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4147 Lennon

From Wikipedia, the free encyclopedia
Asteroid

4147 Lennon
Discovery[1]
Discovered byB. A. Skiff
Discovery siteAnderson Mesa Stn.
Discovery date12 January 1983
Designations
(4147) Lennon
Named after
John Lennon
(musician,The Beatles)[2]
1983 AY · 1971 YG
1980 KA
main-belt · Vestian[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc44.51 yr (16,258 days)
Aphelion2.5524AU
Perihelion2.1712 AU
2.3618 AU
Eccentricity0.0807
3.63yr (1,326 days)
88.732°
0° 16m 17.4s / day
Inclination5.7326°
288.57°
302.94°
Physical characteristics
Dimensions5.171±0.087 km[4][5]
7.13±0.37 km[6]
7.46 km(calculated)[3]
137h[7]
0.20(assumed)[3]
0.240±0.049[6]
0.4166±0.0564[4]
V[7]: 5  · S[3]
12.90[6] · 13.0[1][3][4] · 13.63±0.34[8]

4147 Lennon, provisional designation1983 AY, is a stony Vestianasteroid and a potentiallyslow rotator from the inner regions of theasteroid belt, approximately 7 kilometers in diameter. It was discovered by American astronomerBrian Skiff at Lowell'sAnderson Mesa Station on 12 January 1983.[9] It was later named after musicianJohn Lennon.[2]

Orbit and classification

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Lennon is a member of theVesta family, which is named after the main-belt's second largest asteroid,4 Vesta. It orbits the Sun in theinner main-belt at a distance of 2.2–2.6 AU once every 3 years and 8 months (1,326 days). Its orbit has aneccentricity of 0.08 and aninclination of 6° with respect to theecliptic.[1] The first observation was made atCrimea–Nauchnij in 1971, extending the asteroid'sobservation arc by 12 years prior to its discovery.[9]

Physical characteristics

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Lennon has been characterized as aV-type asteroid.[7]: 5 

Slow rotator

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In October 2004, a rotationallightcurve ofLennon was obtained during a photometricsurvey of V-type asteroids at several observatories in Japan. The fragmentary lightcurve gave a very longrotation period of 137 hours with a high brightness variation of 0.6 inmagnitude (U=1).[7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Lennon measures 5.2 and 7.1 kilometers in diameter and its surface has analbedo of 0.24 of 0.42, respectively.[4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forS-type asteroids of 0.20 and calculates a diameter of 7.5 kilometers with anabsolute magnitude of 13.0.[3] The discrepancy is due to disagreement on the body'sspectral type (V or S).

Naming

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Thisminor planet was named in memory of English musicianJohn Lennon (1940–1980), famous for his song "Imagine" and co-founder ofThe Beatles, one of the most successful bands in the history of popular music.[2]

The minor planets8749 Beatles,4149 Harrison,4148 McCartney and4150 Starr, were named after the band and its three other members. The official naming citation was published by theMinor Planet Center on 10 April 1990 (M.P.C. 16247).[10]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 4147 Lennon (1983 AY)" (2016-06-20 last obs.).Jet Propulsion Laboratory. Retrieved20 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(4147) Lennon".Dictionary of Minor Planet Names – (4147) Lennon.Springer Berlin Heidelberg. p. 354.doi:10.1007/978-3-540-29925-7_4119.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (4147) Lennon". Asteroid Lightcurve Database (LCDB). Retrieved10 August 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. ^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. Retrieved5 December 2016.
  6. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved10 August 2016.
  7. ^abcdHasegawa, S.; Miyasaka, S.; Mito, H.; Sarugaku, Y.; Ozawa, T.; Kuroda, D.; et al. (May 2012). "Lightcurve Survey of V-Type Asteroids. Observations Until 2005".Asteroids.1667: 6281.arXiv:1204.0548.Bibcode:2012LPICo1667.6281H.
  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. Retrieved10 August 2016.
  9. ^ab"4147 Lennon (1983 AY)".Minor Planet Center. Retrieved10 August 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 August 2016.

External links

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