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: 14SP373 # Created Fri Nov 22 02:10:01 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 75 observations of 75 # Arc: 10.83y # First observation: 2013/11/03 # Last observation: 2024/09/01 # Chi-squared of fit: 27.62 DOF: 144 RMS: 0.11 # Min/Max residuals: -0.30 0.58 # Exact a, adot, b, bdot, g, gdot: 1.609258E-05 2.984790E-02 -5.189611E-06 -9.908906E-03 2.941052E-02 -1.025288E-02 # Covariance matrix: 1.3200E-13 -4.6406E-14 -2.2384E-14 1.2681E-14 -2.7528E-14 -9.7316E-14 -4.6406E-14 2.2005E-14 1.1916E-14 -6.7090E-15 1.2353E-14 5.1712E-14 -2.2384E-14 1.1916E-14 6.5127E-14 -1.1363E-14 6.2375E-15 2.9900E-14 1.2681E-14 -6.7090E-15 -1.1363E-14 3.5521E-15 -4.3378E-15 -1.6798E-14 -2.7528E-14 1.2353E-14 6.2375E-15 -4.3378E-15 5.2231E-14 2.8949E-14 -9.7316E-14 5.1712E-14 2.9900E-14 -1.6798E-14 2.8949E-14 1.2967E-13 # lat0 lon0 xBary yBary zBary JD0 -17.298107 19.986244 -0.346355 -0.275973 -0.886555 2456599.535948 # Heliocentric elements and errors Epoch: 2456600.5000 = 2013/11/04 Mean Anomaly: 309.00193 +/- 0.003 Argument of Peri: 311.56575 +/- 0.004 Long of Asc Node: 158.89336 +/- 0.000 Inclination: 24.47431 +/- 0.000 Eccentricity: 0.32573380 +/- 0.0000 Semi-Major Axis: 39.65719304 +/- 0.0014 Time of Perihelion: 2469522.5868 +/- 4.3 Perihelion: 26.73950487 +/- 0.0011 Aphelion: 52.57488121 +/- 0.0020 Period (y) 249.7418 +/- 0.01 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 31.26179610 +/- 0.0002 Ecliptic Y 11.74161988 +/- 0.0001 Ecliptic Z -10.11030468 +/- 0.0001 Ecliptic XDOT -0.00207003 +/- 0.0000 Ecliptic YDOT 0.00220436 +/- 0.0000 Ecliptic ZDOT -0.00059677 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 34.89121126 +/- 0.0002 Geocenter to KBO 34.00165878 +/- 0.0003 # Hcoef: 6.84
The following table shows the complete astrometric record for 14SP373. 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 (14SP373) followed by the observatory code and reference code for the source of the astrometry.
2013 11 03.03517 01 39 50.93 -08 13 17.0 22.6r 14SP373 W84 C~3cnr 2013 11 03.09961 01 39 50.59 -08 13 18.6 14SP373 W84 C~3cnr 2013 11 03.19036 01 39 50.11 -08 13 20.8 14SP373 W84 C~3cnr 2014 09 25.25771 01 50 36.401 -07 41 34.97 22.2r 14SP373 W84 C~4yUX 2014 09 25.25771 01 50 36.40 -07 41 35.0 22.3r 14SP373 W84 C~3cnr 2014 09 25.25909 01 50 36.392 -07 41 34.90 22.3i 14SP373 W84 C~4yUX 2014 09 25.25909 01 50 36.39 -07 41 34.9 22.3i 14SP373 W84 C~3cnr 2014 11 16.15148 01 46 05.660 -08 10 20.70 23.0g 14SP373 W84 C~4yUX 2014 12 24.12239 