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: 14KC102 # Created Fri Nov 22 02:09:54 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 76 observations of 76 # Arc: 7.04y # First observation: 2010/05/11 # Last observation: 2017/05/26 # Chi-squared of fit: 28.56 DOF: 146 RMS: 0.11 # Min/Max residuals: -0.33 0.40 # Exact a, adot, b, bdot, g, gdot: 1.895641E-05 3.827663E-02 5.729051E-08 1.581446E-03 3.222011E-02 -7.287629E-03 # Covariance matrix: 7.8997E-13 -3.4213E-13 1.8758E-14 -1.1202E-14 -1.3801E-13 -8.9357E-13 -3.4213E-13 1.8313E-13 -1.1710E-14 7.1513E-15 9.9128E-14 5.5748E-13 1.8758E-14 -1.1710E-14 3.5410E-13 -7.5993E-14 -7.0765E-15 -3.9301E-14 -1.1202E-14 7.1513E-15 -7.5993E-14 1.7320E-14 4.9344E-15 2.4036E-14 -1.3801E-13 9.9128E-14 -7.0765E-15 4.9344E-15 1.1017E-13 3.3557E-13 -8.9357E-13 5.5748E-13 -3.9301E-14 2.4036E-14 3.3557E-13 1.8709E-12 # lat0 lon0 xBary yBary zBary JD0 12.749161 -117.737575 0.209404 0.218207 -0.964666 2455328.012256 # Heliocentric elements and errors Epoch: 2455328.5000 = 2010/05/12 Mean Anomaly: 325.34047 +/- 0.004 Argument of Peri: 137.16301 +/- 0.006 Long of Asc Node: 162.95781 +/- 0.001 Inclination: 12.58509 +/- 0.000 Eccentricity: 0.26816125 +/- 0.0000 Semi-Major Axis: 39.38598253 +/- 0.0019 Time of Perihelion: 2464020.7275 +/- 6.0 Perihelion: 28.82418827 +/- 0.0021 Aphelion: 49.94777678 +/- 0.0029 Period (y) 247.1842 +/- 0.02 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -14.73004446 +/- 0.0001 Ecliptic Y -27.57317320 +/- 0.0003 Ecliptic Z 6.84928413 +/- 0.0001 Ecliptic XDOT 0.00317539 +/- 0.0000 Ecliptic YDOT -0.00094698 +/- 0.0000 Ecliptic ZDOT -0.00000563 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 32.00272134 +/- 0.0003 Geocenter to KBO 31.03665877 +/- 0.0003 # Hcoef: 7.11
The following table shows the complete astrometric record for 14KC102. 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 (14KC102) followed by the observatory code and reference code for the source of the astrometry.
2010 05 11.51149 16 10 49.956 -08 06 02.90 22.4G 14KC102 F51 C~2kQD 2011 05 14.52389 16 19 24.121 -08 24 00.67 22.2G 14KC102 F51 C~2kQD 2012 05 10.51157 16 28 41.682 -08 43 39.76 22.2G 14KC102 F51 C~2kQD 2012 05 21.48770 16 27 36.716 -08 39 58.80 22.4G 14KC102 F51 C~2kQD 2013 06 09.37255 16 34 49.134 -08 53 43.27 22.1G 14KC102 F51 C~2kQD 2013 06 09.38648 16 34 49.044 -08 53 43.10 22.0G 14KC102 F51 C~2kQD 2013 06 09.40039 16 34 48.955 -08 53 43.10 22.4G 14KC102 F51 C~2kQD 2013 06 18.31707 16 33 55.502 -08 52 37.18 21.8G 14KC102 F51 C~2kQD 2013 07 02.32915 16 32 