贵重气体同位素和同位素同位素学家揭示了黄石气体的深层来源和地下断裂
Michael W Broadley1,2, Peter H Barry2, Rebecca L Tyne1,2
1Department of Earth and Environmental Science, University of Manchester, Manchester M13 9PL, U.K.
概括
这项研究揭示了黄石水热气体中和贵重气体的组成. 这些发现表明,地幔深层的和贵重气体反映了地球的原始建筑材料.
科学领域:
- 地质化学 地质化学
- 同位素地球化学 同位素地球化学
- 行星科学 行星科学
背景情况:
- 对于地球的可居住性至关重要,但它的交付和预算演变仍然不太了解.
- 大气中的占主导地位,但它的起源和行星变化需要进一步调查.
- 水热系统为深层地球过程和挥发性循环提供了洞察力.
研究的目的:
- 研究地球地幔中和贵重气体的起源和演变.
- 在热水样本中分析和贵重气体的同位素组成.
- 在地质时间内限制影响地球预算的来源和过程.
主要方法:
- 在热水气样本中测量同位素 (Δ30).
- 对 (Ar), (Kr) 和 (Xe) 的超高精度同位素测量.
- 使用同位素数据和贵重气体比率的双组分混合模型的应用.
主要成果:
- 观察到δ15N与非放射性贵重气体同位素 (Ar,Kr,Xe) 之间的相关性.
- 表明和贵气在通过岩石CO2的扩散过程中被分化.
- 黄石地幔源δ15N与大气相似;N2/36Ar和36Ar/130Xe比率不同于MORB来源.
结论:
- 黄石地幔源的同位素特征表明,它比以前认为的少被回收材料覆盖.
- 深层地幔中的和贵重气体成分可能反映了形成地球的原始材料.
- 这项研究提供了对地球早期挥发性库存及其演变的关键见解.
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