Schmidt Cassegrain Lens
In addition to the difference so helpfully added by another respondent to the question, in the more general sense I would add this: The Schmidt corrector (developed by Bernhard Schmidt, a German optician working in the 1920s and 1930s) permits an exceptionally wide field scope of very low focal ratio and relatively low aberration: thus, the types of telescopes used for sky surveys (like the famous Palomar set) are made with a very “fast” Schmidt and cover a wide angle of sky. However, the commercial amateur SCT scopes are usually not much faster than f6.3 (typically f10) which negates some of the value of the Schmidt corrector system. Professional Schmidt telescopes may have very large aperture correctors (they are measured by the size of their corrector and not the diameter of the primary mirror; the Palomar Schmidts are 18″ and 48″ systems.) The Maksutov (developed by a Soviet inventor) corrector lens is usually not made in sizes much larger than about 12 inches, due to the mass of the meniscus lens. Amateur Maksutovs are available up to 7″ now, but in the past the most frequently-encountered models were only 3.5″ in diameter. All the optical surfaces are spherical, which makes it easier to construct a very fine instrument giving exceptional performance (re Illingsworth, FACTS ON FILE DICTIONARY OF ASTRONOMY.) More information on telescope types is found in our software program: see our website.
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