Structural Design of Primary Mirror Subassembly for Space Telescope

Article Preview

Abstract:

In order to design a large aperture primary mirror with the diameter of 1150 mm, the parameters impacting on gravity deformation of the mirror were analyzed and discussed in detail, including material selection, diameter-thickness ratio, the number of the support points, location selection and lightweight structure, etc. A novel space mirror structure system was put forward, and its back was opened and supported by six points on back. The dynamic and static and thermal characteristics were analyzed based on the finite element method. Analysis results showed the surface figure accuracy reached to RMS 14.5nm under the action of gravity load along the optical axis direction and the first-order natural frequency was 214Hz which met to the designed indexes requirements.

You might also be interested in these eBooks

Info:

Periodical:

Pages:

903-906

Citation:

Online since:

February 2013

Authors:

Export:

Price:

Permissions CCC:

Permissions PLS:

Сopyright:

© 2013 Trans Tech Publications Ltd. All Rights Reserved

Share:

Citation:

[1] WANG Z S; ZHAI Y. Design of flexible support structure of reflector in space remote sensor, Optics and Precision Engineering, 18(8): 1833-1841 (2010).

Google Scholar

[2] REN J Y; CHEN C Z; HE B. Application of SiC and SiC/Al to TMA Optical Remote Sensor, Optics and Precision Engineering, 16(12): 2537-2543 (2008).

Google Scholar

[3] GUO J. Design of support for primary mirror of space remote sensing camera. Optics and Precision Engineering, 16(9): 1642-1647 (2008).

Google Scholar

[4] YODER P. Opto-mechanical Systems Design [M]. 2nd ed. New York: Marcel Dekker Inc., (1993).

Google Scholar

[5] FRIEDMAN E. Photonics Rules of Thumb [M]. New York, McGraw Hill, ( 2003).

Google Scholar

[6] SUN B Y. Design of flexible supporting structure for optical space remote sensor. Journal of Harbin Institute of Technology, 41(9): 201-203. (2009).

Google Scholar