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: 14UC229
# Created Tue Apr 1 01:10:10 2025
# Orbit generated from Bernstein formalism
# Fitting 39 observations of 39
# Arc: 4.06y
# First observation: 2013/08/09
# Last observation: 2017/08/30
Preliminary a, adot, b, bdot, g, gdot:
-0.000051 0.021441 0.000009 0.000891 0.022648 0.000000
# Chi-squared of fit: 8.19 DOF: 72 RMS: 0.08
# Min/Max residuals: -0.27 0.21
# Exact a, adot, b, bdot, g, gdot:
1.464315E-05 2.135463E-02 7.784597E-07 8.882373E-04 2.262628E-02 2.843122E-03
# Covariance matrix:
1.8859E-13 -8.5435E-14 -6.2542E-16 -2.1526E-15 7.6826E-14 -5.1813E-13
-8.5435E-14 1.5156E-13 -4.1750E-15 6.5311E-15 6.0920E-14 1.8270E-12
-6.2542E-16 -4.1750E-15 1.0050E-13 -4.8094E-14 -4.7319E-15 -6.8190E-14
-2.1526E-15 6.5311E-15 -4.8094E-14 3.6653E-14 3.4212E-15 1.0348E-13
7.6826E-14 6.0920E-14 -4.7319E-15 3.4212E-15 1.5513E-13 1.0639E-12
-5.1813E-13 1.8270E-12 -6.8190E-14 1.0348E-13 1.0639E-12 2.9035E-11
# lat0 lon0 xBary yBary zBary JD0
2.977178 29.338840 0.968787 0.015862 -0.304331 2456514.023888
# Heliocentric elements and errors
Epoch: 2456510.5000 = 2013/08/06
Mean Anomaly: 70.71608 +/- 0.026
Argument of Peri: 327.18757 +/- 0.027
Long of Asc Node: 337.77763 +/- 0.006
Inclination: 3.83887 +/- 0.000
Eccentricity: 0.11084958 +/- 0.0003
Semi-Major Axis: 45.65831419 +/- 0.0042
Time of Perihelion: 2434374.7673 +/- 7.4
Perihelion: 40.59710943 +/- 0.0122
Aphelion: 50.71951896 +/- 0.0125
Period (y) 308.5233 +/- 0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 39.21556960 +/- 0.0007
Ecliptic Y 20.93369029 +/- 0.0004
Ecliptic Z 2.29555299 +/- 0.0000
Ecliptic XDOT -0.00097767 +/- 0.0000
Ecliptic YDOT 0.00241726 +/- 0.0000
Ecliptic ZDOT 0.00012534 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 44.51235617 +/- 0.0006
Geocenter to KBO 44.19639638 +/- 0.0008
# Hcoef: 8.11
The following table shows the complete astrometric record for 14UC229. 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 (14UC229) followed by the observatory code and reference code for the source of the astrometry.
2013 08 09.52311 01 44 46.809 +14 01 18.16 24.2r 14UC229 568 C~2SDi 2013 09 02.44494 01 44 02.563 +13 58 56.44 24.7r 14UC229 568 C~2SDi 2013 09 02.48778 01 44 02.447 +13 58 55.70 24.8r 14UC229 568 C~2SDi 2013 09 03.46375 01 43 59.752 +13 58 44.56 24.8r 14UC229 568 C~2SDi 2013 09 03.51035 01 43 59.620 +13 58 44.11 24.8r 14UC229 568 C~2SDi 2013 10 08.52484 01 41 49.754 +13 48 15.09 25.1r 14UC229 568 C~2SDi 2013 11 01.52560 01 40 03.488 +13 38 30.80 24.1r 14UC229 568 C~2SDi 2013 11 29.26953 01 38 16.312 +13 27 44.29 24.5r 14UC229 568 C~2SDi 2013 12 04.41381 01 38 00.704 +13 26 02.51 24.5r 14UC229 568 C~2SDi 2013 12 05.30424 01 37 58.194 +13 25 46.15 24.1r 14UC229 568 C~2SDi 2014 01 02.26526 01 37 10.019 +13 19 37.61 24.7r 14UC229 568 C~2SDi 2014 07 26.52975 01 49 27.970 +14 29 17.46 25.1r 14UC229 568 C~2SDi 2014 07 26.57298 01 49 27.975 +14 29 17.77 24.8r 14UC229 568 C~2SDi 2014 08 24.54028 01 49 04.072 +14 29 23.85 24.9r 14UC229 568 C~2SDi 2014 08 30.44562 01 48 51.038 +14 28 37.18 25.3r 14UC229 568 C~2SDi 2014 08 30.55222 01 48 50.769 +14 28 36.20 24.8r 14UC229 568 C~2SDi 2014 09 18.47076 01 47 53.248 +14 24 28.71 24.8r 14UC229 568 C~2SDi 2014 09 18.51348 01 47 53.089 +14 24 27.97 24.4r 14UC229 568 C~2SDi 2014 09 23.51179 01 47 34.529 +14 23 00.26 24.4r 14UC229 568 C~2SDi 2014 10 22.30668 01 45 