5175 Ables

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5175 Ables
Discovery 
Synodic rotation period
2.7976±0.0005 h[6]
2.798±0.001 h[7]
0.2897±0.0604[5]
0.30 (assumed)[3]
0.505±0.074[4]
E[3]
13.3[1][3] · 13.2[5][4] · 13.83±0.37[8]

5175 Ables, provisional designation 1988 VS4, is a bright Hungaria

Eugene Shoemaker at the U.S. Palomar Observatory, California, on 4 November 1988.[9] It was named after American astronomer Harold Ables.[2]

Orbit and classification

Ables is a member of the

Hungaria family, which form the innermost dense concentration of asteroids in the Solar System
.

It orbits the Sun at a distance of 1.9–2.0 AU once every 2 years and 9 months (1,008 days). Its orbit has an eccentricity of 0.04 and an inclination of 17° with respect to the ecliptic.[1] A first precovery was obtained at Palomar Observatory in 1954, extending the asteroid's observation arc by 34 years prior to its official discovery observation.[9]

Physical characteristics

Ables has been characterized as a bright E-type asteroid.[3]

Diameter and albedo

Based on the surveys carried out by the NASA's space-based

albedo of 0.29 and 0.51, with a corresponding diameter of 5.7 and 4.3 kilometers, respectively,[5][4] while the Collaborative Asteroid Lightcurve Link assumes an albedo of 0.30 and calculates a diameter of 5.3 kilometers with an absolute magnitude of 13.3.[3]

Lightcurves

Between 2010 and 2014, three rotational

Naming

This

M.P.C. 27459).[11]

References

  1. ^ a b c d "JPL Small-Body Database Browser: 5175 Ables (1988 VS4)" (2017-05-05 last obs.). Jet Propulsion Laboratory. Retrieved 20 June 2017.
  2. ^ .
  3. ^ a b c d e f g "LCDB Data for (5175) Ables". Asteroid Lightcurve Database (LCDB). Retrieved 27 April 2016.
  4. ^ . Retrieved 13 January 2016.
  5. ^ . Retrieved 27 April 2016.
  6. ^ . Retrieved 13 January 2016.
  7. ^ . Retrieved 13 January 2016.
  8. . Retrieved 27 April 2016.
  9. ^ a b "5175 Ables (1988 VS4)". Minor Planet Center. Retrieved 27 April 2016.
  10. ISSN 1052-8091
    . Retrieved 13 January 2016.
  11. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 27 April 2016.

External links