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: 14UK229
# Created Tue Apr 1 01:10:10 2025
# Orbit generated from Bernstein formalism
# Fitting 40 observations of 40
# Arc: 4.06y
# First observation: 2013/08/08
# Last observation: 2017/08/30
Preliminary a, adot, b, bdot, g, gdot:
0.000001 0.025243 0.000002 0.000009 0.025059 0.000000
# Chi-squared of fit: 19.50 DOF: 74 RMS: 0.12
# Min/Max residuals: -0.37 0.25
# Exact a, adot, b, bdot, g, gdot:
1.596336E-05 2.509943E-02 -8.794355E-07 7.838241E-06 2.487508E-02 1.769388E-03
# Covariance matrix:
1.6268E-13 -5.3706E-14 -1.8152E-15 1.7202E-16 9.4613E-14 -2.0502E-13
-5.3706E-14 1.3688E-13 -7.1343E-16 4.7168E-16 4.7703E-14 1.4792E-12
-1.8152E-15 -7.1343E-16 7.2990E-14 -3.4434E-14 -2.6601E-15 -1.1600E-14
1.7202E-16 4.7168E-16 -3.4434E-14 3.2178E-14 5.2544E-16 6.8659E-15
9.4613E-14 4.7703E-14 -2.6601E-15 5.2544E-16 1.4577E-13 7.5472E-13
-2.0502E-13 1.4792E-12 -1.1600E-14 6.8659E-15 7.5472E-13 2.0950E-11
# lat0 lon0 xBary yBary zBary JD0
2.359168 25.182714 0.950037 0.014834 -0.359109 2456513.088478
# Heliocentric elements and errors
Epoch: 2456510.5000 = 2013/08/06
Mean Anomaly: 37.78953 +/- 0.090
Argument of Peri: 44.99528 +/- 0.111
Long of Asc Node: 295.85150 +/- 0.010
Inclination: 2.33901 +/- 0.000
Eccentricity: 0.06910122 +/- 0.0001
Semi-Major Axis: 42.82697839 +/- 0.0029
Time of Perihelion: 2445764.5796 +/- 25.7
Perihelion: 39.86758175 +/- 0.0068
Aphelion: 45.78637504 +/- 0.0070
Period (y) 280.2750 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 37.07831406 +/- 0.0006
Ecliptic Y 16.38750742 +/- 0.0003
Ecliptic Z 1.65481149 +/- 0.0000
Ecliptic XDOT -0.00100565 +/- 0.0000
Ecliptic YDOT 0.00258188 +/- 0.0000
Ecliptic ZDOT 0.00000902 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.57203685 +/- 0.0005
Geocenter to KBO 40.20088337 +/- 0.0006
# Hcoef: 8.46
The following table shows the complete astrometric record for 14UK229. 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 (14UK229) followed by the observatory code and reference code for the source of the astrometry.
2013 08 08.58770 01 29 49.124 +11 56 22.49 24.2r 14UK229 568 C~2SDj 2013 09 01.51405 01 28 56.886 +11 52 36.45 24.3r 14UK229 568 C~2SDj 2013 09 01.55288 01 28 56.752 +11 52 35.94 25.3r 14UK229 568 C~2SDj 2013 09 02.49556 01 28 53.796 +11 52 21.17 24.8r 14UK229 568 C~2SDj 2013 09 02.54696 01 28 53.634 +11 52 20.11 24.4r 14UK229 568 C~2SDj 2013 09 29.51508 01 27 07.594 +11 42 56.60 24.6r 14UK229 568 C~2SDj 2013 10 03.49165 01 26 49.407 +11 41 14.54 24.8r 14UK229 568 C~2SDj 2013 10 04.58571 01 26 44.333 +11 40 45.93 24.3r 14UK229 568 C~2SDj 2013 10 09.38918 01 26 21.791 +11 38 36.88 24.3r 14UK229 568 C~2SDj 2013 10 30.36505 01 24 42.607 +11 28 51.16 23.9r 14UK229 568 C~2SDj 2013 10 31.35588 01 24 38.062 +11 28 23.33 24.2r 14UK229 568 C~2SDj 2013 11 01.30170 01 24 33.763 +11 27 57.09 23.9r 14UK229 568 C~2SDj 2013 11 01.34074 01 24 33.571 +11 27 55.77 24.7r 14UK229 568 C~2SDj 2013 11 01.42897 01 24 33.151 +11 27 53.41 24.4r 14UK229 568 C~2SDj 2013 11 27.35126 01 22 49.971 +11 16 55.56 24.6r 14UK229 568 C~2SDj 2013 12 03.29403 01 22 31.921 +11 14 52.12 25.3r 14UK229 568 C~2SDj 2013 12 04.33911 01 22 29.041 +11 14 31.94 24.6r 14UK229 568 C~2SDj 2013 12 29.23399 01 21 47.580 +11 09 00.44 24.6r 14UK229 568 C~2SDj 2014 07 25.54031 01 35 23.308 +12 27 36.17 24.6r 14UK229 568 C~2SDj 2014 07 25.58207 01 35 23.308 +12 27 35.95 24.7r 14UK229 568 C~2SDj 2014 08 23.54089 01 34 52.297 +12 26 21.87 