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3277 Aaronson

From Wikipedia, the free encyclopedia
Main-belt asteroid

3277 Aaronson
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date8 January 1984
Designations
(3277) Aaronson
Named after
Marc Aaronson
(astronomer)[2]
1984 AF1 · 1962 CF
1971 UV2 · 1982 TU2
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc55.24 yr (20,178 days)
Aphelion3.9927AU
Perihelion2.2900 AU
3.1414 AU
Eccentricity0.2710
5.57yr (2,034 days)
93.558°
0° 10m 37.2s / day
Inclination8.5693°
84.997°
295.32°
Physical characteristics
Dimensions19.88±0.15 km[4]
20.049±0.054 km[5]
26.64 km(calculated)[3]
9.80±0.05h[6]
0.057(assumed)[3]
0.112±0.016[4]
0.1211±0.0122[5]
C[3]
11.4[5] · 11.5[4] · 11.6[1][3] · 11.89±0.21[7]

3277 Aaronson, provisional designation1984 AF1, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 20 kilometers in diameter. It was discovered by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station, near Flagstaff, Arizona, on 8 January 1984, and named in memory of astronomerMarc Aaronson.[8]

Orbit and classification

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TheC-type asteroid orbits the Sun in theouter main-belt at a distance of 2.3–4.0 AU once every 5 years and 7 months (2,034 days). Its orbit has aneccentricity of 0.27 and aninclination of 9° with respect to theecliptic.[1] A firstprecovery was obtained atGoethe Link Observatory in 1962, extending the asteroid'sobservation arc by 22 years prior to its official discovery observation at Anderson Mesa.[8]

Physical characteristics

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Rotation period

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In November 2010, a rotationallightcurve for this asteroid was obtained from photometric observations made at the U.S. Shadowbox Observatory in Carmel, Indiana. It rendered arotation period of9.80±0.05 hours with a brightness amplitude of 0.14 inmagnitude (U=2+).[6]

Diameter and albedo

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Based on NASA's space-basedWISE and its subsequentNEOWISE mission, the asteroid has analbedo of 0.11 and 0.12, and a diameter of 19.9 and 20.0 kilometers, respectively,[4][5] while theCollaborative Asteroid Lightcurve Link (CALL) assumes a lower albedo of 0.06, which translates into a larger diameter of 26.6 kilometers, as the lower the albedo (reflectivity), the higher the body's diameter, for a given absolute magnitude (brightness).[3]

Naming

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Thisminor planet was named in memory of American astronomerMarc Aaronson (1950–1987), killed in the dome of the 4-meterNicholas U. Mayall Telescope of theKitt Peak National Observatory. His fields of research included the detection the decelerative effect of the Virgo cluster on theHubble flow, observations of carbon stars in the globular clusters in the Magellanic clouds, and measurement of the large velocity dispersion indwarf spheroidal galaxies, suggesting that all galaxies do havedark matter halos.[2] The official naming citation was published by theMinor Planet Center on 11 July 1987(M.P.C. 12016).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 3277 Aaronson (1984 AF1)" (2017-05-04 last obs.).Jet Propulsion Laboratory. Retrieved17 June 2017.
  2. ^abSchmadel, Lutz D. (2007). "(3277) Aaronson".Dictionary of Minor Planet Names – (3277) Aaronson.Springer Berlin Heidelberg. p. 273.doi:10.1007/978-3-540-29925-7_3278.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (3277) Aaronson". Asteroid Lightcurve Database (LCDB). Retrieved26 April 2016.
  4. ^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. Retrieved14 January 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. Retrieved14 January 2016.
  6. ^abRuthroff, John C. (April 2011)."Lightcurve Analysis of Eight Main-belt Asteroids and a Revised Period for 185 Eunike".The Minor Planet Bulletin.38 (2):86–88.Bibcode:2011MPBu...38...86R.ISSN 1052-8091. Retrieved14 January 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. Retrieved26 April 2016.
  8. ^ab"3277 Aaronson (1984 AF1)".Minor Planet Center. Retrieved26 April 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved26 April 2016.

External links

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