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: 535466 # Created Sun Nov 24 02:07:27 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 96 observations of 96 # Arc: 9.99y # First observation: 2011/02/14 # Last observation: 2021/02/08 # Chi-squared of fit: 108.41 DOF: 186 RMS: 0.19 # Min/Max residuals: -0.50 1.09 # Exact a, adot, b, bdot, g, gdot: 2.059862E-05 3.670842E-02 1.598890E-06 2.121385E-03 3.069478E-02 1.931165E-04 # 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 17.105815 144.486285 -0.014257 0.291501 -0.947214 2455606.911716 # Heliocentric elements and errors Epoch: 2455606.5000 = 2011/02/14 Mean Anomaly: 1.31424 +/- 0.000 Argument of Peri: 77.03684 +/- 0.000 Long of Asc Node: 65.86446 +/- 0.000 Inclination: 16.92232 +/- 0.000 Eccentricity: 0.21554984 +/- 0.0000 Semi-Major Axis: 42.73043529 +/- 0.0000 Time of Perihelion: 2455234.0421 +/- 0.0 Perihelion: 33.51989680 +/- 0.0000 Aphelion: 51.94097378 +/- 0.0000 Period (y) 279.3278 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -26.15653438 +/- 0.0000 Ecliptic Y 18.65089253 +/- 0.0000 Ecliptic Z 9.58268923 +/- 0.0000 Ecliptic XDOT -0.00187130 +/- 0.0000 Ecliptic YDOT -0.00268186 +/- 0.0000 Ecliptic ZDOT 0.00018593 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 33.52383854 +/- 0.0000 Geocenter to KBO 32.57886508 +/- 0.0000 # Hcoef: 6.84
The following table shows the complete astrometric record for 535466. 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 (535466) followed by the observatory code and reference code for the source of the astrometry.
2011 02 14.41095 10 12 56.377 +29 23 14.58 22.0G 535466 F51 C~2rYI 2011 02 21.29317 10 12 12.607 +29 26 57.02 20.8G 535466 F51 C~2rYI 2011 02 21.30496 10 12 12.552 +29 26 57.46 22.1G 535466 F51 C~2rYI 2011 02 21.31836 10 12 12.468 +29 26 57.60 20.8G 535466 F51 C~2rYI 2011 02 21.33093 10 12 12.393 +29 26 57.99 21.4G 535466 F51 C~2rYI 2012 01 15.61695 10 24 48.766 +28 21 13.14 22.3G 535466 F51 C~2rYI 2012 02 01.59859 10 23 21.060 +28 33 29.72 23.0G 535466 F51 C~2rYI 2012 02 04.57274 10 23 03.725 +28 35 31.76 21.4G 535466 F51 C~2rYI 2012 02 04.58523 10 23 03.641 +28 35 31.78 21.1G 535466 F51 C~2rYI 2013 02 13.36809 10 31 04.481 +27 58 06.95 21.9w 535466 F51 C~1vY1 2013 02 13.38190 10 31 04.407 +27 58 07.73 22.2w 535466 F51 C~1vY1 2013 02 13.39571 10 31 04.313 +27 