Indian Astronomical Supplies Catadioptrics
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Catadioptrics
Catadioptrics use a combination of mirrors and lenses to fold the optics and form an image. There are two popular designs: the Schmidt-Cassegrain and the Maksutov-Cassegrain.
In the Schmidt-Cassegrain the light enters through a thin aspheric
Schmidt correcting lens, then strikes the spherical primary mirror and is reflected back up the tube and intercepted by a
small secondary mirror which reflects the light out an opening in the rear of the instrument where the image is formed at
the eyepiece. Catadioptrics are the most popular type of instrument, with the most modern design, marketed throughout the
world in 3 1/2" and larger apertures.
Schmidt-Cassegrain Advantages
Schmidt-Cassegrain Disadvantages
Maksutov-Cassegrain The Maksutov design is a catadioptric (using both mirrors and lens) design with basically the same advantages and disadvantages as the Schmidt. It uses a thick meniscus correcting lens with a strong curvature and a secondary mirror that is usually an aluminized spot on the corrector. The Maksutov secondary mirror is typically smaller than the Schmidt's giving it slightly better resolution for planetary observing. The Maksutov is heavier than the Schmidt and because of the thick correcting lens takes a long time to reach thermal stability at night in larger apertures (over 90mm). The Maksutov optical design typically is easier to make but requires more material for the corrector lens than the Schmidt-Cassegrain. |
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