South African Astronomical 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 from Observatory, Cape Town, where the headquarters is located. The SAAO has links worldwide for scientific and technological collaboration. Instrumental contributions from the South African Astronomical Observatory include the development of a spherical aberration corrector and the Southern African Large Telescope  (SALT). The Noon Gun on Cape Town's Signal Hill is fired remotely by a time signal from the Observatory. History. The history of the SAAO began when the Royal Observatory at the Cape of Good Hope was founded in 1820, the first scientific institution in Africa. Construction of the main buildings was completed in 1829 at a cost of £30,000 (equivalent to £ in 2022). The post of "Her Majesty's astronomer at the Cape of Good Hope" was awarded the Royal Medal on two occasions; the first to Thomas Maclear in 1869 for measurement of an arc  of the meridian at the Cape of Good Hope and the second to David Gill in 1903 for researches in solar and stellar parallax, and his energetic direction of the Royal Observatory at the Cape of Good Hope. The Republic Observatory, Johannesburg, was merged with the much older Royal Observatory, Cape of Good Hope in January 1972 to form the South African Astronomical Observatory. In 1974 the Radcliffe Observatory telescope was purchased by the CSIR and moved to Sutherland, where it recommenced work in 1976. SAAO was established in January 1972, as a result of a joint agreement by the  Council for Scientific and Industrial Research (CSIR) of South Africa and Science and Engineering Research Council (SERC) of United Kingdom. The headquarters are located on the grounds of the old Royal Observatory where the main building, offices, national library for astronomy and computer facilities are housed. Historic telescopes are also found at the headquarters in a number of domes and a small museum that displays scientific instruments. The South African Astronomical Observatory is administered at present as a National Facility under management of the National Research Foundation (NRF), formerly the Foundation for Research Development (FRD). In 1974, when the Radcliffe  Observatory in Pretoria closed, the Council for Scientific and Industrial Research (CSIR) purchased the 1.9-m Radcliffe telescope and transported it to Sutherland. Facilities. The observatory operates from the campus of the "Royal Observatory, Cape of Good Hope" that was established in 1820 in the suburb of Observatory, Cape Town. The major observing facilities are however located near the town of Sutherland some from Cape Town. Telescopes. 0.50m telescope. This reflector was originally built for the Republic Observatory in 1967, but was moved to the Sutherland site in 1972. No longer in use. The 20" telescope was replaced with  the Meerlicht telescope. The 20" telescope was relocated to the University of Freestate Boyden observatory and commissioned in ~2019 https://www.ufs.ac.za/natagri/departments-and-divisions/physics-home/research-and-publications/astrophysics-research-facilities 0.75m telescope. A Grubb Parsons reflector. 1.0m Telescope. This telescope was originally located at SAAO Head office in Observatory, Cape Town, but has since moved to the Sutherland site. This telescope participates in the PLANET network. 1.9m Telescope. The 1.9-m (74-inch) Radcliffe Telescope was commissioned for the Radcliffe Observatory in Pretoria where it was in use between 1948 and 1974. Following the closure of the Radcliffe Observatory it was moved to Sutherland where it became  operational again in January 1976. Between 1951 and 2004 it was the largest telescope in South Africa. The telescope was manufactured by Sir Howard Grubb, Parsons and Co. Alan Cousins Telescope (ACT). This telescope was originally called the Automatic Photometric Telescope, but has been renamed the Alan Cousins Telescope in honour of Alan William James Cousins. BiSON. One of six telescopes in the Birmingham Solar Oscillations Network Infrared Survey Facility (IRSF). The IRSF is a reflector fitted with a 3 colour Infrared Imager. Originally built as part of the "Magellanic Clouds A Thorough Study" grant from the Japanese Ministry of  Education, Culture, Sports, Science and Technology in 2000. Other studies the telescope participated in include: Las Cumbres Observatory Global Telescope Network. Three telescopes to form part of the LCOGT network were installed in early 2013. MASTER. The MASTER-SAAO Telescope (obs. code: K95) is part of the "Russian Mobile Astronomical System of Telescope-Robots". It saw first light on 21 December 2014. It consists of two paired 0.4-m telescopes. In April 2015 it discovered the first comet from South Africa in 35 years, C/2015 G2 (MASTER). MONET. One of the two telescopes of the MOnitoring NEtwork of Telescopes Project  is located at Sutherland. Its twin can be found at the McDonald Observatory in Texas. The MONET telescopes are Robotic telescope controllable via the Internet and was constructed by the University of Göttingen. Remote Telescope Markup Language is used to control the telescopes remotely. Project Solaris. Two telescopes forming part of Project Solaris is located at the Sutherland site. Solaris-1 and Solaris-2 are both 0.5m f/15 Ritchey–Chrétien telescope. The aims of Project Solaris is to detect circumbinary planets around eclipsing binary stars and to characterise these binaries to improve stellar models. Southern African Large Telescope (SALT). SALT was  inaugurated in November 2005. It is the largest single optical telescope in the Southern Hemisphere, with a hexagonal mirror array 11 meters across. SALT shares similarities with the Hobby-Eberly Telescope (HET) in Texas. The Southern African Large Telescope gathers twenty-five times as much light as any other existing African Telescope. With this larger mirror array, SALT can record distant stars, galaxies and quasars. SuperWASP-South. The Wide Angle Search for Planets consists of two robotic telescopes, the one located at SAAO Sutherland and the other at Roque de los Muchachos Observatory on the island of La Palma in  the Canaries. WASP-17b, the first exoplanet known to have a retrograde orbit was discovered in 2009 using this array. KELT-South. KELT-South ("Kilodegree Extremely Little Telescope South") is a small robotic telescope that is designed to detect transiting extrasolar planets. The telescope is owned and operated by Vanderbilt University and was based on the design of KELT-North, which was conceived and designed at the Ohio State University, Department of Astronomy. The KELT-South telescope will serve as a counterpart to its northern twin, surveying the southern sky for transiting planets over the next few years. MeerLICHT. Optical wide -field telescope, installed in 2017. It has a 60cm effective aperture, and a 1.65 x 1.65 degree field-of-view, sampled at 0.56"/pix. It was designed and manufactured in the Netherlands (Radboud University & NOVA) and is run by a consortium of Radboud University,University of Cape Town, the NRF/SAAO, the University of Oxford, the University of Manchester and the University of Amsterdam. It is the optical eye of MeerKAT, and has as its main-purpose to twin with the MeerKAT radio array to achieve a simultaneous optical-radio coverage of the Southern Skies. It is the prototype of  the BlackGEM array, installed at ESO La Silla in Chile. Yonsei Survey Telescopes for Astronomical Research (YSTAR). The Yonsei Survey Telescopes for Astronomical Research (YSTAR), decommissioned in 2012, was used for the monitoring of variable stars and other transient events. YSTAR was a joint project between SAAO and the Yonsei University, Korea. Geophysical. South African Geodynamic Observatory Sutherland (SAGOS). The GeoForschungsZentrum, Potsdam in co-operation with the National Research Foundation of South Africa constructed the SAGOS between 1998 and 2000. SAGOS consist of a 1 Hz permanent GPS station, a superconducting gravimeter, meteorological sensors, and a tri-axial magnetometer. The  GPS station is also used in support of the CHAllenging Minisatellite Payload ("CHAMP") and Gravity Recovery and Climate Experiment ("GRACE") space missions. SUR Station. The SUR station forms part of the International Deployment of Accelerometers Project and the Global Seismographic Network of the Incorporated Research Institutions for Seismology