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: 523748 # Created Fri Apr 19 01:08:26 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 84 observations of 84 # Arc: 13.06y # First observation: 2010/11/11 # Last observation: 2023/12/04 # Chi-squared of fit: 68.77 DOF: 162 RMS: 0.16 # Min/Max residuals: -0.50 0.58 # Exact a, adot, b, bdot, g, gdot: 1.555527E-05 2.359716E-02 -1.843702E-06 -3.473697E-03 2.468374E-02 -1.855217E-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 -16.767109 61.372781 0.210447 -0.278507 -0.924407 2455512.013686 # Heliocentric elements and errors Epoch: 2455512.5000 = 2010/11/12 Mean Anomaly: 266.29826 +/- 0.000 Argument of Peri: 346.62637 +/- 0.000 Long of Asc Node: 178.67704 +/- 0.000 Inclination: 18.35331 +/- 0.000 Eccentricity: 0.08245677 +/- 0.0000 Semi-Major Axis: 40.94753483 +/- 0.0000 Time of Perihelion: 2480423.1584 +/- 0.0 Perihelion: 37.57113316 +/- 0.0000 Aphelion: 44.32393649 +/- 0.0000 Period (y) 262.0293 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 19.23560661 +/- 0.0000 Ecliptic Y 34.79409668 +/- 0.0000 Ecliptic Z -11.68722980 +/- 0.0000 Ecliptic XDOT -0.00244530 +/- 0.0000 Ecliptic YDOT 0.00098981 +/- 0.0000 Ecliptic ZDOT -0.00030955 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 41.43951320 +/- 0.0000 Geocenter to KBO 40.51257783 +/- 0.0000 # Hcoef: 5.89
The following table shows the complete astrometric record for 523748. 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 (523748) followed by the observatory code and reference code for the source of the astrometry.
2010 11 11.51292 04 10 29.327 +03 59 33.80 22.2G 523748 F51 C~2kQv 2010 11 18.34270 04 09 56.587 +03 57 18.98 22.4G 523748 F51 C~2kQv 2011 02 02.22715 04 05 12.596 +03 57 28.69 22.7G 523748 F51 C~2kQv 2011 09 14.56609 04 18 52.008 +04 29 05.51 22.5G 523748 F51 C~2kQv 2011 10 25.56113 04 17 13.790 +04 10 06.12 21.3G 523748 F51 C~2kQv 2011 12 01.33784 04 14 23.550 +03 57 47.63 21.9w 523748 F51 C~1vXm 2011 12 01.35169 04 14 23.480 +03 57 47.49 22.1w 523748 F51 C~1vXm 2011 12 01.36556 04 14 23.410 +03 57 47.35 22.0w 523748 F51 C~1vXm 2011 12 01.37940 04 14 23.345 +03 57 47.10 22.1w 523748 F51 C~1vXm 2012 10 20.54111 04 23 00.078 +04 15 33.52 22.2w 523748 F51 C~1vXm 2012 10 20.55552 04 23 00.050 +04 15 33.02 22.2w 523748 F51 C~1vXm 2012 10 20.56997 04 22 59.967 +04 15 32.52 22.1w 523748 F51 C~1vXm 2012 10 20.58439 04 22 59.939 +04 15 32.60 21.9w 523748 F51 C~1vXm 2012 11 08.55023 04 21 41.568 +04 07 49.79 21.7G 523748 F51 C~2kQv 2013 11 28.40589 04 25 39.399 +04 05 26.43 22.1w 523748 F51 C~1vXm 2013 11 28.41890 04 25 39.328 +04 05 26.33 21.8w 523748 