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2169 Taiwan

From Wikipedia, the free encyclopedia
Astridian asteroid

2169 Taiwan
Discovery[1]
Discovered byPurple Mountain Obs.
Discovery sitePurple Mountain Obs.
Discovery date9 November 1964
Designations
(2169) Taiwan
Named after
Taiwan[2]
1964 VP1 · 1938 DV1
1975 BH1 · 1977 RF8
1979 FG
main-belt · (middle)[3]
Astrid[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc79.28 yr (28,957 days)
Aphelion2.9244AU
Perihelion2.6564 AU
2.7904 AU
Eccentricity0.0480
4.66yr (1,703 days)
116.98°
0° 12m 41.4s / day
Inclination1.5286°
71.855°
358.45°
Physical characteristics
Dimensions14.39 km(calculated)[3]
16.52±4.57 km[5]
17.96±4.92 km[6]
18.22±0.51 km[7]
18.39±0.30 km[8]
19.263±0.139 km[9][10]
7.252±0.0014h[11]
0.042±0.006[9]
0.0423±0.0059[10]
0.05±0.06[5]
0.05±0.07[6]
0.057(assumed)[3]
0.057±0.015[8]
0.085±0.005[7]
SMASS =C[1] · C[3][12]
12.00[7] · 12.40[8] · 12.488±0.003(R)[11] · 12.50[6][10] · 12.59±0.32[12] · 12.6[1] · 12.69[5] · 12.94[3]

2169 Taiwan, provisional designation1964 VP1, is a carbonaceous Astridianasteroid from the central regions of theasteroid belt, approximately 17 kilometers in diameter. It was discovered on 9 November 1964, by astronomers at thePurple Mountain Observatory near Nanking, China.[13] It was named forTaiwan.[2]

Orbit and classification

[edit]

Taiwan is a member of theAstrid family (515), a smallerasteroid family of nearly 500 carbonaceous asteroids. The family is located in the outermost central main-belt, near a prominentKirkwood gap, that marks the 5:2orbital resonance with Jupiter, and divides the asteroid belt into a central and outer part.[4][14][15]: 23 

Taiwan orbits the Sun at a distance of 2.7–2.9 AU once every 4 years and 8 months (1,703 days). Its orbit has aneccentricity of 0.05 and aninclination of 2° with respect to theecliptic.[1]

The body'sobservation arc begins with its first identification as1938 DV1 atHeidelberg Observatory in February 1938, almost 27 years prior to its official discovery observation at Nanking.[13]

Physical characteristics

[edit]

In theSMASS classification, and according toPanSTARRS photometric survey,Taiwan is a carbonaceousC-type asteroid.[1][12]

Rotation period

[edit]

In September 2010, a rotationallightcurve ofTaiwan was obtained from photometric observations in the R-band by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of 7.252 hours with a brightness variation of 0.17magnitude (U=2).[11]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Taiwan measures between 16.52 and 19.263 kilometers in diameter and its surface has analbedo between 0.042 and 0.085.[5][6][7][8][9][10]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 14.39 kilometers based on anabsolute magnitude of 12.94.[3]

Naming

[edit]

Thisminor planet was named after theTaiwan Province.[2] The official naming citation was published by theMinor Planet Center on 1 February 1980 (M.P.C. 5184).[16]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2169 Taiwan (1964 VP1)" (2017-06-05 last obs.).Jet Propulsion Laboratory. Retrieved4 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2169) Taiwan".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 176.doi:10.1007/978-3-540-29925-7_2170.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2169) Taiwan". Asteroid Lightcurve Database (LCDB). Retrieved4 September 2017.
  4. ^ab"Asteroid 2169 Taiwan – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  5. ^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.
  6. ^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. Retrieved4 September 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. ^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. Retrieved4 September 2017.
  9. ^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. Retrieved4 September 2017.
  10. ^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.
  11. ^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. Retrieved4 September 2017.
  12. ^abcVeres, 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. Retrieved4 September 2017.
  13. ^ab"2169 Taiwan (1964 VP1)".Minor Planet Center. Retrieved4 September 2017.
  14. ^Vokrouhlický, D.; Broz, M.; Bottke, W. F.; Nesvorný, D.; Morbidelli, A. (May 2006)."Yarkovsky/YORP chronology of asteroid families"(PDF).Icarus.182 (1):118–142.Bibcode:2006Icar..182..118V.doi:10.1016/j.icarus.2005.12.010. Retrieved4 September 2017.
  15. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 978-0-8165-3213-1.
  16. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved4 September 2017.

External links

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