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: 531224
# Created Wed Dec 25 02:07:23 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 74 observations of 74
# Arc: 20.36y
# First observation: 2000/02/12
# Last observation: 2020/06/24
# Chi-squared of fit: 62.96 DOF: 142 RMS: 0.16
# Min/Max residuals: -0.67 0.34
# Exact a, adot, b, bdot, g, gdot:
1.643212E-05 2.480685E-02 -3.211229E-07 -1.019382E-03 2.362613E-02 -5.334440E-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
4.291668 -164.551251 0.780891 0.045406 -0.608159 2451586.969873
# Heliocentric elements and errors
Epoch: 2451586.5000 = 2000/02/12
Mean Anomaly: 331.12389 +/- 0.000
Argument of Peri: 174.84922 +/- 0.000
Long of Asc Node: 75.74715 +/- 0.000
Inclination: 4.81875 +/- 0.000
Eccentricity: 0.33216784 +/- 0.0000
Semi-Major Axis: 57.15755879 +/- 0.0000
Time of Perihelion: 2464246.8332 +/- 0.0
Perihelion: 38.17165583 +/- 0.0000
Aphelion: 76.14346175 +/- 0.0000
Period (y) 432.1343 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -41.47108948 +/- 0.0000
Ecliptic Y -10.65037905 +/- 0.0000
Ecliptic Z 3.16742959 +/- 0.0000
Ecliptic XDOT 0.00134565 +/- 0.0000
Ecliptic YDOT -0.00260188 +/- 0.0000
Ecliptic ZDOT -0.00016395 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 42.93400044 +/- 0.0000
Geocenter to KBO 42.32619342 +/- 0.0000
# Hcoef: 6.74
The following table shows the complete astrometric record for 531224. 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 (531224) followed by the observatory code and reference code for the source of the astrometry.
2000 02 12.469130 13 03 31.79 -02 07 14.1 531224 645 C~2VVJ 2000 02 12.469959 13 03 31.78 -02 07 14.1 531224 645 C~2VVJ 2012 04 27.41277 14 05 58.109 -09 09 45.25 21.7i 531224 F51 C~1w3q 2012 04 27.42540 14 05 58.026 -09 09 45.18 22.6w 531224 F51 C~1w3q 2012 04 27.44036 14 05 57.967 -09 09 44.73 22.5w 531224 F51 C~1w3q 2012 04 27.47033 14 05 57.826 -09 09 43.76 22.6w 531224 F51 C~1w3q 2012 05 21.36269 14 04 11.322 -09 01 13.85 22.9w 531224 F51 C~1w3q 2012 05 21.37720 14 04 11.264 -09 01 13.46 23.1w 531224 F51 C~1w3q 2013 05 09.41428 14 11 07.387 -09 43 52.11 22.5w 531224 F51 C~1w3q 2013 05 09.42825 14 11 07.350 -09 43 51.96 22.3w 531224 F51 C~1w3q 2013 05 09.44222 14 11 07.299 -09 43 51.44 22.6w 531224 F51 C~1w3q 2013 07 28.27408 14 08 11.116 -09 34 57.04 23.0G 531224 F51 C~2rXt 2014 03 27.53010 14 20 32.810 -10 38 58.12 22.4w 531224 F51 C~1w3q 2014 03 27.55230 14 20 32.721 -10 38 57.62 22.4w 531224 F51 C~1w3q 2014 04 05.52255 14 19 55.438 -10 35 37.04 22.6w 531224 F51 C~1w3q 2014 04 05.54366 14 19 55.344 -10 35 36.49 22.6w 531224 F51 C~1w3q 2014 04 05.55423 14 19 55.302 -10 35 36.29 22.7w 531224 F51 C~1w3q 2014 05 21.33305 14 16 23.791 -10 18 27.91 23.1G 531224 F51 C~2rXt 2014 05 21.34657 14 16 23.746 -10 18 27.72 23.2G 531224 F51 C~2rXt 2014 05 21.36004 14 16 23.675 -10 18 27.44 22.6G 531224 F51 C~2rXt 2014 05 21.37350 14 16 23.591 -10 18 27.14 531224 F51 C~2rXt 2014 05 27.35789 14 15 58.802 -10 16 40.10 23.4G 531224 F51 C~2rXt 2014 05 27.36900 14 15 58.747 -10 16 39.78 22.5G 531224 F51 C~2rXt 2014 05 29.38507 14 15 50.787 -10 16 06.21 23.3G 531224 F51 C~2rXt 2014 06 06.35440 14 15 