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-IT27] [EE] Carbon in Planetary Interiors

2017年5月23日(火) 15:30 〜 17:00 ポスター会場 (国際展示場 7ホール)

コンビーナ:Craig E Manning(University of California Los Angeles)、大谷 栄治(東北大学大学院理学研究科地学専攻)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、Litasov Konstantin(V.S. Sobolev Institute of Geology and Mineralogy SB RAS)

[SIT27-P05] Existence of Carbon in the Earth’s inner core

Suguru Takahashi1、*Eiji Ohtani1Seiji Kamada2Tatsuya Sakamaki1Naohisa Hirao3 (1.Department of Earth and Planetary Materials Science, Graduate School of Science, Tohoku University、2.Frontier Research Institute of Interdisciplinary Sciences, Tohoku University、3.Japan Synchrotoron Research Institute)

キーワード:Carbon, Fe3C, Melting relation, equation of state, Sound velocity

Carbon is an important candidate for light element in the Earth’s core. There have been contradictory results on the stability of Fe–C compounds, such as Fe3C and Fe7C3 under the core conditions. We observed Fe3C melts incongruently to form Fe7C3 and liquid at 4200 K and 200 GPa, Additionally, it was shown that the C content of the liquid coexisting with Fe7C3 decreases and the Fe–Fe3C eutectic composition shifts toward the Fe-rich direction with increasing pressure. The present result revealed that Fe3C and Fe7C3 are plausible constituents of the inner core, with a possible layering of Fe7C3 in the central region and Fe3C in the outer region of the inner core formed during cooling of the core. We also conducted the equation of state and sound velocity measurements at high pressure and temperature by using XRD and IXS measurements at Spring-8. The results indicate that the sound velocity of the mixture of Fe-Fe3C is higher than the PREM inner core under the Earth’s core conditions. Thus, it is difficult to explain that the Earth’s inner core is composed of only a Fe–Fe3C mixture. Since the inner core temperature is very close to the eutectic temperature of the Fe-Fe3C system, pre-melting effect of Fe3C could be important to account for the sound velocity of the PREM inner core.