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The orbit of 2013 FT28 (right side in light blue, click image to enlarge) and other extreme detached objects, along with the hypothetical Planet Nine's orbit on the right
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| Discovery | |
|---|---|
| Discovered by | Scott S. Sheppard and Chad Trujillo |
| Discovery date | March 16, 2013 |
| Designations | |
| MPC designation | 2013 FT28 |
| Extreme | |
| Orbital characteristics | |
| Epoch 2016-July-31.0 (JD 2457600.5) | |
| Uncertainty parameter 4 | |
| Observation arc | 1089 days (2.98 yr) |
| Aphelion | 546 AU (barycentric) 580 AU |
| Perihelion | 43.6 AU |
| 295 AU (barycentric) 312 AU |
|
| Eccentricity | 0.86 |
| 5051 yr (barycentric) 5460 yr (89370.137 d) |
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| 357.15° | |
| Inclination | 17.3 ° |
| 217.7° | |
| 40.2° | |
| Physical characteristics | |
| Dimensions | 100–400 km |
| 24.3 | |
| 6.7 | |
2013 FT28 is a Trans-Neptunian object. The existence of the TNO was revealed on 30 August 2016. 2013 FT28 is the first high semi-major axis, high perihelion extreme trans-Neptunian object that is anti-aligned with the other known extreme trans-Neptunian objects such as Sedna and 2012 VP113 i.e. its longitude of perihelion differs by 180° from other objects. The orbit of 2013 FT28 appears stable though simulations showed that it there may be some resonant interaction the known giant planets.