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3960 Chaliubieju

From Wikipedia, the free encyclopedia
Main-belt asteroid

3960 Chaliubieju
Discovery[1]
Discovered byPurple Mountain Obs.
Discovery sitePurple Mountain Obs.
Discovery date20 January 1955
Designations
(3960) Chaliubieju
Named after
Cha Liubieju[2]
(friend of a discoverer)
1955 BG · 1984 YZ3
A921 EF
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.45 yr (22,811 days)
Aphelion3.3782AU
Perihelion1.9050 AU
2.6416 AU
Eccentricity0.2788
4.29yr (1,568 days)
217.16°
0° 13m 46.56s / day
Inclination14.414°
84.839°
12.605°
Physical characteristics
Dimensions7.13±1.18 km[4]
8.13±1.44 km[5]
8.997±0.259 km[6]
9.00±0.26 km[6]
14.57 km(calculated)[3]
3.984±0.002h[7]
3.986±0.001 h[8]
0.10(assumed)[3]
0.288±0.030[6]
0.32±0.17[5]
0.34±0.11[4]
S[3]
12.20[5][6] · 12.3[3] · 12.38±0.25[9] · 12.4[1] · 12.57[4]

3960 Chaliubieju, provisional designation1955 BG, is a stonyasteroid from the central regions of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 20 January 1955, by astronomers at thePurple Mountain Observatory in Nanjing, China.[10] The asteroid was named after Cha Liubieju, a friend of one of the discoverers.[2]

Orbit and classification

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Chaliubieju is an asteroid of the main belt'sbackground population that does not belong to any knownasteroid family. It orbits the Sun in thecentral main-belt at a distance of 1.9–3.4 AU once every 4 years and 3 months (1,568 days). Its orbit has aneccentricity of 0.28 and aninclination of 14° with respect to theecliptic.[1]

The asteroid was first identified asA921 EF atBergedorf Observatory in March 1921. The body'sobservation arc begins at Nanjing, two days after its official discovery observation.[10]

Physical characteristics

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Chaliubieju is an assumedS-type asteroid.[3]

Rotation period

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In February 2011, a rotationallightcurve ofChaliubieju was obtained French amateur astronomerPierre Antonini. Lightcurve analysis gave arotation period of 3.986 hours with a brightness variation of 0.27magnitude (U=3).[8] One month later another photometric observation at the Astronomical Research Observatory (H21) gave a concurring period of 3.984 hours and an amplitude of 0.30 magnitude (U=3-).[7]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission ofNASA'sWide-field Infrared Survey Explorer,Chaliubieju measures between 7.13 and 9.00 kilometers in diameter and its surface has analbedo between 0.288 and 0.34,[4][5][6] while theCollaborative Asteroid Lightcurve Link assumes an albedo of 0.10 and calculates a diameter of 14.57 kilometers based on anabsolute magnitude of 12.3.[3]

Naming

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Thisminor planet was named after Cha Liubieju, a friend of one of the discovering astronomers at thePurple Mountain Observatory. Liubieju is noted for her social work with sick and destitute mothers and children in China.[2] The official naming citation was published by theMinor Planet Center on 5 October 1998 (M.P.C. 32787).[11]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 3960 Chaliubieju (1955 BG)" (2017-07-04 last obs.).Jet Propulsion Laboratory. Archived fromthe original on 16 September 2020. Retrieved14 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(3960) Chaliubieju".Dictionary of Minor Planet Names – (3960) Chaliubieju.Springer Berlin Heidelberg. p. 337.doi:10.1007/978-3-540-29925-7_3948.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (3960) Chaliubieju". Asteroid Lightcurve Database (LCDB). Retrieved14 September 2017.
  4. ^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.
  5. ^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. Retrieved14 September 2017.
  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.S2CID 46350317. Retrieved14 September 2017.
  7. ^abLinder, Tyler R.; Sampson, Ryan; Holmes, Robert (January 2013)."Astronomical Research Institute Photometric Results".The Minor Planet Bulletin.40 (1):4–6.Bibcode:2013MPBu...40....4L.ISSN 1052-8091. Retrieved14 September 2017.
  8. ^abBehrend, Raoul."Asteroids and comets rotation curves – (3960) Chaliubieju".Geneva Observatory. Retrieved14 September 2017.
  9. ^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.S2CID 53493339. Retrieved14 September 2017.
  10. ^ab"3960 Chaliubieju (1955 BG)".Minor Planet Center. Retrieved14 September 2017.
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved14 September 2017.

External links

[edit]
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