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Newtonian Reflecting Telescopes


Newtonian reflector telescopes use a concave parabolic primary mirror to collect and focus incoming light. A small, flat diagonal mirror reflects the converging beam of light into the eyepiece on the side of the tube near the top.

Newtonian telescopes offer a number of excellent advantages including:

  • Bright images and complete freedom from color aberrations.
  • Excellent for observing faint deep-sky objects such as nebulae, star clusters and remote galaxies.
  • Lowest cost per inch of aperture due to use of mirrors rather than costly lenses.
  • Fast photographic speeds: f/4 to f/9.

The 6" Newtonian telescope is the most popular size telescope for the serious beginning or intermediate-level astronomy enthusiast, and for good reason. The large light gathering power of the 6" telescope makes it ideal for dark-sky observations of galaxies, star clusters and nebulae, as well as lunar and planetary observing. This makes for a very useful and versatile instrument that can take an observer from his first views through years of advanced observing.


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