38.415 -08 52 13.12 22.0G 14KC102 F51 C~2kQD 2014 04 04.57916 16 49 35.939 -09 33 45.89 21.4G 14KC102 F51 C~2kQD 2014 05 07.52573 16 47 23.321 -09 20 06.36 22.1G 14KC102 F51 C~2kQD 2014 05 07.53840 16 47 23.236 -09 20 06.02 22.4G 14KC102 F51 C~2kQD 2014 05 23.42201 16 45 51.229 -09 14 59.95 21.4G 14KC102 F51 C~2kQD 2014 05 23.43486 16 45 51.144 -09 14 59.61 21.8G 14KC102 F51 C~2kQD 2014 05 23.44771 16 45 51.066 -09 14 59.37 21.5G 14KC102 F51 C~2kQD 2014 05 23.46063 16 45 50.986 -09 14 59.20 21.4G 14KC102 F51 C~2kQD 2014 05 28.38723 16 45 20.658 -09 13 42.83 21.9w 14KC102 F51 C~1vXY 2014 05 28.39995 16 45 20.576 -09 13 42.60 22.0w 14KC102 F51 C~1vXY 2014 05 28.41265 16 45 20.498 -09 13 42.36 22.1w 14KC102 F51 C~1vXY 2014 05 28.42535 16 45 20.412 -09 13 42.35 21.8w 14KC102 F51 C~1vXY 2014 06 08.42253 16 44 11.838 -09 11 28.94 22.0G 14KC102 F51 C~2kQD 2014 06 24.38365 16 42 35.682 -09 09 54.53 21.8w 14KC102 F51 C~1vXY 2014 06 24.39647 16 42 35.607 -09 09 54.57 21.9w 14KC102 F51 C~1vXY 2014 06 24.40929 16 42 35.534 -09 09 54.40 21.8w 14KC102 F51 C~1vXY 2014 06 24.42208 16 42 35.460 -09 09 54.40 21.8w 14KC102 F51 C~1vXY 2014 06 30.37944 16 42 02.208 -09 09 51.49 22.1w 14KC102 F51 C~1vXY 2014 06 30.39081 16 42 02.142 -09 09 51.62 21.9w 14KC102 F51 C~1vXY 2014 06 30.40219 16 42 02.080 -09 09 51.48 21.9w 14KC102 F51 C~1vXY 2014 06 30.41357 16 42 02.013 -09 09 51.54 22.2w 14KC102 F51 C~1vXY 2014 07 28.35570 16 40 01.289 -09 13 33.27 22.0G 14KC102 F51 C~2kQD 2014 08 14.26425 16 39 26.441 -09 18 41.60 22.3w 14KC102 F51 C~1vXY 2014 08 14.27653 16 39 26.443 -09 18 41.93 22.1w 14KC102 F51 C~1vXY 2014 08 14.28883 16 39 26.420 -09 18 42.10 22.3w 14KC102 F51 C~1vXY 2014 08 14.30120 16 39 26.419 -09 18 42.38 22.1w 14KC102 F51 C~1vXY 2014 08 15.26514 16 39 25.453 -09 19 03.27 22.0w 14KC102 F51 C~1vXY 2014 08 15.27748 16 39 25.430 -09 19 03.82 21.9w 14KC102 F51 C~1vXY 2014 08 15.30229 16 39 25.417 -09 19 04.05 22.1w 14KC102 F51 C~1vXY 2015 02 27.60235 16 58 45.504 -10 04 36.25 22.1w 14KC102 F51 C~1vXY 2015 02 27.61363 16 58 45.532 -10 04 35.76 22.2w 14KC102 F51 C~1vXY 2015 02 27.62495 16 58 45.570 -10 04 35.72 22.2w 14KC102 F51 C~1vXY 2015 02 27.63626 16 58 45.601 -10 04 35.72 22.1w 14KC102 F51 C~1vXY 2015 03 30.58953 16 59 03.116 -09 52 15.79 22.0G 14KC102 F51 C~2kQD 2015 03 30.60215 16 59 03.098 -09 52 15.51 22.0G 14KC102 F51 C~2kQD 2015 03 30.61477 16 59 03.059 -09 52 15.25 22.1G 14KC102 F51 C~2kQD 2015 03 30.62742 16 59 03.059 -09 52 14.77 22.1G 14KC102 F51 C~2kQD 2015 03 31.59279 16 59 01.581 -09 51 49.81 22.1G 14KC102 F51 