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: 535229
# Created Fri Nov 22 02:07:30 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 64 observations of 64
# Arc: 11.16y
# First observation: 2011/12/23
# Last observation: 2023/02/20
# Chi-squared of fit: 54.78 DOF: 122 RMS: 0.16
# Min/Max residuals: -0.66 0.55
# Exact a, adot, b, bdot, g, gdot:
1.822955E-05 3.429976E-02 -5.803763E-06 -1.068094E-02 3.092535E-02 4.535172E-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
8.546630 99.079637 0.134787 0.144661 -0.962393 2455918.877176
# Heliocentric elements and errors
Epoch: 2455918.5000 = 2011/12/23
Mean Anomaly: 30.53088 +/- 0.000
Argument of Peri: 108.51740 +/- 0.000
Long of Asc Node: 303.81188 +/- 0.000
Inclination: 19.05687 +/- 0.000
Eccentricity: 0.20101089 +/- 0.0000
Semi-Major Axis: 39.61238573 +/- 0.0000
Time of Perihelion: 2448195.5757 +/- 0.0
Perihelion: 31.64986485 +/- 0.0000
Aphelion: 47.57490661 +/- 0.0000
Period (y) 249.3186 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -5.06396322 +/- 0.0000
Ecliptic Y 32.55968635 +/- 0.0000
Ecliptic Z 4.80536614 +/- 0.0000
Ecliptic XDOT -0.00308757 +/- 0.0000
Ecliptic YDOT 0.00005636 +/- 0.0000
Ecliptic ZDOT -0.00087534 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 33.29960223 +/- 0.0000
Geocenter to KBO 32.33589362 +/- 0.0000
# Hcoef: 7.13
The following table shows the complete astrometric record for 535229. 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 (535229) followed by the observatory code and reference code for the source of the astrometry.
2011 12 23.37641 06 42 15.267 +31 39 12.86 22.1G 535229 F51 C~2rYH 2012 01 03.34691 06 40 56.150 +31 39 27.02 23.2G 535229 F51 C~2rYH 2012 12 31.50519 06 50 06.200 +30 53 25.44 22.5G 535229 F51 C~2rYH 2013 01 01.51402 06 49 58.978 +30 53 27.80 23.1G 535229 F51 C~2rYH 2013 01 10.46715 06 48 55.232 +30 53 32.05 21.9G 535229 F51 C~2rYH 2013 04 11.25775 06 44 27.790 +30 33 01.12 22.8G 535229 F51 C~2rYH 2013 09 14.62090 07 03 08.248 +29 52 47.35 22.6G 535229 F51 C~2rYH 2013 11 25.54628 07 02 35.657 +30 01 04.92 22.4G 535229 F51 C~2rYH 2013 12 04.42972 07 01 47.748 +30 02 30.07 22.6w 535229 F51 C~1vXz 2013 12 04.44367 07 01 47.667 +30 02 30.09 22.4w 535229 F51 C~1vXz 2013 12 04.45766 07 01 47.587 +30 02 30.36 22.3w 535229 F51 C~1vXz 2013 12 04.47165 07 01 47.517 +30 02 30.67 22.4w 535229 F51 C~1vXz 2013 12 26.37431 06 59 25.725 +30 05 12.65 22.1w 535229 F51 C~1vXz 2013 12 26.37499 06 59 25.729 +30 05 12.60 22.1w 535229 F51 C~1vXz 2013 12 26.38973 06 59 25.617 +30 05 12.75 22.4w 535229 F51 C~1vXz 2013 12 26.39042 06 59 25.623 +30 05 12.78 22.2w 535229 F51 C~1vXz 2013 12 26.40517 06 59 25.510 +30 05 12.71 22.6w 535229 F51 C~1vXz 2013 12 26.40585 06 59 25.512 +30 05 12.87 22.4w 535229 F51 C~1vXz 2014 11 20.63391 07 11 20.390 +29 10 16.80 22.5G 535229 F51 C~2rYH 2014 12 26.52041 