Preliminary results of FeO mapping using Imaging Interferometer data from Chang’E-1
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- 作者：ZongCheng Ling (1) (2)
Jiang Zhang (1) (2)
JianZhong Liu (1)
WenXi Zhang (3)
Wei Bian (1)
Xin Ren (1)
LingLi Mu (1)
JianJun Liu (1)
ChunLai Li (1) - 关键词：Chang’E ; 1 ; Imaging Interferometer ; FeO mapping ; Clementine UVVIS
- 刊名：Chinese Science Bulletin
- 出版年：2011
- 出版时间：February 2011
- 年：2011
- 卷：56
- 期：4-5
- 页码：376-379
- 全文大小：713KB
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Jiang Zhang (1) (2)
JianZhong Liu (1)
WenXi Zhang (3)
Wei Bian (1)
Xin Ren (1)
LingLi Mu (1)
JianJun Liu (1)
ChunLai Li (1)
1. National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, China
2. School of Space Science and Physics & Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Shandong University at Weihai, Weihai, 264209, China
3. Academy of Opto-Electronics, Chinese Academy of Sciences, Beijing, 100080, China - ISSN：1861-9541
文摘
Information about the variability, and spatial distribution of iron abundance is important to understand lunar geological history and for future resource utilization. In this paper we present a preliminary model to produce an iron abundance map using images taken by an Imaging Interferometer on board the satellite Chang’E-1. Compared with the Clementine UVVIS images, the images from the Chang’E-1 satellite also allowed for the extraction of FeO abundance distributions on the Moon. However, the preliminary model results suggest an underestimation of ? wt.% for the FeO content of the mare region and an overestimation of ? wt.% for the highland region.