C~2kQD 2015 03 31.60567 16 59 01.570 -09 51 49.56 22.0G 14KC102 F51 C~2kQD 2015 03 31.61859 16 59 01.534 -09 51 49.25 21.4G 14KC102 F51 C~2kQD 2015 03 31.63156 16 59 01.521 -09 51 48.80 22.1G 14KC102 F51 C~2kQD 2015 04 23.55868 16 57 54.686 -09 42 05.54 22.1w 14KC102 F51 C~1vXY 2015 04 23.57142 16 57 54.624 -09 42 05.21 22.0w 14KC102 F51 C~1vXY 2015 04 23.58409 16 57 54.585 -09 42 04.90 22.1w 14KC102 F51 C~1vXY 2015 04 23.59673 16 57 54.523 -09 42 04.47 22.3w 14KC102 F51 C~1vXY 2015 04 24.59172 16 57 50.361 -09 41 40.46 22.0w 14KC102 F51 C~1vXY 2015 04 24.60482 16 57 50.302 -09 41 40.06 22.0w 14KC102 F51 C~1vXY 2015 04 24.61789 16 57 50.253 -09 41 39.71 22.1w 14KC102 F51 C~1vXY 2015 05 22.48987 16 55 23.304 -09 32 03.99 22.0G 14KC102 F51 C~2kQD 2015 05 22.50247 16 55 23.219 -09 32 03.89 21.8G 14KC102 F51 C~2kQD 2015 05 22.51500 16 55 23.142 -09 32 03.71 21.7G 14KC102 F51 C~2kQD 2015 05 22.52755 16 55 23.067 -09 32 03.38 22.0G 14KC102 F51 C~2kQD 2015 06 10.37525 16 53 25.710 -09 28 08.19 22.7G 14KC102 F51 C~2kQD 2015 06 15.37609 16 52 54.542 -09 27 31.82 21.7G 14KC102 F51 C~2kQD 2015 06 15.38863 16 52 54.463 -09 27 31.88 22.1G 14KC102 F51 C~2kQD 2015 06 23.41292 16 52 05.718 -09 26 58.40 21.7G 14KC102 F51 C~2kQD 2015 06 23.42483 16 52 05.634 -09 26 58.55 21.8G 14KC102 F51 C~2kQD 2015 06 23.43678 16 52 05.570 -09 26 58.35 21.7G 14KC102 F51 C~2kQD 2015 06 23.44867 16 52 05.495 -09 26 58.25 21.8G 14KC102 F51 C~2kQD 2015 06 24.41748 16 51 59.766 -09 26 56.49 22.1G 14KC102 F51 C~2kQD 2015 07 13.38574 16 50 18.180 -09 27 51.71 22.2G 14KC102 F51 C~2kQD 2015 07 14.37216 16 50 13.585 -09 27 59.27 21.9G 14KC102 F51 C~2kQD 2015 08 10.28414 16 48 44.453 -09 34 20.00 22.6G 14KC102 F51 C~2kQD 2015 08 10.29607 16 48 44.427 -09 34 20.13 22.5G 14KC102 F51 C~2kQD 2015 08 10.30797 16 48 44.410 -09 34 20.49 22.2G 14KC102 F51 C~2kQD 2015 08 10.31988 16 48 44.394 -09 34 20.59 22.4G 14KC102 F51 C~2kQD 2017 05 26.36073 17 14 13.23 -10 02 09.2 21.6R 14KC102 G37 C~2Gid 2017 05 26.42079 17 14 12.85 -10 02 08.1 14KC102 G37 C~2Gid
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 -0.01 0.00 0.15
2 1.0076 0.00 -0.02 0.00 -0.10
3 1.9986 0.00 -0.05 0.00 0.00
4 2.0287 0.00 0.06 0.00 0.04
5 3.0797 0.00 -0.02 0.00 0.02
6 3.0797 0.00 -0.07 0.00 0.06
7 3.0798 0.00 -0.11 0.00 -0.07
8 3.1042 0.00 0.18 0.00 -0.33
9 3.1426 0.00 -0.07 0.00 -0.04
10 3.8989 0.00 0.15 0.00 0.40
11 3.9891 0.00 0.04 0.00 -0.09
12 3.9891 0.00 -0.19 0.00 -0.02
13 4.0326 0.00 0.05 0.00 -0.02
14 4.0326 0.00 -0.03 0.00 0.11
15 4.0327 0.00 0.00 0.00 0.14
16 4.0327 0.00 0.01 0.00 0.09
