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Reflectors - Refractors - Binoculars - Schmidt Cas- Mountings - Eyepieces - Filters - Goto Telescopes |
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Schmidt-Cassegrain Telescopes
The primary mirror is spherical, with a lens "corrector plate" over the front that holds the secondary mirror. The light is sent back through a hole in the primary to a diagonal mirror, allowing for easy behind the telescope viewing. The system is sealed so the internal optics stay clean and the system stays free of image disabling tube currents. SCT's seldom need collimation. Two concerns keep it from being the "Perfect" telescope. First, the secondary is overly large to accommodate the short tube. This results in scattered light that softens the images and degrades detail. The images are not as sharp as in a long-focus reflector or refractor. Second, the large glass corrector plate is a dust magnet, and a dew collector. This requires constant attention, and the use of a battery operated heat tape wrapped around the front to warm the lens. Nevertheless, SCT's make excellent telescopes for both visual and photographic astronomy. Two companies manufacture most of these telescopes. Celestron and Meade instruments are available through dealers in many camera stores and telescope shops.
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Classical Cassegrain: Developed in 1672, it is shorter than its focal length. The convex secondary mirror magnifies, making the focal length even longer. Long popular with large observatories.
Maksutov-Cassegrain; This design was made popular in the '50 by Questar, and is used today by Celestron with the ETX telescopes. The all spherical optics are known for their optical superiority. Although heavier and more expensive, large versions are prefered by experienced advanced amateurs. |
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