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: 534631 # Created Tue Apr 16 01:08:43 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 86 observations of 86 # Arc: 12.02y # First observation: 2010/09/13 # Last observation: 2022/09/22 # Chi-squared of fit: 34.23 DOF: 166 RMS: 0.11 # Min/Max residuals: -0.32 0.44 # Exact a, adot, b, bdot, g, gdot: 2.247336E-05 5.338191E-02 7.017733E-06 1.524551E-02 3.927921E-02 -1.033243E-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 -1.187566 12.066268 0.368906 -0.019335 -0.931252 2455452.967246 # Heliocentric elements and errors Epoch: 2455452.5000 = 2010/09/13 Mean Anomaly: 356.72839 +/- 0.000 Argument of Peri: 2.90698 +/- 0.000 Long of Asc Node: 15.27306 +/- 0.000 Inclination: 15.94463 +/- 0.000 Eccentricity: 0.34150774 +/- 0.0000 Semi-Major Axis: 40.00839627 +/- 0.0000 Time of Perihelion: 2456292.5095 +/- 0.0 Perihelion: 26.34521918 +/- 0.0000 Aphelion: 53.67157336 +/- 0.0000 Period (y) 253.0667 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 25.88301103 +/- 0.0000 Ecliptic Y 5.15394699 +/- 0.0000 Ecliptic Z -0.52745129 +/- 0.0000 Ecliptic XDOT -0.00082623 +/- 0.0000 Ecliptic YDOT 0.00363454 +/- 0.0000 Ecliptic ZDOT 0.00106389 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 26.39645004 +/- 0.0000 Geocenter to KBO 25.45880633 +/- 0.0000 # Hcoef: 8.15
The following table shows the complete astrometric record for 534631. 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 (534631) followed by the observatory code and reference code for the source of the astrometry.
2010 09 13.46648 00 46 14.602 +03 40 34.65 22.8G 534631 F51 C~2rYC 2010 09 15.52115 00 46 01.524 +03 39 29.11 22.1G 534631 F51 C~2rYC 2010 09 16.47908 00 45 55.345 +03 38 57.91 22.0G 534631 F51 C~2rYC 2010 10 04.46282 00 43 53.358 +03 28 44.08 21.9G 534631 F51 C~2rYC 2010 10 14.30163 00 42 45.273 +03 23 06.39 21.9G 534631 F51 C~2rYC 2010 11 01.24396 00 40 49.239 +03 13 52.43 22.4G 534631 F51 C~2rYC 2011 09 26.48069 00 54 50.240 +05 33 38.50 22.2G 534631 F51 C~2rYC 2011 10 18.37514 00 52 18.310 +05 21 12.04 22.8G 534631 F51 C~2rYC 2011 10 25.26311 00 51 31.959 +05 17 26.60 22.6G 534631 F51 C~2rYC 2012 10 08.41894 01 03 26.993 +07 26 17.38 22.0G 534631 F51 C~2rYC 2012 10 09.35201 01 03 20.467 +07 25 45.66 22.4G 534631 F51 C~2rYC 2012 10 09.36613 01 03 20.335 +07 25 45.27 22.1G 534631 F51 C~2rYC 2012 10 09.38036 01 03 20.237 +07 25 45.04 22.2G 534631 F51 C~2rYC 2012 10 09.39466 01 03 20.131 +07 25 44.43 22.3G 534631 F51 C~2rYC 2013 09 15.59054 01 16 11.290 +09 36 47.41 22.8G 534631 F51 C~2rYC 2013 09 24.54967 01 15 14.347 +09 32 41.90 22.2G 534631 F51 C~2rYC 2014 07 25.52468 01 29 03.632 +11 37 10.69 22.5r 