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List Of Jupiter Trojans (Greek Camp) (1–100000)
This is a partial list of Jupiter's trojans (60° ahead of Jupiter) with numbers 1–100000 . 1–100000 This list contains 561 objects sorted in numerical order. top References {{DEFAULTSORT:List of Jupiter Trojans (Greek camp) (1-100000) Greek_0 Jupiter Trojans (Trojan Camp) The Jupiter trojans, commonly called trojan asteroids or simply trojans, are a large group of asteroids that share the planet Jupiter's orbit around the Sun. Relative to Jupiter, each trojan librates around one of Jupiter's stable Lagrange poi ... Lists of Jupiter trojans ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Jupiter
Jupiter is the fifth planet from the Sun and the List of Solar System objects by size, largest in the Solar System. It is a gas giant with a mass more than two and a half times that of all the other planets in the Solar System combined, but slightly less than one-thousandth the mass of the Sun. Jupiter is the List of brightest natural objects in the sky, third brightest natural object in the Earth's night sky after the Moon and Venus, and it has been observed since Pre-history, prehistoric times. It was named after the Jupiter (mythology), Roman god Jupiter, the king of the gods. Jupiter is primarily composed of hydrogen, but helium constitutes one-quarter of its mass and one-tenth of its volume. It probably has a rocky core of heavier elements, but, like the other giant planets in the Solar System, it lacks a well-defined solid surface. The ongoing contraction of Jupiter's interior generates more heat than it receives from the Sun. Because of its rapid rotation, the planet' ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
659 Nestor
659 Nestor is a dark Jupiter trojan from the Greek camp, approximately in diameter. It was discovered on 23 March 1908, by German astronomer Max Wolf at Heidelberg Observatory in southern Germany, and named after King Nestor from Greek mythology. The carbonaceous Jovian asteroid belongs to the 20 largest Jupiter trojans and has a rotation period of 15.98 hours. Orbit and classification ''Nestor'' is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60 ° ahead its orbit in a 1:1 resonance ''(see Trojans in astronomy)''. It is also a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 4.6–5.8 AU once every 11 years and 9 months (4,294 days; semi-major axis of 5.17 AU). Its orbit has an eccentricity of 0.12 and an inclination of 5 ° with respect to the ecliptic. As no precoveries were taken, the body's observation arc begins with its official discovery observation at Heidelberg in ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Ingrid Van Houten-Groeneveld
Ingrid van Houten-Groeneveld (; 21 October 1921 – 30 March 2015) was a Dutch astronomer. Background In a jointly credited trio with Tom Gehrels and her husband Cornelis Johannes van Houten, she was the discoverer of many thousands of asteroids (credited by the Minor Planet Center with the discovery of 4,641 numbered minor planets). In the Palomar–Leiden survey, Gehrels took the images using the 48-inch Schmidt telescope at Palomar Observatory and shipped the photographic plates to the van Houtens at Leiden Observatory, who analyzed them for new asteroids. The trio are jointly credited with several thousand asteroid discoveries. Van Houten-Groeneveld died on 30 March 2015, at the age of 93, in Oegstgeest, Netherlands. The Themistian main-belt asteroid 1674 Groeneveld – discovered by Karl Reinmuth at Heidelberg and independently discovered by Finnish astronomer Yrjö Väisälä Yrjö Väisälä (; 6 September 1891 – 21 July 1971) was a Finnish astronomer ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Cornelis Johannes Van Houten
Cornelis Johannes van Houten (18 February 1920 – 24 August 2002) was a Dutch astronomer, sometimes referred to as Kees van Houten. Early life and education Born in The Hague, he spent his entire career at Leiden University except for a brief period (1954–1956) as research assistant at Yerkes Observatory. Family He married fellow astronomer Ingrid Groeneveld (who became Ingrid van Houten-Groeneveld) and together they became interested in asteroids. They had one son, Karel. Work as astronomer In a jointly credited trio with Tom Gehrels and Ingrid, he was an extremely prolific discoverer of many thousands of asteroids. Gehrels did a sky survey using the 48-inch Schmidt telescope at Palomar Observatory and shipped the plates to the van Houtens at Leiden Observatory, who analyzed them for new asteroids. The trio are jointly credited with several thousand discoveries. When the orbit of an asteroid is determined, it can be classified as an Apollo asteroid (e.g. 1862 Apollo), an ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1868 Thersites
