Instruct: Given a question, retrieve passages that answer the question.
Query: When was the Berlin Observatory created?
The Berlin Observatory (Berliner Sternwarte) is a German astronomical institution with a series of observatories and related organizations in and around the city of Berlin in Germany, starting from the 18th century. It has its origins in 1700 when Gottfried Leibniz initiated the "Brandenburg Society of Science″ (Sozietät der Wissenschaften) which would later (1744) become the Prussian Academy of Sciences (Preußische Akademie der Wissenschaften). The Society had no observatory but nevertheless an astronomer, Gottfried Kirch, who observed from a private observatory in Berlin. A first small observatory was furnished in 1711, financing itself by calendrical computations.
At the end of the 19th century, the rapid growth of Berlin led to the fact that the Observatory which was once on the edge of the city was now fully surrounded by buildings, and therefore observational activities were nearly impossible to a level required for research. In the middle of the 1890s Wilhelm Foerster and others proposed the building of a new observatory outside of the metropolitan area.
In September 1699, the Reichstag decided to introduce an "improved calendar" to the Protestant German states without having to take on the Gregorian Calendar, introduced by Pope Gregory XIII in 1582. The 'improved calendar' was introduced the following year and resulted in 18 February 1700 being followed by 1 March. A patent for the calendar was granted to the planned Berlin Observatory by Prince-elector Frederick III on 10 May 1700 and eight days later Gottfried Kirch was appointed to Director of the Observatory. On 11 July (his 43rd birthday) the Kurfürst signed a document formally founding an Academy and an Observatory in Berlin. Therefore, Berlin received an academy just like those already existing in London, Paris and Rome - the Prussian Academy of Sciences (originally German name: ″Kurfürstlich-Brandenburgische Societät der Wissenschaften″), based on the plans of Gottfried Wilhelm Leibniz. Leibniz became the first president of the Academy. The fees resulting from the calendar patent were the almost single financial basis of the institution for a long period. The society originally had no actual observatory of its own and Kirch carried out his observations at various private observatories including, from 1705, the private observatory of Geheimrat Bernhard Friedrich von Krosigk on the Wallstrasse, in Cölln. Kirch was assisted by his wife Maria Margarethe and his son Christfried. Maria Margarethe discovered, among other things, the comet of 1702. In the meantime the Kurfürst had been raised in 1701 to the rank of King in Prussia. On 1 January 1710, the capital was expanded by uniting the previously independent towns of Dorotheenstadt, Friedrichstadt, Friedrichwerder, and Cölln and Berlin (the oldest ones).
In 1946 the city of Berlin renamed the observatory "Archenhold-Sternwarte". On 1 June 1948 Diedrich Wattenberg, who had been working with Archenhold, was made director. Annual visitor numbers rose from 8,000 in 1946 to 25,000 in 1949. In 1958, the Great Refractor was decommissioned, but retained as a monument of technology. From 1959 onwards, the observatory was increasingly used for school education in physics and astronomy. To support this, in the 1960s, two further domes were erected in the grounds. A lecture theatre was also added, and in 1966 the #Solar physics cabinet][solar physics cabinet was created, which could project the Sun at diameter or a solar spectrum at length.
In 1878 reference heights were taken from the Amsterdam Ordnance Datum and transferred to the New Berlin Observatory in order to define the Normalhöhenpunkt 1879. Normalnull has been defined as a level going through an imaginary point 37.000 m below "Normalhöhenpunkt 1879". When the New Berlin Observatory was demolished in 1912 the reference point was moved east to the village of Hoppegarten (now part of the town of Müncheberg, Brandenburg, Germany).
From 1883 he was assistant and observer at the Munich observatory. In 1896 he was named director of the Astronomisches Rechen-Institut and professor of theoretical astronomy in Berlin, a position he held until 1909, when he became director of the Strasbourg observatory.
The Berlin Observatory became known worldwide when Johann Gottfried Galle discovered the planet Neptune in 1846. The discoveries of the canal rays by Eugen Goldstein in 1886 in the physical laboratory of the observatory and of the variation in the altitude of the Earth's pole by Karl Friedrich Küstner in 1888 were likewise important.
