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6469 Armstrong

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6469 Armstrong
Discovery [1]
Discovered byA. Mrkos
Discovery siteKleť Obs.
Discovery date14 August 1982
Designations
(6469) Armstrong
Named after
Neil Armstrong
(astronaut,Apollo 11)[2]
1982 PC · 1969 UK1
1972 NN · 1979 WZ6
1982 QL
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc47.45 yr (17,332 days)
Aphelion2.6725AU
Perihelion1.7663 AU
2.2194 AU
Eccentricity0.2041
3.31yr (1,208 days)
226.43°
0° 17m 53.16s / day
Inclination3.9595°
159.41°
150.61°
Physical characteristics
Dimensions2.89 km(calculated)[3]
3.720±0.392 km[4][5]
5.9648±0.1423h[6]
6.040±0.040 h[7]
0.24(assumed)[3]
0.243±0.039[4][5]
S[3]
14.5[1] · 14.340±0.250(R)[7] · 14.3[4] · 14.416±0.007(R)[6] · 14.87[3]

6469 Armstrong, provisional designation1982 PC, is a stony Floraasteroid from the inner regions of theasteroid belt, approximately 3 kilometers in diameter. It was discovered by Czech astronomerAntonín Mrkos atKleť Observatory on 14 August 1982.[8] The asteroid was later named for American astronautNeil Armstrong.[2]

Orbit and classification

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Armstrong is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,208 days). Its orbit has aneccentricity of 0.20 and aninclination of 4° with respect to theecliptic.[1]

In October 1969, it was first identified as1969 UK1 atCrimea–Nauchnij. The body'sobservation arc began 10 years prior to its official discovery at Klet Observatory, with aprecovery taken at Crimea–Nauchnij in July 1972.[8]

Physical characteristics

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Armstrong is a presumedS-type asteroid.[3]

Rotation period

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Two rotationallightcurves ofArmstrong were obtained from photometric observations made at thePalomar Transient Factory, California, in January and February 2014. The lightcurves gave a concurringrotation period of6.040±0.040 and5.9648±0.1423 hours with a brightness variation of 0.65 and 0.70 inmagnitude, respectively (U=2/2).[7][6]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA's space-basedWide-field Infrared Survey Explorer,Armstrong measures 3.7 kilometers in diameter and its surface has analbedo of 0.24.[4][5]

TheCollaborative Asteroid Lightcurve Link assumes an identical albedo of 0.24 – derived from8 Flora, the largest member and namesake of its orbital family – and calculates a diameter of 2.9 kilometers, based on a weaker absolute magnitude of 14.87.[3]

Naming

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Thisminor planet was named after American astronautNeil Armstrong, on the occasion of the 30th anniversary of theApollo 11 mission.[2]

On 20 July 1969, Armstrong was one of the first two humans toland on the Moon, and thefirst person to walk on it, shortly followed byBuzz Aldrin, after whom the asteroid6470 Aldrin is named. The minor planet6471 Collins is named afterMichael Collins, the third crew member of the Apollo 11 mission. In 1966, Armstrong also conducted the first docking in space together withDavid Scott aboardGemini 8. The asteroid's name was suggested by Czech astronomersJana Tichá,Miloš Tichý andZdeněk Moravec, who observed it during its 1995-opposition, shortly before being numbered.[2] The approved naming citation was published by theMinor Planet Center on 4 May 1999 (M.P.C. 34623).[9]

The lunar craterArmstrong is also named in his honor.

References

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  1. ^abcd"JPL Small-Body Database Browser: 6469 Armstrong (1982 PC)" (2017-03-30 last obs.).Jet Propulsion Laboratory. Retrieved21 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(6469) Armstrong".Dictionary of Minor Planet Names – (6469) Armstrong.Springer Berlin Heidelberg. pp. 534–535.doi:10.1007/978-3-540-29925-7_5888.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (6469) Armstrong". Asteroid Lightcurve Database (LCDB). Retrieved10 May 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.S2CID 35447010. Retrieved10 May 2016.
  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.S2CID 118745497. Retrieved5 December 2016.
  6. ^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.S2CID 8342929. Retrieved10 May 2016.
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (August 2015)."Asteroid Spin-rate Study Using the Intermediate Palomar Transient Factory".The Astrophysical Journal Supplement Series.219 (2): 19.arXiv:1506.08493.Bibcode:2015ApJS..219...27C.doi:10.1088/0067-0049/219/2/27.S2CID 17093124. Retrieved10 May 2016.
  8. ^ab"6469 Armstrong (1982 PC)".Minor Planet Center. Retrieved10 May 2016.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved10 May 2016.

External links

[edit]
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