日本地球惑星科学連合2022年大会

講演情報

[E] 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-IT21] 惑星中心核:内部構造・形成・進化

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (23) (Ch.23)

コンビーナ:寺崎 英紀(岡山大学理学部)、コンビーナ:大谷 栄治(東北大学大学院理学研究科地学専攻)、McDonough William F(Department of Earth Science and Research Center for Neutrino Science, Tohoku University, Sendai, Miyagi 980-8578, Japan)、コンビーナ:飯塚 理子(東京大学大学院理学系研究科地殻化学実験施設)、座長:寺崎 英紀(岡山大学理学部)、大谷 栄治(東北大学大学院理学研究科地学専攻)、William F McDonough(Department of Earth Science and Research Center for Neutrino Science, Tohoku University, Sendai, Miyagi 980-8578, Japan)、飯塚 理子(東京大学大学院理学系研究科地殻化学実験施設)


11:00 〜 13:00

[SIT21-P03] Test of density measurement using X-ray absorption method combined laser-heated diamond anvil cell

*鶴岡 椋1寺崎 英紀2、紙名 宏幸2鎌田 誠司3,4近藤 忠1米田 明1、平尾 直久5、河口 沙織5 (1.大阪大学大学院理学研究科宇宙地球科学専攻、2.岡山大学大学院自然科学研究科地球科学専攻、3.東北大学学際科学フロンティア研究所、4.(株)アド・サイエンス、5.高輝度光科学研究センター)

キーワード:X線吸収法、密度、レーザー加熱式ダイヤモンドアンビルセル

Density measurement of liquid iron alloy is important to understand the planetary liquid core.
The X-ray absorption method is an effective method because it can directly determine the liquid density. We have been developing the X-ray absorption method combined with a laser-heated diamond anvil cell (DAC), and performed test measurements using Fe3C as a solid sample.

In X-ray absorption method, density of sample was obtained from measured incident and transmitted X-ray intensities of the samples using Lambert-Beer law. Fe3C sample and reference material (Ni) were loaded into each hole drilled on a pre-indented Re gasket. Al2O3 single crystal was used as pressure medium. High pressure was generated using a symmetric cell with a lever-arm frame. High temperature was generated using laser heating system. X-ray absorption measurements were conducted with monochromatic X-ray of 30 keV at BL10XU beamline in Spring-8.

The X-ray intensities of samples were measured up to 10 GPa and 1700 K. The ratio of incident and transmitted X-ray changes 0.3% from 300 K to 1700 K. The thickness of the sample was determined as 10um from X-ray intensities after quench.