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8026 Johnmckay

From Wikipedia, the free encyclopedia
Hungaria asteroid and very slow rotator

8026 Johnmckay
Discovery[1]
Discovered byE. F. Helin
Discovery sitePalomar Obs.
Discovery date8 May 1991
Designations
(8026) Johnmckay
Named after
John B. McKay(test pilot)[2]
1991 JA1 · 1989 UF2
main-belt · (inner)[1]
Hungaria[2][3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc27.33 yr (9,981 days)
Aphelion2.0697AU
Perihelion1.7809 AU
1.9253 AU
Eccentricity0.0750
2.67yr (976 days)
181.46°
0° 22m 8.04s / day
Inclination19.936°
217.71°
145.66°
Knownsatellites1[4]
Physical characteristics
Dimensions1.690±0.239 km[5][6]
2.54 km(calculated)[3]
355±5 h[7]
372±5h[8]
0.30(assumed)[3]
0.815±0.196[5][6]
E[3]
14.60±0.44[9] · 14.7[5] · 14.9[1][3]

8026 Johnmckay, provisional designation1991 JA1, is abinary[4] Hungariaasteroid and veryslow rotator from the inner regions of theasteroid belt, approximately 2 kilometers in diameter. It was discovered on 8 May 1991, by American astronomerEleanor Helin at the U.S.Palomar Observatory, California, and later named for NASA test pilotJohn B. McKay.[2]

Classification and orbit

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The brightE-type asteroid is a member of theHungaria family, which form the innermost dense concentration of asteroids in the Solar System.Johnmckay orbits the Sun in theinner main-belt at a distance of 1.8–2.1 AU once every 2 years and 8 months (976 days). Its orbit has aneccentricity of 0.08 and aninclination of 20° with respect to theecliptic.[1] The first observation was made at the discovering observatory in 1989, extending the asteroid'sobservation arc by almost 2 years prior to its discovery.[2]

Diameter estimates

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Johnmckay measures 1.7 kilometers in diameter and its surface has an exceptionally highalbedo of 0.81, while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for Hungaria asteroids of 0.30, and calculates a diameter of 2.5 kilometers, based on anabsolute magnitude of 14.9.[3][5][6]

Lightcurves

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Primary

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Two rotationallightcurves ofJohnmckay were obtained for this asteroid from photometric observations by U.S. astronomerBrian D. Warner at the Palmer Divide Station (PDO), Colorado. In August 2010, the first lightcurve gave a longrotation period of372±5 hours with a brightness variation of 1.0 inmagnitude (U=3).[8] The second lightcurve from June 2015, gave a similar period of355±5 with an amplitude of 0.66 in magnitude (U=2).[7]

This makesJohnmckay one of theTop 100+ slowest rotators known to exist.

Moon

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In 2010 a smallasteroid moon was discovered around this asteroid. It has anorbital period of2.300±0.001 hours,[4] while observations at the PDO gave it a period of 2.2981 and 14.93 hours, respectively.[3][7][8]

Naming

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Thisminor planet was named in memory of NASA test pilotJohn B. McKay (1922–1975), one of the first pilots assigned to fly theNorth American X-15. He was also assigned to theX-1E and to theD-558-II. He died in 1975, from injuries he had sustained during a X-15 crash. In 2005, he received posthumous theastronaut badge for a reached peak-altitude of 89,900 metres (295,000 feet).[2] The approved naming citation was published by theMinor Planet Center on 7 February 2012 (M.P.C. 78269).[10]

References

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  1. ^abcde"JPL Small-Body Database Browser: 8026 Johnmckay (1991 JA1)" (2017-02-23 last obs.).Jet Propulsion Laboratory. Retrieved4 July 2017.
  2. ^abcde"8026 Johnmckay (1991 JA1)".Minor Planet Center. Retrieved11 August 2016.
  3. ^abcdefg"LCDB Data for (8026) Johnmckay". Asteroid Lightcurve Database (LCDB). Retrieved11 August 2016.
  4. ^abcJohnston, Robert."(8026) Johnmckay".johnstonsarchive.net. Retrieved29 May 2015.
  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.
  6. ^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.
  7. ^abcWarner, Brian D. (October 2015). "Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2015 March-June".The Minor Planet Bulletin.42 (4):267–276.Bibcode:2015MPBu...42..267W.ISSN 1052-8091.PMID 32455362.
  8. ^abcWarner, Brian D. (January 2011). "A Quartet of Known and Suspected Hungaria Binary Asteroids".The Minor Planet Bulletin.38 (1):33–36.Bibcode:2011MPBu...38...33W.ISSN 1052-8091.
  9. ^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.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved11 August 2016.

External links

[edit]
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Authority control databasesEdit this at Wikidata
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