JpGU-AGU Joint Meeting 2017

講演情報

[EE] ポスター発表

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-IT23] [EE] Structure and Dynamics of Earth and Planetary Mantles

2017年5月22日(月) 15:30 〜 17:00 ポスター会場 (国際展示場 7ホール)

コンビーナ:中川 貴司(海洋研究開発機構数理科学・先端技術研究分野)、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)、芳野 極(岡山大学惑星物質研究所)

[SIT23-P01] Compositional layering within the Large Low Shear-wave Velocity Provinces in the lower mantle

*Maxim Ballmer1,2Lina Schumacher3Vedran Lekic4Christine Thomas3Garrett Ito5 (1.Institut für Geophysik, Departement für Erdwissenschaften, ETH Zürich, 8092 Zürich, Switzerland、2.Earth-Life Science Institute, Tokyo Institute of Technology, Meguro, Tokyo 152-8551, Japan、3.Institut für Geophysik, Westfälische Wilhelms Universität Münster, 48149 Münster, Germany、4.Department of Geology, University of Maryland, College Park, MD 20742, USA、5.School of Ocean and Earth Sciences and Technology, University of Hawai‘i at Manoa, Honolulu, HI 96822, USA)

キーワード:Mantle Convection, Primordial Reservoir

The large low shear-wave velocity provinces (LLSVP) are thermochemical anomalies in the deep Earth’s mantle, thousands of km wide and ~1,800 km high. This study explores the hypothesis that the LLSVPs are compositionally subdivided into two domains: a primordial bottom domain near the core-mantle boundary and a basaltic shallow domain extending from 1,100~2,300 km depth. This hypothesis reconciles published observations in that it predicts that the two domains have different physical properties (bulk-sound vs. shear-wave speed vs. density anomalies), the transition in seismic velocities separating them is abrupt, and both domains remain seismically distinct from the ambient mantle. We here report underside reflections from the top of the LLSVP shallow domain, supporting a compositional origin. By exploring a suite of two-dimensional geodynamic models, we constrain the conditions under which well-separated “double-layered” piles with realistic geometry can persist for billions of years. Results show that long-term separation requires density differences of ~100 kg/m3 between LLSVP materials, providing a constraint for origin and composition. The models further predict short-lived “secondary” plumelets to rise from LLSVP roofs and to entrain basaltic material that has evolved in the lower mantle. Long-lived, vigorous “primary” plumes instead rise from LLSVP margins and entrain a mix of materials, including small fractions of primordial material. These predictions are consistent with the locations of hotspots relative to LLSVPs, and address the geochemical and geochronological record of (oceanic) hotspot volcanism. The study of large-scale heterogeneity within LLSVPs has important implications for our understanding of the evolution and composition of the mantle.