地球地幔中的色素
Antonio Caracausi1,2, Guillaume Avice2, Peter G Burnard2
1Instituto Nazionale di Geofisica e Vulcanologia, Sezione di Palermo, 90146 Palermo, Italy.
Nature
|April 26, 2016
概括
贵族气体同位素揭示了地球地幔和大气挥发物的不同起源. 异同位素分析表明地幔挥发物的小行星来源,与大气前体分开,表明早期的地球积聚过程.
科学领域:
- 地质化学
- 宇宙化学
- 同位素地质学
背景情况:
- 岩层气体中的贵族气体同位素为地球的挥发性起源,地幔演变和大气组成提供了洞察力.
- 尽管有分析的进步,但行星气体在地球的地幔和大气层的双重起源仍然受到限制.
研究的目的:
- 通过使用贵族气体同位素来研究地球地幔和大气中的挥发物质的起源.
- 确定地球地幔和大气中的挥发性物质的宇宙化学来源.
主要方法:
- 德国埃菲尔火山区的高精度岩石气体分析.
- 为了追踪挥发性来源,
主要成果:
- 轻色同位素表明地幔中的原始体成分与大气中的色前体不同.
- 地球大气层和地幔中的挥发物可能起源于不同的宇宙化学来源.
- 艾菲尔岩石起源于一个自445亿年前被隔离的深层地幔,其挥发性/耐火性比较低.
结论:
- 地球的地幔和大气中的挥发物有不同的起源,地幔的挥发物很可能来自小行星.
- 异同位素数据揭示了地球地幔中的显著化学异质,可以追溯到积累.
- 这些发现支持了早期地幔域隔离的模型,并突出了早期地球积聚过程中挥发性材料的增加.
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