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: 523709 # Created Tue Apr 16 01:08:21 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 76 observations of 76 # Arc: 11.18y # First observation: 2012/06/14 # Last observation: 2023/08/20 # Chi-squared of fit: 43.57 DOF: 146 RMS: 0.13 # Min/Max residuals: -0.31 0.40 # Exact a, adot, b, bdot, g, gdot: 1.840667E-05 5.636673E-02 -1.486806E-05 -4.543987E-02 4.960875E-02 -1.236290E-02 # 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 -1.745519 -67.525982 0.492923 -0.027173 -0.890309 2456092.984286 # Heliocentric elements and errors Epoch: 2456092.5000 = 2012/06/14 Mean Anomaly: 322.77975 +/- 0.000 Argument of Peri: 242.26614 +/- 0.000 Long of Asc Node: 109.08407 +/- 0.000 Inclination: 39.11857 +/- 0.000 Eccentricity: 0.25026690 +/- 0.0000 Semi-Major Axis: 25.30262000 +/- 0.0000 Time of Perihelion: 2460898.9386 +/- 0.0 Perihelion: 18.97021162 +/- 0.0000 Aphelion: 31.63502838 +/- 0.0000 Period (y) 127.2789 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 7.58979956 +/- 0.0000 Ecliptic Y -19.62754255 +/- 0.0000 Ecliptic Z -0.61425328 +/- 0.0000 Ecliptic XDOT 0.00257943 +/- 0.0000 Ecliptic YDOT 0.00189319 +/- 0.0000 Ecliptic ZDOT -0.00248572 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 21.05294527 +/- 0.0000 Geocenter to KBO 20.15783711 +/- 0.0000 # Hcoef: 9.03
The following table shows the complete astrometric record for 523709. 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 (523709) followed by the observatory code and reference code for the source of the astrometry.
2012 06 14.48352 19 38 19.378 -23 17 14.62 23.1G 523709 F51 C~2kQ8 2013 06 18.51850 19 53 59.808 -25 21 04.73 22.2w 523709 F51 C~1vXS 2013 06 18.53163 19 53 59.699 -25 21 05.24 22.2w 523709 F51 C~1vXS 2013 06 18.54474 19 53 59.592 -25 21 06.02 22.4w 523709 F51 C~1vXS 2013 06 30.50586 19 52 12.711 -25 32 09.46 21.9G 523709 F51 C~2kQ8 2013 07 04.44930 19 51 34.903 -25 35 47.16 22.1G 523709 F51 C~2kQ8 2013 07 04.46187 19 51 34.764 -25 35 47.63 21.9G 523709 F51 C~2kQ8 2013 07 04.47445 19 51 34.652 -25 35 48.41 22.4G 523709 F51 C~2kQ8 2013 07 17.47978 19 49 24.856 -25 47 28.75 23.1G 523709 F51 C~2kQ8 2014 05 09.59290 20 14 15.288 -26 39 11.91 22.2w 523709 F51 C~1vXS 2014 05 09.60022 20 14 15.307 -26 39 12.63 22.2w 523709 F51 C~1vXS 2014 05 09.60754 20 14 15.279 -26 39 12.66 22.0w 523709 F51 C~1vXS 2014 05 23.57153 20 13 44.409 -26 51 22.93 22.5G 523709 F51 