DocumentCode
2908332
Title
Bonding thin mirror segments without distortion for the International X-Ray Observatory
Author
Evans, Tyler C. ; Chan, Kai-Wing ; Saha, Timo T.
Author_Institution
NASA Goddard Space Flight Center, Greenbelt, MD, USA
fYear
2011
fDate
5-12 March 2011
Firstpage
1
Lastpage
13
Abstract
The International X-Ray Observatory (IXO) uses thin glass optics to maximize large effective area and precise low angular resolution. The thin glass mirror segments must be transferred from their fabricated state to a permanent structure without imparting distortion. IXO will incorporate about fourteen thousand thin mirror segments to achieve the mission goal of 3.0 square meters of effective area at 1.25 keV with an angular resolution of five arc-seconds. To preserve figure and alignment, the mirror segment must be bonded with sub-micron movement at each corner. Recent advances in technology development have produced significant x-ray test results of a bonded pair of mirrors. Three specific bonding cycles will be described highlighting the improvements in procedure, temperature control, and precision bonding. This paper will highlight the recent advances in alignment and permanent bonding as well as the results they have produced.
Keywords
astronomical telescopes; mirrors; International X-Ray Observatory; large effective area; low angular resolution; specific bonding cycles; submicron movement; temperature control; thin glass mirror segments; thin glass optics; Bonding; Glass; Mirrors; Optical distortion; Pins; Reflection; Shape;
fLanguage
English
Publisher
ieee
Conference_Titel
Aerospace Conference, 2011 IEEE
Conference_Location
Big Sky, MT
ISSN
1095-323X
Print_ISBN
978-1-4244-7350-2
Type
conf
DOI
10.1109/AERO.2011.5747382
Filename
5747382
Link To Document