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: 02GH166
# Created Thu Nov 21 02:08:21 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 95 observations of 95
# Arc: 23.30y
# First observation: 2000/03/03
# Last observation: 2023/06/21
# Chi-squared of fit: 124.08 DOF: 184 RMS: 0.20
# Min/Max residuals: -0.71 1.03
# Exact a, adot, b, bdot, g, gdot:
2.056385E-05 3.611394E-02 -1.595034E-06 -5.487108E-03 3.116189E-02 -3.733091E-03
# Covariance matrix:
2.2417E-13 -2.2187E-14 -1.4770E-14 2.3310E-15 9.7644E-15 -1.2511E-14
-2.2187E-14 2.7778E-15 2.2910E-15 -3.5657E-16 3.1233E-16 1.8649E-15
-1.4770E-14 2.2910E-15 1.3116E-13 -8.3241E-15 -2.3775E-16 1.9363E-15
2.3310E-15 -3.5657E-16 -8.3241E-15 5.9115E-16 1.1077E-16 -3.0568E-16
9.7644E-15 3.1233E-16 -2.3775E-16 1.1077E-16 2.6919E-14 -1.3111E-15
-1.2511E-14 1.8649E-15 1.9363E-15 -3.0568E-16 -1.3111E-15 1.6415E-15
# lat0 lon0 xBary yBary zBary JD0
0.518943 -171.810608 0.417068 0.007972 -0.905669 2451606.949069
# Heliocentric elements and errors
Epoch: 2451606.5000 = 2000/03/03
Mean Anomaly: 330.57779 +/- 0.002
Argument of Peri: 219.44635 +/- 0.003
Long of Asc Node: 10.77028 +/- 0.000
Inclination: 8.68025 +/- 0.000
Eccentricity: 0.19056455 +/- 0.0000
Semi-Major Axis: 39.02225126 +/- 0.0012
Time of Perihelion: 2458883.2887 +/- 3.9
Perihelion: 31.58599359 +/- 0.0012
Aphelion: 46.45850894 +/- 0.0016
Period (y) 243.7680 +/- 0.01
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -32.71093607 +/- 0.0002
Ecliptic Y -4.28457482 +/- 0.0000
Ecliptic Z 0.29062751 +/- 0.0000
Ecliptic XDOT 0.00076638 +/- 0.0000
Ecliptic YDOT -0.00308755 +/- 0.0000
Ecliptic ZDOT -0.00048493 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 32.99169301 +/- 0.0002
Geocenter to KBO 32.09056536 +/- 0.0002
# Hcoef: 7.20
The following table shows the complete astrometric record for 02GH166. 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 (02GH166) followed by the observatory code and reference code for the source of the astrometry.
2000 03 03.448326 12 30 54.38 -02 46 16.7 22.2V 02GH166 645 C~2Jx6 2000 03 03.449156 12 30 54.37 -02 46 16.6 22.2V 02GH166 645 C~2Jx6 2000 03 03.451643 12 30 54.36 -02 46 16.6 22.9V 02GH166 645 C~2Jx6 2002 04 03.37286 12 42 31.42 -04 43 38.3 21.5R 02GH166 644 Cl2691 2002 04 09.04270 12 41 59.38 -04 40 33.0 20.7R 02GH166 807 Cf7585 2002 04 09.14504 12 41 58.81 -04 40 29.9 02GH166 807 Cf7585 2002 05 08.34585 12 39 29.86 -04 26 19.4 21.7R 02GH166 