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: 14QU510 # Created Fri Nov 22 02:09:58 2024 # Orbit generated from Bernstein formalism # Fitting 37 observations of 37 # Arc: 4.26y # First observation: 2014/08/22 # Last observation: 2018/11/26 Preliminary a, adot, b, bdot, g, gdot: 0.000017 0.021969 -0.000011 0.002287 0.023547 0.000000 # Chi-squared of fit: 11.90 DOF: 68 RMS: 0.10 # Min/Max residuals: -0.26 0.36 # Exact a, adot, b, bdot, g, gdot: 1.516307E-05 2.209503E-02 1.198765E-06 2.328172E-03 2.369661E-02 7.669834E-04 # Covariance matrix: 2.2233E-13 -5.7252E-14 -7.7251E-15 -8.6227E-15 8.6408E-14 -3.9510E-13 -5.7252E-14 1.7850E-13 -2.7848E-14 2.8630E-14 1.3503E-13 2.4519E-12 -7.7251E-15 -2.7848E-14 1.4887E-13 -5.9604E-14 -3.4285E-14 -4.2163E-13 -8.6227E-15 2.8630E-14 -5.9604E-14 3.5894E-14 1.6828E-14 5.0841E-13 8.6408E-14 1.3503E-13 -3.4285E-14 1.6828E-14 2.2067E-13 1.8230E-12 -3.9510E-13 2.4519E-12 -4.2163E-13 5.0841E-13 1.8230E-12 4.1988E-11 # lat0 lon0 xBary yBary zBary JD0 -42.603623 5.196063 0.599288 -0.553764 -0.602331 2456891.850128 # Heliocentric elements and errors Epoch: 2456890.5000 = 2014/08/21 Mean Anomaly: 156.08635 +/- 0.282 Argument of Peri: 117.37118 +/- 0.281 Long of Asc Node: 86.35081 +/- 0.001 Inclination: 42.12204 +/- 0.000 Eccentricity: 0.05295930 +/- 0.0001 Semi-Major Axis: 40.81497657 +/- 0.0022 Time of Perihelion: 2415596.1922 +/- 74.5 Perihelion: 38.65344401 +/- 0.0047 Aphelion: 42.97650913 +/- 0.0048 Period (y) 260.7579 +/- 0.02 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 31.80077708 +/- 0.0006 Ecliptic Y 2.29246957 +/- 0.0001 Ecliptic Z -28.56618949 +/- 0.0006 Ecliptic XDOT 0.00001023 +/- 0.0000 Ecliptic YDOT 0.00256040 +/- 0.0000 Ecliptic ZDOT 0.00013813 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 42.80855080 +/- 0.0006 Geocenter to KBO 42.20013050 +/- 0.0008 # Hcoef: 6.85
The following table shows the complete astrometric record for 14QU510. 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 (14QU510) followed by the observatory code and reference code for the source of the astrometry.
2014 08 22.34935 01 37 03.405 -36 28 49.59 22.7r 14QU510 W84 C~4yU1 2014 08 22.34935 01 37 03.40 -36 28 49.6 22.9r 14QU510 W84 C~3cnQ 2014 08 22.35072 01 37 03.409 -36 28 49.83 22.8i 14QU510 W84 C~4yU1 2014 08 22.35072 01 37 03.41 -36 28 49.8 22.9i 14QU510 W84 C~3cnQ 2014 11 14.25303 01 30 10.881 -37 04 09.35 22.9i 14QU510 W84 C~4yU1 2014 11 15.25053 01 30 05.965 -37 03 51.93 23.0r 14QU510 W84 C~4yU1 2014 11 15.25053 01 30 05.97 -37 03 51.9 23.1r 14QU510 W84 C~3cnQ 2014 11 27.22148 01 29 11.935 -36 58 55.99 23.8g 14QU510 W84 C~4yU1 2015 08 24.33339 01 42 04.531 -35 45 46.37 23.0i 14QU510 W84 C~4yU1 2015 11 30.21053 01 34 11.280 -36 14 23.43 22.7i 14QU510 W84 C~4yU1 2015 11 30.21053 01 34 11.28 -36 14 23.4 22.9i 14QU510 W84 C~3cnQ 2016 01 11.08830 01 32 49.018 -35 39 00.41 23.5r 14QU510 W84 C~4yU1 2016 01 11.08830 01 32 49.02 -35 39 00.4 23.7r 14QU510 W84 C~3cnQ 2016 01 11.08968 01 32 49.042 -35 39 00.22 24.1g 14QU510 W84 C~4yU1 2016 10 05.37117 01 44 03.388 -35 31 28.51 23.1r 14QU510 W84 C~4yU1 2016 10 05.37117 01 44 03.39 -35 31 28.5 23.3r 14QU510 W84 C~3cnQ 2016 10 05.37254 01 44 03.371 -35 31 28.59 22.6i 14QU510 W84 C~4yU1 2016 10 05.37254 01 44 03.37 -35 31 28.6 22.9i 14QU510 W84 C~3cnQ 2016 10 