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: 14SZ403 # Created Sat Apr 27 01:16:24 2024 # Orbit generated from Bernstein formalism # Fitting 12 observations of 12 # Arc: 4.18y # First observation: 2014/09/25 # Last observation: 2018/11/30 Preliminary a, adot, b, bdot, g, gdot: 0.000085 0.027348 0.000039 0.011540 0.027229 0.000000 # Chi-squared of fit: 2.84 DOF: 18 RMS: 0.09 # Min/Max residuals: -0.18 0.22 # Exact a, adot, b, bdot, g, gdot: 1.588403E-05 2.755726E-02 7.583449E-06 1.163641E-02 2.742025E-02 1.301342E-04 # Covariance matrix: 5.4252E-13 -5.6818E-13 1.6774E-13 -2.6723E-13 -6.8147E-14 -4.8497E-12 -5.6818E-13 9.9455E-13 -3.4813E-13 5.6171E-13 3.6243E-14 1.0147E-11 1.6774E-13 -3.4813E-13 4.4506E-13 -3.2765E-13 1.6913E-14 -3.8877E-12 -2.6723E-13 5.6171E-13 -3.2765E-13 4.1983E-13 -5.7929E-14 6.3571E-12 -6.8147E-14 3.6243E-14 1.6913E-14 -5.7929E-14 4.5279E-13 -8.4538E-13 -4.8497E-12 1.0147E-11 -3.8877E-12 6.3571E-12 -8.4538E-13 1.1428E-10 # lat0 lon0 xBary yBary zBary JD0 -20.455130 13.567965 0.204930 -0.343839 -0.922281 2456925.737488 # Heliocentric elements and errors Epoch: 2456920.5000 = 2014/09/20 Mean Anomaly: 0.44942 +/- 0.143 Argument of Peri: 316.26462 +/- 0.185 Long of Asc Node: 52.31567 +/- 0.001 Inclination: 29.90512 +/- 0.000 Eccentricity: 0.12437952 +/- 0.0001 Semi-Major Axis: 42.70300308 +/- 0.0066 Time of Perihelion: 2456793.2574 +/- 40.4 Perihelion: 37.39162423 +/- 0.0078 Aphelion: 48.01438193 +/- 0.0091 Period (y) 279.0589 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 34.21870031 +/- 0.0008 Ecliptic Y 8.04982979 +/- 0.0002 Ecliptic Z -12.74486670 +/- 0.0003 Ecliptic XDOT -0.00024361 +/- 0.0000 Ecliptic YDOT 0.00276827 +/- 0.0000 Ecliptic ZDOT 0.00108418 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.39185524 +/- 0.0008 Geocenter to KBO 36.46940214 +/- 0.0009 # Hcoef: 7.84
The following table shows the complete astrometric record for 14SZ403. 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 (14SZ403) followed by the observatory code and reference code for the source of the astrometry.
2014 09 25.23671 01 22 01.954 -13 29 08.37 23.0r 14SZ403 W84 C~55S9 2014 11 21.18961 01 17 13.208 -13 42 30.41 23.8r 14SZ403 W84 C~55S9 2015 08 23.38949 01 29 04.882 -11 55 36.95 24.0i 14SZ403 W84 C~55S9 2015 09 13.27672 01 27 49.240 -12 07 57.05 22.8i 14SZ403 W84 C~55S9 2015 09 13.27810 01 27 49.232 -12 07 57.10 23.5r 14SZ403 W84 C~55S9 2015 09 13.27948 01 27 49.219 -12 07 56.98 24.2g 14SZ403 W84 C~55S9 2015 10 22.22357 01 24 30.983 -12 25 55.55 22.6z 14SZ403 W84 C~55S9 2016 08 16.36629 01 34 04.211 -10 37 51.16 23.4i 14SZ403 W84 C~55S9 2016 08 16.42031 01 34 04.086 -10 37 52.95 23.8r 14SZ403 W84 C~55S9 2017 11 27.13679 01 31 08.416 -10 00 17.43 23.5i 14SZ403 W84 C~55S9 2018 11 30.09981 01 35 39.585 -08 45 37.36 23.5r 14SZ403 W84 C~55S9 2018 11 30.10118 01 35 39.578 -08 45 37.40 24.5g 14SZ403 W84 C~55S9
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 0.00 0.00 -0.18
2 0.1559 -4184.48 0.00 927.91 -0.02
3 0.9094 7922.95 -0.18 2662.09 0.13
4 0.9666 6607.22 0.07 2431.94 0.02
5 0.9666 6607.09 0.05 2431.94 0.03
6 0.9666 6606.96 0.02 2432.13 0.22
7 1.0732 3510.75 0.04 2609.89 -0.02
8 1.8922 13859.88 0.07 5147.14 -0.09
9 1.8924 13857.46 -0.01 5146.25 -0.09
10 3.1729 12401.82 -0.11 8268.76 -0.02
11 4.1803 17929.90 0.05 10751.23 0.02
12 4.1803 17929.79 0.00 10751.24 -0.02
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.
14SZ403 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 43.070 43.093 43.047 ecceobj 0.132 0.132 0.132 incobj 29.874 29.874 29.873 qmin 36.606 36.611 36.604 qmax 49.321 49.427 49.316 amean 42.830 42.854 42.807 amin 42.491 42.509 42.467 amax 43.211 43.236 43.174 emean 0.126 0.127 0.126 emin 0.111 0.112 0.110 emax 0.142 0.143 0.142 imean 28.867 28.868 28.865 imin 28.468 28.475 28.467 imax 29.228 29.235 29.228 excite_mean 0.499 0.499 0.499 fracstop 1.000 1.000 1.000 cjmean 2.775 2.775 2.775 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 170.8 171.0 170.8 kozaiamp 180.0 180.0 180.0