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: 13SE101 # Created Tue Apr 1 01:09:41 2025 # Orbit generated from Bernstein formalism # Fitting 37 observations of 38 # Arc: 4.07y # First observation: 2013/08/05 # Last observation: 2017/08/30 Preliminary a, adot, b, bdot, g, gdot: -0.000200 0.025365 -0.000000 -0.000182 0.024702 0.000000 # Chi-squared of fit: 10.40 DOF: 68 RMS: 0.09 # Min/Max residuals: -0.22 0.20 # Exact a, adot, b, bdot, g, gdot: 1.624071E-05 2.517569E-02 3.268364E-07 -1.809388E-04 2.474609E-02 -9.227471E-05 # Covariance matrix: 1.2145E-13 -5.0678E-14 1.4484E-16 1.0179E-16 6.7603E-14 -2.1172E-13 -5.0678E-14 2.5226E-13 9.2158E-16 -1.9349E-15 1.0049E-13 2.4211E-12 1.4484E-16 9.2158E-16 6.2295E-14 -2.3275E-14 7.6897E-16 1.0117E-14 1.0179E-16 -1.9349E-15 -2.3275E-14 2.3615E-14 -1.0359E-15 -2.0670E-14 6.7603E-14 1.0049E-13 7.6897E-16 -1.0359E-15 1.5770E-13 1.1759E-12 -2.1172E-13 2.4211E-12 1.0117E-14 -2.0670E-14 1.1759E-12 2.5745E-11 # lat0 lon0 xBary yBary zBary JD0 -0.813467 11.869917 0.869889 -0.007426 -0.525431 2456510.058828 # Heliocentric elements and errors Epoch: 2456510.5000 = 2013/08/06 Mean Anomaly: 341.48935 +/- 0.128 Argument of Peri: 263.62067 +/- 0.153 Long of Asc Node: 128.70805 +/- 0.020 Inclination: 0.90960 +/- 0.000 Eccentricity: 0.07874062 +/- 0.0001 Semi-Major Axis: 44.21586144 +/- 0.0028 Time of Perihelion: 2462032.3513 +/- 38.2 Perihelion: 40.73427724 +/- 0.0042 Aphelion: 47.69744563 +/- 0.0045 Period (y) 294.0190 +/- 0.03 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 40.23532216 +/- 0.0006 Ecliptic Y 7.57114663 +/- 0.0001 Ecliptic Z -0.57366349 +/- 0.0000 Ecliptic XDOT -0.00058942 +/- 0.0000 Ecliptic YDOT 0.00272281 +/- 0.0000 Ecliptic ZDOT -0.00001973 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 40.94548205 +/- 0.0006 Geocenter to KBO 40.41043020 +/- 0.0006 # Hcoef: 7.71
The following table shows the complete astrometric record for 13SE101. 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 (13SE101) followed by the observatory code and reference code for the source of the astrometry.
2013 08 05.55805 00 44 56.027 +03 56 39.14 23.4r 13SE101 568 C~2NKO 2013 08 08.48371 00 44 50.145 +03 55 58.43 23.6r 13SE101 568 C~2NKO 2013 08 08.52252 00 44 50.068 +03 55 57.82 23.7r 13SE101 568 C~2NKO 2013 08 31.56880 00 43 42.545 +03 48 25.47 23.8r 13SE101 568 C~2NKO 2013 09 01.45434 00 43 39.326 +03 48 04.03 23.6r 13SE101 568 C~2NKO 2013 09 01.49328 00 43 39.179 +03 48 03.06 23.8r 13SE101 568 C~2NKO 2013 09 01.50224 00 43 39.152 +03 48 03.00 23.9r 13SE101 568 C~2NKO 2013 09 05.43382 00 43 24.261 +03 46 25.22 23.6r 13SE101 568 C~2NKO 2013 09 05.47268 00 43 24.112 +03 46 24.11 23.7r 13SE101 568 C~2NKO 2013 09 29.36482 00 41 41.596 +03 35 20.85 23.9r 13SE101 568 C~2NKO 2013 09 29.40366 00 41 41.408 +03 35 19.71 23.7r 13SE101 568 C~2NKO 2013 09 29.50581 00 41 40.968 +03 35 16.89 23.9r 13SE101 568 C~2NKO 2013 09 29.51034 00 41 40.910 +03 35 16.37 24.0r 13SE101 568 C~2NKO 2013 10 05.36346 00 41 14.199 +03 32 25.60 23.3r 13SE101 568 C~2NKO 2013 10 06.37195 00 41 09.588 +03 31 56.19 23.6r 13SE101 568 C~2NKO 2013 10 06.43634 00 41 09.279 +03 31 54.16 23.3r 13SE101 568 C~2NKO 2013 10 07.35873 00 41 05.080 +03 31 27.50 23.9r 13SE101 568 C~2NKO 2013 10 09.49639 00 40 55.296 +03 30 25.45 23.3r 13SE101 568 C~2NKO 2013 11 27.29631 00 37 55.394 +03 11 45.56 