01 43 55.292 -08 10 07.68 22.9g 14SP373 W84 C~4yUX 2014 12 24.12239 01 43 55.29 -08 10 07.7 23.1g 14SP373 W84 C~3cnr 2015 01 14.06682 01 43 43.903 -08 01 36.00 22.3r 14SP373 W84 C~4yUX 2015 01 14.06682 01 43 43.90 -08 01 36.0 22.3r 14SP373 W84 C~3cnr 2015 08 19.37020 02 00 04.143 -07 04 15.94 22.3r 14SP373 W84 C~4yUX 2015 09 04.33612 01 59 28.033 -07 16 25.81 22.1z 14SP373 W84 C~4yUX 2015 09 04.33612 01 59 28.03 -07 16 25.8 22.2z 14SP373 W84 C~3cnr 2015 10 17.18653 01 56 15.175 -07 48 24.83 22.5g 14SP373 W84 C~4yUX 2015 10 17.18653 01 56 15.17 -07 48 24.8 22.5g 14SP373 W84 C~3cnr 2015 11 07.25243 01 54 19.916 -07 59 22.02 22.5r 14SP373 W84 C~4yUX 2015 11 07.25243 01 54 19.92 -07 59 22.0 22.5r 14SP373 W84 C~3cnr 2015 11 07.25381 01 54 19.915 -07 59 22.03 22.4i 14SP373 W84 C~4yUX 2015 11 07.25381 01 54 19.91 -07 59 22.0 22.5i 14SP373 W84 C~3cnr 2015 11 07.25518 01 54 19.910 -07 59 22.12 23.0g 14SP373 W84 C~4yUX 2015 11 07.25518 01 54 19.91 -07 59 22.1 23.0g 14SP373 W84 C~3cnr 2015 11 18.13997 01 53 24.101 -08 02 54.68 21.6z 14SP373 W84 C~4yUX 2015 11 18.13997 01 53 24.10 -08 02 54.7 21.5z 14SP373 W84 C~3cnr 2016 09 14.28227 02 06 27.931 -07 15 38.72 22.0z 14SP373 W84 C~4yUX 2016 09 14.28227 02 06 27.93 -07 15 38.7 22.0z 14SP373 W84 C~3cnr 2016 10 22.29379 02 03 21.281 -07 43 06.94 22.2i 14SP373 W84 C~4yUX 2016 10 22.29379 02 03 21.28 -07 43 06.9 22.3i 14SP373 W84 C~3cnr 2016 10 25.20250 02 03 05.067 -07 44 46.55 22.9g 14SP373 W84 C~4yUX 2016 10 25.20250 02 03 05.07 -07 44 46.5 22.9g 14SP373 W84 C~3cnr 2017 10 22.21469 02 11 10.341 -07 33 24.55 22.1r 14SP373 W84 C~4yUX 2017 10 22.21606 02 11 10.331 -07 33 24.64 21.9i 14SP373 W84 C~4yUX 2017 10 22.21743 02 11 10.323 -07 33 24.63 22.9g 14SP373 W84 C~4yUX 2017 11 10.16930 02 09 24.141 -07 42 46.22 22.1r 14SP373 W84 C~4yUX 2017 11 16.13029 02 08 52.145 -07 44 46.22 22.5g 14SP373 W84 C~4yUX 2017 11 27.19569 02 07 57.034 -07 47 08.04 22.0i 14SP373 W84 C~4yUX 2017 12 07.16926 02 07 14.047 -07 47 42.11 22.4Y 14SP373 W84 C~4yUX 2017 12 14.06214 02 06 48.983 -07 47 13.22 22.3r 14SP373 W84 C~4yUX 2017 12 14.06352 02 06 48.984 -07 47 13.19 22.8g 14SP373 W84 C~4yUX 2017 12 25.11805 02 06 18.128 -07 44 58.20 21.8z 14SP373 W84 C~4yUX 2018 10 20.23330 02 19 19.513 -07 21 45.07 21.4z 14SP373 W84 C~4yUX 2018 11 16.11363 02 16 48.003 -07 34 43.52 21.9i 14SP373 W84 C~4yUX 2018 11 30.10951 02 15 37.036 -07 37 36.82 22.1r 14SP373 W84 C~4yUX 2018 11 30.11088 02 15 37.028 -07 37 36.79 22.5g 14SP373 W84 C~4yUX 2020 10 13.19787 02 36 18.38 -06 54 17.6 21.4G 14SP373 X01 