DOI: 10.1007/s00531-016-1342-z
Scopus记录号: 2-s2.0-84973121830
论文题名: Nature and evolution of lithospheric mantle beneath the southern Ethiopian rift zone: evidence from petrology and geochemistry of mantle xenoliths
作者: Alemayehu M. ; Zhang H.-F. ; Sakyi P.A.
刊名: International Journal of Earth Sciences
ISSN: 14373254
出版年: 2017
卷: 106, 期: 3 起始页码: 939
结束页码: 958
语种: 英语
英文关键词: Depletion
; Dillo–Megado
; Enrichment
; Mantle xenoliths
; Sr–Nd–Hf isotopes
Scopus关键词: enrichment
; hafnium
; host rock
; igneous geochemistry
; lithospheric structure
; mantle source
; neodymium isotope
; petrology
; Quaternary
; rift zone
; strontium isotope
; xenolith
; East African Rift
; Ethiopian Rift
英文摘要:
Mantle xenoliths hosted in Quaternary basaltic lavas from the Dillo and Megado areas of the southern Ethiopian rift are investigated to understand the geochemical composition and associated processes occurring in the lithospheric mantle beneath the region. The xenoliths are comprised of predominantly spinel lherzolite with subordinate harzburgite and clinopyroxenite. Fo content of olivine and Cr# of spinel for peridotites from both localities positively correlate and suggest the occurrence of variable degrees of partial melting and melt extraction. The clinopyroxene from lherzolites is both LREE depleted (La/Sm(N) = 0.11–0.37 × Cl) and LREE enriched (La/Sm(N) = 1.88–15.72 × Cl) with flat HREEs (Dy/Lu(N) = 0.96–1.31 × Cl). All clinopyroxene from the harzburgites and clinopyroxenites exhibits LREE-enriched (La/Sm(N) = 2.92–27.63.1 × Cl and, 0.45 and 1.38 × Cl, respectively) patterns with slight fractionation of HREE. The 143Nd/144Nd and 176Hf/177Hf ratios of clinopyroxene from lherzolite range from 0.51291 to 0.51370 and 0.28289 to 0.28385, respectively. Most of the samples define ages of 900 and 500 Ma on Sm–Nd and Lu–Hf reference isochrons, within the age range of Pan-African crustal formation. The initial Nd and Hf isotopic ratios were calculated at 1, 1.5, 2 and 2.5 Ga plot away from the trends defined by MORB, DMM and E-DMM which were determined from southern Ethiopian peridotites, thus indicating that the Dillo and Megado xenoliths could have been produced by melt extraction from the asthenosphere during the Pan-African orogenic event. There is no significant difference in 87Sr/86Sr ratios between the depleted and enriched clinopyroxene. This suggests that the melts that caused the enrichment of the clinopyroxene are mainly derived from the depleted asthenospheric mantle from which the xenoliths are extracted. Largely, the mineralogical and isotopic compositions of the xenoliths show heterogeneity of the CLM that could have been produced from various degrees of melt extraction, followed by metasomatism. © 2016, Springer-Verlag Berlin Heidelberg.
URL: https://www.scopus.com/inward/record.uri?eid=2-s2.0-84973121830&doi=10.1007%2fs00531-016-1342-z&partnerID=40&md5=633650ea177f3454ad89805309bed48b
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资源类型: 期刊论文
标识符: http://119.78.100.158/handle/2HF3EXSE/70047
Appears in Collections: 影响、适应和脆弱性 气候减缓与适应
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作者单位: State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, P.O. Box 9825, Beijing, China; Department of Earth Science, School of Earth Science and Mining Engineering, Addis Ababa Science and Technology University, P.O. Box 16417, Addis Ababa, Ethiopia; State Key Laboratory of Continental Dynamics, Department of Geology, Northwest University, Xi’an, China; Department of Earth Science, University of Ghana, P.O. Box LG 58, Legon-Accra, Ghana
Recommended Citation:
Alemayehu M.,Zhang H.-F.,Sakyi P.A.. Nature and evolution of lithospheric mantle beneath the southern Ethiopian rift zone: evidence from petrology and geochemistry of mantle xenoliths[J]. International Journal of Earth Sciences,2017-01-01,106(3)