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: 14SU403 # Created Sat Apr 20 01:16:25 2024 # Orbit generated from Bernstein formalism # Fitting 13 observations of 13 # Arc: 4.30y # First observation: 2014/09/24 # Last observation: 2019/01/10 Preliminary a, adot, b, bdot, g, gdot: 0.000095 0.018863 0.000014 -0.008048 0.021104 0.000000 # Chi-squared of fit: 4.80 DOF: 20 RMS: 0.11 # Min/Max residuals: -0.19 0.26 # Exact a, adot, b, bdot, g, gdot: 1.511436E-05 1.876576E-02 -6.039683E-06 -8.007900E-03 2.090897E-02 1.631726E-04 # Covariance matrix: 6.2076E-13 -9.8051E-14 4.2041E-14 -7.8313E-17 3.2656E-13 -5.1096E-15 -9.8051E-14 4.1964E-13 1.5288E-13 -2.0765E-13 3.6240E-13 5.8920E-12 4.2041E-14 1.5288E-13 4.2667E-13 -2.0800E-13 1.9127E-13 2.4569E-12 -7.8313E-17 -2.0765E-13 -2.0800E-13 1.8056E-13 -1.9371E-13 -3.4216E-12 3.2656E-13 3.6240E-13 1.9127E-13 -1.9371E-13 7.1638E-13 5.4882E-12 -5.1096E-15 5.8920E-12 2.4569E-12 -3.4216E-12 5.4882E-12 9.7099E-11 # lat0 lon0 xBary yBary zBary JD0 -39.132280 53.752652 0.801039 -0.383587 -0.471717 2456924.861168 # Heliocentric elements and errors Epoch: 2456920.5000 = 2014/09/20 Mean Anomaly: 356.56701 +/- 0.134 Argument of Peri: 247.98579 +/- 0.192 Long of Asc Node: 177.93553 +/- 0.001 Inclination: 44.47342 +/- 0.000 Eccentricity: 0.16781450 +/- 0.0001 Semi-Major Axis: 58.01683413 +/- 0.0093 Time of Perihelion: 2458459.7149 +/- 60.3 Perihelion: 48.28076809 +/- 0.0101 Aphelion: 67.75290017 +/- 0.0126 Period (y) 441.9155 +/- 0.11 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 22.93770447 +/- 0.0009 Ecliptic Y 29.93720456 +/- 0.0012 Ecliptic Z -30.18409857 +/- 0.0012 Ecliptic XDOT -0.00236781 +/- 0.0000 Ecliptic YDOT 0.00092797 +/- 0.0000 Ecliptic ZDOT -0.00082673 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 48.30584137 +/- 0.0011 Geocenter to KBO 47.82636877 +/- 0.0019 # Hcoef: 6.95
The following table shows the complete astrometric record for 14SU403. 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 (14SU403) followed by the observatory code and reference code for the source of the astrometry.
2014 09 24.36039 04 03 42.891 -19 16 50.45 24.9g 14SU403 W84 C~55S9 2014 11 04.34065 04 01 38.134 -19 44 37.53 23.6r 14SU403 W84 C~55S9 2014 12 11.20664 03 58 58.121 -19 53 18.48 23.2i 14SU403 W84 C~55S9 2015 12 11.21063 04 03 55.429 -20 04 18.25 23.8r 14SU403 W84 C~55S9 2016 01 13.16875 04 01 58.309 -19 55 55.70 24.5g 14SU403 W84 C~55S9 2016 11 03.31890 04 11 33.843 -20 05 18.46 23.0r 14SU403 W84 C~55S9 2016 11 03.34741 04 11 33.708 -20 05 19.60 23.8i 14SU403 W84 C~55S9 2016 11 29.23112 04 09 41.513 -20 14 00.79 24.1g 14SU403 W84 C~55S9 2017 01 30.12183 04 06 17.034 -19 56 37.10 23.1r 14SU403 W84 C~55S9 2017 11 24.31628 04 15 02.074 -20 22 52.84 23.8r 14SU403 W84 C~55S9 2017 11 24.31766 04 15 02.085 -20 22 52.77 24.5g 14SU403 W84 C~55S9 2018 10 18.36238 04 22 27.144 -20 14 05.04 23.4i 14SU403 W84 C~55S9 2019 01 10.16646 04 16 51.413 -20 27 29.07 25.2g 14SU403 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 -0.19 0.00 -0.00
2 0.1122 -2121.95 0.26 -1178.25 -0.01
3 0.2131 -4439.51 -0.07 -1131.77 0.01
4 1.2125 -538.55 0.00 -2802.20 -0.01
5 1.3027 -2013.23 -0.03 -1905.73 -0.04
6 2.1108 5693.62 0.20 -4508.11 0.01
7 2.1108 5691.48 -0.13 -4508.72 -0.19
8 2.1817 4029.28 -0.09 -4602.57 0.15
9 2.3512 1509.40 0.05 -2857.12 0.16
10 3.1676 8248.75 -0.10 -6299.13 -0.03
11 3.1676 8248.92 0.16 -6299.11 -0.01
12 4.0657 14442.68 -0.03 -7494.28 0.00
13 4.2952 9660.31 -0.03 -6977.58 -0.04
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.
14SU403 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 58.342 58.369 58.314 ecceobj 0.172 0.172 0.172 incobj 44.365 44.365 44.365 qmin 47.485 47.495 47.500 qmax 68.656 68.718 68.642 amean 57.831 57.857 57.806 amin 57.301 57.334 57.266 amax 58.417 58.431 58.409 emean 0.160 0.159 0.160 emin 0.146 0.142 0.148 emax 0.175 0.176 0.175 imean 43.987 43.995 43.982 imin 43.753 43.744 43.753 imax 44.243 44.284 44.236 excite_mean 0.713 0.713 0.713 fracstop 1.000 1.000 1.000 cjmean 2.489 2.489 2.489 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 223.8 210.7 228.9 kozaiamp 180.0 180.0 180.0