568 Cf7585 2002 05 08.41063 12 39 29.57 -04 26 17.8 02GH166 568 Cf7585 2010 06 26.28182 13 37 15.969 -13 04 52.74 22.8G 02GH166 F51 C~2r7A 2011 01 21.64768 13 55 05.375 -14 52 54.76 21.6G 02GH166 F51 C~2r7A 2011 04 03.54486 13 51 47.979 -14 44 47.96 22.2G 02GH166 F51 C~2r7A 2011 04 13.41677 13 50 50.012 -14 40 19.76 21.9i 02GH166 F51 C~1vV9 2011 04 13.42870 13 50 49.943 -14 40 19.41 21.6i 02GH166 F51 C~1vV9 2011 04 13.57344 13 50 49.057 -14 40 14.78 22.3g 02GH166 F51 C~1vV9 2012 04 15.42106 13 58 45.075 -15 43 31.87 22.4w 02GH166 F51 C~1vV9 2012 04 15.43498 13 58 44.987 -15 43 31.53 22.1w 02GH166 F51 C~1vV9 2012 04 15.44885 13 58 44.896 -15 43 31.15 22.1w 02GH166 F51 C~1vV9 2012 04 15.46278 13 58 44.819 -15 43 30.79 22.1w 02GH166 F51 C~1vV9 2013 04 12.53334 14 07 22.622 -16 48 29.68 21.9G 02GH166 F51 C~2r7A 2013 05 05.38502 14 05 03.578 -16 37 49.66 22.0G 02GH166 F51 C~2r7A 2013 05 05.39985 14 05 03.483 -16 37 48.98 21.9G 02GH166 F51 C~2r7A 2013 05 05.42940 14 05 03.286 -16 37 48.39 21.8G 02GH166 F51 C~2r7A 2013 05 18.37449 14 03 48.845 -16 31 34.71 22.2G 02GH166 F51 C~2r7A 2014 04 05.47521 14 16 31.314 -17 53 46.11 22.2w 02GH166 F51 C~1vV9 2014 04 05.48710 14 16 31.245 -17 53 46.00 22.0w 02GH166 F51 C~1vV9 2014 04 05.49899 14 16 31.181 -17 53 45.57 22.0w 02GH166 F51 C~1vV9 2014 04 05.51090 14 16 31.103 -17 53 45.33 22.1w 02GH166 F51 C~1vV9 2014 04 29.41018 14 14 06.847 -17 43 38.10 22.3w 02GH166 F51 C~1vV9 2014 04 29.42076 14 14 06.803 -17 43 37.24 22.5w 02GH166 F51 C~1vV9 2014 04 29.43135 14 14 06.711 -17 43 37.33 22.1w 02GH166 F51 C~1vV9 2014 04 29.44193 14 14 06.652 -17 43 37.06 22.1w 02GH166 F51 C~1vV9 2014 05 07.39950 14 13 17.896 -17 39 51.25 21.9G 02GH166 F51 C~2r7A 2014 05 07.41030 14 13 17.856 -17 39 51.05 21.5G 02GH166 F51 C~2r7A 2014 05 07.43138 14 13 17.738 -17 39 49.92 22.3G 02GH166 F51 C~2r7A 2014 05 23.31588 14 11 46.530 -17 32 20.59 22.2w 02GH166 F51 C~1vV9 2014 05 23.32715 14 11 46.463 -17 32 20.33 22.0w 02GH166 F51 C~1vV9 2014 05 23.33843 14 11 46.401 -17 32 20.08 22.2w 02GH166 F51 C~1vV9 2014 05 23.34971 14 11 46.346 -17 32 19.73 22.2w 02GH166 F51 C~1vV9 2014 06 04.32323 14 10 47.110 -17 27 05.56 22.0G 02GH166 F51 C~2r7A 2014 06 20.30471 14 09 46.766 -17 21 14.58 22.1G 02GH166 F51 C~2r7A 2014 06 30.27222 14 09 22.156 -17 18 31.14 22.4G 02GH166 F51 C~2r7A 2014 06 30.28410 14 09 22.133 -17 18 30.67 22.5G 02GH166 F51 C~2r7A 2014 06 30.29599 14 09 22.095 -17 18 30.46 22.4G 