈中,而金伯利岩的形成需要软流圈的条件。金伯利岩在岩石圈水平上的结晶存在困难,但软流圈顶部形成高镁碳酸盐熔体并在岩石圈中进行最小结晶后将其捕获在金刚石中可能解决这些困难。可能需要更复杂的情景来解释HDFs和金伯利岩的形成。
High-density fluids in diamonds from No. 50 kimberlite pipe, Wafangdian, China: the connection to kimberlites
We report the major and trace element composition of high-density fluids (HDFs) trapped in microinclusions in 14 diamonds from Wafangdian, Liaoning, China. This is the first detailed report of the major and trace elements of HDFs from the North China Craton. The trapped fluids are similar to those known from other localities, except for one with a unique Cl-K-Ba-Sr-rich composition that is also extremely enriched in Th and the light rare earth elements (REEs). One diamond contains a saline HDF of typical composition. The other twelve diamonds exhibit high-Mg carbonatitic HDFs with trace element patterns that resemble those of the Wafangdian kimberlites, but with higher concentrations. The nitrogen aggregation level of all the diamonds is similar, with 6–37% of the nitrogen residing in B centers, suggesting mantle residence temperatures of 1100–1200 ºC. Comparing the composition of the carbonatitic HDFs to available experimental data on melting of carbonated peridotite, we show that they can be produced by a very low degree of partial melting (< 0.1%) of mantle peridotite. In an oxidized environment, such melts are stable in most of the lithospheric mantle and the main barrier for their existence is the reduced nature of the lithosphere. With increasing temperature, the experimental melts evolve towards kimberlites. The similar trace element patterns of the HDFs and their host kimberlite also suggest derivation from similar sources. Still, the difference in the formation temperatures means that the HDFs were trapped in the lithosphere, whereas kimberlite formation requires asthenospheric conditions. Crystallization of kimberlite at lithospheric levels face difficulties, but forming high-Mg carbonatitic melt at the top of the asthenosphere and its trapping in diamond after minimal crystallization in the lithosphere may solve them. More complex scenarios may be needed to explain the formation of both HDFs and kimberlites.
期刊介绍:
Mineralogy and Petrology welcomes manuscripts from the classical fields of mineralogy, igneous and metamorphic petrology, geochemistry, crystallography, as well as their applications in academic experimentation and research, materials science and engineering, for technology, industry, environment, or society. The journal strongly promotes cross-fertilization among Earth-scientific and applied materials-oriented disciplines. Purely descriptive manuscripts on regional topics will not be considered.
Mineralogy and Petrology was founded in 1872 by Gustav Tschermak as "Mineralogische und Petrographische Mittheilungen". It is one of Europe''s oldest geoscience journals. Former editors include outstanding names such as Gustav Tschermak, Friedrich Becke, Felix Machatschki, Josef Zemann, and Eugen F. Stumpfl.