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13732 Woodall

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13732 Woodall
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab ETS
Discovery date14 September 1998
Designations
(13732) Woodall
Named after
Ashley Renee Woodall(DCYSC)[2]
1998 RC56 · 1989 EU5
1991 VS13 · 1997 LA16
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.75 yr (10,135 days)
Aphelion2.6124AU
Perihelion2.1366 AU
2.3745 AU
Eccentricity0.1002
3.66yr (1,336 days)
13.655°
0° 16m 9.84s / day
Inclination6.0477°
204.72°
217.49°
Physical characteristics
Dimensions3.92 km(calculated)[3]
8.2987±0.0005h[4]
0.20(assumed)[3]
S[3][5]
B–V =0.864±0.147[6]
V–R =0.468±0.068[6]
14.4[1][3] · 15.23±0.10[5]

13732 Woodall, provisional designation1998 RC56, is a stony Vestianasteroid from the inner regions of theasteroid belt, approximately 4 kilometers in diameter. It was discovered on 14 September 1998, by theLincoln Near-Earth Asteroid Research (LINEAR) team atLincoln Laboratory's Experimental Test Site in Socorro, New Mexico.[7]

Orbit and classification

[edit]

Woodall is a member of theVesta family, which is named after4 Vesta, the second-largest asteroid in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.1–2.6 AU once every 3 years and 8 months (1,336 days). Its orbit has aneccentricity of 0.10 and aninclination of 6° with respect to theecliptic.[1] The firstprecovery was taken atSiding Spring Observatory in 1989, extending the asteroid'sobservation arc by 9 years prior to its official discovery observation.[7]

Physical characteristics

[edit]

Woodall has been characterized as a commonS-type asteroid byPan-STARRS photometric survey.[5]

A rotationallightcurve was obtained based onphotometric observations by Czech astronomerPetr Pravec at theOndřejov Observatory in September 2009. Lightcurve analysis gave a well-definedrotation period of8.2987 hours with a brightness amplitude of0.27 inmagnitude (U=3).[4]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forstony asteroids of 0.20 and calculates a diameter of 3.9 kilometers with anabsolute magnitude of 14.4.[3]

Naming

[edit]

Thisminor 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 theDiscovery Channel Young Scientist Challenge (DCYSC), a science and engineering competition.[2] The approved naming citation was published by theMinor Planet Center on 21 October 2002 (M.P.C. 46767).[8]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 13732 Woodall (1998 RC56)" (2016-11-30 last obs.).Jet Propulsion Laboratory. Retrieved5 July 2017.
  2. ^abSchmadel, 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. ^abcdef"LCDB Data for (13732) Woodall". Asteroid Lightcurve Database (LCDB). Retrieved7 April 2016.
  4. ^abPravec, 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. ^abcVeres, 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. ^abYe, 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. ^ab"13732 Woodall (1998 RC56)".Minor Planet Center. Retrieved7 April 2016.
  8. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved19 May 2016.

External links

[edit]
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Authority control databasesEdit this at Wikidata
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