534631 568 C~2SDm 2014 07 25.56621 01 29 03.642 +11 37 11.40 22.5r 534631 568 C~2SDm 2014 07 25.60786 01 29 03.652 +11 37 12.10 22.4r 534631 568 C~2SDm 2014 08 23.56417 01 28 16.862 +11 39 26.40 22.5r 534631 568 C~2SDm 2014 08 23.61113 01 28 16.690 +11 39 26.12 22.3r 534631 568 C~2SDm 2014 08 27.45651 01 28 02.278 +11 38 54.15 22.5r 534631 568 C~2SDm 2014 08 27.59937 01 28 01.688 +11 38 52.76 22.4r 534631 568 C~2SDm 2014 09 18.39229 01 26 10.002 +11 32 39.14 22.5r 534631 568 C~2SDm 2014 09 18.43188 01 26 09.754 +11 32 38.20 22.4r 534631 568 C~2SDm 2014 09 19.45160 01 26 03.482 +11 32 13.68 22.4G 534631 F51 C~2rYC 2014 10 22.43319 01 22 16.224 +11 15 36.47 22.2r 534631 568 C~2SDm 2014 10 22.47264 01 22 15.938 +11 15 35.13 22.3r 534631 568 C~2SDm 2014 10 22.51153 01 22 15.657 +11 15 33.83 22.3r 534631 568 C~2SDm 2014 10 23.43094 01 22 09.151 +11 15 03.15 22.1r 534631 568 C~2SDm 2014 10 25.43607 01 21 54.999 +11 13 56.14 22.1r 534631 568 C~2SDm 2014 10 25.50080 01 21 54.557 +11 13 53.98 22.1G 534631 F51 C~2rYC 2014 11 19.24343 01 19 16.271 +11 01 03.58 22.3r 534631 568 C~2SDm 2014 11 19.37639 01 19 15.519 +11 00 59.95 22.2r 534631 568 C~2SDm 2014 11 21.22330 01 19 05.564 +11 00 10.57 22.4r 534631 568 C~2SDm 2014 11 21.38502 01 19 04.680 +11 00 06.38 22.4r 534631 568 C~2SDm 2014 11 28.40964 01 18 30.028 +10 57 14.55 22.7G 534631 F51 C~2rYC 2015 09 12.44517 01 37 05.325 +13 29 41.45 22.8G 534631 F51 C~2rYC 2015 09 12.45555 01 37 05.271 +13 29 41.51 22.4G 534631 F51 C~2rYC 2015 09 12.46595 01 37 05.212 +13 29 41.17 22.3G 534631 F51 C~2rYC 2015 09 12.47641 01 37 05.151 +13 29 41.14 22.2G 534631 F51 C~2rYC 2015 09 15.51502 01 36 48.293 +13 28 47.14 22.4w 534631 568 C~2SDm 2015 09 15.57438 01 36 47.946 +13 28 46.03 22.5w 534631 568 C~2SDm 2015 10 13.48307 01 33 43.665 +13 16 45.70 534631 568 C~2SDm 2015 10 13.49677 01 33 43.570 +13 16 45.46 534631 568 C~2SDm 2015 10 13.54938 01 33 43.180 +13 16 43.60 534631 568 C~2SDm 2015 12 03.22349 01 28 21.537 +12 51 01.67 22.8G 534631 F51 C~2rYC 2015 12 07.21672 01 28 05.040 +12 49 36.13 22.3r 534631 568 C~2SDm 2015 12 07.22184 01 28 05.022 +12 49 35.98 24.4u 534631 568 C~2SDm 2015 12 07.22618 01 28 05.003 +12 49 35.96 24.4u 534631 568 C~2SDm 2015 12 07.23049 01 28 04.989 +12 49 35.82 24.5u 534631 568 C~2SDm 2015 12 07.23483 01 28 04.972 +12 49 35.72 24.4u 534631 568 C~2SDm 2015 12 07.23918 01 28 04.973 +12 49 35.75 22.1u 534631 568 C~2SDm 2015 12 07.24354 01 28 04.935 +12 49 35.65 24.5u 534631 568 C~2SDm 2015 12 07.25660 01 28 04.880 +12 49 35.33 24.6u 534631 568 C~2SDm 2015 12 07.26533 01 28 04.847 +12 49 35.17 24.6u 534631 568 C~2SDm 2015 12 07.26968 01 28 04.820 +12 49 35.04 24.3u 534631 568 C~2SDm 2015 