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1264 Letaba

From Wikipedia, the free encyclopedia
Carbonaceous asteroid

1264 Letaba
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date21 April 1933
Designations
(1264) Letaba
Named after
Letaba River[2]
(South Africanriver)
1933 HG · 1930 WC
1954 YB · 1962 HJ
1964 VB
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc84.54 yr (30,877 days)
Aphelion3.3108AU
Perihelion2.4225 AU
2.8667 AU
Eccentricity0.1549
4.85yr (1,773 days)
112.30°
0° 12m 11.16s / day
Inclination24.953°
235.05°
31.529°
Physical characteristics
Dimensions66.040±0.405 km[5]
67.76±17.00 km[6]
67.79±17.67 km[7]
70.180±23.32 km[8]
70.34±0.77 km[9]
73.629±0.870 km[10]
74.35 km(derived)[3]
74.74±2.1 km[11]
12h[12]
16 h[12]
32.16±0.03 h[13]
32.74±0.02 h(best)[14]
33.27±0.01 h[15]
63.74±0.01 h[16]
0.0407±0.0432[8]
0.0462(derived)[3]
0.05±0.07[7]
0.05±0.09[6]
0.0725±0.004[11]
0.0746±0.0114[10]
0.082±0.002[9]
0.093±0.027[5]
SMASS =C[1][3]
9.10[9][10][11] · 9.60[3][7] · 9.67[6] · 9.70[1][8] · 9.87±0.22[17]

1264 Letaba, provisional designation1933 HG, is a carbonaceousasteroid and possibletumbler from thebackground population of the outerasteroid belt, approximately 70 kilometers in diameter. It was discovered on 21 April 1933, by South African astronomerCyril Jackson at theUnion Observatory in Johannesburg.[18] The asteroid was named for theLetaba River in eastern South Africa.[2]

Orbit and classification

[edit]

Letaba is a non-family asteroid of the main belt'sbackground population.[4] It orbits the Sun in theouter asteroid belt at a distance of 2.4–3.3 AU once every 4 years and 10 months (1,773 days;semi-major axis of 2.87 AU). Its orbit has aneccentricity of 0.15 and aninclination of 25° with respect to theecliptic.[1]

The asteroid was first identified as1930 WC atSimeiz Observatory in November 1930. The body'sobservation arc begins at Johannesburg, the night before its official discovery observation.[18]

Physical characteristics

[edit]

In theSMASS classification,Letaba is a carbonaceousC-type asteroid.[1][3]

Rotation period

[edit]

Several rotationallightcurves ofLetaba have been obtained from photometric observations since 2002.[12][13][15][16] The best-rated lightcurve was measured by the Spanish amateur astronomer group OBAS in July 2016. It gave a longer-than averagerotation period of 32.74 hours with a brightness variation of 0.28magnitude (U=3).[14] It might be atumbler due to the lightcurve's inconsistent slope segments (T?).[3][16] Based on its current diameter estimate,Letaba would be the second-largest tumbler just behind the Hildian asteroid1512 Oulu(seeList of tumblers).

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Letaba measures between 66.040 and 74.74 kilometers in diameter and its surface has analbedo between 0.0407 and 0.093.[5][6][7][8][9][10][11]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0462 and a diameter of 74.35 kilometers based on anabsolute magnitude of 9.6.[3]

Naming

[edit]

Thisminor planet was named after theLetaba River, located in eastern South Africa. The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 116).[2]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 1264 Letaba (1933 HG)" (2017-11-02 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 18 September 2020. Retrieved22 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1264) Letaba".Dictionary of Minor Planet Names – (1264) Letaba.Springer Berlin Heidelberg. p. 105.doi:10.1007/978-3-540-29925-7_1265.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (1264) Letaba". Asteroid Lightcurve Database (LCDB). Retrieved22 November 2017.
  4. ^ab"Asteroid 1264 Letaba – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  5. ^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.S2CID 119293330.
  6. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  7. ^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.S2CID 9341381. Retrieved22 November 2017.
  8. ^abcdMasiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017)."NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos".The Astronomical Journal.154 (4): 10.arXiv:1708.09504.Bibcode:2017AJ....154..168M.doi:10.3847/1538-3881/aa89ec.
  9. ^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)
  10. ^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.
  11. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  12. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1264) Letaba". Geneva Observatory. Retrieved22 November 2017.
  13. ^abStephens, Robert D. (December 2002)."Photometry of 430 Hybris, 798 Ruth, 1264 Letaba, and 3786 Yamada".The Minor Planet Bulletin.30 (1):1–2.Bibcode:2003MPBu...30....1S.ISSN 1052-8091. Retrieved22 November 2017.
  14. ^abBrines, Pedro; Lozano, Juan; Rodrigo, Onofre; Fornas, A.; Herrero, David; Mas, Vicente; et al. (April 2017)."Sixteen Asteroids Lightcurves at Asteroids Observers (OBAS) - MPPD: 2016 June-November".The Minor Planet Bulletin.44 (2):145–149.Bibcode:2017MPBu...44..145B.ISSN 1052-8091. Retrieved22 November 2017.
  15. ^abFerrro, Andrea (April 2017)."Rotational Period of Three Main-belt Asteroids".The Minor Planet Bulletin.44 (2): 142.Bibcode:2017MPBu...44..142F.ISSN 1052-8091. Retrieved22 November 2017.
  16. ^abcOey, Julian; Williams, Hasen; Groom, Roger (July 2017)."Lightcurve Analysis of Asteroids from BMO and DRO in 2015".The Minor Planet Bulletin.44 (3):200–204.Bibcode:2017MPBu...44..200O.ISSN 1052-8091. Retrieved22 November 2017.
  17. ^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.S2CID 53493339. Retrieved22 November 2017.
  18. ^ab"1264 Letaba (1933 HG)".Minor Planet Center. Retrieved22 November 2017.

External links

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