23 March 1987 Testing The Primary Mirror Of The W. M. Keck Observatory
Author Affiliations +
Itek Corporation has been awarded a contract for the manufacture of the primary mirror segments for the W. M. heck Observatory. The primary mirror will contain 36 hexagonally-shaped off-axis aspheres which, when aligned, will form the collecting area of a 10-m-diameter mirror. To ensure integration to the telescope, each segment must be the correct part of the desired parent asphere. During fabrication, careful optical and dimensional metrology must be performed on each segment. This paper outlines the in-process and final metrology plans for each segment.
© (1987) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Evan Stryjewski, Evan Stryjewski, R J Zielinski, R J Zielinski, J T Smith, J T Smith, } "Testing The Primary Mirror Of The W. M. Keck Observatory", Proc. SPIE 0680, Surface Characterization and Testing, (23 March 1987); doi: 10.1117/12.939592; https://doi.org/10.1117/12.939592


In-Process Measurement Of Fast Aspherics
Proceedings of SPIE (April 04 1979)
NOAO testing procedures for large optics
Proceedings of SPIE (March 26 1992)
Long-Wavelength Interferometer In The Optical Shop
Proceedings of SPIE (December 25 1979)
Stressed lap polishing of 3.5 m f 1.5 and 1.8...
Proceedings of SPIE (January 01 1992)
Process Development For Active Mirror Facesheets
Proceedings of SPIE (May 03 1988)

Back to Top