07 07 54.228 +29 15 39.28 22.2w 535229 F51 C~1vXz 2014 12 26.53273 07 07 54.147 +29 15 39.24 22.5w 535229 F51 C~1vXz 2014 12 26.54502 07 07 54.065 +29 15 39.44 22.4w 535229 F51 C~1vXz 2015 01 18.28845 07 05 16.683 +29 17 10.55 22.5G 535229 F51 C~2rYH 2015 01 20.32299 07 05 02.989 +29 17 12.01 21.9w 535229 F51 C~1vXz 2015 01 20.33492 07 05 02.899 +29 17 11.97 22.3w 535229 F51 C~1vXz 2015 01 20.34682 07 05 02.812 +29 17 11.92 22.2w 535229 F51 C~1vXz 2015 01 20.35877 07 05 02.728 +29 17 11.86 22.2w 535229 F51 C~1vXz 2015 01 22.29898 07 04 49.807 +29 17 12.29 22.5w 535229 F51 C~1vXz 2015 01 22.31086 07 04 49.718 +29 17 12.21 22.5w 535229 F51 C~1vXz 2015 01 22.32274 07 04 49.648 +29 17 12.26 22.4w 535229 F51 C~1vXz 2015 01 28.32475 07 04 10.797 +29 17 05.89 22.5G 535229 F51 C~2rYH 2015 09 17.59185 07 19 16.021 +28 14 35.33 23.1G 535229 F51 C~2rYH 2015 12 04.62718 07 18 23.572 +28 21 16.90 22.4G 535229 F51 C~2rYH 2016 02 09.26371 07 11 17.413 +28 26 45.58 22.2G 535229 F51 C~2rYH 2016 02 09.27788 07 11 17.318 +28 26 45.53 22.5G 535229 F51 C~2rYH 2016 02 09.29212 07 11 17.263 +28 26 45.40 21.9G 535229 F51 C~2rYH 2016 02 09.30643 07 11 17.172 +28 26 45.50 22.3G 535229 F51 C~2rYH 2017 01 28.43494 07 20 26.744 +27 35 43.96 22.4G 535229 F51 C~2rYH 2017 01 28.44719 07 20 26.669 +27 35 43.30 22.9G 535229 F51 C~2rYH 2017 01 28.45950 07 20 26.552 +27 35 43.69 23.0G 535229 F51 C~2rYH 2017 01 28.47181 07 20 26.466 +27 35 43.58 22.8G 535229 F51 C~2rYH 2017 12 20.47108 07 32 34.360 +26 38 06.62 22.4R 535229 G37 C~2Uxt 2017 12 20.51274 07 32 34.098 +26 38 06.99 535229 G37 C~2Uxt 2017 12 25.53683 07 32 02.799 +26 38 57.67 22.3G 535229 F51 C~2rYH 2017 12 25.54894 07 32 02.729 +26 38 58.00 22.2G 535229 F51 C~2rYH 2017 12 25.56105 07 32 02.644 +26 38 58.15 21.8G 535229 F51 C~2rYH 2017 12 25.57317 07 32 02.567 +26 38 58.27 21.7G 535229 F51 C~2rYH 2018 01 08.37682 07 30 31.852 +26 41 04.65 22.2G 535229 F51 C~2rYH 2018 01 15.32999 07 29 45.114 +26 41 57.78 22.2G 535229 F51 C~2rYH 2018 01 15.33129 07 29 45.097 +26 41 57.64 22.3G 535229 F51 C~2rYI 2018 01 15.34250 07 29 45.013 +26 41 57.91 23.1G 535229 F51 C~2rYI 2018 01 15.34379 07 29 45.001 +26 41 57.62 21.7G 535229 F51 C~2rYI 2018 01 15.35499 07 29 44.940 +26 41 57.76 22.0G 535229 F51 C~2rYI 2018 01 15.35628 07 29 44.931 +26 41 57.61 21.4G 535229 F51 C~2rYI 2018 01 15.36747 07 29 44.867 +26 41 57.87 22.1G 535229 F51 C~2rYI 2018 01 15.36876 07 29 44.843 +26 41 58.20 22.6G 535229 F51 C~2rYI 2018 02 20.24791 07 26 10.657 +26 43 26.99 19.9G 535229 F51 C~2rYI 2018 02 20.27293 07 26 10.566 +26 43 27.07 22.9G 535229 F51 C~2rYI 2020 12 09.410900 07 55 39.129 +23 50 37.10 22.6G 535229 G37 C~4Tuj 2020 12 09.462430 07 55 38.864 +23 50 37.88 535229 G37 C~4Tuj 2020 12 09.507100 07 55 38.660 +23 50 38.52 535229 G37 C~4Tuj 2023 02 20.136030 08 02 30.449 +22 10 40.90 22.5G 535229 G37 C~6IlA 2023 02 20.180810 08 02 30.220 +22 10 41.18 535229 G37 C~6IlA 2023 02 20.226490 08 02 29.984 +22 10 41.55 535229 G37 C~6IlA
