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: 14UX276 # Created Sun Nov 24 02:10:05 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 20 observations of 20 # Arc: 11.08y # First observation: 2013/10/04 # Last observation: 2024/11/01 # Chi-squared of fit: 32.36 DOF: 34 RMS: 0.22 # Min/Max residuals: -0.85 0.47 # Exact a, adot, b, bdot, g, gdot: 1.606835E-05 2.498148E-02 8.153225E-07 1.396355E-03 2.470978E-02 2.051434E-03 # Covariance matrix: 6.9339E-13 -3.5762E-13 2.2920E-14 -1.9769E-14 2.4223E-13 -1.1613E-12 -3.5762E-13 2.1787E-13 -1.4885E-14 1.2507E-14 -1.3888E-13 7.3395E-13 2.2920E-14 -1.4885E-14 1.6488E-13 -2.4477E-14 2.4697E-15 -5.1250E-14 -1.9769E-14 1.2507E-14 -2.4477E-14 7.2449E-15 -8.2589E-15 4.3434E-14 2.4223E-13 -1.3888E-13 2.4697E-15 -8.2589E-15 3.6721E-13 -4.9875E-13 -1.1613E-12 7.3395E-13 -5.1250E-14 4.3434E-14 -4.9875E-13 2.5496E-12 # lat0 lon0 xBary yBary zBary JD0 -8.638205 13.292953 0.044241 -0.149997 -0.988059 2456569.661028 # Heliocentric elements and errors Epoch: 2456570.5000 = 2013/10/05 Mean Anomaly: 38.66116 +/- 0.021 Argument of Peri: 242.53113 +/- 0.024 Long of Asc Node: 82.61800 +/- 0.001 Inclination: 8.99850 +/- 0.000 Eccentricity: 0.11465213 +/- 0.0001 Semi-Major Axis: 45.24256804 +/- 0.0066 Time of Perihelion: 2444633.5981 +/- 6.9 Perihelion: 40.05541142 +/- 0.0079 Aphelion: 50.42972467 +/- 0.0091 Period (y) 304.3190 +/- 0.07 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 39.92091934 +/- 0.0010 Ecliptic Y 9.38947434 +/- 0.0002 Ecliptic Z -6.07833857 +/- 0.0002 Ecliptic XDOT -0.00040129 +/- 0.0000 Ecliptic YDOT 0.00274944 +/- 0.0000 Ecliptic ZDOT 0.00011896 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 41.45821995 +/- 0.0009 Geocenter to KBO 40.46978575 +/- 0.0010 # Hcoef: 7.26
The following table shows the complete astrometric record for 14UX276. 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 (14UX276) followed by the observatory code and reference code for the source of the astrometry.
2013 10 04.16025 01 02 19.567 -02 42 55.96 24.6g 14UX276 W84 C~52UR 2014 10 28.24320 01 05 40.889 -02 15 15.80 23.6r 14UX276 W84 C~52UR 2014 10 28.24457 01 05 40.895 -02 15 15.75 22.8i 14UX276 W84 C~52UR 2014 11 15.02261 01 04 29.991 -02 20 19.87 23.1i 14UX276 W84 C~52UR 2014 11 15.09076 01 04 29.748 -02 20 20.52 23.7r 14UX276 W84 C~52UR 2014 11 16.06419 01 04 26.307 -02 20 32.40 23.2i 14UX276 W84 C~52UR 2014 11 17.11068 01 04 22.661 -02 20 44.86 23.3i 14UX276 W84 C~52UR 2014 11 21.03676 01 04 09.604 -02 21 25.88 22.4z 14UX276 W84 C~52UR 2015 09 04.30277 01 14 37.759 -01 13 19.94 22.9z 14UX276 W84 C~52UR 2016 08 16.40088 01 20 29.789 -00 28 39.02 23.6i 14UX276 W84 C~52UR 2016 08 16.40224 01 20 29.801 -00 28 39.24 23.2r 14UX276 W84 C~52UR 2016 08 25.39991 01 20 08.632 -00 32 10.57 23.3z 14UX276 W84 C~52UR 2016 11 05.18380 01 15 16.388 -01 03 20.18 23.3i 14UX276 W84 C~52UR 2016 11 05.18518 01 15 16.393 -01 03 19.84 23.5r 14UX276 W84 C~52UR 2017 08 22.41422 01 25 17.803 +00 06 01.77 23.1i 14UX276 W84 C~52UR 2017 08 27.37907 01 25 05.246 +00 04 03.04 23.2r 14UX276 W84 C~52UR 2017 09 18.26904 01 23 51.253 -00 05 44.29 23.2r 14UX276 W84 C~52UR 2024 11 01.24356 01 55 34.265 +03 50 58.91 24.1G 14UX276 G37 2024 11 01.29112 01 55 34.050 +03 50 57.96 14UX276 G37 2024 11 01.33676 01 55 33.818 +03 50 57.04 14UX276 G37
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 -0.02 0.00 0.01
2 1.0653 0.00 -0.12 0.00 0.11
3 1.0653 0.00 0.06 0.00 0.19
4 1.1139 0.00 -0.19 0.00 -0.29
5 1.1141 0.00 -0.11 0.00 -0.08
6 1.1168 0.00 -0.04 0.00 0.08
7 1.1196 0.00 0.01 0.00 -0.01
8 1.1304 0.00 0.47 0.00 -0.07
9 1.9169 0.00 0.02 0.00 0.03
10 2.8672 0.00 -0.03 0.00 0.03
11 2.8672 0.00 0.20 0.00 -0.16
12 2.8918 0.00 -0.11 0.00 0.02
13 3.0884 0.00 -0.16 0.00 -0.01
14 3.0884 0.00 0.01 0.00 0.35
15 3.8830 0.00 -0.00 0.00 -0.15
16 3.8966 0.00 0.15 0.00 0.01
17 3.9565 0.00 -0.05 0.00 -0.01
18 11.0776 0.00 -0.57 0.00 -0.20
19 11.0777 0.00 -0.52 0.00 -0.12
20 11.0778 0.00 -0.85 0.00 -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.
14UX276 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 45.532 45.553 45.510 ecceobj 0.120 0.121 0.120 incobj 9.003 9.003 9.003 qmin 39.413 39.418 39.410 qmax 51.401 51.445 51.355 amean 45.242 45.264 45.222 amin 44.876 44.885 44.840 amax 45.655 45.670 45.634 emean 0.112 0.113 0.112 emin 0.098 0.098 0.097 emax 0.127 0.127 0.126 imean 7.233 7.234 7.231 imin 6.729 6.745 6.725 imax 7.824 7.818 7.824 excite_mean 0.169 0.169 0.168 fracstop 1.000 1.000 1.000 cjmean 3.082 3.082 3.082 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 187.1 187.5 186.7 kozaiamp 180.0 180.0 180.0