月球上的太阳风记录:解读行星的太阳前风记录.
K Hashizume1, M Chaussidon, B Marty
1Centre de Recherches Pétrographiques et Géochimiques-CNRS, BP 20, 54501 Vandoeuvre-lès-Nancy Cedex, France. kohash@ess.sci.osaka-u.ac.jp
概括
月球规律石中的太阳风是15N贫乏的,而非太阳能成分是15N丰富的. 这表明星际化合物有助于行星.
科学领域:
- 宇宙化学 宇宙化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 行星体中的同位素与原太阳气体的变化.
- 了解的起源是行星形成和演变的关键.
研究的目的:
- 为了研究月球规石中的同位素组成.
- 为了确定行星物质中的来源.
主要方法:
- 离子微探测器对月球 regolith 粒的分析.
- 在不同的 regolith 组件中分析和同位素.
主要成果:
- 与地球大气相比,月球常规岩中的太阳风在15N中至少减少了24%.
- 一个非太阳能成分,与富含的相关,显示15N丰富.
- 陆地行星和石表现出相对于原太阳气体的系统15N丰富.
结论:
- 简单的星云或行星分成不能解释观察到的15N丰富.
- 富含15N的化合物,可能是星际起源的,一定有助于行星.
- 这些星际化合物可能没有与15N耗尽的原太阳星云保持平衡.
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