The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.
# Object: 11UZ410
# Created Fri Nov 22 02:09:13 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 33 observations of 33
# Arc: 9.27y
# First observation: 2004/09/15
# Last observation: 2013/12/24
# Chi-squared of fit: 14.07 DOF: 60 RMS: 0.12
# Min/Max residuals: -0.39 0.22
# Exact a, adot, b, bdot, g, gdot:
1.671308E-05 2.845345E-02 3.597357E-07 2.519261E-04 2.728308E-02 3.642147E-03
# Covariance matrix:
4.8936E-13 -1.2947E-13 4.2500E-16 -6.4746E-16 -6.2542E-14 -3.0187E-13
-1.2947E-13 1.1088E-13 -3.3398E-16 8.4663E-16 6.2756E-14 4.3395E-13
4.2500E-16 -3.3398E-16 4.3421E-13 -5.5431E-14 -1.8773E-15 -4.3007E-16
-6.4746E-16 8.4663E-16 -5.5431E-14 7.9082E-15 8.6618E-16 3.3633E-15
-6.2542E-14 6.2756E-14 -1.8773E-15 8.6618E-16 1.9595E-13 1.7237E-13
-3.0187E-13 4.3395E-13 -4.3007E-16 3.3633E-15 1.7237E-13 1.8825E-12
# lat0 lon0 xBary yBary zBary JD0
3.883395 20.686075 0.473237 0.060493 -0.890018 2453263.846029
# Heliocentric elements and errors
Epoch: 2453264.5000 = 2004/09/16
Mean Anomaly: 61.13115 +/- 0.015
Argument of Peri: 7.11663 +/- 0.020
Long of Asc Node: 298.58836 +/- 0.003
Inclination: 3.83450 +/- 0.000
Eccentricity: 0.12249335 +/- 0.0001
Semi-Major Axis: 39.37899371 +/- 0.0026
Time of Perihelion: 2437937.5603 +/- 4.1
Perihelion: 34.55532901 +/- 0.0031
Aphelion: 44.20265842 +/- 0.0035
Period (y) 247.1184 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 35.20835622 +/- 0.0006
Ecliptic Y 12.79180366 +/- 0.0002
Ecliptic Z 2.48237969 +/- 0.0000
Ecliptic XDOT -0.00067078 +/- 0.0000
Ecliptic YDOT 0.00279237 +/- 0.0000
Ecliptic ZDOT 0.00005008 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 37.54218479 +/- 0.0005
Geocenter to KBO 36.65271032 +/- 0.0006
# Hcoef: 8.31
The following table shows the complete astrometric record for 11UZ410. The first three columns show the date of observation. The next six columns are RA and DEC. The next column (when provided) is the observed magnitude and filter. The next column is the object name (11UZ410) followed by the observatory code and reference code for the source of the astrometry.
2004 09 15.345286 01 10 28.39 +11 40 23.4 23.4V 11UZ410 645 C~1Rej 2004 09 15.346115 01 10 28.39 +11 40 23.4 23.3V 11UZ410 645 C~1Rej 2004 09 15.348603 01 10 28.38 +11 40 23.4 23.6V 11UZ410 645 C~1Rej 2011 08 30.53207 01 53 59.519 +15 50 15.74 24.7r 11UZ410 568 C~1C6M 2011 08 30.57849 01 53 59.376 +15 50 15.24 24.3r 11UZ410 568 C~1C6M 2011 09 05.58010 01 53 42.121 +15 49 13.14 24.5r 11UZ410 568 C~1C6M 2011 10 25.37276 01 49 58.595 +15 31 08.87 11UZ410 568 C~1C6M 2011 10 25.37795 01 49 58.565 +15 31 08.67 11UZ410 568 C~1C6M 2011 10 25.42724 01 49 58.308 +15 31 07.43 11UZ410 568 C~1C6M 2011 10 25.42724 01 49 58.27 +15 31 07.2 11UZ410 568 C~3j8g 2011 10 25.48711 01 49 57.981 +15 31 05.64 24.2r 11UZ410 568 C~1C6M 2011 10 26.27825 01 49 53.927 +15 30 43.05 24.0r 11UZ410 568 C~1C6M 2011 10 26.27825 01 49 53.91 +15 30 43.2 24.1r 11UZ410 568 C~3j8g 2011 10 26.33093 01 49 53.644 +15 30 41.57 24.0r 11UZ410 568 C~1C6M 2011 10 26.33093 01 49 53.63 +15 30 41.7 24.1r 11UZ410 568 C~3j8g 2011 10 26.37414 01 49 53.40 +15 30 40.4 23.9r 11UZ410 568 C~3j8g 2011 10 31.27710 01 49 28.226 +15 28 19.33 24.0r 11UZ410 568 C~1C6M 2011 10 31.37984 01 49 27.693 +15 28 16.54 24.7r 11UZ410 568 C~1C6M 2011 11 24.27071 01 47 34.744 +15 16 59.86 24.0r 11UZ410 568 C~1C6M 2011 11 28.42497 01 47 17.888 +15 15 10.96 11UZ410 568 C~1C6M 2011 11 30.31655 01 47 10.620 +15 14 22.77 24.6r 11UZ410 568 C~1C6M 2012 01 26.29717 01 46 01.302 +15 02 16.10 24.3r 11UZ410 568 C~1C6M 2012 08 17.57288 02 00 24.713 +16 22 52.76 24.1r 11UZ410 568 C~1C6M 2012 08 24.53062 02 00 12.830 +16 22 30.94 23.9r 11UZ410 568 C~1C6M 2012 10 17.37393 01 56 41.002 +16 06 58.11 24.2r 11UZ410 568 C~1C6M 2013 02 03.26646 01 52 12.103 +15 34 56.92 24.0r 11UZ410 568 C~1C6M 2013 10 29.50257 02 01 43.76 +16 33 13.0 11UZ410 568 C~1C6M 2013 10 29.52988 02 01 43.62 +16 33 12.3 11UZ410 568 C~1C6M 2013 12 23.24828 01 58 01.99 +16 10 29.1 11UZ410 568 C~1C6M 2013 12 23.28018 01 58 01.92 +16 10 28.7 11UZ410 568 C~1C6M 2013 12 24.27043 01 57 59.88 +16 10 12.0 11UZ410 568 C~1C6M 2013 12 24.30685 01 57 59.80 +16 10 11.4 11UZ410 568 C~1C6M 2013 12 24.33872 01 57 59.74 +16 10 10.8 11UZ410 568 C~1C6M
The following table shows the residuals to the orbit fit. The first coumn is the point number. The second column is the time, in years, measured from the first observation. The third and fifth columns are the regularized positions used in the orbit fit. The fourth and sixth columns are the residuals, in arc seconds, for RA and Dec respectively.
