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: 542889 # Created Fri Nov 22 02:07:31 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 97 observations of 97 # Arc: 11.01y # First observation: 2010/08/01 # Last observation: 2021/08/05 # Chi-squared of fit: 62.72 DOF: 188 RMS: 0.14 # Min/Max residuals: -0.64 0.34 # Exact a, adot, b, bdot, g, gdot: 2.615845E-05 8.049981E-02 -6.293572E-06 -2.032877E-02 4.866078E-02 -1.967151E-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 -3.519429 -67.988535 -0.291266 -0.059492 -0.966376 2455409.879976 # Heliocentric elements and errors Epoch: 2455410.5000 = 2010/08/02 Mean Anomaly: 359.60983 +/- 0.000 Argument of Peri: 195.42421 +/- 0.000 Long of Asc Node: 99.67479 +/- 0.000 Inclination: 14.50034 +/- 0.000 Eccentricity: 0.59041112 +/- 0.0000 Semi-Major Axis: 52.53486161 +/- 0.0000 Time of Perihelion: 2455561.2385 +/- 0.0 Perihelion: 21.51769490 +/- 0.0000 Aphelion: 83.55202833 +/- 0.0000 Period (y) 380.7848 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 8.32518578 +/- 0.0000 Ecliptic Y -19.80648376 +/- 0.0000 Ecliptic Z -1.26161626 +/- 0.0000 Ecliptic XDOT 0.00413235 +/- 0.0000 Ecliptic YDOT 0.00187126 +/- 0.0000 Ecliptic ZDOT -0.00113486 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 21.52202320 +/- 0.0000 Geocenter to KBO 20.55047651 +/- 0.0000 # Hcoef: 8.38
The following table shows the complete astrometric record for 542889. 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 (542889) followed by the observatory code and reference code for the source of the astrometry.
2010 08 01.37921 19 37 36.522 -25 06 47.67 21.6G 542889 F51 C~2kP3 2010 08 05.40122 19 37 03.305 -25 08 35.11 21.1G 542889 F51 C~2kP3 2011 07 19.48516 20 00 33.373 -25 17 11.06 21.6G 542889 F51 C~2kP3 2011 07 21.48263 20 00 15.749 -25 18 23.49 21.3G 542889 F51 C~2kP3 2011 07 28.38496 19 59 14.934 -25 22 21.45 21.5G 542889 F51 C~2kP3 2011 07 28.39440 19 59 14.845 -25 22 21.60 21.4G 542889 F51 C~2kP3 2011 07 31.40376 19 58 48.651 -25 24 00.35 21.8w 542889 F51 C~1vWz 2011 07 31.41857 19 58 48.514 -25 24 01.13 21.6w 542889 F51 C~1vWz 2011 07 31.44819 19 58 48.265 -25 24 01.97 21.4w 542889 F51 C~1vWz 2011 08 01.38400 19 58 40.199 -25 24 32.31 22.3G 542889 F51 C~2kP3 2011 08 16.37181 19 56 37.963 -25 31 42.24 21.3G 542889 F51 C~2kP3 2012 06 16.53523 20 25 40.415 -25 00 18.80 22.1G 542889 F51 C~2kP3 2012 06 16.54914 20 25 40.325 -25 00 19.45 22.1G 542889 F51 C~2kP3 2012 06 16.57697 20 25 