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: 602714 # Created Sun Nov 24 02:07:36 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 76 observations of 76 # Arc: 11.09y # First observation: 2011/07/27 # Last observation: 2022/08/27 # Chi-squared of fit: 83.79 DOF: 146 RMS: 0.19 # Min/Max residuals: -0.76 0.71 # Exact a, adot, b, bdot, g, gdot: 2.107053E-05 4.099695E-02 4.873516E-06 8.415845E-03 3.143407E-02 3.091474E-03 # Covariance matrix: 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 # lat0 lon0 xBary yBary zBary JD0 -4.357117 -33.304025 0.395299 -0.070994 -0.931025 2455769.973116 # Heliocentric elements and errors Epoch: 2455770.5000 = 2011/07/28 Mean Anomaly: 3.27918 +/- 0.000 Argument of Peri: 328.94434 +/- 0.000 Long of Asc Node: 345.91756 +/- 0.000 Inclination: 12.25945 +/- 0.000 Eccentricity: 0.48360823 +/- 0.0000 Semi-Major Axis: 63.05807481 +/- 0.0000 Time of Perihelion: 2454104.5126 +/- 0.0 Perihelion: 32.56267064 +/- 0.0000 Aphelion: 93.55347898 +/- 0.0000 Period (y) 500.7480 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 27.07865590 +/- 0.0000 Ecliptic Y -18.25923092 +/- 0.0000 Ecliptic Z -2.41669104 +/- 0.0000 Ecliptic XDOT 0.00222873 +/- 0.0000 Ecliptic YDOT 0.00281191 +/- 0.0000 Ecliptic ZDOT 0.00071048 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 32.74890604 +/- 0.0000 Geocenter to KBO 31.81259274 +/- 0.0000 # Hcoef: 7.56
The following table shows the complete astrometric record for 602714. 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 (602714) followed by the observatory code and reference code for the source of the astrometry.
2011 07 27.47235 22 01 52.407 -16 42 26.70 22.9G 602714 F51 C~346c 2011 07 27.48705 22 01 52.327 -16 42 26.81 22.2G 602714 F51 C~346c 2011 07 27.50174 22 01 52.263 -16 42 27.38 22.0G 602714 F51 C~346c 2011 07 27.51643 22 01 52.196 -16 42 27.60 22.5G 602714 F51 C~346c 2011 08 17.39740 21 59 56.193 -16 51 35.28 22.4G 602714 F51 C~346c 2011 08 30.41828 21 58 40.675 -16 56 57.69 22.7G 602714 F51 C~346c 2011 08 30.43304 21 58 40.609 -16 56 58.10 23.0G 602714 F51 C~346c 2011 08 30.44777 21 58 40.510 -16 56 58.52 21.8G 602714 F51 C~346c 2011 08 30.46259 21 58 40.434 -16 56 58.83 23.0G 602714 F51 C~346c 2012 08 17.43467 22 08 19.842 -15 35 33.35 22.3w 602714 F51 C~1vXg 2012 08 17.44893 22 08 19.754 -15 35 33.73 22.6w 602714 F51 C~1vXg 2012 08 17.47749 22 08 19.591 -15 35 34.45 22.7w 602714 F51 C~1vXg 2013 06 19.57920 