::Reflecting telescope


Mirror::image    Primary::light    Design::books    Mirrors::focus    Optical::focal    Optics::google

24 inch convertible Newtonian/Cassegrain reflecting telescope on display at the Franklin Institute

A reflecting telescope (also called a reflector) is an optical telescope which uses a single or combination of curved mirrors that reflect light and form an image. The reflecting telescope was invented in the 17th century as an alternative to the refracting telescope which, at that time, was a design that suffered from severe chromatic aberration. Although reflecting telescopes produce other types of optical aberrations, it is a design that allows for very large diameter objectives. Almost all of the major telescopes used in astronomy research are reflectors. Reflecting telescopes come in many design variations and may employ extra optical elements to improve image quality or place the image in a mechanically advantageous position. Since reflecting telescopes use mirrors, the design is sometimes referred to as a "catoptric" telescope.

Reflecting telescope sections
Intro  History  Technical considerations  Use in astronomical research   Reflecting telescope designs   Focal planes   See also   References  External links  

PREVIOUS: IntroNEXT: History