C~2kQ8 2014 06 04.56414 20 12 47.858 -27 03 00.65 22.9G 523709 F51 C~2kQ8 2014 06 04.58612 20 12 47.726 -27 03 01.78 22.5G 523709 F51 C~2kQ8 2014 06 04.59721 20 12 47.641 -27 03 02.73 22.8G 523709 F51 C~2kQ8 2014 06 10.54925 20 12 10.283 -27 09 05.74 22.3G 523709 F51 C~2kQ8 2014 06 20.59241 20 10 55.085 -27 19 32.20 22.3G 523709 F51 C~2kQ8 2014 06 30.49035 20 09 28.610 -27 29 53.95 21.9G 523709 F51 C~2kQ8 2014 07 29.40701 20 04 38.923 -27 58 07.09 22.1w 523709 F51 C~1vXS 2014 07 29.41827 20 04 38.797 -27 58 07.80 22.0w 523709 F51 C~1vXS 2014 07 29.42952 20 04 38.680 -27 58 08.50 22.1w 523709 F51 C~1vXS 2014 07 29.44076 20 04 38.569 -27 58 08.91 22.4w 523709 F51 C~1vXS 2014 07 31.41890 20 04 18.435 -27 59 52.30 21.3G 523709 F51 C~2kQ8 2014 08 15.36223 20 01 52.918 -28 11 35.22 22.2G 523709 F51 C~2kQ8 2014 08 22.37761 20 00 51.090 -28 16 14.55 22.2w 523709 F51 C~1vXS 2014 08 22.38909 20 00 50.986 -28 16 14.75 22.5w 523709 F51 C~1vXS 2014 08 22.40057 20 00 50.880 -28 16 15.21 22.4w 523709 F51 C~1vXS 2014 08 22.41202 20 00 50.792 -28 16 15.63 22.2w 523709 F51 C~1vXS 2014 08 23.31669 20 00 43.257 -28 16 49.12 22.1w 523709 F51 C~1vXS 2014 08 23.32800 20 00 43.184 -28 16 49.43 22.3w 523709 F51 C~1vXS 2014 08 23.33934 20 00 43.052 -28 16 50.04 22.4w 523709 F51 C~1vXS 2014 08 23.35063 20 00 42.967 -28 16 50.16 22.3w 523709 F51 C~1vXS 2015 07 24.43556 20 23 51.118 -29 48 21.37 22.2w 523709 F51 C~1vXS 2015 07 24.44587 20 23 51.003 -29 48 22.06 22.3w 523709 F51 C~1vXS 2015 07 24.45618 20 23 50.895 -29 48 22.58 22.0w 523709 F51 C~1vXS 2015 07 24.46650 20 23 50.794 -29 48 23.27 21.8w 523709 F51 C~1vXS 2016 07 12.44642 20 45 13.056 -31 22 30.11 22.3G 523709 F51 C~2kQ8 2016 07 12.45609 20 45 12.967 -31 22 30.68 23.0G 523709 F51 C~2kQ8 2016 07 12.46577 20 45 12.875 -31 22 31.56 22.2G 523709 F51 C~2kQ8 2016 07 12.47544 20 45 12.758 -31 22 32.30 22.6G 523709 F51 C~2kQ8 2016 08 07.39420 20 40 43.323 -31 51 17.30 22.0G 523709 F51 C~2kQ8 2016 08 07.40516 20 40 43.206 -31 51 18.18 22.0G 523709 F51 C~2kQ8 2016 08 07.41613 20 40 43.074 -31 51 18.80 22.4G 523709 F51 C~2kQ8 2016 08 07.42711 20 40 42.969 -31 51 19.19 21.5G 523709 F51 C~2kQ8 2016 08 10.36976 20 40 12.204 -31 54 02.41 22.2G 523709 F51 C~2kQ8 2017 06 22.54924 21 08 31.567 -32 30 22.67 22.2G 523709 F51 C~2kQ8 2017 06 22.56134 21 08 31.484 -32 30 23.69 21.9G 523709 F51 C~2kQ8 2017 06 22.57343 21 08 31.399 -32 30 24.76 22.6G 523709 F51 C~2kQ8 2017 06 22.58551 