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13732 Woodall

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13732 Woodall
Discovery
Discovered byLINEAR
Discovery siteLincoln Lab ETS
Discovery date14 September 1998
Designations
MPC designation(13732) Woodall
Named afterAshley Renee Woodall (DCYSC)
Alternative designations1998 RC56 · 1989 EU5
1991 VS13 · 1997 LA16
Minor planet categorymain-belt · Vestian
Orbital characteristics
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.75 yr (10,135 days)
Aphelion2.6124 AU
Perihelion2.1366 AU
Semi-major axis2.3745 AU
Eccentricity0.1002
Orbital period (sidereal)3.66 yr (1,336 days)
Mean anomaly13.655°
Mean motion0° 16 9.84 / day
Inclination6.0477°
Longitude of ascending node204.72°
Argument of perihelion217.49°
Physical characteristics
Dimensions3.92 km (calculated)
Synodic rotation period8.2987±0.0005 h
Geometric albedo0.20 (assumed)
Spectral typeS
B–V = 0.864±0.147
V–R = 0.468±0.068
Absolute magnitude (H)14.4 · 15.23±0.10

13732 Woodall, provisional designation 1998 RC56, is a stony Vestian asteroid from the inner regions of the asteroid belt, approximately 4 kilometers in diameter. It was discovered on 14 September 1998, by the Lincoln Near-Earth Asteroid Research (LINEAR) team at Lincoln Laboratory's Experimental Test Site in Socorro, New Mexico.

Orbit and classification

Woodall is a member of the Vesta family, which is named after 4 Vesta, the second-largest asteroid in the main-belt. It orbits the Sun in the inner main-belt at a distance of 2.1–2.6 AU once every 3 years and 8 months (1,336 days). Its orbit has an eccentricity of 0.10 and an inclination of 6° with respect to the ecliptic. The first precovery was taken at Siding Spring Observatory in 1989, extending the asteroid's observation arc by 9 years prior to its official discovery observation.

Physical characteristics

Woodall has been characterized as a common S-type asteroid by Pan-STARRS photometric survey.

A rotational lightcurve was obtained based on photometric observations by Czech astronomer Petr Pravec at the Ondřejov Observatory in September 2009. Lightcurve analysis gave a well-defined rotation period of 8.2987 hours with a brightness amplitude of 0.27 in magnitude (U=3).

The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 3.9 kilometers with an absolute magnitude of 14.4.

Naming

This minor planet was named after Ashley Renee Woodall (born 1987) student at the U.S. Austin Academy for Excellence in Garland, Texas. In 2002, she was a finalist of the Discovery Channel Young Scientist Challenge (DCYSC), a science and engineering competition. The approved naming citation was published by the Minor Planet Center on 21 October 2002 (M.P.C. 46767).

References

  1. ^ "JPL Small-Body Database Browser: 13732 Woodall (1998 RC56)" (2016-11-30 last obs.). Jet Propulsion Laboratory. Retrieved 5 July 2017.
  2. ^ Schmadel, Lutz D. (2007). "(13732) Woodall". Dictionary of Minor Planet Names – (13732) Woodall. Springer Berlin Heidelberg. p. 803. doi:10.1007/978-3-540-29925-7_8874. ISBN 978-3-540-00238-3.
  3. ^ "LCDB Data for (13732) Woodall". Asteroid Lightcurve Database (LCDB). Retrieved 7 April 2016.
  4. ^ Pravec, P.; Vokrouhlický, D.; Polishook, D.; Scheeres, D. J.; Harris, A. W.; Galád, A.; et al. (August 2010). "Formation of asteroid pairs by rotational fission". Nature. 466 (7310): 1085–1088. arXiv:1009.2770. Bibcode:2010Natur.466.1085P. doi:10.1038/nature09315. PMID 20740010. S2CID 4418631.
  5. ^ Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results". Icarus. 261: 34–47. arXiv:1506.00762. Bibcode:2015Icar..261...34V. doi:10.1016/j.icarus.2015.08.007. S2CID 53493339.
  6. ^ Ye, Q.-z. (February 2011). "BVRI Photometry of 53 Unusual Asteroids". The Astronomical Journal. 141 (2): 8. arXiv:1011.0133. Bibcode:2011AJ....141...32Y. doi:10.1088/0004-6256/141/2/32. S2CID 119307210.
  7. ^ "13732 Woodall (1998 RC56)". Minor Planet Center. Retrieved 7 April 2016.
  8. "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 19 May 2016.

External links

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