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: 16SB106 # Created Wed May 8 01:18:01 2024 # Orbit generated from Bernstein formalism # Fitting 14 observations of 14 # Arc: 4.17y # First observation: 2014/08/18 # Last observation: 2018/10/18 Preliminary a, adot, b, bdot, g, gdot: 0.000078 0.022039 -0.000001 -0.000070 0.023308 0.000000 # Chi-squared of fit: 2.36 DOF: 22 RMS: 0.07 # Min/Max residuals: -0.13 0.20 # Exact a, adot, b, bdot, g, gdot: 1.529697E-05 2.194780E-02 3.039333E-08 -6.792056E-05 2.316518E-02 -4.348203E-04 # Covariance matrix: 7.9223E-13 -1.4252E-13 -1.9959E-15 1.1124E-15 5.4181E-13 -1.0483E-12 -1.4252E-13 3.4739E-13 5.7613E-16 -1.3208E-15 1.9691E-13 4.4420E-12 -1.9959E-15 5.7613E-16 3.3222E-13 -1.1274E-13 -1.9929E-15 1.1297E-14 1.1124E-15 -1.3208E-15 -1.1274E-13 5.5810E-14 3.1008E-16 -2.1392E-14 5.4181E-13 1.9691E-13 -1.9929E-15 3.1008E-16 8.2397E-13 2.2686E-12 -1.0483E-12 4.4420E-12 1.1297E-14 -2.1392E-14 2.2686E-12 6.8442E-11 # lat0 lon0 xBary yBary zBary JD0 -4.633542 -1.040573 0.565760 -0.067951 -0.839943 2456887.797898 # Heliocentric elements and errors Epoch: 2456880.5000 = 2014/08/11 Mean Anomaly: 268.36163 +/- 0.200 Argument of Peri: 2.54858 +/- 0.180 Long of Asc Node: 91.24998 +/- 0.008 Inclination: 4.55110 +/- 0.000 Eccentricity: 0.03457146 +/- 0.0004 Semi-Major Axis: 43.91448794 +/- 0.0064 Time of Perihelion: 2483937.8363 +/- 58.6 Perihelion: 42.39630000 +/- 0.0176 Aphelion: 45.43267587 +/- 0.0178 Period (y) 291.0181 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 43.85009676 +/- 0.0017 Ecliptic Y -1.36019553 +/- 0.0001 Ecliptic Z -3.48723545 +/- 0.0001 Ecliptic XDOT -0.00000965 +/- 0.0000 Ecliptic YDOT 0.00259020 +/- 0.0000 Ecliptic ZDOT -0.00000373 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.00956634 +/- 0.0017 Geocenter to KBO 43.16822941 +/- 0.0017 # Hcoef: 6.82
The following table shows the complete astrometric record for 16SB106. 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 (16SB106) followed by the observatory code and reference code for the source of the astrometry.
2014 08 18.29712 00 03 34.216 -04 39 51.30 23.0i 16SB106 W84 C~55a1 2014 10 01.27583 00 00 37.932 -05 00 00.80 23.1i 16SB106 W84 C~55a1 2014 10 29.18235 23 58 49.918 -05 10 21.16 22.9i 16SB106 W84 C~55a1 2014 11 14.01786 23 58 04.933 -05 13 51.40 22.5z 16SB106 W84 C~55a1 2016 09 22.095104 00 10 32.24 -03 56 03.6 22.9r 16SB106 W84 C~55a1 2016 09 22.096481 00 10 32.24 -03 56 03.4 24.0g 16SB106 W84 C~55a1 2016 09 30.179479 00 09 57.58 -03 59 45.5 23.2r 16SB106 W84 C~55a1 2016 09 30.180845 00 09 57.57 -03 59 45.6 22.7i 16SB106 W84 C~55a1 2016 11 26.120521 00 06 51.39 -04 16 03.6 22.7i 16SB106 W84 C~55a1 2016 11 26.121887 00 06 51.37 -04 16 03.4 23.4r 16SB106 W84 C~55a1 2017 10 17.22970 00 13 26.163 -03 36 36.43 23.3i 16SB106 W84 C~55a1 2017 10 17.23107 00 13 26.154 -03 36 36.46 23.4r 16SB106 W84 C~55a1 2018 10 18.17954 00 18 01.851 -03 06 34.81 23.1z 16SB106 W84 C~55a1 2018 10 18.18092 00 18 01.847 -03 06 34.75 23.1i 16SB106 W84 C~55a1
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 -0.07 0.00 -0.02
2 0.1204 -2898.79 0.02 -59.19 0.05
3 0.1968 -4626.80 0.03 13.50 -0.07
4 0.2402 -5327.42 0.02 87.55 0.04
5 2.0966 6784.18 -0.05 -93.57 -0.09
6 2.0966 6784.26 0.13 -93.39 0.10
7 2.1188 6219.51 0.01 -88.83 -0.03
8 2.1188 6219.33 -0.07 -88.87 -0.07
9 2.2747 3273.75 0.03 130.67 -0.09
10 2.2747 3273.56 -0.13 130.97 0.20
11 3.1648 9641.52 0.09 -69.81 -0.03
12 3.1648 9641.39 0.05 -69.78 -0.01
13 4.1667 14160.89 -0.06 -81.89 -0.03
14 4.1667 14160.85 -0.00 -81.81 0.05
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.
16SB106 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.258 44.277 44.239 ecceobj 0.034 0.034 0.034 incobj 4.553 4.553 4.553 qmin 41.404 41.399 41.392 qmax 46.923 46.952 46.895 amean 44.065 44.084 44.046 amin 43.716 43.743 43.709 amax 44.418 44.435 44.396 emean 0.041 0.041 0.041 emin 0.025 0.025 0.025 emax 0.057 0.057 0.057 imean 2.875 2.873 2.876 imin 2.203 2.208 2.197 imax 3.512 3.509 3.519 excite_mean 0.065 0.065 0.065 fracstop 1.000 1.000 1.000 cjmean 3.097 3.097 3.097 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 174.1 174.8 173.5 kozaiamp 180.0 180.0 180.0