12 07.27404 01 28 04.819 +12 49 34.95 24.3u 534631 568 C~2SDm 2015 12 07.27834 01 28 04.803 +12 49 34.88 24.3u 534631 568 C~2SDm 2015 12 07.28352 01 28 04.772 +12 49 34.80 22.4r 534631 568 C~2SDm 2015 12 07.45332 01 28 04.085 +12 49 31.27 22.6w 534631 568 C~2SDm 2015 12 07.45744 01 28 04.066 +12 49 31.21 22.6w 534631 568 C~2SDm 2015 12 14.36266 01 27 40.493 +12 47 27.45 22.2G 534631 F51 C~2rYC 2015 12 31.26584 01 27 10.631 +12 44 51.29 22.5G 534631 F51 C~2rYC 2015 12 31.27707 01 27 10.629 +12 44 51.35 22.7G 534631 F51 C~2rYC 2015 12 31.28823 01 27 10.610 +12 44 51.28 22.4G 534631 F51 C~2rYC 2015 12 31.29945 01 27 10.609 +12 44 51.42 22.7G 534631 F51 C~2rYD 2016 08 10.52099 01 49 15.935 +15 22 45.76 22.6G 534631 F51 C~2rYD 2016 08 10.53390 01 49 15.940 +15 22 45.88 22.8G 534631 F51 C~2rYD 2016 08 10.54685 01 49 15.923 +15 22 46.03 22.1G 534631 F51 C~2rYD 2016 08 10.55979 01 49 15.903 +15 22 46.30 22.3G 534631 F51 C~2rYD 2016 10 06.51624 01 44 56.255 +15 13 38.34 22.2G 534631 F51 C~2rYD 2016 10 06.52878 01 44 56.163 +15 13 37.54 22.3G 534631 F51 C~2rYD 2016 10 06.54126 01 44 56.077 +15 13 37.09 22.8G 534631 F51 C~2rYD 2016 10 06.55383 01 44 55.991 +15 13 37.01 22.5G 534631 F51 C~2rYD 2017 08 25.55831 01 59 10.372 +17 12 45.29 22.5w 534631 568 C~2SDm 2017 08 30.58085 01 58 54.473 +17 12 54.83 22.7w 534631 568 C~2SDm 2017 09 21.57504 01 57 09.852 +17 09 55.65 22.4G 534631 F51 C~2rYD 2017 09 21.58894 01 57 09.765 +17 09 55.46 22.6G 534631 F51 C~2rYD 2017 09 21.60282 01 57 09.671 +17 09 55.28 22.7G 534631 F51 C~2rYD 2017 09 21.61671 01 57 09.596 +17 09 54.95 22.7G 534631 F51 C~2rYD 2017 10 22.45238 01 53 38.648 +16 57 33.14 21.8G 534631 F51 C~2rYD 2018 01 13.25702 01 47 29.375 +16 25 38.20 22.3G 534631 F51 C~2rYD 2022 09 22.460619 02 51 50.050 +25 29 52.85 22.4w 534631 F52 C~5qem 2022 09 22.470791 02 51 50.015 +25 29 52.56 22.6w 534631 F52 C~5qem 2022 09 22.491222 02 51 49.887 +25 29 53.08 22.8w 534631 F52 C~5qem
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 -0.12 0.00 -0.25
2 0.0056 0.00 0.10 0.00 0.05
3 0.0082 0.00 -0.02 0.00 -0.04
4 0.0575 0.00 -0.04 0.00 -0.04
5 0.0844 0.00 -0.02 0.00 0.14
6 0.1335 0.00 0.03 0.00 -0.13
7 1.0349 0.00 0.14 0.00 0.21
8 1.0949 0.00 -0.03 0.00 -0.06
9 1.1137 0.00 0.06 0.00 -0.02
10 2.0697 0.00 -0.12 0.00 -0.17
11 2.0722 0.00 0.44 0.00 -0.18
12 2.0723 0.00 -0.02 0.00 -0.09
13 2.0723 0.00 0.04 0.00 0.16
14 2.0724 0.00 -0.01 0.00 0.04
15 3.0065 0.00 0.01 0.00 0.20
16 3.0310 0.00 0.03 0.00 0.24
17 3.8633 0.00 0.03 0.00 -0.04
18 3.8634 0.00 0.01 0.00 -0.02
19 3.8635 0.00 0.00 0.00 -0.01
20 3.9428 0.00 -0.04 0.00 -0.01
21 3.9429 0.00 -0.05 0.00 0.03
22 3.9534 0.00 0.01 0.00 -0.03
23 3.9538 0.00 -0.00 0.00 -0.03
