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: 14SU373 # Created Fri Nov 22 02:10:02 2024 # Orbit generated from Bernstein formalism # Fitting 39 observations of 40 # Arc: 4.17y # First observation: 2014/09/30 # Last observation: 2018/12/02 Preliminary a, adot, b, bdot, g, gdot: -0.000658 0.032178 -0.000084 -0.001499 0.027533 0.000000 # Chi-squared of fit: 9.09 DOF: 72 RMS: 0.09 # Min/Max residuals: -0.24 0.21 # Exact a, adot, b, bdot, g, gdot: 1.780663E-05 3.120485E-02 -8.633597E-07 -1.479714E-03 2.730324E-02 -7.893459E-03 # Covariance matrix: 3.1491E-13 -2.5036E-13 -1.9559E-14 9.8917E-15 5.3044E-14 -1.5529E-12 -2.5036E-13 2.9441E-13 6.2443E-15 -9.1119E-15 3.8492E-14 2.0898E-12 -1.9559E-14 6.2443E-15 1.3460E-13 -5.1378E-14 -3.2788E-14 4.2700E-14 9.8917E-15 -9.1119E-15 -5.1378E-14 2.7803E-14 5.6071E-15 -7.0009E-14 5.3044E-14 3.8492E-14 -3.2788E-14 5.6071E-15 1.9109E-13 3.3489E-13 -1.5529E-12 2.0898E-12 4.2700E-14 -7.0009E-14 3.3489E-13 1.6351E-11 # lat0 lon0 xBary yBary zBary JD0 -28.775430 10.817717 0.072006 -0.481846 -0.877702 2456930.738618 # Heliocentric elements and errors Epoch: 2456930.5000 = 2014/09/30 Mean Anomaly: 337.23464 +/- 0.007 Argument of Peri: 318.15265 +/- 0.018 Long of Asc Node: 106.28795 +/- 0.001 Inclination: 28.15420 +/- 0.000 Eccentricity: 0.39853814 +/- 0.0001 Semi-Major Axis: 55.25908730 +/- 0.0075 Time of Perihelion: 2466418.5289 +/- 2.2 Perihelion: 33.23623341 +/- 0.0079 Aphelion: 77.28194119 +/- 0.0124 Period (y) 410.7842 +/- 0.08 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 32.52682157 +/- 0.0005 Ecliptic Y 6.14438374 +/- 0.0001 Ecliptic Z -17.63086000 +/- 0.0003 Ecliptic XDOT -0.00134350 +/- 0.0000 Ecliptic YDOT 0.00292524 +/- 0.0000 Ecliptic ZDOT 0.00025108 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.50459702 +/- 0.0005 Geocenter to KBO 36.62569516 +/- 0.0006 # Hcoef: 7.54
The following table shows the complete astrometric record for 14SU373. 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 (14SU373) followed by the observatory code and reference code for the source of the astrometry.
2014 09 30.23784 01 26 45.328 -22 05 58.57 24.1g 14SU373 W84 C~4yUX 2014 09 30.23784 01 26 45.33 -22 05 58.6 24.2g 14SU373 W84 C~3cnr 2014 12 17.14284 01 21 08.583 -22 07 19.46 23.1r 14SU373 W84 C~4yUX 2014 12 17.14284 01 21 08.58 -22 07 19.4 23.4r 14SU373 W84 C~3cnr 2015 01 12.05566 01 20 58.965 -21 47 21.89 23.2i 14SU373 W84 C~4yUX 2015 09 04.35272 01 35 48.609 -21 05 21.15 22.4i 14SU373 W84 C~4yUX 2015 09 04.35272 01 35 48.61 -21 05 21.0 23.2i 14SU373 W84 C~3cnr 2015 10 07.23338 01 33 20.830 -21 28 31.21 23.1r 14SU373 W84 C~4yUX 2015 10 07.23338 01 33 20.83 -21 28 31.2 23.1r 14SU373 W84 C~3cnr 2015 10 18.24765 01 32 22.331 -21 33 41.09 23.7r 14SU373 W84 C~4yUX 2015 11 06.13569 01 30 43.393 -21 38 17.07 23.5r 14SU373 W84 C~4yUX 2015 11 06.13569 01 30 43.39 -21 38 17.1 23.4r 14SU373 W84 C~3cnr 2015 11 08.25729 01 30 32.868 -21 38 25.37 21.1r 14SU373 W84 C~4yUX 2015 11 08.25729 01 30 32.86 -21 38 25.8 22.1r 14SU373 W84 C~3cnr 2015 11 08.25866 01 30 32.853 -21 38 26.10 22.5i 14SU373 W84 C~4yUX 2015 11 18.15415 01 29 46.596 -21 38 06.52 22.7z 14SU373 W84 C~4yUX 2016 01 03.10809 01 27 52.781 -21 15 41.90 22.6i 14SU373 W84 C~4yUX 2016 01 03.10809 01 27 52.78 -21 15 41.9 22.7i 14SU373 W84 C~3cnr 2016 01 03.10946 01 27 52.790 -21 15 41.98 23.2r 14SU373 W84 C~4yUX 2016 01 03.10946 01 27 52.79 -21 15 42.0 23.4r 14SU373 W84 C~3cnr 2016 10 05.26710 01 40 39.683 -20 44 45.85 23.1i 14SU373 W84 