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229762 Gǃkúnǁʼhòmdímà

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(229762) 2007 UK126
2007 UK126 photographed by the UK Schmidt Telescope (Precovery, 1997)).
(229762) 2007 UK126 photographed by the UK Schmidt Telescope.
Discovery[1]
Discovered byM. E. Schwamb
M. E. Brown
D. L. Rabinowitz
Discovery date19 October 2007
Designations
(229762) 2007 UK126
Scat-ext[2][3]
Orbital characteristics[4]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 2
Observation arc12117 days (33.17 yr)
Aphelion109.7388 AU (16.41669 Tm) (Q)
Perihelion37.4839 AU (5.60751 Tm) (q)
73.6114 AU (11.01211 Tm) (a)
Eccentricity0.49079 (e)
631.58 yr (230683 d)
342.70708° (M)
0° 0m 5.618s / day (n)
Inclination23.34333° (i)
131.26955° (Ω)
346.58117° (ω)
Known satellites1[5][6]
Earth MOID36.5042 AU (5.46095 Tm)
Jupiter MOID32.2457 AU (4.82389 Tm)
TJupiter6.088
Physical characteristics
Dimensions648+60
−46
[7]
599±77 km[6]
612 km[8]
Mean density
<1.74 g/cm3[7]
11.05 h (0.460 d)
0.167+0.058
−0.038
[6]
20.8[1]
3.69±0.10[6]
3.5[4]

(229762) 2007 UK126, also written as (229762) 2007 UK126, is a scattered disc object (SDO) with a bright absolute magnitude of 3.7.[6] This makes it probably a dwarf planet. As of August 2011, Mike Brown lists it as highly likely a dwarf planet.[9] Its light-curve amplitude is estimated to be Δm=0.111 mag.[10]

Its orbital eccentricity of 0.49 suggests that it was gravitationally scattered onto its eccentric orbit. It will come to perihelion in February 2046.[4]

It has been observed 73 times over 11 oppositions with precovery images back to 1982.[4]

Satellite

It has been reported that (229762) 2007 UK126 has a satellite, but a mass estimate has not been made.[6] The magnitude difference between the primary and the satellite is 3.79 mag. The satellite has a tentative diameter of 139 km, a semi-major axis of 3600 km, and an orbital period of 3.7 d.[5]

See also

References

  1. ^ a b "2007 UK126". Minor Planet Electronic Circ., 2008-D38 (2008). Bibcode:2008MPEC....D...38S. Retrieved 2008-07-11. {{cite journal}}: Cite journal requires |journal= (help)
  2. ^ Marc W. Buie (2012-05-08). "Orbit Fit and Astrometric record for 229762". SwRI (Space Science Department). Retrieved 2012-05-07.
  3. ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2012-05-07.
  4. ^ a b c d "JPL Small-Body Database Browser: 229762 (2007 UK126)" (2013-12-01 last obs and observation arc=31 years). Retrieved 7 April 2016.
  5. ^ a b (229762) 2007 UK126, Johnston's Archive. Last updated 20 September 2011
  6. ^ a b c d e f Santos-Sanz, P.; Lellouch, E.; Fornasier, S.; Kiss, C.; Pal, A.; Müller, T. G.; Vilenius, E.; Stansberry, J.; Mommert, M.; Delsanti, A.; Mueller, M.; Peixinho, N.; Henry, F.; Ortiz, J. L.; Thirouin, A.; Protopapa, S.; Duffard, R.; Szalai, N.; Lim, T.; Ejeta, C.; Hartogh, P.; Harris, A. W.; Rengel, M. (2012). ""TNOs are Cool": A survey of the trans-Neptunian region IV. Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel-PACS". Astronomy & Astrophysics. 541: A92. arXiv:1202.1481. Bibcode:2012A&A...541A..92S. doi:10.1051/0004-6361/201118541.
  7. ^ a b Results from the 2014 November 15th multi-chord stellar occultation by the TNO (229762) 2007 UK126, 2016.
  8. ^ Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)" Archived October 18, 2011, at the Wayback Machine
  9. ^ Michael E. Brown (May 7, 2012). "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Archived from the original on 2011-10-18. Retrieved 2012-05-07. {{cite web}}: Unknown parameter |deadurl= ignored (|url-status= suggested) (help)
  10. ^ Roland, S., Bruzzone, S., Nowajewski, P., Tancredi, G., Barrera, L., Martinez, M., Troncoso, P., & Vasquez, S. (2009). Lightcurves of Icy “Dwarf Planets” (Plutoids)