02GH166 F51 C~2r7A 2014 06 30.30787 14 09 22.087 -17 18 30.63 22.1G 02GH166 F51 C~2r7A 2015 01 23.66786 14 27 39.160 -18 54 47.28 21.9G 02GH166 F51 C~2r7A 2015 03 02.65598 14 27 30.380 -19 01 19.17 22.5G 02GH166 F51 C~2r7A 2015 04 01.49942 14 25 27.793 -18 56 10.61 22.5G 02GH166 F51 C~2r7A 2015 04 13.19071 14 24 21.48 -18 52 10.0 22.4V 02GH166 W84 C~2J8o 2015 04 13.33664 14 24 20.61 -18 52 06.7 02GH166 W84 C~2J8o 2015 04 13.38815 14 24 20.29 -18 52 05.5 02GH166 W84 C~2J8o 2015 04 25.42135 14 23 06.644 -18 47 09.07 22.6G 02GH166 F51 C~2r7A 2015 04 25.43328 14 23 06.588 -18 47 08.66 22.2G 02GH166 F51 C~2r7A 2015 04 25.44520 14 23 06.504 -18 47 08.46 22.3G 02GH166 F51 C~2r7A 2015 05 19.38967 14 20 40.599 -18 36 08.06 22.0G 02GH166 F51 C~2r7A 2015 05 21.32391 14 20 29.581 -18 35 14.42 22.1G 02GH166 F51 C~2r7A 2015 05 21.33603 14 20 29.509 -18 35 13.78 22.4G 02GH166 F51 C~2r7A 2015 05 21.34822 14 20 29.440 -18 35 13.52 21.9G 02GH166 F51 C~2r7A 2015 05 21.36035 14 20 29.371 -18 35 13.28 22.4G 02GH166 F51 C~2r7A 2015 06 18.29546 14 18 18.824 -18 23 37.59 22.3w 02GH166 F51 C~1vV9 2015 06 18.30776 14 18 18.783 -18 23 37.33 22.2w 02GH166 F51 C~1vV9 2015 06 18.32004 14 18 18.738 -18 23 37.13 22.1w 02GH166 F51 C~1vV9 2015 06 18.33234 14 18 18.695 -18 23 36.75 22.2w 02GH166 F51 C~1vV9 2015 06 19.28262 14 18 15.436 -18 23 17.37 22.3w 02GH166 F51 C~1vV9 2015 06 19.29451 14 18 15.399 -18 23 17.06 22.5w 02GH166 F51 C~1vV9 2015 06 19.30641 14 18 15.361 -18 23 16.94 22.6w 02GH166 F51 C~1vV9 2015 06 19.31830 14 18 15.322 -18 23 16.57 22.1w 02GH166 F51 C~1vV9 2016 02 12.58705 14 36 28.184 -19 57 57.13 21.7G 02GH166 F51 C~2r7A 2016 02 12.59918 14 36 28.171 -19 57 57.37 22.1G 02GH166 F51 C~2r7A 2016 02 12.61129 14 36 28.163 -19 57 57.26 22.3G 02GH166 F51 C~2r7A 2016 02 12.62349 14 36 28.178 -19 57 57.66 22.5G 02GH166 F51 C~2r7A 2016 03 16.49888 14 35 19.089 -19 58 52.56 22.4G 02GH166 F51 C~2r7A 2016 03 16.51060 14 35 19.060 -19 58 52.62 22.3G 02GH166 F51 C~2r7A 2016 03 16.53396 14 35 18.953 -19 58 52.37 22.3G 02GH166 F51 C~2r7A 2016 04 12.46713 14 33 02.635 -19 52 06.11 21.8G 02GH166 F51 C~2r7A 2016 04 12.47879 14 33 02.564 -19 52 06.02 21.7G 02GH166 F51 C~2r7A 2016 04 12.49044 14 33 02.481 -19 52 05.79 22.9G 02GH166 F51 C~2r7A 2016 05 02.40092 14 30 59.561 -19 44 06.34 22.2G 02GH166 F51 C~2r7A 2016 05 02.41254 14 30 59.476 -19 44 06.07 22.4G 02GH166 F51 C~2r7A 2016 05 02.43579 14 30 59.339 -19 44 05.20 22.2G 02GH166 