日本地球惑星科学連合2023年大会

講演情報

[E] オンラインポスター発表

セッション記号 S (固体地球科学) » S-CG 固体地球科学複合領域・一般

[S-CG47] ハードロック掘削科学:陸上・深海底掘削、そしてオフィオライト

2023年5月24日(水) 15:30 〜 17:00 オンラインポスターZoom会場 (4) (オンラインポスター)

コンビーナ:星出 隆志(秋田大学国際資源学部)、針金 由美子(産業技術総合研究所)、高澤 栄一(新潟大学理学部理学科地質科学科プログラム)、道林 克禎(名古屋大学 大学院環境学研究科 地球環境科学専攻 地質・地球生物学講座 岩石鉱物学研究室)

現地ポスター発表開催日時 (2023/5/23 17:15-18:45)

15:30 〜 17:00

[SCG47-P02] Relationship between the ultramafic complex and boninite in the Salahi block, the Oman ophiolite

*藤野 珠妃1高澤 栄一1,2 (1.新潟大学理学部理学科地質科学プログラム、2.国立研究開発法人海洋開発研究機構)

キーワード:オマーンオフィオライト、超苦鉄質複合岩体、ボニナイト

Oman ophiolite is the world's largest ophiolite, located at the eastern tip of the Arabian Peninsula, and is thought to be an ophiolite transformed from spreading ridge to subduction zone setting (Umino et al., 1990; Arai et al., 2006). The ultramafic complex consisting of peridotites and pyroxenites exists in the basal part of the Salahi mantle section, located in the northern part of Oman ophiolite. This peridotite contains spinel with high Cr# (=Cr/[Cr+Al] atomic ratio). In particular, the spinel in dunite has a composition similar to that of spinel in boninite, and is compositionally different from the spinel in the peridotite that forms the main part of the Salahi mantle section and the Moho Transition Zone. During the formation of the subduction zone, fluids liberated from the metamorphic sole entered the mantle section and reacted with the residual harzburigte to form boninite as well as high Cr# spinel-bearing dunite as the residue (Nomoto and Takazawa, 2013).
Therefore, the purpose of this study is to clarify how peridotites and pyroxenites, including the ultramafic complex dunite, are related to boninite formation. This will lead to a better understanding of melt formation and reaction with mantle peridotites in subduction zone environment. The main subjects of the study were dunite, harzburgite, wehrlite, pyroxenites, and boninite. In addition, boninite data from Ishikawa et al (2005), Kusano et al (2014), and Yamazaki (2013MS) are used for comparison. We conducted observation of thin sections under polarized-microscope, major elemental analysis (spinel, olivine, clinopyroxene and orthopyroxene) using SEM-EDS and trace element analysis of clinopyroxene using LA-ICP-MS.
The dunites in the ultramafic complex have similarities to forearc peridotites and boninites with respect to spinel composition, as well as some that are inferred to be cumulate crystallized from a melt. Wehrlite, orthopyroxenite, and some harzburgite also have similarities to boninite in the Cr#, Mg# (=Mg/[Mg+Fe]), and TiO2 compositions of spinel. Magma produced by flux melting of lherzolite was saturated with olivine and clinopyroxene, which may have crystallized wehrlite and pyroxenite to form boninite magma. In this case, dunite and harzburigte in the ultramafic complex are considered to be residues produced by flux melting of lherzolite.
Clinopyroxene phenocrysts in boninites show LREE-depleted chondrite-normalized REE pattern. Clinopyroxenes in dunite, wehrlite, clinopyroxenite, orthopyroxenite and some harzburgite have REE patterns similar to those of boninite. The deference in spinel Cr# observed in these rocks are due to a difference in the degree of melting for producing primary boninite magma in equilibrium with harzburgite and dunite. Therefore, the entire rocks in the ultramafic complex is considered to be genetically related to boninite. In addition, wehrlite, pyroxenites were formed by crystal differentiation from primary boninite magma.