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孟治国, 常文清, 沈朝, 平劲松, 黄少鹏, 蔡占川, 张渊智. 史密斯海月球长期科研站选址与潜在科学目标分析[J]. 深空探测学报(中英文), 2022, 9(5): 521-531. DOI: 10.15982/j.issn.2096-9287.2022.20220028
引用本文: 孟治国, 常文清, 沈朝, 平劲松, 黄少鹏, 蔡占川, 张渊智. 史密斯海月球长期科研站选址与潜在科学目标分析[J]. 深空探测学报(中英文), 2022, 9(5): 521-531. DOI: 10.15982/j.issn.2096-9287.2022.20220028
MENG Zhiguo, CHANG Wenqing, SHEN Chao, PING Jinsong, HUANG Shaopeng, CAI Zhanchuan, ZHANG Yuanzhi. Site Selection and Potential Scientific Targets Analysis of Mare Smythii for Constructing Long-Term Lunar Research Station[J]. Journal of Deep Space Exploration, 2022, 9(5): 521-531. DOI: 10.15982/j.issn.2096-9287.2022.20220028
Citation: MENG Zhiguo, CHANG Wenqing, SHEN Chao, PING Jinsong, HUANG Shaopeng, CAI Zhanchuan, ZHANG Yuanzhi. Site Selection and Potential Scientific Targets Analysis of Mare Smythii for Constructing Long-Term Lunar Research Station[J]. Journal of Deep Space Exploration, 2022, 9(5): 521-531. DOI: 10.15982/j.issn.2096-9287.2022.20220028

史密斯海月球长期科研站选址与潜在科学目标分析

Site Selection and Potential Scientific Targets Analysis of Mare Smythii for Constructing Long-Term Lunar Research Station

  • 摘要: 月球史密斯海(Mare Smythii)位于月球正面与背面的交界处,具有丰富的地质单元和科学价值。结合SLDEM 2015高程数据、克莱门汀紫外/可见光数据、“月神1号”(Selene-1)多波段成像仪数据和“嫦娥二号”(Chang’E-2, CE-2)微波辐射计数据,对史密斯海的地质、地形、物质成分和微波热辐射等特征进行了系统分析。在此基础上,从科研、资源和能源的角度,建议建立以(88oE,1oN)为中心的月球长期科研站;最后,结合月表地形特征设计了3条巡视路线,初步确定和规划了14个以月球科学和资源利用为目标的值得探测的考察点并分析了其科学价值。论文的研究结果对我国未来建设长期运行的月球科研站具有重要的参考价值。

     

    Abstract: The Moon is the nearest neighbor of the Earth and the first planet for human deep space exploration. Thus, the construction of long-term lunar research station will be great significant to further explore the deep space in 21st century. Mare Smythii is located at the junction of the lunar farside and nearside, and it is rich in the geological diversities and scientific values. In this paper, combined with the SLDEM 2015 elevation data, Clementine UV/VIS data, Kaguya MI data, and Chang'E-2 microwave radiometer data, the geological significance, topography, material composition, and microwave thermal emission features of Mare Smythii are thoroughly analyzed. Then, the region centered at (88oE, 1oN) is proposed for constructing the long-term lunar research station with high priority from the perspectives of scientific research, resources, and energy. Finally, three routes are outlined according to the surface topography, and 14 candidate exploring sites are planned aiming to scientific studies and resource utilizations. This study is of essential significance for the construction of the long term lunar research stations in future.

     

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