相关实验视频
Updated: Jul 12, 2026

06:14
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
概括
研究了月球岩石的红外吸收和热特性. 结果表明辐射是月球表面热流的关键,新的导电量测量低于之前的估计.
科学领域:
- 地质物理学 地质物理学
- 行星科学 行星科学
- 材料科学 材料科学 材料科学
背景情况:
- 了解月球表面的热特性对于任务规划和解释遥感数据至关重要.
- 以前在地球上测量月球岩的导热率可能无法完全反映现场条件.
研究的目的:
- 为了研究月球岩石的红外吸收特性.
- 测量月球岩石样本的特定热量和导热率.
- 确定月球表面层中占主导地位的传热机制.
主要方法:
- 红外光谱学被用来分析从2到2000微米的吸收特性.
- 在月球岩石样本上进行了特定热量和导热率的直接测量.
- 开发了一种新的方法来确定月球表面层的平均导热率.
主要成果:
- 描述了月球岩石的红外吸收特性.
- 直接测量提供了特定的热量和热导率数据.
- 纯辐射似乎是月球表面热流中的主要因素.
- 新的导电率值低于之前报告的地球测量值.
- 在~10米深处的月球岩石表现出多孔和碎片的特征.
结论:
- 辐射显著影响月球表面内的热传递.
- 开发的方法可以更准确地评估月球导热率.
- 月球岩石的多孔性延伸到相当深处,影响热模型.
相关概念视频
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