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机构地区:[1]南京大学天文系,南京210093 [2]中国科学院广州地球化学研究所
出 处:《南京大学学报(自然科学版)》2004年第1期94-108,共15页Journal of Nanjing University(Natural Science)
基 金:国家自然科学基金(40072075)
摘 要: 近几十年来,月球多色测光研究成为天文学一个重要领域.尤其是近年Clementine飞船作了几乎整个月球表面的多色测光,得到高分辨月球多色图像.联系Apollo等飞船取回月球样品的实验结果,结合理论研究和新的分析方法,揭示于全月球表面和区域的特性.本文综述一些重要进展和最新成果,包括一些主要概念(反照率,位相函数、全月面累积测光和区域测光)、测光模型、分光反照率测定结果,尤其是Clemmentine飞船资料的分析研究结果———光度参数、月面温度分布、FeO和TiO2分布、月壤成熟度、盆地抛出物、火山沉积物和区域地质.During recent decades, multispectral photometry and relevant researches of the moon have become an important task. Especially in recent years, spacecraft Clementine made multispectral photometry of almost the whole lunar surface and obtained lunar multispectral images with high resolution. In combination with experimental results of lunar samples returned by spacecrafts Apollo and others, integrated with theoretic researches and new analytical methods, properties of the whole lunar surface and regions were revealed. In this paper, some important progress and recent results in the field were presented comprehensively, including some main concepts (albedos, phase function, photometries of the whole lunar disk and regions), photometry models, measured results of spectral albedo, especially the analyzed and researched results of the whole lunar surface and regions obtained from the data of spacecraft Clemmentine data photometric parameters, distributions of temperature, FeO and TiO_2 contents on the lunar disk, maturity of lunar regolith, ejection from basins, pyroclastic deposits, as well as regional geology.
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