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2127 Tanya

From Wikipedia, the free encyclopedia
Main-belt asteroid

2127 Tanya
Discovery[1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date29 May 1971
Designations
(2127) Tanya
Named after
Tanya Savicheva
(Russian child diarist)[2]
1971 KB1 · 1953 GH1
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc64.14 yr (23,428 days)
Aphelion3.3125AU
Perihelion3.1076 AU
3.2100 AU
Eccentricity0.0319
5.75yr (2,101 days)
343.14°
0° 10m 17.04s / day
Inclination13.094°
106.39°
185.54°
Physical characteristics
Dimensions30.18 km(calculated)[3]
37.736±0.197 km[4]
40.111±0.397 km[5]
41.19±1.05 km[6]
41.43±9.46 km[7]
43.89±16.43 km[8]
7.864±0.0211h[9]
0.03±0.06[8]
0.04±0.03[7]
0.0437±0.0049[5]
0.048±0.007[4]
0.055±0.003[6]
0.057(assumed)[3]
C[3][10]
10.70[6] · 10.70±0.83[10] · 10.879±0.002(R)[9] · 10.90[8] · 11.0[5] · 11.1[1] · 11.15[7] · 11.33[3]

2127 Tanya, provisional designation1971 KB1, is a carbonaceousasteroid from the outer region of theasteroid belt, approximately 40 kilometers in diameter. It was discovered on 29 May 1971, by Russian astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnij, on the Crimean peninsula.[11] It was named in memory ofTanya Savicheva, a Russian child diarist during World War II.[2]

Orbit

[edit]

Tanya is a carbonaceousC-type asteroid, that orbits the Sun in theouter main-belt at a distance of 3.1–3.3 AU once every 5 years and 9 months (2,101 days). Its orbit has aneccentricity of 0.03 and aninclination of 13° with respect to theecliptic.[1] It was first identified as1953 GH1 atGoethe Link Observatory in 1953, extending the body'sobservation arc by 18 years prior to its official discovery at Nauchnij.[11]

Lightcurve

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In October 2013, a rotationallightcurve ofTanya was obtained from photometric observations at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 7.8640 hours with a brightness variation of 0.18magnitude (U=2).[9]

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,Tanya measures between 37.736 and 43.89 kilometers in diameter, and its surface has a lowalbedo between 0.03 and 0.055.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a much smaller diameter of 30.18 kilometers based on anabsolute magnitude of 11.33.[3]

Naming

[edit]

Thisminor planet was named by the discover for the memory of the young Russian girlTanya Savicheva (1930–1944), who died after theSiege of Leningrad (1941–1944) on theEastern Front during World War II. She wrote a well-known diary, describing the death of her parents and other relatives.[2] The approved naming citation was published by theMinor Planet Center on 1 April 1980 (M.P.C. 5283).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2127 Tanya (1971 KB1)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved3 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2127) Tanya".Dictionary of Minor Planet Names – (2127) Tanya.Springer Berlin Heidelberg. p. 172.doi:10.1007/978-3-540-29925-7_2128.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2127) Tanya". Asteroid Lightcurve Database (LCDB). Retrieved27 March 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.S2CID 119293330. Retrieved27 March 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.S2CID 35447010.
  6. ^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)
  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. ^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. Retrieved27 March 2017.
  9. ^abcWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929. Retrieved27 March 2017.
  10. ^abVeres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved27 March 2017.
  11. ^ab"2127 Tanya (1971 KB1)".Minor Planet Center. Retrieved27 March 2017.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 March 2017.

External links

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