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: 531682 # Created Thu Apr 25 01:08:36 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 61 observations of 61 # Arc: 7.24y # First observation: 2010/10/09 # Last observation: 2018/01/03 # Chi-squared of fit: 67.24 DOF: 116 RMS: 0.19 # Min/Max residuals: -0.48 0.85 # Exact a, adot, b, bdot, g, gdot: 1.379637E-05 1.904691E-02 -7.335733E-07 -1.793602E-03 2.184785E-02 1.582647E-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 -7.213180 53.306201 0.603005 -0.099434 -0.785512 2455478.935036 # Heliocentric elements and errors Epoch: 2455478.5000 = 2010/10/09 Mean Anomaly: 136.48680 +/- 0.000 Argument of Peri: 88.14411 +/- 0.000 Long of Asc Node: 180.27702 +/- 0.000 Inclination: 8.93647 +/- 0.000 Eccentricity: 0.11183028 +/- 0.0000 Semi-Major Axis: 42.86056616 +/- 0.0000 Time of Perihelion: 2416621.1275 +/- 0.0 Perihelion: 38.06745698 +/- 0.0000 Aphelion: 47.65367534 +/- 0.0000 Period (y) 280.6048 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 28.09386330 +/- 0.0000 Ecliptic Y 36.68435353 +/- 0.0000 Ecliptic Z -5.74711823 +/- 0.0000 Ecliptic XDOT -0.00181304 +/- 0.0000 Ecliptic YDOT 0.00156774 +/- 0.0000 Ecliptic ZDOT -0.00024790 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 46.56213160 +/- 0.0000 Geocenter to KBO 45.77107011 +/- 0.0000 # Hcoef: 5.98
The following table shows the complete astrometric record for 531682. 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 (531682) followed by the observatory code and reference code for the source of the astrometry.
2010 10 09.43427 03 31 01.814 +11 36 31.84 21.9G 531682 F51 C~2rXv 2010 10 09.45032 03 31 01.763 +11 36 31.56 22.0G 531682 F51 C~2rXv 2010 10 09.46646 03 31 01.716 +11 36 31.33 22.9G 531682 F51 C~2rXv 2012 10 21.54726 03 39 08.665 +11 51 55.90 22.6w 531682 F51 C~1w3s 2012 10 21.56332 03 39 08.592 +11 51 55.24 22.5w 531682 F51 C~1w3s 2012 10 21.57933 03 39 08.514 +11 51 54.86 22.6w 531682 F51 C~1w3s 2012 12 10.27514 03 35 35.188 +11 38 24.63 22.2w 531682 F51 C~1w3s 2012 12 10.29059 03 35 35.104 +11 38 24.57 22.4w 531682 F51 C~1w3s 2012 12 10.31620 03 35 35.017 +11 38 24.03 22.4w 531682 F51 C~1w3s 2012 12 10.31620 03 35 35.017 +11 38 24.04 22.4w 531682 F51 C~3i3Z 2013 03 05.24285 03 33 50.365 +11 42 51.82 22.5w 531682 F51 C~1w3s 2013 03 05.25076 03 33 50.397 +11 42 52.13 22.8G 531682 F51 C~2rXv 2013 11 09.51066 03 42 16.923 +11 55 32.42 22.7w 531682 F51 C~1w3s 2013 11 09.52573 03 42 16.868 +11 55 32.07 22.8w 531682 F51 C~1w3s 2013 11 09.52639 03 42 16.846 +11 55 32.16 22.2w 531682 F51 C~1w3s 2013 11 09.54084 03 42 16.781 +11 55 32.08 22.5w 531682 F51 C~1w3s 2013 11 09.54150 03 42 16.771 +11 55 32.20 22.4w 531682 F51 C~1w3s 2013 11 09.55599 03 42 16.719 +11 