Effelsberg 100-m Radio Telescope

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Effelsberg 100-m Radio Telescope
Effelsberg total2.jpg
Radio telescope at Effelsberg
Organisation Max Planck Institute for Radio Astronomy in Bonn
Location(s) Effelsberg, North Rhine-Westphalia
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Altitude 319 m
Wavelength radio 408 MHz – 86 GHz
Built 1971
Telescope style parabolic reflector
Diameter 100 m
Collecting area 7,850 m2
Focal length 30 m
Mounting alt-azimuth fully steerable primary
Website http://www.mpifr-bonn.mpg.de/8964/effelsberg
Commons page [[Commons:Category:Lua error in Module:Wikidata at line 446: attempt to index field 'wikibase' (a nil value). |Related media on Wikimedia Commons]]

The Effelsberg 100-m Radio Telescope is a radio telescope in the Ahrgebirge (part of the Eifel) in Bad Münstereifel, district of Euskirchen, North Rhine-Westphalia, Germany. For 29 years the Effelsberg Radio Telescope was the largest fully steerable radio telescope on Earth. In 2000 it was surpassed by the Robert C. Byrd Green Bank Telescope in Green Bank, West Virginia with an elliptical 100 by 110-metre aperture.[1]

Geography

The telescope is located about 1.3 km northeast of the village of Effelsberg, a southeastern part of the town of Bad Münstereifel. It is placed less than 300 m west of the 398 m high Hünerberg, which is already in the neighbouring Land of Rhineland-Palatinate.

In the vicinity of the telescope, the boundary of the Land of North Rhine-Westphalia is the Effelsberger Bach, which runs only a few metres east of the telescope. The Effelsberger Bach is 6.5 km long, flowing from the Effelsberger Wald into the Sahrbach, which in turn flows south and into the Ahr river.

A hiking path leads past the telescope; in 2004 part of this was turned into a planet trail with information panels about the Solar System with its planets. The trail ends at the 39 cm model of the Sun next to the visitor centre.

Radio telescope

The Effelsberg radio telescope is operated by the Max Planck Institute for Radio Astronomy in Bonn, the radio astronomy institute from the Max-Planck-Gesellschaft. It was constructed from 1968 to 1971 and inaugurated on 1 August 1972. A major technical difficulty in building a radio telescope of 100 m diameter was how to deal with the deformation as the – supposedly parabolic – mirror moves and tilts. The Finite element method was used to construct the mirror support in such a way that the deformed mirror will always take a parabolic shape. The focus will move during such deformation, and the receiver has to be moved accordingly. Tests after completion of the telescope showed that the intended accuracy of the mirror surface of 1 mm had not only been met, but exceeded significantly.

About 45% of the observing time is available to external astronomers. The Effelsberg 100-m telescope was involved in several surveys, including the one at 408 MHz (73 cm) by Haslam et al.[2][3]

Technical data of the antenna[4]
Reflector Diameter 100 m
Aperture 7,854 m2
Number of Surface Elements (Panels) 2,352
Shape Accuracy of Surface < 0.5 mm
Focal Length in Prime Focus 30 m
Secondary Mirror Diameter (Gregory-Reflector) 6.5 m
Aperture Stop
– in Prime Focus f/0.3
– in Secondary Focus f/3.85
Angular Resolution (Beam Width)
– at 21 cm wavelength (1.4 GHz) 9.4' (arc minutes)
– at 3 cm wavelength (10 GHz) 1.15' (arc minutes)
– at 3.5 mm wavelength (86 GHz) 10" (arc seconds)
Azimuth Track Diameter 64 m
Setting Accuracy of Track ±0.25 mm
Azimuth Range 480°
Maximum Rotation Speed 30°/min.
Pointing Accuracy
– Blind Pointing 10"
– Repeatability 2"
Power Output of the 16 Azimuth Drives 10.2 kW each
Radius of Elevation Gear Track 28 m
Elevation Range from 7° to 94°
– during observations from 8.1° to 89°
Maximum Tilt Speed 16°/min.
Power Output of the 4 Elevation Drives 17.5 kW each
Total Weight 3,200 t
Construction Period 1968–1971
Height of Track above Sea Level 319 m
Commencement of Operation 1 August 1972
Constructed by Arbeitsgemeinschaft Krupp/MAN

See also

External links

References

  1. ↑ Newly Commissioned Green Bank Telescope Bags New Pulsars, NRAO, 2002-01-04
  2. ↑ Haslam, C. G. T.; Salter, C. J.; Stoffel, H.; Wilson, W. E., A 408 MHz all-sky continuum survey. II – The atlas of contour maps, Astronomy and Astrophysics Supplement Series, vol. 47, Jan. 1982, p. 1, 2, 4–51, 53–142.
  3. ↑ http://adsabs.harvard.edu/cgi-bin/bib_query?1981A%26A...100..209H
  4. ↑ http://www3.mpifr-bonn.mpg.de/div/effelsberg/antenna/antenna_spec.html
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