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2903 Zhuhai

From Wikipedia, the free encyclopedia
Main-belt asteroid

2903 Zhuhai
Discovery[1]
Discovered byPurple Mountain Obs.
Discovery sitePurple Mountain Obs.
Discovery date23 October 1981
Designations
(2903) Zhuhai
Named after
Zhuhai[1](Chinese city)
1981 UV9 · 1955 MC
1973 UK4 · 1975 GC
1977 TN7 · 1977 VL2
main-belt[1][2] · (middle)
background[3] · Maria[4][5]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc62.44yr (22,808 d)
Aphelion2.7128AU
Perihelion2.4104 AU
2.5616 AU
Eccentricity0.0590
4.10 yr (1,497 d)
236.34°
0° 14m 25.44s / day
Inclination14.350°
232.57°
243.97°
Physical characteristics
13.58±0.90 km[6]
13.581±0.896 km[6]
14.01±0.86 km[7]
5.263±0.002 h[8]
5.268±0.003 h[9]
6.152 h[4]
0.146±0.020[7]
0.20(assumed)[10]
0.276±0.141[6]
S[10][11]
11.35[6]
11.60±0.40[11]
11.7[2][10]
12.00[7]

2903 Zhuhai, provisional designation1981 UV9, is a stony background or Marianasteroid from the central regions of theasteroid belt, approximately 14 kilometers (8.7 miles) in diameter. It was discovered on 23 October 1981, by astronomers atPurple Mountain Observatory near Nanjing, China.[1] TheS-type asteroid has arotation period of 5.26 hours.[10] It was named for the Chinese city ofZhuhai.[1]

Orbit and classification

[edit]

Based on osculating Keplerianorbital elements,Zhuhai has also been classified as a member of theMaria family (506), a largefamily of stony asteroids, named after170 Maria.[4] When applying thehierarchical clustering method to itsproper orbital elements, the asteroid is both a non-family asteroid of the main belt'sbackground population (according to Nesvorný),[3] as well as a core member of the Maria family (according to Milani and Knežević).[5]

It orbits the Sun in thecentral main-belt at a distance of 2.4–2.7 AU once every 4 years and 1 month (1,497 days;semi-major axis of 2.56 AU). Its orbit has aneccentricity of 0.06 and aninclination of 14° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1955 MC atGoethe Link Observatory in June 1955, or 26 years prior to its official discovery observation at Nanjing.[1]

Physical characteristics

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Zhuhai has been characterized as a common, stonyS-type asteroid byPan-STARRS photometric survey.[10][11]

Rotation period

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Until 2012, three rotationallightcurves ofZhuhai have been obtained fromphotometric observations.[8][9][4] Best-rated lightcurve from theOakley Southern Sky Observatory gave a well-definedrotation period of 5.263 hours with a brightness amplitude of 0.32magnitude (U=3).[8][10]

Diameter and albedo

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According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Zhuhai measures between 13.58 and 14.01 kilometers in diameter and its surface has analbedo between 0.146 and 0.276.[6][7] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 13.58 kilometers based on anabsolute magnitude of 11.7.[10]

Naming

[edit]

Thisminor planet was named after the city of located in theGuangdong province of southern China.[1] The official naming citation was published by theMinor Planet Center on 11 March 1990 (M.P.C. 16041).[12]

References

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  1. ^abcdefg"2903 Zhuhai (1981 UV9)".Minor Planet Center. Retrieved27 April 2018.
  2. ^abcd"JPL Small-Body Database Browser: 2903 Zhuhai (1981 UV9)" (2017-11-25 last obs.).Jet Propulsion Laboratory. Retrieved27 April 2018.
  3. ^ab"Small Bodies Data Ferret".Nesvorny HCM Asteroid Families V3.0. Archived fromthe original on 2 August 2017. Retrieved27 April 2018.
  4. ^abcdAlvarez-Candal, Alvaro; Duffard, René; Angeli, Cláudia A.; Lazzaro, Daniela; Fernández, Silvia (December 2004). "Rotational lightcurves of asteroids belonging to families".Icarus.172 (2):388–401.Bibcode:2004Icar..172..388A.doi:10.1016/j.icarus.2004.06.008.
  5. ^ab"Asteroid 2903 Zhuhai – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved29 October 2019.
  6. ^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.
  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 catalog
  8. ^abcMoravec, Patricia; Cochren, Joseph; Gerhardt, Michael; Harris, Andrew; Karnemaat, Ryan; Melton, Elizabeth; et al. (October 2012). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2012 January-April".The Minor Planet Bulletin.39 (4):213–216.Bibcode:2012MPBu...39..213M.ISSN 1052-8091.
  9. ^abLi, Bin; Zhao, Haibin; Yao, Jingshen (October 2011). "The Lightcurve Analysis of Five Asteroids".The Minor Planet Bulletin.38 (4):179–180.Bibcode:2011MPBu...38..179L.ISSN 1052-8091.
  10. ^abcdefg"LCDB Data for (2903) Zhuhai". Asteroid Lightcurve Database (LCDB). Retrieved27 April 2018.
  11. ^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.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved27 April 2018.

External links

[edit]
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