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  2. List of Solar System objects most distant from the Sun

    en.wikipedia.org/wiki/List_of_Solar_System...

    One particularly distant body is 90377 Sedna, which was discovered in November 2003.It has an extremely eccentric orbit that takes it to an aphelion of 937 AU. [2] It takes over 10,000 years to orbit, and during the next 50 years it will slowly move closer to the Sun as it comes to perihelion at a distance of 76 AU from the Sun. [3] Sedna is the largest known sednoid, a class of objects that ...

  3. Sedna (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Sedna_(dwarf_planet)

    Morbidelli and Kenyon have suggested that Sedna did not originate in the Solar System, but was captured by the Sun from a passing extrasolar planetary system, specifically that of a brown dwarf about 1/20th the mass of the Sun (M ☉) [63] [64] [71] or a main-sequence star 80 percent more massive than the Sun, which, owing to its larger mass ...

  4. 541132 Leleākūhonua - Wikipedia

    en.wikipedia.org/wiki/541132_Leleākūhonua

    [9] [19] It was initially estimated to be 300 km (190 mi) in diameter under the assumption of an albedo of 0.15, [5] though observations of a single-chord stellar occultation at Penticton, Canada on 20 October 2018 suggested a smaller diameter of 220 km (140 mi), corresponding to a higher albedo of 0.21.

  5. List of possible dwarf planets - Wikipedia

    en.wikipedia.org/wiki/List_of_possible_dwarf_planets

    The number of dwarf planets in the Solar System is unknown. Estimates have run as high as 200 in the Kuiper belt [1] and over 10,000 in the region beyond. [2] However, consideration of the surprisingly low densities of many large trans-Neptunian objects, as well as spectroscopic analysis of their surfaces, suggests that the number of dwarf planets may be much lower, perhaps only nine among ...

  6. Sednoid - Wikipedia

    en.wikipedia.org/wiki/Sednoid

    The sednoids' orbits cannot be explained by perturbations from the giant planets, [9] nor by interaction with the galactic tides. [4] If they formed in their current locations, their orbits must originally have been circular; otherwise accretion (the coalescence of smaller bodies into larger ones) would not have been possible because the large relative velocities between planetesimals would ...

  7. ʻOumuamua - Wikipedia

    en.wikipedia.org/wiki/ʻOumuamua

    The pull of the Sun's gravity caused it to speed up until it reached its maximum speed of 87.71 km/s (315,800 km/h; 196,200 mph) as it passed south of the ecliptic on 6 September, where the Sun's gravity bent its orbit in a sharp turn northward at its closest approach (perihelion) on 9 September at a distance of 0.255 AU (38,100,000 km ...

  8. Eris (dwarf planet) - Wikipedia

    en.wikipedia.org/wiki/Eris_(dwarf_planet)

    [2] [58] It retained this distinction until the discovery of 2018 VG 18 in 2018. [ 59 ] As of 2008, there were approximately forty known TNOs , most notably 2006 SQ 372 , 2000 OO 67 and Sedna , that are currently closer to the Sun than Eris, even though their semimajor axis is larger than that of Eris (67.8 AU).

  9. 2018 VG18 - Wikipedia

    en.wikipedia.org/wiki/2018_VG18

    2018 VG 18 is the second-most distant natural object ever observed in the Solar System, after 2018 AG 37 (132 AU), which was also discovered by Sheppard's team in January 2018. As of 2024 [update] , 2018 VG 18 is 123.6 AU (18 billion km) from the Sun and is moving farther away until it reaches aphelion in 2063. [ 8 ]