Things You'll Need
Instructions
Choose the size for your primary mirror. Newton used a metal concave mirror of about two inches in diameter. Modern concave mirrors are usually made of glass or coated with aluminum.
Determine your primary mirror's focal length. Shine a bright light at the concave mirror and use a vertically held piece of cardboard to find the spot where the reflected light is the brightest. That is the focal point.
Make the main telescope tube. The length of the tube needs only to be longer than the primary mirror's focal length, and the tube should be only slightly wider than the diameter of that mirror.
Attach the primary mirror snugly in one end of your telescope tube. Use brackets screwed into the tube to hold the mirror without damaging it.
Fix a flat mirror at a 45-degree angle within the tube. This diagonal mirror must be at the location of the primary mirror's focal point.
Build the observing tube above the diagonal mirror. This is a small tube rising vertically from the main tube, the width of your observing lenses. Use glue to connect the tubes securely.
Insert your magnifying lens into the observing tube. Although any convex lens will work, you will get the best results with commercial telescope lenses. Secure the lens with a screw in the observing tube: tighten the screw to hold the lens, loosen it to release.