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(202421) 2005 UQ513

Classical Kuiper belt object


Classical Kuiper belt object

FieldValue
minorplanetyes
background#C2E0FF
name
discovery_ref
discovererM. E. Brown
D. L. Rabinowitz
C. A. Trujillo
discovered21 October 2005
mpc_name
mp_categoryclassical (MPC)
ScatExt (DES)
orbit_ref
epoch13 January 2016 (JD 2457400.5)
aphelion49.689 AU (Q)
perihelion36.713 AU (q)
time_periastron≈ 30 July 2123
±3 days
semimajor43.201 AU (a)
eccentricity0.15018 (e)
period283.95 yr (103713 d)
inclination25.7315° (i)
asc_node307.8679° (Ω)
mean_anomaly223.93° (M)
arg_peri221.89° (ω)
satellites0
dimensions
sidereal_day7.03 hr?
albedo
magnitude20.8
abs_magnitude3.91
mean_motion/ day (n)
rotation7.03 h
observation_arc8474 days (23.20 yr)
earliest_precovery_date15 September 1990
uncertainty3
moid35.763 AU
jupiter_moid31.568 AU
tisserand5.253

D. L. Rabinowitz C. A. Trujillo ScatExt (DES) ±3 days

**** (provisional designation ****) is a classical Kuiper belt object with an absolute magnitude of 3.91, and estimated to be around in diameter. Like Quaoar, it has a very red spectrum, which indicates that its surface probably contains many complex, processed organic molecules. Its light curve shows variations of Δm=0.3 mag, but no period has been determined.

Classification

has a perihelion of 37.3 AU. The Minor Planet Center (MPC) classifies it as a classical Kuiper belt object (cubewano) while the Deep Ecliptic Survey (DES) classifies it as ScatExt (scattered-extended). Although dynamically it would have been a good candidate to be a member of the Haumea collisional family, given its red spectrum, it is probably not.

Distance

As of December 2018, it is currently 48.0 AU from the Sun. It will come to perihelion in 2123.

It has been observed 194 times over 14 oppositions with precovery images back to 1990.

References

References

  1. [http://ssd.jpl.nasa.gov/horizons.cgi?find_body=1&body_group=sb&sstr=2005UQ513 JPL Horizons] Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is [[3-sigma]].)
  2. 1102.1971
  3. Ragozzine, D.. (2007). "Candidate Members and Age Estimate of the Family of Kuiper Belt Object {{mp". The Astronomical Journal.
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