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2985 Shakespeare

From Wikipedia, the free encyclopedia

2985 Shakespeare
Shakespeare modeled from itslightcurve
Discovery [1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date12 October 1983
Designations
(2985) Shakespeare
Named after
William Shakespeare
(poet & playwright)[2]
1983 TV1 · 1962 JJ
1976 GV · 1978 RY4
1978 TM3 · 1980 BT3
main-belt · Koronis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc54.68 yr (19,971 days)
Aphelion2.9783AU
Perihelion2.7184 AU
2.8483 AU
Eccentricity0.0456
4.81yr (1,756 days)
87.549°
0° 12m 18s / day
Inclination2.6496°
34.228°
277.66°
Physical characteristics
10.31 km(calculated)[3]
10.472±0.101 km[4][5]
6.0567±0.0020 h[6]
6.06±0.02 h[7]
6.080±0.040 h[8]
0.24(assumed)[3]
0.255±0.034[4][5]
S[3]
11.918±0.003(R)[6] · 11.930±0.240(R)[8] · 12.0[4] · 12.1[1][3]

2985 Shakespeare (prov. designation:1983 TV1) is a stony Koronianasteroid from the outer region of theasteroid belt. It was discovered on 12 October 1983, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station near Flagstaff, Arizona, and later named afterWilliam Shakespeare.[2][9] The presumedS-type asteroid has arotation period of 6.1 hours and measures approximately 10 kilometers (6.2 miles) in diameter.

Classification and orbit

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TheS-type asteroid is a member of theKoronis family, a group consisting of about 200 known bodies. It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 10 months (1,756 days). Its orbit has aneccentricity of 0.05 and aninclination of 3° with respect to theecliptic.[1] It was first identified as1962 JJ atGoethe Link Observatory in 1962. The body'sobservation arc begins with its identification1976 GV atCrimea–Nauchnij, 7 years prior to its official discovery observation at Anderson Mesa.[9]

Naming

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Thisminor planet was named afterWilliam Shakespeare (1564–1616), the English renaissance dramatist and poet.[2] The approved naming citation was published by theMinor Planet Center on 29 September 1985 (M.P.C. 10044).[10]

Physical characteristics

[edit]

Rotation period and poles

[edit]

Three different rotationallightcurves, obtained fromphotometric observations taken at thePalomar Transient Factory and a group of seven observatories, respectively, found a concurringrotation period of 6.06–6.08 hours with a brightness variation between 0.37 and 0.53magnitude (U=2/3/2).[6][7][8]

Diameter and albedo

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According to the space-basedNEOWISE mission of NASA'sWide-field Infrared Survey Explorer, the body has analbedo of 0.26 and measures 10.5 kilometers in diameter,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for members of the Koronis family of 0.24 and calculates a diameter of 10.3 kilometers with anabsolute magnitude of 12.1.[3]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2985 Shakespeare (1983 TV1)" (2017-01-07 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2985) Shakespeare".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 246.doi:10.1007/978-3-540-29925-7_2986.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2985) Shakespeare". Asteroid Lightcurve Database (LCDB). Retrieved6 December 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.
  5. ^abcMasiero, 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. Retrieved6 December 2016.
  6. ^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. Retrieved6 December 2016.
  7. ^abSlivan, Stephen M.; Binzel, Richard P.; Boroumand, Shaida C.; Pan, Margaret W.; Simpson, Christine M.; Tanabe, James T.; et al. (May 2008)."Rotation rates in the Koronis family, complete to H≈11.2".Icarus.195 (1):226–276.Bibcode:2008Icar..195..226S.doi:10.1016/j.icarus.2007.11.019. Retrieved6 December 2016.
  8. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27. Retrieved6 December 2016.
  9. ^ab"2985 Shakespeare (1983 TV1)".Minor Planet Center. Retrieved6 December 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 December 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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