58 08.17 22.0w 535466 F51 C~1vY1 2013 02 13.40966 10 31 04.227 +27 58 08.62 22.3w 535466 F51 C~1vY1 2013 03 01.50009 10 29 24.215 +28 07 00.24 22.5G 535466 F51 C~2rYI 2014 01 26.62697 10 41 35.328 +26 59 53.59 22.5G 535466 F51 C~2rYI 2014 01 26.63993 10 41 35.266 +26 59 54.34 21.9G 535466 F51 C~2rYI 2014 02 10.54927 10 40 13.780 +27 10 28.50 21.8i 535466 F51 C~1vY1 2014 02 10.56156 10 40 13.693 +27 10 29.04 21.5i 535466 F51 C~1vY1 2014 02 10.57358 10 40 13.624 +27 10 29.34 21.5i 535466 F51 C~1vY1 2014 02 10.58542 10 40 13.561 +27 10 30.04 21.6i 535466 F51 C~1vY1 2014 12 27.47109 10 51 56.094 +25 50 02.66 22.3G 535466 F51 C~2rYI 2015 01 15.60814 10 51 03.645 +26 03 40.45 21.2i 535466 F51 C~1vY1 2015 01 15.62047 10 51 03.598 +26 03 41.10 21.6i 535466 F51 C~1vY1 2015 01 15.63282 10 51 03.548 +26 03 41.58 21.6i 535466 F51 C~1vY1 2015 01 27.56751 10 50 12.006 +26 12 37.61 21.8w 535466 F51 C~1vY1 2015 01 27.57850 10 50 11.945 +26 12 38.10 22.2w 535466 F51 C~1vY1 2015 01 27.58950 10 50 11.899 +26 12 38.79 22.1w 535466 F51 C~1vY1 2015 01 27.60053 10 50 11.837 +26 12 39.15 22.1w 535466 F51 C~1vY1 2015 04 20.33532 10 42 46.641 +26 44 34.03 22.5w 535466 F51 C~1vY1 2015 04 20.34814 10 42 46.601 +26 44 33.94 22.4w 535466 F51 C~1vY1 2015 04 20.36105 10 42 46.569 +26 44 34.03 22.5w 535466 F51 C~1vY1 2015 04 20.37405 10 42 46.522 +26 44 33.77 22.2w 535466 F51 C~1vY1 2015 04 21.38443 10 42 43.172 +26 44 23.68 23.1G 535466 F51 C~2rYI 2015 04 24.37607 10 42 33.897 +26 43 50.20 22.1G 535466 F51 C~2rYI 2016 01 03.54554 11 00 07.849 +25 05 18.53 22.2G 535466 F51 C~2rYI 2016 01 14.46542 10 59 37.361 +25 13 08.05 22.2G 535466 F51 C~2rYI 2016 01 14.47857 10 59 37.322 +25 13 08.61 22.2G 535466 F51 C~2rYI 2016 01 14.49169 10 59 37.253 +25 13 09.37 21.7G 535466 F51 C~2rYI 2016 01 14.50483 10 59 37.221 +25 13 09.76 22.3G 535466 F51 C~2rYI 2016 01 21.46756 10 59 11.265 +25 18 21.16 22.4G 535466 F51 C~2rYI 2016 01 30.47247 10 58 31.215 +25 25 05.30 21.0G 535466 F51 C~2rYI 2016 01 31.46888 10 58 26.391 +25 25 49.73 21.7G 535466 F51 C~2rYI 2016 01 31.48116 10 58 26.321 +25 25 50.35 21.0G 535466 F51 C~2rYI 2016 01 31.49381 10 58 26.259 +25 25 50.90 21.6G 535466 F51 C~2rYI 2016 01 31.50661 10 58 26.191 +25 25 51.46 22.1G 535466 F51 C~2rYI 2016 01 31.57629 10 58 25.838 +25 25 54.43 21.7G 535466 F51 C~2rYJ 2016 01 31.58918 10 