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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >SHRIMP U-Pb dating, trace elements and the Lu-Hf isotope system of coesite-bearing zircon from amphibolite in the SW Sulu UHP terrane, eastern China
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SHRIMP U-Pb dating, trace elements and the Lu-Hf isotope system of coesite-bearing zircon from amphibolite in the SW Sulu UHP terrane, eastern China

机译:中国东部苏鲁超高压地块中角闪石中含辉矾岩锆石的SHRIMP U-Pb年代,微量元素和Lu-Hf同位素体系

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In this study, we link mineral inclusion data, trace element analyses, U-Pb age and Hf isotope composition obtained from distinct zircon domains of complex zircon to unravel the origin and multi-stage metamorphic evolution of amphibolites from the Sulu ultrahigh-pressure (UHP) terrane, eastern China. Zircon grains separated from amphibolites from the CCSD-MH drill hole (G12) and Niushan outcrop (G13) were subdivided into two main types based on cathodoluminescence (CL) and Laser Raman spectroscopy: big dusty zircons with inherited cores and UHP metamorphic rims and small clear zircons. Weakly zoned, grey-white luminescent inherited cores preserve mineral inclusions of Cpx + Pl + Ap +/- Qtz indicative of a mafic igneous protolith. Dark grey luminescent overgrowth rims contain the coesite eclogite-facies mineral inclusion assemblage Coe + Grt + Omp + Phe + Ap, and formed at T = 732-839 degrees C and P = 3.0-4.0 GPa. In contrast, white luminescent small clear zircons preserve mineral inclusions formed during retrograde HP quartz eclogite to LP amphibolite-facies metamorphism (T= 612-698 degrees C and P = 0.70-1.05 GPa). Inherited zircons from both samples yield SHRIMP Pb-206/U-238 ages of 695-520 Ma with an upper intercept age of 800 +/- 31 Ma. The UHP rims yield consistent Triassic ages around 236-225 and 239-225 Ma for G12 and G13 with weighted means of 229 +/- 3 and 231 +/- 3 Ma, respectively. Small clear zircons from both samples give Pb-206/U-238 ages around 219-210 Ma with a weighted mean of 214 +/- 3 Ma, interpreted as the age of retrograde quartz eclogite-facies metamorphism. Matrix amphibole from both samples indicate Ar-Ar ages of 209 +/- 0.7 and 207 +/- 0.7 Ma, respectively, probably dating late amphibolite-facies retrogression. The data suggest subduction of Neoproterozoic mafic igneous rocks to UHP conditions in Middle Triassic (similar to 230 Ma) times and subsequent exhumation to an early HP (similar to 214 Ma) and a late LP stage (similar to 208 Ma) over a period of similar to 16 and 6 Myr, respectively. Thus, early exhumation from a mantle depth of 120-100 km to about 60 km occurred at an average rate of 0.3 cm/y, while subsequent exhumation to a middle crustal level took place at approximately 0.54 cm/y. These exhumation rates are considerably slower than those obtained for UHP rocks in the Dora Maira and Kokchetav massifs (2-3 cm/y). Based on similar P-T estimates and trace element and Hf isotope compositions, Sulu amphibolites can be identified as retrograde UHP eclogites. The epsilon Hf-(800) of +8 implies a significant input from the depleted mantle to the Sulu-Dabie terrane during the middle Neoproterozoic. Overgrown rims are characterized by a distinct trace element composition with low Lu/Hf and Th/U and significantly higher Hf-176/Hf-177 ratios than inherited cores, consistent with formation during/after garnet (re-)crystallization and fractionation of the Lu-Hf system during UHP metamorphism. The combined dataset suggests homogenization of the Hf-176/Hf-177 ratio within the metamorphic mineral assemblage and during protolith formation. Observed variations are explained by mixing of material from both domains during laser ablation, e.g., due to partial recrystallization of inherited cores. (c) 2008 Elsevier Ltd. All rights reserved.
机译:在这项研究中,我们将从复杂锆石的不同锆石域获得的矿物包裹体数据,微量元素分析,U-Pb年龄和Hf同位素组成,以揭示苏禄超高压(UHP)闪石的起源和多阶段变质演化。 )中国东部的terrane。从阴极射线发光(CL)和激光拉曼光谱学的角度出发,将从CCSD-MH钻孔(G12)和牛山露头(G13)的角闪石中分离出的锆石颗粒分为两种主要类型:尘土大的锆石,具有继承的核,UHP变质的边缘小。清除锆石。薄弱区域,灰白色发光的继承核保留了Cpx + Pl + Ap +/- Qtz的矿物包裹体,表明镁铁质火成原生质。暗灰色发光的过度生长轮缘包含堇青石榴辉岩相矿物包裹体组合Coe + Grt + Omp + Phe + Ap,在T = 732-839摄氏度和P = 3.0-4.0 GPa时形成。相反,白色发光的小透明锆石保留了从逆向HP石英榴辉岩到LP闪石相变质(T = 612-698摄氏度和P = 0.70-1.05 GPa)形成的矿物包裹体。从两个样品中继承的锆石产生的SHRIMP Pb-206 / U-238年龄为695-520 Ma,上限为800 +/- 31 Ma。 UHP轮缘对G12和G13产生一致的三叠纪年龄,分别为236-225和239-225 Ma,加权平均数分别为229 +/- 3和231 +/- 3 Ma。来自两个样品的小的透明锆石给出的Pb-206 / U-238年龄约为219-210 Ma,加权平均值为214 +/- 3 Ma,这被解释为逆向石英榴辉岩相变质的年龄。来自两个样品的基质闪石表明Ar-Ar年龄分别为209 +/- 0.7 Ma和207 +/- 0.7 Ma,可能年代为晚闪石相回退。数据表明,新元古代镁铁质火成岩在中三叠世(约230 Ma)时间内被超高压条件所俯冲,随后在一段时期内发掘到早期HP(类似于214 Ma)和LP晚期(类似于208 Ma)。分别类似于16和6 Myr。因此,从地幔深度120-100 km到大约60 km的早期发掘出土的平均速率为0.3 cm / y,而随后的发掘到中地壳水平的发掘出率约为0.54 cm / y。这些掘尸速度比在多拉·迈伊拉(Dora Maira)和科科切察夫(Kokchetav)地块(2-3 cm / y)的超高压岩石采掘速度要慢得多。基于相似的P-T估算值以及痕量元素和Hf同位素组成,可以将Sulu闪石视为逆行UHP榴辉岩。 εHf-(800)为+8表示在新元古代中期从枯竭的地幔到苏鲁-大比地层有大量输入。杂草丛生的轮缘的特征是独特的痕量元素组成,其Lu / Hf和Th / U较低,Hf-176 / Hf-177的比率比遗传核高得多,这与石榴石(再)结晶和分馏过程中/之后的形成一致。超高压变质过程中的Lu-Hf系统。合并的数据集表明,在变质矿物组合中和原生石形成过程中,Hf-176 / Hf-177比率均质化。观察到的变化是通过在激光烧蚀过程中混合两个畴中的材料来解释的,例如,由于继承核的部分重结晶。 (c)2008 Elsevier Ltd.保留所有权利。

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