Alternative names | Observatoire de Marseille | ||||
---|---|---|---|---|---|
Organization | Observatoire des Science de l'Univers Institut Pythéas | ||||
Observatory code | 014 | ||||
Location | Marseille, France | ||||
Coordinates | 43°18′20″N5°23′41″E / 43.30547°N 5.39477°E | ||||
Altitude | 40 m (130 ft) | ||||
Established | 1702 | ||||
Website | www | ||||
Telescopes | |||||
| |||||
Marseille Observatory (French : Observatoire de Marseille) 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).
The old Palais Longchamp facilities are a noted tourist attraction in Marseille, and a planetarium was also added in 2001. [1] [2] One of the noted exhibits is the Foucault glass-mirror telescope, and various items from centuries of astronomical activities.
Foucault's telescope is a noted historical example because it was the forerunner of the modern style of big reflecting telescopes which use a minute layer of metal on a figured piece of glass. Before this, the main technology was to make the whole mirror of metal, and it would really be another half-century before silvered glass mirrors really caught on for astronomy. A major change in the 20th century was to shift from using solution to coat the glass with silver to using a vapor deposition process.
The observatory was founded in 1701 in Montee des Accoules (a location near Vieux Port, Marseille, France). [3] Antoine Laval was the first director. [3]
The 1761 Transit of Venus was observed from the Marseilles Observatory. [4] A telescope 6 feet long made by James Short was used for this observation. [4] These observations were conducted by the astronomer Louis Lagrange. [4]
In 1789 Jean-Louis Pons began work at Marseille Observatory as a doorkeeper, but he also received lessons in astronomy; by 1801 he had discovered his first comet. [5] Pons would become one of the most prolific comet discovers, finding 37 in all, a significant portion of all comet discoveries for a quarter of a century. [5]
Astronomer Jean-Félix Adolphe Gambart discovered 16 comets from the old observatory. [6] Another astronomer of Marseilles Observatory was Benjamin Valz.
Jean-Louis Pons (1761-1831) discovered his first comet in 1801, and went on to find 37 more in his career many of them at Marseilles Observatory. [5]
The Comet Pons-Brook was discovered by Pons in July 1812, however it was not seen again until June 1883. [7] (The next time it was recovered was in 1953.) [7] Some other famous comets discovered by Pons include 7P/Pons–Winnecke, 12P/Pons–Brooks, and 273P/Pons–Gambart, among many others. [5] (see also Comet Pons)
Pons also discovered comets that came to be known by other names including Encke's Comet, Comet Crommelin, and Biela's Comet. [5] This is not unusual as comet discoveries are sometimes later determined to be re-discoveries of previously observed comets or co-discoveries (discovered at the same time by others). Similarly, some comets were named for the first person to compute the comet's orbit, as in the case of Halley's comet. [5]
Foucault operated his 80 cm silver-on-glass reflector at Marseille Observatory, [8] a telescope with aperture 80 cm (31.5 inches) from about 1862 to its retirement in 1965. [9] [10] The telescope was noted for being a pioneering design, that used silver-coated glass in a reflecting telescope. [9]
In 1863 Marseilles Observatory became a branch of the Paris Observatory. [11] This led to a new building inaugurated by 1864, designed by the architect of Notre Dame de la Garde, also the 80 cm reflector was installed by that year [11] (at the Palais Longchamp site).
Work continued on improvements and by 1866 a Comet Seeker telescope of 18 cm aperture by Martin had been installed, and a 25.8 cm (10.25") aperture refractor by Merz by 1872. [11] The Merz refractor was on equatorial mounting with governor done by Foucault. [11]
There was also instruments and facilities for magnetic studies. [11]
1872 Marseilles reported several new nebula discovered using the Eichens searcher. [12]
In 1873 Marseilles Observatory announced the discovery of 300 new nebula. [13] Of these 75 had their positions accurately cataloged, which was done by comparing the location of the nebula with previously cataloged stars of known position. [13]
In 1873 Marseilles Observatory detached from the Paris Observatory. [14]
In 1874 the Comet C/1874 H1 was discovered from the observatory.
In 1914, the Orion nebula was observed with the Perot-Fabry interferometer. [15]
In 1965 the Foucault 80 cm reflecting telescope was retired. [10]
In 1989 the Marseille telescope was completed at the observatory, and then sent to the southern hemisphere later that year. [16] The telescope is a reflecting telescope with 36 cm (~14.2") diameter mirror with a low-expansion glass-ceramic of the Richey-Chrétien type. [16]
Starting in 1990 Marseille Observatory had a study of H alpha (H-alpha (Hα)) in the southern galactic plane. [17] This included observations of the Magellanic Clouds also. [17] This study used the 36 cm Marseille telescope at La Silla observatory in the southern hemisphere for data. [18] The telescope was equipped with both a photon counter and a Fabry-Perot interferometer for this study. [18]
In 1999 Marseilles Observatory published a study on simulating the formation of proto-planets and planetesimals with a large planetary body. [19] This simulation used the GRAPE-4 system. [19]
In 2000, Marseille Observatory merged with the Laboratoire d'Astrophysique Spatiale to become the Laboratoire d'Astrophysique de Marseille (LAM) within the broader Observatoire Astronomique Marseille Provence which also included the Haute-Provence Observatory.
In 2008, LAM was relocated to a new 10,000 square meter facility in the Technopôle Chateau-Gombert in Marseille. The facility includes two major technology platforms for qualification of space instruments and for fabrication and metrology of optical mirrors. LAM astronomers specialize in cosmology and galaxy evolution, exoplanets and Solar System, and R&D in optics and instrumentation.