22 20 38.154 -13 57 25.76 21.8G 602714 F51 C~346c 2013 08 09.43358 22 17 23.943 -14 14 48.64 22.0G 602714 F51 C~346c 2013 08 09.45171 22 17 23.851 -14 14 49.31 21.8G 602714 F51 C~346c 2013 08 09.46595 22 17 23.771 -14 14 49.63 21.6G 602714 F51 C~346c 2013 08 09.48019 22 17 23.693 -14 14 50.05 22.4G 602714 F51 C~346c 2013 08 26.50394 22 15 47.905 -14 22 27.54 22.2G 602714 F51 C~346c 2013 08 31.40387 22 15 20.022 -14 24 34.17 22.5w 602714 F51 C~1vXg 2013 08 31.41839 22 15 19.935 -14 24 34.39 22.4w 602714 F51 C~1vXg 2013 08 31.43286 22 15 19.856 -14 24 35.10 22.7w 602714 F51 C~1vXg 2014 07 06.56770 22 27 58.884 -12 44 20.61 23.5G 602714 F51 C~346c 2014 07 06.57845 22 27 58.842 -12 44 21.34 22.5G 602714 F51 C~346c 2014 07 06.58920 22 27 58.820 -12 44 21.18 22.9G 602714 F51 C~346c 2014 07 06.59998 22 27 58.763 -12 44 21.36 22.8G 602714 F51 C~346c 2014 07 25.52380 22 26 46.635 -12 50 51.13 22.6w 602714 F51 C~1vXg 2014 07 25.53591 22 26 46.576 -12 50 51.27 22.8w 602714 F51 C~1vXg 2014 07 25.54803 22 26 46.527 -12 50 51.38 22.7w 602714 F51 C~1vXg 2014 07 25.56014 22 26 46.476 -12 50 51.81 22.5w 602714 F51 C~1vXg 2014 08 03.47484 22 26 03.695 -12 54 34.91 22.6w 602714 F51 C~1vXg 2014 08 03.48833 22 26 03.618 -12 54 35.20 22.6w 602714 F51 C~1vXg 2014 08 03.51518 22 26 03.486 -12 54 35.94 23.0w 602714 F51 C~1vXg 2014 08 05.46854 22 25 53.559 -12 55 27.08 23.0G 602714 F51 C~346c 2014 08 05.48214 22 25 53.450 -12 55 27.46 23.1G 602714 F51 C~346c 2014 08 05.49565 22 25 53.383 -12 55 27.60 22.9G 602714 F51 C~346c 2014 08 05.50915 22 25 53.326 -12 55 27.99 22.2G 602714 F51 C~346c 2014 08 20.42829 22 24 32.666 -13 02 11.77 22.4w 602714 F51 C~1vXg 2014 08 20.44113 22 24 32.598 -13 02 12.12 22.4w 602714 F51 C~1vXg 2014 08 20.46688 22 24 32.454 -13 02 12.85 22.2w 602714 F51 C~1vXg 2014 09 02.34782 22 23 19.779 -13 07 59.63 22.4G 602714 F51 C~346c 2014 09 02.36143 22 23 19.711 -13 08 00.14 23.1G 602714 F51 C~346c 2014 09 02.37504 22 23 19.638 -13 07 59.94 23.1G 602714 F51 C~346c 2014 09 02.38862 22 23 19.561 -13 08 00.37 23.0G 602714 F51 C~346c 2014 09 12.42196 22 22 24.184 -13 12 10.85 22.2G 602714 F51 C~346c 2014 11 10.24430 22 19 08.173 -13 21 47.01 24.1G 602714 F51 C~346c 2014 11 17.24872 22 19 07.946 -13 20 35.57 24.1G 602714 F51 C~346c 2014 11 25.20599 22 19 14.850 -13 18 33.60 23.1G 602714 F51 C~346c 2015 07 12.53637 22 35 33.332 -11 28 44.25 22.8G 602714 F51 C~346c 2015 07 28.52183 22 34 30.185 -11 