F51 C~1vXm 2013 11 28.43192 04 25 39.260 +04 05 25.97 21.8w 523748 F51 C~1vXm 2013 11 28.44499 04 25 39.189 +04 05 25.99 21.9w 523748 F51 C~1vXm 2013 12 11.39096 04 24 35.093 +04 03 09.13 22.9G 523748 F51 C~2kQv 2014 09 18.61999 04 35 12.659 +04 37 12.15 22.2G 523748 F51 C~2kQv 2014 10 02.54958 04 34 54.274 +04 30 41.48 21.9G 523748 F51 C~2kQv 2014 10 02.57908 04 34 54.209 +04 30 40.52 22.1G 523748 F51 C~2kQv 2014 10 02.59390 04 34 54.193 +04 30 40.20 22.7G 523748 F51 C~2kQv 2014 10 26.55848 04 33 43.946 +04 19 48.63 22.3w 523748 F51 C~1vXm 2014 10 26.57092 04 33 43.914 +04 19 48.90 22.3w 523748 F51 C~1vXm 2014 10 26.58331 04 33 43.847 +04 19 48.19 21.8w 523748 F51 C~1vXm 2014 10 26.59575 04 33 43.785 +04 19 47.77 22.1w 523748 F51 C~1vXm 2014 11 11.51472 04 32 36.258 +04 13 39.24 22.9G 523748 F51 C~2kQv 2014 11 21.46933 04 31 48.745 +04 10 33.24 21.9w 523748 F51 C~1vXm 2014 11 21.48151 04 31 48.694 +04 10 32.84 22.1w 523748 F51 C~1vXm 2014 11 21.49362 04 31 48.637 +04 10 32.69 21.9w 523748 F51 C~1vXm 2014 11 21.50574 04 31 48.570 +04 10 32.44 22.0w 523748 F51 C~1vXm 2014 11 23.49694 04 31 38.771 +04 09 59.97 21.6G 523748 F51 C~2kQv 2014 12 15.35843 04 29 50.378 +04 06 03.72 21.4G 523748 F51 C~2kQv 2015 01 09.25981 04 28 02.858 +04 06 32.36 21.9w 523748 F51 C~1vXm 2015 01 09.27288 04 28 02.817 +04 06 32.36 21.9w 523748 F51 C~1vXm 2015 01 09.28597 04 28 02.776 +04 06 32.60 22.4w 523748 F51 C~1vXm 2015 01 09.29910 04 28 02.725 +04 06 32.66 22.1w 523748 F51 C~1vXm 2015 10 21.53993 04 39 36.460 +04 25 08.00 22.3G 523748 F51 C~2kQv 2015 10 21.55186 04 39 36.429 +04 25 07.64 22.3G 523748 F51 C~2kQv 2015 10 21.56374 04 39 36.372 +04 25 07.13 22.4G 523748 F51 C~2kQv 2015 10 21.57558 04 39 36.335 +04 25 06.82 21.9G 523748 F51 C~2kQv 2015 11 02.55195 04 38 51.149 +04 20 07.87 22.3G 523748 F51 C~2kQv 2015 11 02.57573 04 38 51.051 +04 20 07.26 22.2G 523748 F51 C~2kQv 2015 11 02.58758 04 38 50.998 +04 20 06.82 22.8G 523748 F51 C~2kQv 2015 11 03.52816 04 38 47.067 +04 19 45.04 22.1G 523748 F51 C~2kQv 2015 12 02.43196 04 36 30.238 +04 11 05.92 22.2G 523748 F51 C~2kQv 2016 10 13.56409 04 45 32.545 +04 31 14.26 22.2G 523748 F51 C~2kQv 2016 11 01.53440 04 44 27.382 +04 23 08.08 20.9G 523748 F51 C~2kQv 2017 01 21.27502 04 38 26.374 +04 14 57.99 21.9G 523748 F51 C~2kQv 2017 10 20.57060 04 50 47.462 +04 30 56.63 22.9G 523748 F51 C~2kQv 2017 11 17.45011 04 48 54.311 +04 20 27.02 21.5G 523748 F51 C~2kQv 2017 11 17.46152 04 48 54.266 +04 20 26.88 21.4G 523748 F51 C~2kQv 2017 11 17.47299 04 48 54.196 +04 20 26.28 22.0G 523748 F51 C~2kQv 2017 11 17.48448 04 48 54.163 +04 20 26.30 22.0G 523748 F51 C~2kQv 