Refracting telescope

A refracting telescope (refractor) is a telescope which uses lenses to refract light. This refraction causes parallel light rays to converge at a focal point; while those which were not parallel converge upon a focal plane. This can enable a user to view a distant object as if it were brighter, clearer, and/or larger. These are similar to microscopes. The monocular is a type of refractor. A typical refractor has two lenses, an objective lens and an eyepiece lens. The objective lens has two pieces of glass (with different densities), "crown" and "flint glass". Each side of each piece is ground and polisheded, and then the two pieces are glued together. The curvatures are designed to cancel chromatic and spherical aberration.

Table of contents

1 Technical Difficulties 2 Notable Refracting Telescopes 3 See also:

Technical Difficulties

For research purposes, refracting telescopes have become unpopular. They are criticized for their relatively high-degree of chromatic and spherical aberration. There is also the problem of lens sagging, a result of gravity affecting glass. There is a further problem of mis-refraction; caused by air bubbles trapped within the lenses. In addition, glass is opaque to certain wavelengths, and even visible light is dimmed when it passes through glass. Many of these problems are avoided by using reflecting telescopes.

Notable Refracting Telescopes

• Yerkes Observatory (102cm)
• Lick Observatory (91cm)
• Paris Observatory (83cm + 62cm)
• Nice Observatory (76cm)