日本地球惑星科学連合2016年大会

講演情報

インターナショナルセッション(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-IT07] Structure and dynamics of Earth and Planetary deep interiors

2016年5月22日(日) 13:45 〜 15:15 201B (2F)

コンビーナ:*芳野 極(岡山大学地球物質科学研究センター)、趙 大鵬(東北大学大学院理学研究科附属地震・噴火予知研究観測センター)、中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)、座長:Kono Yoshio(Carnegie Institution for Science Washington)、亀山 真典(国立大学法人愛媛大学地球深部ダイナミクス研究センター)

14:30 〜 14:45

[SIT07-16] Three-dimensional mantle convection and material cycling with continental dispersal and coalescence

*柳 竜之介1吉田 晶樹2 (1.東京工業大学、2.JAMSTEC)

キーワード:continental dispersal and coalescence, material cycling

The Earth is unique among the solar terrestrial planets, having the continents and the abundant liquid water on its surface. In this study, we have developed a three-dimensional mantle convection model that incorporates these two features into the numerical program, and investigate how the flow-temperature field and water distribution occur under the circumstances of continental dispersal and coalescence. In this numerical simulation of 3-D spherical mantle convection, supercontinent is introduced in the model set up in order to study how continental dispersal and coalescence happens and affect the structures of the interior. In addition, water is also introduced, considering water solubility of mantle rocks. The results show that water is transported to broader regions effectively once continental dispersal occurred, due to enhanced flow velocity associated with increased horizontal temperature gradient partly with the blanketing effect beneath the supercontinent. This process distributes the water in a spatially wide region as a “migrating entrance” of water into the mantle. Once the water subducts with the cold down-going flow and reaches CMB (core mantle boundary), then it horizontally spreads to be heated up. In some case, dehydration of Phase H may occur to generate a fluid that migrates upward and hydrate the overlying mantle, which occurs near the boundary between the cold continental domain and the warmer oceanic domain, yet within the hydrated cold domain beneath the (super)continent region. This mechanism, together with the near-surface process described above, may create a hydrous domain beneath the continental region where a rather uniform hydration may prevail. Therefore, the effective redistribution with a global scale structure can be created simultaneously. Such a mechanism could be important to account for the observed geochemical mantle hemispheres.