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: 535230 # Created Sun Nov 24 02:07:27 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 83 observations of 83 # Arc: 13.48y # First observation: 2010/11/09 # Last observation: 2024/05/02 # Chi-squared of fit: 87.30 DOF: 160 RMS: 0.18 # Min/Max residuals: -0.81 0.77 # Exact a, adot, b, bdot, g, gdot: 1.417645E-05 2.377717E-02 1.078798E-05 1.821871E-02 2.593097E-02 2.180241E-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 16.392708 123.438508 0.960106 0.066306 -0.225380 2455510.138066 # Heliocentric elements and errors Epoch: 2455510.5000 = 2010/11/10 Mean Anomaly: 6.23901 +/- 0.000 Argument of Peri: 12.74689 +/- 0.000 Long of Asc Node: 102.10174 +/- 0.000 Inclination: 40.71084 +/- 0.000 Eccentricity: 0.31987789 +/- 0.0000 Semi-Major Axis: 56.70634272 +/- 0.0000 Time of Perihelion: 2452807.4192 +/- 0.0 Perihelion: 38.56723724 +/- 0.0000 Aphelion: 74.84544819 +/- 0.0000 Period (y) 427.0273 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -19.71096165 +/- 0.0000 Ecliptic Y 31.59625271 +/- 0.0000 Ecliptic Z 10.88386468 +/- 0.0000 Ecliptic XDOT -0.00191771 +/- 0.0000 Ecliptic YDOT -0.00164576 +/- 0.0000 Ecliptic ZDOT 0.00191034 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 38.79820587 +/- 0.0000 Geocenter to KBO 38.56390221 +/- 0.0000 # Hcoef: 6.20
The following table shows the complete astrometric record for 535230. 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 (535230) followed by the observatory code and reference code for the source of the astrometry.
2010 11 09.63730 08 41 24.174 +35 15 57.83 21.9G 535230 F51 C~2rYI 2011 01 15.49061 08 37 24.685 +36 01 01.45 22.4G 535230 F51 C~2rYI 2011 10 26.61118 08 48 57.780 +35 45 00.00 20.9G 535230 F51 C~2rYI 2011 11 25.64995 08 49 03.655 +36 03 50.94 21.6G 535230 F51 C~2rYI 2011 12 23.62846 08 47 33.095 +36 24 15.10 22.0G 535230 F51 C~2rYI 2012 02 11.38979 08 42 41.514 +36 53 07.38 22.4G 535230 F51 C~2rYI 2012 02 15.40474 08 42 17.326 +36 54 31.20 21.1G 535230 F51 C~2rYI 2012 02 28.29897 08 41 04.960 +36 57 48.11 22.1G 535230 F51 C~2rYI 2012 02 28.31093 08 41 04.915 +36 57 48.42 22.3G 535230 F51 C~2rYI 2012 12 22.60925 08 55 40.657 +37 00 03.94 22.8G 535230 F51 C~2rYI 2013 01 11.55070 08 53 56.809 +37 14 15.40 21.1G 535230 F51 C~2rYI 2013 02 01.43603 08 51 48.200 +37 26 22.56 21.9G 535230 F51 C~2rYI 2013 02 14.31430 08 50 28.313 +37 31 45.47 22.0r 535230 F51 C~2VW8 2013 02 14.32635 08 50 28.258 +37 31 45.92 22.0r 535230 F51 C~2VW8 2013 02 14.33979 08 50 28.187 +37 31 46.07 22.2g 535230 F51 C~2VW8 2014 01 20.52408 09 01 19.866 +37 54 15.76 21.2G 535230 F51 C~2rYI 2014 03 02.28561 08 57 13.119 +38 11 11.06 21.9G 535230 F51 C~2rYI 2014 11 09.63708 09 13 18.740 +37 32 06.67 22.2G 535230 F51 C~2rYI 2014 12 26.56993 09 11 54.958 +38 07 58.05 22.1G 535230 F51 C~2rYI 2014 12 26.58261 09 11 54.922 +38 07 58.83 22.0w 535230 F51 C~1vXz 2014 12 26.59569 09 11 54.870 +38 07 59.23 22.4w 535230 F51 C~1vXz 2014 12 26.60837 09 11 54.812 +38 07 59.68 22.4w 535230 F51 C~1vXz 2015 01 13.55320 09 10 23.198 +38 21 32.35 21.3i 535230 F51 C~1vXz 2015 01 13.57704 09 10 23.073 +38 21 33.43 21.5i 535230 F51 C~1vXz 2015 01 13.58888 09 10 23.005 +38 21 34.05 21.4i 535230 F51 C~1vXz 2015 01 27.42358 09 08 59.880 +38 30 34.86 21.7i 535230 F51 C~1vXz 2015 01 27.43607 09 08 59.792 +38 30 34.98 21.6i 535230 F51 C~1vXz 2015 01 27.44856 09 08 59.714 +38 30 35.64 21.5i 535230 F51 C~1vXz 2015 03 20.29329 09 04 07.656 +38 45 47.08 21.9G 535230 F51 C~2rYI 2015 03 20.30540 09 04 07.617 +38 45 47.13 22.2G 535230 F51 C~2rYI 2015 03 20.31756 09 04 07.555 +38 45 47.05 22.5G 535230 F51 C~2rYI 2015 03 20.32975 09 04 07.518 +38 45 47.03 22.2G 535230 F51 C~2rYI 2015 03 22.29989 09 03 59.789 +38 45 42.40 21.6G 535230 F51 C~2rYI 2015 03 22.31203 09 03 59.734 +38 45 42.42 21.7G 535230 F51 C~2rYI 2015 03 22.33645 09 03 59.652 +38 45 42.26 21.9G 535230 F51 C~2rYI 2015 05 03.25076 09 02 59.125 +38 34 18.59 22.1G 535230 F51 C~2rYI 2015 11 17.61572 09 21 35.593 +38 05 55.23 22.2G 535230 F51 C~2rYI 2015 12 03.66865 09 21 25.458 +38 18 10.78 21.1G 535230 F51 C~2rYI 2015 12 12.57310 09 21 06.136 +38 25 25.53 22.4G 535230 F51 C~2rYI 2015 12 12.58436 09 21 06.114 +38 25 26.08 21.9G 535230 F51 C~2rYI 2015 12 12.59568 09 21 06.070 +38 25 26.66 22.0G 535230 F51 C~2rYI 2015 12 12.60705 09 21 06.049 +38 25 27.25 22.3G 535230 F51 C~2rYI 2015 12 31.54462 09 19 55.897 +38 40 58.34 21.4G 535230 F51 C~2rYI 2016 01 27.53087 09 17 26.522 +39 00 30.22 21.6G 535230 F51 C~2rYI 2016 02 12.34329 09 15 47.386 +39 08 58.90 22.2G 535230 F51 C~2rYI 2016 02 12.35476 09 15 47.319 +39 08 59.04 22.3G 535230 F51 C~2rYI 2016 02 12.36751 09 15 47.232 +39 08 59.48 22.3G 535230 F51 C~2rYI 2016 02 12.37897 09 15 47.155 +39 09 00.04 22.2G 535230 F51 C~2rYI 2016 02 24.42619 09 14 33.577 +39 13 29.06 22.1G 535230 F51 C~2rYI 2016 11 26.63194 09 29 51.203 +38 39 33.01 21.8G 535230 F51 C~2rYI 2016 12 22.59397 09 28 55.135 +39 01 03.16 22.0G 535230 F51 C~2rYI 2016 12 22.60596 09 28 55.096 +39 01 04.05 22.0G 535230 F51 C~2rYI 2016 12 22.61793 09 28 55.038 +39 01 04.30 21.9G 535230 F51 C~2rYI 2016 12 22.62989 09 28 54.994 +39 01 05.09 22.3G 535230 F51 C~2rYI 2017 02 