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Marseilles Observatory
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 Longchamps facilities are a noted tourist destination in Marseilles area, and a planetarium was also added in 2001. 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 meta ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Marseille
Marseille ( , , ; also spelled in English as Marseilles; oc, Marselha ) is the prefecture of the French department of Bouches-du-Rhône and capital of the Provence-Alpes-Côte d'Azur region. Situated in the camargue region of southern France, it is located on the coast of the Gulf of Lion, part of the Mediterranean Sea, near the mouth of the Rhône river. Its inhabitants are called ''Marseillais''. Marseille is the second most populous city in France, with 870,731 inhabitants in 2019 (Jan. census) over a municipal territory of . Together with its suburbs and exurbs, the Marseille metropolitan area, which extends over , had a population of 1,873,270 at the Jan. 2019 census, the third most populated in France after those of Paris and Lyon. The cities of Marseille, Aix-en-Provence, and 90 suburban municipalities have formed since 2016 the Aix-Marseille-Provence Metropolis, an Indirect election, indirectly elected Métropole, metropolitan authority now in charge of wider metropo ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Jean-Félix Adolphe Gambart
Jean-Félix Adolphe Gambart (12 May 1800 – 23 July 1836) was a French astronomer. He was born in Sète in Hérault department, the son of a sea captain. His intelligence was noticed at a young age by Alexis Bouvard, who persuaded him to join the astronomy profession. In 1819 he joined the Marseilles Observatory and became the director in 1822. During his career he recorded a number of observations of the satellites of Jupiter, and discovered a total of 13 comets. In 1832 he observed the transit of Mercury across the Sun, noting that the planet appeared deformed as it approached the edge. He suffered from tuberculosis, and in 1836 died from cholera in Paris, aged 36. The crater Gambart on the moon is named after him.Antonín Rükl: ''Atlas Měsíce'' (Atlas of the Moon), Aventinum (Prague 1991), chapter Stadius, p. 90, Crater Gamb ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Palais Longchamp
The Palais Longchamp is a monument in the 4th arrondissement of Marseille, France. It houses the Musée des beaux-arts and Muséum d'histoire naturelle de Marseille. The surrounding Longchamp Park (French: ''Parc Longchamp'') is listed by the French Ministry of Culture as one of the Notable Gardens of France. History The Palais Longchamp was created to celebrate the construction of the Canal de Marseille, which was built to bring water from the river Durance to Marseille. Although the foundation stone was laid by the Duke of Orleans on 15 November 1839, the building took 30 years to complete, partly because of the enormous expense and partly because of difficulties with local regulations. Designed by the architect Henri-Jacques Espérandieu, the building was centered on the structure and elaborate fountain known as the ''château d'eau'' ("water castle"). Description The Palais Longchamp has three main parts: * The ''château d'eau'' * The east wing, which houses the Musée ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Notre-Dame De La Garde
Notre-Dame de la Garde (literally: Our Lady of the Guard), known to local citizens as ''la Bonne Mère'' (French for 'the Good Mother'), is a Catholic basilica in Marseille, France, and the city's best-known symbol. The site of a popular Assumption Day pilgrimage, it was the most visited site in Marseille. It was built on the foundations of an ancient fort at the highest natural point in Marseille, a limestone outcropping on the south side of the Old Port of Marseille. Construction of the basilica began in 1853 and lasted for over forty years. It was originally an enlargement of a medieval chapel but was transformed into a new structure at the request of Father Bernard, the chaplain. The plans were made and developed by the architect Henri-Jacques Espérandieu. It was consecrated while still unfinished on 5 June 1864. The basilica consists of a lower church or crypt in the Romanesque style, carved from the rock, and an upper church of Neo-Byzantine style decorated with mosa ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Paris Observatory
The Paris Observatory (french: Observatoire de Paris ), 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 Paris Observatory was founded in 1667. Construction was completed by the early 1670s and coincided with a major push for increased science, and the founding of the Royal Academy of Sciences. King Louis XIV's minister of finance organized a "scientific powerhouse" to increase understanding of astronomy, maritime navigation, and science in general. Through the centuries the Paris Observatory has continued in support of astronomical activities, and in the 21st century connects multiple sites and organizations, supporting astronomy and science, past and present. Constitution Administrat ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Halley's Comet
