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2939 Coconino

From Wikipedia, the free encyclopedia
Stony Nysian asteroid from the inner regions of the asteroid belt
2939 Coconino
Discovery[1]
Discovered byE. Bowell
Discovery siteAnderson Mesa Stn.
Discovery date21 February 1982
Designations
(2939) Coconino
Named after
Coconino County
(U.S. county in Arizona)[2]
1982 DP · 1952 HU3
1976 ST4
main-belt · Nysa[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc40.69 yr (14,861 days)
Aphelion2.8399AU
Perihelion2.0394 AU
2.4396 AU
Eccentricity0.1641
3.81yr (1,392 days)
47.539°
Inclination3.9489°
349.97°
237.31°
Physical characteristics
Dimensions5.607±0.177 km[4][5]
9.40 km(calculated)[3]
4.68138±0.00004h[6]
0.20(assumed)[3]
0.512±0.043[4][5]
S[3]
12.5[1][3] · 12.6[4] · 12.92±0.10[7]

2939 Coconino, provisional designation1982 DP, is a stony Nysianasteroid from the inner regions of theasteroid belt, approximately 6 kilometers in diameter. It was discovered on 21 February 1982, by American astronomerEdward Bowell at Lowell'sAnderson Mesa Station in Flagstaff, United States.[8] It is named after theCoconino County in Arizona.[2]

Orbit and classification

[edit]

Coconino is a stonyS-type asteroid and a member of the main-belt'sNysa family, which is named after its largest member44 Nysa. It orbits the Sun in theinner main-belt at a distance of 2.0–2.8 AU once every 3 years and 10 months (1,392 days). Its orbit has aneccentricity of 0.16 and aninclination of 4° with respect to theecliptic.[1]It was first identified as1952 HU3 atMcDonald Observatory in 1952, extending the body'sobservation arc by 30 years prior to its official discovery observation at Flagstaff.[8]

Physical characteristics

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Rotation period

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In February 2005, a rotationallightcurve ofCoconino was obtained from photometric observations by astronomer Horácio Correia. Lightcurve analysis gave a well-definedrotation period of 4.68138 hours with a brightness amplitude of 0.46magnitude (U=3).[6]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Coconino measures 5.607 kilometers in diameter and its surface has a highalbedo of 0.512,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and consequently calculates a larger diameter of 9.40 kilometers, using anabsolute magnitude of 12.5.[3]

Naming

[edit]

Thisminor planet was named after the U.S.Coconino County, Arizona, of which the city of Flagstaff with its discovering observatory is the county seat. The word "Coconino" derives from the language of theHopi Tribe of Arizona.[2] The official naming citation was published by theMinor Planet Center on 17 February 1984 (M.P.C. 8544).[9]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2939 Coconino (1982 DP)" (2017-06-02 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 12 March 2017. Retrieved14 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2939) Coconino".Dictionary of Minor Planet Names – (2939) Coconino.Springer Berlin Heidelberg. p. 242.doi:10.1007/978-3-540-29925-7_2940.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2939) Coconino". Asteroid Lightcurve Database (LCDB). Retrieved9 March 2017.
  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. Retrieved9 March 2017.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2939) Coconino".Geneva Observatory. Retrieved9 March 2017.
  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. Retrieved9 March 2017.
  8. ^ab"2939 Coconino (1982 DP)".Minor Planet Center. Retrieved9 March 2017.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 March 2017.

External links

[edit]
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