(202421) 2005 UQ513
Sidereal rotation period | 7.03 hr?[3] | |
0.31+0.12 −0.065[8] | ||
20.8 [9] | ||
3.97 [3] | ||
(202421) 2005 UQ513 (
provisional designation 2005 UQ513) is a cubewano with an absolute magnitude of 3.97.[3] Its spectrum has a weak signature of absorption by water ice.[10][11] Like Quaoar, it has a very red spectrum,[12][13] which indicates that its surface probably contains many complex, processed organic molecules.[12] Its light curve shows variations of Δm=0.3 mag, but no period has been determined.[13]
Classification
2005 UQ513 has a perihelion of 37.3 AU.[3] The Minor Planet Center (MPC) classifies it as a cubewano[4] while the Deep Ecliptic Survey (DES) classifies it as ScatExt (scattered-extended).[5] Although dynamically it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum, it is not.[12][13]
Distance
As of December 2018, it is currently 48.0 AU from the Sun.[9] It will come to perihelion in 2123.[7]
It has been observed 194 times over 14
See also
References
- ^ Lowe, Andrew. "(202421) 2005 UQ513 Precovery Images". andrew-lowe.ca.
- Bibcode:2007MPEC....R...02B.
- ^ a b c d e f g "JPL Small-Body Database Browser: (2005 UQ513)" (2011-12-26 last obs., 12 opp). Retrieved 7 April 2016.
- ^ a b "MPEC 2010-S44 : DISTANT MINOR PLANETS (2010 OCT. 11.0 TT)". IAU Minor Planet Center. 2010-09-25. Retrieved 2011-01-26.
- ^ Marc W. Buie. "Orbit Fit and Astrometric record for 202421"(2012/05/06 using 59 observations). SwRI (Space Science Department). Retrieved 2012-05-05.
- ^ "AstDyS (202421) 2005UQ513 Orbital information". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
- ^ 3-sigma.)
- ^ arXiv:1403.6309
- ^ a b "AstDyS (202421) 2005UQ513 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
- S2CID 8387493. Retrieved 2009-12-05.
- arXiv:1102.1971
- ^ arXiv:0807.2670
- ^ arXiv:0912.3171
External links