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Trojan asteroids

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Trojan asteroids, two groups of asteroids asteroid, planetoid, or minor planet, small body orbiting the sun. More than 10,000 asteroids have orbits sufficiently well known to have been cataloged and named; thousands more exist.
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 that revolve about the sun in the same orbit as Jupiter; one group is about 60° ahead of the planet in the orbit, the other about 60° behind it. In 1990, a similar asteroid, Eureka, was found in the orbit of Mars. Some of the Trojan asteroids are composed of ice and dirt, rather than rock, making it possible that they are captured comets. The Trojan asteroids represent one possible special solution to the famous three-body problem (see celestial mechanics celestial mechanics, the study of the motions of astronomical bodies as they move under the influence of their mutual gravitation. Celestial mechanics analyzes the orbital motions of planets, dwarf planets, comets, asteroids, and natural and artificial satellites
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), with each group forming an equilateral triangle with Jupiter and the sun. The first Trojan asteroid discovered was Achilles, observed in 1904 by the German astronomer Max Wolf; all of these asteroids are named for heroes of the Trojan War Trojan War, in Greek mythology, war between the Greeks and the people of Troy. The strife began after the Trojan prince Paris abducted Helen, wife of Menelaus of Sparta. When Menelaus demanded her return, the Trojans refused.
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Trojan asteroids

Two groups of asteroids named for heroes of Greece and Troy in Homer's Iliad. These objects revolve around the Sun at the Lagrangian points (see Joseph-Louis Lagrange) in Jupiter's orbit. Achilles, the first, was discovered in 1906. About 650 are known, but their actual number is estimated in the thousands. The term Trojan also applies to objects occupying the corresponding Lagrangian points in the orbits of other planets. Two such asteroids were discovered in Mars's orbit in the 1990s.



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Past simulations have tracked the trajectories of these planetesimals and showed they wind up forming the Kuiper belt of icy debris where Pluto sits, some of the distant satellites of Jupiter and Saturn, and Trojan asteroids, bodies that share Jupiter's orbit but are centred at two points ahead of and behind the planet.
Some of the debris became trapped by Jupiter's gravity and could account for the planet's retinue of Trojan asteroids, a group of objects that lead and trail the planet today, and have not been explained by any other theory, says Levison.
The sun, Jupiter, and the so-called Trojan asteroids, for instance, form such a triangle, which rotates about the system's center of mass.
 
 
 
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