Observatory code | 004 |
---|---|
Location | Toulouse, France |
Coordinates | 43°36′44″N1°27′46″E / 43.61233°N 1.46278°E |
Established | 1733, 1841, 1981 |
Related media on Commons | |
The Toulouse Observatory (French : Observatoire de Toulouse) is located in Toulouse, France and was established in 1733. [1]
It was founded by l'Académie des Sciences, Inscriptions et Belles-Lettres de Toulouse ("Academy of Science, Inscriptions and the Humanities of Toulouse"). It was moved 1841 and again in 1981.[ citation needed ]
In 1987, Genevieve Soucail of the Toulouse Observatory and her collaborators presented data of a blue ring-like structure in Abell 370 and proposed a gravitational lensing interpretation [2]
In the 1990s the observatory worked on MEGACAM with several other institutions. [3]
The observatory was started by Garipuy in the 1730s with support from the Academy of Sciences. [4]
Félix Tisserand was a famous director from 1873 to 1878. He published Recueil d'exercices sur le calcul infinitesimal as well as making several expeditions, including an 1874 trip to Japan. Henri Joseph Anastase Perrotin was Tisserand's assistant astronomer, and they both went to the Paris Observatory in 1878. Tisserand was succeeded by Benjamin Baillaud.
Director | Life span | Years of directorship |
---|---|---|
Frédéric Petit | 1810–1865 | 1838–1865 |
Théodore Despeyrous | 1815–1883 | 1865–1866 |
Pierre Daguin | 1814–1884 | 1866–1870 |
Félix Tisserand | 1845–1896 | 1873–1878 |
Benjamin Baillaud | 1848–1934 | 1878–1907 |
Eugène Cosserat | 1866–1931 | 1908–1931 |
Emile Paloque | 1891–1982 | 1931–1960 |
Roger Bouigues | 1920– | 1961–1971 |
Jean Rösch | 1915–1999 | 1971–1981 |
The observatory was originally founded in 1733. [5] Launch instruments at the observatory included two refractors and 28 inch quadrant, and one clock. [6] [4] By 1840 and additional clock by Julien le Roi of Paris was added. [6]
Among the early observations at the observatory were the 1736 and 1743 transits of Mercury. [4] These observations were conducted by Garipuy, who also observed the transit of Mercury in 1753. [4] Garipuy also built and observatory in his house and conducted observations from there. [4]
By 1770 a new larger observatory was established and again in the 1840s. [7]
In 1871-1873 Toulouse observatory switched from being a municipal to provincial observatory. [8]
In 1873 a 4.5 inch (10.8 cm) refractor by Secretan was added to the Observatory. [9]
In 1875 a reflecting telescope by Henry Brothers was added. [10] [11] The 83 centimetres (33 in) diameter aperture was a reflecting telescope (i.e. mirror) mounted on an equatorial. [10] In 1880 the reflector was re mounted on a cast iron design by Gautier, replacing the wood mounting. [8]
Also in 1880 a new refractor (lens) was acquired, a 9 inch (22 cm) aperture by Brunner. [8] Several other instruments were added at this time, and in the early 1900s a new telescope for the Pic Du Midi mountaintop observatory was also added. [8]
In the 1880s Toulouse Observatory sent some of its oldest instruments to a museum. [12] This included a transit instrument by Lennel dating to 1774, Dollond telescope, and several quadrants. [12]
The observatory participated in the Carte Du Ciel project, recording over a thousand plates (i.e. astronomical photographs) between 1887 and 1939. [8]
In the 1980s astronomers of Toulouse Observatory discovered a gravitational lens in space. [13] They found an arc around Abel 370 and were able to recognized it as this phenomenon. [13]
The observatory has used many telescopes over its lifetime. [10] For example, an 83 cm aperture reflecting telescope was installed in 1875. [11]
Yerkes Observatory is an astronomical observatory located in Williams Bay, Wisconsin, United States. The observatory was operated by the University of Chicago Department of Astronomy and Astrophysics from its founding in 1897 until 2018. Ownership was transferred to the non-profit Yerkes Future Foundation (YFF) in May 2020, which began millions of dollars of restoration and renovation of the historic building and grounds. Yerkes re-opened for public tours and programming in May 2022. The April 2024 issue of National Geographic magazine featured a story about the Observatory and ongoing work to restore it to relevance for astronomy, public science engagement and exploring big ideas through art, science, culture and landscape. The observatory offers tickets to programs and tours on its website.
The Nice Observatory is an astronomical observatory located in Nice, France on the summit of Mount Gros. The observatory was founded in 1879, by the banker Raphaël Bischoffsheim. The architect was Charles Garnier, and Gustave Eiffel designed the main dome.
A refracting telescope is a type of optical telescope that uses a lens as its objective to form an image. The refracting telescope design was originally used in spyglasses and astronomical telescopes but is also used for long-focus camera lenses. Although large refracting telescopes were very popular in the second half of the 19th century, for most research purposes, the refracting telescope has been superseded by the reflecting telescope, which allows larger apertures. A refractor's magnification is calculated by dividing the focal length of the objective lens by that of the eyepiece.
The Paris Observatory, a research institution of the Paris Sciences et Lettres University, is the foremost astronomical observatory of France, and one of the largest astronomical centers in the world. Its historic building is on the Left Bank of the Seine in central Paris, but most of the staff work on a satellite campus in Meudon, a suburb southwest of Paris.