In 2012, the Observatoire Astronomique Marseille Provence merged with other earth-sciences research institutes from Aix-Marseille University and became a new entity called the Observatoire des Science de l'Univers Institut Pythéas (OSU-IP) which now includes 6 major labs for earth and universe sciences: CEREGE, IMBE, MIO, LAM. LPED, MIO as well as the Haute-Provence Observatory.
The old Marseille Observatory site is a noted tourist attraction in the Palais Longchamp area. [20] Exhibits include the Foucault telescope, and there is also a planetarium. [6] The planetarium has 30-seats and opened in 2001. [2]
The facilities at Plateau Longchamp date from the 1860s, the older site was at Vieux Port. [14]
The Ring Nebula is a planetary nebula in the northern constellation of Lyra.[C] Such a nebula is formed when a star, during the last stages of its evolution before becoming a white dwarf, expels a vast luminous envelope of ionized gas into the surrounding interstellar space.
Jean-Louis Pons was a French astronomer. Despite humble beginnings and being self-taught, he went on to become the greatest visual comet discoverer of all time: between 1801 and 1827 Pons discovered thirty-seven comets, more than any other person in history.
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.
Maximilian Franz Joseph Cornelius Wolf was a German astronomer and a pioneer in the field of astrophotography. He was the chairman of astronomy at the University of Heidelberg and director of the Heidelberg-Königstuhl State Observatory from 1902 until his death in 1932.
Boyden Observatory is an astronomical research observatory and science education centre located in Maselspoort, 20 kilometres (12 mi) north-east of the city of Bloemfontein in Free State, South Africa. The observatory is managed by the Physics Department of the University of the Free State (UFS). The Friends of Boyden assist the observatory as a public support group, organising open evenings and protecting its public interest. Boyden also makes use of members of ASSA Bloemfontein Centre, the amateur astronomy club of the city, for presenters and telescope assistants.
William Robert Brooks was a British-born American astronomer, mainly noted as being one of the most prolific discoverers of new comets of all time, second only to Jean-Louis Pons.
The Haute-Provence Observatory is an astronomical observatory in the southeast of France, about 90 km east of Avignon and 100 km north of Marseille. It was established in 1937 as a national facility for French astronomers. Astronomical observations began in 1943 using the 1.20 m telescope, and the first research papers based on observations made at the observatory were published in 1944. Foreign observers first used the observatory in 1949, when Geoffrey and Margaret Burbidge visited.
Leuschner Observatory, originally called the Students' Observatory, is an observatory jointly operated by the University of California, Berkeley and San Francisco State University. The observatory was built in 1886 on the Berkeley campus. For many years, it was directed by Armin Otto Leuschner, for whom the observatory was renamed in 1951. In 1965, it was relocated to its present home in Lafayette, California, approximately 10 miles (16 km) east of the Berkeley campus. In 2012, the physics and astronomy department of San Francisco State University became a partner.
A comet seeker is a type of small telescope adapted especially to searching for comets: commonly of short focal length and large aperture, in order to secure the greatest brilliancy of light. This style of telescope was used to discover the asteroid 9 Metis in 1848.
NGC 6751, also known as the Glowing Eye Nebula, is a planetary nebula in the constellation Aquila. It is estimated to be about 6,500 light-years away.
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 Crossley telescope is a 36-inch (910 mm) reflecting telescope located at Lick Observatory in the U.S. state of California. It was used between 1895 and 2010, and was donated to the observatory by Edward Crossley, its namesake.
The Geneva Observatory is an astronomical observatory at Sauverny (CH) in the municipality of Versoix, Canton of Geneva, in Switzerland. It shares its buildings with the astronomy department of the École Polytechnique Fédérale de Lausanne. It has been active in discovering exoplanets, in stellar photometry, modelling stellar evolution, and has been involved in the European Space Agency's Hipparcos, INTEGRAL, Gaia, and Planck missions.
Puckett Observatory is a private astronomical observatory located in the state of Georgia. It is owned and operated by Tim Puckett. Its primary observation goals are the study of comets and the discovery of supernovae. To facilitate the latter goal it sponsors the Puckett Observatory World Supernova Search whose astronomers have discovered 369 supernovae.
273P/Pons–Gambart, also called Comet Pons-Gambart, is a periodic comet in a retrograde orbit first discovered on June 21, 1827 by Jean-Louis Pons and Jean-Félix Adolphe Gambart. It has a 186 year orbit and it fits the classical definition of a Halley-type comet. Its last perihelion was in December 2012 and will next come to perihelion around August 2191.
Emmanuel H. Hugot is a French astrophysicist, deputy director at the Laboratoire d'Astrophysique de Marseille. known for his contribution to the developments of new technologies that help to improve telescopes used by professional astronomers around the world. This includes the development of more efficient curved detectors, but also improvements in the manufacturing methods for optical elements and active optics systems. The technologies developed by Hugot and his group are used on the SPHERE instrument mounted on the European Very Large Telescope, as well as the coronagraphic instrument of the future NASA's Nancy Grace Roman Space Telescope, which are used to detect exoplanets.
Denis Burgarella is a French astrophysicist at Laboratoire d'astrophysique de Marseille.
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).
{{cite web}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link){{cite web}}
: CS1 maint: multiple names: authors list (link) CS1 maint: numeric names: authors list (link)