AEROSPACE CHINA

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China Aerospace Academy of Systems Science and Engineering

ISSN 1671-0940

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AEROSPACE CHINA ›› 2019, Vol. 20 ›› Issue (3): 14-21.doi: 10.3969/j.issn.1671-0940.2019.03.002

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Characteristics of Staring Imaging Spectrometer and Its Application Prospect in Asteroid Exploration

  

  1. Shanghai Institute of Technical Physics of the CAS, Shanghai 200083
  • Online:2019-10-11 Published:2019-11-01
  • About author:HE Zhiping (1977.7− ), received his Ph.D. in Physics and Electronics from the Chinese Academy of Sciences in 2009. He is currently a research professor of the Shanghai Institute of Technical Physics, Chinese Academy of Sciences. He has been engaged in space optics and opto-electronics technology and system research for a long time, in which in-situ spectral and imaging detection on the surface of lunar and planets has been successfully applied in the Chang’e 3 and Chang’e 4 projects in China. At present, he participates in the research and development of spectral exploration payloads for China’s Chang’e 5 and Mars exploration missions.

Abstract: Compared with traditional ground asteroid observations, deep space exploration is an important way to explore and comprehensively understand the characteristics of asteroids. Imaging spectrometer integrates morphological measurement and spectral measurement, and has the ability to acquire image and spectral data simultaneously. By combining morphometry and spectrometry, it is possible to achieve efficient identification and quantitative analysis of the chemical components of the exploration target, and has the strong advantage in the field of asteroid exploration. 
This paper analyzes the principle of the staring imaging spectrometer and the technological progress in various countries. Based on the requirements of light, small payloads and the space characteristics of spectroscopic devices, the application of staring imaging spectrometer is discussed. Then, this paper introduces the conceptual design of an acousto-optic staring imaging spectrometer, combined with the technical characteristics of its area array stare frame imaging and fast electronic control spectrum selection. An experimental verification is carried out, which provides a reference for the feasibility of this type of instrument in asteroid exploration.