55 31.74 22.4w 531682 F51 C~1w3s 2013 11 09.55665 03 42 16.718 +11 55 31.52 22.4w 531682 F51 C~1w3s 2013 11 26.32178 03 41 02.017 +11 51 00.01 22.6w 531682 F51 C~1w3s 2013 11 26.35235 03 41 01.892 +11 50 59.62 22.5w 531682 F51 C~1w3s 2013 11 26.36773 03 41 01.839 +11 50 59.32 22.6w 531682 F51 C~1w3s 2013 11 26.36773 03 41 01.838 +11 50 59.32 22.6w 531682 F51 C~3i3Z 2014 07 31.61079 03 49 08.489 +12 27 11.58 23.3G 531682 F51 C~2rXv 2014 10 25.56086 03 47 45.896 +12 09 08.66 22.3G 531682 F51 C~2rXv 2014 12 12.44510 03 44 18.972 +11 56 50.46 21.5G 531682 F51 C~2rXv 2015 01 15.36535 03 42 29.156 +11 53 59.33 22.9G 531682 F51 C~2rXv 2015 07 26.60073 03 53 11.893 +12 35 39.88 23.0G 531682 F51 C~2rXv 2015 10 10.57908 03 53 03.478 +12 22 21.03 22.8G 531682 F51 C~2rXv 2015 11 07.39614 03 51 18.662 +12 14 08.24 22.7G 531682 F51 C~2rXv 2015 11 08.37948 03 51 14.465 +12 13 51.34 22.7G 531682 F51 C~2rXv 2015 11 18.37933 03 50 30.200 +12 11 07.40 21.9G 531682 F51 C~2rXv 2015 12 02.31311 03 49 27.923 +12 07 46.07 23.1G 531682 F51 C~2rXv 2015 12 02.32578 03 49 27.851 +12 07 46.09 22.5G 531682 F51 C~2rXv 2015 12 02.33851 03 49 27.800 +12 07 45.67 22.8G 531682 F51 C~2rXv 2015 12 02.35133 03 49 27.744 +12 07 45.66 22.1G 531682 F51 C~2rXv 2015 12 03.31539 03 49 23.511 +12 07 33.17 22.9G 531682 F51 C~2rXv 2016 01 03.31632 03 47 23.998 +12 03 13.07 23.0G 531682 F51 C~2rXv 2016 01 03.33051 03 47 23.983 +12 03 13.25 22.5G 531682 F51 C~2rXv 2016 01 03.34434 03 47 23.878 +12 03 12.81 22.3G 531682 F51 C~2rXv 2016 01 03.35830 03 47 23.871 +12 03 13.09 22.6G 531682 F51 C~2rXv 2016 01 13.34620 03 46 56.470 +12 02 55.01 22.7G 531682 F51 C~2rXv 2016 01 13.36906 03 46 56.432 +12 02 54.89 22.9G 531682 F51 C~2rXv 2016 01 31.26219 03 46 26.430 +12 03 49.10 22.4G 531682 F51 C~2rXv 2016 01 31.27490 03 46 26.405 +12 03 49.04 22.8G 531682 F51 C~2rXv 2016 01 31.28772 03 46 26.397 +12 03 49.08 22.8G 531682 F51 C~2rXv 2016 01 31.30060 03 46 26.372 +12 03 49.12 22.5G 531682 F51 C~2rXv 2016 10 12.57998 03 57 17.979 +12 29 51.96 23.0G 531682 F51 C~2rXv 2016 10 28.59897 03 56 20.252 +12 25 11.22 22.4G 531682 F51 C~2rXv 2017 08 05.60234 04 02 13.265 +12 51 10.64 22.8G 531682 F51 C~2rXv 2017 09 22.54337 04 02 29.419 +12 43 20.58 23.0G 531682 F51 C~2rXv 2017 09 24.55710 04 02 25.903 +12 42 50.35 22.6G 531682 F51 C~2rXv 2017 11 18.37011 03 59 15.918 +12 27 43.71 22.1G 531682 F51 C~2rXv 2017 12 08.49272 03 57 46.136 +12 23 19.10 23.1G 531682 F51 C~2rXv 2017 12 20.30226 03 56 57.130 +12 21 29.07 22.4R 531682 G37 C~2Uwm 2017 12 20.41668 03 56 56.673 +12 21 28.44 531682 G37 C~2Uwm 2017 12 24.26139 03 56 41.939 +12 21 01.27 23.5G 531682 F51 C~2rXv 2017 12 24.27419 03 56 41.866 +12 21 01.07 22.8G 531682 F51 C~2rXv 2017 12 24.28694 03 56 41.844 +12 21 00.87 22.9G 531682 F51 C~2rXv 2017 12 24.29971 03 56 41.777 +12 21 00.85 22.3G 531682 F51 C~2rXv 2018 01 03.34361 03 56 06.867 +12 20 11.90 23.5G 531682 F51 C~2rXv
