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
红外成像显示,月球热异常是稳定的特征,而不是暂时的. 一个新发现的线性异常,可能与内部地质过程有关,在月球地裂口附近被发现.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 地质物理学 地质物理学
背景情况:
- 月食为研究月球的热性质提供了独特的机会.
- 以前的红外观测已经确定了月球表面的热异常.
研究的目的:
- 为了比较两个月食的红外图像,以评估热异常的稳定性.
- 识别和描述任何新的热特性.
主要方法:
- 获取并对1968年4月13日和1964年12月19日月食的红外图像进行比较分析.
- 在月球表面的热异常分布和强度的检查.
主要成果:
- 在月球玛丽亚上观察到的大部分热异常在两个日食之间表现出一致的强度和分布,这表明长期稳定.
- 发现了一种新的线性热异常,在月球下午显示了增强的热特征.
- 这种新的异常似乎与月球地裂线的空间相关.
结论:
- 大多数玛丽亚热异常的稳定性表明它们可能是持久的地质或地物理特征.
- 新发现的线性异常的特征表明,其潜在起源与月球内部的过程或地下结构有关.
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