地理研究

地理研究 ›› 2014, Vol. 33 ›› Issue (6): 1023-1030.doi: 10.11821/dlyj201406003

• 月球研究 • 上一篇    下一篇

嫦娥一号月球地形模型的一些应用研究

平劲松1,2, 苏晓莉2, 黄倩3, 鄢建国4, 沈玉凌5   

  1. 1. 中国科学院国家天文台中科院月球与深空探测重点实验室, 北京 100012;
    2. 中国科学院上海天文台天文地球动力学中心, 上海 200030;
    3. 中国地质大学地球科学院, 武汉 430070;
    4. 武汉大学测绘遥感信息工程国家重点实验室, 武汉 430070;
    5. 中国科学院新疆生态与地理研究所, 乌鲁木齐 830011
  • 收稿日期:2014-03-12 修回日期:2014-04-28 出版日期:2014-06-10 发布日期:2014-06-10
  • 作者简介:平劲松（1969-），男，河北定州人，博士，研究员，主要从事月球与深空探测科学研究。E-mail：jsping@bao.ac.cn
  • 基金资助:
    中科院月球与深空探测重点实验室与宇航动力学国家重点实验室联合资助

Some application researches based on lunar topography model of Chang'E-1 Orbiter

PING Jinsong1,2, SU Xiaoli2, HUANG Qian3, YAN Jianguo4, SHEN Yuling5   

  1. 1. Key Laboratory of Lunar & Deep Space Exploration, National Astronomical Observatories of CAS, Beijing 100012, China;
    2. Research Center of Astro-Geodynamics, Shanghai Astronomical Observatory, CAS, Shaghai 200030, China;
    3. Faculty of Earth Sciences, China University of Geosciences, Wuhan 430070, China;
    4. State Key Laboratory of Information Engineering in Surveying, Mapping and Remote Sensing, Wuhan University, Wuhan 430070, China;
    5. Xinjiang Institute of Ecology and Geography, CAS, Urumqi 830011, China
  • Received:2014-03-12 Revised:2014-04-28 Online:2014-06-10 Published:2014-06-10

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摘要： 利用嫦娥一号绕月卫星激光高度计数据获取得到的新的360 阶次的地形模型CLTMs03，开展了初步应用研究，包括对嫦娥一号CCD立体相机数据进行了校对，发现并了解立体相机分析中的约900 m的垂向系统误差；利用撞击坑计数法，基于标校后的照相数据对嫦娥一号地形中新发现的玉兔火山区域的年龄特征进行了分析；结合新的CLTM-s03 地形模型和CEGM-02 重力场模型，新证实了西拉德撞击坑是一个布格质量瘤异常区域。

关键词: 嫦娥一号, 卫星, 月球地形

Abstract: Primary studies were carried out using the new 360 orders and degrees of lunar topography model CLTM-s03 obtained by laser altimetry data of Chang'E-1 lunar orbiter. 3D CCD image data was validated; a constant vertical bias of ~900 m in the CCD DTM was found and corrected track by track. The differences between CCD DTM and CLTM-s03 are close to 2.0 km. The errors are mainly from orbits, angle bias for the CCD camera installing, as well as the image error. To obtain a higher accuracy lunar DTM of 20-30 m at radical direction, advantages of both LAM DEM and CCD DTM are required. The long wavelength parts of DTM are suggested to use the LAM DEM model which may cover 0-360 orders and degrees. The middle and short wavelength parts will use the 3D CCD images, where the long wavelength parts of CCD have been cancelled. Igneous and impacting activity dominates the evolution history of the Moon. By using Chang'E-1 image data, we found several shield volcanoes, including YUTU shield volcano with Marius Hills and the Aristarchus Plateau shield volcano. The classical lunar surface crater density counting method was used to study the age of them based on the validated CCD image data. It is found that the surface impacting age of YUTU shield volcano is about 3.52±0.02Ga. By combining the topography data with the gravity data, it is found that this shield volcanic area has higher crustal density, lower elasticity thickness and remarkable inner magma load. Additionally, we removed the terrestrial gravity constrained by topography from free air gravity, and then obtained the Buguar gravity of the Moon. The high resolution of gravity and topography data help us to find three new mass concentrating areas under the surface of the Moon. The Szilard Crater, one of the new mascons, is located to the northeast of Richardson Crater on the farside of the Moon. The newly identified mascons will benefit the investigation of the lunar igneous evolution.

Key words: Chang'E-1, orbiter, lunar topography