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: 523717
# Created Sat Apr 20 01:08:27 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 86 observations of 86
# Arc: 7.21y
# First observation: 2010/05/10
# Last observation: 2017/07/25
# Chi-squared of fit: 52.25 DOF: 166 RMS: 0.14
# Min/Max residuals: -0.49 0.47
# Exact a, adot, b, bdot, g, gdot:
1.804922E-05 3.519952E-02 -2.218212E-06 -4.732799E-03 3.077939E-02 4.950450E-03
# Covariance matrix:
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00
# lat0 lon0 xBary yBary zBary JD0
6.175258 -121.487134 0.161493 0.107278 -0.992031 2455326.989106
# Heliocentric elements and errors
Epoch: 2455326.5000 = 2010/05/10
Mean Anomaly: 33.68020 +/- 0.000
Argument of Peri: 92.20924 +/- 0.000
Long of Asc Node: 96.30598 +/- 0.000
Inclination: 9.66132 +/- 0.000
Eccentricity: 0.19846271 +/- 0.0000
Semi-Major Axis: 39.36235826 +/- 0.0000
Time of Perihelion: 2446887.4756 +/- 0.0
Perihelion: 31.55039796 +/- 0.0000
Aphelion: 47.17431857 +/- 0.0000
Period (y) 246.9618 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -17.52524567 +/- 0.0000
Ecliptic Y -28.31374758 +/- 0.0000
Ecliptic Z 3.49484725 +/- 0.0000
Ecliptic XDOT 0.00241943 +/- 0.0000
Ecliptic YDOT -0.00204133 +/- 0.0000
Ecliptic ZDOT -0.00037122 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 33.48150572 +/- 0.0000
Geocenter to KBO 32.48922863 +/- 0.0000
# Hcoef: 6.36
The following table shows the complete astrometric record for 523717. 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 (523717) followed by the observatory code and reference code for the source of the astrometry.
2010 05 10.48834 15 50 42.134 -13 48 02.58 21.5G 523717 F51 C~2kQC 2010 05 11.49325 15 50 36.263 -13 47 44.71 21.4G 523717 F51 C~2kQC 2010 06 04.41817 15 48 15.554 -13 41 32.45 21.5G 523717 F51 C~2kQC 2010 06 04.43024 15 48 15.490 -13 41 32.32 21.4G 523717 F51 C~2kQC 2010 06 07.37441 15 47 58.847 -13 40 56.15 21.7G 523717 F51 C~2kQC 2010 06 07.38586 15 47 58.772 -13 40 56.13 21.9G 523717 F51 C~2kQC 2010 08 09.26186 15 44 32.325 -13 41 02.23 21.6G 523717 F51 C~2kQC 2011 05 21.43759 15 57 30.315 -14 26 12.53 22.2G 523717 F51 C~2kQC 2013 07 01.31495 16 09 17.343 -15 37 55.14 21.8w 523717 F51 C~1vXX 2013 07 01.32831 16 09 17.286 -15 37 55.11 21.6w 523717 F51 C~1vXX 2013 07 01.34166 16 09 17.222 -15 37 54.96 21.7w 523717 F51 C~1vXX 2013 07 01.35499 16 09 17.158 -15 37 54.88 21.8w 523717 F51 C~1vXX 2013 08 27.24916 16 07 32.424 -15 43 34.44 21.6w 523717 F51 C~1vXX 2013 08 27.25314 16 07 32.438 -15 43 34.58 21.7w 523717 F51 C~1vXX 2013 08 27.25716 16 07 32.436 -15 43 34.54 22.0w 523717 F51 C~1vXX 2013 08 27.26113 16 07 32.450 -15 43 34.44 21.9w 523717 F51 C~1vXX 