日本地球惑星科学連合2015年大会

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セッション記号 M (領域外・複数領域) » M-TT 計測技術・研究手法

[M-TT44] 地球化学の最前線: 未来の地球化学を展望して

2015年5月26日(火) 16:15 〜 18:00 102B (1F)

コンビーナ:*平田 岳史(京都大学大学院理学研究科地球惑星科学専攻)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、角皆 潤(名古屋大学大学院環境学研究科)、小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)、橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)、鈴木 勝彦(独立行政法人海洋研究開発機構・地球内部ダイナミクス領域)、下田 玄(産業技術総合研究所地質調査総合センター)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、横山 祐典(東京大学 大気海洋研究所 海洋底科学部門/地球表層圏変動研究センター)、横山 哲也(東京工業大学大学院理工学研究科地球惑星科学専攻)、座長:平田 岳史(京都大学大学院理学研究科地球惑星科学専攻)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)

17:15 〜 17:30

[MTT44-07] We are always on the frontier!

*圦本 尚義1 (1.北海道大学)

キーワード:地球化学, 最前線

Oxygen isotope anomaly in the solar system was found from a meteorite by Clayton et al. (1973). The origin is still unknown and it is principally unsolved although we can infer it precisely. More interesting puzzle for the oxygen isotope anomaly than the origin may be the anomalous distribution among minerals and within a mineral in a Ca-Al-rich inclusion (CAI). CAIs are the oldest rock in the solar system, and are largely mm to cm in size. The CAIs formed in the solar nebula by crystallization from liquid droplet or from surrounding hot gas. However, nobody has been succeeded to describe how to establish heterogeneous oxygen isotope anomaly in a CAI according to known chemical reactions so far because the oxygen isotopic distribution is apparently inconsistent with phase relation and crystal growth in the chemical system of CAIs. This is mysterious because the chemical system of CAIs seems to be much simple comparing with terrestrial rocks. In this talk, I show an attempt to clarify this mystery predicts that oxygen isotope anomaly distributes globally but changes the degree systematically on all solar system objects including outer planets. The global change of oxygen isotope anomaly in the solar system should involve isotope anomalies of hydrogen and nitrogen. The attempt also predicts that isotope anomalies of these three elements are universally observed in exoplanetary systems, which degrees may be an indicator for habitability. These predictions can be proved by development of planetary explorations and astronomical observations, which are parts of cosmochemistry, even if the origin of the oxygen isotope anomaly in the solar system is principally an unsolved issue.

References:
Yurimoto, H. (2014) That's One Thing, This Is Something Else! Kakenhi NEWS 2014, vol. 2, 7.
http://www.jsps.go.jp/j-grantsinaid/29_essay/no63.html
http://www.jsps.go.jp/english/e-grants/kakenhi_essay/grants11_63.html

Yurimoto, H. (2009) Anatomy of Protosolar System. JGL 5 (3), 8-9.
http://www2.jpgu.org/publication/jgl/JGL-Vol5-3.pdf

Yurimoto, H. (2006) Preface. Yuseijin 15, 43.
https://www.wakusei.jp/book/pp/2006/2006-2-01/2006-2-01.pdf