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: 14UO250 # Created Fri Nov 22 02:10:08 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 33 observations of 33 # Arc: 6.05y # First observation: 2014/10/02 # Last observation: 2020/10/20 # Chi-squared of fit: 12.41 DOF: 60 RMS: 0.11 # Min/Max residuals: -0.28 0.24 # Exact a, adot, b, bdot, g, gdot: 1.416453E-05 2.300117E-02 -6.502892E-06 -1.201851E-02 2.561277E-02 -2.068471E-03 # Covariance matrix: 1.8091E-13 -9.0531E-14 -2.4888E-14 3.0670E-14 7.2695E-14 -4.7215E-13 -9.0531E-14 9.0436E-14 3.2682E-14 -4.0613E-14 2.1484E-14 6.2344E-13 -2.4888E-14 3.2682E-14 1.3115E-13 -5.5194E-14 8.3825E-15 2.8390E-13 3.0670E-14 -4.0613E-14 -5.5194E-14 4.1626E-14 -1.1361E-14 -3.5274E-13 7.2695E-14 2.1484E-14 8.3825E-15 -1.1361E-14 3.3123E-13 1.6952E-13 -4.7215E-13 6.2344E-13 2.8390E-13 -3.5274E-13 1.6952E-13 5.4152E-12 # lat0 lon0 xBary yBary zBary JD0 -6.241505 27.892692 0.328974 -0.102866 -0.942113 2456932.822448 # Heliocentric elements and errors Epoch: 2456932.5000 = 2014/10/02 Mean Anomaly: 302.10047 +/- 0.034 Argument of Peri: 261.28902 +/- 0.045 Long of Asc Node: 195.97891 +/- 0.000 Inclination: 28.28608 +/- 0.000 Eccentricity: 0.10096335 +/- 0.0001 Semi-Major Axis: 41.90204992 +/- 0.0040 Time of Perihelion: 2472866.4641 +/- 15.1 Perihelion: 37.67147872 +/- 0.0051 Aphelion: 46.13262113 +/- 0.0057 Period (y) 271.2446 +/- 0.04 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 35.29144905 +/- 0.0008 Ecliptic Y 18.31110991 +/- 0.0004 Ecliptic Z -4.24503241 +/- 0.0001 Ecliptic XDOT -0.00147252 +/- 0.0000 Ecliptic YDOT 0.00200024 +/- 0.0000 Ecliptic ZDOT -0.00125294 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 39.98509631 +/- 0.0007 Geocenter to KBO 39.04310453 +/- 0.0009 # Hcoef: 7.36
The following table shows the complete astrometric record for 14UO250. 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 (14UO250) followed by the observatory code and reference code for the source of the astrometry.
2014 10 02.32167 01 52 33.670 +04 53 22.49 24.3g 14UO250 W84 C~4yUz 2014 10 02.32304 01 52 33.664 +04 53 22.72 23.0r 14UO250 W84 C~4yUz 2014 10 23.26265 01 50 56.947 +04 41 15.08 23.9r 14UO250 W84 C~4yUz 2014 10 23.26542 01 50 56.929 +04 41 14.99 22.4i 14UO250 W84 C~4yUz 2014 10 23.26542 01 50 56.93 +04 41 15.0 22.6i 14UO250 W84 C~3coQ 2014 10 29.23599 01 50 28.629 +04 37 57.81 22.9r 14UO250 W84 C~4yUz 2014 10 29.23599 01 50 28.62 +04 37 57.8 23.3r 14UO250 W84 C~3coQ 2015 10 18.22426 01 57 18.157 +04 33 19.17 23.0r 14UO250 W84 C~4yUz 2015 11 06.17272 01 55 48.346 +04 23 03.16 23.4i 14UO250 W84 C~4yUz 2015 11 06.17409 01 55 48.345 +04 23 03.22 23.4r 14UO250 W84 C~4yUz 2015 11 06.17409 01 55 48.34 +04 23 03.2 23.4r 14UO250 W84 C~3coQ 2015 11 06.17545 01 55 48.346 +04 23 03.00 24.2g 14UO250 W84 C~4yUz 2015 11 18.17421 01 54 54.74 +04 17 28.2 23.3r 14UO250 W84 C~3coQ 2016 09 09.29496 02 05 49.306 +04 44 00.76 23.4r 14UO250 W84 C~4yUz 2016 09 09.29496 02 05 