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1922 Zulu

From Wikipedia, the free encyclopedia
Main-belt carbonaceous asteroid

1922 Zulu
Discovery[1]
Discovered byE. Johnson
Discovery siteJohannesburg Obs.
Discovery date25 April 1949
Designations
(1922) Zulu
Named after
Zulu(tribe)[2]
1949 HC
main-belt · (outer)[1][3]
2:1 res[4]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc67.70 yr (24,727 days)
Aphelion4.7945AU
Perihelion1.6775 AU
3.2360 AU
Eccentricity0.4816
5.82yr (2,126 days)
187.91°
0° 10m 9.48s / day
Inclination35.446°
226.53°
31.395°
Earth MOID0.7153 AU
Jupiter MOID0.6296 AU
Physical characteristics
Dimensions12.41±2.60 km[5]
19.30 km(calculated)[3]
20.561±0.321 km[6][7]
18.64±0.01h[8]
18.65 h[9]
0.055±0.006[6][7]
0.057(assumed)[3]
0.16±0.05[5]
C[3]
12.2[6] · 12.27±0.24[10] · 12.3[1][3][5]

1922 Zulu, provisional designation1949 HC, is a carbonaceousasteroid in a strongly unstable resonance with Jupiter, located in the outermost regions of theasteroid belt, and approximately 20 kilometers in diameter. It was discovered on 25 April 1949, by South African astronomerErnest Johnson atUnion Observatory in Johannesburg, and named for the South AfricanZulu people.[2][11]

Orbit and classification

[edit]

Zulu is one of few strongly unstable asteroids located near the 2:1orbital resonance with the gas giantJupiter, that corresponds to one of the prominentKirkwood gaps in the asteroid belt.[4]

It orbits the Sun at a distance of 1.7–4.8 AU once every 5 years and 10 months (2,126 days). Its orbit has aneccentricity of 0.48 and aninclination of 35° with respect to theecliptic.[1] The body'sobservation arc begins with its official discovery observation at Johannesburg, as noprecoveries were taken and no prior identifications were made.[11]

Zulu was lost shortly after its 1949-discovery(seeLost asteroid), and only rediscovered in 1974 by Richard Eugene McCrosky, Cheng-yuan Shao and JH Bulger based on a predicted position by C. M. Bardwell of theCincinnati Observatory.[12] It is quite highly inclined for asteroids in the asteroid belt, with an inclination of 35.4 degrees. This may be related to its 2:1 resonance with Jupiter.

Physical characteristics

[edit]

In May 2002, a rotationallightcurve ofZulu was obtained from photometric observations by American astronomerRobert Stephens at the Santana Observatory in California. Lightcurve analysis gave a well-definedrotation period of 18.64 hours with a brightness variation of 0.11magnitude (U=3).[8] One month later, French amateur astronomersRené Roy and Laurent Brunetto obtained another lightcurve with a concurring period of 18.65 hours and an amplitude of 0.09 magnitude (U=1).[9]

According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Zulu measures 12.41 and 20.561 kilometers in diameter and its surface has analbedo of 0.055 and 0.16.[5][6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceousC-type asteroid of 0.057 and calculates a diameter of 19.30 kilometers with anabsolute magnitude of 12.3.[3]

Naming

[edit]

Thisminor planet was named after the South AfricanZulu people, in recognition of the tribesmen who devotedly worked at the Johannesburg Union Observatory. The name also closely relates to1362 Griqua and1921 Pala, which also received tribal names and librate in the 2:1 ratio of Jupiter's mean motion as well.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3938).[13]

See also

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References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 1922 Zulu (1949 HC)" (2017-01-05 last obs.).Jet Propulsion Laboratory. Retrieved31 March 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1922) Zulu".Dictionary of Minor Planet Names – (1922) Zulu.Springer Berlin Heidelberg. p. 154.doi:10.1007/978-3-540-29925-7_1923.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1922) Zulu". Asteroid Lightcurve Database (LCDB). Retrieved31 March 2017.
  4. ^abRoig, F.; Nesvorný, D.; Ferraz-Mello, S. (September 2002)."Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution [ Erratum: 2002MNRAS.336.1391R ]".Monthly Notices of the Royal Astronomical Society.335 (2):417–431.Bibcode:2002MNRAS.335..417R.doi:10.1046/j.1365-8711.2002.05635.x.
  5. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved31 March 2017.
  6. ^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.
  7. ^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. Retrieved31 March 2017.
  8. ^abStephens, R. D. (December 2002)."Photometry of 769 Tatjana, 818 Kapteyna, 1922 Zulu, and 3687 Dzus".The Minor Planet Bulletin.29: 72.Bibcode:2002MPBu...29...72S. Retrieved31 March 2017.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1922) Zulu".Geneva Observatory. Retrieved31 March 2017.
  10. ^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. Retrieved31 March 2017.
  11. ^ab"1922 Zulu (1949 HC)".Minor Planet Center. Retrieved31 March 2017.
  12. ^Brian G. Marsden (24 October 1974)."International Astronomical Union Circular 2710 – 1949 HC (3rd item)". Central Bureau for Astronomical Telegrams. Retrieved31 March 2017.
  13. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.Bibcode:2009dmpn.book.....S.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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