C~4yUX 2016 10 05.26710 01 40 39.68 -20 44 45.9 22.9i 14SU373 W84 C~3cnr 2016 10 05.26847 01 40 39.677 -20 44 45.85 23.4r 14SU373 W84 C~4yUX 2016 10 05.26847 01 40 39.68 -20 44 45.9 23.5r 14SU373 W84 C~3cnr 2016 10 06.19656 01 40 34.87 -20 45 17.5 14SU373 W84 C~5iq6 2016 10 06.32702 01 40 34.18 -20 45 21.9 23.9V 14SU373 W84 C~5iq6 2016 10 28.28279 01 38 36.999 -20 54 23.03 22.9i 14SU373 W84 C~4yUX 2016 10 28.28279 01 38 37.00 -20 54 23.0 23.1i 14SU373 W84 C~3cnr 2016 10 28.28416 01 38 36.996 -20 54 23.05 23.3r 14SU373 W84 C~4yUX 2016 10 28.28416 01 38 37.00 -20 54 23.0 23.4r 14SU373 W84 C~3cnr 2016 10 28.28554 01 38 36.989 -20 54 23.13 23.9g 14SU373 W84 C~4yUX 2016 10 28.28554 01 38 36.99 -20 54 23.1 23.9g 14SU373 W84 C~3cnr 2017 09 26.27404 01 48 40.322 -19 53 56.23 23.4r 14SU373 W84 C~4yUX 2017 09 26.27540 01 48 40.317 -19 53 56.20 23.3i 14SU373 W84 C~4yUX 2017 09 26.27678 01 48 40.313 -19 53 56.34 24.1g 14SU373 W84 C~4yUX 2018 10 01.29869 01 55 34.242 -19 10 18.57 22.9z 14SU373 W84 C~4yUX 2018 10 21.13658 01 53 50.323 -19 20 56.57 22.3Y 14SU373 W84 C~4yUX 2018 11 16.23743 01 51 32.604 -19 26 06.17 23.1r 14SU373 W84 C~4yUX 2018 11 16.23881 01 51 32.603 -19 26 06.11 23.7i 14SU373 W84 C~4yUX 2018 12 02.09289 01 50 22.712 -19 23 34.39 23.9g 14SU373 W84 C~4yUX
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 0.00
2 0.0000 0.01 0.07 -0.04 -0.04
3 0.2133 -4286.83 0.04 1880.69 -0.02
4 0.2133 -4286.81 0.05 1880.62 -0.10
5 0.2842 -3913.76 0.03 3026.80 0.21
6 0.9284 8409.45 -0.24 41.39 -0.11
7 0.9284 8409.52 -0.17 41.52 0.02
8 1.0185 5942.67 0.03 -317.16 0.07
9 1.0185 5942.67 0.03 -317.17 0.06
10 1.0486 5071.84 -0.02 -245.26 0.08
11 1.1003 3706.24 -0.10 97.08 -0.11
12 1.1003 3706.29 -0.05 97.09 -0.10
13 1.1061 3569.75 0.07 151.97 0.13
14 1.1061 3570.03 ( 0.36) 152.31 ( 0.48)
15 1.1061 3569.53 -0.06 151.74 -0.13
16 1.1332 2994.45 -0.17 444.69 0.13
17 1.2591 2126.91 -0.00 2337.11 0.11
18 1.2591 2126.92 0.01 2337.10 0.11
19 1.2591 2126.99 0.06 2336.96 -0.10
20 1.2591 2127.00 0.07 2336.98 -0.08
21 2.0151 12627.69 -0.06 -636.78 -0.02
22 2.0151 12627.75 0.00 -636.75 0.01
23 2.0151 12627.69 0.05 -636.78 -0.02
24 2.0151 12627.67 0.04 -636.71 0.04
25 2.0177 12552.92 0.00 -635.32 0.09
26 2.0180 12542.25 -0.01 -635.00 0.08
27 2.0782 10823.46 -0.00 -397.20 0.01
28 2.0782 10823.43 -0.03 -397.22 -0.01
29 2.0782 10823.46 0.10 -397.20 -0.02
30 2.0782 10823.39 0.03 -397.22 -0.04
31 2.0782 10823.26 0.01 -397.25 -0.09
32 2.0782 10823.29 0.03 -397.23 -0.07
33 2.9898 20086.02 0.08 -934.21 -0.09
34 2.9898 20085.97 0.14 -934.15 -0.02
35 2.9898 20085.86 0.14 -934.25 -0.12
36 4.0029 26569.39 -0.11 -1284.53 -0.09
37 4.0572 24944.32 0.08 -1171.95 0.03
38 4.1287 23044.60 -0.13 -550.65 -0.00
39 4.1287 23044.61 -0.03 -550.59 0.01
40 4.1721 22223.59 -0.03 38.30 0.20
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.
14SU373 quality flag:3 Type: 5:2EEE 5:2EEE 5:2EEE axisobj 55.917 55.936 55.899 ecceobj 0.403 0.403 0.403 incobj 28.158 28.158 28.158 qmin 32.166 32.096 32.240 qmax 80.220 80.298 80.177 amean 55.462 55.462 55.461 amin 54.679 54.666 54.618 amax 56.451 56.494 56.542 emean 0.383 0.399 0.398 emin 0.343 0.368 0.372 emax 0.422 0.423 0.420 imean 27.243 26.508 26.524 imin 25.679 25.605 25.790 imax 28.795 27.697 27.417 excite_mean 0.597 0.599 0.599 fracstop 1.000 1.000 1.000 cjmean 2.772 2.770 2.771 libcent 0 179.7 181.0 179.9 libamp 0 135.1 139.8 145.4 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 123.4 144.5 154.8 kozaiamp 180.0 180.0 180.0