Berlin Observatory
The construction of the new Berlin Observatory proceeded from a cabinet order of 10 November 1830 according to the design of Schinkel. An approximately one hectare plot was acquired at a price of 15,000 Thalers in the present-day area of Berlin-Kreuzberg. The foundation stone was laid on 22 October 1832 and the observatory was ready by 1835, on the area currently bounded by the streets ″Friedrichstraße″, ″Besselstraße″ and ″Lindenstraße″. The southern end of the ″Charlottenstraße″ was later named ″Enckeplatz″ in honor of the director at that time and the observatory acquired the address of Enckeplatz 3 A (now: ″Enckestraße 11″).
Paul ten Bruggencate
After the war, the observations were continued. Ten Bruggencate established a second solar observatory in Switzerland where the weather conditions were more favorable compared to the often cloudy skies over Germany. The Locarno Observatory was planned and built in the late 1950s. Ten Bruggencate was the president of the Academy of Sciences Göttingen from 1958 until 1961. He also remained as director of the Göttingen University Observatory until his death in 1961. The Locarno Observatory became fully operational shortly after his death.
The Locarno Observatory was closed in 1984 and the equipment transferred to the Teide Observatory on Tenerife, Spain. Teide Observatory also hosts telescopes of the Kiepenheuer Institute for Solar Physics.
The crater Ten Bruggencate on the Moon is named after him.