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1457 Ankara

From Wikipedia, the free encyclopedia
Stony asteroid from the central region of the asteroid belt

1457 Ankara
Shape ofAnkara modelled from itslightcurve
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date3 August 1937
Designations
(1457) Ankara
Named after
Ankara(Turkish capital)[2]
1937 PA · 1933 SA
1934 XG · 1936 FL1
1943 YD · 1966 BG
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 16 February 2017 (JD 2457800.5)
Uncertainty parameter 0
Observation arc82.95 yr (30,296 days)
Aphelion3.1134AU
Perihelion2.2802 AU
2.6968 AU
Eccentricity0.1545
4.43yr (1,618 days)
63.234°
0° 13m 21.36s / day
Inclination6.0913°
296.31°
296.31°
Physical characteristics
Dimensions17.834±0.207 km[4]
18.495±0.068 km[5]
18.95±0.63 km[6]
19.82±0.26 km[7]
29.08 km(calculated)[3]
31.8±0.6h[8]
0.1(assumed)[3]
0.258±0.051[6]
0.262±0.008[7]
0.3038±0.0536[5]
0.320±0.037[4]
S[3]
10.60[7][5] · 10.70[6] · 10.8[1][3]

1457 Ankara, provisional designation1937 PA, is a stonyasteroid from the central region of theasteroid belt, approximately 18 kilometers in diameter. It was discovered on 3 August 1937, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany, and later named for the Turkish capital city ofAnkara.[2][9]

Orbit and classification

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Ankara orbits the Sun in themiddle of the main-belt at a distance of 2.3–3.1 AU once every 4 years and 5 months (1,618 days). Its orbit has aneccentricity of 0.15 and aninclination of 6° with respect to theecliptic.[1] It was first observed as1933 SA atUccle Observatory in 1933, extending the body'sobservation arc by 4 years prior to its official discovery observation at Heidelberg.[9]

Physical characteristics

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Rotation period

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A rotationallightcurve ofAnkara was obtained from photometric observations by French amateur astronomerRené Roy in September 2004. Lightcurve analysis gave arotation period of 31.8 hours with a brightness variation of 0.21magnitude (U=2).[8] While not being aslow rotator,Ankara's spin rate is slower than that of most asteroids, which typically rotate within 20 hours once around their axis.

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,Ankara measures between 17.834 and 19.82 kilometers in diameter and its surface has analbedo between 0.258 and 0.320.[4][5][6][7]

TheCollaborative Asteroid Lightcurve Link (CALL) assumes a lower albedo of 0.10 – a compromise value that lies between the albedos forstony (0.20) andcarbonaceous (0.057) asteroids, chosen by CALL for all non-family asteroids with asemi-major axis between 2.6 and 2.7 AU – and consequently calculates a larger diameter of 29.08 kilometers with anabsolute magnitude of 10.8, as a body's diameter and albedo are inversely related to each other.[3]

Naming

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Thisminor planet was named after the Turkish capitalAnkara. The official naming citation was proposed by Wolfgang Gleißberg, a German Solar astronomer, who immigrated to Turkey, after he was dismissed at the Breslau Observatory in Nazi Germany in 1933, because he had a Jewish grandfather. The citation was first mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H131).[2][10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1457 Ankara (1937 PA)" (2016-08-27 last obs.).Jet Propulsion Laboratory. Retrieved27 April 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1457) Ankara".Dictionary of Minor Planet Names – (1457) Ankara.Springer Berlin Heidelberg. p. 117.doi:10.1007/978-3-540-29925-7_1458.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1457) Ankara". Asteroid Lightcurve Database (LCDB). Retrieved27 April 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. Retrieved27 April 2017.
  5. ^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.
  6. ^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. Retrieved27 April 2017.
  7. ^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)
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1457) Ankara".Geneva Observatory. Retrieved27 April 2017.
  9. ^ab"1457 Ankara (1937 PA)".Minor Planet Center. Retrieved27 April 2017.
  10. ^Angelika Rieber."Wolfgang Gleissberg – Refuge in Turkey". Project Jewish Life in Frankfurt. Archived fromthe original on 4 January 2017. Retrieved27 April 2017.

External links

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Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
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