| Project/Area Number |
06559004
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| Research Category |
Grant-in-Aid for Scientific Research (A)
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| Allocation Type | Single-year Grants |
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| Section | 試験 |
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| Research Field |
広領域
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| Research Institution | The University of Tokyo |
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Principal Investigator |
ONAKA Takashi The University of Tokyo, Graduate School of Science, Associate Professor, 大学院・理学系研究科, 助教授 (30143358)
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| Co-Investigator(Kenkyū-buntansha) |
MIURA Shinji NIKON CORPORATION,Manager, 特機設計部, 研究職(課長)
KAWADA Mitsunobu Institute of Space and Aeronautical Science, Research Associate, 宇宙圏研究科, 助手 (50280558)
KOHNO Tsuguo Tokyo Metropolitan Institute of Technology, Professor, 工学部, 教授 (00161878)
MURAKAMI Hiroshi Institute of Space and Aeronautical Science, Associate Professor, 宇宙圏研究科, 助教授 (40135299)
TANABE Toshihiko The University of Tokyo, Faculty of Science, Research Associate, 大学院・理学系研究科, 助手 (90179812)
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| Project Period (FY) |
1994 – 1996
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| Project Status |
Completed (Fiscal Year 1996)
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| Budget Amount *help |
¥11,000,000 (Direct Cost: ¥11,000,000)
Fiscal Year 1996: ¥900,000 (Direct Cost: ¥900,000)
Fiscal Year 1995: ¥3,600,000 (Direct Cost: ¥3,600,000)
Fiscal Year 1994: ¥6,500,000 (Direct Cost: ¥6,500,000)
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| Keywords | cooled telescope / infrared observation / light-weight mirror / space-borne instruments / silicon carbide / space observation |
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| Research Abstract |
We fabricated a spherical mirror of 150mm in diameter, which was made of SiC (silicon carbide) as a test mirror for the space-borne light-weight cooled telescope for the infrared use. The optical tests of the mirror indicate the distortion of the mirror at low temperatures (<200K). The amount of the distortion was, however, 0.6mum peak-to-valley at most, and we attributed it to the bi-metal effects produced by the difference in the thermal contraction between the CVD SiC on the surface and the porous SiC of the core. We did not detect very large distortions due to SiC material itself, which shows a quite contrast to the metalic mirrors. The porous SiC has a specific weight of 2 g cm^<-3>, which is quite advantageous for light-weight mirrors of space-borne telescopes. The CVD SiC is required to obtain high-quality polishing. The distortion was reproducable and we concluded that it could be reduced to a negligeble level if we could have a sufficient accuracy in figuring the SiC blank of the mirror. The present investigation showed that SiC mirrors are very promising for the light-weight mirror for space-borne cooled telescopes in future, but we still need to improve the blank processes to achieve the goal.
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