惑星分光観測衛星プロジェクトチーム

金丸 礼

カネマル レイ  (Rei Kanemaru)

基本情報

所属
国立研究開発法人宇宙航空研究開発機構 宇宙科学研究所 研究開発員
学位
博士(理学)(2021年9月 総合研究大学院大学 複合科学研究科 極域科学専攻)
学士(2016年3月 岡山理科大学 生物地球学部 生物地球学科)

研究者番号
20961296
ORCID ID
 https://orcid.org/0000-0002-3624-0458
J-GLOBAL ID
202301009651096753
researchmap会員ID
R000062029

受賞

 1

主要な論文

 13
  • Kanemaru Rei, Yamaguchi Akira, Sekine Toshimori, Imae Naoya, Nishido Hirotsugu, Kobayashi Takamichi
    Journal of Mineralogical and Petrological Sciences advpub 2024年6月13日  査読有り筆頭著者責任著者
    We performed a cathodoluminescence (CL) study of Ca-rich plagioclase (An85-86Ab14Or<1) in Stillwater gabbronorite experimentally shocked at 20.1, 29.8, and ∼41 GPa, for characterization of the shock effects. Chroma CL image of unshocked plagioclase showed the homogeneous red CL emission. In contrast, experimentally shocked plagioclase showed the heterogeneous CL emission colors in red and blue. The Raman spectra analysis identified that the red and blue portions correspond to plagioclase and maskelynite, respectively. In our observation, plagioclase experimentally shocked at 20 GPa was partially converted into maskelynite. At 30 GPa, most of plagioclase were converted into maskelynite. At 40 GPa, plagioclase was fully converted into maskelynite. Our observations of Ca-rich plagioclase indicated that the maskelynization starts at a slightly lower pressure and completes at a higher pressure than those in the previous studies (∼24 GPa and ∼28 GPa, respectively). These pressure differences may be due to the high sensitivity of CL, which allows for the detection of small (a few µm in size) and rare phases that may have been overlooked in the traditional methods. The CL spectra of plagioclase showed a continuous change with increasing shock pressure. Hence, the CL imaging method using plagioclase and maskelynite is found to be very effective to estimate precisely shock pressure. In particular, there was a marked decrease in the CL intensity of Mn2+ and Fe3+ centers. Furthermore, the shock-induced center around the UV region was observed in experimentally shocked plagioclase and maskelynite. These CL features reflect the destruction of the framework structure to varying extents depending upon shock pressure. Combined with the FTIR analysis in the present study, the transition of plagioclase to maskelynite was clearly illustrated in spectra. The reflectivity decreased continuously with increasing shock pressures during maskelynization. Additionally, the absorption at ∼8.6 µm observed in plagioclase was absent in maskelynite. This feature can be used as a diagnostic feature to characterize plagioclase and maskelynite by FTIR. The combination of detailed petrology using CL and FTIR spectra provides valuable insights into the shock scale for achondrites and planetary materials rich in shock-experienced plagioclase.
  • 金丸 礼, 矢田 達, 田原 瑠衣, 中山 悠, 深井 稜汰, 畠田 健太朗, 石崎 拓也, 榎戸 祐馬, 小野寺 圭祐, 保田 慶直, 西村 征洋, 坂本 佳奈子, 人見 勇矢, 副島 広道, 熊谷 和也, 小嶋 智子, 安部 正真, 岡田 達明, 臼井 寛裕
    遊・星・人 33(1) 78-86 2024年3月  筆頭著者責任著者
  • Rei Kanemaru, Kazuya Kumagai, Hiromichi Soejima, Toru Yada, Masahiro Nishimura, Masanao Abe, Tatsuaki Okada, Kasumi Yogata, Kanako Sakamoto, Akiko Miyazaki, Kana Nagashima, Rui Tahara, Arisa Nakano, Tomoko Ojima, Ryota Fukai, Takuya Ishizaki, Kentaro Hatakeda, Yuya Hitomi, Yuka Sugiyama, Ayako Nakata, Yuma Enokido, Haruna Sugahara, Shino Suzuki, Shogo Tachibana, Tomohiro Usui
    JAXA Special Publication 23(006E) 1-39 2024年1月  筆頭著者責任著者
  • KANEMARU, Rei, KUMAGAI, Kazuya, SOEJIMA, Hiromichi, YADA, Toru, NISHIMURA, Masahiro, ABE, Masanao, OKADA, Tatsuaki, YOGATA, Kasumi, SAKAMOTO, Kanako, MIYAZAKI, Akiko, NAGASHIMA, Kana, TAHARA, Rui, NAKANO, Arisa, OJIMA, Tomoko, FUKAI, Ryota, ISHIZAKI, Takuya, HATAKEDA, Kentaro, HITOMI, Yuya, SUGIYAMA, Yuka, SUGAHARA, Haruna, SUZUKI, Shino, TACHIBANA, Shogo, USUI, Tomohiro
    JAXA Special Publication 22(005E) 1-35 2023年2月3日  筆頭著者責任著者
  • Rei Kanemaru, Naoya Imae, Akira Yamaguchi, Atsushi Takenouchi, Hirotsugu Nishido
    Polar Science 2020年12月  査読有り筆頭著者責任著者

主要なMISC

 50

共同研究・競争的資金等の研究課題

 2

学術貢献活動

 5