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1467 Mashona

From Wikipedia, the free encyclopedia
Asteroid

1467 Mashona
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date30 July 1938
Designations
(1467) Mashona
Named after
Shona people (Mashona)
(natives ofMashonaland)[2]
1938 OE · 1930 DL
1936 DK · 1936 FA1
1948 EG · A923 CB
main-belt · (outer)[1]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc94.41 yr (34,483 days)
Aphelion3.8268AU
Perihelion2.9485 AU
3.3877 AU
Eccentricity0.1296
6.24yr (2,277 days)
255.30°
0° 9m 29.16s / day
Inclination21.910°
326.50°
349.55°
Physical characteristics
Dimensions89.160±0.728 km[3]
90.93±28.77 km[4]
95.08±1.30 km[5]
104.119±1.062 km[6]
107.54 km(calculated)[7]
9.740±0.0029h[8]
9.744±0.001 h[9]
9.76 h[10]
0.05±0.03[4]
0.057(assumed)[7]
0.0609±0.0111[6]
0.074±0.002[5]
0.083±0.014[3]
Tholen = GC[1] · GC[7]
B–V = 0.743[1]
U–B = 0.373[1]
8.515±0.001(R)[8]
8.57[1][4][5][6][7]

1467 Mashona, provisional designation1938 OE, is a rare-type carbonaceousasteroid from the outer regions of theasteroid belt, approximately 100 kilometers in diameter, making it one of the top 200largest asteroids currently known to exist. It was discovered on 30 July 1938, by South African astronomerCyril Jackson at theJohannesburg Observatory in South Africa.[11] It was later named after the nativeShona people of Zimbabwe.[2]

Classification and orbit

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Mashona orbits the Sun in theouter main-belt at a distance of 2.9–3.8 AU once every 6 years and 3 months (2,277 days). Its orbit has aneccentricity of 0.13 and aninclination of 22° with respect to theecliptic.[1] It is a member of theCybele asteroid group.[12]

In February 1923, it was first identified as1923 CB atHeidelberg Observatory in Germany. The body'sobservation arc begins at Johannesburg, 5 days after its official discovery observation.[11]

Mashona was the highest numbered asteroid used in calculating the future orbit of101955 Bennu.[13]

Physical characteristics

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In theTholen classification,Mashona is a rare GC-type, aspectral type that transitions between the commonC and rareG-type asteroids.[1]

Lightcurves

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Until April 2010, three rotationallightcurves ofMashona have been obtained from photometric observations. Lightcurve analysis gave a well-definedrotation period between 9.74 and 9.76 hours with a brightness amplitude varying from 0.24 to 0.31magnitude (U=3/2/3).[8][9][10]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Mashona measures between 89.160 and 104.119 kilometers in diameter and its surface has analbedo between 0.05 and 0.083.[3][4][5][6] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 107.54 kilometers based on anabsolute magnitude of 8.57.[7] Among nearly half a million asteroids,Mashona belongs to the 200 largest bodies.[14]

Naming

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Thisminor planet was named for theShona people (Mashona), natives ofMashonaland in Zimbabwe, then Rhodesia.[2] The officialnaming citation was published by theMinor Planet Center in April 1953 (M.P.C. 909).[15]

References

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  1. ^abcdefghi"JPL Small-Body Database Browser: 1467 Mashona (1938 OE)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved24 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1467) Mashona".Dictionary of Minor Planet Names – (1467) Mashona.Springer Berlin Heidelberg. p. 117.doi:10.1007/978-3-540-29925-7_1468.ISBN 978-3-540-00238-3.
  3. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved24 July 2017.
  4. ^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. Retrieved24 July 2017.
  5. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011)."Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  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. ^abcde"LCDB Data for (1467) Mashona". Asteroid Lightcurve Database (LCDB). Retrieved24 July 2017.
  8. ^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. Retrieved24 July 2017.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1467) Mashona".Geneva Observatory. Retrieved24 July 2017.
  10. ^abLagerkvist, Claes-Ingvar; Erikson, Anders; Lahulla, Felix; De Martino, Mario; Nathues, Andreas; Dahlgren, Mats (January 2001)."A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids".Icarus.149 (1):190–197.Bibcode:2001Icar..149..190L.doi:10.1006/icar.2000.6507. Retrieved24 July 2017.
  11. ^ab"1467 Mashona (1938 OE)".Minor Planet Center. Retrieved24 July 2017.
  12. ^Lagerkvist, Claes-Ingvar; et al. (January 2001), "A Study of Cybele Asteroids. I. Spin Properties of Ten Asteroids",Icarus,149 (1):190–197,Bibcode:2001Icar..149..190L,doi:10.1006/icar.2000.6507.
  13. ^Farnocchia, Davide; Chesley, Steven R.; Takahashi, Yu (2021)."Ephemeris and hazard assessment for near-Earth asteroid (101955) Bennu based on OSIRIS-REx data".Icarus.doi:10.1016/j.icarus.2021.114594.
  14. ^Wm. Robert Johnston (7 February 2015)."The largest asteroids and outer solar system objects". Johnston's Archive. Retrieved24 July 2017.
  15. ^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.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

[edit]
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