月球的大气层. 月球表面成分和石撞击如何调节月球外层中的和
A Colaprete1, M Sarantos2, D H Wooden3
1Space Science Division, NASA Ames Research Center, Moffett Field, Mountain View, CA, USA. anthony.colaprete-1@nasa.gov.
概括
月球外层中的和呈现出不同的周期和变化. 石撞击和表面成分对这些元素有很大影响,尤其是KREEP地区的.
科学领域:
- 月球科学
- 行星大气层
- 外层的组成
背景情况:
- 和是月球外层的微量气体.
- 它们的亮线发射使得它们很容易被观察到.
- 之前的研究暗示存在差异,但缺乏连续数据.
研究的目的:
- 分析月球外层中和的时间和空间变化.
- 为了确定石轰炸的影响和表面组成.
- 研究这些元素的月球日 (月) 和年周期.
主要方法:
- 利用月球大气和尘埃环境探测器 (LADEE) 的紫外线和可见光谱仪 (UVS) 的数据.
- 分析和的连续测量.
- 与月球表面组成相关的外层丰度,包括KREEP区域.
主要成果:
- 观察到月球和的时间和空间变化.
- 确定了两个物种的单独月度周期和的年度周期.
- 测量显示KREEP区域的可重复变化和增强,表明表面成分的依赖性.
结论:
- 流星轰炸和表面组成是月球外层变化的关键驱动因素.
- 的分布与KREEP等特定表面特征密切相关.
- 持续的监测提供了对外层动态和月球表面相互作用的关键见解.
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