F51 C~2r7A 2017 01 31.62604 14 44 54.250 -20 51 10.02 23.0G 02GH166 F51 C~2r7A 2017 04 01.49912 14 42 53.644 -20 53 42.99 22.4G 02GH166 F51 C~2r7A 2017 04 01.51035 14 42 53.575 -20 53 42.78 22.2G 02GH166 F51 C~2r7A 2017 04 01.52157 14 42 53.517 -20 53 42.53 22.2G 02GH166 F51 C~2r7A 2017 04 01.53277 14 42 53.465 -20 53 42.48 22.2G 02GH166 F51 C~2r7A 2017 04 25.45725 14 40 33.849 -20 46 00.19 21.7G 02GH166 F51 C~2r7A 2017 05 18.32251 14 38 10.467 -20 36 13.82 22.0G 02GH166 F51 C~2r7A 2017 05 18.33426 14 38 10.379 -20 36 13.58 22.0G 02GH166 F51 C~2r7A 2017 05 18.35772 14 38 10.238 -20 36 13.28 22.6G 02GH166 F51 C~2r7A 2018 04 13.49797 14 50 44.721 -21 47 13.82 22.2G 02GH166 F51 C~2r7A 2022 06 20.296321 15 20 40.390 -24 53 19.01 22.3w 02GH166 F52 C~5hTJ 2022 06 20.315348 15 20 40.286 -24 53 18.44 22.1w 02GH166 F52 C~5hTJ 2022 06 20.324911 15 20 40.256 -24 53 18.08 22.1w 02GH166 F52 C~5hTJ 2023 06 21.314091 15 30 00.273 -25 41 05.24 21.9w 02GH166 F52 C~6r1w 2023 06 21.337410 15 30 00.139 -25 41 04.74 21.9w 02GH166 F52 C~6r1w 2023 06 21.348997 15 30 00.093 -25 41 04.03 22.2w 02GH166 F52 C~6r1w
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 -0.52 0.00 -0.04
2 0.0000 0.00 -0.61 0.00 0.03
3 0.0000 0.00 -0.57 0.00 -0.04
4 2.0833 0.00 -0.37 0.00 -0.03
5 2.0988 0.00 0.80 0.00 0.25
6 2.0991 0.00 1.03 0.00 0.04
7 2.1790 0.00 0.55 0.00 -0.02
8 2.1792 0.00 0.47 0.00 0.01
9 10.3130 0.00 -0.71 0.00 0.01
10 10.8862 0.00 -0.06 0.00 -0.43
11 11.0831 0.00 -0.33 0.00 -0.21
12 11.1101 0.00 -0.06 0.00 -0.18
13 11.1101 0.00 -0.00 0.00 -0.16
14 11.1105 0.00 -0.06 0.00 0.34
15 12.1177 0.00 -0.01 0.00 0.07
16 12.1177 0.00 -0.04 0.00 0.02
17 12.1177 0.00 -0.12 0.00 0.02
18 12.1178 0.00 0.01 0.00 -0.01
19 13.1091 0.00 -0.12 0.00 -0.09
20 13.1716 0.00 0.16 0.00 -0.02
21 13.1717 0.00 0.09 0.00 0.23
22 13.1717 0.00 -0.16 0.00 -0.04
23 13.2072 0.00 -0.36 0.00 -0.06
24 14.0891 0.00 0.09 0.00 -0.05
25 14.0891 0.00 0.09 0.00 -0.20
26 14.0891 0.00 0.16 0.00 -0.03
27 14.0892 0.00 0.03 0.00 -0.05
28 14.1546 0.00 0.11 0.00 -0.21
29 14.1546 0.00 0.45 0.00 0.35
30 14.1546 0.00 0.07 0.00 -0.03
31 14.1547 0.00 0.19 0.00 -0.06
32 14.1765 0.00 -0.23 0.00 -0.08
33 14.1765 0.00 0.17 0.00 -0.19
34 14.1765 0.00 0.34 0.00 0.33
35 14.2200 0.00 0.02 0.00 0.10
36 14.2201 0.00 -0.06 0.00 0.06
37 14.2201 0.00 -0.07 0.00 -0.00
38 14.2201 0.00 0.03 0.00 0.04
39 14.2529 0.00 -0.03 0.00 -0.17
40 14.2967 0.00 0.17 0.00 0.20
41 14.3240 0.00 -0.07 0.00 -0.08