2017 12 23.31395 04 45 56.561 +04 14 35.58 21.8G 523748 F51 C~2kQv 2017 12 23.32531 04 45 56.507 +04 14 35.73 21.8G 523748 F51 C~2kQv 2017 12 23.33677 04 45 56.458 +04 14 35.59 22.0G 523748 F51 C~2kQv 2017 12 23.34829 04 45 56.401 +04 14 35.58 21.9G 523748 F51 C~2kQv 2018 01 06.36902 04 44 54.094 +04 15 15.53 22.1G 523748 F51 C~2kQv 2018 01 06.38119 04 44 54.045 +04 15 15.59 22.4G 523748 F51 C~2kQv 2018 01 06.39325 04 44 54.001 +04 15 15.74 22.1G 523748 F51 C~2kQv 2018 01 13.28909 04 44 27.319 +04 16 12.21 21.8G 523748 F51 C~2kQv 2018 01 13.30245 04 44 27.254 +04 16 12.22 20.9G 523748 F51 C~2kQv 2018 01 13.33038 04 44 27.163 +04 16 12.60 21.4G 523748 F51 C~2kQv 2019 01 11.129194 04 50 12.23 +04 18 33.9 22.1V 523748 H21 C~2u4S 2019 01 11.138543 04 50 12.17 +04 18 33.8 22.0V 523748 H21 C~2u4S 2019 01 11.158461 04 50 12.13 +04 18 34.6 22.4V 523748 H21 C~2u4S 2020 12 17.47002 05 03 21.212 +04 22 30.68 21.8w 523748 F51 C~4TuJ 2020 12 17.48072 05 03 21.158 +04 22 30.76 21.9w 523748 F51 C~4TuJ 2020 12 17.49144 05 03 21.117 +04 22 30.98 22.0w 523748 F51 C~4TuJ 2021 01 08.36598 05 01 38.322 +04 23 20.87 21.9w 523748 F51 C~4YAZ 2021 01 08.37720 05 01 38.272 +04 23 21.03 22.1w 523748 F51 C~4YAZ 2021 01 08.38835 05 01 38.216 +04 23 21.17 21.9w 523748 F51 C~4YAZ 2023 10 26.587884 05 24 31.120 +04 42 07.92 21.9w 523748 F51 C~7QqP 2023 10 26.599303 05 24 31.077 +04 42 07.82 22.0w 523748 F51 C~7QqP 2023 10 26.609807 05 24 31.023 +04 42 07.40 22.1w 523748 F51 C~7QqP 2023 10 26.620308 05 24 31.014 +04 42 07.14 22.1w 523748 F51 C~7QqP 2023 11 19.502252 05 22 58.402 +04 33 48.30 21.9w 523748 F51 C~7b10 2023 11 19.513990 05 22 58.356 +04 33 48.06 21.9w 523748 F51 C~7b10 2023 11 19.524688 05 22 58.277 +04 33 48.05 21.8w 523748 F51 C~7b10 2023 12 04.380063 05 21 46.186 +04 30 29.39 21.8w 523748 F52 C~7b10 2023 12 04.392911 05 21 46.120 +04 30 29.20 21.9w 523748 F52 C~7b10 2023 12 04.418613 05 21 45.983 +04 30 29.04 21.9w 523748 F52 C~7b10
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 -0.07 0.00 -0.09
2 0.0187 0.00 0.03 0.00 -0.13
3 0.2265 0.00 -0.03 0.00 0.06
4 0.8407 0.00 0.58 0.00 0.13
5 0.9529 0.00 0.16 0.00 -0.20
6 1.0536 0.00 -0.03 0.00 0.21
7 1.0536 0.00 -0.04 0.00 0.24
8 1.0537 0.00 -0.05 0.00 0.28
9 1.0537 0.00 0.02 0.00 0.20
10 1.9412 0.00 -0.17 0.00 -0.03
11 1.9413 0.00 0.20 0.00 -0.15
12 1.9413 0.00 -0.24 0.00 -0.26
13 1.9413 0.00 0.13 0.00 0.20
14 1.9933 0.00 -0.06 0.00 -0.16
15 3.0469 0.00 0.06 0.00 -0.08
16 3.0470 0.00 -0.02 0.00 -0.00
17 3.0470 0.00 -0.05 0.00 -0.19
18 3.0470 0.00 -0.12 0.00 0.01
19 3.0825 0.00 0.09 0.00 0.01
20 3.8524 0.00 0.06 0.00 -0.13
21 3.8906 0.00 -0.06 0.00 0.05
