来自MESSENGER X射线光谱仪的水星表面的主要元素组成
Larry R Nittler1, Richard D Starr, Shoshana Z Weider
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015, USA. lnittler@ciw.edu
概括
水星 水星 水星 水星 水星
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 天体化学是天体化学.
背景情况:
- 水星的表面成分在很大程度上是未知的.
- 了解水星的组成,可以了解地球行星的形成.
研究的目的:
- 用X射线光数据分析水星的表面组成.
- 为了比较水星的组成与其他陆地行星,并限制其形成历史.
主要方法:
- 由MESSENGER航天器获得的X射线光谱的分析.
- 与行星地和石材料模型进行元素比率 (Mg/Si,Al/Si,Ca/Si,Fe,S,Ti) 的比较.
主要成果:
- 水星的表面具有高的Mg/Si和低的Al/Si和Ca/Si比率,与富含地的月球地不同.
- 硫的丰富度至少是地球或月球的10倍.
- 低表面铁和的丰度不支持不透明的氧化物作为表面反射力的主要贡献者.
结论:
- 水星的表面成分表明,它是由高度减少的物质形成的,可能是恩斯塔提特地铁或无水彗星尘埃.
- 这个星球的地并不像月球那样富含地.
- 该组合挑战了依赖不透明氧化物用于水星低反射率的模型.
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