01.42130 09 25 21.214 +39 31 37.49 22.0G 535230 F51 C~2rYI 2017 11 19.61184 09 38 10.269 +38 57 56.49 22.4G 535230 F51 C~2rYI 2017 11 19.62285 09 38 10.264 +38 57 57.01 22.2G 535230 F51 C~2rYI 2017 12 13.53847 09 37 49.003 +39 17 23.67 22.1G 535230 F51 C~2rYI 2017 12 13.54948 09 37 48.972 +39 17 24.05 22.2G 535230 F51 C~2rYI 2017 12 13.56052 09 37 48.944 +39 17 24.62 22.1G 535230 F51 C~2rYI 2017 12 13.57162 09 37 48.905 +39 17 25.04 23.0G 535230 F51 C~2rYI 2017 12 20.46488 09 37 29.862 +39 23 21.62 22.2R 535230 G37 C~2VW8 2017 12 20.52488 09 37 29.656 +39 23 24.90 535230 G37 C~2VW8 2018 01 09.51968 09 36 06.593 +39 40 17.46 22.5G 535230 F51 C~2rYI 2018 01 20.44778 09 35 07.444 +39 48 43.57 22.4G 535230 F51 C~2rYI 2018 01 20.45166 09 35 07.416 +39 48 43.71 22.2G 535230 F51 C~2rYI 2018 01 20.45894 09 35 07.383 +39 48 44.00 22.2G 535230 F51 C~2rYI 2018 01 20.46291 09 35 07.356 +39 48 44.20 22.3G 535230 F51 C~2rYI 2018 01 20.47020 09 35 07.310 +39 48 44.47 22.1G 535230 F51 C~2rYI 2018 01 20.47406 09 35 07.286 +39 48 44.62 22.3G 535230 F51 C~2rYI 2018 01 20.48140 09 35 07.241 +39 48 45.07 22.1G 535230 F51 C~2rYI 2018 01 20.48527 09 35 07.225 +39 48 45.23 22.2G 535230 F51 C~2rYI 2018 01 23.44907 09 34 49.964 +39 50 53.03 22.4G 535230 F51 C~2rYI 2021 01 08.54675 10 01 49.872 +40 39 07.48 22.2w 535230 F51 C~4YAm 2021 01 08.55786 10 01 49.794 +40 39 08.21 22.2w 535230 F51 C~4YAm 2021 01 08.56896 10 01 49.763 +40 39 08.88 22.3w 535230 F51 C~4YAm 2022 03 02.236400 10 05 26.546 +41 28 59.67 22.0G 535230 G37 C~5V3k 2022 03 02.293280 10 05 26.206 +41 29 00.61 535230 G37 C~5V3k 2022 03 02.346570 10 05 25.857 +41 29 01.89 535230 G37 C~5V3k 2024 05 02.254094 10 18 24.836 +41 48 28.18 22.1w 535230 F52 C~82e4 2024 05 02.266001 10 18 24.815 +41 48 27.71 22.2w 535230 F52 C~82e4 2024 05 02.277892 10 18 24.815 +41 48 27.51 22.3w 535230 F52 C~82e4 2024 05 02.289897 10 18 24.776 +41 48 26.85 22.0w 535230 F52 C~82e4
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 0.10 0.00 0.05
2 0.1830 0.00 0.40 0.00 -0.03
3 0.9609 0.00 0.01 0.00 0.19
4 1.0432 0.00 -0.67 0.00 -0.01
5 1.1198 0.00 -0.04 0.00 0.21
6 1.2560 0.00 -0.06 0.00 -0.30
7 1.2670 0.00 -0.27 0.00 -0.14
8 1.3023 0.00 -0.23 0.00 -0.07
9 1.3023 0.00 0.05 0.00 0.10
10 2.1190 0.00 0.37 0.00 0.77
11 2.1736 0.00 0.18 0.00 -0.81
12 2.2308 0.00 -0.09 0.00 0.20
13 2.2661 0.00 -0.11 0.00 -0.24
14 2.2661 0.00 0.17 0.00 -0.04
15 2.2661 0.00 0.35 0.00 -0.18
16 3.1975 0.00 -0.15 0.00 0.22
17 3.3091 0.00 -0.10 0.00 -0.33
18 4.0000 0.00 -0.44 0.00 0.23
19 4.1285 0.00 -0.19 0.00 0.07
20 4.1285 0.00 0.12 0.00 0.25
21 4.1286 0.00 0.23 0.00 0.03
