地球地幔中的石Kr表明大气层的晚期增积源
Greg Holland1, Martin Cassidy, Chris J Ballentine
1School of Earth, Atmospheric, and Environmental Sciences, University of Manchester, Oxford Road, Manchester M13 9PL, UK. g.holland@manchester.ac.uk
概括
在地球地幔中发现的原始 (Kr) 表明挥发性物质起源于石或早期太阳星云. 地球的大气和海洋很可能从晚些时候的挥发性捕获中获得了贵气,而不是早期的排气.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 高贵气体同位素对于了解行星挥发性物质的起源和分布至关重要.
- 地球挥发物质的来源和传递机制仍然是行星科学中的一个关键问题.
研究的目的:
- 通过分析贵重气体同位素来调查地球挥发物质的起源.
- 为了确定地球地幔中原始 (Kr) 的来源.
主要方法:
- 在地球地幔的样本中对Kr和Xenon (Xe) 的高精度同位素分析.
- 同位素特征与潜在的外星来源 (如石和太阳星云) 的比较.
主要成果:
- 在地球地幔样本中发现了原始的Kr.
- 克尔的同位素组成与石或分成部分的太阳星云起源一致.
- 结合的Kr和Xe同位素数据表明,地球内部的挥发物与碳酸合金相匹配.
结论:
- 地球内部的挥发性物质很可能起源于类似于碳状地质的增积材料.
- 大气和海洋的贵气主要来自后来的挥发性捕获事件.
- 冲击脱气或早期脱气是地球大气和海洋贵气的不那么重要的来源.
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