Halley's Comet or Comet Halley, officially designated 1P/Halley, is a short-period comet visible from Earth every 75–79 years. Halley is the only known short-period comet that is regularly visible to the naked eye from Earth, and thus the only naked-eye comet that can appear twice in a human lifetime. Halley last appeared in the inner parts of the Solar System in 1986 and will next appear in mid-2061. Halley's periodic returns to the inner Solar System have been observed and recorded by astronomers around the world since at least 240 BC. But it was not until 1705 that the English astronomer Edmond Halley understood that these appearances were reappearances of the same comet. As a result of this discovery, the comet is named after Halley. During its 1986 visit to the inner Solar System, Halley's Comet became the first comet to be observed in detail by spacecraft, providing the first observational data on the structure of a comet nucleus and the mechanism of coma and tail f ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Biela's Comet
Biela's Comet or Comet Biela (official designation: 3D/Biela) was a periodic Jupiter-family comet first recorded in 1772 by Montaigne and Messier and finally identified as periodic in 1826 by Wilhelm von Biela. It was subsequently observed to split in two and has not been seen since 1852. As a result, it is currently considered to have been destroyed, although remnants appeared to have survived for some time as a meteor shower, the Andromedids. Discovery The comet was first recorded on 8 March 1772 by Jacques Leibax Montaigne; during the same apparition it was independently discovered by Charles Messier. It was also recorded in 1805 by Jean-Louis Pons, but was not recognized as the same object. After the 1805 apparition a number of attempts were made by Gauss (1806) and Bessel (1806) to calculate a definitive orbit. Gauss and Olbers both noted a similarity between the 1805 and 1772 comets but they were not able to prove a link. Confirmation as periodic It was Wilhelm von ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Comet Crommelin
Comet Crommelin, also known as Comet Pons-Coggia-Winnecke-Forbes, is a periodic comet with an orbital period of almost 28 years. It fits the classical definition of a Halley-type comet with (20 years < < 200 years). It is named after the Andrew C. D. Crommelin who calculated its orbit in 1930. It is one of only four comets not named after their discoverer(s), the other three being Comets |
Encke's Comet
Comet Encke , or Encke's Comet (official designation: 2P/Encke), is a periodic comet that completes an orbit of the Sun once every 3.3 years. (This is the shortest period of a reasonably bright comet; the faint main-belt comet 311P/PanSTARRS has a period of 3.2 years.) Encke was first recorded by Pierre Méchain on 17 January 1786, but it was not recognized as a periodic comet until 1819 when its orbit was computed by Johann Franz Encke. Like Halley's Comet, it is unusual in its being named after the calculator of its orbit rather than its discoverer. Like most comets, it has a very low albedo, reflecting only 4.6% of the light its nucleus receives, although comets generate a large coma and tail that can make them much more visible during their perihelion (closest approach to the Sun). The diameter of the nucleus of Encke's Comet is 4.8 km. Discovery As its official designation implies, Encke's Comet was the first periodic comet discovered after Halley's Comet (designated ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Comet Pons
Comet Pons may refer to any one of these comets: * C/1801 N1 * C/1802 Q1 * C/1804 E1 * C/1806 V1 (a.k.a. 1806 II) * C/1808 F1 (a.k.a. 1808 I) * C/1808 M1 (a.k.a. 1808 II) * C/1810 Q1 * C/1811 W1 (a.k.a. 1811 II) * C/1813 C1 (a.k.a. 1813 I) * C/1813 G1 (a.k.a. 1813 II) * C/1816 B1 * C/1817 Y1 (a.k.a. 1818 II) * C/1818 W2 (a.k.a. 1818 III) * C/1822 K1 (a.k.a. 1822 III) * C/1822 N1 (a.k.a. 1822 IV) * C/1825 N1 (a.k.a. 1825 IV) * C/1825 P1 (a.k.a. 1825 II) * C/1825 V1 (a.k.a. 1826 II) * C/1826 P1 (a.k.a. 1826 IV) * C/1826 U1 (a.k.a. 1826 V) * C/1826 Y1 (a.k.a. 1827 I) * C/1827 P1 (a.k.a. 1827 III) Comet Pons may also be a partial reference to: * Comet Nicollet-Pons, C/1821 B1 * 12P/Pons-Brooks (a.k.a. 12P/1812 O1, 12P/1883 R1, 1884 I, 1883b, 12P/1953 M1, 1954 VII, 1953c) * 273P/Pons-Gambart (a.k.a. 273P/1827 M1, 1827 II, 273P/2012 V4) * 7P/Pons-Winnecke (a.k.a. 7P/1819 L1, 1819 III, 7P/1858 E1, 1858 II, 7P/1869 G1, 1869 I, 1869a, 1875 I, 1875b, 1886 VI, 1886d, 1 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
273P/Pons–Gambart
273P/Pons–Gambart, also called Comet Pons-Gambart, is a short-period comet first discovered on June 21, 1827 by Jean-Louis Pons and Jean-Félix Adolphe Gambart. It has a 186 year orbit. It fits the classical definition of a Halley-type comet with (20 years < < 200 years). It was lost and was not recovered until November 7, 2012, when amateur astronomer Rob Matson discovered a comet, and it was identified that the pre-recovery short-arc orbital calculations for Pons-Gambart were completely wrong because the comet only had a 1-month with poor data. The original name when first discovered ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
12P/Pons–Brooks
12P/Pons–Brooks is a periodic comet with an orbital period of 71 years. It fits the classical definition of a Halley-type comet with (20 years < < 200 years). The next passage is 21 April 2024, with closest approach to Earth being on 2 June 2024. The is estimated to be around 30 km in diameter assuming it was not producing too much dust and gas during the 2020 ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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