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: 14SL403 # Created Fri Nov 22 02:10:03 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 11 observations of 11 # Arc: 5.05y # First observation: 2013/11/08 # Last observation: 2018/11/28 # Chi-squared of fit: 6.16 DOF: 16 RMS: 0.13 # Min/Max residuals: -0.20 0.31 # Exact a, adot, b, bdot, g, gdot: 1.550320E-05 2.406970E-02 -4.621486E-07 4.924155E-04 2.424670E-02 2.746668E-03 # Covariance matrix: 6.0353E-13 -4.6012E-13 -2.2931E-14 -1.9226E-15 -2.2696E-13 -2.8739E-12 -4.6012E-13 6.9698E-13 -5.9574E-14 2.5462E-15 -1.3038E-13 4.9816E-12 -2.2931E-14 -5.9574E-14 3.5975E-13 -9.4969E-14 2.1838E-13 -4.1342E-13 -1.9226E-15 2.5462E-15 -9.4969E-14 4.9491E-14 1.2659E-15 1.9976E-14 -2.2696E-13 -1.3038E-13 2.1838E-13 1.2659E-15 1.1235E-12 -7.6433E-13 -2.8739E-12 4.9816E-12 -4.1342E-13 1.9976E-14 -7.6433E-13 3.8378E-11 # lat0 lon0 xBary yBary zBary JD0 -35.587044 -26.863084 -0.943263 -0.174010 -0.243401 2456604.610328 # Heliocentric elements and errors Epoch: 2456604.5000 = 2013/11/08 Mean Anomaly: 63.38259 +/- 0.048 Argument of Peri: 193.82160 +/- 0.054 Long of Asc Node: 61.24755 +/- 0.001 Inclination: 35.38763 +/- 0.000 Eccentricity: 0.14233900 +/- 0.0003 Semi-Major Axis: 43.50169569 +/- 0.0107 Time of Perihelion: 2438153.2759 +/- 15.5 Perihelion: 37.30970796 +/- 0.0154 Aphelion: 49.69368342 +/- 0.0174 Period (y) 286.9244 +/- 0.11 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 30.61335129 +/- 0.0013 Ecliptic Y -14.44611064 +/- 0.0007 Ecliptic Z -24.00081818 +/- 0.0011 Ecliptic XDOT 0.00147579 +/- 0.0000 Ecliptic YDOT 0.00229428 +/- 0.0000 Ecliptic ZDOT -0.00013513 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 41.49577579 +/- 0.0012 Geocenter to KBO 41.24270162 +/- 0.0018 # Hcoef: 7.39
The following table shows the complete astrometric record for 14SL403. 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 (14SL403) followed by the observatory code and reference code for the source of the astrometry.
2013 11 08.10955 23 26 51.210 -42 51 02.08 23.9r 14SL403 W84 C~52UA 2013 11 08.11249 23 26 51.216 -42 51 02.05 23.6i 14SL403 W84 C~52UA 2014 09 20.16530 23 37 23.685 -42 17 41.70 23.8r 14SL403 W84 C~52UA 2014 09 30.14918 23 36 23.531 -42 19 22.14 23.8i 14SL403 W84 C~52UA 2014 11 14.16055 23 32 58.936 -42 05 24.49 23.7r 14SL403 W84 C~52UA 2015 09 04.24119 23 45 15.431 -41 26 45.02 22.7z 14SL403 W84 C~52UA 2015 10 04.13208 23 42 17.499 -41 35 30.40 23.4r 14SL403 W84 C~52UA 2015 10 04.13344 23 42 17.478 -41 35 30.43 23.4i 14SL403 W84 C~52UA 2016 10 03.16757 23 48 23.533 -40 50 27.36 23.3r 14SL403 W84 C~52UA 2018 09 19.33780 00 01 25.540 -39 14 08.97 22.9r 14SL403 W84 C~52UA 2018 11 28.05523 23 56 14.886 -38 58 45.78 24.3r 14SL403 W84 C~52UA
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 -0.06 0.00 0.16
2 0.0000 0.00 0.17 0.00 0.08
3 0.8653 0.00 -0.17 0.00 -0.01
4 0.8926 0.00 -0.20 0.00 -0.04
5 1.0159 0.00 -0.05 0.00 -0.18
6 1.8210 0.00 0.31 0.00 0.04
7 1.9029 0.00 0.15 0.00 -0.03
8 1.9029 0.00 -0.04 0.00 -0.05
9 2.9023 0.00 0.08 0.00 0.02
10 4.8630 0.00 -0.19 0.00 -0.09
11 5.0539 0.00 0.08 0.00 0.13
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.
14SL403 quality flag:3 Type: 7:4EEE 7:4EEE 7:4EEE Type: 7:4EII 7:4EII 7:4EII axisobj 43.716 43.716 43.716 ecceobj 0.144 0.144 0.144 incobj 35.414 35.414 35.414 qmin 30.239 30.221 30.235 qmax 57.838 57.853 57.819 amean 43.724 43.724 43.724 amin 43.312 43.313 43.323 amax 44.235 44.234 44.229 emean 0.213 0.214 0.213 emin 0.126 0.127 0.122 emax 0.308 0.308 0.308 imean 32.943 32.928 32.947 imin 30.888 30.871 30.875 imax 34.567 34.528 34.614 excite_mean 0.588 0.588 0.588 fracstop 1.000 1.000 1.000 cjmean 2.660 2.660 2.660 libcent 0 180.7 182.8 179.1 libamp 0 96.4 94.0 98.6 libcent 1 180.5 180.0 181.2 libamp 1 114.2 112.7 115.9 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 180.5 180.2 180.8 kozaiamp 29.4 29.1 29.8