24.6r 14UK229 568 C~2SDj 2014 09 18.36363 01 33 28.903 +12 19 31.48 24.6r 14UK229 568 C~2SDj 2014 09 18.40832 01 33 28.728 +12 19 30.54 24.5r 14UK229 568 C~2SDj 2014 09 23.44649 01 33 07.867 +12 17 39.68 24.4r 14UK229 568 C~2SDj 2014 10 22.40934 01 30 53.659 +12 05 05.53 24.4r 14UK229 568 C~2SDj 2014 10 22.44880 01 30 53.462 +12 05 04.45 24.2r 14UK229 568 C~2SDj 2014 10 22.48819 01 30 53.261 +12 05 03.21 24.4r 14UK229 568 C~2SDj 2014 10 23.40059 01 30 48.911 +12 04 37.98 24.2r 14UK229 568 C~2SDj 2014 10 25.26507 01 30 40.062 +12 03 45.58 24.8r 14UK229 568 C~2SDj 2014 11 21.36159 01 28 42.199 +11 51 42.65 24.2r 14UK229 568 C~2SDj 2015 02 18.23136 01 28 42.200 +11 46 35.34 24.5r 14UK229 568 C~2SDj 2015 09 15.51940 01 39 13.041 +12 52 05.49 24.7w 14UK229 568 C~2SDj 2015 09 15.57846 01 39 12.808 +12 52 04.36 24.8w 14UK229 568 C~2SDj 2015 10 09.44415 01 37 29.607 +12 42 53.99 24.8w 14UK229 568 C~2SDj 2015 10 09.48680 01 37 29.402 +12 42 52.90 24.6w 14UK229 568 C~2SDj 2015 10 13.48307 01 37 10.459 +12 41 07.30 14UK229 568 C~2SDj 2015 10 13.54938 01 37 10.133 +12 41 05.46 14UK229 568 C~2SDj 2017 01 31.22024 01 38 28.587 +12 43 46.42 24.5w 14UK229 568 C~2SDj 2017 08 25.59230 01 51 17.508 +13 57 58.13 24.8w 14UK229 568 C~2SDj 2017 08 30.61365 01 51 05.614 +13 57 08.49 24.9w 14UK229 568 C~2SDj
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 -0.00 0.00 0.18
2 0.0655 -796.07 0.15 72.22 0.05
3 0.0656 -798.08 0.05 72.47 0.18
4 0.0682 -843.86 -0.09 74.74 0.03
5 0.0683 -846.47 -0.11 74.63 -0.24
6 0.1422 -2501.64 -0.13 126.22 -0.01
7 0.1531 -2787.62 -0.04 130.33 -0.01
8 0.1561 -2867.46 0.11 131.37 0.03
9 0.1692 -3222.94 -0.19 134.25 -0.37
10 0.2266 -4794.39 0.13 131.89 0.12
11 0.2293 -4866.80 0.06 130.92 -0.01
12 0.2319 -4935.26 0.25 130.09 0.04
13 0.2320 -4938.37 0.01 129.91 -0.12
14 0.2323 -4944.99 -0.10 130.02 0.03
15 0.3033 -6599.47 0.18 85.50 0.06
16 0.3195 -6892.21 -0.27 70.24 0.07
17 0.3224 -6939.10 0.04 67.37 0.02
18 0.3905 -7629.77 0.05 -11.83 0.02
19 0.9609 5246.50 -0.04 -47.08 0.02
20 0.9610 5246.42 -0.29 -47.28 -0.36
21 1.0403 4796.05 0.13 48.78 0.04
22 1.1110 3508.17 -0.07 111.57 0.17
23 1.1111 3505.43 0.03 111.63 0.13
24 1.1249 3180.26 0.10 119.99 0.04
25 1.2042 1072.80 0.16 138.51 -0.04
26 1.2043 1069.71 0.10 138.56 0.01
27 1.2044 1066.51 -0.08 138.49 -0.07
28 1.2069 997.90 -0.06 138.44 0.21
29 1.2120 857.92 -0.05 137.36 -0.05
30 1.2862 -1016.31 -0.11 101.72 -0.21
31 1.5295 -1129.66 -0.21 -183.93 0.21
32 2.1025 8916.84 0.10 107.77 -0.07
33 2.1026 8913.25 0.05 107.94 -0.04
34 2.1680 7304.26 0.03 138.79 -0.01
35 2.1681 7301.06 0.03 138.86 0.01
36 2.1790 7004.09 0.12 140.58 -0.05
37 2.1792 6998.97 0.03 140.59 -0.08
38 3.4815 8129.17 -0.04 -123.89 0.07
39 4.0466 20261.00 -0.02 61.40 0.08
40 4.0603 20079.69 -0.04 75.26 -0.06
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.
14UK229 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.062 43.071 43.053 ecceobj 0.075 0.075 0.075 incobj 2.339 2.339 2.339 qmin 38.760 38.763 38.783 qmax 47.031 46.933 46.987 amean 42.759 42.768 42.749 amin 42.408 42.435 42.412 amax 43.124 43.132 43.107 emean 0.072 0.072 0.071 emin 0.047 0.047 0.047 emax 0.091 0.089 0.091 imean 4.410 4.408 4.405 imin 3.039 3.038 3.026 imax 5.280 5.274 5.279 excite_mean 0.105 0.105 0.105 fracstop 1.000 1.000 1.000 cjmean 3.073 3.073 3.073 libcent 0 -180.0 -180.0 -180.0 libamp 0 -180.0 -180.0 -180.0 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 179.7 180.2 180.4 kozaiamp 180.0 179.9 180.0