Jupiter trojans are asteroids that share the planet Jupiter’s orbit around the Sun. Relative to Jupiter, each Trojan librates around one of Jupiter’s stable Lagrange points: L4, lying 60° ahead of the planet in its orbit, or L5, 60° behind. The first Jupiter trojan discovered, 588 Achilles, was spotted in 1906 by German astronomer Max Wolf. Estimates of the total Jupiter troJans range from 1 million to 7,000, depending on the method used to calculate their orbits.
About Jupiter trojan in brief

They vary in densities from 0. 8 to 2. 5 g·cm−3, with the densities between 0.8 and 2.5 g·cm+3 at the leading and trailing points of their orbits, and 0.4 to 0.5 g cm+2 at the trailing points. The term ‘Trojan Asteroid’ is normally understood to specifically mean the Jupiter tro jans. But the general term ‘trojan’ is sometimes more generally applied to other small Solar System bodies with similar relationships to larger bodies, such as Mars and Neptune. There are also a number of recently discovered Earth trojan asteroids, as well as a more recently discovered Mars trojan asteroid, and a Neptune trojan. The asteroids are named after Greek heroes of Troy, and those in the trailing orbit after the Greek spy in the Trojan node in Jupiter’s Jupiter node. They were named before the rule was devised, resulting in a Trojan spy node in the Greek Trojan War. Those associated with Jupiter were the first to be discovered, with Achilles being the first asteroid known to reside at the L5 Lagrangian point. By 1938, 11 Jupitertrojans had been detected. This number increased to 14 only in 1961. As instruments improved, the rate of discovery grew rapidly: by January 2000, a total of 257 had been discovered. By May 2003, the number had grown to 1, and by October 2000, there were 257 of them.
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This page is based on the article Jupiter trojan published in Wikipedia (as of Dec. 06, 2020) and was automatically summarized using artificial intelligence.