2014 02 26.61279 16 25 07.759 -16 36 38.28 21.8G 523717 F51 C~2kQC 2014 05 23.41406 16 20 39.542 -16 20 59.80 21.7w 523717 F51 C~1vXX 2014 05 23.42696 16 20 39.468 -16 20 59.62 21.8w 523717 F51 C~1vXX 2014 05 23.43980 16 20 39.396 -16 20 59.43 21.6w 523717 F51 C~1vXX 2014 05 23.45269 16 20 39.310 -16 20 59.22 21.6w 523717 F51 C~1vXX 2014 05 28.44143 16 20 09.608 -16 19 58.71 21.6G 523717 F51 C~2kQC 2014 06 08.37518 16 19 04.915 -16 17 59.91 21.2i 523717 F51 C~1vXX 2014 06 08.38803 16 19 04.830 -16 17 59.76 21.1i 523717 F51 C~1vXX 2014 06 08.41390 16 19 04.684 -16 17 59.67 21.4i 523717 F51 C~1vXX 2014 06 26.33412 16 17 26.165 -16 15 40.14 21.5w 523717 F51 C~1vXX 2014 06 26.34473 16 17 26.120 -16 15 40.53 21.5w 523717 F51 C~1vXX 2014 06 26.35537 16 17 26.046 -16 15 40.58 21.4w 523717 F51 C~1vXX 2014 06 28.33347 16 17 16.145 -16 15 30.17 22.1w 523717 F51 C~1vXX 2014 06 28.34406 16 17 16.089 -16 15 30.14 21.8w 523717 F51 C~1vXX 2014 06 28.35464 16 17 16.032 -16 15 30.10 21.6w 523717 F51 C~1vXX 2014 07 28.32374 16 15 23.876 -16 15 22.35 21.3G 523717 F51 C~2kQC 2014 07 31.29758 16 15 17.390 -16 15 37.16 20.5G 523717 F51 C~2kQC 2014 08 22.25090 16 15 00.227 -16 19 01.01 21.9w 523717 F51 C~1vXX 2014 08 22.26258 16 15 00.232 -16 19 01.22 22.1w 523717 F51 C~1vXX 2014 08 22.27425 16 15 00.226 -16 19 01.45 22.1w 523717 F51 C~1vXX 2014 08 22.28592 16 15 00.230 -16 19 01.40 21.9w 523717 F51 C~1vXX 2015 03 20.61532 16 32 43.938 -17 08 41.32 21.8w 523717 F51 C~1vXX 2015 03 20.62610 16 32 43.950 -17 08 41.45 21.6w 523717 F51 C~1vXX 2015 03 20.62676 16 32 43.954 -17 08 41.28 20.8G 523717 F51 C~2kQC 2015 03 20.63690 16 32 43.937 -17 08 41.22 21.7w 523717 F51 C~1vXX 2015 03 21.57695 16 32 42.857 -17 08 33.99 21.8w 523717 F51 C~1vXX 2015 03 21.58758 16 32 42.873 -17 08 33.94 21.9w 523717 F51 C~1vXX 2015 03 21.59819 16 32 42.857 -17 08 33.83 22.1w 523717 F51 C~1vXX 2015 03 21.60886 16 32 42.816 -17 08 33.91 21.8w 523717 F51 C~1vXX 2015 05 21.43420 16 28 36.810 -16 57 02.74 21.6G 523717 F51 C~2kQC 2015 05 21.44629 16 28 36.741 -16 57 02.67 22.0G 523717 F51 C~2kQC 2015 05 21.45840 16 28 36.670 -16 57 02.42 21.6G 523717 F51 C~2kQD 2015 05 21.47051 16 28 36.595 -16 57 02.27 21.7G 523717 F51 C~2kQD 2015 06 11.36461 16 26 32.932 -16 53 25.57 21.5G 523717 F51 C~2kQD 2015 06 11.37671 16 26 32.859 -16 53 25.41 21.2G 523717 F51 C~2kQD 2015 06 11.38878 16 26 32.795 -16 53 25.32 21.1G 523717 F51 C~2kQD 2015 06 11.40085 16 26 32.718 -16 53 25.18 21.7G 523717 F51 C~2kQD 2015 06 13.38154 16 26 21.260 -16 53 08.41 21.6G 523717 F51 C~2kQD 2015 06 13.38219 16 26 21.262 -16 53 08.29 21.6G 523717 F51 C~2kQD 2015 06 13.39364 16 26 21.197 -16 53 08.32 22.2G 523717 F51 C~2kQD 2015 06 