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2120 Tyumenia

From Wikipedia, the free encyclopedia
Dark background asteroid

2120 Tyumenia
Shape model ofTyumenia from itslightcurve
Discovery[1]
Discovered byT. Smirnova
Discovery siteCrimean Astrophysical Obs.
Discovery date9 September 1967
Designations
(2120) Tyumenia
Named after
Tyumen Oblast[2]
(Western Siberia)
1967 RM · 1941 WS
1971 KA
main-belt · (outer)[3]
background[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc75.96 yr (27,746 days)
Aphelion3.4494AU
Perihelion2.6682 AU
3.0588 AU
Eccentricity0.1277
5.35yr (1,954 days)
162.29°
0° 11m 3.12s / day
Inclination17.573°
222.46°
75.509°
Physical characteristics
38.619±0.412 km[5]
40.93 km(derived)[3]
41.18±2.4 km[6]
43.65±20.27 km[7]
43.90±0.80 km[8]
47.00±14.23 km[9]
51.485±0.395 km[10]
2.769±0.001 h[11][a]
17.47±0.07 h[12]
17.507±0.006 h[13]
0.029±0.005[10]
0.03±0.02[7]
0.03±0.03[9]
0.0420(derived)[3]
0.064±0.003[8]
0.068±0.003[14]
0.0721±0.009[6]
0.0819±0.0132[5]
C(assumed)[3]
10.40[5][6][8] · 10.90[9][10] · 11.0[1][3] · 11.14[7]

2120 Tyumenia (prov. designation:1967 RM) is a darkbackground asteroid, approximately 45 kilometers (28 miles) in diameter, located in the outer regions of theasteroid belt. It was discovered on 9 September 1967, by Soviet astronomerTamara Smirnova at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean peninsula.[15] The asteroid was named for the now Russian district ofTyumen Oblast in Western Siberia.[2]

Orbit and classification

[edit]

Tyumenia is a non-family asteroid from the main belt'sbackground population.[4] It orbits the Sun in theouter asteroid belt at a distance of 2.7–3.4 AU once every 5 years and 4 months (1,954 days;semi-major axis of 3.06 AU). Its orbit has aneccentricity of 0.13 and aninclination of 18° with respect to theecliptic.[1] The body'sobservation arc begins with its identification as1941 WS atTurku Observatory in November 1941, almost 26 years prior to its official discovery observation at Nauchnyj.[15]

Naming

[edit]

Thisminor planet was named after the district ofTyumen Oblast of the formerRussian Soviet Federative Socialist Republic (1917–1991). Tyumen Oblast is located east of theUral Mountains in Western Siberia, in the center of an oil-gas basin.[2] The region is Russia's largest producer of oil and natural gas. The official naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5283).[16]

Physical characteristics

[edit]

Tyumenia is an assumed carbonaceousC-type asteroid.[3]

Rotation period

[edit]

Three rotationallightcurves ofTyumenia have been obtained from photometric observations since 2004.(U=2/2/2).[11][12][13] The consolidated lightcurve gave a shortrotation period of 2.769 hours with a brightness amplitude between 0.33 and 0.39magnitude.[3][a]

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Tyumenia measures between 38.619 and 51.49 kilometers in diameter and its surface has analbedo between 0.029 and 0.0819.[5][6][7][8][9][10][14] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0420 and a diameter of 40.93 kilometers based on anabsolute magnitude of 11.0.[3]

Notes

[edit]
  1. ^abLightcurve plot of 2120 Tyumenia, Palmer Divide Observatory, B. D. Warner (2004) yxz () web: rotation period2.769±0.001 hours with a brightness amplitude of0.33±0.02 mag. Quality Code of 2. Summary figures at theLCDB

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2120 Tyumenia (1967 RM)" (2017-11-01 last obs.).Jet Propulsion Laboratory. Retrieved5 December 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2120) Tyumenia".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 172.doi:10.1007/978-3-540-29925-7_2121.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (2120) Tyumenia". Asteroid Lightcurve Database (LCDB). Retrieved5 December 2017.
  4. ^ab"Asteroid 2120 Tyumenia – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  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.S2CID 35447010.
  6. ^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.
  7. ^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.
  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. ^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. Retrieved5 December 2017.
  10. ^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.S2CID 46350317. Retrieved5 December 2017.
  11. ^abWarner, Brian D. (March 2005)."Lightcurve analysis for asteroids 242, 893, 921, 1373, 1853, 2120, 2448 3022, 6490, 6517, 7187, 7757, and 18108"(PDF).Minor Planet Bulletin.32 (1):4–7.Bibcode:2005MPBu...32....4W.ISSN 1052-8091. Retrieved18 March 2020.
  12. ^abOliver, Robert Lemke; Shipley, Heath; Ditteon, Richard (October 2008)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2008 March"(PDF).Minor Planet Bulletin.35 (4):149–150.Bibcode:2008MPBu...35..149O.ISSN 1052-8091. Archived fromthe original(PDF) on 17 March 2020. Retrieved18 March 2020.
  13. ^abPligge, Zachary; Hall, Ben; Ditteon, Richard (July 2011)."Asteroid Lightcurve Analysis at the Oakley Observatory: 2010 September thru October"(PDF).Minor Planet Bulletin.38 (3):137–138.Bibcode:2011MPBu...38..137P.ISSN 1052-8091. Retrieved18 March 2020.
  14. ^abMasiero, 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.S2CID 119293330.
  15. ^ab"2120 Tyumenia (1967 RM)".Minor Planet Center. Retrieved5 December 2017.
  16. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved5 December 2017.


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