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: 14UW229
# Created Sun Dec 22 02:10:08 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 33 observations of 33
# Arc: 11.17y
# First observation: 2013/09/01
# Last observation: 2024/11/01
# Chi-squared of fit: 15.43 DOF: 60 RMS: 0.12
# Min/Max residuals: -0.40 0.30
# Exact a, adot, b, bdot, g, gdot:
1.150338E-05 1.478310E-02 4.194576E-06 3.651834E-03 1.897323E-02 -1.670756E-03
# Covariance matrix:
3.3787E-13 -5.6816E-14 7.7112E-15 -1.4098E-14 2.5522E-13 -3.1147E-13
-5.6816E-14 1.0544E-13 -1.9142E-14 2.8151E-14 2.8860E-14 6.4436E-13
7.7112E-15 -1.9142E-14 6.2322E-14 -1.3430E-14 -7.0728E-15 -1.2212E-13
-1.4098E-14 2.8151E-14 -1.3430E-14 1.2292E-14 7.5000E-15 1.7961E-13
2.5522E-13 2.8860E-14 -7.0728E-15 7.5000E-15 2.9156E-13 1.8347E-13
-3.1147E-13 6.4436E-13 -1.2212E-13 1.7961E-13 1.8347E-13 4.1112E-12
# lat0 lon0 xBary yBary zBary JD0
4.433054 24.847600 0.725704 0.054381 -0.700749 2456537.034238
# Heliocentric elements and errors
Epoch: 2456536.5000 = 2013/09/01
Mean Anomaly: 234.01953 +/- 0.038
Argument of Peri: 157.44867 +/- 0.030
Long of Asc Node: 7.00746 +/- 0.000
Inclination: 14.61284 +/- 0.000
Eccentricity: 0.16996263 +/- 0.0001
Semi-Major Axis: 47.85577762 +/- 0.0045
Time of Perihelion: 2498852.1206 +/- 16.9
Perihelion: 39.72208384 +/- 0.0064
Aphelion: 55.98947141 +/- 0.0074
Period (y) 331.0623 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 48.62592647 +/- 0.0014
Ecliptic Y 21.72089612 +/- 0.0006
Ecliptic Z 4.07409759 +/- 0.0001
Ecliptic XDOT -0.00115766 +/- 0.0000
Ecliptic YDOT 0.00181653 +/- 0.0000
Ecliptic ZDOT 0.00050689 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 53.41240767 +/- 0.0013
Geocenter to KBO 52.70593606 +/- 0.0015
# Hcoef: 6.91
The following table shows the complete astrometric record for 14UW229. 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 (14UW229) followed by the observatory code and reference code for the source of the astrometry.
2013 09 01.53346 01 25 23.858 +13 44 34.20 24.3r 14UW229 568 C~2SDl 2013 09 01.57230 01 25 23.741 +13 44 33.60 21.9r 14UW229 568 C~2SDl 2013 10 09.40859 01 23 16.799 +13 35 08.53 24.2r 14UW229 568 C~2SDl 2013 10 30.38445 01 21 56.987 +13 28 00.65 23.9r 14UW229 568 C~2SDl 2013 10 31.38098 01 21 53.326 +13 27 39.72 24.1r 14UW229 568 C~2SDl 2013 11 01.32125 01 21 49.874 +13 27 20.17 24.0r 14UW229 568 C~2SDl 2013 11 01.36050 01 21 49.728 +13 27 19.39 23.7r 14UW229 568 C~2SDl 2013 11 01.36717 01 21 49.696 +13 27 19.36 24.1r 14UW229 568 C~2SDl 2013 11 01.45478 01 21 49.383 +13 27 17.57 24.5r 14UW229 568 C~2SDl 2013 11 05.42745 01 21 35.062 +13 25 55.10 23.9r 14UW229 568 C~2SDl 2013 11 05.47445 01 21 34.865 +13 25 54.43 24.1r 14UW229 568 C~2SDl 2013 11 05.47937 01 21 34.857 +13 25 54.20 24.6r 14UW229 568 C~2SDl 2013 11 27.37664 01 20 25.965 +13 18 53.04 24.0r 14UW229 568 C~2SDl 2013 12 04.35870 01 20 08.811 +13 16 58.35 24.4r 14UW229 568 C~2SDl 2013 12 29.31207 01 19 32.873 +13 12 17.00 23.7r 14UW229 