21 08 31.318 -32 30 25.90 22.0G 523709 F51 C~2kQ8 2017 06 23.55089 21 08 24.901 -32 31 49.59 22.1G 523709 F51 C~2kQ8 2017 06 23.56070 21 08 24.844 -32 31 50.49 22.3G 523709 F51 C~2kQ8 2017 06 23.57049 21 08 24.766 -32 31 51.32 22.4G 523709 F51 C~2kQ8 2017 06 23.58029 21 08 24.696 -32 31 51.97 22.1G 523709 F51 C~2kQ8 2017 08 14.34968 21 00 09.465 -33 37 48.19 22.4G 523709 F51 C~2kQ8 2017 08 14.35967 21 00 09.374 -33 37 48.65 22.2G 523709 F51 C~2kQ8 2017 08 14.36965 21 00 09.244 -33 37 49.23 21.8G 523709 F51 C~2kQ8 2017 08 14.37962 21 00 09.146 -33 37 49.88 21.6G 523709 F51 C~2kQ8 2020 08 14.40717 22 08 58.382 -37 22 21.97 21.2w 523709 F51 C~46kk 2020 08 14.41685 22 08 58.282 -37 22 22.77 21.5w 523709 F51 C~46kk 2020 08 14.43613 22 08 58.067 -37 22 24.16 21.3w 523709 F51 C~46kk 2022 07 26.484613 23 02 13.197 -37 51 43.90 21.6w 523709 F52 C~5kPj 2022 07 26.494072 23 02 13.121 -37 51 44.66 21.7w 523709 F52 C~5kPj 2022 07 26.503624 23 02 13.070 -37 51 45.80 21.6w 523709 F52 C~5kPj 2022 07 26.513168 23 02 13.008 -37 51 46.73 21.8w 523709 F52 C~5kPj 2022 08 05.521160 23 00 53.860 -38 10 18.40 21.7w 523709 F52 C~5kPj 2022 08 05.530082 23 00 53.776 -38 10 19.40 21.8w 523709 F52 C~5kPj 2022 08 05.538929 23 00 53.685 -38 10 20.46 21.6w 523709 F52 C~5kPj 2023 08 20.438233 23 24 28.634 -38 37 05.96 21.3w 523709 F52 C~78vu 2023 08 20.438912 23 24 28.620 -38 37 06.01 21.6w 523709 F52 C~78vu 2023 08 20.447237 23 24 28.529 -38 37 06.56 21.4w 523709 F52 C~78vu 2023 08 20.447905 23 24 28.526 -38 37 06.86 21.6w 523709 F52 C~78vu 2023 08 20.456303 23 24 28.476 -38 37 07.75 21.5w 523709 F52 C~78vu 2023 08 20.456975 23 24 28.458 -38 37 07.54 21.5w 523709 F52 C~78vu 2023 08 20.465321 23 24 28.365 -38 37 08.32 21.7w 523709 F52 C~78vu 2023 08 20.466006 23 24 28.362 -38 37 08.66 21.7w 523709 F52 C~78vu
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 -0.11 0.00 0.06
2 1.0104 0.00 -0.19 0.00 -0.12
3 1.0104 0.00 -0.14 0.00 0.10
4 1.0104 0.00 -0.07 0.00 0.04
5 1.0432 0.00 -0.04 0.00 -0.16
6 1.0540 0.00 0.14 0.00 -0.15
7 1.0540 0.00 -0.08 0.00 0.07
8 1.0540 0.00 0.11 0.00 -0.02
9 1.0897 0.00 0.24 0.00 -0.15
10 1.9004 0.00 -0.20 0.00 0.05
11 1.9004 0.00 0.19 0.00 -0.31
12 1.9004 0.00 -0.12 0.00 0.02
13 1.9386 0.00 -0.13 0.00 -0.08
14 1.9715 0.00 0.18 0.00 -0.01
15 1.9715 0.00 0.17 0.00 0.18
16 1.9716 0.00 -0.11 0.00 -0.10
17 1.9879 0.00 0.28 0.00 -0.09
18 2.0154 0.00 -0.05 0.00 0.02
19 2.0425 0.00 0.16 0.00 -0.02
