6469 Armstrong
| Discovery [1] | |
|---|---|
| Discovered by | A. Mrkos |
| Discovery site | Kleť Obs. |
| Discovery date | 14 August 1982 |
| Designations | |
| MPC designation | 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 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 46.26 yr (16,898 days) |
| Aphelion | 2.6725 AU |
| Perihelion | 1.766 AU |
| 2.2193 AU | |
| Eccentricity | 0.2042 |
| 3.31 yr (1,208 days) | |
| 107.1022° | |
| 0° 17m 53.16s / day | |
| Inclination | 3.9596° |
| 159.4117° | |
| 150.6702° | |
| Earth MOID | 0.7525 AU |
| Physical characteristics | |
| Dimensions |
3.720±0.392 km[4] 2.89 km (calculated)[3] |
|
6.040±0.040 h[5] 5.9648±0.1423 h[6] | |
|
0.2432±0.0393[4] 0.24 (assumed)[3] | |
| S [3] | |
|
14.5[1] 14.340±0.250 (R)[5] 14.3[4] 14.416±0.007 (R)[6] 14.87[3] | |
|
| |
6469 Armstrong, provisional designation 1982 PC, is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 3 kilometers in diameter. It was discovered by Czech astronomer Antonín Mrkos at Kleť Observatory on 14 August 1982.[7]
The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun at a distance of 1.8–2.7 AU once every 3 years and 4 months (1,208 days). Its orbit has an eccentricity of 0.20 and an inclination of 4° with respect to the ecliptic.[1] The first used precovery was taken at Crimea-Nauchnij in 1972, extending the asteroid's observation arc by 10 years prior to its discovery.[7]
Two rotational light-curves of this asteroid were obtained from photometric observations made at the Palomar Transient Factory, California, in January and February 2014. The light-curves gave a concurring rotation period of 6.040±0.040 and 5.9648±0.1423 hours with a brightness variation of 0.65 and 0.70 in magnitude, respectively (U=2/2).[5][6]
According to the survey carried out by the NEOWISE mission of NASA's space-based Wide-field Infrared Survey Explorer, the asteroid measures 3.7 kilometers in diameter and its surface has an albedo of 0.24,[4] while the Collaborative Asteroid Lightcurve Link assumes an identical albedo of 0.24 – derived from 8 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]
The minor planet was named after U.S. astronaut Neil Armstrong (1930–2012), on the occasion of the 30th anniversary of the Apollo 11 mission. On 20 July 1969, Armstrong was one of the first two humans to land on the Moon, and the first person to walk on it, shortly followed by Buzz Aldrin, after whom the asteroid 6470 Aldrin is named. The minor planet 6471 Collins is named after the third crew member of the Apollo 11 mission. In 1966, Armstrong also conducted the first docking in space together with David Scott aboard Gemini 8. The asteroid's name was suggested by Czech astronomers Jana Tichá, Miloš Tichý and Zdeněk Moravec, who observed it during its 1995-opposition, shortly before being numbered.[2] The lunar crater Armstrong is also named in his honor. Naming citation was published on 4 May 1999 (M.P.C. 34623).[8]
References
- 1 2 3 4 "JPL Small-Body Database Browser: 6469 Armstrong (1982 PC)" (2016-01-21 last obs.). Jet Propulsion Laboratory. Retrieved 10 May 2016.
- 1 2 Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (6469) Armstrong. Springer Berlin Heidelberg. pp. 534–535. ISBN 978-3-540-00238-3. Retrieved 10 May 2016.
- 1 2 3 4 5 6 "LCDB Data for (6469) Armstrong". Asteroid Lightcurve Database (LCDB). Retrieved 10 May 2016.
- 1 2 3 4 Mainzer, 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. Retrieved 10 May 2016. - 1 2 3 Chang, 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. Retrieved 10 May 2016.
- 1 2 3 Waszczak, 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. Retrieved 10 May 2016.
- 1 2 "6469 Armstrong (1982 PC)". Minor Planet Center. Retrieved 10 May 2016.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 10 May 2016.
External links
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (5001)-(10000) – Minor Planet Center
- 6469 Armstrong at the JPL Small-Body Database
