(86047) 1999 OY3
Discovery | |
---|---|
Discovery date | July 18, 1999 |
Designations | |
MPC designation | (86047) 1999 OY3 |
none | |
Cubewano (MPC)[1] Extended (DES)[2] | |
Orbital characteristics[3] | |
Aphelion | 51.642 AU |
Perihelion | 36.361 AU |
44.002 AU | |
Eccentricity | 0.174 |
49.9° | |
Inclination | 24.2° |
301.8° | |
305.4° | |
Physical characteristics | |
Dimensions | 73 km[4][5] |
Albedo | 0.7 (assumed) |
Spectral type |
B-V=0.75, V-R=0.26[6] B-V=0.71; V-R=0.37[7] |
6.8[3] | |
|
(86047) 1999 OY3, also written as (86047) 1999 OY3, is a trans-Neptunian object that resides in the Kuiper belt beyond Pluto. It was discovered on July 18, 1999 at the Mauna Kea Observatory, Hawaii.
Haumea family
1999 OY3 is a candidate member of the Haumea family and probably has a very high albedo.[8]
Of the known Haumea-family members, 2009 OY3 has the dimmest absolute magnitude (H) of the group at 6.8, suggesting that it is also the smallest member of the group.
References
- ↑ "MPEC 2009-R09 :Distant Minor Planets (2009 SEPT. 16.0 TT)". IAU Minor Planet Center. 2009-09-04. Retrieved 2009-10-04.
- ↑ Marc W. Buie. "Orbit Fit and Astrometric record for 86047" (last observation: 2006-08-02 using 37 observations over 7.04 years). SwRI (Space Science Department). Retrieved 2009-10-04.
- ↑ 3.0 3.1 "JPL Small-Body Database Browser: 86047 (1999 OY3)" (last observation: 2006-08-02; arc: 7.04 years). Retrieved 2010-01-10.
- ↑ Assuming a Haumea-like albedo of 0.7
- ↑ Dan Bruton. "Conversion of Absolute Magnitude to Diameter for Minor Planets". Department of Physics & Astronomy (Stephen F. Austin State University). Archived from the original on 23 March 2010. Retrieved 2009-12-27.
- ↑ Snodgrass, Carry, Dumas, Hainaut (2009). "Characterisation of candidate members of (136108) Haumea's family". Astrophysical Journal. arXiv:0912.3171. Bibcode:2010A&A...511A..72S. doi:10.1051/0004-6361/200913031.
- ↑ Tegler, Stephen C. (2007-02-01). "Kuiper Belt Object Magnitudes and Surface Colors". Archived from the original on 1 September 2006. Retrieved 2006-11-07.
- ↑ D. Ragozzine; M. E. Brown (2007). "Candidate Members and Age Estimate of the Family of Kuiper Belt Object 2003 EL61". The Astronomical Journal 134 (6): 2160–2167. arXiv:0709.0328. Bibcode:2007AJ....134.2160R. doi:10.1086/522334.
External links
- Orbital simulation from JPL (Java) / Horizons Ephemeris
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