58 25.798 +25 25 54.84 22.0G 535466 F51 C~2rYJ 2016 01 31.60207 10 58 25.709 +25 25 56.02 21.4G 535466 F51 C~2rYJ 2016 01 31.61456 10 58 25.652 +25 25 56.03 20.8G 535466 F51 C~2rYJ 2016 02 05.39486 10 58 01.459 +25 29 26.93 22.2G 535466 F51 C~2rYJ 2016 02 05.40786 10 58 01.389 +25 29 27.44 22.3G 535466 F51 C~2rYJ 2016 02 05.42087 10 58 01.322 +25 29 28.07 22.3G 535466 F51 C~2rYJ 2016 02 05.43391 10 58 01.236 +25 29 28.70 21.9G 535466 F51 C~2rYJ 2016 02 10.38714 10 57 34.600 +25 33 01.54 22.1G 535466 F51 C~2rYJ 2016 02 10.39815 10 57 34.552 +25 33 01.70 22.1G 535466 F51 C~2rYJ 2016 02 10.40913 10 57 34.490 +25 33 02.25 22.2G 535466 F51 C~2rYJ 2016 02 10.42014 10 57 34.431 +25 33 02.74 22.2G 535466 F51 C~2rYJ 2016 02 11.53843 10 57 28.212 +25 33 49.75 21.9G 535466 F51 C~2rYJ 2016 02 11.55111 10 57 28.131 +25 33 50.34 21.8G 535466 F51 C~2rYJ 2016 02 11.56376 10 57 28.065 +25 33 50.86 22.1G 535466 F51 C~2rYJ 2016 02 26.58611 10 56 00.176 +25 43 33.04 21.6G 535466 F51 C~2rYJ 2016 04 29.36551 10 50 49.531 +25 55 16.76 22.3G 535466 F51 C~2rYJ 2016 04 29.37793 10 50 49.507 +25 55 16.47 21.8G 535466 F51 C~2rYJ 2016 04 29.39035 10 50 49.463 +25 55 16.43 22.1G 535466 F51 C~2rYJ 2016 05 03.31019 10 50 40.324 +25 54 09.08 22.2G 535466 F51 C~2rYJ 2016 05 28.27963 10 50 23.347 +25 42 17.92 22.2G 535466 F51 C~2rYJ 2016 05 28.29124 10 50 23.354 +25 42 17.49 22.4G 535466 F51 C~2rYJ 2016 05 28.30293 10 50 23.369 +25 42 17.09 22.2G 535466 F51 C~2rYJ 2016 05 28.31458 10 50 23.371 +25 42 16.71 21.9G 535466 F51 C~2rYJ 2017 01 31.46880 11 06 46.639 +24 35 18.35 22.0G 535466 F51 C~2rYJ 2017 01 31.47997 11 06 46.615 +24 35 18.70 21.9G 535466 F51 C~2rYJ 2017 01 31.49123 11 06 46.548 +24 35 19.42 21.5G 535466 F51 C~2rYJ 2017 01 31.50242 11 06 46.472 +24 35 20.08 21.6G 535466 F51 C~2rYJ 2017 03 15.46110 11 02 42.274 +25 01 53.05 22.1G 535466 F51 C~2rYJ 2017 03 21.28739 11 02 08.386 +25 04 05.46 22.3G 535466 F51 C~2rYJ 2017 03 21.30015 11 02 08.317 +25 04 05.64 22.4G 535466 F51 C~2rYJ 2017 03 21.31292 11 02 08.247 +25 04 05.86 22.0G 535466 F51 C~2rYJ 2017 03 21.32561 11 02 08.172 +25 04 06.14 22.0G 535466 F51 C~2rYJ 2017 12 31.54448 11 16 36.759 +23 20 27.60 22.3G 535466 F51 C~2rYJ 2017 12 31.55719 11 16 36.729 +23 20 28.11 22.1G 535466 F51 C~2rYJ 2017 12 31.56992 11 16 36.705 +23 20 28.65 22.9G 535466 F51 C~2rYJ 2017 