日本地球惑星科学連合2015年大会

講演情報

口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS22] 太陽系における惑星物質の形成と進化

2015年5月28日(木) 16:15 〜 18:00 A02 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*伊藤 正一(京都大学大学院理学研究科)、臼井 寛裕(東京工業大学地球惑星科学科)、瀬戸 雄介(神戸大学大学院理学研究科)、宮原 正明(広島大学理学研究科地球惑星システム学専攻)、木村 眞(茨城大学理学部)、大谷 栄治(東北大学大学院理学研究科地学専攻)、三浦 均(名古屋市立大学大学院システム自然科学研究科)、薮田 ひかる(大阪大学大学院理学研究科宇宙地球科学専攻)、座長:臼井 寛裕(東京工業大学地球惑星科学科)

16:30 〜 16:45

[PPS22-21] 衝撃を受けた隕石中のメージャーライトガーネットの対称性

*富岡 尚敬1宮原 正明2伊藤 元雄1 (1.海洋研究開発機構高知コア研究所、2.広島大学理学研究科地球惑星システム学専攻)

キーワード:メージャーライト, 衝撃変成, 高圧相転移, TEM

Majorite is a garnet-structured mineral with a composition on the join (Mg,Fe)SiO3-(Mg,Fe)3Al2Si3O12, which contains Si in the octahedral sites. Al-free majorite samples synthesized by Kawai-type multianvil apparatus are known to have a tetragonal symmetry (space group I41/a) [1]. However, all of natural Al-free majorite samples found in shocked chondrites have been reported to be cubic (Ia-3d) [2]. Single-crystal X-ray study of a synthetic MgSiO3 majorite clarified the tetragonal distortion of majorite is caused by Mg-Si ordering in the octahedral sites [3]. Subsequent microstructural observations of synthetic Al-free majorite by TEM concluded that the tetragonal phase is formed from the cubic phase through the cation ordering even upon rapid quenching (103 ℃/sec) and the symmetry reduction phase derives modulated and twinning structures [4]. On the contrary, cubic (Mg,Fe)SiO3 majorite in shocked chondrites is inferred to have been preserved due to higher cooling rate than that in high-pressure synthesis where the cation ordering is inhibited.
Due to very small tetragonal distortion from the cubic phase (c/a = 0.99) and very week extra reflections for the tetragonal phase, it is difficult to judge the symmetry of small amount of natural majorite samples by powder X-ray diffractometry. For the symmetry analyses of submicron-sized grains, single-crystal electron diffraction is a suitable method, since the intensities of weak reflections to diagnose the tetragonal symmetry are enhanced by the effect of dynamical diffraction. In this study, we revisit symmetries of majorite grains in shocked ordinary chondrites (Tenham; L6, Y-75100; H6) and also synthetic (Mg,Fe)SiO3 majorite by TEM. The intensity of {101} reflections, which appears only for the I41/a tetragonal phase, is under investigation by selected are electron diffraction.

References:
[1] e.g. Kato, T., and Kumazawa, M. (1985) Garnet phase of MgSiO3 filling the pyroxene-ilmenite gap at very high temperature. Nature, 316, 803-805.
[2] e.g. Smith, J.V., and Mason, B. (1970) Pyroxene-garnet transformation in Coorara meteorite. Science, 168, 832-833; Jeanloz, R. (1981) Majorite: Vibrational and compressional properties of a high-pressure phase. J. Geophys. Res., 86, 6171-6179.
[3] Angel, R.J., Finger, L.W., Hazen, R.M., Kanzaki, M., Weidner, D.J., Liebermann, R.C., Veblen, D. R. (1989) Structure and twinning of single-crystal MgSiO3 garnet synthesized at 17 GPa and 1800 ℃. Amer. Mineral., 74, 509-512.
[4] e.g. Heinemann, S., Sharp, T.G., Seifert, F., and Rubie, D.C. (1997) The cubic-tetragonal phase transition in the system majorite (Mg4Si4O12) - pyrope (Mg3Al2Si3O12), and garnet symmetry in the Earth's transition zone. Phys. Chem. Minerals, 24, 206-221.; Tomioka, N., Fujino, K., Ito, E., Katsura, T., Sharp, T., and Kato, T. (2002) Microstructures and structural phase transition in (Mg,Fe)SiO3 majorite. Eur. J. Mineral., 14, 7-14.