29.29155 01 41 49.776 -35 37 53.43 23.2i 14QU510 W84 C~4yU1 2016 10 29.29155 01 41 49.77 -35 37 53.4 23.2i 14QU510 W84 C~3cnQ 2016 10 29.29293 01 41 49.785 -35 37 53.48 23.1r 14QU510 W84 C~4yU1 2016 10 29.29293 01 41 49.78 -35 37 53.5 23.2r 14QU510 W84 C~3cnQ 2016 10 29.29431 01 41 49.751 -35 37 53.63 23.9g 14QU510 W84 C~4yU1 2016 10 29.29431 01 41 49.75 -35 37 53.6 24.1g 14QU510 W84 C~3cnQ 2016 12 19.15408 01 38 12.482 -35 17 06.01 23.1r 14QU510 W84 C~4yU1 2016 12 19.15408 01 38 12.48 -35 17 06.0 23.4r 14QU510 W84 C~3cnQ 2016 12 19.15546 01 38 12.484 -35 17 05.98 22.8i 14QU510 W84 C~4yU1 2016 12 19.15546 01 38 12.48 -35 17 06.0 23.0i 14QU510 W84 C~3cnQ 2016 12 20.15962 01 38 10.231 -35 16 15.87 24.1g 14QU510 W84 C~4yU1 2016 12 20.15962 01 38 10.23 -35 16 15.8 24.4g 14QU510 W84 C~3cnQ 2017 10 28.29608 01 46 56.046 -34 52 23.06 22.9r 14QU510 W84 C~4yU1 2017 10 28.29745 01 46 56.021 -34 52 22.90 23.1i 14QU510 W84 C~4yU1 2017 10 28.29883 01 46 56.024 -34 52 23.01 23.8g 14QU510 W84 C~4yU1 2017 12 25.13915 01 42 56.829 -34 27 57.18 22.4z 14QU510 W84 C~4yU1 2018 02 06.03409 01 43 17.772 -33 42 22.28 22.9i 14QU510 W84 C~4yU1 2018 11 17.03800 01 50 06.192 -34 04 58.27 22.6z 14QU510 W84 C~4yU1 2018 11 26.10685 01 49 23.423 -34 02 00.47 23.0i 14QU510 W84 C~4yU1
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 -0.09 0.00 0.07
2 0.0000 0.06 -0.03 -0.02 0.05
3 0.0000 0.01 -0.00 -0.23 -0.12
4 0.0000 -0.02 -0.03 -0.25 -0.14
5 0.2297 -5363.69 -0.12 549.40 -0.03
6 0.2324 -5407.07 -0.08 592.78 -0.07
7 0.2324 -5407.14 -0.15 592.79 -0.07
8 0.2652 -5835.83 0.26 1161.18 0.09
9 1.0047 4451.25 0.11 421.59 -0.08
10 1.2727 -1389.18 0.07 1773.04 0.06
11 1.2727 -1389.20 0.05 1773.01 0.03
12 1.3874 -1234.04 0.09 4114.71 0.08
13 1.3874 -1234.06 0.06 4114.72 0.09
14 1.3874 -1233.71 0.36 4114.74 0.04
15 2.1219 6136.13 0.10 428.35 -0.04
16 2.1219 6136.16 0.12 428.35 -0.04
17 2.1219 6135.89 -0.04 428.38 -0.02
18 2.1219 6135.91 -0.03 428.39 -0.02
19 2.1874 4534.14 -0.11 920.89 0.16
20 2.1874 4534.19 -0.06 920.82 0.09
21 2.1874 4534.20 0.03 920.74 -0.04
22 2.1874 4534.26 0.09 920.72 -0.05
23 2.1874 4533.83 -0.25 920.84 0.02
24 2.1874 4533.83 -0.26 920.80 -0.01
25 2.3266 2856.21 0.02 3327.70 0.06
26 2.3266 2856.23 0.04 3327.68 0.04
27 2.3266 2856.21 0.02 3327.70 -0.02
28 2.3266 2856.27 0.07 3327.69 -0.02
29 2.3294 2857.14 -0.16 3384.98 0.03
30 2.3294 2857.12 -0.19 3384.91 -0.04
31 3.1840 9158.45 0.04 1362.80 -0.09
32 3.1840 9158.27 -0.06 1363.09 0.17
33 3.1840 9158.24 0.00 1362.98 0.01
34 3.3423 7365.22 -0.00 4131.06 -0.03
35 3.4598 8977.48 0.01 6362.53 0.04
36 4.2373 12653.09 0.07 2582.08 -0.17
37 4.2622 12290.51 0.02 3011.15 -0.03
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.
14QU510 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 41.121 41.128 41.114 ecceobj 0.046 0.046 0.046 incobj 42.140 42.140 42.140 qmin 38.310 38.305 38.316 qmax 43.770 43.764 43.731 amean 40.946 40.953 40.939 amin 40.647 40.641 40.646 amax 41.255 41.264 41.241 emean 0.050 0.050 0.050 emin 0.040 0.041 0.041 emax 0.061 0.061 0.061 imean 40.605 40.605 40.605 imin 40.373 40.381 40.374 imax 40.845 40.846 40.851 excite_mean 0.653 0.653 0.653 fracstop 1.000 1.000 1.000 cjmean 2.505 2.505 2.505 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 200.0 200.3 199.6 kozaiamp 179.9 180.0 180.0