23.9r 13SE101 568 C~2NKO 2013 11 27.34255 00 37 55.273 +03 11 45.14 24.2r 13SE101 568 C~2NKO 2013 12 05.24487 00 37 40.154 +03 10 16.93 24.3r 13SE101 568 C~2NKO 2014 06 25.60449 00 50 17.592 +04 30 49.44 23.8r 13SE101 568 C~2NKO 2014 06 26.60333 00 50 19.325 +04 30 58.97 24.1r 13SE101 568 C~2NKO 2014 07 23.57931 00 50 33.053 +04 31 47.51 23.6r 13SE101 568 C~2NKO 2014 07 27.55990 00 50 29.691 +04 31 21.08 24.3r 13SE101 568 C~2NKO 2014 08 24.50155 00 49 30.224 +04 24 32.50 24.2r 13SE101 568 C~2NKO 2014 08 28.47368 00 49 17.265 +04 23 06.95 23.9r 13SE101 568 C~2NKO 2014 10 23.30719 00 45 18.619 +03 57 39.28 24.5r 13SE101 568 C~2NKO 2014 10 27.27389 00 45 01.701 +03 55 53.66 23.8r 13SE101 568 C~2NKO 2014 11 24.28665 00 43 23.770 +03 45 52.32 23.8r 13SE101 568 C~2NKO 2014 11 25.31299 00 43 21.112 +03 45 36.64 23.7r 13SE101 568 C~2NKO 2014 12 17.35510 00 42 45.333 +03 42 13.97 23.8r 13SE101 568 C~2NKO 2015 01 17.25897 00 43 09.773 +03 45 27.44 24.4r 13SE101 568 C~2NKO 2017 07 17.61600 01 06 33.026 +06 09 47.86 13SE101 568 C~2NKO 2017 07 23.61854 01 06 32.724 +06 09 37.27 13SE101 568 C~2NKO 2017 08 25.50837 01 05 37.011 +06 03 12.27 23.6w 13SE101 568 C~2NKO 2017 08 30.45058 01 05 21.590 +06 01 32.31 23.4w 13SE101 568 C~2NKO 2017 08 30.49734 01 05 21.432 +06 01 31.16 23.6w 13SE101 568 C~2NKO
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 -0.09
2 0.0080 -96.93 -0.04 -3.14 0.11
3 0.0081 -98.23 0.06 -3.25 0.02
4 0.0712 -1205.18 -0.22 -25.22 0.15
5 0.0736 -1257.91 -0.04 -26.14 -0.03
6 0.0737 -1260.32 -0.05 -26.17 -0.05
7 0.0738 -1260.71 0.10 -26.07 0.05
8 0.0845 -1504.09 0.00 -29.03 -0.01
9 0.0846 -1506.57 0.03 -29.18 -0.15
10 0.1501 -3178.53 0.10 -39.93 0.04
11 0.1502 -3181.57 -0.02 -39.88 0.08
12 0.1504 -3188.74 ( 0.51) -39.90 ( 0.03)
13 0.1505 -3189.74 -0.15 -40.04 -0.11
14 0.1665 -3624.68 0.13 -40.81 -0.01
15 0.1692 -3699.74 0.15 -40.87 -0.02
16 0.1694 -3704.80 -0.04 -40.93 -0.11
17 0.1719 -3773.10 0.16 -40.87 0.02
18 0.1778 -3932.24 -0.20 -40.67 0.16
19 0.3114 -6851.60 0.03 -16.18 -0.14
20 0.3115 -6853.43 -0.08 -15.85 0.12
21 0.3332 -7096.60 0.09 -8.24 0.06
22 0.8872 5230.14 -0.00 15.22 0.00
23 0.8899 5257.74 -0.02 13.93 0.00
24 0.9638 5465.89 -0.04 -21.12 -0.04
25 0.9747 5409.26 0.19 -25.94 0.13
26 1.0512 4430.52 0.00 -56.73 -0.01
27 1.0621 4218.60 0.02 -60.17 0.06
28 1.2149 334.75 -0.21 -76.52 -0.15
29 1.2258 60.43 0.04 -75.01 -0.05
30 1.3025 -1523.70 0.20 -56.45 -0.10
31 1.3053 -1566.45 0.01 -55.34 0.07
32 1.3656 -2138.66 -0.15 -32.67 0.04
33 1.4502 -1726.29 -0.02 2.49 -0.10
34 3.9481 21032.24 0.03 -125.48 0.05
35 3.9646 21023.94 -0.06 -133.58 -0.09
36 4.0546 20099.82 -0.00 -171.38 -0.03
37 4.0682 19846.69 0.06 -175.63 0.13
38 4.0683 19844.05 -0.02 -175.79 -0.01
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.
13SE101 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.464 44.472 44.455 ecceobj 0.083 0.083 0.083 incobj 0.909 0.909 0.909 qmin 39.663 39.675 39.662 qmax 48.977 48.958 48.936 amean 44.185 44.185 44.176 amin 43.820 43.837 43.826 amax 44.577 44.567 44.558 emean 0.083 0.082 0.083 emin 0.066 0.065 0.066 emax 0.099 0.099 0.099 imean 1.365 1.343 1.354 imin 0.589 0.546 0.560 imax 1.981 1.976 1.985 excite_mean 0.087 0.086 0.086 fracstop 1.000 1.000 1.000 cjmean 3.095 3.095 3.095 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 198.0 200.8 200.4 kozaiamp 180.0 180.0 179.9