1868 Thersites is a large Jupiter trojan from the Greek camp, approximately in diameter. Discovered during the Palomar–Leiden survey at Palomar in 1960, it was later named after the warrior Thersites from Greek mythology. The presumed carbonaceous C-type asteroid belongs to the 50 largest Jupiter trojans and has a rotation period of 10.48 hours. Discovery ''Thersites'' was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten at Leiden, on photographic plates taken by Tom Gehrels at the Palomar Observatory in California. On the same day, the group discovered another Jupiter trojan, 1869 Philoctetes. The body's observation arc begins with a precovery taken at Palomar in March 1954, more than 6 years prior to its official discovery observation. Palomar–Leiden survey The provisional survey designation "P-L" stands for ''Palomar–Leiden'', named after the Palomar and Leiden observatories, which collaborated on the fruitful Palomarâ ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1749 Telamon
1749 Telamon is a dark Jupiter Trojan from the Greek camp, approximately in diameter. It was discovered by German astronomer Karl Reinmuth at the Heidelberg Observatory on 23 September 1949, and named after Telamon from Greek mythology. The D-type asteroid is the principal body of the proposed Telamon family and belongs to the #Largest Jupiter trojans, 60 largest Jupiter trojans. It has a rotation period of 17.0 hours and possibly a spherical shape. Classification and orbit ''Telamon'' is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60degree (angle), ° ahead of the Gas Giant's orbit in a Orbital resonance, 1:1 resonance ''(see Trojans in astronomy)''. It orbits the Sun at a distance of 4.6–5.7 Astronomical unit, AU once every 11 years and 8 months (4,268 days; semi-major axis of 5.15 AU). Its orbit has an orbital eccentricity, eccentricity of 0.11 and an orbital inclination, inclination of 6Degree (angle), ° with respe ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Seth Barnes Nicholson
Seth Barnes Nicholson (November 12, 1891 – July 2, 1963) was an American astronomer. He worked at the Lick observatory in California, and is known for discovering several moons of Jupiter in the 20th century. Nicholson was born in Springfield, Illinois, and was raised in rural Illinois. He was educated at Drake University, where he became interested in astronomy. In 1914, at the University of California's Lick Observatory, while observing the recently discovered Jupiter moon Pasiphaë, he discovered a new one, Sinope, whose orbit he computed for his Ph.D. thesis in 1915. He spent his entire career at Mount Wilson Observatory, where he discovered three more Jovian moons: Lysithea and Carme in 1938, and Ananke in 1951. While at the Palomar Observatory in 1957, he discovered 1647 Menelaus, an asteroid near Jupiter. Other work included computing the orbits of several comets and also that of Pluto. Sinope, Lysithea, Carme, and Ananke were simply designated as "Jupiter IX", ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1647 Menelaus
1647 Menelaus is a mid-sized Jupiter trojan from the Greek camp, approximately in diameter. It was discovered on 23 June 1957 by American astronomer Seth Nicholson at the Palomar Observatory in California, and later named after the Spartan King Menelaus from Greek mythology. The dark asteroid has a rotation period of 17.7 hours. It is the principal body of the proposed Menelaus cluster, which encompasses several, mostly tentative Jovian asteroid families. Orbit and classification ''Menelaus'' is a dark Jovian asteroid in a 1:1 orbital resonance with Jupiter. It is located in the leading Greek camp at the Gas Giant's Lagrangian point, 60 ° ahead on its orbit . Since the discovery of the first Jupiter trojan, 588 Achilles, by astronomer Max Wolf in 1906, more than 7000 Jovian asteroids have already been discovered. It orbits the Sun at a distance of 5.1–5.3 AU once every 11 years and 11 months (4,347 days; semi-major axis of 5.21 AU). Its orbit has an eccentrici ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