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 0.03 0.00 -0.11
2 0.0000 0.00 0.07 0.00 -0.09
3 0.0001 0.00 0.18 0.00 -0.01
4 2.0345 0.00 -0.10 0.00 0.24
5 2.0346 0.00 -0.25 0.00 -0.12
6 2.0346 0.00 -0.48 0.00 -0.19
7 2.1707 0.00 -0.00 0.00 -0.09
8 2.1707 0.00 -0.30 0.00 0.02
9 2.1708 0.00 -0.01 0.00 -0.23
10 2.1708 0.00 -0.01 0.00 -0.24
11 2.4033 0.00 0.24 0.00 -0.15
12 2.4033 0.00 0.46 0.00 0.03
13 3.0858 0.00 0.05 0.00 0.01
14 3.0858 0.00 0.23 0.00 -0.07
15 3.0858 0.00 -0.06 0.00 0.03
16 3.0858 0.00 -0.06 0.00 0.20
17 3.0859 0.00 -0.17 0.00 0.34
18 3.0859 0.00 0.02 0.00 0.13
19 3.0859 0.00 0.05 0.00 -0.08
20 3.1318 0.00 -0.39 0.00 0.16
21 3.1319 0.00 -0.20 0.00 0.21
22 3.1319 0.00 0.03 0.00 0.14
23 3.1319 0.00 0.05 0.00 0.14
24 3.8088 0.00 0.03 0.00 0.38
25 4.0442 0.00 -0.01 0.00 0.34
26 4.1753 0.00 -0.09 0.00 0.00
27 4.2681 0.00 -0.08 0.00 0.05
28 4.7944 0.00 0.13 0.00 -0.17
29 5.0024 0.00 -0.09 0.00 -0.12
30 5.0786 0.00 0.12 0.00 -0.26
31 5.0813 0.00 0.85 0.00 -0.34
32 5.1087 0.00 -0.18 0.00 0.17
33 5.1468 0.00 0.12 0.00 -0.04
34 5.1469 0.00 -0.11 0.00 0.14
35 5.1469 0.00 -0.02 0.00 -0.12
36 5.1469 0.00 0.00 0.00 0.04
37 5.1496 0.00 0.13 0.00 -0.06
38 5.2344 0.00 0.09 0.00 -0.13
39 5.2345 0.00 0.54 0.00 0.10
40 5.2345 0.00 -0.38 0.00 -0.29
41 5.2346 0.00 0.18 0.00 0.04
42 5.2619 0.00 -0.10 0.00 -0.01
43 5.2620 0.00 0.17 0.00 -0.12
44 5.3110 0.00 0.08 0.00 0.17
45 5.3110 0.00 -0.10 0.00 0.03
46 5.3110 0.00 -0.03 0.00 -0.00
47 5.3111 0.00 -0.21 0.00 -0.04
48 6.0100 0.00 0.21 0.00 0.06
49 6.0538 0.00 -0.22 0.00 -0.11
50 6.8232 0.00 0.01 0.00 0.03
51 6.9544 0.00 0.09 0.00 -0.03
52 6.9600 0.00 -0.05 0.00 0.08
53 7.1100 0.00 -0.07 0.00 0.06
54 7.1651 0.00 0.07 0.00 0.02
55 7.1974 0.00 -0.03 0.00 0.04
56 7.1978 0.00 -0.07 0.00 0.30
57 7.2083 0.00 0.07 0.00 0.10
58 7.2083 0.00 -0.29 0.00 -0.02
59 7.2084 0.00 0.11 0.00 -0.14
60 7.2084 0.00 -0.16 0.00 -0.08
61 7.2359 0.00 -0.00 0.00 -0.27
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.
531682 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.028 43.028 43.028 ecceobj 0.109 0.109 0.109 incobj 8.928 8.928 8.928 qmin 37.428 37.428 37.427 qmax 48.370 48.362 48.374 amean 42.733 42.733 42.733 amin 42.386 42.379 42.381 amax 43.113 43.114 43.113 emean 0.103 0.103 0.103 emin 0.084 0.084 0.084 emax 0.122 0.122 0.122 imean 9.646 9.646 9.646 imin 8.561 8.561 8.561 imax 10.583 10.585 10.580 excite_mean 0.197 0.197 0.197 fracstop 1.000 1.000 1.000 cjmean 3.040 3.040 3.040 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 181.7 181.7 181.7 kozaiamp 180.0 180.0 180.0