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1194 Aletta

From Wikipedia, the free encyclopedia
Main-belt asteroid

1194 Aletta
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date13 May 1931
Designations
(1194) Aletta
Named after
Aletta Jackson
(discoverer's wife)[2]
1931 JG · 1946 KC
1962 SB
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc85.07 yr (31,072 days)
Aphelion3.1812AU
Perihelion2.6452 AU
2.9132 AU
Eccentricity0.0920
4.97yr (1,816 days)
138.73°
0° 11m 53.52s / day
Inclination10.870°
291.32°
243.18°
Physical characteristics
Dimensions41.358±0.191 km[4]
42.67±0.77 km[5]
46.371±1.188 km[6]
55.22±20.92 km[7]
55.23 km(derived)[3]
55.39±1.4 km[8]
19.7±0.1h[9]
20.39±0.01 h[10]
20.3903±0.2170 h[11]
0.03±0.03[7]
0.0333(derived)[3]
0.0375±0.0065[6]
0.0479±0.003[8]
0.085±0.004[5]
0.087±0.011[4]
C[3]
10.2[5][6][8] · 10.5[12] · 10.6[1][3][7] · 10.644±0.001(R)[11]

1194 Aletta, provisional designation1931 JG, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 55 kilometers in diameter. It was discovered on 13 May 1931, by South African astronomerCyril Jackson atJohannesburg Observatory in South Africa.[13] It was later named after the discoverer's wife Aletta Jackson.[2]

Classification and orbit

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Aletta is a darkC-type asteroid and orbits the Sun at a distance of 2.6–3.2 AU once every 4 years and 12 months (1,816 days). Its orbit has aneccentricity of 0.09 and aninclination of 11° with respect to theecliptic.[1] The body'sobservation arc begins at Johannesburg, one week after its official discovery observation. Noprecoveries were taken and no prior identifications were made.[13]

Physical characteristics

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Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Aletta measures between 41.358 and 55.39 kilometers in diameter, and its surface has analbedo between 0.03 and 0.87.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0333 and a diameter of 55.23 kilometers based on anabsolute magnitude of 10.6.[3]

Rotation period

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In November 2007, American astronomer James W. Brinsfield obtained the first everlightcurve ofAletta with period of 19.7 hours and a brightness variation of 0.32magnitude at Via Capote Observatory (U=2).[9] Two morelightcurves were obtained by Australian astronomer Julian Oey at Leura/Kingsgrove Observatory in March 2010, and by the Survey conducted at thePalomar Transient Factory, California, in October 2012. Lightcurve analysis gave a concurringrotation period of 20.39 and 20.3903 hours with an amplitude of 0.28 and 0.27 magnitude, respectively (U=2+/2).[10][11]

Naming

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The discoverer named thisminor planet for his wife, Aletta Jackson (née Maria Aletta Lessing).[2] Naming citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 111).[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1194 Aletta (1931 JG)" (2016-06-14 last obs.).Jet Propulsion Laboratory. Retrieved1 February 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1194) Aletta".Dictionary of Minor Planet Names – (1194) Aletta.Springer Berlin Heidelberg. p. 100.doi:10.1007/978-3-540-29925-7_1195.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1194) Aletta". Asteroid Lightcurve Database (LCDB). Retrieved1 February 2017.
  4. ^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. Retrieved1 February 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. ^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. Retrieved1 February 2017.
  8. ^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.
  9. ^abBrinsfield, James W. (June 2008)."The Rotation Periods of 531 Zerlina, 1194 Aleta 1352 Wawel, 2005 Hencke, 2648 Owa, and 3509 Sanshui".The Minor Planet Bulletin.35 (2):86–87.Bibcode:2008MPBu...35...86B.ISSN 1052-8091. Retrieved1 February 2017.
  10. ^abOey, Julian (October 2011)."Lightcurve Analysis of Asteroids from Leura and Kingsgrove Observatory for the Second Half of 2009 and 2010".The Minor Planet Bulletin.38 (4):221–223.Bibcode:2011MPBu...38..221O.ISSN 1052-8091. Retrieved1 February 2017.
  11. ^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. Retrieved1 February 2017.
  12. ^Faure, Gerard; Garrett, Lawrence (October 2009)."Suggested Revised H Values of Selected Asteroids: Report Number 4".The Minor Planet Bulletin.36 (4):140–143.Bibcode:2009MPBu...36..140F.ISSN 1052-8091. Retrieved1 February 2017.
  13. ^ab"1194 Aletta (1931 JG)".Minor Planet Center. Retrieved1 February 2017.

External links

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