陆地贵气体特征的起源
Svyatoslav S Shcheka1, Hans Keppler
1Bayerisches Geoinstitut, Universität Bayreuth, 95440 Bayreuth, Germany. svyatoslav.shcheka@uni-bayreuth.de
Nature
|October 12, 2012
概括
在地球大气层中,相对于气相对来说,气是耗尽的. 这项研究表明,地球早期的矿结晶捕获了气,导致大气中的气耗尽.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 矿物物理 矿物物理
背景情况:
- 在地球和火星大气层中,相对于气相对于气相对显著耗尽,而与形石相比,气显著耗尽.
- 大气中这种贵重气体枯竭的原因尚不清楚.
研究的目的:
- 为了研究和在MgSiO中的可溶性 ((3) 矿石,这是地球下层地幔的主要矿物.
- 提出一种模型来解释行星大气中相对于的相对于的观察到的耗尽.
主要方法:
- 在高压和高温条件下在MgSiO(3) 矿中实验性确定和的溶解度.
- 早期地球和火星大气演变的地球化学建模.
主要成果:
- 在MgSiO(3) 矿中,的溶解度很大 (超过1重百分比),而的溶解度则小很多.
- 来自岩海洋的矿的结晶,优先将气隔离到下层地幔中.
结论:
- 矿中和的不同溶解度为观察到的大气耗尽提供了一种机制.
- 这一过程发生在早期的岩海洋结晶过程中,解释了地球和潜在的火星大气中的与的比率.
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