Wilhelm Foerster led the observatory until the end of his life in 1903. It was his impulse that led to the erection of the Astrophysikalischen Observatoriums Potsdam in 1874 for on the Telegrafenberg in Potsdam. On the Telegrafenberg stood formerly the „Telegraphenstation4" which given the hill its name. In the same year Foerster founded the Berlin Astronomische Rechen-Institut (as "Rechen-Institut zur Herausgabe des Berliner Astronomischen Jahrbuchs"), on the basis of the ever-growing extent of calculation of astronomical ephemerides, which occupied its own building at ″Lindenstraße 91″, but on the grounds and in association with the observatory. Most of the astronomers now worked in this theoretical section– separate from the practical, observational section. The section was led by Friedrich Tietjen, who had been working at the obervatory since 1861. In 1865 he discovered the asteroid (86) Semele. After Tietjens death, Julius Bauschinger was called to Berlin in 1896 as his successor. In the following year he achieved in making the institute fully independent of the observatory.[29] In 1912 it moved into a new building in Berlin-Lichterfelde. In 1944 it was placed under the control of the Navy and transferred to Sermuth in Saxony to avoid the bombing. After the Second World War the greater part was brought to Heidelberg in 1945. Only a small remaining section returned to the observatory, which by now had moved to Potsdam-Babelsberg and it was again incorporated in 1956.[30]
When the time came to seek a successor by virtue of Bode's retirement, both Carl Friedrich Gauß and Friedrich Wilhelm Bessel turned the post down.[13] On the recommendation of Bessel, Johann Franz Encke,[14] since 1822 Director of the Seeberg Observatory near Gotha, was called to Berlin by King Frederick William III in 1825 and named director of the Berlin Observatory. Thanks to the influence of Alexander von Humboldt, expensive instruments were obtained and with his aid Encke was also able to get the Prussian King to agree to the construction of a new observatory, situated on the edge of the city at that time. A condition was that the observatory should be made available to the public on two evenings in the week.
The last two scientific events took place when Wilhelm Julius Foerster was director of the observatory, which was meanwhile attached to the University of Berlin. He prepared the basis for the astronomical observatories in Potsdam: in 1874 the foundation of the AOP on the Telegrafenberg and in 1913 the removal of the Berlin Observatory to Babelsberg.
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 Enckeplatz3A (now: ″Enckestraße 11″).[20]
At the end of the 19th century the Berlin Observatory, originally built outside the border of the town, was enclosed by blocks of flats, so scientific observations were almost impossible. Therefore, Foerster proposed the removal of the observatory to a place outside Berlin with better observational conditions. In 1904 he appointed Karl Hermann Struve, former director of the observatory of Königsberg, as his successor to realize this project.
On 23 September 1846, Galle and astronomy student Heinrich Louis d’Arrest, since 1845 assistant at the observatory, discovered the planet Neptune, on the basis of positional calculations send by the Frenchman Urbain Le Verrier. After an initial lack of success they conferred the Le Verrier data with a newly published sheet of the „Berliner Akademische Sternkarte", edited by the Prussian Academy of Science. The letter from Le Verrier had coincidentally reached his close acquaintance Galle on the same day as Encke's 55th birthday, who gave his permission to search around the given celestial positions. At other observatories, the request of the French astronomer was viewed as not having sufficiently promising chances of success, of detecting another large planet on the basis of the deviations between theory and observations for the orbit of Uranus. This included Paris Observatory, whose director Le Verrier later became.[25] By virtue of the discovery of Neptune, Berlin Observatory gained worldwide renown.
The new location in the original Schlosspark was a part of the Gemeinde . The "villa settlement" of Neubabelsberg was united in 1938 with the town of to form the town of Babelsberg. Then almost straightaway in 1939 this became incorporated into Potsdam. The designation "Berlin-Babelsberg" was nevertheless retained by the observatory for a few years still. Only after 1945 was the word Berlin discarded.[42] Ihr IAU-Code ist 536.
The tower of the old observatory served as Telegraphenstation1 between 1832 and 1849, one of the 62 stations of the Prussian optical telegraph from Berlin via Köln to Koblenz.[6] On 3 July 1903 the tower was torn down.[19] The entire area of the Marstall complex between Dorotheenstraße and Unter den Linden was taken over in 1914 by the Berlin State Library.
After test observations by Paul Guthnick in the summer of 1906 a new site was found on a hill in the eastern part of the Royal Park of Babelsberg. The ground was placed at the observatory's disposal by the crown free of charge. The costs of the new buildings and the new instruments amounted to 1.5 million Goldmark and could be covered by selling the landed property of the Berlin Observatory. The old observatory built by Schinkel was pulled down later. In June 1911 the construction of a new observatory began in Babelsberg and on 2 August 1913 the removal from Berlin to Babelsberg was complete.
