List of Solar System objects most distant from the Sun

These Solar System minor planets are the furthest from the Sun as of January 2026. The objects have been categorized by their approximate distance from the Sun on that date, and not by the calculated aphelion of their orbit. The list changes over time because the objects are moving in their orbits. Some objects are inbound and some are outbound. It would be difficult to detect long-distance comets if it were not for their comas, which become visible when heated by the Sun. Distances are measured in astronomical units (AU, Sun–Earth distances). The distances are not the minimum (perihelion) or the maximum (aphelion) that may be achieved by these objects in the future.

This list does not include near-parabolic comets of which many are known to be currently more than 100 AU (15 billion km) from the Sun, but are currently too far away to be observed by telescope. Trans-Neptunian objects are typically announced publicly months or years after their discovery, so as to make sure the orbit is correct before announcing it. Due to their greater distance from the Sun and slow movement across the sky, trans-Neptunian objects with observation arcs less than several years often have poorly constrained orbits. Particularly distant objects take several years of observations to establish a crude orbit solution before being announced. For instance, the most distant known trans-Neptunian object 2018 AG37 was discovered by Scott Sheppard in January 2018 but was announced three years later in February 2021.

Notable objects

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. 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. Sedna is the largest known sednoid, a class of objects that play an important role in the Planet Nine hypothesis. The discovery of 2017 OF201 challenges the existence of the hypothetical Planet Nine as its orbit is anti-aligned to the calculated orbit of Planet Nine. It is suggested that the hypothetical planet would have ejected 2017 OF201 from its present-day orbit over times scales of less than 100 million years, though it could be in a temporary orbit.

Pluto (30–49 AU, about 34 AU in 2015) was the first Kuiper belt object to be discovered (1930) and is the largest known dwarf planet.

Six original and eight additional ETNO objects orbits with their positions near their perihelion in purple, with hypothetical Planet Nine orbit in green

Known distant objects

This is a list of known objects at heliocentric distances of more than 80 AU. In theory, the Oort cloud could extend over 120,000 AU (2 ly) from the Sun.

Most distant observable objects in the Solar System (distances in January 2026)
Object name Distance from the Sun (AU) Radial velocity
(AU/yr)
Perihelion Aphelion Semimajor
axis
Apparent
magnitude
Absolute
magnitude (H)
Discovery date Refs
January 2026 At discovery date
Great Comet of 1680
(for comparison)
262.2 1.16 +0.47 0.006 889 444 1680-11-14
Voyager 1
(for comparison)
169.2 +3.56 8.79
Hyperbolic
−3.22
Voyager 2
(for comparison)
141.7 +3.17 21.3
Hyperbolic
−4.03
Pioneer 10
(for comparison)
140.1 +2.50 5.06
Hyperbolic
–6.94
2018 AG37 132.4 132.6 +0.03 27.1 145.0 86.0 25.4 4.2 2018-01-15
2018 VG18 123.9 123.4 +0.05 37.8 123.9 81.3 24.6 3.7 2018-11-10
Heliopause
(for comparison)
~120
Pioneer 11
(for comparison)
116.2 +2.33 9.35
Hyperbolic
–8.14
2020 BE102 110.3 111.2 –0.15 32.9 116.9 74.9 25.6 5.1 2020-01-24
2020 FY30 98.4 99.2 −0.13 35.6 107.7 71.6 24.8 4.7 2020-03-24
2020 FA31 98.0 97.1 +0.15 39.5 102.4 71.0 25.4 5.4 2020-03-24
Eris
136199
95.5 97.0 −0.09 38.3 97.5 67.9 18.8 −1.2 2003-10-21
2020 FQ40 92.2 92.5 −0.05 38.2 93.1 65.6 25.7 6.1 2020-03-24
2015 TH367 92.0 88.2 +0.36 28.9 136.4 82.6 26.3 6.6 2015-10-13
2017 OF201 91.0 85.6 +0.63 44.9 1630 840 22.8 3.5 2017-07-23
2021 DR15 90.2 89.4 +0.16 37.8 96.5 67.2 23.1 3.6 2021-02-17
Gonggong
225088
89.7 85.4 +0.21 33.7 101.2 67.5 21.5 1.6 2007-07-17
2014 UZ224 87.4 92.5 −0.46 38.3 177.0 107.6 23.2 3.4 2014-10-21
2015 FG415 86.6 88.0 −0.15 36.2 92.1 64.1 25.5 6.0 2015-03-17
2014 FC69 86.7 83.7 +0.25 40.4 104.4 72.4 24.2 4.6 2014-03-25
2006 QH181 85.1 82.9 +0.18 37.5 96.7 67.1 23.7 4.3 2006-08-21
Sedna
90377
83.0 89.6 −0.26 76.2 937 484.4 21.0 1.3 2003-11-14
2015 VO166 85.7 82.5 +0.30 38.3 113.2 75.8 25.5 5.9 2015-11-06
2012 VP113 85.0 82.9 +0.18 80.4 462 271.2 23.3 4.0 2012-11-05
2017 SN132 84.8 81.2 +0.43 42.0 110.0 76.0 25.2 5.8 2017-09-16
2015 TJ367 81.3 77.0 +0.41 33.6 128.4 81.0 25.8 6.7 2015-10-13
2013 FS28 80.8 87.9 −0.56 34.2 358.2 196.2 24.3 4.9 2013-03-16
2021 DP15 80.2 79.4 0.16 36.2 86.1 61.1 24.9 5.9 2021-02-16
2015 UH87 80.2 82.4 −0.22 34.3 90.0 62.2 25.2 6.0 2015-10-16
1I/ʻOumuamua
(for comparison)
50.4 1.21 +5.70 0.256
Hyperbolic
–1.27 39 22.1 2017-10-19
This table includes all observable objects located at least 80 AU from the Sun on 1 January 2026.


  1. AU/yr indicates whether the object is moving inwards or outwards in its orbit, and the rate at which it does so.
  2. Distance and orbital elements are crudely estimated based on a short observation arc.

See also

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