31.833 +14 12 29.55 24.0r 14UC229 568 C~2SDi 2014 10 22.35220 01 45 31.620 +14 12 28.55 24.3r 14UC229 568 C~2SDi 2014 10 22.40142 01 45 31.396 +14 12 27.40 24.4r 14UC229 568 C~2SDi 2014 10 25.51256 01 45 17.474 +14 11 11.17 24.5r 14UC229 568 C~2SDi 2014 11 20.24396 01 43 29.263 +14 00 48.48 24.5r 14UC229 568 C~2SDi 2014 11 20.38425 01 43 28.716 +14 00 45.38 24.1r 14UC229 568 C~2SDi 2014 11 21.44138 01 43 24.756 +14 00 21.09 24.7r 14UC229 568 C~2SDi 2015 02 19.25614 01 42 55.637 +13 52 26.23 24.1r 14UC229 568 C~2SDi 2015 10 09.40974 01 51 11.619 +14 46 39.69 25.0w 14UC229 568 C~2SDi 2015 10 09.42762 01 51 11.540 +14 46 39.37 24.9w 14UC229 568 C~2SDi 2015 10 09.45292 01 51 11.433 +14 46 38.69 24.8w 14UC229 568 C~2SDi 2015 10 09.47042 01 51 11.344 +14 46 38.27 24.8w 14UC229 568 C~2SDi 2015 10 09.51628 01 51 11.151 +14 46 37.39 24.7w 14UC229 568 C~2SDi 2015 10 13.42514 01 50 54.078 +14 45 10.11 14UC229 568 C~2SDi 2015 10 14.47894 01 50 49.414 +14 44 46.09 24.4r 14UC229 568 C~2SDi 2015 10 14.54658 01 50 49.115 +14 44 44.55 14UC229 568 C~2SDi 2015 12 07.40784 01 47 12.510 +14 24 06.08 24.9w 14UC229 568 C~2SDi 2016 09 27.46659 01 56 38.981 +15 18 53.00 24.5w 14UC229 568 C~2SDi 2017 08 25.57304 02 02 57.135 +15 53 14.88 24.9w 14UC229 568 C~2SDi 2017 08 30.59490 02 02 47.027 +15 52 44.10 24.5w 14UC229 568 C~2SDi
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 0.06 0.00 -0.03
2 0.0655 -652.05 0.01 98.05 0.16
3 0.0656 -653.89 -0.04 97.97 -0.11
4 0.0683 -694.51 -0.04 101.62 0.00
5 0.0684 -696.46 0.01 101.88 0.08
6 0.1643 -2687.36 0.06 194.20 0.19
7 0.2300 -4342.84 -0.09 208.60 -0.04
8 0.3059 -6034.87 0.08 173.25 -0.19
9 0.3200 -6284.22 -0.12 161.29 -0.27
10 0.3225 -6324.32 0.04 159.38 0.07
11 0.3990 -7114.13 -0.00 72.28 0.02
12 0.9610 4418.14 0.11 118.54 -0.06
13 0.9611 4418.32 -0.02 118.81 -0.02
14 1.0404 4095.52 -0.06 247.02 0.05
15 1.0566 3901.87 -0.06 270.23 -0.13
16 1.0569 3897.87 -0.10 270.69 -0.13
17 1.1087 3028.55 0.02 334.83 0.02
18 1.1088 3026.13 -0.02 334.96 0.00
19 1.1225 2742.83 0.11 348.52 -0.02
20 1.2013 851.52 0.03 393.30 0.01
21 1.2014 848.27 -0.02 393.47 0.14
22 1.2016 844.81 -0.00 393.55 0.18
23 1.2101 628.48 0.06 394.57 -0.00
24 1.2805 -1064.37 0.10 376.36 0.08
25 1.2809 -1072.91 0.04 376.32 0.21
26 1.2838 -1135.43 -0.10 374.33 -0.04
27 1.5297 -1701.59 -0.04 83.30 -0.04
28 2.1653 6194.14 0.00 565.12 -0.02
29 2.1654 6192.95 0.02 565.22 0.05
30 2.1654 6191.26 0.04 565.13 -0.09
31 2.1655 6189.90 -0.13 565.19 -0.07
32 2.1656 6186.97 0.04 565.35 0.01
33 2.1763 5924.22 0.05 570.55 -0.01
34 2.1792 5852.38 -0.05 571.82 0.02
35 2.1794 5847.78 0.03 571.90 0.01
36 2.3269 2467.04 0.03 523.58 -0.01
37 3.1347 11322.11 -0.09 727.68 0.03
38 4.0439 17189.43 0.04 799.61 0.02
39 4.0577 17040.77 0.00 820.02 -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.
14UC229 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 45.921 45.935 45.908 ecceobj 0.115 0.115 0.114 incobj 3.830 3.830 3.830 qmin 39.841 39.809 39.849 qmax 51.695 51.730 51.625 amean 45.598 45.611 45.585 amin 45.217 45.226 45.204 amax 46.021 46.030 46.004 emean 0.110 0.111 0.110 emin 0.097 0.097 0.097 emax 0.124 0.124 0.123 imean 4.827 4.827 4.827 imin 4.302 4.303 4.303 imax 5.291 5.289 5.289 excite_mean 0.139 0.139 0.138 fracstop 1.000 1.000 1.000 cjmean 3.097 3.097 3.097 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 176.0 176.0 175.9 kozaiamp 180.0 180.0 180.0