Royal Observatory, Cape of Good Hope

The Royal Observatory, Cape of Good Hope, is the oldest continuously existing scientific institution in South Africa. Founded by the British Board of Longitude in 1820, it now forms the headquarters building of the South African Astronomical Observatory.
The institution was located on a small hill south-east from the centre of Cape Town. Over the following century a suburb of the city grew up in the area; the suburb was named Observatory after the pre-existing Royal Observatory. It was declared a National Heritage Site in December 2018 and has also been the subject of an ICOMOS/IAU Case Study as a World Heritage Site.
History.
The proposal for a Southern observatory in all likelihood originated among the same group of people who founded the Royal Astronomical Society in the United Kingdom. Its official establishment took place on 20 October 1820 through an Order in Council of King George IV of the United Kingdom. It remained a separate entity until 1972 when it was amalgamated with the Republic Observatory Johannesburg to form the present-day South African Astronomical Observatory. Its site is now the headquarters of the South African Astronomical Observatory.
In accordance with its mandate, the principal activity of the Observatory was Astrometry and it was over its existence responsible for publishing many catalogues of star positions. In the 20th century it turned in part towards Astrophysics but by the nineteen-fifties the city lights of Cape Town had rendered work on faint objects impossible and a new site in the Karoo semi-desert was sought. An agreement to facilitate this was ratified on 23 September 1970. Nevertheless, several telescopes remained in operation until the 1990s. These are rarely made use of today except for public outreach events. Alan Cousins was the last serious observer to work from the Royal Observatory site.
The Royal Observatory was responsible for a number of significant events in the history of astronomy. The second HM Astronomer, Thomas Henderson, aided by his assistant, Lieutenant William Meadows, made the first observations that led to a believable stellar parallax, namely of Alpha Centauri. However, he lost priority as the discoverer of stellar parallax to Friedrich Wilhelm Bessel who published his own (later) observations of 61 Cygni before Henderson got around to his.
Around 1840, Thomas Maclear re-measured the controversial meridian of Nicolas-Louis de La Caille, showing that the latter's geodetic measurements had been correct but that nearby mountains had affected his latitude determinations
In 1882, David Gill obtained long-exposure photographs of the great comet of that year showing the presence of stars in the background. This led him to undertake in collaboration with J.C. Kapteyn of Groningen the Cape Photographic Durchmusterung, the first stellar catalogue prepared by photographic means. In 1886, he proposed to Admiral A.E.B. Mouchez of Paris Observatory the holding of an international congress to promote a photographic catalogue of the whole sky. In 1887 this congress took place in Paris and resulted in the Carte du Ciel project. The Cape Observatory was assigned the zone between declinations −40° and −52°. The Carte du Ciel is regarded as the precursor of the International Astronomical Union.
In 1897 Frank McClean, a close friend of Gill's and the donor of the McClean telescope, discovered the presence of oxygen in a number of stars using an objective prism attached to the Astrographic Telescope.
In 1911, J.K.E. Halm, then the Chief Assistant, put forward a pioneering paper on stellar dynamics in which he hypothesized that the star streams discovered by Kapteyn arose from a Maxwellian distribution of stellar velocities. This paper also contains the first suggestion that stars obey a mass-luminosity relationship.
A later 20th-century HM Astronomer, H. Spencer Jones, was active in an international project for determining the solar parallax through observations of the minor planet Eros.
In the second half of the twentieth century Alan Cousins set up very precise southern standards for UBV and introduced a widely used system of VRI photometry that enjoyed international recognition for precision.
In 1977 the occultation of the star SAO 158687 was observed by Joseph Churms from the former Royal Observatory and these observations provided needed confirmation of the Uranian rings discovered from the Kuiper aeroplane by Elliot et al.
During the 19th century the Observatory was regarded as the main advisor to the colonial government on scientific matters. it served as the repository for standard weights and measures of the Colony and was responsible for timekeeping and geodetic surveying. A magnetic observatory was constructed in 1841 but burned down during the following decade. The Observatory also possesses a long series of meteorological records.
The history of the Royal Observatory has been the subject of several works.
Astronomers at the Cape.
The Royal Observatory's directors were known as His or Her Majesty's Astronomers at the Cape. They were as follows: 
A full list of people who worked at the Royal Observatory and their publications, up to 1913, is given in Gill (1913). Other notable staff included:
Principal buildings.
A heritage survey was recorded in 2011 of a complete list of the buildings at the Observatory. They include:
Principal telescopes.
Historically, the main building contained a 10 feet focal length Transit by Dollond and a 6-feet Mural Circle by Thomas Jones. These were replaced by in 1855 by an 8-inch Transit Circle designed by George Biddell Airy, Astronomer Royal at Greenwich. The Airy instrument was removed in 1950. Some parts of these telescopes are in the Observatory's Astronomical Museum.
A 40-inch reflector by Grubb Parsons was installed in 1964 but was removed to Sutherland in 1972.
Astronomical Museum.
The former spectroscopic laboratory of the McClean telescope was converted into a museum in 1987, retaining the original 19th-century fittings. The building still contains the original hydraulic apparatus for raising the observing floor and a darkroom which contains specimens of darkroom equipment taken from various domes after photography went out of use. Items on display include telescope models, measuring machines, altazimuth instruments by Dollond (1820) and Bamberg (ca 1900), calculating machines, early office equipment, early electronic devices, lenses from early telescopes including the photographic telescopes of Gill, a clockwork telescope drive, a signal pistol, chemistry equipment etc.
Natural history.
The Royal Observatory site is situated in the Two Rivers Urban Park, a wetland area. The underlying rock is Malmesbury shale with a zone of greywacke and quartzitic limestone. Some of its original ecology is preserved and it supports a wide variety of animals and plant life. It is the northern limit of the Western Leopard Toad (Bufo Pantherinus) and the only remaining natural habitat of the rare iris, Moraea aristata.