月球表面材料的特异性热量从凯尔文90度到350度
概括
对阿波罗11号月球样本的特定热量测量显示,随着温度的平稳增加. 这一发现影响了对月球表面热参数的理解,月球表面的热参数在白天和夜晚之间有很大差异.
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:
- 了解月球规格岩的热特性对于表面勘探和热建模至关重要.
- 阿波罗11号任务提供了独特的样本用于现场分析.
研究的目的:
- 测量阿波罗11号月球样本 (10057和10084) 的特定热量.
- 要确定从90K到350K的比热的温度依赖性.
- 评估对月球表面热参数的影响.
主要方法:
- 用adiabatic热量计来测量特定热量.
- 样本包括状玄武岩类岩石和月球土壤.
主要成果:
- 特定热量在90K时平稳地从大约0.06cal/g/K增加到350K时0.2cal/g/K.
- 测量的特定热值是分析月球材料的特征.
结论:
- 特定热量数据为月球热模型提供了必要的参数.
- 月球表面的计算热参数 (gamma) 显示了大约2倍的日间变化.
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