Space Schmidt telescope
Abstract
The 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.
- Publication:
-
International Conference on Advanced Technology Optical Telescopes
- Pub Date:
- October 1982
- DOI:
- 10.1117/12.933514
- Bibcode:
- 1982SPIE..332..141W
- Keywords:
-
- Radiation Detectors;
- Reflecting Telescopes;
- Schmidt Telescopes;
- Spaceborne Telescopes;
- Ultraviolet Astronomy;
- Ultraviolet Telescopes;
- Cameras;
- Electronography;
- Far Ultraviolet Radiation;
- Focusing;
- Graphite-Epoxy Composites;
- Long Duration Space Flight;
- Magnetic Control;
- Optics;
- Pointing Control Systems;
- Radiation Shielding;
- Wide Angle Lenses;
- Astronomy