中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Petrogenesis of Mantle-Hosted Granitoids from the Samail Ophiolite

文献类型:期刊论文

作者Angelo, Tiago Valim2; Spencer, Christopher J.2; Cavosie, Aaron J.3,4; Thomas, Robert5; Li, Hong-Yan1
刊名JOURNAL OF PETROLOGY
出版日期2023-05-01
卷号64期号:5页码:17
关键词sediment melting supra-subduction zone mantle ophiolite granitoid
ISSN号0022-3530
DOI10.1093/petrology/egad021
英文摘要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.
WOS研究方向Geochemistry & Geophysics
语种英语
WOS记录号WOS:000980718300002
源URL[http://ir.gig.ac.cn/handle/344008/74200]  
专题同位素地球化学国家重点实验室
通讯作者Angelo, Tiago Valim
作者单位1.Chinese Acad Sci, Guangzhou Inst Geochem, State Key Lab Isotope Geochem, Guangzhou 510640, Peoples R China
2.Queens Univ, Dept Geol Sci & Geol Engn, Kingston, ON K7L 3N6, Canada
3.Curtin Univ, Space Sci & Technol Ctr, Sch Earth & Planetary Sci, Perth, WA 6845, Australia
4.Curtin Univ, Inst Geosci Res, Sch Earth & Planetary Sci, Perth, WA 6845, Australia
5.Council Geosci, POB 572, ZA-7535 Bellville, South Africa
推荐引用方式
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.

入库方式: OAI收割

来源:广州地球化学研究所

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。