568 C~2SDl 2014 09 23.46889 01 27 12.664 +14 10 40.09 24.0r 14UW229 568 C~2SDl 2014 10 22.42878 01 25 23.704 +14 01 40.84 24.2r 14UW229 568 C~2SDl 2014 10 22.46820 01 25 23.553 +14 01 39.89 23.9r 14UW229 568 C~2SDl 2014 10 22.50765 01 25 23.405 +14 01 39.03 24.3r 14UW229 568 C~2SDl 2014 10 25.43103 01 25 12.237 +14 00 38.58 24.8r 14UW229 568 C~2SDl 2014 11 19.23833 01 23 44.793 +13 52 12.25 24.5r 14UW229 568 C~2SDl 2014 11 19.37128 01 23 44.358 +13 52 09.68 24.4r 14UW229 568 C~2SDm 2014 11 21.21867 01 23 38.713 +13 51 34.47 24.5r 14UW229 568 C~2SDm 2014 11 21.38105 01 23 38.216 +13 51 31.28 24.3r 14UW229 568 C~2SDm 2015 02 19.22673 01 23 30.831 +13 46 14.05 23.8r 14UW229 568 C~2SDm 2015 02 19.24767 01 23 30.906 +13 46 14.58 23.9r 14UW229 568 C~2SDm 2015 10 09.43173 01 29 12.012 +14 36 49.76 24.5w 14UW229 568 C~2SDm 2015 10 09.47451 01 29 11.847 +14 36 48.94 24.3w 14UW229 568 C~2SDm 2015 10 09.50371 01 29 11.734 +14 36 48.39 24.4w 14UW229 568 C~2SDm 2015 12 07.42436 01 25 52.078 +14 17 40.58 24.5w 14UW229 568 C~2SDm 2024 11 01.240060 01 55 31.459 +19 04 47.28 24.2G 14UW229 G37 C~8SSm 2024 11 01.287440 01 55 31.260 +19 04 46.35 14UW229 G37 C~8SSm 2024 11 01.333070 01 55 31.071 +19 04 45.39 14UW229 G37 C~8SSm
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 0.25 0.00 -0.16
2 0.0001 0.00 0.06 0.00 -0.40
3 0.1037 0.00 0.02 0.00 -0.09
4 0.1611 0.00 -0.08 0.00 0.08
5 0.1639 0.00 0.12 0.00 -0.07
6 0.1664 0.00 0.00 0.00 -0.04
7 0.1665 0.00 0.00 0.00 -0.01
8 0.1666 0.00 -0.10 0.00 0.10
9 0.1668 0.00 0.09 0.00 0.14
10 0.1777 0.00 0.10 0.00 -0.01
11 0.1778 0.00 -0.31 0.00 0.30
12 0.1778 0.00 -0.17 0.00 0.17
13 0.2378 0.00 -0.10 0.00 0.30
14 0.2569 0.00 0.13 0.00 -0.04
15 0.3252 0.00 -0.07 0.00 -0.04
16 1.0594 0.00 -0.05 0.00 -0.09
17 1.1387 0.00 -0.14 0.00 0.11
18 1.1388 0.00 -0.10 0.00 -0.03
19 1.1389 0.00 -0.01 0.00 -0.07
20 1.1469 0.00 0.20 0.00 0.01
21 1.2148 0.00 0.12 0.00 0.03
22 1.2152 0.00 -0.07 0.00 0.01
23 1.2202 0.00 0.02 0.00 -0.01
24 1.2207 0.00 0.08 0.00 -0.15
25 1.4666 0.00 -0.15 0.00 -0.14
26 1.4667 0.00 0.04 0.00 0.08
27 2.1024 0.00 -0.01 0.00 -0.02
28 2.1025 0.00 0.02 0.00 -0.03
29 2.1026 0.00 0.04 0.00 -0.03
30 2.2639 0.00 0.11 0.00 0.08
31 11.1669 0.00 0.05 0.00 -0.00
32 11.1670 0.00 -0.03 0.00 0.02
33 11.1671 0.00 -0.06 0.00 -0.01
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.
14UW229 quality flag:3 Type: 2:1E 2:1E 2:1E axisobj 48.068 48.068 48.068 ecceobj 0.164 0.164 0.164 incobj 14.557 14.557 14.557 qmin 37.358 37.358 37.358 qmax 58.597 58.597 58.597 amean 47.798 47.798 47.798 amin 47.354 47.354 47.354 amax 48.305 48.305 48.305 emean 0.181 0.181 0.181 emin 0.147 0.147 0.147 emax 0.214 0.214 0.214 imean 14.644 14.644 14.644 imin 13.809 13.809 13.809 imax 15.637 15.637 15.638 excite_mean 0.312 0.312 0.312 fracstop 1.000 1.000 1.000 cjmean 3.027 3.027 3.027 libcent 0 276.4 276.4 276.4 libamp 0 24.2 24.2 24.2 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 171.9 171.9 171.9 kozaiamp 180.0 180.0 180.0