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1126 Otero

From Wikipedia, the free encyclopedia
Main-belt asteroid

1126 Otero
Alightcurve-based 3D-model ofOtero
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date11 January 1929
Designations
(1126) Otero
Named after
Carolina Otero
(Spanish courtesan)[2]
1929 AC · 1926 GD
1948 RN1 · 1949 YO
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc90.71 yr (33,133 days)
Aphelion2.6052AU
Perihelion1.9394 AU
2.2723 AU
Eccentricity0.1465
3.43yr (1,251 days)
291.09°
0° 17m 15.72s / day
Inclination6.5045°
1.0892°
136.08°
Physical characteristics
Dimensions8.87±1.56 km[4]
10.974±0.892 km[5]
11.74 km(derived)[3]
3.648±0.002h[6]
3.64808±0.00014 h[a]
0.1994(derived)[3]
0.37±0.13[4]
0.399±0.320[5]
SMASS =A[1] · A[3]
11.41[5] · 11.57±0.05(R)[a] · 11.9[1] · 12.098±0.071[3][7] · 12.10[4]

1126 Otero, provisional designation1929 AC, is a rare-type Florianasteroid from the inner regions of theasteroid belt, approximately 10 kilometers in diameter. It was discovered on 11 January 1929, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[8] It was named after Spanish courtesanCarolina Otero.[2]

Classification and orbit

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Otero is a member of theFlora family, one of the largest families of stony asteroids in the main belt. It orbits the Sun in theinner main-belt at a distance of 1.9–2.6 AU once every 3 years and 5 months (1,251 days). Its orbit has aneccentricity of 0.15 and aninclination of 7° with respect to theecliptic.[1] It was first identified as1926 GD atUccle/Heidelberg in 1926, extending the asteroid'sobservation arc by 3 years prior to its official discovery at Heidelberg.[8]

Physical parameters

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In theSMASS classification,Otero is a rareA-type asteroid.[1]

Lightcurves

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Two rotationallightcurve ofOtero were obtained from photometric observations by astronomersPetr Pravec andRobert Stepens in February 2008. Lightcurve analysis gave a concurring, well-definedrotation period of 3.648 hours with a brightness variation of 0.69 and 0.70magnitude, respectively (U=3/3).[6][a]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Otero measures 8.87 and 10.974 kilometers in diameter and its surface has analbedo of 0.37 and 0.399, respectively.[4][5] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.1994 and a diameter of 11.74 kilometers with anabsolute magnitude of 12.098 from Petr Pravec's revised WISE-data.[3][7]

Naming

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Thisminor planet was named by the discoverer for Galician-born Spanish courtesan, dancer and actressCarolina Otero (1868–1965), who was also known as "La Belle Otero". During theBelle Époque, she was the most sought after woman in all of Europe and led an excessive life thanks to her numerous rich and famous lovers. The official naming citation was first published by theAstronomical Calculation Institute (RI 803).[2]

Space-based observations

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Otero was observed byESA's missionHera from a distance of 2.8 millions km on May 11, 2025 as the spacecraft was heading towardDidymos.[9]

Hera observation of Otero on May 11th 2025.

Notes

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  1. ^abcPravec (2008) web:lightcurve plot of (1126) Otero by Petr Pravec of the Ondrejov Asteroid Photometry Project, with rotation period3.64808±0.00014 hours and a brightness amplitude of0.69 mag. Summary figures atCollaborative Asteroid Lightcurve Link andPravec, P.; Wolf, M.; Sarounova, L. (2008)

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1126 Otero (1929 AC)" (2016-12-21 last obs.).Jet Propulsion Laboratory. Retrieved26 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1126) Otero".Dictionary of Minor Planet Names – (1126) Otero.Springer Berlin Heidelberg. pp. 95–96.doi:10.1007/978-3-540-29925-7_1127.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1126) Otero". Asteroid Lightcurve Database (LCDB). Retrieved14 March 2017.
  4. ^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.
  5. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved14 March 2017.
  6. ^abStephens, Robert D. (September 2008)."Asteroids Observed from GMARS and Santana Observatories - Late 2007 and Early 2008".The Minor Planet Bulletin.35 (3):126–128.Bibcode:2008MPBu...35..126S.ISSN 1052-8091. Retrieved14 March 2017.
  7. ^abPravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012)."Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations".Icarus.221 (1):365–387.Bibcode:2012Icar..221..365P.doi:10.1016/j.icarus.2012.07.026. Retrieved14 March 2017.
  8. ^ab"1126 Otero (1929 AC)".Minor Planet Center. Retrieved14 March 2017.
  9. ^"First asteroid sightings push Hera's camera to the limit" (Article).European Space Agency. Retrieved6 August 2025.

External links

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