中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The peridotite-pyroxenite sequence of Rocca d'Argimonia (Ivrea-Verbano Zone, Italy): Evidence for reactive melt flow and slow cooling in the lowermost continental crust

文献类型:期刊论文

作者Tribuzio, Riccardo1,2,3; Renna, Maria Rosaria4; Antonicelli, Marta3; Liu, Tong5; Wu, Fu-Yuan5; Langone, Antonio2,3
刊名CHEMICAL GEOLOGY
出版日期2023-03-05
卷号619页码:17
ISSN号0009-2541
关键词Melt-peridotite reaction Nd-Hf-Sr isotopes U-Pb zircon geochronology Isotopic disequilibrium Post-collisional Variscan evolution Slow cooling evolution
DOI10.1016/j.chemgeo.2023.121315
英文摘要The present study investigates the origin of a - 400 m thick peridotite-pyroxenite sequence, locally known as Rocca d'Argimonia, which is encased within the lowest levels of the -8 km thick Mafic Complex, a gabbrodioritic batholith from the lower continental crust section of the Ivrea-Verbano Zone (Southern Alps). The broad purpose of this work is to elucidate the evolution of mantle-derived magmas emplaced in the lowermost continental crust. We also wish to provide new geochronological constraints on the intrusion and the cooling evolution of the Lower Mafic Complex, which are still mostly unknown. Zircon grains separated from two gabbronorites enclosing the peridotite-pyroxenite sequence document a whole reset of the original U-Pb isotopic system at 286 +/- 2 Ma. A Rocca d'Argimonia peridotite provided a consistent age of 296 +/- 19 Ma, based on a Lu-Hf clinopyroxene-amphibole alignment (initial epsilon Hf = +7.9). These results are interpreted to date the early cooling evolution of the Lower Mafic Complex. The clinopyroxeneamphibole peridotite pair also gave a Rb-Sr alignment corresponding to an age of 250 +/- 16 Ma (initial 87Sr/86Sr = 0.7045), which is reconciled with the subsequent, slow cooling evolution of the Lower Mafic Complex. The Rocca d'Argimonia peridotites (dunites to harzburgites and lherzolites) have whole-rock epsilon Nd(286 Ma) and epsilon Hf(286 Ma) values ranging from +0.4 to -1.1 and from +8.8 to +3.4, respectively, and 87Sr/86Sr(286 Ma) ratios varying from 0.7048 to 0.7060. The peridotites are crosscut by gabbronorite dykes and associated with olivinefree orthopyroxene-dominated pyroxenites. The gabbronorite dykes and the pyroxenites share the Nd-Hf-Sr signature of the peridotites. The gabbronorites enclosing the peridotite-pyroxenite sequence differ in the relatively enriched Nd-Hf-Sr isotopic fingerprint (epsilon Nd(286 Ma) = -4.5 to -5.6, epsilon Hf(286 Ma) = +0.2 to -2.5, 87Sr/86Sr(286 Ma) = 0.7073 to 0.7086). Remarkably, pyroxenes from the pyroxenites typically contain higher Cr2O3 than the peridotite counterparts (e.g., 0.23-0.37 wt% Cr2O3 in peridotite orthopyroxenes and 0.43-0.50 wt% Cr2O3 in pyroxenite orthopyroxenes). We propose that the peridotite-pyroxenite sequence formed by reactive melt percolation through an olivinerich spinel-bearing matrix. In particular, the relatively high Cr2O3 content of the pyroxenitic pyroxenes is attributed to redistribution of Cr released by the breakdown of accessory spinel that was originally present in the olivine-dominated matrix, in response to a high melt/solid ratio. The melt residual after the crystallization of the pyroxenites continued to percolate the olivine-dominated matrix, thereby forming spinel-bearing lherzolites, harzburgites and dunites with the progression of the melt migration process. The chemically most primitive dunite records Nd-Hf-Sr isotopic disequilibrium conditions, thereby providing further information about the process of reactive melt flow. It is inferred that the original olivine-dominated matrix crystallized from a mantle magma having a slightly enriched Nd-Hf-Sr isotopic signature, whereas the percolating melts overall had a relatively depleted Nd-Hf-Sr isotopic fingerprint, despite being variably contaminated by the continental crust.
WOS关键词LARGE MAFIC INTRUSION ; SESIA MAGMATIC SYSTEM ; U-PB ZIRCON ; LU-HF ; SM-ND ; CHEMICAL EVOLUTION ; LHERZOLITE MASSIF ; IGNEOUS PROVINCE ; CHILAS COMPLEX ; TRACE-ELEMENT
WOS研究方向Geochemistry & Geophysics
语种英语
出版者ELSEVIER
WOS记录号WOS:000923019600001
源URL[http://ir.iggcas.ac.cn/handle/132A11/106833]  
专题地质与地球物理研究所_岩石圈演化国家重点实验室
通讯作者Renna, Maria Rosaria
作者单位1.Ist Nazl Oceanog & Geofis Sperimentale, Borgo Grotta Gigante 42-C, I-34010 Trieste, Italy
2.CNR, Ist Geosci & Georisorse, Unita Pavia, Via Ferrata 1, I-27100 Pavia, Italy
3.Univ Pavia, Dipartimento Sci Terra & Ambiente, Via Ferrata 1, I-27100 Pavia, Italy
4.Univ Messina, Dipartimento Sci Matemat & Informat Sci Fis & Sci, Messina, Italy
5.Chinese Acad Sci, Inst Geol & Geophys, Beituchengxilu 19, Beijing, Peoples R China
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Tribuzio, Riccardo,Renna, Maria Rosaria,Antonicelli, Marta,et al. The peridotite-pyroxenite sequence of Rocca d'Argimonia (Ivrea-Verbano Zone, Italy): Evidence for reactive melt flow and slow cooling in the lowermost continental crust[J]. CHEMICAL GEOLOGY,2023,619:17.
APA Tribuzio, Riccardo,Renna, Maria Rosaria,Antonicelli, Marta,Liu, Tong,Wu, Fu-Yuan,&Langone, Antonio.(2023).The peridotite-pyroxenite sequence of Rocca d'Argimonia (Ivrea-Verbano Zone, Italy): Evidence for reactive melt flow and slow cooling in the lowermost continental crust.CHEMICAL GEOLOGY,619,17.
MLA Tribuzio, Riccardo,et al."The peridotite-pyroxenite sequence of Rocca d'Argimonia (Ivrea-Verbano Zone, Italy): Evidence for reactive melt flow and slow cooling in the lowermost continental crust".CHEMICAL GEOLOGY 619(2023):17.

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来源:地质与地球物理研究所

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