C~4UE4 2020 10 13.25301 02 36 18.06 -06 54 20.5 21.5G 14SP373 X01 C~4UE4 2020 12 07.29698 02 31 14.876 -07 16 05.18 22.1w 14SP373 F51 C~4NsP 2020 12 07.30736 02 31 14.855 -07 16 05.00 22.1w 14SP373 F51 C~4NsP 2020 12 07.31773 02 31 14.805 -07 16 05.03 22.1w 14SP373 F51 C~4NsP 2020 12 07.32811 02 31 14.745 -07 16 04.95 22.2w 14SP373 F51 C~4NsP 2021 09 04.587164 02 47 14.333 -06 10 06.74 21.8w 14SP373 F51 C~4yUX 2021 09 04.599593 02 47 14.307 -06 10 07.42 22.0w 14SP373 F51 C~4yUX 2021 09 04.611942 02 47 14.275 -06 10 08.03 22.0w 14SP373 F51 C~4yUX 2021 09 04.624315 02 47 14.265 -06 10 08.77 22.0w 14SP373 F51 C~4yUX 2021 09 30.505677 02 45 48.655 -06 31 34.09 22.0w 14SP373 F52 C~55S6 2021 09 30.516615 02 45 48.610 -06 31 34.89 21.9w 14SP373 F52 C~55S6 2021 09 30.527528 02 45 48.558 -06 31 35.56 21.9w 14SP373 F52 C~55S6 2021 09 30.538434 02 45 48.509 -06 31 35.84 21.9w 14SP373 F52 C~55S6 2023 10 17.516264 03 01 51.185 -06 16 10.95 21.7w 14SP373 F51 C~7B5x 2023 10 17.528001 03 01 51.123 -06 16 11.60 21.9w 14SP373 F51 C~7B5x 2023 10 17.539061 03 01 51.054 -06 16 12.14 21.8w 14SP373 F51 C~7B5x 2023 10 17.550106 03 01 50.998 -06 16 12.55 21.8w 14SP373 F51 C~7B5x 2023 12 31.231752 02 55 15.804 -06 33 38.06 21.9w 14SP373 F51 C~7dJ1 2023 12 31.253286 02 55 15.724 -06 33 37.73 21.6w 14SP373 F51 C~7dJ1 2023 12 31.263836 02 55 15.710 -06 33 37.50 22.0w 14SP373 F51 C~7dJ1 2023 12 31.266956 02 55 15.703 -06 33 37.53 22.0w 14SP373 F51 C~7dJ1 2023 12 31.278946 02 55 15.641 -06 33 37.35 21.9w 14SP373 F51 C~7dJ1 2023 12 31.290972 02 55 15.616 -06 33 37.22 22.2w 14SP373 F51 C~7dJ1 2024 01 04.242045 02 55 04.261 -06 32 09.77 21.9w 14SP373 F52 C~7dJ1 2024 01 04.265501 02 55 04.200 -06 32 09.38 21.9w 14SP373 F52 C~7dJ1 2024 01 04.277204 02 55 04.169 -06 32 09.07 21.8w 14SP373 F52 C~7dJ1 2024 09 01.588264 03 13 21.764 -05 23 59.22 22.0w 14SP373 F52 C~8Df9 2024 09 01.598942 03 13 21.774 -05 23 59.68 21.7w 14SP373 F52 C~8Df9 2024 09 01.620229 03 13 21.740 -05 24 00.53 21.9w 14SP373 F52 C~8Df9
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 -0.03
2 0.0002 0.00 0.01 0.00 0.00
3 0.0004 0.00 0.02 0.00 0.08
4 0.8931 0.00 0.04 0.00 -0.07
5 0.8931 0.00 0.05 0.00 -0.04
6 0.8932 0.00 -0.01 0.00 0.09
7 0.8932 0.00 0.02 0.00 0.09
8 1.0352 0.00 0.04 0.00 -0.06
9 1.1392 0.00 0.03 0.00 -0.01
10 1.1392 0.00 0.06 0.00 0.01
11 1.1965 0.00 0.01 0.00 -0.06
12 1.1965 0.00 0.05 0.00 -0.06
13 1.7915 0.00 0.10 0.00 0.02
14 1.8352 0.00 -0.06 0.00 0.01
15 1.8352 0.00 -0.11 0.00 0.02
16 1.9525 0.00 -0.01 0.00 -0.01
17 1.9525 0.00 0.06 0.00 -0.04
