AnEarth trojan is anasteroid that orbits theSun in the vicinity of theEarth–SunLagrange pointsL4 (leading 60°) orL5 (trailing 60°), thus having an orbit similar to Earth's. Only two Earth trojans have so far been discovered. The name"trojan" was first used in 1906 for theJupiter trojans, the asteroids that were observed near the Lagrangian points ofJupiter's orbit.
An Earth-based search forL5 objects was conducted in 1994, covering 0.35 square degrees of sky, under poor observing conditions.[5] That search failed to detect any objects:
In February 2017, theOSIRIS-REx spacecraft performed a search from within the L4 region on its way to asteroid Bennu.[6] No additional Earth trojans were discovered.[7]
In April 2017, theHayabusa2 spacecraft searched theL5 region while proceeding toasteroid Ryugu,[8] but did not find any asteroids there.[9]
A hypotheticalplanet-sized Earth trojan the size ofMars, given the nameTheia, is thought by proponents of thegiant-impact hypothesis to be the origin of theMoon. The hypothesis states that the Moon formed after Earth and Theia collided,[10] showering material from the two planets into space. This material eventuallyaccreted around Earth and into a single orbiting body, the Moon.[11]
At the same time, material from Theia mixed and combined with Earth's mantle and core. Supporters of the giant-impact hypothesis theorise that Earth's large core in relation to its overall volume is as a result of this combination.
Astronomy continues to retain interest in the subject. A publication[12]describes these reasons thus:
The survival to the present day of an ancient [Earth Trojan] population is reasonably assured provided Earth's orbit itself was not strongly perturbed since its formation. It is therefore pertinent to consider that modern theoretical models of planet formation find strongly chaotic orbital evolution during the final stages of assembly of the terrestrial planets and the Earth–Moon system.
Such chaotic evolution may at first sight appear unfavorable to the survival of a primordial population of[Earth trojans]. However, during and after the chaotic assembly of the terrestrial planets, it is likely that a residual planetesimal population, of a few percent of Earth's mass, was present and helped to damp the orbital eccentricities and inclinations of the terrestrial planets to their observed low values, as well as to provide the so-called "late veneer" of accreting planetesimals to account for the abundance patterns of the highly siderophile elements in Earth's mantle.
Such a residual planetesimal population would also naturally lead to a small fraction trapped in the Earth's Trojan zones as Earth's orbit circularized. In addition to potentially hosting an ancient, long-term stable population of asteroids, Earth's Trojan regions also provide transient traps for NEOs that originate from more distal reservoirs of small bodies in the solar system like the main asteroid belt.
Several other small objects have been found on an orbital path associated with Earth. Although these objects are in 1:1 orbital resonance, they are not Earth trojans, because they do notlibrate around a definite Sun–Earth Lagrangian point, neitherL4 norL5.
Earth has another noted companion, asteroid3753 Cruithne. About 5 km across, it has a peculiar type of orbital resonance called anoverlapping horseshoe, and is probably only a temporary liaison.[13]
469219 Kamoʻoalewa, anasteroid discovered on 27 April 2016, is possibly the most stablequasi-satellite ofEarth.[14]
![Illustration of Trojan Asteroid 2020 XL5 [15]](/mt/?noimg=&dark=on&url=https%3a%2f%2fen.wikipedia.org%2fwiki%2fFile%3aIllustration_of_Trojan_Asteroid_2020_XL5.jpg)
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