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: 14SY403 # Created Tue Apr 23 01:16:15 2024 # Orbit generated from Bernstein formalism # Fitting 11 observations of 11 # Arc: 4.02y # First observation: 2014/09/25 # Last observation: 2018/10/01 Preliminary a, adot, b, bdot, g, gdot: 0.000287 0.023614 -0.000098 -0.005742 0.024276 0.000000 # Chi-squared of fit: 2.48 DOF: 16 RMS: 0.08 # Min/Max residuals: -0.12 0.18 # Exact a, adot, b, bdot, g, gdot: 1.597871E-05 2.415992E-02 -3.970285E-06 -5.862010E-03 2.425961E-02 6.258921E-03 # Covariance matrix: 5.9466E-13 -2.4682E-13 -4.7848E-14 1.8103E-14 2.4117E-13 -1.0578E-12 -2.4682E-13 4.8576E-13 1.2220E-14 -9.3190E-14 2.9760E-13 5.3460E-12 -4.7848E-14 1.2220E-14 4.6208E-13 -1.7312E-13 -9.2668E-14 1.7107E-13 1.8103E-14 -9.3190E-14 -1.7312E-13 1.1631E-13 -7.1083E-14 -1.2721E-12 2.4117E-13 2.9760E-13 -9.2668E-14 -7.1083E-14 8.9754E-13 4.0345E-12 -1.0578E-12 5.3460E-12 1.7107E-13 -1.2721E-12 4.0345E-12 7.2980E-11 # lat0 lon0 xBary yBary zBary JD0 -26.144108 -0.842440 -0.046068 -0.442410 -0.901660 2456925.714078 # Heliocentric elements and errors Epoch: 2456920.5000 = 2014/09/20 Mean Anomaly: 38.08671 +/- 0.018 Argument of Peri: 176.41961 +/- 0.034 Long of Asc Node: 118.92829 +/- 0.001 Inclination: 28.81888 +/- 0.000 Eccentricity: 0.30258382 +/- 0.0004 Semi-Major Axis: 51.84341196 +/- 0.0142 Time of Perihelion: 2442495.7035 +/- 3.2 Perihelion: 36.15643416 +/- 0.0207 Aphelion: 67.53038977 +/- 0.0260 Period (y) 373.2919 +/- 0.15 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 38.00185813 +/- 0.0014 Ecliptic Y -0.51076101 +/- 0.0000 Ecliptic Z -18.16329780 +/- 0.0007 Ecliptic XDOT 0.00037799 +/- 0.0000 Ecliptic YDOT 0.00271668 +/- 0.0000 Ecliptic ZDOT -0.00090501 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 42.12252943 +/- 0.0013 Geocenter to KBO 41.22077553 +/- 0.0016 # Hcoef: 7.26
The following table shows the complete astrometric record for 14SY403. 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 (14SY403) followed by the observatory code and reference code for the source of the astrometry.
2014 09 25.21330 00 41 12.641 -24 10 28.99 23.4i 14SY403 W84 C~55S9 2014 10 27.18200 00 38 43.601 -24 21 27.15 23.5r 14SY403 W84 C~55S9 2014 12 12.12302 00 36 32.903 -24 12 07.04 23.7r 14SY403 W84 C~55S9 2016 09 05.33601 00 54 34.394 -23 20 55.10 23.9i 14SY403 W84 C~55S9 2016 10 08.16723 00 52 08.213 -23 39 44.30 23.4i 14SY403 W84 C~55S9 2016 10 08.16860 00 52 08.201 -23 39 44.35 23.5r 14SY403 W84 C~55S9 2016 10 28.14083 00 50 36.491 -23 45 10.98 24.4g 14SY403 W84 C~55S9 2016 12 21.10058 00 48 15.067 -23 31 46.76 23.7r 14SY403 W84 C~55S9 2016 12 21.10197 00 48 15.061 -23 31 46.78 23.1i 14SY403 W84 C~55S9 2017 11 23.06961 00 54 50.646 -23 25 00.87 23.1z 14SY403 W84 C~55S9 2018 10 01.33738 01 04 17.384 -22 56 53.20 22.6i 14SY403 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 -0.05 0.00 0.03
2 0.0875 -2121.86 -0.08 291.51 0.02
3 0.2133 -3494.45 0.08 1566.13 -0.09
4 1.9469 11187.38 -0.10 -2256.75 -0.01
5 2.0368 8877.42 0.13 -2346.51 -0.02
6 2.0368 8877.25 0.06 -2346.48 0.00
7 2.0915 7603.93 0.18 -2067.87 0.04
8 2.2393 6226.86 -0.01 -475.60 0.00
9 2.2393 6226.78 -0.11 -475.59 -0.03
10 3.1618 11274.38 -0.11 -2578.18 0.16
11 4.0168 19023.27 0.01 -4726.90 -0.12
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.
14SY403 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 52.369 52.413 52.326 ecceobj 0.308 0.308 0.307 incobj 28.796 28.796 28.796 qmin 34.637 34.363 34.522 qmax 70.160 70.640 70.330 amean 52.048 52.095 52.040 amin 51.494 51.598 51.520 amax 52.701 52.758 52.682 emean 0.314 0.320 0.314 emin 0.294 0.298 0.293 emax 0.333 0.339 0.335 imean 26.838 26.595 26.810 imin 26.383 26.108 26.323 imax 27.563 27.348 27.457 excite_mean 0.550 0.550 0.550 fracstop 1.000 1.000 1.000 cjmean 2.806 2.807 2.806 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 187.0 181.9 185.4 kozaiamp 180.0 180.0 179.9