22 3.8907 0.00 -0.14 0.00 -0.08
23 3.8907 0.00 0.08 0.00 0.02
24 3.9563 0.00 -0.11 0.00 -0.12
25 3.9564 0.00 0.13 0.00 0.47
26 3.9564 0.00 -0.15 0.00 0.07
27 3.9564 0.00 -0.35 0.00 -0.04
28 4.0000 0.00 -0.14 0.00 -0.50
29 4.0273 0.00 -0.12 0.00 0.24
30 4.0273 0.00 0.02 0.00 0.04
31 4.0273 0.00 0.07 0.00 0.09
32 4.0274 0.00 -0.02 0.00 0.05
33 4.0328 0.00 0.03 0.00 0.10
34 4.0927 0.00 0.02 0.00 -0.20
35 4.1608 0.00 -0.29 0.00 0.02
36 4.1609 0.00 -0.18 0.00 -0.08
37 4.1609 0.00 -0.06 0.00 0.06
38 4.1609 0.00 -0.09 0.00 0.02
39 4.9419 0.00 -0.10 0.00 0.13
40 4.9419 0.00 0.05 0.00 0.08
41 4.9420 0.00 -0.18 0.00 -0.12
42 4.9420 0.00 -0.12 0.00 -0.12
43 4.9748 0.00 0.11 0.00 -0.03
44 4.9748 0.00 0.14 0.00 -0.08
45 4.9749 0.00 0.10 0.00 -0.24
46 4.9775 0.00 -0.14 0.00 -0.08
47 5.0566 0.00 0.02 0.00 0.17
48 5.9221 0.00 0.00 0.00 0.02
49 5.9740 0.00 0.36 0.00 -0.04
50 6.1951 0.00 0.28 0.00 0.03
51 6.9406 0.00 -0.11 0.00 0.17
52 7.0169 0.00 -0.01 0.00 0.27
53 7.0170 0.00 0.15 0.00 0.34
54 7.0170 0.00 -0.07 0.00 -0.05
55 7.0170 0.00 0.27 0.00 0.17
56 7.1151 0.00 -0.07 0.00 -0.06
57 7.1152 0.00 -0.05 0.00 0.10
58 7.1152 0.00 0.04 0.00 -0.03
59 7.1152 0.00 0.02 0.00 -0.03
60 7.1536 0.00 -0.11 0.00 -0.11
61 7.1536 0.00 -0.08 0.00 -0.13
62 7.1537 0.00 0.01 0.00 -0.05
63 7.1726 0.00 0.08 0.00 -0.24
64 7.1726 0.00 -0.15 0.00 -0.36
65 7.1727 0.00 0.05 0.00 -0.26
66 8.1660 0.00 0.21 0.00 -0.02
67 8.1660 0.00 -0.13 0.00 -0.20
68 8.1660 0.00 0.45 0.00 0.42
69 10.0998 0.00 -0.04 0.00 -0.13
70 10.0998 0.00 -0.02 0.00 -0.01
71 10.0999 0.00 0.18 0.00 0.25
72 10.1598 0.00 0.05 0.00 0.04
73 10.1598 0.00 0.02 0.00 0.11
74 10.1598 0.00 -0.10 0.00 0.16
75 12.9557 0.00 0.05 0.00 -0.13
76 12.9557 0.00 -0.06 0.00 0.05
77 12.9558 0.00 -0.37 0.00 -0.12
78 12.9558 0.00 -0.02 0.00 -0.12
79 13.0212 0.00 0.12 0.00 -0.03
80 13.0212 0.00 0.25 0.00 -0.08
81 13.0213 0.00 -0.18 0.00 0.09
82 13.0619 0.00 0.01 0.00 0.07
83 13.0620 0.00 0.02 0.00 0.01
84 13.0620 0.00 -0.06 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.
523748 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 41.130 41.129 41.130 ecceobj 0.081 0.081 0.081 incobj 18.337 18.337 18.337 qmin 36.465 36.456 36.462 qmax 45.545 45.533 45.495 amean 40.873 40.874 40.872 amin 40.553 40.553 40.553 amax 41.210 41.208 41.206 emean 0.090 0.090 0.090 emin 0.075 0.075 0.075 emax 0.105 0.106 0.105 imean 18.446 18.446 18.446 imin 17.682 17.695 17.700 imax 19.230 19.228 19.231 excite_mean 0.329 0.329 0.329 fracstop 1.000 1.000 1.000 cjmean 2.938 2.938 2.938 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 173.0 173.2 173.2 kozaiamp 180.0 180.0 180.0