34 20.51 21.9G 602714 F51 C~346c 2015 08 21.41190 22 32 27.956 -11 44 49.06 22.2G 602714 F51 C~346c 2015 08 21.42310 22 32 27.926 -11 44 49.18 22.9G 602714 F51 C~346c 2015 08 21.43424 22 32 27.808 -11 44 50.39 23.1G 602714 F51 C~346c 2015 08 21.44537 22 32 27.773 -11 44 50.34 23.0G 602714 F51 C~346c 2015 10 26.29605 22 27 23.290 -12 06 29.06 22.4G 602714 F51 C~346c 2015 11 03.27030 22 27 07.839 -12 06 44.69 23.3G 602714 F51 C~346c 2016 07 07.53491 22 43 29.720 -10 10 21.57 22.9G 602714 F51 C~346c 2016 10 25.26019 22 35 10.941 -10 50 11.35 22.6G 602714 F51 C~346c 2016 10 25.27133 22 35 10.912 -10 50 11.76 22.5G 602714 F51 C~346c 2016 10 25.28248 22 35 10.878 -10 50 11.77 22.6G 602714 F51 C~346c 2016 10 25.29367 22 35 10.847 -10 50 11.97 22.8G 602714 F51 C~346c 2017 08 01.48157 22 49 36.569 -09 00 57.04 23.0G 602714 F51 C~346c 2017 08 01.49290 22 49 36.504 -09 00 57.31 22.5G 602714 F51 C~346c 2017 08 01.50424 22 49 36.478 -09 00 57.87 22.5G 602714 F51 C~346c 2017 08 01.51558 22 49 36.403 -09 00 58.51 23.2G 602714 F51 C~346c 2017 08 03.49426 22 49 27.461 -09 01 45.53 21.9G 602714 F51 C~346c 2017 09 14.36425 22 45 47.115 -09 20 38.50 22.4G 602714 F51 C~346c 2017 09 14.37569 22 45 47.069 -09 20 38.65 22.5G 602714 F51 C~346c 2017 09 14.38712 22 45 46.990 -09 20 39.14 22.6G 602714 F51 C~346c 2017 09 14.39854 22 45 46.927 -09 20 39.65 22.7G 602714 F51 C~346c 2017 10 10.35087 22 43 42.032 -09 30 26.48 22.9G 602714 F51 C~346c 2021 10 03.131660 23 13 45.583 -04 22 50.48 22.9G 602714 G37 C~55Qu 2021 10 03.184770 23 13 45.332 -04 22 51.90 602714 G37 C~55Qu 2021 10 03.237690 23 13 45.065 -04 22 53.22 602714 G37 C~55Qu 2022 08 27.247340 23 24 01.961 -02 50 36.02 22.8G 602714 G37 C~5nzo 2022 08 27.294110 23 24 01.721 -02 50 37.33 602714 G37 C~5nzo 2022 08 27.341100 23 24 01.489 -02 50 38.51 602714 G37 C~5nzo
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 -0.04 0.00 -0.16
2 0.0000 0.00 -0.08 0.00 0.11
3 0.0001 0.00 0.12 0.00 -0.08
4 0.0001 0.00 0.28 0.00 0.08
5 0.0573 0.00 0.11 0.00 -0.18
6 0.0929 0.00 -0.21 0.00 -0.15
7 0.0930 0.00 0.09 0.00 -0.22
8 0.0930 0.00 -0.10 0.00 -0.30
9 0.0931 0.00 0.06 0.00 -0.26
10 1.0594 0.00 -0.05 0.00 0.12
11 1.0595 0.00 -0.12 0.00 0.12
12 1.0596 0.00 -0.06 0.00 0.15
13 1.8976 0.00 0.21 0.00 0.45
14 2.0369 0.00 -0.03 0.00 0.07
15 2.0369 0.00 0.10 0.00 -0.11
16 2.0369 0.00 0.09 0.00 -0.04
17 2.0370 0.00 0.10 0.00 -0.08
18 2.0836 0.00 -0.02 0.00 -0.06
19 2.0970 0.00 -0.01 0.00 0.03