13.39430 16 26 21.193 -16 53 08.16 22.0G 523717 F51 C~2kQD 2015 07 09.35041 16 24 07.983 -16 50 52.21 22.1w 523717 F51 C~1vXX 2015 07 09.36231 16 24 07.935 -16 50 52.20 21.8w 523717 F51 C~1vXX 2015 07 09.37414 16 24 07.887 -16 50 52.27 21.8w 523717 F51 C~1vXX 2015 07 09.38601 16 24 07.832 -16 50 52.22 22.0w 523717 F51 C~1vXX 2015 07 12.35340 16 23 55.411 -16 50 48.04 21.8w 523717 F51 C~1vXX 2015 07 12.36506 16 23 55.361 -16 50 47.96 21.7w 523717 F51 C~1vXX 2015 07 12.37686 16 23 55.310 -16 50 48.00 21.8w 523717 F51 C~1vXX 2015 07 12.38875 16 23 55.281 -16 50 48.02 21.7w 523717 F51 C~1vXX 2015 08 06.28879 16 22 43.381 -16 51 59.36 20.8G 523717 F51 C~2kQD 2015 08 08.31267 16 22 40.397 -16 52 13.30 22.4G 523717 F51 C~2kQD 2016 03 18.58914 16 40 18.578 -17 41 41.74 22.3G 523717 F51 C~2kQD 2016 05 03.50436 16 37 54.165 -17 34 21.45 22.1G 523717 F51 C~2kQD 2016 06 08.44188 16 34 28.121 -17 28 09.17 21.5G 523717 F51 C~2kQD 2016 06 08.45160 16 34 28.073 -17 28 09.05 21.7G 523717 F51 C~2kQD 2016 06 08.46134 16 34 28.004 -17 28 08.90 21.5G 523717 F51 C~2kQD 2016 06 08.47109 16 34 27.943 -17 28 08.84 21.5G 523717 F51 C~2kQD 2016 06 13.40554 16 33 59.134 -17 27 29.35 21.6G 523717 F51 C~2kQD 2016 08 18.26100 16 30 04.369 -17 28 01.03 22.0G 523717 F51 C~2kQD 2017 04 25.50542 16 46 12.371 -18 08 03.32 21.1G 523717 F51 C~2kQD 2017 05 04.53662 16 45 29.555 -18 06 32.85 21.7G 523717 F51 C~2kQD 2017 05 04.54781 16 45 29.496 -18 06 32.54 22.2G 523717 F51 C~2kQD 2017 05 04.55906 16 45 29.432 -18 06 32.49 22.2G 523717 F51 C~2kQD 2017 05 04.57030 16 45 29.354 -18 06 32.58 22.3G 523717 F51 C~2kQD 2017 05 19.54461 16 44 08.075 -18 04 03.57 22.4G 523717 F51 C~2kQD 2017 05 27.41411 16 43 22.102 -18 02 49.26 21.3G 523717 F51 C~2kQD 2017 06 20.35978 16 41 01.544 -17 59 47.39 21.6G 523717 F51 C~2kQD 2017 06 20.37090 16 41 01.475 -17 59 47.30 21.6G 523717 F51 C~2kQD 2017 06 20.38200 16 41 01.408 -17 59 47.20 21.2G 523717 F51 C~2kQD 2017 07 25.30942 16 38 21.719 -17 58 38.78 21.5G 523717 F51 C~2kQD
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 -0.04
2 0.0028 0.00 -0.03 0.00 -0.08
3 0.0683 0.00 -0.06 0.00 0.03
4 0.0683 0.00 0.03 0.00 0.01
5 0.0763 0.00 0.08 0.00 -0.05
6 0.0764 0.00 -0.06 0.00 -0.17
7 0.2485 0.00 -0.09 0.00 -0.11
8 1.0293 0.00 0.04 0.00 -0.31
9 3.1426 0.00 -0.04 0.00 -0.02
10 3.1426 0.00 0.05 0.00 -0.04
11 3.1427 0.00 0.03 0.00 0.06
12 3.1427 0.00 0.01 0.00 0.09
13 3.2985 0.00 -0.25 0.00 0.01
14 3.2985 0.00 -0.12 0.00 -0.07
15 3.2985 0.00 -0.22 0.00 0.03
16 3.2985 0.00 -0.09 0.00 0.19
17 3.8005 0.00 0.29 0.00 -0.01
18 4.0354 0.00 -0.09 0.00 -0.03
19 4.0354 0.00 -0.03 0.00 -0.01
20 4.0355 0.00 0.05 0.00 0.02
21 4.0355 0.00 -0.07 0.00 0.07
