在早期太阳星云中铁的同位素均性
1Department of Earth Sciences, University of Oxford, UK. xiangz@earth.ox.ac.uk
Nature
|July 19, 2001
概括
石和地球上的铁同位素显示出变化,但落在一条线上,表明早期太阳星云中的同质化. 这发生在行星小积累和体规则形成之前.
科学领域:
- 太空化学 太空化学
- 同位素地质化学 同位素地质化学
- 星球科学 星球科学
背景情况:
- 早期太阳星云的化学和同位素均性是宇宙化学的一个关键问题.
- 对具有多个同位素的元素的同位素研究可以揭示太阳星云的初始组成.
- 石中的氧同位素异常表明了最初的异质性或银河系进化影响.
研究的目的:
- 在石和陆地样本中研究铁的同位素组成.
- 为了确定铁同位素是否为太阳星云中的初始同质性提供了支持或反对的证据.
- 为了确定与早期太阳系过程相对的铁同位素均质化的时间.
主要方法:
- 在不同样本中测量三种铁同位素 (例如,54Fe,57Fe,58Fe) 的相对丰度.
- 使用三同位素图形分析同位素数据.
- 在地球外 (流星) 和地球上的物质中对同位素变异的比较.
主要成果:
- 在石和陆地样本中检测到铁同位素丰度的显著变化.
- 所有分析的太阳系材料,当在三同位素图上绘制时,沿着单一的质量分数线对齐.
- 这种对齐表明,铁同位素在太阳星云中经历了质量分化和同质化.
结论:
- 太阳系中的铁同位素与最初同质的储备相一致.
- 铁同位素的均质化发生在太阳星云中,在行星积聚和体形成之前.
- 铁同位素数据不支持早期太阳星云中具有独特铁同位素特征的明显前体材料的存在.
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