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                TYPES 
                        OF TELESCOPES
               
              
              
             
               
              
             
               
             
             
              
               
                
                 Refracting 
                        Telescopes
                
               
              
              
             
              
               Light enters 
                        through a large convex (outward curving) glass lens called 
                        the objective. This lens refracts, or bends, the light 
                        toward the eyepiece, where it produces an image. One of 
                        the main problems with refracting telescopes is a phenomenon 
                        referred to as chromatic aberration, which causes objects 
                        to appear to be surrounded by rainbow-colored halos. To 
                        compensate for this problem, a special second lens is 
                        mounted behind the main objective to focus more of the 
                        colors of light at a single point. Because they can produce 
                        "true" images (rather than the inverted images seen with 
                        reflectors), refracting telescopes are useful both for 
                        stargazing and land observation, such as bird-watching.
              
              
             
               
              
             
               
             
             
              
               
                Reflecting 
                        Telescopes
               
              
              
             
              
               Reflecting 
                        telescopes use a series of mirrors to gather and focus 
                        light. In a Newtonian reflector, light passes through 
                        the open tube of the telescope until it reaches the primary 
                        parabolic mirror. This curved mirror reflects the light 
                        rays to a secondary flat mirror, which reflects the light 
                        to the eyepiece of the telescope. There the image (inverted) 
                        is brought into focus. Because it is technically simpler 
                        to build and support large, high-quality mirrors rather 
                        than lenses, most large optical telescopes are of the 
                        reflecting type. Reflectors in general yield the largest 
                        aperture per dollar and account for about 90 percent of 
                        telescopes used by amateurs. Advanced amateurs commonly 
                        use an aperture of at least 152 millimeters (6 inches).
              
              
             
               
              
             
               
             
             
              
               
                Catadiatropic 
                        Telescope
               
              
              
             
              
               Invented by 
                        Bernhard Schmidt in 1930, the catadiatropic telescope
              
              
               
              
              
               the 
                        name means "reflecting and refracting"
              
              
               
              
              
               employs 
                        a combination of lenses and mirrors. Light passes through 
                        a thin lens on its way to a spherical primary mirror. 
                        The reflected light then hits a convex secondary mirror 
                        and is transmitted to the focal point through a small 
                        opening in the primary mirror. This configuration allows 
                        the optics to be housed in a short tube. Compact and portable, 
                        catadiatropic telescopes are popular among experienced 
                        amateur astronomers.
              
              
             
               
              
             
              
                
              
              
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