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A telescope is an instrument that collects and focuses light. The nature of the optical design determines how the light is focused. Some
telescopes, known as refractors, use lenses. Other telescopes, known as reflectors, use mirrors. The Maksutov-Cassegrain optical system
uses a combination of mirrors and lenses and is referred to as a compound or catadioptric telescope. This unique design offers large-diameter
optics while maintaining very short tube lengths, making them extremely portable. The Maksutov-Cassegrain system consists of a corrector
plate, a spherical primary mirror, and a secondary mirror spot. Once light rays enter the optical system, they travel the length of the optical
tube three times.
Fig 5-2a - Actual image
orientation as seen with the
unaided eye
Fig 5-2b - Reversed from left to
right, as viewed through the
eyepiece
Figure 5-1
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The optics of the NexStar have enhanced multi-layer coatings on the primary and secondary mirrors for increased reflectivity and a multi
coated corrector for the finest anti-reflection characteristics.
Inside the optical tube, a black tube extends out from the center hole in the primary mirror. This is the primary baffle tube and it prevents
stray light from passing through to the eyepiece or camera.
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The image orientation changes depending on how the eyepiece is inserted into the telescope. The NexStar uses three reflective surfaces to
bounce the light to the eyepiece. This produces an image that is right-side-up, but reversed from left-to-right (i.e., reversed). This is normal
for the Maksutov-Cassegrain design.
27
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