Back 2010 GB174 Catalan 2010 GB174 German 2010 GB174 Spanish 2010 GB174 French 2010 GB174 Japanese 2010 GB174 Portuguese 2010 GB174 Russian 2010 GB174 Vietnamese
 Orbits of 2010 GB174 (dark blue) and other scattered/detached objects, along with hypothetical Planet Nine on the right | |
| Discovery | |
|---|---|
| Discovery date | 12 April 2010 |
| Designations | |
Designation | 2010 GB174 |
| detached object | |
| Orbital characteristics[1] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Observation arc | 2.64 years |
| Earliest precovery date | 26 June 2009 |
| Aphelion | |
| Perihelion | 48.7±0.3 AU |
| Eccentricity | 0.869±0.01 |
| 3.22°±0.4° | |
| 0° 0m 0.575s / day | |
| Inclination | 21.54° |
| 130.6° (Ω) | |
| ≈ 1951-Aug-20[4] | |
| 347.8°±0.4° (ω) | |
| Physical characteristics | |
| Dimensions | |
| Albedo | 0.08 (assumed)[5] |
| 25.2[7] | |
| 6.6[1] | |
2010 GB174 is a detached object, discovered on 12 April 2010 on data taken at the Canada France Hawaii Telescope as part of the Next Generation Virgo Cluster Survey.[8][9] It never gets closer than 48.5 AU from the Sun (about the outer edge of the Kuiper belt). Its large eccentricity strongly suggests that it was gravitationally scattered onto its current orbit. It is, like all detached objects, outside the current influence of Neptune, so how it got its current orbit is unknown. 2010 GB174 has the third highest Tisserand parameter relative to Jupiter of any Trans-Neptunian object, after Sedna and 2012 VP113. It has not been observed since 2015.[1] It comes to opposition in late March each year in the constellation of Virgo.
Precovery images have been found back to 26 June 2009.[1]
It reached perihelion (closest approach to the Sun) in mid-1951[4] and has moved beyond 70 AU in September 2014.[7] It is possibly a dwarf planet.[5]
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AstDySwas invoked but never defined (see the help page). - ^ Chen, Ying-Tung; Kavelaars, J. J.; Gwyn, Stephen; Ferrarese, Laura; Côté, Patrick; Jordán, Andrés; Suc, Vincent; Cuillandre, Jean-Charles; Ip, Wing-Huen (1 September 2013). "Discovery of a New Member of the Inner Oort Cloud from the Next Generation Virgo Cluster Survey". The Astrophysical Journal. 775 (1): L8. arXiv:1308.6041. Bibcode:2013ApJ...775L...8C. doi:10.1088/2041-8205/775/1/L8. ISSN 0004-637X.
- ^ "Home". NGVS. Retrieved 11 January 2022.
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