refracting telescope
Quick Summary
A refracting telescope, or refractor, uses a lens to bend light and magnify distant objects. This bending of light is called refraction. The primary lens, known as the objective lens, gathers light from a celestial object and focuses it. A second lens, the eyepiece, then magnifies this focused image for the observer.1
Refracting telescopes are commonly used to view objects like the Moon, planets such as Jupiter and Mars, and binary stars. The size of the objective lens, called the aperture, determines the telescope's light-gathering power. While effective, refractors can suffer from distortions like chromatic aberration, where different colors of light do not focus at the same point. The largest refractor ever built had a 1-meter aperture.12
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