首页> 外文期刊>International Journal of Earth Sciences >Post-collisional melting of crustal sources: constraints from geochronology, petrology and Sr, Nd isotope geochemistry of the Variscan Sichevita and Poniasca granitoid plutons (South Carpathians, Romania)
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Post-collisional melting of crustal sources: constraints from geochronology, petrology and Sr, Nd isotope geochemistry of the Variscan Sichevita and Poniasca granitoid plutons (South Carpathians, Romania)

机译:碰撞后地壳物质的融化:年代学,岩石学和瓦里斯卡纳Sichevita和Poniasca花岗岩类云母的Sr,Nd同位素地球化学的制约(罗马尼亚南喀尔巴阡山脉)

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The Sichevita and Poniasca plutons belong to an alignment of granites cutting across the metamorphic basement of the Getic Nappe in the South Carpathians. The present work provides SHRIMP age data for the zircon population from a Poniasca biotite diorite and geochemical analyses (major and trace elements, Sr-Nd isotopes) of representative rock types from the two intrusions grading from biotite diorite to biotite K-feldspar porphyritic monzogranite. U-Pb zircon data yielded 311 ±2 Ma for the intrusion of the biotite diorite. Granites are mostly high-K leucogranites, and biotite diorites are magnesian, and calcic to calc-alkaline. Sr, and Nd isotope and trace element data (REE, Th, Ta, Cr, Ba and Rb) permit distinguishing five different groups of rocks corresponding to several magma batches: the Poniasca biotite diorite (P_1) shows a clear crustal character while the Poniasca granite (P_2) is more juvenile. Conversely, Sichevita biotite diorite (S_1), and a granite (S_2~*) are more juvenile than the other Sichevita granites (S_2). Geochemical modelling of major elements and REE suggests that fractional crystallization can account for variations within P_1 and S_1 groups. Dehydration melting of a number of protoliths may be the source of these magma batches. The Variscan basement, a subduction accretion wedge, could correspond to such a heterogeneous source. The intrusion of the Sichevita-Po-niasca plutons took place in the final stages of the Variscan orogeny, as is the case for a series of European granites around 310 Ma ago, especially in Bulgaria and in Iberia, no Alleghenian granitoids (late Carboniferous-early Permian times) being known in the Getic nappe. The geodynamical environment of Sichevita-Poniasca was typically post-collisional of the Variscan orogenic phase.
机译:Sichevita和Poniasca岩体属于花岗岩排列,横切南喀尔巴阡山脉Getic Nappe的变质基底。本工作提供了Poniasca黑云母闪长岩锆石种群的SHRIMP年龄数据,以及从黑云母闪长岩到黑云母钾长石斑岩辉长花岗岩的两次侵入的代表性岩石类型的地球化学分析(主要和微量元素,Sr-Nd同位素)。 U-Pb锆石数据对黑云母闪长岩的侵入产生311±2 Ma。花岗岩大多为高钾白云母花岗岩,黑云母闪长岩为镁质钙,钙至钙碱性。 Sr,Nd同位素和痕量元素数据(REE,Th,Ta,Cr,Ba和Rb)可以区分对应于几个岩浆批次的五组不同的岩石:Poniasca黑云母闪长岩(P_1)显示出清晰的地壳特征,而Poniasca花岗岩(P_2)较为幼稚。相反,Sichevita黑云母闪长岩(S_1)和花岗岩(S_2〜*)比其他Sichevita花岗岩(S_2)幼。主要元素和REE的地球化学模拟表明,分级结晶可以解释P_1和S_1组内的变化。许多原岩的脱水熔融可能是这些岩浆批次的来源。俯冲吸积楔形瓦里斯坎地下室可能对应于这种异质源。 Sichevita-Po-niasca岩体的侵入发生在瓦里斯卡造山运动的最后阶段,在310 Ma以前的一系列欧洲花岗岩就是这种情况,特别是在保加利亚和伊比利亚,没有Alleghenian花岗岩(晚石炭纪-二叠纪早期)在盖蒂克的棉布中广为人知。 Sichevita-Poniasca的地球动力学环境通常在Variscan造山相碰撞后。

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