日本地球惑星科学連合2022年大会

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[E] 口頭発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT18] GEOPHYSICAL PROPERTIES AND TRANSPORT PROCESSES IN THE DEEP CRUST AND MANTLE

2022年5月23日(月) 09:00 〜 10:30 102 (幕張メッセ国際会議場)

コンビーナ:Bjorn Mysen(Geophysical Laboratory, Carnegie Inst. Washington)、コンビーナ:大谷 栄治(東北大学大学院理学研究科地学専攻)、高橋 菜緒子(東北大学大学院理学研究科)、コンビーナ:北 佐枝子(建築研究所)、座長:大谷 栄治(東北大学大学院理学研究科地学専攻)、高橋 直樹(千葉県立中央博物館)


09:45 〜 10:00

[SIT18-04] Garnet pyroxenites explain high electrical conductivity in the East African deep lithosphere

*Thomas P. Ferrand1、Emily J. Chin2 (1.Institut für Geologische Wissenschaften, Freie Universität Berlin, Berlin 12249, Germany、2.Geosciences Research Division, Scripps Institution of Oceanography, UC San Diego, La Jolla, USA)

キーワード:Tanzanian craton, Lithospheric mantle, Electrical conductivity, Grain-boundary network, Garnet pyroxenite, Hydrogarnet

In Tanzania, the deep lithospheric mantle (>70 km depth) is characterized by significantly higher electrical conductivity within the cratonic root than in the Mozambique belt. Such contrasts are typically attributed to changes in volatiles and/or melt content, with changes in mineralogy deemed insufficient to impact conductivity. To test this assumption, electrical conductivity measurements were conducted at pressure-temperature conditions relevant to the Tanzanian lithosphere (1.5 and 3 GPa; from 400 to >1500°C) on xenoliths from Engorora, Northern Tanzania. Once garnet becomes stable in fertile mantle rocks (>60 km, 1.7 GPa), it nucleates at grain boundaries, forming the backbone of a conductive network. At 3 GPa, such garnet-rich networks increase conductivity by a factor of 100 regardless of temperature. Numerical models demonstrate that the observed low (<10-2 Sm-1) and high (>10-1 Sm-1) conductivity values are best explained by low and high degrees of garnet connectivity, respectively. Such high electrical conductivities in cratonic roots can be explained by the presence of connected garnet clusters or garnet pyroxenites, suggesting mantle refertilization. Our results are consistent with long-term craton stability, but the garnet-rich network likely results from metasomatism due to plume impingement and may represent an unstable structure prior to loss of cratonic lithosphere.