(374158) 2004 UL

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(374158) 2004 UL
Discovery
Synodic rotation period
38±h[5][a]
0.20 (assumed)[4]

(374158) 2004 UL is a sub-kilometer

perihelion of any known asteroid, after (137924) 2000 BD19.[citation needed
]

It was discovered on 18 October 2004 by the

Lincoln Lab's ETS near Socorro, New Mexico.[2]

Orbit and classification

This Apollo asteroid orbits the Sun at a distance of 0.09–2.44 

semi-major axis of 1.27 AU). Its orbit has an outstandingly high eccentricity of 0.93 and an inclination of 24° with respect to the ecliptic.[1]

Due to its orbit, it is also a

Physical characteristics

2004 UL is an assumed stony S-type asteroid.[4]

In October 2014, a rotational

U=2).[5]

Based on a generic magnitude-to-diameter conversion, 2004 UL measures between 0.5 and 1.2 kilometers.[3] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 0.516 kilometers with an absolute magnitude of 18.8.[4]

Numbering and naming

This

M.P.C. 85347).[6] As of 2018, it has not been named.[2]

Notes

  1. ^ a b Lightcurve plot for (374158) by B. D. Warner at the CS3-Palmer Divide Station from October/November 2014
  2. ^ a b c Jewitt (2013). Abs. magnitude of 18.77 (R). Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (374158)

References

  1. ^ a b c d e f "JPL Small-Body Database Browser: 374158 (2004 UL)" (2016-10-07 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2017.
  2. ^ a b c d "374158 (2004 UL)". Minor Planet Center. Retrieved 18 August 2016.
  3. ^ a b "NEODyS (374158) 2004UL". Near Earth Objects – Dynamic Site. Retrieved 7 March 2014.
  4. ^ a b c d e f "LCDB Data for (374158)". Asteroid Lightcurve Database (LCDB). Retrieved 18 August 2016.
  5. ^
    ISSN 1052-8091
    . Retrieved 18 August 2016.
  6. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 26 February 2018.

External links