Sylvain Arend
Sylvain Julien Victor Arend (6 August 1902 – 18 February 1992) was a Belgian astronomer born in Robelmont, Luxembourg province, Belgium. His main interest was astrometry. Together with Georges Roland, he discovered the bright comet C/1956 R1 (Arend-Roland). He also discovered, or co-discovered, the periodic comets 49P/Arend-Rigaux and 50P/Arend, Nova Scuti 1952, and a number of asteroids, including notably the Amor asteroid 1916 Boreas and the Trojan asteroid 1583 Antilochus. He also discovered 1652 Hergé which is named after Hergé, the creator of ''The Adventures of Tintin''. The asteroid 1563 Noël is named after his son, Emanuel Arend. In 1948 Arend started together with sixteen other people the skeptic organisation Comité Para The Comité Para, in full Comité belge pour l'Analyse Critique des parasciences ("Belgian Committee for the Critical Analysis of Parasciences"), is a Francophone Belgian skeptical non-profit organisation. Founded in 1949, the Comité ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1583 Antilochus
1583 Antilochus is a large Jupiter trojan from the Greek camp, approximately in diameter. It was discovered on 19 September 1950, by Belgian astronomer Sylvain Arend at Uccle Observatory in Belgium, and later named after the hero Antilochus from Greek mythology. The dark D-type asteroid belongs to the 20 largest Jupiter trojans and has a rotation period of 15.9 hours. It forms an asteroid pair with 3801 Thrasymedes. Classification and orbit ''Antilochus'' is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60 ° ahead of its orbit in a 1:1 resonance . It is also a non-family asteroid in the Jovian background population. It orbits the Sun at a distance of 4.9–5.4 AU once every 11 years and 7 months (4,244 days; semi-major axis of 5.13 AU). Its orbit has an eccentricity of 0.05 and an inclination of 29 ° with respect to the ecliptic. The asteroid was first observed as ' at Heidelberg Observatory in November 1926. The ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1437 Diomedes
1437 Diomedes is a large Jupiter trojan from the Greek camp, approximately in diameter. It was discovered on 3 August 1937, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. The dark D/P-type asteroid belongs to the largest Jupiter trojans and has a notably elongated shape and a longer than average rotation period of 24.49 hours. ''Diomedes'' was the first Jupiter trojan successfully observed during an occultation event of star. It was named after the hero Diomedes from Greek mythology. Orbit and classification ''Diomedes'' is a dark Jovian asteroid orbiting in the leading Greek camp at Jupiter's Lagrangian point, 60 ° ahead of the Gas Giant's orbit in a 1:1 resonance . It is also a non-family asteroid in the Jovian background population. Jupiter trojans are thought to have been captured into their orbits during or shortly after the early stages of the formation of the Solar System. More than 4,500 Jupiter trojans in the ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
1404 Ajax
1404 Ajax is a carbonaceous Jupiter trojan from the Greek camp, approximately kilometers in diameter. It was discovered on 17 August 1936, by German astronomer Karl Reinmuth at Heidelberg Observatory in southern Germany, and named after the legendary warrior Ajax from Greek mythology. The assumed C-type asteroid belongs to the 40 largest Jupiter trojans and has a longer than average rotation period of 29.4 hours. Orbit and classification ''Ajax'' is a C-type asteroid, that orbits in the leading Greek camp at Jupiter's Lagrangian point, 60 ° ahead of its orbit ''(see Trojans in astronomy)''. It is also a non-family asteroid in the Jovian background population. Jupiter trojans are thought to have been captured into their orbits during or shortly after the early stages of the formation of the Solar System. More than 4,500 Jupiter trojans in the Greek camp and 7,000 in total have been discovered. It orbits the Sun at a distance of 4.7–5.9 AU once every 12 years and ... [...More Info...] [...Related Items...] OR: [Wikipedia] [Google] [Baidu] |
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