小行星433埃罗斯的元素组成:NEAR-shoemaker X射线光谱仪的结果
1Goddard Space Flight Center, Code 691, Greenbelt, MD 20771, USA. Space Sciences Building, Cornell University, Ithaca, NY 14853, USA. Max-Planck-Institut fur Chemie, Postfach 3060, D-55020 Mainz, Germany. Department of Planetary Science, Spac.
概括
对小行星433 Eros的分析揭示了原始的,混凝土组成. 低含量表明没有全球差异化,而硫耗尽可能表明撞击或融事件.
科学领域:
- 行星科学 行星科学
- 小行星组成分析分析.
- 地质化学 地质化学
背景情况:
- 小行星433 Eros是一颗靠近地球的小行星.
- 了解小行星的组成,可以了解太阳系早期的过程.
研究的目的:
- 为了确定小行星433 Eros的主要元素组成比率.
- 调查埃罗斯的组成对其形成和演变的影响.
主要方法:
- 从成像数据中分析主要元素组成比率.
- 元素比率的比较 (Mg/Si,Al/Si,Ca/Si,Fe/Si) 与混凝土模型.
主要成果:
- 所有分析的地区都显示的丰度很低,这与全球差异化相矛盾.
- 元素的比例强烈地表明了Eros的原始,混凝土组成.
- 与普通地铁相比,观察到硫的显著减少,以及和的可能减少.
结论:
- 433 Eros的组成最好解释为原始和混凝土.
- 观察到的耗尽可能表明有限的部分融化或冲击诱导的挥发.
- 埃罗斯的组成提供了关于早期太阳系条件和小行星处理的线索.
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