Gregorian reflector
Quick Summary
A Gregorian telescope is a type of reflecting telescope invented by James Gregory. It uses a primary paraboloidal mirror with a hole in the center and a secondary ellipsoidal mirror. Light is reflected from the primary mirror, passes through the hole, and is then reflected by the secondary mirror to the eyepiece, producing an erect image. While this design offers an upright view, it has a limited field of view.1
Reflecting telescopes, in general, use mirrors to gather and focus light, unlike refracting telescopes that use lenses. This design avoids chromatic aberration and allows for shorter, more cost-effective tubes. Various configurations exist, including the Newtonian, Cassegrain, and Gregorian designs, each with specific mirror arrangements to achieve different optical properties.2
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