Principles of Telescopes

By G. A. Davis|J. D. Keller
Pearson Allyn Bacon Prentice Hall

All telescopes are designed to do one thing: collect light. By using a telescope, you are condensing the light from a larger area through a system of mirrors and or lenses to a small area that can be seen through the pupil of your eye. For instance, using a 6-inch optical telescope will increase the amount of light that reaches your pupil by approximately 200 times. Thus, a very dim object that typically cannot be seen with the naked eye in the nighttime sky will appear much brighter through a telescope.

Except for close objects, such as the moon and planets, and for viewing nebular objects such as galaxies, the magnification of a telescope is of little value. Even with the world’s largest telescope, all stars appear as just a pinpoint of light. But through the telescope, the pinpoint will be much brighter. Thus, when purchasing a telescope you should be much more concerned about how much light a telescope collects than its magnification.

Optical telescopes are divided into two basic categories: refracting telescopes and reflecting telescopes.

Refracting Telescopes  Refracting telescopes utilize a system of lenses that collect and refract light to magnify the image (Figure ). They have a larger diameter lens called the objective lens and a small lens called an eyepiece. Good refracting telescopes utilize multiple lens systems to correct for color aberrations. Chapter discusses lenses in the section on “Stations for Sight”.

Reflecting Telescopes  Reflecting telescopes utilize one or more concave mirrors for the objective lens to condense the light and a small lens called an eyepiece.

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