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首页> 外文期刊>Tectonophysics: International Journal of Geotectonics and the Geology and Physics of the Interior of the Earth >Composition and thermal structure of the lithospheric mantle beneath kimberlite pipes from the Catoca cluster, Angola
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Composition and thermal structure of the lithospheric mantle beneath kimberlite pipes from the Catoca cluster, Angola

机译:安哥拉卡托卡星团金伯利岩管下岩石圈地幔的成分和热结构

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摘要

Garnet, clinopyroxene and ilmenite xenocrysts from three Angolan kimberlite pipes belonging to the Catoca cluster (Angola Caquele, Camitongo I and II, and Catoca) from the SW part of the Congo-Kasai craton, reveal similar features which suggest a similarity of mantle structure. PT estimates for pyropes, Cr-diopsides and picroilmenites reveal similar geothermal conditions of ~37-40mW/m ~2. This is slightly higher than the values determined for the Catoca pipe. Higher temperature conditions ~45mW/m 2 were determined for low-Cr pyroxenes and omphacites. The similar general mineralogy and suggested mantle lithology, as well as reconstructed layering of the sub-continental lithospheric mantle (SCLM), are similar for Camitongo I-II as well as for Caquele and Catoca pipes. Heating at depths of 7.5-4.5GPa (240-140km) is a general feature of the SCLM beneath the field. The high temperature trend for low-Cr and hybrid pyroxenes from the base of the SCLM up to 30GPa (100km) represents the PT path of the protokimberlite melts. PT conditions for ilmenites mainly correspond to colder conditions of crystallization in wall rocks and the outer parts of magmatic channels.Individual geochemical features of the minerals for each SCLM suggest pervasive metasomatism in lower part of the SCLM. Clinopyroxene trace element patterns from the Caquele pipe reveal a lherzolitic affinity; they are LILE-enriched with Ba peaks due to phlogopite melting, while those from Camitongo I-II show Ta-Nb enrichment and Pb troughs. The ilmenite trends trace the mantle column from deep to shallow mantle, evolving to Fe-ilmenites due to advanced AFC of protokimberlite magma that also produced abundant Fe-rich clinopyroxenes. The rise of calculated fO _2 correlates with the position of protokimberlites. Comparison with the thermal gradient derived from peridotitic inclusions from Catoca cluster is lower than for Lesotho possibly related to the thicker lithospheric roots beneath the Congo-Kasai craton.
机译:来自刚果-Kasai克拉通西南部的三块属于Catoca簇的安哥拉金伯利岩管(安哥拉Caquele,Camitongo I和II和Catoca)的石榴石,斜辉石和钛铁矿异形体显示出相似的特征,表明地幔结构相似。 PT估算的吡咯,Cr-二叠氮化物和微蓝铁矿显示相似的地热条件为〜37-40mW / m〜2。这比为Catoca管道确定的值略高。确定了低Cr辉石和噬菌体的较高温度条件〜45mW / m 2。对于Camitongo I-II以及Caquele和Catoca管道,相似的一般矿物学和建议的地幔岩性,以及次大陆岩石圈地幔(SCLM)的重构分层都相似。 SCLM的一般特征是在7.5-4.5GPa(240-140km)的深度加热。从SCLM底部到30GPa(100km)的低Cr和杂化辉石的高温趋势代表了原金伯利岩熔体的PT路径。钛铁矿的PT条件主要对应于围岩和岩浆通道外部结晶的较冷条件。每种SCLM矿物的个别地球化学特征表明,SCLM下部普遍存在交代作用。 Caquele管道中的次氯铵痕量元素图谱显示了亮沸石亲和力。由于金云母融化,它们富含LILE,并带有Ba峰,而来自Camitongo I-II的那些峰则显示了Ta-Nb富集和Pb槽。钛铁矿的趋势是从地幔柱的深部到浅部,从铁基钛矿岩浆的高级AFC演化为铁钛铁矿,这也产生了富铁的富斜辉石。计算出的fO _2的增加与原金伯利岩的位置相关。与来自Catoca团簇的钙质包裹体的热梯度相比,莱索托的热梯度要低,这可能与刚果-Kasai克拉通下面的岩石圈根部较厚有关。

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