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  2. Trojan (celestial body) - Wikipedia

    en.wikipedia.org/wiki/Trojan_(celestial_body)

    Whether or not a system of star, planet, and trojan is stable depends on how large the perturbations are to which it is subject. If, for example, the planet is the mass of Earth, and there is also a Jupiter-mass object orbiting that star, the trojan's orbit would be much less stable than if the second planet had the mass of Pluto.

  3. Jupiter trojan - Wikipedia

    en.wikipedia.org/wiki/Jupiter_trojan

    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 points : either L 4 , existing 60° ahead of the planet in its orbit, or L 5 , 60° behind.

  4. 17365 Thymbraeus - Wikipedia

    en.wikipedia.org/wiki/17365_Thymbraeus

    Minor planet category. Jupiter trojan [2] [1] Trojan (L 5) [3] ... 17365 Thymbraeus (provisional designation 1978 VF 11) is a Jupiter trojan from the Trojan camp, ...

  5. List of directly imaged exoplanets - Wikipedia

    en.wikipedia.org/wiki/List_of_directly_imaged_e...

    Motion interpolation of seven images of the HR 8799 system taken from the W. M. Keck Observatory over seven years, featuring four exoplanets. This is a list of extrasolar planets that have been directly observed, sorted by observed separations. This method works best for young planets that emit infrared light and are far from the glare of the star.

  6. 624 Hektor - Wikipedia

    en.wikipedia.org/wiki/624_Hektor

    Hektor is the first known trojan with a satellite companion and, so far, one of only four known binary trojan asteroids in the L 4 group (the others being 16974 Iphthime, 3548 Eurybates, and 15094 Polymele). 617 Patroclus, another large trojan asteroid of the L 5 group, consists of two almost equal-sized components. [13]

  7. (706765) 2010 TK7 - Wikipedia

    en.wikipedia.org/wiki/(706765)_2010_TK7

    [4] [5] Trojan objects are most easily conceived as orbiting at a Lagrangian point, a dynamically stable location (where the combined gravitational force acts through the Sun's and Earth's barycenter) 60 degrees ahead of or behind a massive orbiting body, in a type of 1:1 orbital resonance. In reality, they oscillate around such a point.

  8. 1437 Diomedes - Wikipedia

    en.wikipedia.org/wiki/1437_Diomedes

    1437 Diomedes / ˌ d aɪ ə ˈ m iː d iː z / is a large Jupiter trojan from the Greek camp, approximately 150 kilometers (90 miles) in diameter.It was discovered on 3 August 1937, by astronomer Karl Reinmuth at the Heidelberg-Königstuhl State Observatory in southwest Germany. [1]

  9. 1404 Ajax - Wikipedia

    en.wikipedia.org/wiki/1404_Ajax

    1404 Ajax / ˈ eɪ dʒ æ k s / is a carbonaceous Jupiter trojan from the Greek camp, approximately 83 kilometers (52 miles) 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. [1]