20 2.0970 0.00 -0.05 0.00 0.18
21 2.0971 0.00 0.02 0.00 -0.16
22 2.9435 0.00 0.04 0.00 0.36
23 2.9435 0.00 -0.09 0.00 -0.19
24 2.9435 0.00 0.09 0.00 0.15
25 2.9435 0.00 -0.26 0.00 0.15
26 2.9953 0.00 0.00 0.00 -0.15
27 2.9954 0.00 -0.04 0.00 -0.00
28 2.9954 0.00 0.07 0.00 0.17
29 2.9954 0.00 0.15 0.00 0.03
30 3.0199 0.00 0.14 0.00 -0.01
31 3.0199 0.00 0.03 0.00 0.05
32 3.0200 0.00 0.13 0.00 0.01
33 3.0253 0.00 0.36 0.00 -0.04
34 3.0254 0.00 -0.20 0.00 -0.06
35 3.0254 0.00 -0.14 0.00 0.15
36 3.0254 0.00 0.07 0.00 0.12
37 3.0663 0.00 -0.21 0.00 0.14
38 3.0663 0.00 -0.13 0.00 0.14
39 3.0664 0.00 -0.09 0.00 0.12
40 3.1016 0.00 -0.21 0.00 -0.18
41 3.1017 0.00 -0.06 0.00 -0.33
42 3.1017 0.00 0.01 0.00 0.23
43 3.1018 0.00 0.02 0.00 0.15
44 3.1292 0.00 0.09 0.00 0.15
45 3.2903 0.00 0.09 0.00 0.06
46 3.3094 0.00 0.05 0.00 -0.16
47 3.3312 0.00 0.71 0.00 0.27
48 3.9591 0.00 0.19 0.00 -0.11
49 4.0029 0.00 0.05 0.00 0.19
50 4.0683 0.00 -0.43 0.00 0.20
51 4.0683 0.00 0.07 0.00 0.39
52 4.0683 0.00 -0.76 0.00 -0.51
53 4.0684 0.00 -0.35 0.00 -0.15
54 4.2487 0.00 0.14 0.00 -0.17
55 4.2705 0.00 -0.08 0.00 0.11
56 4.9475 0.00 0.21 0.00 0.04
57 5.2479 0.00 -0.05 0.00 0.25
58 5.2479 0.00 -0.04 0.00 -0.08
59 5.2479 0.00 -0.10 0.00 -0.01
60 5.2480 0.00 -0.12 0.00 -0.13
61 6.0151 0.00 -0.01 0.00 0.23
62 6.0151 0.00 -0.21 0.00 0.23
63 6.0151 0.00 0.18 0.00 -0.06
64 6.0152 0.00 -0.17 0.00 -0.44
65 6.0206 0.00 -0.04 0.00 -0.46
66 6.1352 0.00 0.09 0.00 -0.00
67 6.1353 0.00 0.33 0.00 0.15
68 6.1353 0.00 0.08 0.00 -0.03
69 6.1353 0.00 0.08 0.00 -0.24
70 6.2064 0.00 0.10 0.00 -0.13
71 10.1866 0.00 -0.02 0.00 -0.01
72 10.1868 0.00 0.11 0.00 -0.05
73 10.1869 0.00 -0.01 0.00 -0.00
74 11.0849 0.00 -0.01 0.00 0.03
75 11.0851 0.00 -0.05 0.00 -0.03
76 11.0852 0.00 0.07 0.00 0.04
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.
602714 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 62.597 62.596 62.597 ecceobj 0.480 0.480 0.480 incobj 12.241 12.241 12.241 qmin 30.782 30.750 31.272 qmax 120.064 104.835 116.399 amean 69.390 61.602 70.063 amin 61.455 55.288 61.456 amax 76.132 68.732 74.422 emean 0.535 0.480 0.536 emin 0.466 0.431 0.466 emax 0.582 0.526 0.564 imean 11.714 11.420 12.157 imin 9.289 9.266 10.386 imax 13.816 13.970 13.947 excite_mean 0.573 0.519 0.576 fracstop 1.000 1.000 1.000 cjmean 2.943 2.947 2.947 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 152.1 179.8 200.8 kozaiamp 180.0 180.0 179.9