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Encyclopedia > Radiotelescope

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.

Enlarge
The Parkes 64 metre radio telescope in New South Wales, Australia (the bigger of the two shown)

The largest individual radio telescope is the RATAN-600 (http://www.sao.ru/ratan/) (Russia) with 576 metre diameter of circular antenna (RATAN-600 description (http://www.sao.ru/ratan/technic/desc.html.en)). The largest radio telescope in Europe is the 100 metre diameter antenna in Effelsberg, Germany, which also was the largest fully steerable telecope for 30 years until the Green Bank Telescope was opened in 2000. The largest radio telescope in the United States unitil 1998 was Ohio State University's The Big Ear. A typical size of the single antenna of a radio telescope is 25 metre, dozens of radio telescopes with comparable sizes are operated in radio observatories all over the world.


The best-known (although non-steerable) radio telescope probably is the Arecibo radio telescope located in Arecibo, Puerto Rico.


Another well-known radio telescope is the Very Large Array (VLA), in Socorro, New Mexico. The largest RT 'LOw Frequency ARray' is currently being constructed in western Europe [1] (http://www.lofar.org/), 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

External Link

  • LOFAR (http://www.lofar.org/)

  Results from FactBites:
 
History of the Ohio State University Big Ear Radiotelescope (2171 words)
The Ohio State Radiotelescope is larger than three football fields in size, and equivalent in sensitivity to a circular dish 175 feet in diameter.
The beam of the telescope is elliptical, being 40 minutes of arc in the declination (vertical) direction, and 8 minutes of arc in the right ascension (horizontal) direction.
Of course, there are always many distant stars and galaxies in the beam of a radiotelescope all the time, but that is not significant.
  More results at FactBites »


 

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