16O

Ko Hashizume1, Marc Chaussidon

  • 1Department of Earth and Space Sciences, Graduate School of Science, Osaka University, Toyonaka, Osaka 560-0043, Japan. kohash@ess.sci.osaka-u.ac.jp

Nature
|April 1, 2005
PubMed
まとめ

原始的な隕石は異常な酸素同位体を示しており,初期の太陽系の組成に関する疑問を提起しています. 月面の粒子の太陽風の分析は16O濃縮が顕著であることを明らかにし,未知の質量独立反応が起こったことを示唆しています.

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