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1257 Móra

From Wikipedia, the free encyclopedia
Main-belt asteroid

1257 Móra
Discovery[1]
Discovered byK. Reinmuth
Discovery siteHeidelberg Obs.
Discovery date8 August 1932
Designations
(1257) Móra
Named after
Kráoly Móra
(Hungarian astronomer)[2]
1932 PE · 1928 QA
1935 KL · 1964 VO
1964 WA
main-belt · (inner)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc88.80 yr (32,434 days)
Aphelion2.6962AU
Perihelion2.2815 AU
2.4888 AU
Eccentricity0.0833
3.93yr (1,434 days)
335.03°
0° 15m 3.6s / day
Inclination3.9231°
213.94°
18.983°
Physical characteristics
Dimensions10.79 km(derived)[3]
14.72±4.32 km[4]
17.05±6.10 km[5]
21.392±1.126 km[6][7]
21.47±0.64 km[8]
5.28h[9]
5.2948±0.0004 h[10]
5.3±0.1 h[10]
0.051±0.007[6][7]
0.08±0.07[5]
0.096±0.007[8]
0.10±0.07[4]
0.20(assumed)[3]
C[9] · S[3]
B–V = 0.630[1]
U–B = 0.320[1]
11.50[8] · 12.00[5] · 12.09[4] · 12.1[1] · 12.2[3][6][9]

1257 Móra, provisional designation1932 PE, is anasteroid from the inner regions of theasteroid belt, approximately 15 kilometers in diameter. It was discovered on 8 August 1932, by German astronomerKarl Reinmuth atHeidelberg Observatory in southwest Germany.[11] The asteroid was named after Hungarian astronomerKároly Móra [hu].[2]

Orbit and classification

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Móra orbits the Sun in theinner main-belt at a distance of 2.3–2.7 AU once every 3 years and 11 months (1,434 days). Its orbit has aneccentricity of 0.08 and aninclination of 4° with respect to theecliptic.[1] Identified as1928 QA, it was first observed at Heidelberg andAlgiers Observatory in 1928, extending the body'sobservation arc by 4 years prior to its official discovery observation.[11]

Physical characteristics

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Rotation period

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American astronomerRichard Binzel and French amateur astronomerRené Roy obtained three rotationallight curves ofMóra from photometric observation taken in 1983 and 2009/11, respectively. Light curve analysis gave a well-definedrotation period between 2.28 and 2.30 hours with a change in brightness of 0.23 to 0.43magnitude (U=3/2+/3).[9][10] The short period is just above the threshold of 2.2 hours for the so-calledfast rotators.

Diameter, albedo and spectral type

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According to the space-based surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Móra measures between 14.72 and 21.47 kilometers in diameter and its surface has analbedo between 0.051 and 0.10.[4][5][6][7][8]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stonyS-type asteroids of 0.20 and derives a shorter diameter of 10.79 kilometers,[3] while Richard Binzel classified it as a carbonaceousC-type asteroid during his photometric observations in the 1980s.[9]

Naming

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Thisminor planet was named in honour of Hungarian astronomer Károly Móra (1899–1938). The official naming citation was mentioned inThe Names of the Minor Planets byPaul Herget in 1955 (H 116). As a curiosity, astronomerPaul Wild reshuffled the letters and numbers of the designation "1257 Mora" to construct a name for his discovery2517 Orma in 1968 (orma also means "trace, track" in Italian).[2]

References

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  1. ^abcdef"JPL Small-Body Database Browser: 1257 Mora (1932 PE)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved26 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1257) Móra".Dictionary of Minor Planet Names – (1257) Móra.Springer Berlin Heidelberg. p. 104.doi:10.1007/978-3-540-29925-7_1258.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1257) Móra". Asteroid Lightcurve Database (LCDB). Retrieved25 January 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. ^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. Retrieved25 January 2017.
  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.S2CID 35447010.
  7. ^abcMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved25 January 2017.
  8. ^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)
  9. ^abcdeBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved25 January 2017.
  10. ^abcBehrend, Raoul."Asteroids and comets rotation curves – (1257) Móra".Geneva Observatory. Retrieved25 January 2017.
  11. ^ab"1257 Mora (1932 PE)".Minor Planet Center. Retrieved25 January 2017.

External links

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