IAG-IASPEI 2017

講演情報

Oral

IASPEI Symposia » S15. Mid-mantle structure

[S15-1] Structure and dynamics of the mid mantle

2017年8月2日(水) 13:30 〜 15:00 Room 402 (Kobe International Conference Center 4F, Room 402)

Chairs: Christine Houser (Tokyo Institute of Technology) , Nicholas Schmerr (University of Maryland)

13:30 〜 14:00

[S15-1-01] First principles investigation of the high-pressure behavior of the FeOOH-AlOOH-phase H (MgSiO4H2) system

Jun Tsuchiya1, 4, Elizabeth C. Thompson2, Taku Tsuchiya1,4, Masayuki Nishi1,4, Yasuhiro Kuwayama3 (1.Ehime University, Matsuyama, Ehime, Japan, 2.University of Chicago, Chicago, IL, United States, 3.The University of Tokyo, Tokyo, Japan, 4.Earth-Life Science Institute-Ehime Satellite (ELSI-ES), Matsuyama, Ehime, Japan)

invited

It is believed that water is carried into the Earth's deep interior by hydrous minerals such as dense hydrous magnesium silicates (DHMSs) in the descending cold plate. A number of studies have been conducted to determine the high-pressure behaviors of DHMSs. In recent years, we discovered a new DHMS, phase H, stable at lower mantle pressure condition; and the solid solution formed by phase H and delta-AlOOH has been proposed as the most important carrier of water to the deepest part of Earth's mantle (Tsuchiya 2013, Nishi et al. 2014, Ohira et al. 2014). However, those hydrous phases are not denser than surrounding (dry) mantle minerals (Tsuchiya and Mookherjee 2015) and their gravitational stability in deeper part of the Earth is questionable. Therefore, the effect of denser elements such as Fe on the stability of DHMS is intrinsically connected to the ability of these phases to transport water into Earth's deep interior. In order to assess the effect of Fe on the phase relation of phase H and delta-AlOOH, we determined the high-pressure behavior of the end-member composition of this system, epsilon-FeOOH. We have discovered a new high-pressure phase transition in FeOOH at lower mantle conditions using both theoretical and experimental methods. Here we show the high-pressure structures and physical properties of the FeOOH-AlOOH-phase H system using first principles calculation and discuss possible geophysical implications.