基于Apollo和嫦娥五号样品的月球红外光谱研究
Infrared Spectroscopic Study of the Moon Based on Apollo and Chang’E-5 Samples
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摘要: 随着遥感技术进步和深空探测的快速发展, 热红外高光谱遥感是行星遥感前沿热点方向. 红外光谱蕴含了天体的物质成分、温度、表层物理性质等丰富的信息. 现有月球红外光谱研究主要基于Apollo古老样品, 缺乏对年轻月壤样品的研究. 嫦娥五号(Chang'E-5, CE-5)首次采集到年轻月壤, 为深入认识月球热红外光谱特征提供了新的样本, 综合利用古老Apollo样品与年轻CE-5样品光谱数据, 对月球的红外光谱特征进行分析, 揭示了不同地体与成熟度对月球红外光谱的影响. 研究结果表明, 月球不同地体的红外光谱整体形态相似, 发射率在4 μm附近达到最低, 然后急剧上升, 在8 μm附近达到发射率最大值. 不同地体的光谱特征存在差异, CE-5样品CF (Christiansen Frequency)值大于绝大部分Apollo样品, 与Apollo 11的CF值相近, 反映其富镁铁质的矿物组成特征. CE-5样品与Apollo 16样品5.45 μm处钙长石发射峰更显著. CE-5样品11.4 μm辉石发射谷更深. 太空风化影响月壤红外光谱, 主要表现为RB (Reststrahlen Bands)段的发射率升高、光谱对比度降低. 月壤CF特征与SCFM (硅、钙、铁、镁)指数相关且不受成熟度影响. 研究结果为月球及其他天体热红外高光谱遥感研究提供支撑.Abstract: With the advancement of remote sensing technology and the rapid development of deep space exploration, thermal infrared hyperspectral remote sensing has become a frontier hotspot in planetary remote sensing. Infrared spectra contain rich information about the material composition, temperature, and surface physical properties of celestial bodies. Current research on the infrared spectra of the Moon is mainly based on the ancient Apollo samples, lacking studies on younger lunar soil samples. China's Chang'E-5 (CE-5) mission has for the first time collected young lunar soil, providing new samples for a deeper understanding of the thermal infrared spectral characteristics of the Moon. By comprehensively utilizing the spectral data of the ancient Apollo samples and the young CE-5 samples, the infrared spectral characteristics of the moon were analyzed to reveal the influence of different terrains and maturity on the infrared spectra of the moon. The results show that the overall shapes of the infrared spectra of different lunar terrains are similar, with the emissivity reaching its minimum around 4 μm and then sharply increasing to reach the maximum around 8 μm. There are differences in spectral characteristics among different terrains; the CF (Christiansen Frequency) value of the CE-5 samples is greater than that of most Apollo samples and is similar to that of Apollo 11, reflecting its mafic-rich mineral composition characteristics. The plagioclase emission peak at 5.45 μm is more pronounced in the CE-5 samples compared to Apollo 16 samples. The pyroxene emission valley at 11.4 μm is deeper in the CE-5 samples. Space weathering affects the infrared spectra of lunar soil, mainly manifested as an increase in the emissivity of RB (Reststrahlen Bands) and a decrease in spectral contrast. The CF characteristics of lunar soil are related to the SCFM (Si, Ca, Fe, Mg) index and are not affected by maturity. The research results provide support for the thermal infrared hyperspectral remote sensing studies of the moon and other celestial bodies.
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