Knowledge Management System Of Guangzhou Institute of Geochemistry，CAS
| Angelo, Tiago Valim1; Spencer, Christopher J.1; Cavosie, Aaron J.2,3; Thomas, Robert4; Li, Hong-Yan5 | |
| Petrogenesis of Mantle-Hosted Granitoids from the Samail Ophiolite | |
| Source Publication | JOURNAL OF PETROLOGY
 |
| ISSN | 0022-3530 |
| 2023-05-01 | |
| Volume | 64Issue:5Pages:17 |
| DOI | 10.1093/petrology/egad021 |
| Language | 英语 |
| WOS Research Area | Geochemistry & Geophysics |
| Abstract | Granitoids with evolved chemical signatures, intruding both oceanic crustal rocks and mantle peridotite, are well known in the Samail supra-subduction ophiolite of Oman and United Arab Emirates. The former are metaluminous tonalites and trondhjemites have positive epsilon Nd, relatively low delta O-18 values, resemble ridge 'tholeiitic' granitoids with MORB-like affinity, and formed by fractionation of basalt/gabbro or anatexis of oceanic crust. In contrast, the mantle-hosted granitoids are peraluminous, with negative epsilon Nd and high delta O-18 values. They can be modeled as having formed by mixing between partial melts of metabasalt and metasedimentary rocks with minimal mantle contribution. The mantle-hosted granitoids resemble typical peraluminous S-type granitoids (e.g. Himalaya, Variscan, Lachlan) but are compositionally distinct in having notably scattered data values of K2O, Na2O, CaO, Rb/Sr, relatively higher silica and, lower (Al2O3 + FeO + MgO + TiO2 wt%) and Th/Yb as compared to typical S-types. The mantle-hosted granitoids mainly originate from the subducted slab, and mostly intruded mantle peridotite in the lithospheric mantle, with no apparent association with the overriding oceanic plate and little interaction (e.g. assimilation) with the mantle. While the specific controls on geochemical variations remain speculative, results from this study show that the Samail mantle-hosted S-type granitoids are compositionally distinct from classic S-type granitoids formed in orogenic belts. While global S-type granitoids may be mineralogically similar, the Samail mantle-hosted granitoids preserve different geochemical signatures, reflecting their formation in distinct tectonic setting, including the mantle. |
| Keyword | sediment melting supra-subduction zone mantle ophiolite granitoid |
| WOS ID | WOS:000980718300002 |
| Indexed By | SCI |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.gig.ac.cn/handle/344008/74201 |
| Collection | 同位素地球化学国家重点实验室 |
| Corresponding Author | Angelo, Tiago Valim |
| Affiliation | 1.Queens Univ, Dept Geol Sci & Geol Engn, Kingston, ON K7L 3N6, Canada 2.Curtin Univ, Space Sci & Technol Ctr, Sch Earth & Planetary Sci, Perth, WA 6845, Australia 3.Curtin Univ, Inst Geosci Res, Sch Earth & Planetary Sci, Perth, WA 6845, Australia 4.Council Geosci, POB 572, ZA-7535 Bellville, South Africa 5.Chinese Acad Sci, Guangzhou Inst Geochem, State Key Lab Isotope Geochem, Guangzhou 510640, Peoples R China |
| Recommended Citation GB/T 7714 | Angelo, Tiago Valim,Spencer, Christopher J.,Cavosie, Aaron J.,et al. Petrogenesis of Mantle-Hosted Granitoids from the Samail Ophiolite[J]. JOURNAL OF PETROLOGY,2023,64(5):17. |
| APA | Angelo, Tiago Valim,Spencer, Christopher J.,Cavosie, Aaron J.,Thomas, Robert,&Li, Hong-Yan.(2023).Petrogenesis of Mantle-Hosted Granitoids from the Samail Ophiolite.JOURNAL OF PETROLOGY,64(5),17. |
| MLA | Angelo, Tiago Valim,et al."Petrogenesis of Mantle-Hosted Granitoids from the Samail Ophiolite".JOURNAL OF PETROLOGY 64.5(2023):17. |
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