Japan Geoscience Union Meeting 2014

Presentation information

Oral

Symbol S (Solid Earth Sciences) » S-IT Science of the Earth's Interior & Techtonophysics

[S-IT39_2AM2] Deep Earth science: Dynamics of plate, mantle, and core

Fri. May 2, 2014 11:00 AM - 12:45 PM 416 (4F)

Convener:*Shingo Watada(Ocean Hemisphere Research Center, Earthquake Research Institute, University of Tokyo), Takeshi Sakai(Geodynamics Research Center, Ehime University), Takashi Nakagawa(JAMSTEC/IFREE), Chair:Kenji Kawai(Department of Earth and Planetary Sciences, Tokyo Institute of Technology)

11:45 AM - 12:00 PM

[SIT39-11] Simultaneous measurement of liquid Fe-C density and sound velocity at high pressure

*Yuta SHIMOYAMA1, Hidenori TERASAKI1, Yusaku TAKUBO1, Satoru URAKAWA2, Souma KUWABARA1, Yoshinori KATAYAMA3 (1.Graduate School of Science, Osaka University, 2.Department of Earth Sciences, Okayama University, 3.Japan Atomic Energy Agency)

Keywords:Density, Sound velocity, liquid Fe-C

The cores of terrestrial planets, such as Mercury, Mars and Moon are considered to contain some light elements. The effect of light elements on density and bulk modulus of liquid iron is necessary for estimating of these core compositions. Sound velocity of liquid iron alloys is also important for identifying light elements in the core by comparison with observed seismic data.In this study, we have measured density and sound velocity of liquid Fe-C at SPring-8 beamline BL22XU. Density was measured using X-ray absorption method (Katayama et al., 1993) and sound velocity was measured using pulse-echo overlapping method (Higo et al., 2009). Experimental conditions were 1.2-2.9 GPa and 1650-1850 K. Obtained density values of this study were consistent with our previous results (Shimoyama et al., 2013). In sound velocity measurement, we could observe clear sample wave signal. Measured compressional wave velocity of liquid Fe-C was found to increase with pressure.