5642 Bobbywilliams

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5642 Bobbywilliams
Discovery 
Synodic rotation period
4.8341±0.0003 h[5]
0.20 (assumed)[4]
S[4]
14.0[1][4] · 14.24±0.23[6]

5642 Bobbywilliams, provisional designation 1990 OK1, is an eccentric, stony

Mars-crosser from the inner regions of the asteroid belt
, approximately 4.7 kilometers in diameter.

It was discovered on 27 July 1990, by American astronomer Henry E. Holt at Palomar Observatory in California, United States.[3] The asteroid was named for JPL engineer Bobby Williams.[2]

Orbit and classification

Bobbywilliams orbits the Sun in the inner main-belt at a distance of 1.5–3.1 AU once every 3 years and 6 months (1,287 days). Its orbit has an eccentricity of 0.33 and an inclination of 25° with respect to the ecliptic.[1] A first precovery was taken at the Australian Siding Spring Observatory in 1975, extending the body's observation arc by 15 years prior to its official discovery at Palomar.[3]

Physical characteristics

Rotation period

In July 2011, a rotational

U=3).[5]

Diameter and albedo

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 4.71 kilometers with an absolute magnitude of 14.0.[4]

Naming

This

M.P.C. 35483).[7]

References

  1. ^ a b c d e "JPL Small-Body Database Browser: 5642 Bobbywilliams (1990 OK1)" (2017-03-29 last obs.). Jet Propulsion Laboratory. Retrieved 21 June 2017.
  2. ^ .
  3. ^ a b c "5642 Bobbywilliams (1990 OK1)". Minor Planet Center. Retrieved 1 August 2016.
  4. ^ a b c d e f "LCDB Data for (5642) Bobbywilliams". Asteroid Lightcurve Database (LCDB). Retrieved 1 August 2016.
  5. ^
    ISSN 1052-8091
    . Retrieved 1 August 2016.
  6. . Retrieved 1 August 2016.
  7. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 1 August 2016.

External links