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5677 Aberdonia

From Wikipedia, the free encyclopedia
Main-belt asteroid

5677 Aberdonia
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.[2]
Discovery date21 September 1987
Designations
(5677) Aberdonia
Named after
University of Aberdeen
(Scottish university)[3]
1987 SQ1 · 1973 UL1
1978 WN16 · 1989 AK8
main-belt · Koronis[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.27 yr (22,744 days)
Aphelion3.0052AU
Perihelion2.6635 AU
2.8344 AU
Eccentricity0.0603
4.77yr (1,743 days)
49.056°
0° 12m 23.4s / day
Inclination1.5003°
201.12°
216.63°
Physical characteristics
Dimensions8.19 km(calculated)[4]
8.798±0.114 km[5][6]
5.0813±0.0410h[7]
0.24(assumed)[4]
0.250±0.022[5]
S[4]
12.6[1][4] · 12.4[5] · 13.224±0.003(S)[7] · 12.70±0.32[8]

5677 Aberdonia, provisional designation1987 SQ1, is a stony Koronisasteroid from the outer region of theasteroid belt, approximately 8 kilometers in diameter. It was discovered on 21 September 1987, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station in Flagstaff, Arizona, United States.[2] The asteroid was named for the ScottishUniversity of Aberdeen.[3]

Orbit and classification

[edit]

TheS-type asteroid is a member of theKoronis family, a group consisting of about 200 known bodies with nearlyecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.7–3.0 AU once every 4 years and 9 months (1,743 days). Its orbit has aneccentricity of 0.06 and aninclination of 2° with respect to the ecliptic.[1]

In 1954, a firstprecovery was obtained atPalomar Observatory, extending the body'sobservation arc by 33 years prior to its official discovery at Anderson Mesa.[2]

Physical characteristics

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Lightcurves

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In October 2011, a rotationallightcurve ofAberdonia was obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of5.0813 hours with a brightness amplitude of 0.20magnitude (U=2).[7]

Diameter and albedo

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According to theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Aberdonia measures 8.8 kilometers in diameter and its surface has analbedo of 0.25,[5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 and calculates a diameter of 8.2 kilometers with anabsolute magnitude of 12.6.[4]

Naming

[edit]

Thisminor planet was named for the ScottishUniversity of Aberdeen on its 500th anniversary in 1995.James Clerk Maxwell andGeorge Paget Thomson are the university's best known former holders of chairs of natural philosophy.[3]

The university is also known for its first chair of medicine in the English-speaking world, and for having taught astronomy already in the late 16th century.[3] The approved naming citation was published by theMinor Planet Center on 15 February 1995(M.P.C. 24765).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 5677 Aberdonia (1987 SQ1)" (2017-03-29 last obs.).Jet Propulsion Laboratory. Retrieved21 June 2017.
  2. ^abc"5677 Aberdonia (1987 SQ1)".Minor Planet Center. Retrieved26 April 2016.
  3. ^abcdSchmadel, Lutz D. (2007). "(5677) Aberdonia".Dictionary of Minor Planet Names – (5677) Aberdonia.Springer Berlin Heidelberg. p. 481.doi:10.1007/978-3-540-29925-7_5373.ISBN 978-3-540-00238-3.
  4. ^abcdef"LCDB Data for (5677) Aberdonia". Asteroid Lightcurve Database (LCDB). Retrieved26 April 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. Retrieved26 April 2016.
  6. ^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.
  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. Retrieved26 April 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. Retrieved26 April 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 April 2016.

External links

[edit]
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