First designs for the 100-metre radio telescope were presented by the companies Krupp and MAN, and eventually Krupp was awarded the contract. The actual building work was then carried out by the consortium “Arbeitsgemeinschaft Stahlbau-Radioteleskop”, or ARGE STAR (consortium steel construction radio telescope), which was founded especially for this purpose.
On the lookout for an appropriate location
The search for an appropriate location began several years before the construction work. There were several important points to consider:
- No proximity to larger human settlements
- No proximity to high voltage transmission lines
- No proximity to radio and television stations, if possible
It was also hoped that the location would make it possible to avoid radiation from radar transmitters, but this proved impossible. Therefore, it was decided to position the telescope in a valley where the surrounding landscape would guarantee the utmost protection from earthly signals. The valley needed to be running from North to South so that celestial objects like the centre of the Milky Way could still be observed.
One out of 30: Effelsberg
From a selection of more than 30 different locations a valley near the village of Effelsberg in the Eifel region was picked. The proximity to Bonn was one of the reasons for the decision. From a selection of more than 30 different locations a valley near the village of Effelsberg in the Eifel region was picked. The proximity to Bonn was one of the reasons for the decision. Another crucial point was the fact that the valley was so deep that even in its highest position, the primary focus of the telescope was still protected by the high hills surrounding the valley. In addition, within several kilometres the landscape features several hills which are higher than the top the telescope by at least 100 metres.
Start of construction in February 1968
The telescope is situated in a valley oriented in the North–South direction. Two creeks had to be relocated before building work was begun. In February 1968, when the site had been prepared, the foundation was laid.
The valley’s soil consists of greywacke, which is an old metamorphised sedimentary stone. This stone is solid, yet craggy. Therefore, the first measure step was to harden the soil by adding concrete. For stability reasons, the foundations had to be strongly connected to the bedrock. The base ring which carries the weight of the telescope rests on 154 concrete pillars which are between 7 and 11 metres long.
Completion in 1972
The building of the steel construction began in October 1968. The twelve parts of the primary mirror dish were built and assembled on a flattened assembly field, right next to the telescope. In December 1969, the first of the twelve parts was lifted up and positioned. April 1970 saw the lifting up of the twelfth part and thus the completion of the steel skeleton, the framework of the telescope. On August 1st, 1972, the Max Planck Institute for Radio Astronomy celebrated the launch into operation of the 100-metre radio telescope in Effelsberg.
New secondary mirror under construction
A new secondary mirror for the 100-metre radio telescope was put into operation in October 2006. An active optic system (with 100 actuators) makes it possible to correct the surface of the secondary mirror, allowing an optimal operation of the radio telescope even at millimetre wavelengths. This improvement will ensure that Germany continues to have one of the world's most flexible and most precise radio telescopes.
Die feierliche Inbetriebnahme des 100-Meter Radioteleskops Effelsberg fand dann am 1. August 1972 statt.
Seit der Inbetriebnahme wird das Teleskop ständig dem aktuellen Stand der Technik angepaßt.
1976: Erstellung des Erweiterungsbaus am Institutsgebäude
1977: Brand im Besucherpavillon, Neubau
1982: Austausch Paneele im inneren Bereich
1985: erster Austausch des Subreflektors
1996: Ersatz der Laufschiene
2000: Erneuerung der äußeren Paneelringe
2002: Installation neuer Getriebe für den Azimut-Antrieb
2004: Errichtung des Faradayraums
2005: Fertigstellung des ersten Teils der LOFAR-Station
Neuer Sekundärspiegel im Bau
2006 Für das 100-m-Radioteleskop Effelsberg wurde ein neuer Sekundärspiegel gebaut, der seit Oktober 2006 im Einsatz ist. Mit einer motorgesteuerten Korrektur der Oberfläche des Sekundärspiegels (aktive Optik mit ca. 100 Aktuatoren) ist es möglich, das Radioteleskop auch bei Millimeterwellenlängen optimal zu betreiben. Mit dieser Verbesserung steht in Deutschland eines der weltweit flexibelsten und leistungsfähigsten Radioteleskope bereit.
2009: Revision der Elevationsgetriebe
Fertigstellung des zweiten Teils der LOFAR-Station