40.162 -25 00 20.66 21.0G 542889 F51 C~2kP3 2012 07 28.42823 20 20 10.806 -25 29 16.52 21.3G 542889 F51 C~2kP3 2012 08 11.36121 20 18 11.670 -25 37 20.96 21.6G 542889 F51 C~2kP3 2013 06 30.48163 20 44 50.030 -25 03 27.00 21.7r 542889 F51 C~1vWz 2013 06 30.49132 20 44 49.968 -25 03 27.47 21.6r 542889 F51 C~1vWz 2013 06 30.50250 20 44 49.888 -25 03 28.04 21.3i 542889 F51 C~1vWz 2013 06 30.51351 20 44 49.790 -25 03 28.59 21.6i 542889 F51 C~1vWz 2013 07 08.48606 20 43 51.298 -25 09 37.76 22.6G 542889 F51 C~2kP3 2013 07 13.47486 20 43 11.944 -25 13 27.62 21.6w 542889 F51 C~1vWz 2013 07 13.49442 20 43 11.787 -25 13 28.54 21.8w 542889 F51 C~1vWz 2013 07 13.50903 20 43 11.677 -25 13 29.23 21.7w 542889 F51 C~1vWz 2013 07 14.47250 20 43 03.870 -25 14 13.23 21.4G 542889 F51 C~2kP3 2013 07 17.46702 20 42 39.263 -25 16 29.47 21.8G 542889 F51 C~2kP3 2013 07 17.47737 20 42 39.171 -25 16 29.91 21.5G 542889 F51 C~2kP3 2013 07 18.45863 20 42 31.006 -25 17 14.21 21.7G 542889 F51 C~2kP3 2013 07 18.46855 20 42 30.928 -25 17 14.54 21.6G 542889 F51 C~2kP3 2013 08 02.40074 20 40 23.074 -25 27 55.67 21.6w 542889 F51 C~1vWz 2013 08 02.41438 20 40 22.952 -25 27 56.25 21.7w 542889 F51 C~1vWz 2013 08 02.42803 20 40 22.824 -25 27 57.06 22.1w 542889 F51 C~1vWz 2013 08 02.44169 20 40 22.709 -25 27 57.28 21.6w 542889 F51 C~1vWz 2013 08 23.39768 20 37 29.235 -25 40 09.34 22.0G 542889 F51 C~2kP3 2013 08 26.34609 20 37 07.089 -25 41 31.56 21.9G 542889 F51 C~2kP3 2014 06 13.59609 21 06 37.742 -24 33 18.14 22.1G 542889 F51 C~2kP3 2014 07 27.43149 21 01 49.931 -25 08 14.92 21.7w 542889 F51 C~1vWz 2014 07 27.44341 21 01 49.826 -25 08 15.50 21.6w 542889 F51 C~1vWz 2014 07 27.45531 21 01 49.726 -25 08 15.96 21.5w 542889 F51 C~1vWz 2014 07 27.46721 21 01 49.633 -25 08 16.54 21.5w 542889 F51 C~1vWz 2014 07 29.45300 21 01 32.930 -25 09 48.89 21.5w 542889 F51 C~1vWz 2014 07 29.46355 21 01 32.843 -25 09 49.05 21.4w 542889 F51 C~1vWz 2014 07 29.47409 21 01 32.750 -25 09 49.67 21.7w 542889 F51 C~1vWz 2014 07 29.48462 21 01 32.658 -25 09 50.20 21.7w 542889 F51 C~1vWz 2014 07 30.39037 21 01 25.029 -25 10 31.71 21.6w 542889 F51 C~1vWz 2014 07 30.40227 21 01 24.927 -25 10 32.25 21.7w 542889 F51 C~1vWz 2014 07 30.41418 21 01 24.815 -25 10 32.78 21.6w 542889 F51 C~1vWz 2014 07 30.42611 21 01 24.726 -25 10 33.33 21.6w 542889 F51 C~1vWz 2014 07 30.47505 21 01 24.304 -25 10 35.46 21.7w 542889 F51 C~1vWz 2014 07 30.48584 21 01 24.203 -25 10 35.99 21.6w 542889 F51 C~1vWz 2014 