日本地球惑星科学連合2018年大会

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[EE] 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-PS02] Regolith Science

2018年5月22日(火) 09:00 〜 10:30 A02 (東京ベイ幕張ホール)

コンビーナ:和田 浩二(千葉工業大学惑星探査研究センター)、中村 昭子(神戸大学大学院理学研究科地球惑星科学専攻)、Patrick Michel(共同)、Kevin John Walsh (Southwest Research Institute Boulder)、座長:中村 昭子(Graduate School of Science, Kobe University)

09:15 〜 09:30

[PPS02-02] 硫黄による宇宙風化作用の強化

*佐々木 晶1田中 宏和1岡崎 瑞祈1三宅 亮2土山 明2 (1.大阪大学大学院理学研究科宇宙地球科学専攻、2.京都大学大学院理学研究科地球惑星科学専攻)

キーワード:宇宙風化作用、レゴリス熟成度、微小隕石、硫黄、硫化鉄、反射率の低下

Space weathering should control the change of brightness and color of the surface regolith of airless silicate bodies: optical darkening, reddening and weakening of absorption bands. Formation of nanophase iron particles through solar wind implantation or micrometeorite bombardments is the cause of the optical property changes of the space weathering. A small S-type asteroid Itokawa, which was observed by HAYABUSA spacecraft has weakly weathered LL5/6 spectrum, which was confirmed by detailed analyses of returned samples. The returned samples contain not only nanophase iron but also nanophase FeS (and MgS) particles play some role in space weathering.



In the present study, we conducted laboratory simulation experiments using nano-second pulse laser irradiation simulating high-speed micrometeorite impacts, and found that additional FeS (45-75µm, 10wt%) as well as additional Fe should promote optical change compatible with space weathering, especially darkening of infrared spectra of olivine. We observed laser-irradiated sample by TEM. The amorphous layer about 200 nm thickness is formed around an olivine particle. Abundant nano particles are observed both at the bottom and the surface of the amorphous layer. On the basis of lattice parameters, we confirmed nano Fe particles but we did not find nano FeS particles. There is possibility that additional FeS promoted production of nanophase iron particles, which would have enhanced the space weathering effect. We also tried preliminary experiments with addition of pure sulfur particles (45-75µm, 10wt%) instead of FeS particles. We observed small change of reflectance after pulse laser irradiation which is less significant compared with the case of additional FeS. We have started very preliminary experiments using FeS2, which may enhance the spectral darkening and reddening as FeS.