astro.wikisort.org - Asteroid 2006 HJ123 (also written 2006 HJ123) is a trans-Neptunian object (TNO). It was discovered in 2006 by Marc W. Buie. The object is a plutino (in 2:3 resonance with Neptune).[2]
(469987) 2006 HJ123|
Discovered by | Marc W. Buie |
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Discovery date | 27 April 2006 |
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Alternative designations | 2006 HJ123 |
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Minor planet category | TNO (plutino)[2] |
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Epoch 13 January 2016 (JD 2457400.5) |
Uncertainty parameter 3 |
Observation arc | 1838 days (5.03 yr) |
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Aphelion | 51.444 AU (7.6959 Tm) |
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Perihelion | 27.626 AU (4.1328 Tm) |
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Semi-major axis | 39.535 AU (5.9144 Tm) |
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Eccentricity | 0.30123 |
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Orbital period (sidereal) | 248.59 yr (90798.1 d) |
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Mean anomaly | 309.05° |
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Mean motion | 0° 0m 14.273s /day |
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Inclination | 12.433° |
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Longitude of ascending node | 222.53° |
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Time of perihelion | ≈ 26 April 2051[4] ±1 days |
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Argument of perihelion | 101.59° |
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Earth MOID | 26.636 AU (3.9847 Tm) |
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Jupiter MOID | 22.7401 AU (3.40187 Tm) |
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Dimensions | 283.1+142.3 −110.8 km[5] |
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Geometric albedo | 0.136+0.308 −0.089[5] |
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Temperature | ~44 K |
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Absolute magnitude (H) | 5.32 ± 0.66,[5] 5.7[3] |
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Physical properties
The size of 2006 HJ123 was measured by the Herschel Space Telescope to be 283+142
−111 km.[5]
References
- "List Of Transneptunian Objects". IAU Minor Planet Center. Retrieved 14 May 2012.
- Marsden, Brian G. (11 June 2006). "MPEC 2006-L50 : 2006 HF123, 2006 HG123, 2006 HH123, 2006 HJ123". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Retrieved 14 May 2012.
- "JPL Small-Body Database Browser: (2006 HJ123)" (2012-05-14 last obs). Retrieved 30 March 2016.
- JPL Horizons Observer Location: @sun (Perihelion occurs when deldot changes from negative to positive. Uncertainty in time of perihelion is 3-sigma.)
- Mommert, Michael; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E.; Müller, T. G.; Peixinho, N.; Lellouch, E.; Szalai, N.; Henry, F.; Duffard, R.; Fornasier, S.; Hartogh, P.; Mueller, M.; Ortiz, J. L.; Protopapa, S.; Rengel, M.; Thirouin, A. (May 2012). "TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel-PACS observations". Astronomy & Astrophysics. 541: A93. arXiv:1202.3657. Bibcode:2012A&A...541A..93M. doi:10.1051/0004-6361/201118562.
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