JpGU-AGU Joint Meeting 2017

Presentation information

[JJ] Oral

S (Solid Earth Sciences) » S-GC Geochemistry

[S-GC54] [JJ] Frontiers in Geochemistry

Wed. May 24, 2017 1:45 PM - 3:15 PM 101 (International Conference Hall 1F)

convener:Hiroyuki Kagi(Geochemical Research Center, Graduate School of Science, University of Tokyo), Yusuke Yokoyama(Atmosphere and Ocean Research Institute, University of Tokyo), Shogo Tachibana(Department of Natural History Scieces, Hokkaido University), Chairperson:Hiroyuki Kagi(Geochemical Research Center, Graduate School of Science, University of Tokyo), Chairperson:Yusuke Yokoyama(Atmosphere and Ocean Research Institute, University of Tokyo)

3:00 PM - 3:15 PM

[SGC54-06] In situ neutron diffraction of iron hydride under high pressure and temperature in Fe-silicate-water system: Implications for the Earth's evolution

*Riko Iizuka-Oku1, Takehiko Yagi1, Hirotada Gotou2, Takuo Okuchi3, Takanori Hattori4, Asami Sano-Furukawa4 (1.Geochemical Research Center, Graduate School of Science, The University of Tokyo, 2.The Institute for Solid State Physics, The University of Tokyo , 3.Institute for Planetary Materials, Okayama University, 4.J-PARC Center, Japan Atomic Energy Agency)

Keywords:Hydrogen, Neutron diffraction, In situ high pressure and high temperature observation, Core-mantle formation

Hydrogen is the most abundant element in the solar system and considered to be one of the promising candidates of the light element in the Earth’s core. However, the amount of hydrogen dissolved in the core and its process are still unknown because hydrogen cannot be detected by X-ray and it easily escapes from iron by the release of pressure. In this study, we have conducted high-pressure and high-temperature in-situ neutron diffraction experiments on the iron-hydrous mineral system using high-pressure “PLANET” beamline at J-PARC. We observed that the water which is released from hydrous mineral at about 4 GPa reacts with iron and they form both iron oxide and iron hydride. The obtained iron hydride remained stable after further increase in temperature. This formation of iron hydride occurred below 1000K, at the temperatures where no materials melted. This suggests the possibility that hydrogen had preferentially dissolved into iron before any other light elements have dissolved in the very early stage of Earth’s evolution.