(202421) 2005 UQ513

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(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

oppositions with precovery images back to 1990.[3]

See also

References

  1. ^ Lowe, Andrew. "(202421) 2005 UQ513 Precovery Images". andrew-lowe.ca.
  2. .
  3. ^ 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.
  4. ^ a b "MPEC 2010-S44 : DISTANT MINOR PLANETS (2010 OCT. 11.0 TT)". IAU Minor Planet Center. 2010-09-25. Retrieved 2011-01-26.
  5. ^ (2012/05/06 using 59 observations). SwRI (Space Science Department). Retrieved 2012-05-05.
  6. ^ "AstDyS (202421) 2005UQ513 Orbital information". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
  7. ^
    3-sigma
    .)
  8. ^
    arXiv:1403.6309
  9. ^ a b "AstDyS (202421) 2005UQ513 Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 2012-05-05.
  10. S2CID 8387493
    . Retrieved 2009-12-05.
  11. ^
  12. ^

External links