Safekipedia

Detached object

Adapted from Wikipedia · Discoverer experience

The Crab Nebula is a beautiful cosmic cloud formed from the remnants of an ancient star explosion, showing colorful gases spreading through space.

Detached objects are a special group of small planets found far away from the Sun, in a part of space called the outer Solar System. These objects belong to a larger family known as trans-Neptunian objects, which orbit beyond the planet Neptune. What makes detached objects different is their distance from the Sun. They orbit so far out that the gravity of Neptune and other planets barely affects them, making them seem "detached" from the rest of the Solar System.

Unlike most other trans-Neptunian objects, which have been moved by the gravity of large planets like Neptune, detached objects stay in orbits that are far away from these influences. They have points of closest approach to the Sun that are much larger than those of other objects, such as Pluto, Makemake, and Eris. Because of this, scientists sometimes call them extended scattered disc objects, distant detached objects, or scattered–extended objects.

Scientists have found at least nine of these detached objects. The most famous one is Sedna, which is the largest, farthest, and best known. Objects like Sedna, with very large orbits and very distant points of closest approach to the Sun, are called sednoids. As of 2025, four sednoids are known, including 2012 VP113, Leleākūhonua, and 2023 KQ14. These objects show patterns in their orbits that might be caused by the pull of planets we have not yet discovered.

Orbits

Detached objects have orbits that stay very far from the Sun. Their closest points to the Sun are much larger than the farthest point of Neptune's orbit. These objects often have very stretched-out, long paths around the Sun, reaching up to a few hundred times the distance from the Earth to the Sun.

Scientists are still trying to understand how these objects got their unusual orbits. Some ideas include the pull of a passing star, a very far-off object about the size of a planet, or the movement of Neptune long ago. Another idea is the possible influence of a large, unseen planet far beyond Neptune.

Classification

Detached objects are a special group of objects far from the Sun in our Solar System. They belong to a larger group called trans-Neptunian objects (TNOs). Unlike most TNOs, detached objects have orbits that keep them far away from the planet Neptune. This distance means Neptune's gravity does not affect them much, making them seem "detached" from the rest of the Solar System.

These objects usually come closer to the Sun (perihelion) at a distance greater than 40 AU, which is much farther than Neptune's orbit. Because of this, they do not interact strongly with Neptune. Some scientists think these objects might be part of a region called the inner Oort cloud or a link between a group of objects called the scattered disc and the Oort cloud. Studying these objects helps us learn more about how the giant planets moved and how the Solar System formed.

Possible detached objects

See also: Sednoid and Extreme trans-Neptunian object

This is a list of objects found by discovery date that might be detached objects because they are not easily moved by Neptune's orbit. They are close to the Sun but still far enough to seem "detached" from the rest of the Solar System.

These objects have points where they get closest to the Sun (perihelion) more than 40 AU away and their average distance from the Sun (semi-major axis) is more than 47.7 AU away.

Some other objects are also thought to be detached objects, though they are a little closer to the Sun, with perihelion distances between 38–40 AU.

