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1 See also  





2 References  





3 External links  














54598 Bienor






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54598 Bienor
Discovery
Discovered byDES
Discovery siteCerro Tololo Obs.
Discovery date27 August 2000
Designations

MPC designation

(54598) Bienor
Pronunciation/bˈnɔːr/[1]

Named after

Biēnor

Alternative designations

2000 QC243

Minor planet category

Centaur[2]
AdjectivesBienorian /b.ɪˈnɔːriən/
Symbol (astrological)
Orbital characteristics[2]
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 0
Observation arc24775 days (67.83 yr)
Aphelion19.715 AU (2.9493 Tm)
Perihelion13.172 AU (1.9705 Tm)

Semi-major axis

16.444 AU (2.4600 Tm)
Eccentricity0.19894

Orbital period (sidereal)

66.68 yr (24355 d)

Average orbital speed

7.26 km/s

Mean anomaly

318.473°

Mean motion

0° 0m 53.039s / day
Inclination20.745°

Longitude of ascending node

337.728°

Argument of perihelion

153.374°
Earth MOID12.199 AU (1.8249 Tm)
Jupiter MOID7.873 AU (1.1778 Tm)
TJupiter3.575
Physical characteristics

Mean diameter

187.5±15.5 km[3]
198 km[4]
207±30 km[5]

Sidereal rotation period

9.14 h (0.381 d)[2]

Geometric albedo

0.03–0.05[5]
0.05±0.019[3]
Temperature~ 69 K

Spectral type

BR[4]
B–V = 0.711±0.059[6]
V–R = 0.476±0.046[6]

Apparent magnitude

~ 19.2[7]

Absolute magnitude (H)

7.5[2]

54598 Bienor /bˈnɔːr/ is a centaur that grazes the orbit of Uranus. It is named after the mythological centaur Bienor. Its closest approach to the Sun (perihelion) is 13.2 AU.[2] As of 2020, Bienor is 14.2 AU from the Sun[7] and will reach perihelion in January 2028.[2] It measured approximately 198 kilometers (120 miles) in diameter.[4]

See also

[edit]

References

[edit]
  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  • ^ a b c d e f "JPL Small-Body Database Browser: 54598 Bienor (2000 QC243)" (2020-11-11 last obs). Jet Propulsion Laboratory. Retrieved 20 December 2020.
  • ^ a b Bauer, J. M.; Grav, T.; Blauvelt, E.; Mainzer, A. K. (August 2013). "Centaurs and Scattered Disk Objects in the Thermal Infrared: Analysis of WISE/NEOWISE Observations". The Astrophysical Journal. 773 (1): 11. arXiv:1306.1862. Bibcode:2013ApJ...773...22B. doi:10.1088/0004-637X/773/1/22. S2CID 51139703.
  • ^ a b c Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 12 August 2021.
  • ^ a b Stansberry, J.; Grundy, W.; Brown, M.; et al. (2008). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". In Barucci, M. Antonietta (ed.). The Solar System Beyond Neptune. arXiv:astro-ph/0702538.
  • ^ a b Hainaut, O. R.; Boehnhardt, H.; Protopapa, S. (October 2012). "Colours of minor bodies in the outer solar system. II. A statistical analysis revisited". Astronomy and Astrophysics. 546: 20. arXiv:1209.1896. Bibcode:2012A&A...546A.115H. doi:10.1051/0004-6361/201219566. S2CID 54776793. Retrieved 26 September 2019.
  • ^ a b "AstDyS (54598) Bienor Ephemerides". Department of Mathematics, University of Pisa, Italy. Retrieved 20 December 2020.
  • [edit]


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