哈迪时代 (Hadean) 岩石的氧化状态以及对早期地球大气层的影响
Dustin Trail1, E Bruce Watson, Nicholas D Tailby
1Department of Earth and Environmental Sciences, Rensselaer Polytechnic Institute, Troy, New York 12180, USA. traild@rpi.edu
Nature
|December 2, 2011
概括
早期地球的大气组成受到火山排气的影响. 研究表明,Hadean magma的氧气含量与今天相似,这表明早期的大气层没有减少.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 早期地球的历史 历史 历史
背景情况:
- 磁性排气显著塑造了地球的早期大气层 (超过4000万年前).
- 大气的组成取决于火山喷发的氧气流动性 (氧气压力).
- 由于岩石记录有限,对哈迪纪 (在3850万年前之前) 磁石氧化状态的直接证据很少.
研究的目的:
- 为了确定Hadean岩融化的氧化状态.
- 为了限制地球最早大气层的组成.
- 为了研究早期陆地岩的氧化还原条件.
主要方法:
- 在晶体中使用合物进行氧化还原敏感校准.
- 分析了可以追溯到大约4.4亿年前的古老的岩火性碎石.
- 哈迪时代石的氧气流动性与现代和古时代地幔衍生的岩进行了比较.
主要成果:
- 哈迪时代的岩融化表现出与法雅岩-磁石-石英缓冲区一致的氧气流动性,类似于今天的条件.
- 选择的哈迪纪石表明氧气的流动性可比于现代地幔衍生的岩,早在4.350亿年前.
- 早期陆地岩的氧化状态与今天的氧化状态没有显著不同.
结论:
- 在太阳系形成大约2亿年后,地球内部的排气并没有导致大气减少.
- 费亚利特-磁铁-石英缓冲区很可能控制了海底岩中的氧化还原条件.
- 早期地球的大气层可能具有氧化成分,影响了它的进化.
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