1 0.0000 0.00 -0.03 0.00 -0.06
2 0.0000 0.00 0.03 0.00 -0.04
3 0.0000 0.00 0.05 0.00 0.02
4 6.9547 0.00 -0.02 0.00 0.14
5 6.9548 0.00 -0.27 0.00 0.05
6 6.9712 0.00 0.11 0.00 -0.06
7 7.1075 0.00 0.19 0.00 0.04
8 7.1076 0.00 0.14 0.00 -0.01
9 7.1077 0.00 -0.39 0.00 -0.08
10 7.1077 0.00 0.18 0.00 0.15
11 7.1078 0.00 -0.00 0.00 0.07
12 7.1100 0.00 -0.06 0.00 0.18
13 7.1100 0.00 0.19 0.00 0.03
14 7.1102 0.00 -0.12 0.00 0.17
15 7.1102 0.00 0.09 0.00 0.04
16 7.1103 0.00 -0.17 0.00 0.10
17 7.1237 0.00 -0.03 0.00 -0.07
18 7.1240 0.00 -0.02 0.00 0.09
19 7.1894 0.00 0.17 0.00 -0.07
20 7.2008 0.00 -0.11 0.00 -0.06
21 7.2059 0.00 -0.06 0.00 -0.17
22 7.3619 0.00 -0.09 0.00 -0.19
23 7.9212 0.00 -0.10 0.00 -0.14
24 7.9403 0.00 0.02 0.00 -0.01
25 8.0877 0.00 -0.01 0.00 -0.15
26 8.3858 0.00 0.04 0.00 0.22
27 9.1202 0.00 0.06 0.00 -0.08
28 9.1203 0.00 0.12 0.00 -0.01
29 9.2701 0.00 0.01 0.00 -0.14
30 9.2702 0.00 0.01 0.00 0.00
31 9.2729 0.00 -0.03 0.00 0.00
32 9.2730 0.00 -0.08 0.00 0.01
33 9.2731 0.00 0.02 0.00 -0.05
The following table comes from a 10My integration of the orbit of the object. Three columns are shown. The first column is the result of integrating the nominal orbit. The other two columns are based on clones of the nominal orbit that are +/- 3 sigma from the nominal orbit. If all three types agree then the classificiation is deemed secure. The basis for these calculations is described in more detail in AJ, 129, 1117 (2005). Any use made of these calculations should refer to and credit this publication and the Deep Ecliptic Survey Team.
11UZ410 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.849 39.850 39.849 ecceobj 0.127 0.127 0.127 incobj 3.833 3.833 3.833 qmin 33.819 33.817 33.822 qmax 45.599 45.597 45.600 amean 39.459 39.459 39.459 amin 39.059 39.060 39.059 amax 39.915 39.918 39.912 emean 0.122 0.122 0.122 emin 0.103 0.103 0.103 emax 0.143 0.143 0.143 imean 5.519 5.520 5.518 imin 4.805 4.808 4.802 imax 6.232 6.232 6.231 excite_mean 0.155 0.155 0.155 fracstop 1.000 1.000 1.000 cjmean 3.024 3.024 3.024 libcent 0 179.1 179.3 179.3 libamp 0 75.9 76.3 75.8 libcent 1 -180.0 -180.0 -180.0 libamp 1 -180.0 -180.0 -180.0 libcent 2 -180.0 -180.0 -180.0 libamp 2 -180.0 -180.0 -180.0 libcent 3 -180.0 -180.0 -180.0 libamp 3 -180.0 -180.0 -180.0 libcent 4 -180.0 -180.0 -180.0 libamp 4 -180.0 -180.0 -180.0 kozaimean 181.5 181.7 181.7 kozaiamp 180.0 180.0 180.0