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Encyclopedia :
R :
RA :
RAD :
Radio telescope |
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Radio telescopeIn 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. One of the first of these telescopes was the 76 metre dish at Jodrell Bank, constructed in the mid 1950's and which became operational in 1957.
The best-known (although non-steerable) radio telescope probably is the Arecibo radio telescope located in Arecibo, Puerto Rico. . As with many radio telescopes, this is an interferometric array formed from several smaller telescopes. Another well-known radio telescope is the Very Large Array (VLA), in Socorro, New Mexico. This telescope consists of an interferometric array formed from several receivers. The largest exisiting radio telescope array is the GMRT. A larger array, the 'LOw Frequency ARray' is currently being constructed in western Europe, consisting of 25000 small antennas over an area of several 100s of kilometres in diameter. The sub-field of astronomy related to observations made through radio telescopes is known as radio astronomy. Many celestial objects, such as pulsars or active galaxies (like quasars), produce radio-frequency radiation and so are best "visible" or even only visible in the radio region of electromagnetic spectrum. By examining the frequency, power and timing of radio emissions from these objects, astronomers can improve our understanding of the Universe Radio telescopes are also occasionally involved in SETI and tracking space probes (see Deep Space Network). Related topics
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