22 4.0492 0.00 0.12 0.00 0.03
23 4.0791 0.00 0.23 0.00 0.09
24 4.0791 0.00 0.10 0.00 0.11
25 4.0792 0.00 0.21 0.00 -0.05
26 4.1283 0.00 0.32 0.00 0.45
27 4.1283 0.00 0.47 0.00 -0.00
28 4.1283 0.00 0.18 0.00 -0.11
29 4.1337 0.00 0.10 0.00 0.04
30 4.1338 0.00 0.06 0.00 0.02
31 4.1338 0.00 0.01 0.00 0.00
32 4.2158 0.00 -0.06 0.00 -0.15
33 4.2240 0.00 -0.15 0.00 0.32
34 4.2841 0.00 -0.01 0.00 0.13
35 4.2841 0.00 -0.01 0.00 0.07
36 4.2842 0.00 -0.17 0.00 -0.01
37 4.2842 0.00 -0.18 0.00 0.18
38 4.8600 0.00 -0.39 0.00 0.29
39 4.8601 0.00 -0.02 0.00 0.07
40 4.8601 0.00 0.05 0.00 0.24
41 4.8601 0.00 -0.02 0.00 0.22
42 4.8627 0.00 -0.26 0.00 0.09
43 4.8627 0.00 0.19 0.00 0.05
44 4.8627 0.00 0.15 0.00 0.08
45 4.8628 0.00 -0.25 0.00 -0.08
46 5.0293 0.00 -0.08 0.00 -0.08
47 5.0293 0.00 -0.03 0.00 -0.15
48 5.0293 0.00 -0.00 0.00 -0.04
49 5.0294 0.00 -0.04 0.00 -0.03
50 5.0866 0.00 0.03 0.00 -0.11
51 5.0866 0.00 0.01 0.00 -0.05
52 5.0867 0.00 0.12 0.00 -0.07
53 5.0867 0.00 0.04 0.00 -0.03
54 5.0921 0.00 -0.12 0.00 -0.07
55 5.0921 0.00 -0.03 0.00 0.04
56 5.0921 0.00 0.00 0.00 -0.08
57 5.0921 0.00 -0.00 0.00 0.07
58 5.1632 0.00 0.01 0.00 0.07
59 5.1632 0.00 0.08 0.00 0.06
60 5.1633 0.00 0.14 0.00 -0.03
61 5.1633 0.00 0.10 0.00 -0.01
62 5.1714 0.00 0.05 0.00 0.06
63 5.1715 0.00 0.03 0.00 0.13
64 5.1715 0.00 0.01 0.00 0.07
65 5.1715 0.00 0.31 0.00 0.04
66 5.2397 0.00 -0.49 0.00 -0.31
67 5.2452 0.00 -0.04 0.00 -0.04
68 5.8565 0.00 -0.08 0.00 0.10
69 5.9822 0.00 0.04 0.00 -0.12
70 6.0806 0.00 -0.02 0.00 -0.14
71 6.0807 0.00 0.13 0.00 -0.11
72 6.0807 0.00 -0.03 0.00 -0.04
73 6.0807 0.00 -0.06 0.00 -0.06
74 6.0942 0.00 0.02 0.00 0.05
75 6.2745 0.00 0.14 0.00 -0.12
76 6.9597 0.00 -0.08 0.00 -0.38
77 6.9844 0.00 0.06 0.00 -0.12
78 6.9844 0.00 0.04 0.00 0.08
79 6.9845 0.00 -0.05 0.00 0.01
80 6.9845 0.00 -0.36 0.00 -0.19
81 7.0255 0.00 0.12 0.00 -0.24
82 7.0470 0.00 -0.02 0.00 0.02
83 7.1126 0.00 0.07 0.00 -0.00
84 7.1126 0.00 -0.01 0.00 0.02
85 7.1126 0.00 -0.06 0.00 0.06
86 7.2083 0.00 -0.03 0.00 0.12
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.
523717 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.117 39.117 39.117 ecceobj 0.195 0.195 0.195 incobj 9.673 9.673 9.673 qmin 30.013 30.013 30.013 qmax 49.177 49.178 49.177 amean 39.455 39.455 39.455 amin 39.117 39.117 39.117 amax 39.853 39.853 39.854 emean 0.213 0.213 0.213 emin 0.191 0.191 0.191 emax 0.236 0.236 0.236 imean 7.153 7.153 7.154 imin 6.195 6.194 6.195 imax 8.154 8.154 8.154 excite_mean 0.247 0.247 0.247 fracstop 1.000 1.000 1.000 cjmean 2.983 2.983 2.983 libcent 0 180.4 180.4 180.4 libamp 0 20.4 20.2 20.6 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 171.6 171.6 171.6 kozaiamp 180.0 180.0 180.0