18 2.0102 0.00 0.05 0.00 0.03
19 2.0102 0.00 -0.01 0.00 0.01
20 2.0102 0.00 0.01 0.00 0.07
21 2.0102 0.00 0.08 0.00 0.04
22 2.0102 0.00 0.12 0.00 -0.00
23 2.0102 0.00 0.12 0.00 -0.02
24 2.0400 0.00 -0.00 0.00 -0.08
25 2.0400 0.00 0.01 0.00 -0.06
26 2.8645 0.00 -0.02 0.00 -0.03
27 2.8645 0.00 -0.00 0.00 -0.05
28 2.9685 0.00 -0.12 0.00 -0.02
29 2.9685 0.00 -0.10 0.00 -0.06
30 2.9765 0.00 0.01 0.00 -0.02
31 2.9765 0.00 -0.03 0.00 -0.07
32 3.9676 0.00 -0.06 0.00 -0.00
33 3.9676 0.00 -0.10 0.00 -0.05
34 3.9676 0.00 -0.10 0.00 0.01
35 4.0195 0.00 -0.06 0.00 -0.08
36 4.0359 0.00 -0.15 0.00 -0.06
37 4.0661 0.00 -0.05 0.00 0.02
38 4.0935 0.00 -0.07 0.00 0.06
39 4.1123 0.00 -0.07 0.00 -0.00
40 4.1123 0.00 0.01 0.00 0.02
41 4.1426 0.00 -0.03 0.00 0.02
42 4.9615 0.00 -0.08 0.00 0.14
43 5.0351 0.00 -0.03 0.00 0.03
44 5.0734 0.00 -0.05 0.00 -0.04
45 5.0734 0.00 -0.07 0.00 -0.00
46 6.9436 0.00 0.58 0.00 0.42
47 6.9438 0.00 0.29 0.00 -0.11
48 7.0945 0.00 -0.23 0.00 -0.01
49 7.0945 0.00 0.18 0.00 0.18
50 7.0945 0.00 0.14 0.00 0.15
51 7.0946 0.00 -0.04 0.00 0.23
52 7.8372 0.00 -0.05 0.00 0.06
53 7.8373 0.00 -0.04 0.00 -0.01
54 7.8373 0.00 -0.13 0.00 -0.01
55 7.8373 0.00 0.11 0.00 -0.14
56 7.9082 0.00 -0.02 0.00 0.23
57 7.9082 0.00 0.05 0.00 -0.04
58 7.9083 0.00 0.02 0.00 -0.19
59 7.9083 0.00 0.03 0.00 0.06
60 9.9534 0.00 0.01 0.00 0.12
61 9.9534 0.00 0.05 0.00 -0.02
62 9.9535 0.00 -0.07 0.00 -0.09
63 9.9535 0.00 0.00 0.00 -0.02
64 10.1580 0.00 0.02 0.00 0.05
65 10.1580 0.00 -0.15 0.00 -0.05
66 10.1581 0.00 0.15 0.00 -0.03
67 10.1581 0.00 0.19 0.00 -0.13
68 10.1581 0.00 -0.16 0.00 -0.19
69 10.1581 0.00 0.04 0.00 -0.30
70 10.1689 0.00 -0.11 0.00 0.11
71 10.1690 0.00 -0.05 0.00 -0.05
72 10.1690 0.00 -0.03 0.00 -0.02
73 10.8297 0.00 -0.24 0.00 -0.10
74 10.8297 0.00 0.08 0.00 -0.03
75 10.8298 0.00 -0.08 0.00 0.16
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.
14SP373 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.810 39.810 39.810 ecceobj 0.324 0.324 0.324 incobj 24.410 24.410 24.410 qmin 25.907 26.057 25.913 qmax 53.560 53.386 53.461 amean 39.454 39.455 39.454 amin 39.005 39.005 39.009 amax 40.018 40.009 40.006 emean 0.295 0.269 0.295 emin 0.258 0.159 0.257 emax 0.340 0.337 0.340 imean 24.583 25.480 24.584 imin 22.947 22.872 22.933 imax 25.999 28.340 25.989 excite_mean 0.511 0.509 0.511 fracstop 1.000 1.000 1.000 cjmean 2.752 2.752 2.752 libcent 0 179.5 180.0 179.7 libamp 0 90.2 94.4 91.3 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 212.5 149.9 210.8 kozaiamp 180.0 180.0 180.0