In 1927 Fanselau started work at the Meteorological Institute of the University of Berlin and the following year moved to the Magnetic Observatory, led by Adolf Schmidt. The first few years he was engaged in the construction of the observatory in Niemegk. The electrification of the Berlin Stadtbahn disturbed geomagnetic observations in Potsdam and Seddin. In 1929 he developed the Fanselau coil, a modified version of the Helmholtz coil, which uses a special arrangement of coils to improve the homogeneity of the generated magnetic field. In 1933 he became head of the observatory at Niemegk. In 1935 he qualified as a professor of geophysics in Berlin, and in 1941 he commenced a teaching position there. In 1940 he joined the Nazi Party.
Born in Hitdorf am Rhein, he studied at the University of Bonn receiving his doctorate in 1901 under Friedrich Küstner. He worked from 1901 at the Royal Observatory of Berlin and studied variable stars and specifically Mira. As Berlin expanded, it became less possible to conduct astronomical observations there and Guthnick used, from 1906 onwards, the local park known as Babelsberg. An observatory was later built there after approval by the government. He was appointed professor of astrophysics at the University of Berlin in 1916. In 1921, he became director of the Babelsberg Observatory. 
A brief History of Astronomy in Berlin and the Wilhelm-Foerster-Observatory Astrophysics Institute Potsdam
Friedrich Simon Archenhold (2 October 1861 in Lichtenau, Westphalia – 14 October 1939 in Berlin) was an astronomer who founded the Treptow Observatory (today the Archenhold Observatory) in Berlin-Treptow. He graduated from the Realgymnasium in Lippstadt before entering Friedrich Wilhelm University in 1882, where he and Wilhelm Förster founded the Urania Astronomical Society at the Berlin University Observatory.
He was born in Berlin and received his education at universities in Bonn and Berlin, then became an assistant at Bonn Observatory in 1914. In 1930 he became a full professor and was appointed director of the Leipzig Observatory and Vienna Observatory. Between 1918 and 1974 he published nearly 100 scientific papers. In 1931–32, he and Heribert Schneller discovered that Zeta Aurigae is an eclipsing binary.
Johann III Bernoulli served from 1764 to 1787 as Director of the Old Observatory and was succeeded by Johann Elert Bode. Lambert fetched Bode to Berlin in 1773, in order to publish an almanac; after Lambert' death, Bode became the sole editor.[8] The first edition of the Berliner Astronomisches Jahrbuch (for 1776) had already appeared by 1774, initiating the longest-lasting publication series in astronomy, lasting until 1959. By virtue of this medium, Berlin Observatory developed into an information source of prime importance within Europe.[9] Originally Bode had the venerable Christine Kirch to assist him with the work on the calendar. In 1774, he married a granddaughter of one of her sisters; she was likewise entrusted with astronomical work in line with the Kirch family tradition.[10] Christine Kirch died in 1782. As director of the observatory, Bode was able, through favors from Frederick William III of Prussia, to extend the till then rather third-class-equipped institution with a second observing level. When Bode entered a petition to this effect on 2 November 1798, space for observing within the tower was still limited to the third storey. The two storeys over it were united to a single spacious level. From there, the observing activities could be extended, once the calculated cost of 4465 Thalers and the plan was approved on 7 April 1800 and the required conversion was completed by June 1801. The construction work was supervised by Oberhofbaurat and Schlossbaumeister Bock.[11]
Carl Gustav Witt (October 29, 1866 – January 3, 1946) was a German astronomer and discover of two asteroids who worked at the Berlin Urania Observatory, a popular observatory of the Urania astronomical association of Berlin.
By virtue of the nationalization of the Sonnenberg Observatory the Universitätssternwarte Berlin-Babelsberg took it on as a new department in 1931, i.e. an out-station in .[43]
Because Foerster was not a member of the Academy, the Observatory was separated from the Academy in 1889 and affiliated to the Berlin University.[31] The original Academy Observatory had already been used by the University since the founding of Berlin University in 1809.[32] In 1890 Friedrich Simon Archenhold became a worker at the Observatory and erected on the instructions of Foerster a photographic outpost on the Halensee in Grunewald for the photographing of nebulae.[33]