同位素证据表明,积聚蒸汽损失塑造了行星的组成
Remco C Hin1, Christopher D Coath1, Philip J Carter2
1School of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, Bristol BS8 1RJ, UK.
Nature
|September 30, 2017
概括
星球上的同位素比原始的石更重. 这种差异很可能来自行星积聚过程中的蒸气损失,而不是星云或核心过程.
科学领域:
- 星球科学
- 宇宙化学
- 同位素地化学
背景情况:
- 差异化行星在化学上与原始的状石不同.
- 在行星中挥发性枯竭的起源 (积聚与星云分离) 仍在争论中.
- 同位素组成为行星形成过程提供了洞察力.
研究的目的:
- 调查行星体中的化学分离的起源.
- 要确定挥发性耗尽是由于积累或雾过程.
- 分析微分体中的同位素组成.
主要方法:
- 开发了一种改进的分析方法来减少测量不准确性.
- 在差异化行星体和状石中测量同位素组成.
- 在行星形成阶段模拟的同位素分离.
主要成果:
- 所有研究的差异化物体的同位素成分比状石更重.
- 在太阳星云凝聚,核心形成或酸盐分化过程中的分化不能解释观察到的同位素变化.
- 在行星积累过程中通过蒸汽逃逸的同位素分离提供了一个可行的解释.
结论:
- 在行星上同位素的变化最好通过在积累过程中显著的蒸气损失来解释.
- 这种涉及液体蒸汽分离和逃逸的机制也会影响和铁同位素.
- 在生长过程中,行星体中约有40%的蒸气损失是观测到的元素和同位素组成.
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