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月球上的无石与陆地挥发物丰富
Jeremy W Boyce1, Yang Liu, George R Rossman
1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125-2500, USA. jwboyce@alum.mit.edu
Nature
|July 24, 2010
概括
月球岩石,特别是玄武岩14053,含有惊人的 (H), (Cl) 和硫 (S) 含量. 这些发现表明,月球可能比以前认为的更富有挥发性.
科学领域:
- 地质化学 地质化学
- 月球科学 月球科学
- 行星科学 行星科学
背景情况:
- 与地球相比,月球通常被认为是挥发性元素的枯竭.
- 月球爆炸性火山活动的证据表明,一些 magma 溶解了富含 CO 的蒸汽阶段.
- 之前的研究缺乏在月球岩石中发现土著 (H) 的明确证据.
研究的目的:
- 为了研究月球基岩14053.3中晚期阿帕的挥发性含量.
- 为了将挥发性度与在陆地岩石中发现的度进行比较.
- 评估对月球挥发性库存和地幔组成的影响.
主要方法:
- 在月球玄武岩14053.3的无样本上进行了定量离子微探测测量.
- 分析了 (H), (Cl) 和硫 (S) 的度.
- 考虑了亚岩形成模型 (变态和火性).
主要成果:
- 来自月球基岩14053的阿帕石显示H,Cl和S度与陆地阿帕石相比较.
- 挥发性含量表明,要么是 magma 后的添加,要么是来自挥发性丰富的融物 (大约. 1600 ppm 的 H2O, 3500 ppm 的 Cl).
- 变态和火热模型都支持一些月球材料中的大量挥发性库存.
结论:
- 某些月球材料具有类似于陆地岩石的挥发性库存.
- 这挑战了月球普遍耗尽挥发性物质的观念.
- 月球地幔或地的部分可能比以前假设的更富有挥发性.
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