概括
月球岩的发光非常低,这表明对观测到的月球发光的贡献很小. 陆地岩石和矿物显示出更高的发光,威利米特是非常明亮的.
科学领域:
- 地质地质地质地质地质地
- 行星科学 行星科学
- 光物理学的光学物理学
背景情况:
- 月球表现出发光,这种现象需要对其来源进行调查.
- 了解月球发光是特征其表面组成和过程的关键.
研究的目的:
- 量化月球岩石的发光效率,并将其与地球样本进行比较.
- 评估阿波罗11号站点材料对月球整体发光的潜在贡献.
主要方法:
- 在四个月球岩石,两个陆地岩石 (花岩,加布罗) 和一个陆地矿物质 (willemite) 上进行了发光测量.
- 频谱曲线与硫酸标准进行了比较,以准确确定效率.
- 激发是使用3000安格斯特罗姆的紫外线进行的.
主要成果:
- 月球样本的发光效率较低 (<6 x 10^-5).
- 陆地的gabbro在组成上与月球样本相似,其效率相对较低 (<8 x 10^-5).
- 花岩具有更高的效率 (约. 10^-4),而威利米特显示显著更高的发光率 (约. 2 x 10^-2). 这样就没有问题了.
结论:
- 阿波罗11号月球样本的发光效率非常低.
- 这些发现表明,阿波罗11号站点的材料对观测到的月球发光有很小的贡献.
- 陆地岩石和矿物质表现出广泛的发光特性,其中一些明显超过月球样本.
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