The Refracting Telescope consists of a long hollow tube with a large lens, known as the objective lens, situated at the front end and an eyepiece at the opposite end. Starlight enters the telescope through the objective lens which gathers it and focuses it into the eyepiece. The eyepiece magnifies the image thereby making distant objects appear closer.
The Refracting Telescope has several advantages:
- its simple construction makes the refractor more sturdy and is therefore less liable to go out of alignment than a Reflecting Telescope; indeed a refractor can go many years without needing any realignment
- small refractors are extremely portable and very easy to set up, an important consideration if you need to travel long distances to reach a dark-sky site
- the telescope tube assembly is sealed at both ends (by the lenses), therefore providing protection against dust and moisture
- all Refracting Telescopes suffer from chromatic aberration, which leads to false colour appearing around images, due to the fact that they use lenses to focus light
- small errors in the grinding of the lens can result in distorted images
- larger telescopes are less portable
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