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4149 Harrison

From Wikipedia, the free encyclopedia
Main-belt asteroid
4149 Harrison
Discovery[1]
Discovered byB. A. Skiff
Discovery siteAnderson Mesa Stn.
Discovery date9 March 1984
Designations
(4149) Harrison
Named after
George Harrison
(guitarist,The Beatles)[2]
1984 EZ
main-belt · Eunomia[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc39.32 yr (14,360 days)
Aphelion2.9955AU
Perihelion2.3356 AU
2.6655 AU
Eccentricity0.1238
4.35yr (1,590 days)
204.95°
0° 13m 35.4s / day
Inclination12.923°
154.73°
76.653°
Physical characteristics
Dimensions8.14 km(derived)[3]
10.130±0.081[4]
10.739±0.042 km[5]
3.7490±0.0002h[a]
3.956±0.001 h[6]
0.1856±0.0479[5]
0.21(assumed)[3]
0.230±0.035[4]
S[3]
12.3[1][5] · 12.31±0.16(R)[a] · 12.54±0.22[7] · 12.76[3]

4149 Harrison, provisional designation1984 EZ, is a stony Eunomianasteroid from the middle region of theasteroid belt, approximately 10 kilometers in diameter. The asteroid was discovered on 9 March 1984, by American astronomerBrian Skiff at Lowell'sAnderson Mesa Station in Flagstaff, Arizona, and named after musicianGeorge Harrison.[8]

Orbit and classification

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Harrison is a member of theEunomia family, a large group ofS-type asteroids and the most prominent family in the intermediate main-belt. It orbits the Sun in thecentral main-belt at a distance of 2.3–3.0 AU once every 4 years and 4 months (1,590 days). Its orbit has aneccentricity of 0.12 and aninclination of 13° with respect to theecliptic.[1] A firstprecovery was taken atPalomar Observatory in 1977, extending the body'sobservation arc by 7 years prior to its discovery.[8]

Physical characteristics

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Rotation period

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A rotationallightcurve ofHarrison was obtained from photometric observations by Czech astronomerPetr Pravec atOndřejov Observatory in May 2015. It gave a well-definedrotation period of3.7490±0.0002 hours with a brightness variation of 0.42 inmagnitude (U=3).[a] During the following month, photometric observations at three Italian observatories gave a second lightcurve with a period of3.956±0.001 hours and an amplitude of 0.37 in magnitude (U=2+).[6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Harrison measures 10.1 and 10.7 kilometers in diameter and its surface has analbedo of 0.19 and 0.23, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.21 – derived from15 Eunomia, the family's largest member and namesake – and calculates a diameter of 8.1 kilometers with anabsolute magnitude of 12.76.[3]

Naming

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Thisminor planet was named in honor of guitarist, singer and songwriter,George Harrison (1943–2001), who was the lead guitarist of the English rock bandThe Beatles, after which the main-belt asteroid8749 Beatles is named.[2] The minor planets4147 Lennon,4148 McCartney and4150 Starr honor the other three members of the band. The official naming citation was published by theMinor Planet Center on 10 April 1990 (M.P.C. 16248).[9]

Notes

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  1. ^abcPravec (2015) web:lightcurve plot of (4149) Harrison with a rotation period3.7490±0.0002 hours with a brightness amplitude of0.42 mag. G:0.15±0.2, abs. magnitude:12.31±0.16, phase: 11.1, PABL: 256.2, and PABB: 17.3. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) andPravec, P.; Wolf, M.; Sarounova, L. (2015)

References

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  1. ^abcd"JPL Small-Body Database Browser: 4149 Harrison (1984 EZ)" (2017-02-04 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(4149) Harrison".Dictionary of Minor Planet Names – (4149) Harrison.Springer Berlin Heidelberg. p. 355.doi:10.1007/978-3-540-29925-7_4121.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4149) Harrison". Asteroid Lightcurve Database (LCDB). Retrieved10 August 2016.
  4. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.S2CID 119293330. Retrieved5 December 2016.
  5. ^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.S2CID 35447010.
  6. ^abPapini, Riccardo; Franco, Lorenzo; Marchini, Alessandro; Salvaggio, Fabio (October 2015)."Rotation Period Determination for 4149 Harrison and (5633) 1978 UL7".The Minor Planet Bulletin.42 (4):281–283.Bibcode:2015MPBu...42..281P.ISSN 1052-8091. Retrieved10 August 2016.
  7. ^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. Retrieved10 August 2016.
  8. ^ab"4149 Harrison (1984 EZ)".Minor Planet Center. Retrieved10 August 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 August 2016.

External links

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