12 31.58260 11 16 36.699 +23 20 28.98 22.5G 535466 F51 C~2rYJ 2018 01 14.48847 11 16 06.713 +23 30 00.50 22.1G 535466 F51 C~2rYJ 2018 01 14.50206 11 16 06.694 +23 30 01.22 22.2G 535466 F51 C~2rYJ 2018 01 14.51558 11 16 06.631 +23 30 01.85 22.2G 535466 F51 C~2rYJ 2018 01 14.52907 11 16 06.600 +23 30 02.30 22.0G 535466 F51 C~2rYJ 2018 02 10.42105 11 14 14.297 +23 49 55.57 22.0G 535466 F51 C~2rYJ 2018 02 10.43384 11 14 14.227 +23 49 56.10 21.9G 535466 F51 C~2rYJ 2018 02 10.44666 11 14 14.163 +23 49 56.40 22.1G 535466 F51 C~2rYJ 2018 03 10.34193 11 11 34.045 +24 07 29.84 22.1G 535466 F51 C~2rYJ 2018 03 10.35373 11 11 33.983 +24 07 30.03 22.3G 535466 F51 C~2rYJ 2018 03 10.36553 11 11 33.909 +24 07 30.39 22.5G 535466 F51 C~2rYJ 2018 03 10.37737 11 11 33.852 +24 07 30.97 22.2G 535466 F51 C~2rYJ 2021 02 08.44957 11 38 18.701 +21 03 44.39 21.7w 535466 F51 C~4fMK 2021 02 08.46309 11 38 18.626 +21 03 44.89 21.9w 535466 F51 C~4fMK 2021 02 08.49028 11 38 18.527 +21 03 45.82 21.9w 535466 F51 C~4fMK
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 -0.42 0.00 0.03
2 0.0188 0.00 -0.50 0.00 0.01
3 0.0189 0.00 -0.18 0.00 0.09
4 0.0189 0.00 -0.15 0.00 -0.18
5 0.0189 0.00 -0.05 0.00 -0.18
6 0.9177 0.00 -0.30 0.00 0.10
7 0.9642 0.00 1.09 0.00 -0.21
8 0.9724 0.00 0.27 0.00 0.07
9 0.9724 0.00 0.13 0.00 -0.41
10 1.9985 0.00 -0.08 0.00 -0.12
11 1.9986 0.00 0.10 0.00 0.13
12 1.9986 0.00 -0.03 0.00 0.05
13 1.9986 0.00 -0.02 0.00 -0.03
14 2.0427 0.00 0.12 0.00 -0.30
15 2.9493 0.00 0.08 0.00 -0.08
16 2.9493 0.00 0.14 0.00 0.10
17 2.9901 0.00 0.21 0.00 -0.01
18 2.9901 0.00 0.01 0.00 0.04
19 2.9902 0.00 0.05 0.00 -0.13
20 2.9902 0.00 0.16 0.00 0.10
21 3.8660 0.00 -0.50 0.00 0.06
22 3.9184 0.00 -0.17 0.00 -0.05
23 3.9184 0.00 -0.16 0.00 0.06
24 3.9185 0.00 -0.19 0.00 -0.01
25 3.9511 0.00 0.27 0.00 0.19
26 3.9512 0.00 0.17 0.00 0.19
27 3.9512 0.00 0.30 0.00 0.39
28 3.9512 0.00 0.18 0.00 0.26
29 4.1778 0.00 -0.20 0.00 0.12
30 4.1778 0.00 -0.13 0.00 0.14
31 4.1778 0.00 0.06 0.00 0.35
32 4.1779 0.00 0.03 0.00 0.22
33 4.1806 0.00 -0.08 0.00 -0.26
34 4.1888 0.00 -0.10 0.00 -0.09
35 4.8847 0.00 0.44 0.00 0.40
36 4.9146 0.00 -0.09 0.00 -0.05
37 4.9146 0.00 0.01 0.00 -0.08
38 4.9147 0.00 -0.34 0.00 0.10
39 4.9147 0.00 -0.13 0.00 -0.10
40 4.9338 0.00 -0.13 0.00 0.12
41 4.9584 0.00 -0.04 0.00 -0.11
42 4.9611 0.00 0.10 0.00 -0.07
