Named after | Dwingeloo |
---|---|
Part of | Top 100 of Dutch monuments 1940-1958 |
Location(s) | Dwingeloo, Drenthe, Netherlands |
Coordinates | 52°48′43″N6°23′46″E / 52.8119°N 6.3961°E |
Telescope style | observatory radio telescope |
Diameter | 25 m (82 ft 0 in) |
Related media on Commons | |
The Dwingeloo Radio Observatory is a single-dish radio telescope near the village of Dwingeloo (Dutch pronunciation: [ˈdʋɪŋəloː] ) in the northeastern Netherlands. Construction started in 1954, and the telescope was completed in 1956. The radio telescope has a diameter of 25 m. [1] At the time of completion it was the largest radio telescope in the world, but it was overtaken in 1957 by the 250 foot (76 m) Lovell Telescope.
As of 2000, it was no longer in operation in an official capacity. Since August 2009, the radio telescope has been a national heritage site ( rijksmonument ). [1] The telescope dish was removed for restoration in June 2012. [2] The "C.A. Muller Radio Astronomy Station" foundation ("CAMRAS" for short) restored the telescope to working order. The dish was remounted in November 2012. [3]
Radio amateurs along with amateur and professional astronomers, use the telescope for projects, one being Earth–Moon–Earth communication, also known as moonbounce, which allows for people on different parts of Earth to communicate via the Moon. In this technique, radio wave signals are aimed at the Moon by one location, bounce off the Moon's surface, and are detected by an antenna at a different location on Earth. "Visual Moonbounce" is a technology to moonbounce images at amateur-radio frequencies. It is based on artistic research with the Dwingeloo Radiotelescoop by artist Daniela De Paulis as part of her project "OPTICKS" [4] [5] [6]
The radio telescope is owned by ASTRON, the Netherlands Institute for Radio Astronomy. The site of the Dwingeloo Radio Observatory also houses most of the staff of ASTRON and a test site for the Low Frequency Array radio telescope, LOFAR.
Two galaxies are named after this telescope: Dwingeloo 1 and Dwingeloo 2.
A radio telescope is a specialized antenna and radio receiver used to detect radio waves from astronomical radio sources in the sky. Radio telescopes are the main observing instrument used in radio astronomy, which studies the radio frequency portion of the electromagnetic spectrum emitted by astronomical objects, just as optical telescopes are the main observing instrument used in traditional optical astronomy which studies the light wave portion of the spectrum coming from astronomical objects. Unlike optical telescopes, radio telescopes can be used in the daytime as well as at night.
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Earth–Moon–Earth communication (EME), also known as Moon bounce, is a radio communications technique that relies on the propagation of radio waves from an Earth-based transmitter directed via reflection from the surface of the Moon back to an Earth-based receiver.
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Owens Valley Radio Observatory (OVRO) is a radio astronomy observatory located near Big Pine, California (US) in Owens Valley. It lies east of the Sierra Nevada, approximately 350 kilometers (220 mi) north of Los Angeles and 20 kilometers (12 mi) southeast of Bishop. It was established in 1956, and is owned and operated by the California Institute of Technology (Caltech). The Owens Valley Solar Array portion of the observatory has been operated by New Jersey Institute of Technology (NJIT) since 1997.
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ASTRON is the Netherlands Institute for Radio Astronomy. Its main office is in Dwingeloo in the Dwingelderveld National Park in the province of Drenthe. ASTRON is part of the institutes organization of the Dutch Research Council (NWO).
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