49.31 +04 44 00.8 23.6r 14UO250 W84 C~3coQ 2016 09 09.29635 02 05 49.316 +04 44 00.64 23.8i 14UO250 W84 C~4yUz 2016 09 09.29635 02 05 49.31 +04 44 00.6 23.5i 14UO250 W84 C~3coQ 2016 09 09.29774 02 05 49.315 +04 44 00.95 24.2g 14UO250 W84 C~4yUz 2016 10 23.20859 02 02 48.106 +04 18 53.91 22.3r 14UO250 W84 C~4yUz 2016 10 23.20859 02 02 48.11 +04 18 54.0 22.7r 14UO250 W84 C~3coQ 2016 10 28.23573 02 02 24.011 +04 16 08.68 23.0i 14UO250 W84 C~4yUz 2016 10 28.23711 02 02 24.001 +04 16 08.60 23.8g 14UO250 W84 C~4yUz 2016 10 28.23711 02 02 24.00 +04 16 08.6 23.8g 14UO250 W84 C~3coQ 2017 09 18.30162 02 11 17.888 +04 27 48.65 22.9r 14UO250 W84 C~4yUz 2017 09 18.30299 02 11 17.882 +04 27 48.89 22.5i 14UO250 W84 C~4yUz 2017 09 18.30931 02 11 17.856 +04 27 48.71 23.9g 14UO250 W84 C~4yUz 2017 10 22.22735 02 08 52.451 +04 08 09.83 23.5r 14UO250 W84 C~4yUz 2017 10 29.24005 02 08 18.698 +04 04 19.57 23.3z 14UO250 W84 C~4yUz 2017 11 16.18225 02 06 54.574 +03 55 36.45 23.0r 14UO250 W84 C~4yUz 2017 11 16.18363 02 06 54.575 +03 55 36.64 23.2g 14UO250 W84 C~4yUz 2018 11 29.17618 02 11 58.999 +03 39 12.27 24.2g 14UO250 W84 C~4yUz 2020 10 20.299780 02 27 04.985 +03 33 41.62 23.1G 14UO250 G37 C~4Kxo 2020 10 20.352440 02 27 04.720 +03 33 39.84 14UO250 G37 C~4Kxo
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 0.07 0.00 -0.17
2 0.0000 0.00 0.07 0.00 0.10
3 0.0573 0.00 -0.02 0.00 0.03
4 0.0573 0.00 -0.09 0.00 0.03
5 0.0573 0.00 -0.08 0.00 0.04
6 0.0737 0.00 0.09 0.00 0.01
7 0.0737 0.00 0.22 0.00 0.02
8 1.0429 0.00 -0.15 0.00 -0.28
9 1.0947 0.00 -0.09 0.00 0.01
10 1.0947 0.00 -0.09 0.00 0.09
11 1.0947 0.00 -0.01 0.00 0.11
12 1.0947 0.00 0.10 0.00 -0.07
13 1.1276 0.00 -0.05 0.00 -0.06
14 1.9383 0.00 -0.06 0.00 -0.00
15 1.9383 0.00 -0.12 0.00 -0.04
16 1.9383 0.00 0.00 0.00 -0.16
17 1.9383 0.00 0.09 0.00 -0.12
18 1.9383 0.00 0.14 0.00 0.24
19 2.0586 0.00 -0.14 0.00 0.10
20 2.0586 0.00 -0.20 0.00 0.01
21 2.0723 0.00 0.06 0.00 0.04
22 2.0723 0.00 -0.00 0.00 0.01
23 2.0723 0.00 0.01 0.00 0.01
24 2.9623 0.00 0.08 0.00 -0.10
25 2.9623 0.00 0.07 0.00 0.19
26 2.9623 0.00 0.02 0.00 0.22
27 3.0552 0.00 0.01 0.00 -0.03
28 3.0744 0.00 -0.09 0.00 -0.00
29 3.1235 0.00 0.11 0.00 -0.07
30 3.1235 0.00 0.22 0.00 0.15
31 4.1584 0.00 0.10 0.00 -0.18
32 6.0506 0.00 0.03 0.00 -0.02
33 6.0507 0.00 -0.12 0.00 -0.02
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.
14UO250 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 42.189 42.189 42.189 ecceobj 0.101 0.101 0.101 incobj 28.170 28.170 28.170 qmin 37.268 37.297 37.256 qmax 46.839 46.895 46.816 amean 41.934 41.936 41.932 amin 41.607 41.605 41.605 amax 42.281 42.287 42.278 emean 0.093 0.093 0.093 emin 0.079 0.080 0.080 emax 0.108 0.109 0.108 imean 28.510 28.510 28.509 imin 28.164 28.164 28.164 imax 28.869 28.865 28.878 excite_mean 0.486 0.486 0.486 fracstop 1.000 1.000 1.000 cjmean 2.784 2.784 2.784 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 178.7 178.8 179.0 kozaiamp 179.9 179.9 180.0