![]() Main building of the Royal Observatory, Cape of Good Hope | |
Organization | South African Astronomical Observatory |
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Observatory code | 051 ![]() |
Location | Observatory, Cape Town |
Coordinates | 33°56′05″S18°28′39″E / 33.9347°S 18.4776°E |
Altitude | 15m |
Established | 20 October 1820 |
Closed | 31 December 1971 |
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The Royal Observatory, Cape of Good Hope, is a former scientific institution in South Africa. [1] Founded by the British Board of Longitude in 1820, its main building is now the headquarters building of the South African Astronomical Observatory.
The institution was located on a small hill 5 kilometres (3.1 mi) south-east from the centre of Cape Town. During the succeeding century a suburb of the city formed in the area; the suburb was named Observatory after the pre-existing Royal Observatory. It was declared a National Heritage Site in December 2018 [2] and has also been the subject of an ICOMOS/IAU Case Study as a World Heritage Site. [3]
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. [4] The official establishment of the Royal Observatory, Cape of Good Hope occurred on 20 October 1820 [1] 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. [5] 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. [6] [7]
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. [8] [9]
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. [10]
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. [11]
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. [12]
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. [13]
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. [14] 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. [15] [16] [17] [18] [19]
The Royal Observatory's directors were known as His or Her Majesty's Astronomers at the Cape. They were as follows: [17]
A full list of people who worked at the Royal Observatory and their publications, up to 1913, is given in Gill (1913). [15] Other notable staff included:
A heritage survey was recorded in 2011 of a complete list of the buildings at the Observatory. [20] They include:
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. [3] Some parts of these telescopes are in the Observatory's Astronomical Museum.
A 40-inch reflector by Grubb Parsons was installed in 1964 but moved to Sutherland in 1972.
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. [22] 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.
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. [23]
Astrometry is a branch of astronomy that involves precise measurements of the positions and movements of stars and other celestial bodies. It provides the kinematics and physical origin of the Solar System and this galaxy, the Milky Way.
Abbé Nicolas-Louis de Lacaille, formerly sometimes spelled de la Caille, was a French astronomer and geodesist who named 14 out of the 88 constellations. From 1750 to 1754, he studied the sky at the Cape of Good Hope in present-day South Africa. Lacaille observed over 10,000 stars using just a half-inch refracting telescope.
Edward James Stone FRS FRAS was an English astronomer.
The Carte du Ciel and the Astrographic Catalogue were two distinct but connected components of a massive international astronomical project, initiated in the late 19th century, to catalogue and map the positions of millions of stars as faint as 11th or 12th magnitude. Twenty observatories from around the world participated in exposing and measuring more than 22,000 (glass) photographic plates in an enormous observing programme extending over several decades. Despite, or because of, its vast scale, the project was only ever partially successful – the Carte du Ciel component was never completed, and for almost half a century the Astrographic Catalogue part was largely ignored. However, the appearance of the Hipparcos Catalogue in 1997 has led to an important development in the use of this historical plate material.
Thomas Henderson FRSE FRS FRAS was a Scottish astronomer and mathematician noted for being the first person to measure the distance to Alpha Centauri, the major component of the nearest stellar system to Earth, the first to determine the parallax of a fixed star, and for being the first Astronomer Royal for Scotland.
Sir David Gill was a Scottish astronomer who is known for measuring astronomical distances, for astrophotography and geodesy. He spent much of his career in South Africa.
Robert Thorburn Ayton Innes FRSE FRAS was a British-born South African astronomer best known for discovering Proxima Centauri in 1915, and numerous binary stars. He was also the first astronomer to have seen the Great January Comet of 1910, on 12 January. He was the founding director of a meteorological observatory in Johannesburg, which was later converted to an astronomical observatory and renamed to Union Observatory. He was the first Union Astronomer. Innes House, designed by Herbert Baker, built as his residence at the observatory, today houses the South African Institute of Electrical Engineers.
William Henry Finlay (FRAS) was a South African astronomer. He was First Assistant at the Cape Observatory from 1873 to 1898 under Edward James Stone. He discovered the periodic comet 15P/Finlay. Earlier, he was one of the first to spot the "Great Comet of 1882". The first telegraphic determinations of longitude along the western coast of Africa were made by Finlay and T. F. Pullen.
Union Observatory also known as Johannesburg Observatory (078) is a defunct astronomical observatory in Johannesburg, South Africa that was operated between 1903 and 1971. It is located on Observatory Ridge, the city's highest point at 1,808 metres altitude in the suburb Observatory.
South African Astronomical Observatory (SAAO) is the national centre for optical and infrared astronomy in South Africa. It was established in 1972. The observatory is run by the National Research Foundation of South Africa. The facility's function is to conduct research in astronomy and astrophysics. The primary telescopes are located in Sutherland, which is 370 kilometres (230 mi) from Observatory, Cape Town, where the headquarters is located.
Sir Thomas Maclear was an Irish-born South African astronomer who became Her Majesty's astronomer at the Cape of Good Hope.
James Dunlop FRSE was a Scottish astronomer, noted for his work in Australia. He was employed by Sir Thomas Brisbane to work as astronomer's assistant at his private observatory, once located at Paramatta, New South Wales, about 23 kilometres (14 mi) west of Sydney during the 1820s and 1830s. Dunlop was mostly a visual observer, doing stellar astrometry work for Brisbane, and after its completion, then independently discovered and catalogued many new telescopic southern double stars and deep-sky objects. He later became the Superintendent of Paramatta Observatory when it was finally sold to the New South Wales Government.
Grubb Parsons was a historic manufacturer of telescopes, active in the 19th and 20th centuries. They built numerous large research telescopes, including several that were the largest in the world of their type.
John Jackson was a Scottish astronomer.
David Stanley Evans was a British astronomer, noted for his use of lunar occultations to measure stellar angular diameters during the 1950s.
The Great Melbourne Telescope was built by the Grubb Telescope Company in Dublin, Ireland in 1868, and installed at the Melbourne Observatory in Melbourne, Australia in 1869. In 1945 that Observatory closed and the telescope was sold and moved to the Mount Stromlo Observatory near Canberra. It was rebuilt in the late 1950s. In 2003 the telescope, still in use as an observatory, was severely damaged in a bushfire. About 70% of the components were salvageable; a project to restore the telescope to working condition started in 2013.
Ian Stewart Glass is an infrared astronomer and scientific historian living in Cape Town, South Africa.
Potsdam Great Refractor is an historic astronomical telescope in an observatory in Potsdam, Germany.
The Yapp telescope is a 36-inch reflecting telescope of the United Kingdom, now located at the Observatory Science Centre at Herstmonceux.
Brian Warner was a British South African optical astronomer who was Emeritus Distinguished Professor of natural philosophy at the University of Cape Town. Warner's research included cataclysmic variable stars, pulsars, degenerate stars and binary stars. He also researched and published on the history of astronomy in South Africa.