DesignationDiameter
(km)
Hq
(AU)
a
(AU)
Q
(AU)
ω (°)Discovery
Year
DiscovererNotes & Refs
2000 CR1052436.344.252221.2398316.932000M. W. Buie
2000 YW1342164.741.20757.79574.383316.4812000Spacewatch≈3:8 Neptune resonance
2001 FL193818.740.2950.2660.23108.62001R. L. Allen, G. Bernstein, R. Malhotraorbit extremely poor, might not be a TNO
2001 KA776345.043.4147.7452.07120.32001M. W. Buieborderline classical KBO
2002 CP1542226.5425262502002M. W. Buieorbit fairly poor, but definitely a detached object
2003 UY2911477.441.1948.9556.7215.62003M. W. Buieborderline classical KBO
Sedna9951.576.072483.3890311.612003M. E. Brown, C. A. Trujillo, D. L. RabinowitzSednoid
2004 PD1122676.1407090402004M. W. Buieorbit very poor, might not be a detached object
Alicanto2226.547.308315584326.9252004Cerro Tololo (unspecified)
2004 XR1906124.151.08557.33663.586284.932004R. L. Allen, B. J. Gladman, J. J. Kavelaars
J.-M. Petit, J. W. Parker, P. Nicholson
very high inclination; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination of 2004 XR190 to obtain a very high perihelion
2005 CG812676.141.0354.1067.1857.122005CFEPS
2005 EO2971617.241.21562.9884.75349.862005M. W. Buie
2005 TB1903724.546.19775.546104.896171.0232005A. C. Becker, A. W. Puckett, J. M. KubicaNeptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a high perihelion
2006 AO1011687.12006Mauna Kea (unspecified)orbit extremely poor, might not be a TNO
2007 JJ435584.540.38348.39056.3976.5362007Palomar (unspecified)borderline classical KBO
2007 LE381767.041.79854.5667.3253.962007Mauna Kea (unspecified)
2008 ST2916404.242.2799.3156.4324.372008M. E. Schwamb, M. E. Brown, D. L. Rabinowitz≈1:6 Neptune resonance
2009 KX361118.01001002009Mauna Kea (unspecified)orbit extremely poor, might not be a TNO
2010 DN934864.745.10255.50165.9033.012010Pan-STARRS≈2:5 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a high perihelion
2010 ER654045.040.03599.71159.39324.192010D. L. Rabinowitz, S. W. Tourtellotte
2010 GB1742226.548.8360670347.72010Mauna Kea (unspecified)
2012 FH841617.2425670102012Las Campanas (unspecified)
2012 VP1137024.080.47256431293.82012S. S. Sheppard, C. A. TrujilloSednoid
2013 FQ282806.045.963.180.32302013S. S. Sheppard, C. A. Trujillo≈1:3 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a high perihelion
2013 FT282026.743.531058040.32013S. S. Sheppard
2013 GP1362126.641.061155.1269.142.382013OSSOS
2013 GQ1362226.540.7949.0657.33155.32013OSSOSborderline classical KBO
2013 GG1382126.646.6447.79248.9461282013OSSOSborderline classical KBO
2013 JD641118.042.60373.12103.63178.02013OSSOS
2013 JJ641477.444.0448.15852.272179.82013OSSOSborderline classical KBO
2013 SY992026.750.02694133832.12013OSSOS
2013 SK1001347.645.46861.6177.7611.52013OSSOS
2013 UT152556.343.89195.7348252.332013OSSOS
2013 UB171767.044.4962.3180.13308.932013OSSOS
2013 VD241287.84050701972013Dark Energy Surveyorbit very poor, might not be a detached object
2013 YJ1513365.440.86672.35103.83141.832013Pan-STARRS
2014 EZ517703.740.7052.4964.28329.842014Pan-STARRS
2014 FC695334.640.2873.06105.8190.572014S. S. Sheppard, C. A. Trujillo
2014 FZ711856.955.976.296.52452014S. S. Sheppard, C. A. Trujillo≈1:4 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a very high perihelion
2014 FC725094.551.67076.329100.9932.852014Pan-STARRS≈1:4 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a very high perihelion
2014 JM803525.546.0063.0080.0196.12014Pan-STARRS≈1:3 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a high perihelion
2014 JS803065.540.01348.29156.569174.52014Pan-STARRSborderline classical KBO
