Astronomy:2011 FW62
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Short description: Trans-Neptunian asteroid
Discovery | |
---|---|
Discovery date | 2011 |
Designations | |
2011 FW62 · 2015 AJ281 | |
Minor planet category | plutino[1] |
Orbital characteristics[2] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 3 | |
|{{{apsis}}}|helion}} | 48.835 astronomical unit|AU (7.3056 Tm) |
|{{{apsis}}}|helion}} | 37.564 AU (5.6195 Tm) |
43.199 AU (6.4625 Tm) | |
Eccentricity | 0.130456 |
Orbital period | 283.94 yr (103,709 d) |
Mean anomaly | 284.586° |
Mean motion | 0° 0m 12.497s / day |
Inclination | 26.805° |
Longitude of ascending node | 256.130° |
8.233° | |
Physical characteristics | |
Dimensions | 503 km for assumed albedo of 0.07,[3] but likely much smaller if a haumeid |
Absolute magnitude (H) | 5.0 [2] |
2011 FW62, also designated 2015 AJ281, 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
- ↑ "2010 FW62". Minor Planet Center. http://www.minorplanetcenter.net/db_search/show_object?object_id=2011+FW62.
- ↑ 2.0 2.1 2.2 "JPL Small-Body Database Browser: (2011 FW62)". http://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2011FW62.
- ↑ Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. http://www.gps.caltech.edu/~mbrown/dps.html.
- ↑ Proudfoot, Benjamin; Ragozzine, Darin (May 2019). "Modeling the Formation of the Family of the Dwarf Planet Haumea". The Astronomical Journal 157 (6): 230. doi:10.3847/1538-3881/ab19c4. Bibcode: 2019AJ....157..230P.
External links
- 2011 FW62 at AstDyS-2, Asteroids—Dynamic Site
- 2011 FW62 at the JPL Small-Body Database
Original source: https://en.wikipedia.org/wiki/2011 FW62.
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