24 4.0135 0.00 -0.01 0.00 -0.04
25 4.0136 0.00 -0.03 0.00 -0.05
26 4.0164 0.00 -0.09 0.00 -0.08
27 4.1067 0.00 -0.06 0.00 -0.04
28 4.1068 0.00 -0.07 0.00 -0.06
29 4.1069 0.00 -0.07 0.00 -0.05
30 4.1094 0.00 -0.02 0.00 -0.01
31 4.1149 0.00 -0.02 0.00 -0.01
32 4.1151 0.00 0.29 0.00 0.00
33 4.1828 0.00 -0.01 0.00 0.03
34 4.1832 0.00 -0.07 0.00 0.01
35 4.1882 0.00 -0.03 0.00 0.04
36 4.1887 0.00 -0.10 0.00 0.09
37 4.2079 0.00 -0.11 0.00 -0.17
38 4.9965 0.00 -0.04 0.00 -0.13
39 4.9965 0.00 0.01 0.00 0.10
40 4.9966 0.00 -0.01 0.00 -0.07
41 4.9966 0.00 -0.06 0.00 0.08
42 5.0049 0.00 0.01 0.00 0.03
43 5.0051 0.00 -0.01 0.00 0.03
44 5.0815 0.00 -0.01 0.00 0.01
45 5.0815 0.00 0.07 0.00 0.20
46 5.0817 0.00 -0.02 0.00 -0.00
47 5.2204 0.00 -0.20 0.00 -0.20
48 5.2313 0.00 -0.02 0.00 0.02
49 5.2314 0.00 0.02 0.00 -0.03
50 5.2314 0.00 -0.00 0.00 0.04
51 5.2314 0.00 0.05 0.00 -0.02
52 5.2314 0.00 0.05 0.00 -0.03
53 5.2314 0.00 0.33 0.00 0.09
54 5.2314 0.00 0.02 0.00 0.08
55 5.2315 0.00 -0.01 0.00 0.02
56 5.2315 0.00 0.02 0.00 0.04
57 5.2315 0.00 -0.12 0.00 -0.00
58 5.2315 0.00 0.12 0.00 -0.01
59 5.2315 0.00 0.14 0.00 0.01
60 5.2315 0.00 -0.01 0.00 0.04
61 5.2320 0.00 -0.16 0.00 -0.03
62 5.2320 0.00 -0.21 0.00 -0.00
63 5.2509 0.00 -0.07 0.00 -0.16
64 5.2972 0.00 -0.03 0.00 -0.03
65 5.2972 0.00 0.05 0.00 0.06
66 5.2973 0.00 -0.12 0.00 0.02
67 5.2973 0.00 -0.03 0.00 0.19
68 5.9084 0.00 -0.24 0.00 -0.00
69 5.9085 0.00 0.08 0.00 -0.03
70 5.9085 0.00 0.08 0.00 -0.03
71 5.9085 0.00 0.03 0.00 0.09
72 6.0645 0.00 -0.02 0.00 0.42
73 6.0645 0.00 -0.06 0.00 -0.04
74 6.0645 0.00 -0.02 0.00 -0.15
75 6.0646 0.00 0.04 0.00 0.12
76 6.9489 0.00 -0.02 0.00 0.01
77 6.9627 0.00 -0.03 0.00 0.04
78 7.0229 0.00 0.15 0.00 -0.02
79 7.0229 0.00 0.10 0.00 0.02
80 7.0230 0.00 -0.06 0.00 0.06
81 7.0230 0.00 0.07 0.00 -0.04
82 7.1074 0.00 -0.10 0.00 0.08
83 7.3341 0.00 0.41 0.00 -0.20
84 12.0246 0.00 0.01 0.00 -0.00
85 12.0247 0.00 0.23 0.00 -0.32
86 12.0247 0.00 -0.19 0.00 0.13
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.
534631 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 40.017 40.017 40.017 ecceobj 0.342 0.342 0.342 incobj 15.938 15.938 15.938 qmin 25.830 25.750 25.876 qmax 54.047 54.033 54.023 amean 39.455 39.454 39.455 amin 38.886 38.912 38.888 amax 40.212 40.137 40.202 emean 0.330 0.333 0.331 emin 0.316 0.319 0.318 emax 0.345 0.347 0.344 imean 15.953 15.909 15.842 imin 15.326 15.420 15.210 imax 16.514 16.518 16.422 excite_mean 0.430 0.431 0.429 fracstop 1.000 1.000 1.000 cjmean 2.840 2.838 2.841 libcent 0 179.3 178.7 178.5 libamp 0 128.9 127.0 130.8 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 169.2 179.2 170.4 kozaiamp 180.0 179.9 179.9