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2197 Shanghai

From Wikipedia, the free encyclopedia
Asteroid

2197 Shanghai
Discovery[1]
Discovered byPurple Mountain Obs.
Discovery sitePurple Mountain Obs.
Discovery date30 December 1965
Designations
(2197) Shanghai
Named after
Shanghai(Chinese city)[2]
1965 YN · 1942 VN
1955 DA · 1964 UN
1967 JT · 1975 SD
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.10 yr (22,682 days)
Aphelion3.5508AU
Perihelion2.7595 AU
3.1551 AU
Eccentricity0.1254
5.60yr (2,047 days)
60.923°
0° 10m 33.24s / day
Inclination2.4980°
56.369°
70.991°
Physical characteristics
Dimensions20.198±0.136 km[1][4]
20.20±0.14 km[3][4]
22.23 km(derived)[3]
23.88±0.70 km[5]
5.9384±0.0023h[6]
5.99±0.05 h[7]
0.0898(derived)[3]
0.106±0.007[5]
0.119±0.014[4]
C[3]
11.20[5] · 11.40[4] · 11.304±0.001(R)[6] · 11.5[1][3] · 11.54±0.19[8]

2197 Shanghai, provisional designation1965 YN, is a carbonaceous Themistianasteroid from the outer region of theasteroid belt, approximately 22 kilometers in diameter.

The asteroid was discovered on 30 December 1965, by astronomers at thePurple Mountain Observatory in Nanjing, China, and named after the city ofShanghai.[2][9]

Orbit and classification

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Shanghai is a member of theThemis family, a dynamical family ofouter-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun at a distance of 2.8–3.6 AU once every 5 years and 7 months (2,047 days). Its orbit has aneccentricity of 0.13 and aninclination of 2° with respect to theecliptic.[1]

Physical characteristics

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The dark body has been characterized as aC-type asteroid.[3]

Rotation period

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In December 2010, a rotationallightcurve ofShanghai was obtained for this asteroid from photometric observations taken at the U.S.Palomar Transient Factory in California. It gave arotation period of5.9384 hours with a brightness variation of 0.16magnitude (U=2).[6]

One month later in January 2011, a similar period of5.99 hours with an amplitude of 0.16 magnitude was derived by French amateur astronomerPierre Antonini (U=2).[7]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Shanghai measures 20.2 and 23.9 kilometers in diameter and its surface has analbedo of 0.119 and 0.106, respectively.[4][5] TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0898 and a diameter of 22.2 kilometers with anabsolute magnitude of 11.5.[3]

Naming

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Thisminor planet is named afterShanghai, the most populous city of China (pop. 24 million as of 2014). Located in theYangtze River Delta in eastern China, it has theworld's busiest container port.[2] The official naming citation was published by theMinor Planet Center on 1 June 1981 (M.P.C. 6059).[10]

References

[edit]
  1. ^abcde"JPL Small-Body Database Browser: 2197 Shanghai (1965 YN)" (2017-03-31 last obs.).Jet Propulsion Laboratory. Retrieved11 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2197) Shanghai".Dictionary of Minor Planet Names – (2197) Shanghai.Springer Berlin Heidelberg. p. 179.doi:10.1007/978-3-540-29925-7_2198.ISBN 978-3-540-00238-3.
  3. ^abcdefgh"LCDB Data for (2197) Shanghai". Asteroid Lightcurve Database (LCDB). Retrieved1 September 2016.
  4. ^abcdeMasiero, 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. Retrieved1 September 2016.
  5. ^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)
  6. ^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. Retrieved1 September 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2197) Shanghai".Geneva Observatory. Retrieved1 September 2016.
  8. ^Veres, 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. Retrieved1 September 2016.
  9. ^"2197 Shanghai (1965 YN)".Minor Planet Center. Retrieved1 September 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved1 September 2016.

External links

[edit]
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