Summarizing Telescopes
Telescopes Summary
- Simple telescopes can be made with two lenses. They are used for viewing objects at large distances and utilize the entire range of the electromagnetic spectrum.
- The angular magnification M for a telescope is given by
\(M=\cfrac{\theta \prime }{\theta }=-\cfrac{{f}_{\text{o}}}{{f}_{\text{e}}}\text{,}\)
where \(\theta \) is the angle subtended by an object viewed by the unaided eye, \(\theta \prime \) is the angle subtended by a magnified image, and \({f}_{\text{o}}\) and \({f}_{\text{e}}\) are the focal lengths of the objective and the eyepiece.
Glossary
adaptive optics
optical technology in which computers adjust the lenses and mirrors in a device to correct for image distortions
angular magnification
a ratio related to the focal lengths of the objective and eyepiece and given as \(M=-\cfrac{{f}_{\text{o}}}{{f}_{\text{e}}}\)
This lesson is part of:
Vision and Optical Instruments
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