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2094 Magnitka

From Wikipedia, the free encyclopedia
Flora asteroid from the inner regions of the asteroid belt

2094 Magnitka
Shape model ofMagnitka from itslightcurve
Discovery[1]
Discovered byCrimean Astrophysical Obs.
Discovery siteCrimean Astrophysical Obs.
Discovery date12 October 1971
Designations
(2094) Magnitka
Named after
Magnitogorsk(Russian city)[2]
1971 TC2 · 1941 WK
1951 WP · 1956 EB
1964 TD · 1968 WE
1977 FG
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc75.36 yr (27,524 days)
Aphelion2.4474AU
Perihelion2.0170 AU
2.2322 AU
Eccentricity0.0964
3.34yr (1,218 days)
149.03°
0° 17m 43.8s / day
Inclination5.0289°
281.93°
251.58°
Physical characteristics
9.91±0.58 km[4]
10.121±0.408 km[5]
12.053±0.055 km[6]
12.167 km[7]
12.17 km(taken)[3]
12.58±1.04 km[8]
12.69±1.1 km[9]
6.11±0.02 h[10]
6.1124±0.0002h[a]
6.24±0.01 h[11]
0.120[3][7]
0.1278±0.0129[6]
0.132±0.025[5]
0.1739±0.035[9]
0.194±0.042[8]
0.285±0.036[4]
S[3]
11.90[8] · 12.0±0.2(R)[a] · 12.0[4][9] · 12.1[1] · 12.45[6] · 12.49±0.206[7] · 12.49[3]

2094 Magnitka (prov. designation:1971 TC2) is aFlora asteroid from the inner regions of theasteroid belt, approximately 12 kilometers (7.5 miles) in diameter. It was discovered on 12 October 1971, at and by theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[12] The discovery has not been attributed to an observing astronomer. It was later named for the city ofMagnitogorsk.[2]

Orbit and classification

[edit]

Magnitka is a member of theFlora family, one of the largest families ofstony asteroids. It orbits the Sun in theinner main-belt at a distance of 2.0–2.4 AU once every 3 years and 4 months (1,218 days). Its orbit has aneccentricity of 0.10 and aninclination of 5° with respect to theecliptic.[1] It was first identified as1941 WK at the FinnishTurku Observatory, extending the body'sobservation arc by 30 years prior to its official discovery observation.[12]

Naming

[edit]

Thisminor planet was named for the city ofMagnitogorsk, Russia, one of the largest centers of metallurgy of the formerSoviet Union.[2] The city is located at the far-east of theUral Mountains, about 250 kilometers southwest of the city ofChelyabinsk in the Chelyabinsk Oblast region, also known for the spectacular air-burst of theChelyabinsk meteor in 2013. The officialnaming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5282).[13]

Physical characteristics

[edit]
Lightcurve-based 3D-model ofMagnitka

Lightcurves

[edit]

In October 2006, two rotationallightcurves forMagnitka were obtained from photometric observations byPetr Pravec at Ondřejov Observatory and by John Menke at his Menke Observatory, respectively. Lightcurve analysis gave a concurringrotation period of 6.11 hours with a brightness variation of 0.80 and 0.86magnitude (U=3-/n.a.), respectively, indicating a non-spheroidal shape forMagnitka.[10][a] In March 2016,Pierre Antonini obtained a tentative lightcurve, which gave a period of 6.24 hours and an amplitude of 0.85 (U=2+).[11]

Diameter and albedo

[edit]

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, the asteroid measures between 9.9 and 12.7 kilometers in diameter and its surface has analbedo between 0.132.[4][5][6][7][8][9] TheCollaborative Asteroid Lightcurve Link agrees with Pravec's revised thermal WISE data,[7] taking an albedo of 0.12, and a diameter of 12.17 kilometers with anabsolute magnitude of 12.49.[3]

Notes

[edit]
  1. ^abcPravec (2006): Observed on 26 January 2006; rotation period of6.1124±0.0002 hours; brightness amplitude of0.86 magnitude; no quality code assessment. Summary figures for (2094) Magnitka atLight Curve Database

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2094 Magnitka (1971 TC2)" (2017-03-26 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2094) Magnitka".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 170.doi:10.1007/978-3-540-29925-7_2095.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2094) Magnitka". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2016.
  4. ^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)
  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. Retrieved7 December 2016.
  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. ^abcdePravec, 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. Retrieved7 December 2016.
  8. ^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. Retrieved7 December 2016.
  9. ^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.
  10. ^abMenke, John; Cooney, Walt; Gross, John; Terrell, Dirk; Higgins, David (October 2008)."Asteroid Lightcurve Analysis at Menke Observatory".The Minor Planet Bulletin.35 (4):155–160.Bibcode:2008MPBu...35..155M.ISSN 1052-8091. Retrieved7 December 2016.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2094) Magnitka".Geneva Observatory. Retrieved1 September 2016.
  12. ^ab"2094 Magnitka (1971 TC2)".Minor Planet Center. Retrieved7 December 2016.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 December 2016.


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