The Stockholm Observatory is an astronomical observatory and institution in Stockholm, Sweden, founded in the 18th century and today part of Stockholm University. In 1931, the new Stockholm Observatory, nicknamed "Saltis", was inaugurated on the Karlsbaderberget at Saltsjöbaden, near Stockholm, and operated until 2001.
Markree Observatory was an astronomical observatory in County Sligo, Ireland. The asteroid 9 Metis was discovered from this observatory in 1848 by Cooper's assistant Andrew Graham using a comet seeker telescope. The observatory was also home to the largest refractor of the early 1830s, which had a 13.3-inch (340 mm) aperture Cauchoix of Paris lens; the largest in the world at that time. The observatory also housed a number of instruments and was operated to varying degrees throughout the 19th century.
Marseille Observatory is an astronomical observatory located in Marseille, France, with a history that goes back to the early 18th century. In its 1877 incarnation, it was the discovery site of a group of galaxies known as Stephan's Quintet, discovered by its director Édouard Stephan. Marseille Observatory is now run as a joint research unit by Aix-Marseille University and the French National Center for Scientific Research (CNRS).
Hamburg Observatory is an astronomical observatory located in the Bergedorf borough of the city of Hamburg in northern Germany. It is owned and operated by the University of Hamburg, Germany since 1968, although it was founded in 1825 by the City of Hamburg and moved to its present location in 1912. It has operated telescopes at Bergedorf, at two previous locations in Hamburg, at other observatories around the world, and it has also supported space missions.
The Royal Observatory of Belgium has been situated in the Uccle municipality of Brussels since 1890.
The Bordeaux Observatory is an astronomical observatory affiliated with the University of Bordeaux. Built in Floirac, France in 1893 its lenses were focused between +11 and +17 degrees declination. Until 1970 it had taken over 4,000 photographic plates. Bordeaux Observatory is home to a large collection of instruments and archives from well over a century of astronomical activities. Until the 2016 it was actively used until the institution moved to a new location at the University. In the French language the name is Observatoire de Bordeaux.
The Dearborn Observatory is an astronomical observatory located on the Evanston campus of Northwestern University. The observatory was originally constructed in 1888, through an agreement between the university and the Chicago Astronomical Society. In the summer of 1939, Dearborn Observatory had to be moved to make way for the construction of the Technological Institute.
The Kuffner observatory is one of two telescope-equipped public astronomical observatories situated in Austria's capital, Vienna. It is situated in the West of the city's Ottakring district, on the slope of the Gallitzinberg at 302 m altitude. Originally a private research institution, it was converted into an educational astronomy facility after World War II as buildings and city lights had encroached to a degree that severely hampered scientific nightsky observations. Today the main tasks of the observatory consist in public education on astronomy, operating and preserving the historical equipment, and minor projects in scientific astronomy.
Great refractor refers to a large telescope with a lens, usually the largest refractor at an observatory with an equatorial mount. The preeminence and success of this style in observational astronomy defines an era in modern telescopy in the 19th and early 20th century. Great refractors were large refracting telescopes using achromatic lenses. They were often the largest in the world, or largest in a region. Despite typical designs having smaller apertures than reflectors, great refractors offered a number of advantages and were popular for astronomy. It was also popular to exhibit large refractors at international exhibits, and examples of this include the Trophy Telescope at the 1851 Great Exhibition, and the Yerkes Great Refractor at the 1893 World's Fair in Chicago.
The Shuckburgh telescope or Shuckburgh equatorial refracting telescope was a 4.1 inches (10.4 cm) diameter aperture telescope on an equatorial mount completed in 1791 for Sir George Shuckburgh (1751–1804) in Warwickshire, England, and built by British instrument maker Jesse Ramsden (1735–1800). It was transferred to the Royal Observatory, Greenwich in 1811 and the London Science Museum in 1929. Even though it has sometimes not been regarded as particularly successful, its design was influential. It was one of the larger achromatic doublet telescopes at the time, and one of the largest to have an equatorial mount. It was also known as the eastern equatorial for its location.
Robert-Aglaé Cauchoix was a French optician and instrument maker, whose lenses played a part in the race of the great refractor telescopes in the first half of the 19th century.
The Greenwich 28-inch refractor is a telescope at the Royal Observatory, Greenwich, where it was first installed in 1893. It is a 28-inch ( 71 cm) aperture objective lens telescope, otherwise known as a refractor, and was made by the telescope maker Sir Howard Grubb. The achromatic lens was made Grubb from Chance Brothers glass. The mounting is older however and dates to the 1850s, having been designed by Royal Observatory director George Airy and the firm Ransomes and Simms. The telescope is noted for its spherical dome which extends beyond the tower, nicknamed the "onion" dome. Another name for this telescope is "The Great Equatorial" which it shares with the building, which housed an older but smaller telescope previously.
Potsdam Great Refractor is an historic astronomical telescope in an observatory in Potsdam, Germany.
Meudon Great Refractor is a double telescope with lenses, in Meudon, France. It is a twin refracting telescope built in 1891, with one visual and one photographic, on a single square-tube together on an equatorial mount, inside a dome. The Refractor was built for the Meudon Observatory, and is the largest double doublet refracting telescope in Europe, but about the same size as several telescopes in this period, when this style of telescope was popular. Other large telescopes of a similar type include the James Lick telescope (91.4), Potsdam Great Refractor (80+50 cm), and the Greenwich 28 inch refractor (71.1 cm).