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32226 Vikulgupta

From Wikipedia, the free encyclopedia
Stony Flora asteroid from the inner regions of the asteroid belt

32226 Vikulgupta
Yellow-Blue orbit is of 32226 Vikulgupta.
Discovery[1]
Discovered byLINEAR
Discovery siteLincoln Lab's ETS
Discovery date23 July 2000
Designations
(32226) Vikulgupta
Named after
Vikul Gupta
(2016Intel STS awardee)[2]
2000 OQ23 · 1999 CY85
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc19.56 yr (7,143 days)
Aphelion2.5878AU
Perihelion2.0633 AU
2.3256 AU
Eccentricity0.1128
3.55yr (1,295 days)
322.00°
0° 16m 40.44s / day
Inclination4.2004°
302.69°
320.95°
Physical characteristics
Dimensions3.11 km(calculated)[3]
3.776±0.134 km[4][5]
2.57±0.05h[6]
2.5724±0.0006 h[7]
0.215±0.036[5]
0.2153±0.0356[4]
0.24(assumed)[3]
S[3]
14.4[4] · 14.55±0.16(R)[6] · 14.613±0.005(R)[7] · 14.7[1][3] · 15.33±0.43[8]

32226 Vikulgupta (provisional designation2000 OQ23) is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 3.5 kilometers in diameter.

The asteroid was discovered on 23 July 2000, by theLINEAR team atLincoln Laboratory's Experimental Test Site near Socorro, New Mexico, in the United States. It was named for Vikul Gupta, a 2016Intel STS awardee.[2]

Orbit and classification

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Vikulgupta is a member of theFlora family, one of the largest groups ofstony asteroids 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 7 months (1,295 days). Its orbit has aneccentricity of 0.11 and aninclination of 4° with respect to theecliptic.[1]

A firstprecovery was taken atWhipple Observatory in 1997, extending the asteroid'sobservation arc by 3 years prior to its official discovery observation at Socorro.[2]

Physical characteristics

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Rotation period

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In February 2013, two rotationallightcurves of Vikulgupta were obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of2.57 and2.5724 hours with a brightness variation of 0.35 and 0.34magnitude, respectively (U=2/2).[6][7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer, Vikulgupta measures 3.8 kilometers in diameter and its surface has analbedo of 0.215,[4] while theCollaborative Asteroid Lightcurve Link assumes analbedo of 0.24 – derived from8 Flora, the largest member and namesake of its orbital family – and calculates a diameter of 3.1 kilometers with anabsolute magnitude of 14.7.[3]

Naming

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Thisminor planet was named after Vikul Gupta (born 1998), a science competition finalist in the 2016Intel Science Talent Search, who was awarded for his computer science project. At the time, he attended the U.S.Oregon Episcopal School in Portland.[2] The approved naming citation was published by theMinor Planet Center on 21 May 2016 (M.P.C. 100315).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 32226 Vikulgupta (2000 OQ23)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved27 June 2017.
  2. ^abcd"32226 Vikulgupta (2000 OQ23)".Minor Planet Center. Retrieved24 May 2016.
  3. ^abcdef"LCDB Data for (32226) Vikulgupta". Asteroid Lightcurve Database (LCDB). Retrieved24 May 2016.
  4. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011)."NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results".The Astrophysical Journal.741 (2): 25.arXiv:1109.6407.Bibcode:2011ApJ...741...90M.doi:10.1088/0004-637X/741/2/90. Retrieved24 May 2016.
  5. ^abMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68. Retrieved2 December 2016.
  6. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (June 2014)."313 New Asteroid Rotation Periods from Palomar Transient Factory Observations".The Astrophysical Journal.788 (1): 21.arXiv:1405.1144.Bibcode:2014ApJ...788...17C.doi:10.1088/0004-637X/788/1/17. Retrieved24 May 2016.
  7. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75. Retrieved24 May 2016.
  8. ^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. Retrieved24 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 May 2016.

External links

[edit]
Minor planets
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Authority control databasesEdit this at Wikidata
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