21.458 -10 14 07.67 23.0G 531224 F51 C~2rXt 2014 06 18.34614 14 14 45.069 -10 11 56.51 22.4G 531224 F51 C~2rXt 2014 06 28.28748 14 14 23.136 -10 10 55.83 23.0G 531224 F51 C~2rXt 2014 06 28.29823 14 14 23.111 -10 10 55.72 22.8G 531224 F51 C~2rXt 2014 06 28.30895 14 14 23.080 -10 10 55.67 22.8G 531224 F51 C~2rXt 2014 06 28.31968 14 14 23.069 -10 10 55.50 22.6G 531224 F51 C~2rXt 2015 03 17.57847 14 27 23.058 -11 20 27.07 23.2G 531224 F51 C~2rXt 2015 03 18.56476 14 27 19.859 -11 20 08.65 22.4G 531224 F51 C~2rXt 2015 03 19.56331 14 27 16.544 -11 19 50.15 23.3G 531224 F51 C~2rXt 2015 04 23.39143 14 24 48.894 -11 07 06.36 22.2G 531224 F51 C~2rXt 2015 04 24.51677 14 24 43.521 -11 06 40.02 23.2w 531224 F51 C~2rXt 2015 04 25.45626 14 24 38.993 -11 06 18.30 23.0G 531224 F51 C~2rXt 2015 05 24.36028 14 22 24.676 -10 56 04.15 22.7G 531224 F51 C~2rXt 2015 06 13.33606 14 21 10.055 -10 51 07.15 19.4G 531224 F51 C~2rXt 2016 02 10.59998 14 34 37.926 -12 04 39.25 23.8G 531224 F51 C~2rXt 2016 02 20.64665 14 34 33.517 -12 03 42.45 22.7G 531224 F51 C~2rXt 2016 03 06.52350 14 34 09.241 -12 00 58.18 22.7G 531224 F51 C~2rXt 2016 03 06.53512 14 34 09.197 -12 00 58.31 22.8G 531224 F51 C~2rXt 2016 03 06.54676 14 34 09.172 -12 00 58.00 22.7G 531224 F51 C~2rXt 2016 03 06.55838 14 34 09.138 -12 00 57.80 23.2G 531224 F51 C~2rXt 2016 03 13.56209 14 33 50.928 -11 59 11.35 22.6G 531224 F51 C~2rXt 2016 03 13.57454 14 33 50.895 -11 59 11.17 22.7G 531224 F51 C~2rXt 2016 04 05.51236 14 32 27.084 -11 51 46.87 22.4G 531224 F51 C~2rXt 2016 04 17.45734 14 31 33.096 -11 47 20.56 22.0G 531224 F51 C~2rXt 2016 04 30.41197 14 30 31.021 -11 42 25.63 22.5G 531224 F51 C~2rXt 2016 04 30.42457 14 30 30.944 -11 42 25.34 22.9G 531224 F51 C~2rXt 2016 04 30.43719 14 30 30.910 -11 42 24.97 22.2G 531224 F51 C~2rXt 2016 04 30.44981 14 30 30.841 -11 42 24.87 22.4G 531224 F51 C~2rXt 2016 05 07.39252 14 29 57.288 -11 39 51.27 22.5G 531224 F51 C~2rXt 2016 05 07.40355 14 29 57.260 -11 39 51.12 22.4G 531224 F51 C~2rXt 2016 05 07.41461 14 29 57.214 -11 39 50.93 22.4G 531224 F51 C~2rXt 2016 05 07.42566 14 29 57.169 -11 39 50.48 22.3G 531224 F51 C~2rXt 2016 06 29.28189 14 26 41.551 -11 27 05.42 23.0G 531224 F51 C~2rXt 2016 06 29.29428 14 26 41.530 -11 27 05.38 22.3G 531224 F51 C~2rXt 2016 06 29.30659 14 26 41.503 -11 27 05.29 22.6G 531224 F51 C~2rXt 2016 06 29.31887 14 26 41.497 -11 27 05.22 22.8G 531224 F51 C~2rXt 2017 02 24.61333 14 40 48.366 -12 40 14.80 23.0G 531224 F51 C~2rXt 2017 03 22.46146 14 39 46.689 -12 34 18.78 22.9G 531224 F51 C~2rXt 2017 04 05.48811 14 38 52.598 -12 29 44.00 22.6G 531224 F51 C~2rXt 2017 04 20.43943 14 37 44.902 -12 24 19.24 23.3G 531224 F51 C~2rXt 2017 05 27.31076 14 34 50.359 -12 11 32.15 23.0G 531224 F51 C~2rXt 2018 03 18.53782 14 46 28.023 -13 12 48.20 22.5G 531224 F51 C~2rXt 2018 04 12.53720 14 44 52.180 -13 04 57.66 23.1G 531224 F51 C~2rXt 2018 05 19.37927 14 41 55.306 -12 51 57.23 22.5G 531224 F51 C~2rXt 2020 06 21.29245 14 52 46.929 -13 58 16.36 22.4w 531224 F52 C~3yK1 2020 06 21.30429 14 52 46.883 -13 58 16.53 22.2w 531224 F52 C~3yK1 2020 06 21.31610 14 52 46.835 -13 58 16.23 22.4w 531224 F52 C~3yK1 2020 06 24.29044 14 52 37.628 -13 57 48.02 22.6w 531224 F51 C~3ywr 2020 06 24.30147 14 52 37.627 -13 57 47.75 22.5w 531224 F51 C~3ywr 2020 06 24.31252 14 52 37.589 -13 57 47.94 22.6w 531224 F51 C~3ywr
