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超轻量镜面系统的研制
引用本文:许金鑫,;郭伟远.超轻量镜面系统的研制[J].云南天文台台刊,2008(2):192-198.
作者姓名:许金鑫  ;郭伟远
作者单位:[1]中国科学院国家天文台南京天文光学技术研究所,江苏南京210042; [2]中国科学院研究生院,北京100049
摘    要:空间望远镜的研制一直要求系统的轻量化,美国宇航局(NASA)最近研制的韦伯太空望远镜,其主镜系统面密度相对于哈勃空间望远镜已大幅减轻。在韦伯望远镜主镜系统的研制过程中,NASA开展了一系列关于超轻量镜面系统的验证计划,多家机构拿出多个方案参与竞标。本文选取几个比较典型的方案,介绍这些镜面系统的设计思想、结构、材料、加工以及相关测试结果,期望能对国内相关方面的工作提供参考。

关 键 词:空间望远镜  超轻量镜面系统  韦伯望远镜

The Research on the Ultra- light Mirror System
Institution:XU Jin - xin, GUO Wei - yuan( 1. National Astronomical Observatories/Nanjing Institute of Astronomical Optics & Technology, Chinese Academy of Sciences, Nanjing 210042, China; 2. Graduate University of Chinese Academy of Science, Beijing 100049, China)
Abstract:The space telescope system is required to be light. The JWST (the James Webb Space Telescope) which has recently produced by NASA (American National Aeronautics and Space Administration)gets much smaller area density of primary mirror system than HST ( the Hubble Space Telescope). JWST was formerly known as the NGST ( Next Generation Space Telescope) , and it has a basic goal in NASA to produce a larger space telescope than the HST with the same cost and mass. In order to design the lightest primary mirror system, NASA scheduled a series of programs such as NMSD ( NGST Mirror System Demonstrator) ,SBMD (Small Beryllium Mirror Demonstrator ) and AMSD (Advanced Mirror System Demonstrator). Many institutes competed for those programs, they all have good schemes for the ultra - light mirror system. In this article, several typical projects are introduced with respect to the design idea, structure, material, manufacture and test results.
Keywords:space telescope  ultra - light mirror system  JWST
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