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 -0.16 0.00 0.08
2 0.0300 0.00 -0.14 0.00 -0.06
3 1.0243 0.00 0.19 0.00 -0.17
4 1.0271 0.00 0.05 0.00 0.16
5 1.0516 0.00 -0.25 0.00 -0.35
6 1.3002 0.00 0.27 0.00 -0.06
7 1.7283 0.00 0.10 0.00 -0.02
8 1.9252 0.00 0.35 0.00 -0.17
9 1.9495 0.00 -0.19 0.00 0.08
10 1.9495 0.00 -0.18 0.00 -0.04
11 1.9496 0.00 -0.14 0.00 0.10
12 1.9496 0.00 0.05 0.00 0.28
13 2.0096 0.00 -0.13 0.00 0.06
14 2.0096 0.00 0.01 0.00 0.00
15 2.0096 0.00 -0.11 0.00 0.07
16 2.0096 0.00 0.05 0.00 0.10
17 2.0097 0.00 -0.08 0.00 -0.06
18 2.0097 0.00 0.02 0.00 0.10
19 2.9110 0.00 0.01 0.00 0.05
20 3.0093 0.00 -0.00 0.00 0.06
21 3.0093 0.00 0.06 0.00 -0.05
22 3.0094 0.00 0.11 0.00 0.07
23 3.0716 0.00 -0.25 0.00 0.09
24 3.0772 0.00 0.24 0.00 0.05
25 3.0772 0.00 0.11 0.00 0.01
26 3.0773 0.00 0.03 0.00 -0.05
27 3.0773 0.00 -0.01 0.00 -0.12
28 3.0826 0.00 0.07 0.00 0.07
29 3.0826 0.00 -0.07 0.00 -0.01
30 3.0827 0.00 0.08 0.00 0.03
31 3.0991 0.00 -0.04 0.00 0.05
32 3.7350 0.00 -0.29 0.00 0.21
33 3.9487 0.00 0.00 0.00 -0.21
34 4.1311 0.00 0.03 0.00 -0.11
35 4.1311 0.00 -0.20 0.00 -0.11
36 4.1312 0.00 0.18 0.00 -0.20
37 4.1312 0.00 0.03 0.00 -0.06
38 5.1008 0.00 0.48 0.00 0.55
39 5.1008 0.00 0.54 0.00 -0.14
40 5.1008 0.00 -0.03 0.00 0.23
41 5.1009 0.00 -0.13 0.00 0.10
42 5.9934 0.00 0.07 0.00 0.04
43 5.9935 0.00 -0.00 0.00 -0.00
44 6.0073 0.00 -0.03 0.00 -0.19
45 6.0073 0.00 0.10 0.00 0.02
46 6.0074 0.00 -0.01 0.00 0.06
47 6.0074 0.00 0.01 0.00 0.06
48 6.0452 0.00 -0.02 0.00 -0.14
49 6.0642 0.00 0.05 0.00 0.07
50 6.0642 0.00 -0.07 0.00 -0.08
51 6.0642 0.00 -0.19 0.00 0.11
52 6.0643 0.00 -0.24 0.00 -0.19
53 6.0643 0.00 -0.01 0.00 -0.13
54 6.0643 0.00 -0.01 0.00 -0.29
55 6.0643 0.00 0.17 0.00 -0.11
56 6.0643 0.00 -0.05 0.00 0.21
57 6.1626 0.00 -0.66 0.00 -0.15
58 6.1626 0.00 -0.22 0.00 -0.01
59 8.9638 0.00 0.18 0.00 -0.26
60 8.9640 0.00 -0.05 0.00 -0.00
61 8.9641 0.00 0.12 0.00 0.19
62 11.1616 0.00 -0.06 0.00 0.07
63 11.1617 0.00 0.03 0.00 0.02
64 11.1618 0.00 0.08 0.00 0.06
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.
535229 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.757 39.757 39.756 ecceobj 0.204 0.204 0.204 incobj 19.058 19.058 19.058 qmin 27.196 27.196 27.197 qmax 52.478 52.475 52.470 amean 39.455 39.455 39.455 amin 39.004 39.003 39.005 amax 40.000 39.997 39.998 emean 0.253 0.254 0.254 emin 0.179 0.179 0.179 emax 0.312 0.312 0.312 imean 18.086 18.084 18.085 imin 15.684 15.680 15.687 imax 20.865 20.865 20.865 excite_mean 0.403 0.403 0.403 fracstop 1.000 1.000 1.000 cjmean 2.866 2.866 2.866 libcent 0 178.5 178.7 178.6 libamp 0 91.1 91.3 91.1 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 89.4 89.4 89.5 kozaiamp 71.3 71.4 71.3