一种非地球上的16O丰富的同位素组成,用于原太阳星云
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
概括
原始的石显示出不寻常的氧同位素,引发了关于早期太阳系组成的问题. 对月球颗粒中的太阳风的分析揭示了显著的16O丰富,这表明发生了未知的质量独立反应.
科学领域:
- 太空化学 太空化学
- 行星科学 行星科学
- 天体物理学 天体物理学
背景情况:
- 原始石表现出大量的氧同位素变化,这些变化无法通过依赖质量的分离来解释.
- 由于天文观测的局限性,原太阳气体的组成仍然不确定.
研究的目的:
- 精确确定太阳风的氧同位素组成.
- 为了调查早期太阳系中异常氧同位素的起源.
主要方法:
- 在太阳风粒子中氧气同位素的分析植入在月球 regolith 金属粒中.
- 纳米尺度层的高分辨率同位素分析.
主要成果:
- 与地球,火星和石相比,月球颗粒中的太阳风颗粒显示在16O (>20 +/- 4千分之一) 中具有丰富性.
- 这种丰富意味着太阳积聚盘中存在未知的质量独立的同位素反应.
结论:
- 太阳风的氧气同位素成分与大批行星材料有很大不同.
- 未知反应,可能涉及光化学自我屏蔽,在早期的太阳系中改变了同位素比率,独立于同位素质量.
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