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Astronomical telescopes come in a wide variety, ranging from the plastic tube sold in toy stores to the famous Hubble telescope flying in the sky. Here, we only focus on the most basic information necessary for a backyard astronomer.

An astronomical telescope is used to collect light from a celestial object and produce a magnified image. There are two basic types of optical telescopes: refractor and reflector. The former uses lenses and the latter uses mirrors. The primary lens or mirror that focuses light is the objective. Both kinds use an eyepiece to magnify the image formed by the objective. In astronomical observations, refractors are commonly used for lunar and planetary studies, while reflectors are preferred for extragalactic studies.

In addition to these two common types, there are a number of other designs which use a combination of lenses and mirrors to take advantages of both refractors and reflectors, such as Schmidt-Cassegrain telescopes and Maksutov telescopes.

reflectors

How reflector telescopes work

The reflecting telescope (shown above) was first designed by Isaac Newton in 1668. Here, a primary parabolic mirror reflects light rays to an inclined flat mirror, which, in turn, reflects the rays to an observer located at the side of the tube. This design has essentially remained the same today in most amateur reflectors.

The most attractive feature of a reflector telescopes is that it provides the lowest dollar/aperture ratio of any telescope type. Therefore, for the same money, a reflector gathers most light, which is important in deep space viewing. Small amateur reflectors, such as a 3" (76 mm) or a 4.5" (114 mm) are also light enough for easy transportation. Because of the open tube design, a reflector requires alignment and cleaning once a while. The image from a reflector is usually upside-down and is therefore not suitable for terrestrial viewing.

refractors


How refractor telescopes work

The refracting telescope (shown above) was invented in 1609 by Galileo Galilei who used it to discover Jovian satellites, lunar mountains, et al. Galileo's refracting telescope suffered from a number of defects in image formation, particularly aberrations, due to the use of simple lenses. Modern optical telescopes use compound objective lenses to minimize aberrations. The compound lens consists of one convex lens of crown glass and one concave lens of flint glass. In addition, all lenses are coated with anti-reflective coatings to maximize transmission. In common designs for amateur astronomy, light from the objective lens is often turned 90 degrees by a flat mirror before entering the eye piece.

Refractors provide the best image quality among amateur telescopes, thanks in particular to the compound objective lens. Images of planets and the Moon are extremely crispy and sharp. They are also used for viewing objects on land, when an erecting eye piece is used. In addition to their high performance, refractors are also maintenance-free and very portable due to their light weight and compactness. Thus, refractor has always been one of the most favorable among amateur astronomers. The disadvantage of a refractor telescope is that it is the most expensive in terms of dollar/aperture ratio. However, thanks to the web, you can now directly buy from the factory at very affordable prices.

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