日本地球惑星科学連合2016年大会

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セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS01] Outer Solar System Exploration Today, and Tomorrow

2016年5月22日(日) 09:00 〜 10:30 A02 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*木村 淳(東京工業大学地球生命研究所)、藤本 正樹(宇宙航空研究開発機構・宇宙科学研究本部)、笠羽 康正(東北大学大学院 理学研究科 地球物理学専攻)、佐々木 晶(大阪大学大学院理学研究科宇宙地球科学専攻)、谷川 享行(産業医科大学医学部)、関根 康人(東京大学大学院理学系研究科地球惑星科学専攻)、Sayanagi Kunio(Atmospheric and Planetary Sciences Department, Hampton University)、Vance Steven(Jet Propulsion Laboratory, Caltech)、座長:鎌田 俊一(北海道大学 創成研究機構)、藤本 正樹(宇宙航空研究開発機構・宇宙科学研究本部)

09:15 〜 09:30

[PPS01-02] Insulator to electronic conductor transition of synthetic planetary ices at interior conditions of icy giants compressed by laser-driven shock wave

*奥地 拓生1尾崎 典雅2喜田 美佳2小川 剛史2Albertazzi Bruno2宮西 宏併2兒玉 了祐2Purevjav Narangoo1佐野 孝好2坂和 洋一2 (1.岡山大学、2.大阪大学)

キーワード:icy giant planets, laser-driven shock compression, off-Hugoniot conditions, planetary magnetic field

Ices in the universe are consisting of hydrogen, oxygen, carbon, and nitrogen. These elements coalesced to develop into icy giant planets such as Uranus and Neptune in the solar system, as well as some water planets occurring in extrasolar planetary systems. Properties of such planetary ices at elevated pressures and temperatures are essential clues for understanding the layering structures and material circulations inside these giants. Here by using high-power nanosecond laser pulses from GEKKO-XII glass laser at Institute of Laser Engineering at Osaka University, such ices of several compositional types are dynamically compressed, where their equation-of-state (P-V-T) and optical reflectivity (R) are measured at in situ conditions using fast optical diagnostics (Figure). We have successfully observed the transition from insulator to electronic conductor state of the planetary ices which include carbon and/or nitrogen components, as well as that transition of pure H2O ice observed by our previous work [1]. We have also observed the transition at off-Hugoniot conditions using a sample-precompression technique with a diamond anvil cell, which was effectively coupled with laser-driven shock to increase the shock-pressure and to decrease the shock-temperature. These results provide us a new insight about the nature of conducting media inside the icy giants and about the origin of magnetic fields from deep inside of them.
[1] T. Kimura, N. Ozaki, T. Sano, T. Okuchi, et al., J. Chem. Phys., 142, 164504 (2015).