This bright TNO was discovered in 2005 and reobserved during the 2006 and 2007 apparitions. The three-opposition orbit was quite uncertain for searching for images on archival plates from the 1990s. Fortunately, 2005 UQ513 was also predicted to be on NEAT scans from 2001 and 2002 when the uncertainty was smaller, and images were found on seven nights. Stacking of the individual scans from each night helped to show the object more clearly.
With an updated orbit from the 2001 and 2002 astrometry, additional images were found in DSS data from 1990-1992.
The following astrometry was submitted to the Minor Planet Center:
K05Up3Q 1990 09 15.30174 23 11 22.52 +16 37 06.8 261
K05Up3Q 1991 10 03.25035 23 13 14.70 +17 08 00.1 261
K05Up3Q 1992 09 26.28194 23 16 43.07 +17 49 15.8 261
K05Up3Q C2001 08 22.34931 23 48 12.85 +23 37 07.8 20.5 R 644
K05Up3Q C2001 09 21.27441 23 46 08.72 +23 30 37.2 20.4 R 644
K05Up3Q C2001 09 26.20079 23 45 47.49 +23 28 42.4 19.7 R 644
K05Up3Q C2001 09 30.44927 23 45 29.37 +23 26 55.1 19.9 R 644
K05Up3Q C2002 08 22.47770 23 51 36.89 +24 13 41.9 19.6 R 644
K05Up3Q C2002 10 15.19649 23 47 52.99 +23 56 51.3 21.2 R 644
K05Up3Q C2002 11 01.10292 23 46 53.79 +23 47 25.0 20.5 R 644
At the end of this page are the elements and residuals with the new data. The new orbit is much more accurate because the object
has now been observed for 17 years instead of two years. 2005 UQ513 was numbered in December 2008.
View the Discovery Announcement.
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2002 Aug. 22.47770 UTC RA 23h51m36.89s Dec. +24°13'41.9" 3 x 60-second exposure stack Size = 150" x 150" Palomar Mountain/NEAT |
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2001 Sep. 26.20079 UTC RA 23h45m47.49s Dec. +23°28'42.4" 3 x 20-second exposure stack Size = 150" x 150" Palomar Mountain/NEAT |
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1992 Sep. 26.28194 UTC RA 23h16m43.07s Dec. +17°49'15.8" 70-minute exposure Size = 150" x 150" Palomar Mountain-DSS plate XJ677-A16P |
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1991 Oct. 03.25035 UTC RA 23h13m14.70s Dec. +17°08'00.1" 65-minute exposure Size = 150" x 150" Palomar Mountain-DSS plate XJ604-A0OO |
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1990 Sep. 15.30174 UTC RA 23h11m22.52s Dec. +16°37'06.8" 75-minute exposure Size = 150" x 150" Palomar Mountain-DSS plate XP676-A0YI |
Epoch 2007 Oct. 27.0 TT = JDT 2454400.5 MPC M 212.70038 (2000.0) P Q n 0.00346286 Peri. 222.55095 -0.93244179 -0.11252150 T = 2496937.51325 JDT a 43.2692767 Node 307.64850 +0.31031071 -0.73618066 q = 36.9070977 e 0.1470369 Incl. 25.69947 -0.18509342 -0.66736568 P 285 H 3.7 G 0.15 U 3 From 42 observations at 8 oppositions, 1990-2007, mean residual 0".31. Residuals 19900915 675 0.4+ 0.2+ 20051022 644 0.1- 0.2+ 20051130 644 0.0 0.1+ 19911003 675 0.2- 0.1+ 20051022 644 0.2+ 0.2- 20051130 644 0.0 0.1+ 19920926 675 0.3- 0.0 20051023 644 0.2+ 0.1+ 20060915 644 0.5+ 0.1- 20010822 644 0.3- 0.3- 20051023 644 0.4+ 0.1- 20060916 644 0.1+ 0.2+ 20010921 644 0.1+ 0.2+ 20051023 644 0.2+ 0.2+ 20060916 644 0.2- 0.5- 20010926 644 0.1+ 0.6- 20051024 644 0.2+ 0.1+ 20060923 644 0.1- 0.3+ 20010930 644 0.1+ 0.2- 20051024 644 0.3+ 0.2+ 20060925 644 0.0 0.0 20020822 644 0.2- 0.1+ 20051024 644 0.2+ 0.1+ 20060926 644 0.1- 0.1+ 20021015 644 0.9- 0.5+ 20051026 644 0.3+ 0.1+ 20071006 A74 0.0 0.4+ 20021101 644 0.3+ 0.1+ 20051026 644 0.3+ 0.0 20071006 A74 0.1- 0.4+ 20051021 644 0.5+ 0.2- 20051026 644 0.5+ 0.0 20071006 A74 0.4- 1.0+ 20051021 644 0.3+ 0.1- 20051104 644 0.2- 0.3- 20071031 A74 0.4- 0.4- 20051021 644 0.3- 0.2- 20051104 644 0.2- 0.3- 20071031 A74 0.3- 0.2- 20051022 644 0.1+ 0.1- 20051104 644 0.2- 0.3- 20071031 A74 0.8- 0.6-
DSS precovery images are from DSS plate archive scans, which are © copyright California Institute of Technology.
NEAT precovery images are from SkyMorph, which is a NASA Applied Information Systems Research (AISR) funded project.