プロトソーラー星雲のための地球外の16O豊富な同位体組成
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
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.
科学分野:
- 宇宙化学 (コスモケミストリー)
- 惑星科学 惑星科学
- 天体物理学 天体物理学
背景:
- 原始的な隕石は,質量依存分割によって説明できない大きな酸素同位体変動を示しています.
- プロトソーラーガスの構成は,天文観測の限界のために不確実である.
研究 の 目的:
- 太陽風の酸素同位体組成を正確に決定するために.
- 太陽系初期における異常な酸素同位体の起源を調査する.
主な方法:
- 月面のレゴリトの金属粒に埋め込まれた太陽風の粒子における酸素同位体の分析.
- ナノメートルスケールの層の高解像度の同位体分析.
主要な成果:
- 月面の粒子の太陽風粒子は,地球,火星,隕石と比較して16O (>20 +/- 4 per thousand) の濃度を示しています.
- この濃縮は,太陽の蓄積円盤に,未知の質量独立の同位体反応が存在することを示唆している.
結論:
- 太陽風の酸素同位体組成は,惑星の大量物質と大きく異なる.
- 未知の反応は,潜在的に光化学的自己遮蔽を含み,同位体質量に関係なく,初期太陽系における同位体の比率を変化させた.
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