43 4.9612 0.00 -0.03 0.00 -0.00
44 4.9612 0.00 -0.01 0.00 -0.02
45 4.9612 0.00 -0.07 0.00 -0.03
46 4.9614 0.00 -0.13 0.00 -0.15
47 4.9615 0.00 0.24 0.00 -0.31
48 4.9615 0.00 -0.13 0.00 0.30
49 4.9615 0.00 -0.04 0.00 -0.25
50 4.9746 0.00 0.05 0.00 0.02
51 4.9747 0.00 0.04 0.00 -0.04
52 4.9747 0.00 0.07 0.00 0.02
53 4.9747 0.00 -0.18 0.00 0.07
54 4.9883 0.00 -0.18 0.00 0.18
55 4.9883 0.00 0.02 0.00 -0.13
56 4.9884 0.00 0.02 0.00 -0.05
57 4.9884 0.00 0.06 0.00 -0.03
58 4.9915 0.00 0.03 0.00 -0.05
59 4.9915 0.00 -0.11 0.00 0.01
60 4.9915 0.00 -0.02 0.00 0.01
61 5.0326 0.00 0.69 0.00 0.51
62 5.2045 0.00 -0.06 0.00 -0.03
63 5.2046 0.00 0.07 0.00 -0.12
64 5.2046 0.00 -0.09 0.00 0.04
65 5.2153 0.00 0.47 0.00 0.03
66 5.2837 0.00 -0.07 0.00 -0.02
67 5.2837 0.00 -0.09 0.00 -0.02
68 5.2838 0.00 0.01 0.00 0.02
69 5.2838 0.00 -0.08 0.00 0.08
70 5.9632 0.00 -0.20 0.00 -0.13
71 5.9632 0.00 0.25 0.00 -0.28
72 5.9633 0.00 0.07 0.00 -0.06
73 5.9633 0.00 -0.25 0.00 0.10
74 6.0809 0.00 -0.14 0.00 -0.03
75 6.0969 0.00 -0.11 0.00 0.08
76 6.0969 0.00 -0.03 0.00 -0.01
77 6.0969 0.00 0.03 0.00 -0.06
78 6.0970 0.00 0.02 0.00 -0.04
79 6.8778 0.00 0.05 0.00 -0.01
80 6.8779 0.00 -0.12 0.00 0.01
81 6.8779 0.00 -0.20 0.00 0.06
82 6.8780 0.00 -0.01 0.00 -0.10
83 6.9160 0.00 -0.17 0.00 -0.04
84 6.9161 0.00 0.17 0.00 0.08
85 6.9161 0.00 -0.16 0.00 0.12
86 6.9161 0.00 -0.01 0.00 -0.01
87 6.9898 0.00 0.00 0.00 0.16
88 6.9898 0.00 -0.03 0.00 0.13
89 6.9898 0.00 0.03 0.00 -0.13
90 7.0662 0.00 -0.22 0.00 0.02
91 7.0662 0.00 -0.08 0.00 -0.15
92 7.0663 0.00 -0.11 0.00 -0.15
93 7.0663 0.00 0.11 0.00 0.07
94 9.9850 0.00 0.04 0.00 0.03
95 9.9851 0.00 -0.14 0.00 -0.07
96 9.9852 0.00 0.28 0.00 -0.35
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.
535466 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 42.902 42.902 42.902 ecceobj 0.218 0.218 0.218 incobj 16.904 16.904 16.904 qmin 30.769 32.797 32.955 qmax 59.945 53.265 53.434 amean 42.826 42.774 42.871 amin 41.639 42.223 42.361 amax 45.945 43.395 43.425 emean 0.226 0.206 0.204 emin 0.184 0.180 0.176 emax 0.305 0.232 0.232 imean 15.191 15.424 15.662 imin 11.565 14.253 14.225 imax 17.125 16.965 16.983 excite_mean 0.347 0.337 0.338 fracstop 1.000 1.000 1.000 cjmean 2.944 2.953 2.953 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 181.1 182.7 178.1 kozaiamp 180.0 179.9 179.9