沙特阿拉伯西北部Harrat Ash Shaam (Al Harrah)中新世-第四纪陆相玄武岩的岩石成因与演化

IF 2.9 2区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Shelby Bowden , Tanya Furman , David W. Graham , Mansour Alhumimidi , Willis Hames , Ali Assiri , Mazen Alyousif , Ramzi Almutairi , Hamad Alqahtani , Abdurahman Bin Rogaib , Abdulaziz Bin Rushood , Khaled AlYousef , Sultan Alkhammali
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引用次数: 0

摘要

Harrat Ash Shaam中新世—新近玄武岩的地球化学组成记录了沙特阿拉伯北部次大陆岩石圈地幔响应区域构造的时空演化。HAS熔岩表现出两期明显的岩浆活动:(1)广泛分布的渐新世/早中新世至中新世中形成高原的喷涌式亚碱性玄武岩;(2)晚中新世的历史原始碱性玄武岩,由叠加在现有火山高原上的单成因煤渣锥喷发而成。地球化学证据表明,源区矿物学由中新世早期的尖晶石橄榄岩/辉石岩(含少量水相(角闪孔/辉云岩))向第四纪的石榴石橄榄岩/辉石岩(含丰富的角闪孔和辉云岩)转变。第四纪(1至5 GPa,≈1300-1500°C)和中新世/上新世(1至3 GPa,≈1250-1400°C)熔岩的熔体平衡压力和温度,加上稀土元素的证据(例如,第四纪的Tb/Ybn = 3.7,中新世的为2.6),表明熔体区域随着时间的推移而加深。橄榄石3He/4He比值在6 ~ 9 RA之间,不需要深部地幔柱的贡献;我们认为早中新世玄武岩的成因涉及软流圈熔体的贡献。新生代HAS火山岩的成岩作用分两个阶段。渐新世至中中新世岩浆形成于岩石圈和次岩石圈地幔绝热熔融过程中,与阿兹拉克-锡尔罕地堑在阿拉伯半岛的广泛伸展运动有关。晚中新世到现在的岩浆活动可能是由不稳定的(致密的、交代的)岩石圈沉降到下伏的软流圈,引发岩石圈和软流圈的融化,这是在沿着死海断层的构造运动之后和同时发生的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Petrogenesis and evolution of Miocene-Quaternary continental basalts at Harrat Ash Shaam (Al Harrah), NW Saudi Arabia
The geochemical compositions of Miocene-recent basalts from Harrat Ash Shaam (HAS) contain a record of the temporal and spatial evolution of the subcontinental lithospheric mantle in response to regional tectonics in northern Saudi Arabia. HAS lavas show two distinct episodes of magmatism: (1) widespread Oligocene/early-Miocene through mid-Miocene effusive, plateau-forming subalkaline basalts and (2) Late-Miocene through historic primitive alkaline basalts erupted from monogenetic cinder cones superimposed on the existing volcanic plateau. Geochemical evidence indicates a change in the source region mineralogy from spinel peridotite/pyroxenite with minor amounts of hydrous phases (amphibole/phlogopite) in the early Miocene to garnet peridotite/pyroxenite with abundant amphibole and phlogopite in the Quaternary. Melt equilibration pressures and temperatures in Quaternary (1 to >5 GPa, 1300–1500 C) and Miocene/Pliocene (<1 to 3 GPa, 1250–1400 C) lavas, plus REE evidence (e.g., Tb/Ybn = 3.7 in the Quaternary vs. 2.6 in the Miocene), suggest a deepening of the melt region through time. Olivine 3He/4He ratios range from 6 to 9 RA and do not require contributions from a deep-seated mantle plume; we suggest that genesis of the older Miocene basalts involved contributions of melt from the asthenosphere. Petrogenesis of Cenozoic HAS lavas occurred in two stages. Oligocene through mid-Miocene magmas formed from adiabatic melting of lithospheric and sub-lithospheric mantle associated with movement along the Azraq-Sirhan Graben during widespread extension across the Arabian Peninsula. Late-Miocene through present day magmatism was likely triggered by foundering of unstable (dense, metasomatized) lithosphere into the underlying asthenosphere, triggering lithospheric and asthenospheric melting subsequent to and coeval with tectonic movement along the Dead Sea Fault.
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来源期刊
Lithos
Lithos 地学-地球化学与地球物理
CiteScore
6.80
自引率
11.40%
发文量
286
审稿时长
3.5 months
期刊介绍: Lithos publishes original research papers on the petrology, geochemistry and petrogenesis of igneous and metamorphic rocks. Papers on mineralogy/mineral physics related to petrology and petrogenetic problems are also welcomed.
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