(673087) 2015 AJ281
(Redirected from 2011 FW62)
| Discovery | |
|---|---|
| Discovery date | 2011 |
| Designations | |
| 2011 FW62 · 2015 AJ281 | |
| plutino[1] | |
| Orbital characteristics[2] | |
| Epoch 31 May 2020 (JD 2459000.5) | |
| Uncertainty parameter 3 | |
| Aphelion | 48.835 AU (7.3056 Tm) |
| Perihelion | 37.564 AU (5.6195 Tm) |
| 43.199 AU (6.4625 Tm) | |
| Eccentricity | 0.130456 |
| 283.94 yr (103,709 d) | |
| 284.586° | |
| 0° 0m 12.497s / day | |
| Inclination | 26.805° |
| 256.130° | |
| 8.233° | |
| Physical characteristics | |
| Dimensions | 503 km for assumed albedo of 0.07,[3] but likely much smaller if a haumeid |
| 5.0 [2] | |
(673087) 2015 AJ281 (also designated 2011 FW62) is a magnitude-5.0 trans-Neptunian object that was discovered in 2011.[2] Its orbital elements were very uncertain and it was lost. It was recovered on 6 January 2015 as 2015 AJ281. 2011 FW62 has been identified as a member of the Haumea family in a dynamical study led by Proudfoot and Ragozzine in 2019.[4]
References
[edit]- ^ "2010 FW62". Minor Planet Center. Retrieved 31 August 2012.
- ^ a b c "JPL Small-Body Database Browser: (2011 FW62)" (2011-05-26 last obs). Retrieved 12 April 2016.
- ^ Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Archived from the original on 18 October 2011. Retrieved 31 August 2012.
- ^ Proudfoot, Benjamin; Ragozzine, Darin (May 2019). "Modeling the Formation of the Family of the Dwarf Planet Haumea". The Astronomical Journal. 157 (6): 230. arXiv:1904.00038. Bibcode:2019AJ....157..230P. doi:10.3847/1538-3881/ab19c4. S2CID 90262136.
External links
[edit]- (673087) 2015 AJ281 at AstDyS-2, Asteroids—Dynamic Site
- (673087) 2015 AJ281 at the JPL Small-Body Database
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