Refracting telescopes use lenses to bend and focus light. The main components of a refracting telescope include a large objective lens, which gathers light, and an eyepiece lens, which magnifies the image formed by the objective lens. When light enters the telescope, it is refracted, or bent, by the objective lens, bringing the image into focus at the eyepiece where it can be viewed by the observer.
Reflecting telescopes use mirrors to gather and focus light. The primary mirror at the bottom of the telescope gathers incoming light and reflects it back up to a smaller secondary mirror, which in turn reflects the light to the eyepiece. Reflecting telescopes are often preferred for astronomical observations because they can be made much larger and are free from the color distortion that can occur in refracting telescopes.