42 14.3240 0.00 -0.05 0.00 0.23
43 14.3240 0.00 -0.26 0.00 0.27
44 14.3241 0.00 -0.02 0.00 -0.07
45 14.8918 0.00 -0.01 0.00 -0.11
46 14.9958 0.00 0.27 0.00 -0.34
47 15.0775 0.00 -0.11 0.00 -0.17
48 15.1095 0.00 -0.12 0.00 -0.03
49 15.1099 0.00 0.08 0.00 -0.07
50 15.1100 0.00 -0.06 0.00 -0.07
51 15.1430 0.00 -0.28 0.00 0.01
52 15.1430 0.00 0.01 0.00 0.11
53 15.1430 0.00 -0.11 0.00 0.00
54 15.2086 0.00 0.02 0.00 0.01
55 15.2139 0.00 -0.09 0.00 -0.10
56 15.2139 0.00 -0.13 0.00 0.20
57 15.2140 0.00 -0.11 0.00 0.12
58 15.2140 0.00 -0.09 0.00 0.03
59 15.2905 0.00 0.02 0.00 0.07
60 15.2905 0.00 0.07 0.00 0.08
61 15.2905 0.00 0.05 0.00 0.02
62 15.2906 0.00 0.07 0.00 0.15
63 15.2932 0.00 -0.02 0.00 -0.00
64 15.2932 0.00 0.05 0.00 0.07
65 15.2932 0.00 0.11 0.00 -0.06
66 15.2933 0.00 0.15 0.00 0.07
67 15.9456 0.00 0.03 0.00 -0.01
68 15.9457 0.00 -0.13 0.00 -0.10
69 15.9457 0.00 -0.22 0.00 0.15
70 15.9457 0.00 0.03 0.00 -0.10
71 16.0357 0.00 -0.12 0.00 0.14
72 16.0358 0.00 0.16 0.00 -0.01
73 16.0358 0.00 -0.02 0.00 0.05
74 16.1096 0.00 0.03 0.00 0.07
75 16.1096 0.00 0.02 0.00 -0.08
76 16.1096 0.00 -0.17 0.00 -0.10
77 16.1641 0.00 0.29 0.00 0.00
78 16.1642 0.00 0.13 0.00 -0.03
79 16.1642 0.00 0.31 0.00 0.22
80 16.9149 0.00 -0.12 0.00 0.15
81 17.0789 0.00 0.06 0.00 -0.07
82 17.0789 0.00 -0.09 0.00 -0.02
83 17.0789 0.00 -0.06 0.00 0.07
84 17.0789 0.00 0.04 0.00 -0.04
85 17.1444 0.00 0.11 0.00 -0.06
86 17.2070 0.00 -0.03 0.00 0.06
87 17.2071 0.00 -0.26 0.00 -0.01
88 17.2071 0.00 -0.21 0.00 -0.34
89 18.1110 0.00 0.01 0.00 -0.14
90 22.2966 0.00 0.15 0.00 -0.17
91 22.2967 0.00 0.05 0.00 -0.03
92 22.2967 0.00 0.34 0.00 0.12
93 23.2987 0.00 -0.08 0.00 -0.05
94 23.2988 0.00 -0.24 0.00 -0.07
95 23.2988 0.00 -0.01 0.00 0.38
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.
02GH166 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.011 39.011 39.011 ecceobj 0.190 0.190 0.190 incobj 8.682 8.682 8.682 qmin 30.626 30.623 30.646 qmax 48.897 48.899 48.905 amean 39.456 39.456 39.456 amin 38.964 38.968 38.977 amax 40.040 40.013 40.021 emean 0.204 0.204 0.204 emin 0.183 0.182 0.182 emax 0.224 0.224 0.224 imean 8.600 8.616 8.604 imin 8.063 8.062 8.064 imax 9.422 9.417 9.424 excite_mean 0.253 0.253 0.253 fracstop 1.000 1.000 1.000 cjmean 2.979 2.979 2.978 libcent 0 179.8 180.6 179.7 libamp 0 105.6 106.0 105.7 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 181.9 182.4 182.0 kozaiamp 180.0 180.0 179.9