54598 Bienor 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]
54598 Bienor|
| Discovered by | DES |
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| Discovery site | Cerro Tololo Obs. |
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| Discovery date | 27 August 2000 |
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MPC designation | (54598) Bienor |
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| Pronunciation | [3] |
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Named after | Biānor[1] |
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Alternative designations | 2000 QC243 |
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Minor planet category | Centaur [2] |
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| Adjectives | Bienorian |
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| Epoch 31 May 2020 (JD 2459000.5) |
| Uncertainty parameter 0 |
| Observation arc | 24775 days (67.83 yr) |
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| Aphelion | 19.715 AU (2.9493 Tm) |
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| Perihelion | 13.172 AU (1.9705 Tm) |
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Semi-major axis | 16.444 AU (2.4600 Tm) |
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| Eccentricity | 0.19894 |
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Orbital period | 66.68 yr (24355 d) |
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Average orbital speed | 7.26 km/s |
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Mean anomaly | 318.473° |
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Mean motion | 0° 0m 53.039s / day |
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| Inclination | 20.745° |
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Longitude of ascending node | 337.728° |
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Argument of perihelion | 153.374° |
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| Earth MOID | 12.199 AU (1.8249 Tm) |
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| Jupiter MOID | 7.873 AU (1.1778 Tm) |
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| TJupiter | 3.575 |
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|
| Dimensions | 207±30 km[4] 187.5±15.5 km[5] |
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Sidereal rotation period | 9.14 h (0.381 d)[2] |
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Geometric albedo | 0.03–0.05[4] 0.05±0.019[5] |
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| Temperature | ~ 69 K |
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Spectral type | B–V = 0.711±0.059[6] V–R = 0.476±0.046[6] |
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Apparent magnitude | ~ 19.2[7] |
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Absolute magnitude (H) | 7.5[2] |
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