Radio telescope

In contrast to an "ordinary" telescope, which produces visible light images, a radio telescope "sees" radio waves emitted by radio sources, typically by means of a large parabolic ("dish") antenna, or arrays of them. The first of these was the 9m telescope constructed by Grote Reber in 1937. In the early 1950s the Cambridge Interferometer mapped the radio sky to produce the famous 2C and 3C surveys of radio sources. In the late 1950s and early 1960s the largest single-dish radio telescope in the world was the 76 metre telescope at Jodrell Bank, which became operational in 1957. This was just the latest of many radio telescopes constructed during the middle of the 20th Century, and has been surpassed by more modern telescopes and arrays of telescopes.

See also

• Aperture synthesis
• Complete list of radio telescopes on Wikipedia
• Alternative, smaller list of radio telescopes