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 -0.08
2 0.0000 0.00 -0.12 0.00 -0.10
3 12.2052 0.00 0.34 0.00 0.19
4 12.2052 0.00 0.01 0.00 -0.04
5 12.2053 0.00 0.19 0.00 0.05
6 12.2053 0.00 0.23 0.00 0.31
7 12.2708 0.00 0.00 0.00 -0.07
8 12.2708 0.00 0.03 0.00 0.06
9 13.2374 0.00 -0.31 0.00 0.17
10 13.2374 0.00 0.12 0.00 0.01
11 13.2374 0.00 0.33 0.00 0.23
12 13.4560 0.00 -0.01 0.00 0.18
13 14.1193 0.00 0.09 0.00 0.15
14 14.1193 0.00 0.09 0.00 0.17
15 14.1439 0.00 0.07 0.00 0.03
16 14.1439 0.00 0.06 0.00 0.09
17 14.1440 0.00 0.14 0.00 0.05
18 14.2693 0.00 -0.11 0.00 -0.06
19 14.2693 0.00 0.10 0.00 -0.12
20 14.2694 0.00 -0.09 0.00 -0.09
21 14.2694 0.00 -0.46 0.00 -0.05
22 14.2858 0.00 0.01 0.00 -0.27
23 14.2858 0.00 -0.14 0.00 -0.14
24 14.2914 0.00 0.14 0.00 -0.13
25 14.3132 0.00 -0.09 0.00 -0.11
26 14.3460 0.00 -0.34 0.00 -0.02
27 14.3732 0.00 0.15 0.00 -0.10
28 14.3732 0.00 0.08 0.00 -0.03
29 14.3733 0.00 -0.08 0.00 -0.02
30 14.3733 0.00 0.06 0.00 0.11
31 15.0913 0.00 -0.06 0.00 -0.01
32 15.0940 0.00 0.15 0.00 0.23
33 15.0968 0.00 0.28 0.00 0.05
34 15.1921 0.00 -0.02 0.00 -0.02
35 15.1952 0.00 0.33 0.00 0.18
36 15.1978 0.00 -0.12 0.00 0.12
37 15.2769 0.00 -0.04 0.00 -0.05
38 15.3316 0.00 -0.19 0.00 -0.11
39 15.9949 0.00 -0.14 0.00 -0.04
40 16.0224 0.00 0.07 0.00 -0.11
41 16.0631 0.00 0.20 0.00 0.14
42 16.0632 0.00 -0.04 0.00 -0.15
43 16.0632 0.00 0.00 0.00 -0.00
44 16.0632 0.00 -0.09 0.00 0.03
45 16.0824 0.00 -0.02 0.00 0.07
46 16.0824 0.00 0.04 0.00 0.04
47 16.1452 0.00 -0.18 0.00 -0.16
48 16.1779 0.00 -0.37 0.00 -0.67
49 16.2134 0.00 -0.06 0.00 0.04
50 16.2134 0.00 -0.28 0.00 0.05
51 16.2135 0.00 0.14 0.00 0.13
52 16.2135 0.00 0.04 0.00 -0.05
53 16.2325 0.00 -0.54 0.00 0.17
54 16.2325 0.00 -0.15 0.00 0.08
55 16.2326 0.00 -0.03 0.00 0.03
56 16.2326 0.00 0.10 0.00 0.24
57 16.3773 0.00 -0.03 0.00 -0.09
58 16.3773 0.00 0.04 0.00 -0.11
59 16.3774 0.00 0.02 0.00 -0.07
60 16.3774 0.00 0.30 0.00 -0.06
61 17.0353 0.00 -0.27 0.00 -0.13
62 17.1061 0.00 0.11 0.00 -0.22
63 17.1445 0.00 -0.05 0.00 0.12
64 17.1854 0.00 -0.03 0.00 -0.21
65 17.2864 0.00 -0.07 0.00 -0.08
66 18.0946 0.00 -0.05 0.00 0.04
67 18.1631 0.00 -0.08 0.00 -0.15
68 18.2640 0.00 -0.04 0.00 0.17
69 20.3554 0.00 0.17 0.00 0.10
70 20.3555 0.00 0.06 0.00 -0.18
71 20.3555 0.00 -0.07 0.00 -0.00
72 20.3636 0.00 -0.22 0.00 0.09
73 20.3637 0.00 0.28 0.00 0.26
74 20.3637 0.00 0.22 0.00 -0.02
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.
531224 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 57.149 57.149 57.149 ecceobj 0.332 0.332 0.332 incobj 4.819 4.819 4.819 qmin 37.670 37.660 37.640 qmax 78.747 78.669 78.688 amean 57.654 57.655 57.661 amin 56.999 56.987 56.966 amax 58.488 58.476 58.468 emean 0.334 0.334 0.334 emin 0.323 0.323 0.323 emax 0.346 0.346 0.346 imean 3.140 3.143 3.140 imin 2.797 2.782 2.767 imax 3.579 3.579 3.579 excite_mean 0.339 0.339 0.339 fracstop 1.000 1.000 1.000 cjmean 3.127 3.127 3.127 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 200.7 199.3 197.4 kozaiamp 180.0 180.0 180.0