20 2.1216 0.00 -0.01 0.00 0.22
21 2.1217 0.00 -0.14 0.00 0.11
22 2.1217 0.00 -0.14 0.00 -0.00
23 2.1217 0.00 -0.05 0.00 0.18
24 2.1271 0.00 0.29 0.00 -0.12
25 2.1680 0.00 0.09 0.00 0.11
26 2.1873 0.00 -0.03 0.00 -0.09
27 2.1873 0.00 -0.11 0.00 0.14
28 2.1873 0.00 -0.22 0.00 0.10
29 2.1873 0.00 -0.06 0.00 0.10
30 2.1898 0.00 0.06 0.00 0.03
31 2.1899 0.00 0.40 0.00 0.14
32 2.1899 0.00 -0.13 0.00 -0.06
33 2.1899 0.00 0.03 0.00 0.24
34 3.1073 0.00 0.04 0.00 -0.02
35 3.1074 0.00 -0.04 0.00 -0.08
36 3.1074 0.00 -0.01 0.00 0.03
37 3.1074 0.00 0.12 0.00 -0.03
38 4.0766 0.00 0.09 0.00 -0.13
39 4.0766 0.00 0.20 0.00 0.03
40 4.0766 0.00 0.28 0.00 -0.13
41 4.0766 0.00 -0.03 0.00 -0.15
42 4.1476 0.00 -0.07 0.00 0.20
43 4.1476 0.00 -0.06 0.00 -0.05
44 4.1477 0.00 -0.27 0.00 -0.05
45 4.1477 0.00 -0.08 0.00 0.18
46 4.1557 0.00 0.17 0.00 -0.07
47 5.0214 0.00 0.08 0.00 0.04
48 5.0214 0.00 0.06 0.00 0.07
49 5.0215 0.00 0.02 0.00 0.04
50 5.0215 0.00 0.03 0.00 -0.05
51 5.0241 0.00 -0.10 0.00 -0.08
52 5.0242 0.00 0.07 0.00 -0.13
53 5.0242 0.00 -0.08 0.00 -0.11
54 5.0242 0.00 -0.11 0.00 0.09
55 5.1660 0.00 -0.08 0.00 -0.09
56 5.1660 0.00 0.17 0.00 0.02
57 5.1660 0.00 -0.16 0.00 0.00
58 5.1660 0.00 -0.02 0.00 -0.08
59 8.1668 0.00 -0.06 0.00 -0.06
60 8.1668 0.00 0.04 0.00 -0.08
61 8.1669 0.00 0.00 0.00 0.06
62 10.1136 0.00 -0.13 0.00 -0.26
63 10.1136 0.00 -0.24 0.00 0.07
64 10.1137 0.00 0.04 0.00 0.02
65 10.1137 0.00 0.16 0.00 0.19
66 10.1411 0.00 -0.05 0.00 0.16
67 10.1411 0.00 -0.12 0.00 0.12
68 10.1412 0.00 -0.30 0.00 0.01
69 11.1813 0.00 0.05 0.00 -0.15
70 11.1813 0.00 -0.06 0.00 -0.13
71 11.1813 0.00 -0.19 0.00 0.14
72 11.1813 0.00 -0.14 0.00 -0.09
73 11.1813 0.00 0.36 0.00 -0.15
74 11.1813 0.00 0.19 0.00 0.13
75 11.1813 0.00 0.04 0.00 0.18
76 11.1813 0.00 0.10 0.00 -0.10
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.
523709 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 25.233 25.233 25.233 ecceobj 0.251 0.251 0.251 incobj 39.112 39.112 39.112 qmin 15.191 16.701 16.821 qmax 35.478 34.054 33.887 amean 25.029 25.084 25.152 amin 23.799 24.173 24.778 amax 25.874 25.662 25.538 emean 0.228 0.245 0.183 emin 0.085 0.120 0.033 emax 0.397 0.337 0.330 imean 37.372 37.136 37.925 imin 33.415 35.162 35.339 imax 39.133 38.803 39.395 excite_mean 0.654 0.654 0.645 fracstop 0.290 0.152 0.619 cjmean 2.602 2.599 2.609 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 209.3 201.9 196.7 kozaiamp 179.7 179.8 180.0