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Proceedings Article

Construction of the Keck Observatory

[+] Author Affiliations
Jerry E. Nelson, Terry S. Mast

Univ. of California/Berkeley and Lawrence Berkeley Lab. (USA)

Proc. SPIE 1236, Advanced Technology Optical Telescopes IV, 47 (July 1, 1990); doi:10.1117/12.19171
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From Conference Volume 1236

  • Advanced Technology Optical Telescopes IV
  • Lawrence D. Barr
  • Tucson, AZ | February 11, 1990

abstract

The W.M. Keck Observatory and its Ten-Meter Telescope are nearing completion at the summit of Mauna Kea. The 10-m diameter primary mirror has a 17.5-m focal length and is composed of 36 hexagonal segments. There will be seven Ritchey-Chretien f/15 foci: two of them at Nasmyth foci, one at Cassegrain focus, and four at bent Cassegrain foci on the elevation ring. There will also be an f/25 IR focal plane at the intersection of the optical and elevation axes, whose focus will be chopped by a beryllium secondary mirror. Image quality with a FWHM of the order of about 0.25 arcsec, and an 80-percent enclosed energy diameter of about 0.40 arcsec, are anticipated.

© (1990) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Jerry E. Nelson and Terry S. Mast
"Construction of the Keck Observatory", Proc. SPIE 1236, Advanced Technology Optical Telescopes IV, 47 (July 1, 1990); doi:10.1117/12.19171; http://dx.doi.org/10.1117/12.19171


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