Meshesha Daniel, Chekol Takele, Negussia Sileshe
Mineral Exploration, Extraction and Processing Center of Excellence, Addis Ababa Science and Technology University, P.O. Box 16417, Addis Ababa, Ethiopia.
Department of Geology, College of Applied Sciences, Addis Ababa Science and Technology University, P.O. Box 16417, Addis Ababa, Ethiopia.
Heliyon. 2021 Dec 18;7(12):e08634. doi: 10.1016/j.heliyon.2021.e08634. eCollection 2021 Dec.
Major and trace element data are presented for basaltic lavas from western rift margin of central Main Ethiopian Rift located at Kella area to investigate the processes involved in the petrogenesis of the erupted magmas and the nature of mantle source compositions. Kella area is composed of Quaternary (<1.6 Ma), Miocene (10.6-8.3 Ma) and Oligocene basalts (30-29 Ma) ranging from alkaline to tholeiitic in composition. The geochemical variations of basaltic samples from Kella area exhibit two compositionally distinct basaltic groups. The Oligocene tholeiitic basalts display low MgO (5.29-6.11 wt.%), TiO (2.15-2.47 wt.%), PO (0.28-0.34 wt.%), and high ratio of CaO/AlO (0.68-0.72) and La/Nb (0.89-1.10). Whereas Quaternary and Miocene alkaline basalts display high MgO (7.40-8.86 wt.%), TiO (2.4-2.53 wt.%), PO (0.44-0.52 wt.%) and low ratio of CaO/AlO (0.62-0.66) and La/Nb (0.71-0.76). The contrasting incompatible element ratios (e.g., K/Nb, La/Nb, Rb/Zr and Zr/Nb) between tholeiite and alkaline basalts reflect differences in their mantle sources. Major and trace element variations, therefore, reflect the involvement of two geochemically distinct mantle sources in the petrogenesis of Kella basaltic lavas: i) the Oligocene tholeiite basaltic melts derived from enriched asthenosphere mantle source (E-MORB) and ii) the Miocene and Quaternary alkali basaltic melts show a close similarity with ocean island basalts (OIBs) geochemistry, and this end member ascribed to the arrival of Afar plume head. The geochemical modeling reveals that the Oligocene tholeiite basaltic melts produced by an equilibrium melting with 3-5 % degree of partial melting in spinel lherzolite mantle source, whereas the alkali basalts were produced with ∼2% degree of partial melting within spinel-garnet lherzolite transition zone mantle sources.
本文给出了位于凯拉地区的埃塞俄比亚主裂谷中部西裂谷边缘玄武质熔岩的主量和微量元素数据,以研究喷发岩浆的岩石成因过程以及地幔源区成分的性质。凯拉地区由第四纪(<1.6 Ma)、中新世(10.6 - 8.3 Ma)和渐新世玄武岩(30 - 29 Ma)组成,成分从碱性到拉斑玄武质。凯拉地区玄武岩样品的地球化学变化显示出两个成分不同的玄武岩组。渐新世拉斑玄武岩具有低MgO(5.29 - 6.11 wt.%)、TiO(2.15 - 2.47 wt.%)、PO(0.28 - 0.34 wt.%),以及高CaO/AlO比值(0.68 - 0.72)和La/Nb比值(0.89 - 1.10)。而第四纪和中新世碱性玄武岩具有高MgO(7.40 - 8.86 wt.%)、TiO(2.4 - 2.53 wt.%)、PO(0.44 - 0.52 wt.%),以及低CaO/AlO比值(0.62 - 0.66)和La/Nb比值(0.71 - 0.76)。拉斑玄武岩和碱性玄武岩之间不相容元素比值(如K/Nb、La/Nb、Rb/Zr和Zr/Nb)的差异反映了它们地幔源区的不同。因此,主量和微量元素的变化反映了两种地球化学性质不同的地幔源区参与了凯拉玄武质熔岩的岩石成因:i)渐新世拉斑玄武质熔体源自富集软流圈地幔源区(E - MORB),ii)中新世和第四纪碱性玄武质熔体在地球化学上与洋岛玄武岩(OIBs)相似,这种端元成分归因于阿法尔地幔柱头部的到来。地球化学模拟表明,渐新世拉斑玄武质熔体是由尖晶石二辉橄榄岩地幔源区以3 - 5%的部分熔融程度平衡熔融产生的,而碱性玄武岩是在尖晶石 - 石榴石二辉橄榄岩过渡带地幔源区内以约2%的部分熔融程度产生的。