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Space Schmidt telescopeThe complete survey takes in 3627 fields, each 4.87 deg in diameter, arranged in a hexagonal pattern superimposed on the celestial equatorial coordinate system. The declination bands are spaced every 3 deg, 20 min. The optical instrument is a folded all-reflecting Schmidt system with an aperture of 0.74 m, a focal length of 2.0 m (f/2.7), a circlar field with a diameter of 4.87 deg, and a limiting image diameter of less than 2 arcsec over the entire field. The detector is an electrographic camera having a photocathode diameter of 170 mm. In discussing the telescope structure, it is pointed out that the optical support system is to be of graphite-epoxy construction. The focal tolerance (the most critical optical tolerance) is to be + or - 12 microns. Regarding contamination control, it is expected that with appropriate design it will be possible to operate in sunlight for observations in a restricted portion of the sky, at least more than 90 deg from the sun, depending on the geometry and reflectivity of the platform or spacecraft configuration.
Document ID
19830049776
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Wray, J. D.
(Texas Univ. Austin, TX, United States)
Smith, H. J.
(Texas, University Austin, Tx, United States)
Henize, K. G.
(NASA Johnson Space Center Astronaut Office, Houston, TX, United States)
Carruthers, G. R.
(U.S. Navy, E. O. Hulburt Center for Space Research, Washington DC, United States)
Date Acquired
August 11, 2013
Publication Date
January 1, 1982
Subject Category
Astronomy
Meeting Information
Meeting: International Conference on Advanced Technology Optical Telescopes
Location: Tucson, AZ
Start Date: March 11, 1982
End Date: March 13, 1982
Accession Number
83A30994
Distribution Limits
Public
Copyright
Other

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