17 4.0462 0.00 0.14 0.00 0.03
18 4.0462 0.00 0.12 0.00 0.08
19 4.0463 0.00 0.15 0.00 0.14
20 4.0463 0.00 0.07 0.00 -0.04
21 4.0764 0.00 0.06 0.00 -0.13
22 4.1201 0.00 0.08 0.00 0.03
23 4.1202 0.00 0.08 0.00 -0.03
24 4.1202 0.00 0.11 0.00 0.11
25 4.1202 0.00 0.12 0.00 0.09
26 4.1365 0.00 0.11 0.00 0.05
27 4.1366 0.00 0.06 0.00 -0.07
28 4.1366 0.00 0.07 0.00 0.08
29 4.1366 0.00 0.01 0.00 0.03
30 4.2131 0.00 0.14 0.00 0.06
31 4.2594 0.00 -0.25 0.00 -0.08
32 4.2595 0.00 -0.01 0.00 -0.14
33 4.2595 0.00 -0.14 0.00 -0.05
34 4.2595 0.00 0.06 0.00 -0.06
35 4.2622 0.00 -0.02 0.00 0.05
36 4.2622 0.00 -0.17 0.00 -0.23
37 4.2623 0.00 0.03 0.00 0.09
38 4.7997 0.00 -0.15 0.00 0.06
39 4.7997 0.00 -0.16 0.00 0.32
40 4.7998 0.00 -0.01 0.00 0.13
41 4.7998 0.00 0.02 0.00 -0.10
42 4.8845 0.00 0.07 0.00 -0.03
43 4.8846 0.00 0.10 0.00 -0.08
44 4.8846 0.00 -0.19 0.00 -0.14
45 4.8846 0.00 0.11 0.00 0.01
46 4.8873 0.00 -0.10 0.00 0.02
47 4.8873 0.00 0.07 0.00 -0.06
48 4.8874 0.00 -0.14 0.00 -0.09
49 4.8874 0.00 -0.01 0.00 0.03
50 4.9502 0.00 0.01 0.00 -0.04
51 4.9502 0.00 -0.11 0.00 -0.02
52 4.9502 0.00 0.12 0.00 -0.02
53 4.9503 0.00 -0.01 0.00 0.10
54 4.9530 0.00 0.02 0.00 0.05
55 4.9530 0.00 -0.01 0.00 0.13
56 4.9531 0.00 0.11 0.00 0.17
57 5.0294 0.00 0.09 0.00 0.00
58 5.0294 0.00 -0.02 0.00 -0.10
59 5.0294 0.00 -0.02 0.00 -0.13
60 5.0295 0.00 0.02 0.00 -0.00
61 5.0811 0.00 -0.29 0.00 -0.08
62 5.0948 0.00 -0.00 0.00 -0.01
63 5.0948 0.00 -0.00 0.00 -0.14
64 5.1168 0.00 0.10 0.00 -0.04
65 5.1168 0.00 -0.08 0.00 -0.22
66 5.1168 0.00 0.05 0.00 -0.04
67 5.1169 0.00 0.00 0.00 0.03
68 5.1195 0.00 -0.08 0.00 -0.11
69 5.1715 0.00 -0.07 0.00 -0.09
70 5.1742 0.00 -0.04 0.00 0.03
71 5.2478 0.00 -0.07 0.00 -0.10
72 5.2479 0.00 -0.11 0.00 0.00
73 5.2479 0.00 -0.02 0.00 -0.12
74 5.2479 0.00 0.09 0.00 0.01
75 7.0413 0.00 0.12 0.00 0.03
76 7.0415 0.00 0.03 0.00 0.33
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.
14KC102 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.085 39.085 39.085 ecceobj 0.265 0.265 0.265 incobj 12.595 12.595 12.595 qmin 28.018 28.012 28.020 qmax 51.380 51.467 51.367 amean 39.454 39.455 39.455 amin 39.017 39.023 39.031 amax 39.941 39.938 39.945 emean 0.249 0.249 0.249 emin 0.193 0.192 0.192 emax 0.288 0.289 0.287 imean 13.278 13.273 13.280 imin 10.741 10.728 10.752 imax 16.049 16.049 16.051 excite_mean 0.341 0.341 0.341 fracstop 1.000 1.000 1.000 cjmean 2.919 2.919 2.919 libcent 0 180.1 179.9 179.5 libamp 0 62.9 63.1 63.6 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 91.4 91.4 91.5 kozaiamp 48.3 48.4 48.2