2014 OJ3944235.040.8052.9765.14271.602014Pan-STARRSin 3:7 Neptune resonance
2014 QR4411936.842.667.893.02832014Dark Energy Survey
2014 SR3492026.647.6300540341.12014S. S. Sheppard, C. A. Trujillo
2014 SS3491347.6451402401482014S. S. Sheppard, C. A. Trujillo≈2:10 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a high perihelion
2014 ST3733305.550.13104.0157.8297.522014Dark Energy Survey
2014 UT2281547.343.9748.59353.21649.92014OSSOSborderline classical KBO
2014 UA2302226.542.2755.0567.84132.82014OSSOS
2014 UO231978.342.2555.1167.98234.562014OSSOS
2014 WK5095844.040.0850.7961.50135.42014Pan-STARRS
2014 WB5561477.442.62805202342014Dark Energy Survey
2015 AL2812936.14248541202015Pan-STARRSborderline classical KBO
orbit very poor, might not be a detached object
2015 AM2814864.841.38055.37269.364157.722015Pan-STARRS
2015 BE5193525.544.8247.86650.909293.22015Pan-STARRSborderline classical KBO
2015 FJ3451177.95163.075.2782015S. S. Sheppard, C. A. Trujillo≈1:3 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a very high perihelion
2015 GP502226.540.455.270.01302015S. S. Sheppard, C. A. Trujillo
2015 KH1626713.941.6362.2982.95296.8052015S. S. Sheppard, D. J. Tholen, C. A. Trujillo
2015 KG1631018.340.502826161032.062015OSSOS
2015 KH1631177.940.06157.2274230.292015OSSOS≈1:12 Neptune resonance
2015 KE1721068.144.137133.12222.115.432015OSSOS1:9 Neptune resonance
2015 KG1722806.0425569352015R. L. Allen
D. James
D. Herrera
orbit fairly poor, might not be a detached object
2015 KQ1741547.349.3155.4061.48294.02015Mauna Kea (unspecified)≈2:5 Neptune resonance; Neptune Mean Motion Resonance (MMR) along with the Kozai Resonance (KR) modified the eccentricity and inclination to obtain a very high perihelion
2015 RX2452556.245.541078065.32015OSSOS
Leleākūhonua3005.565.0210422019118.02015S. S. Sheppard, C. A. Trujillo, D. J. TholenSednoid
2017 DP1211617.240.5250.4860.45217.92017
2017 FP1611687.140.8847.9955.12182017borderline classical KBO
2017 SN132975.840.94979.868118.786148.7692017S. S. Sheppard, C. A. Trujillo, D. J. Tholen
2018 VM351347.645.289240.575435.861302.0082018Mauna Kea (unspecified)
DesignationDiameter
(km)
Hq
(AU)
a
(AU)
Q
(AU)
ω (°)Discovery
Year
DiscovererNotes & Refs
2003 HB571477.438.116166.229411.0822003Mauna Kea (unspecified)
2003 SS4221687.0439.574198.181356.788206.8242003Cerro Tololo (unspecified)
2005 RH521287.838.957152.6266.332.2852005CFEPS
2007 TC4341687.039.577128.41217.23351.0102007Las Campanas (unspecified)1:9 Neptune resonance
2012 FL842126.638.607106.25173.89141.8662012Pan-STARRS
2014 FL721936.838.1104170259.492014Cerro Tololo (unspecified)
2014 JW803525.538.161142.62247.1131.612014Pan-STARRS
2014 YK502935.638.972120.52202.1169.312014Pan-STARRS
2015 DM3198.7839.491272.302505.11343.2272015OSSOS
2015 GT50888.638.46333627129.32015OSSOS

Images

A colorful image of Ceres, a dwarf planet, showing bright craters like Haulani and Oxo on its surface.
A colorful image of the planet Pluto showing its icy surface and famous 'heart' region, taken by NASA's New Horizons spacecraft.
A colorful illustration of the planets in our solar system, showing Mercury, Venus, Earth with its Moon, Mars, Jupiter, Saturn, Uranus, and Neptune.
A stunning view of our planet Earth from space, showing Africa, Antarctica, and the Arabian Peninsula as seen by the Apollo 17 crew in 1972.
A stunning view of Earth rising over the lunar horizon, as seen by astronauts on the Apollo 8 mission.

Related articles

This article is a child-friendly adaptation of the Wikipedia article on Detached object, available under CC BY-SA 4.0.

Images from Wikimedia Commons. Tap any image to view credits and license.