22 4.1286 0.00 0.21 0.00 -0.12
23 4.1777 0.00 -0.02 0.00 0.01
24 4.1778 0.00 0.18 0.00 0.09
25 4.1778 0.00 0.20 0.00 0.21
26 4.2157 0.00 0.05 0.00 0.27
27 4.2157 0.00 -0.08 0.00 -0.06
28 4.2158 0.00 -0.07 0.00 0.16
29 4.3577 0.00 -0.09 0.00 -0.04
30 4.3577 0.00 0.08 0.00 0.03
31 4.3578 0.00 -0.10 0.00 -0.03
32 4.3578 0.00 0.10 0.00 -0.03
33 4.3632 0.00 -0.00 0.00 -0.01
34 4.3632 0.00 -0.11 0.00 0.05
35 4.3633 0.00 0.10 0.00 -0.04
36 4.4781 0.00 -0.66 0.00 -0.02
37 5.0212 0.00 0.14 0.00 -0.22
38 5.0651 0.00 0.15 0.00 -0.19
39 5.0895 0.00 0.02 0.00 -0.09
40 5.0895 0.00 0.16 0.00 -0.10
41 5.0896 0.00 -0.02 0.00 -0.08
42 5.0896 0.00 0.15 0.00 -0.05
43 5.1414 0.00 0.06 0.00 0.07
44 5.2153 0.00 -0.03 0.00 -0.08
45 5.2586 0.00 -0.03 0.00 -0.17
46 5.2586 0.00 0.06 0.00 -0.34
47 5.2587 0.00 -0.03 0.00 -0.24
48 5.2587 0.00 -0.09 0.00 0.01
49 5.2917 0.00 0.05 0.00 0.13
50 6.0479 0.00 0.11 0.00 -0.07
51 6.1190 0.00 0.02 0.00 0.03
52 6.1190 0.00 0.11 0.00 0.31
53 6.1190 0.00 -0.09 0.00 -0.04
54 6.1191 0.00 -0.08 0.00 0.15
55 6.2308 0.00 -0.04 0.00 0.09
56 7.0280 0.00 0.11 0.00 -0.08
57 7.0280 0.00 -0.05 0.00 -0.06
58 7.0935 0.00 0.11 0.00 0.21
59 7.0935 0.00 0.05 0.00 0.02
60 7.0936 0.00 0.04 0.00 0.02
61 7.0936 0.00 -0.14 0.00 -0.13
62 7.1125 0.00 0.07 0.00 -0.02
63 7.1126 0.00 -0.09 0.00 0.16
64 7.1674 0.00 -0.13 0.00 0.02
65 7.1973 0.00 0.03 0.00 0.06
66 7.1973 0.00 -0.05 0.00 0.02
67 7.1973 0.00 0.10 0.00 -0.01
68 7.1973 0.00 0.04 0.00 0.02
69 7.1974 0.00 -0.01 0.00 -0.03
70 7.1974 0.00 -0.03 0.00 -0.05
71 7.1974 0.00 -0.06 0.00 0.07
72 7.1974 0.00 0.04 0.00 0.06
73 7.2055 0.00 -0.23 0.00 0.07
74 10.1654 0.00 0.02 0.00 -0.06
75 10.1654 0.00 -0.40 0.00 0.08
76 10.1655 0.00 -0.11 0.00 0.17
77 11.3090 0.00 0.08 0.00 0.04
78 11.3091 0.00 0.24 0.00 -0.21
79 11.3093 0.00 -0.07 0.00 -0.02
80 13.4774 0.00 0.05 0.00 0.03
81 13.4774 0.00 -0.02 0.00 -0.07
82 13.4775 0.00 0.23 0.00 0.10
83 13.4775 0.00 -0.10 0.00 -0.19
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.
535230 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 57.053 57.053 57.053 ecceobj 0.324 0.323 0.324 incobj 40.658 40.658 40.658 qmin 37.373 37.374 37.371 qmax 77.364 77.335 77.392 amean 56.933 56.933 56.934 amin 56.360 56.339 56.339 amax 57.686 57.692 57.679 emean 0.323 0.323 0.321 emin 0.312 0.313 0.310 emax 0.342 0.341 0.342 imean 39.079 39.073 39.109 imin 38.681 38.680 38.681 imax 39.359 39.350 39.413 excite_mean 0.708 0.708 0.708 fracstop 1.000 1.000 1.000 cjmean 2.550 2.550 2.550 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 121.4 121.4 122.4 kozaiamp 107.6 107.7 109.9