相关实验视频
Updated: Jun 20, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
月球水分的时间和空间变化,由深度冲击航天器观察到
Jessica M Sunshine1, Tony L Farnham, Lori M Feaga
1University of Maryland, College Park, MD 20742, USA. jess@astro.umd.edu
概括
月亮的月亮的月亮
科学领域:
- 月球科学 月球科学
- 地质化学 地质化学
- 太空探索 太空探索
背景情况:
- 月球被认为很大程度上是干燥的,但最近的发现表明表面水化.
- 在月球表面已经检测到水 (H2O) 和 (OH).
研究的目的:
- 为了研究月球表面水分的日间变化和来源.
- 量化不同月球地形上的水分水平.
主要方法:
- 来自深度冲击航天器的近红外吸收数据的分析.
- 在不同的月球区域之间和随着时间的推移,水分水平的比较.
主要成果:
- 观测到月球表面的水分,特别是在北极附近,H2O含量低于0.5%的重量.
- 水分水平每天波动,与温度相关,而不是太阳辐射.
- 在一个月球日内,海基岩的水分变化比高地 (~50%) 更多 (~70%).
结论:
- 月球表面的水分化是一个动态的白天过程,不仅仅取决于成分.
- 快速的水合变化表明白天的水组离子来源,可能来自太阳风.
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