07 30.49665 21 01 24.102 -25 10 36.54 21.6w 542889 F51 C~1vWz 2014 07 30.50744 21 01 24.009 -25 10 37.05 21.6w 542889 F51 C~1vWz 2014 08 22.38689 20 58 12.102 -25 26 00.36 21.9w 542889 F51 C~1vWz 2014 08 22.39837 20 58 12.018 -25 26 00.66 21.7w 542889 F51 C~1vWz 2014 08 22.40983 20 58 11.928 -25 26 01.04 21.8w 542889 F51 C~1vWz 2014 08 22.42128 20 58 11.831 -25 26 01.48 21.7w 542889 F51 C~1vWz 2014 09 13.29780 20 55 37.944 -25 35 23.29 21.8G 542889 F51 C~2kP3 2014 09 13.30879 20 55 37.887 -25 35 23.48 21.8G 542889 F51 C~2kP3 2014 09 28.25835 20 54 27.163 -25 38 01.49 21.7w 542889 F51 C~1vWz 2014 09 28.27064 20 54 27.100 -25 38 01.63 21.9w 542889 F51 C~1vWz 2014 09 28.28299 20 54 27.061 -25 38 01.66 21.9w 542889 F51 C~1vWz 2014 09 28.29557 20 54 27.002 -25 38 01.67 22.0w 542889 F51 C~1vWz 2015 06 29.53866 21 25 08.192 -24 18 49.80 21.6i 542889 F51 C~1vX0 2015 06 29.56068 21 25 08.075 -24 18 50.73 21.6i 542889 F51 C~1vX0 2015 06 29.57168 21 25 08.006 -24 18 51.29 21.6i 542889 F51 C~1vX0 2015 06 30.55657 21 25 02.696 -24 19 40.86 22.3G 542889 F51 C~2kP3 2015 08 16.37995 21 19 11.550 -24 58 10.98 22.4G 542889 F51 C~2kP3 2016 07 08.51958 21 43 29.208 -23 52 01.60 22.2G 542889 F51 C~2kP3 2016 07 08.52966 21 43 29.167 -23 52 01.76 22.2G 542889 F51 C~2kP3 2016 07 08.54980 21 43 29.046 -23 52 03.03 22.3G 542889 F51 C~2kP3 2016 08 10.43112 21 39 28.901 -24 20 47.69 21.8G 542889 F51 C~2kP3 2016 08 10.44144 21 39 28.827 -24 20 48.18 22.1G 542889 F51 C~2kP3 2016 08 10.45175 21 39 28.732 -24 20 48.50 22.0G 542889 F51 C~2kP3 2016 08 10.46206 21 39 28.659 -24 20 49.16 21.7G 542889 F51 C~2kP3 2017 07 25.46815 22 00 24.134 -23 24 32.82 22.2G 542889 F51 C~2kP3 2017 07 25.47836 22 00 24.046 -23 24 33.45 21.9G 542889 F51 C~2kP3 2017 07 25.48857 22 00 23.971 -23 24 34.18 22.1G 542889 F51 C~2kP3 2017 07 25.49879 22 00 23.898 -23 24 34.44 21.7G 542889 F51 C~2kP3 2017 08 18.43666 21 57 20.531 -23 45 28.40 22.0G 542889 F51 C~2kP3 2017 08 18.44780 21 57 20.433 -23 45 28.90 21.9G 542889 F51 C~2kP3 2017 08 18.45904 21 57 20.351 -23 45 29.35 22.0G 542889 F51 C~2kP3 2017 08 18.47027 21 57 20.270 -23 45 29.73 21.9G 542889 F51 C~2kP3 2017 09 26.32989 21 52 36.538 -24 06 58.70 23.3G 542889 F51 C~2kP3 2017 12 08.22411 21 52 51.025 -23 41 34.27 21.6G 542889 F51 C~2kP3 2018 08 13.48087 22 16 12.329 -22 52 40.81 22.1w 542889 F51 C~2j3i 2018 08 13.49186 22 16 12.211 -22 52 41.52 22.1w 542889 F51 C~2j3i 2018 08 13.51383 22 16 12.028 -22 52 42.64 22.1w 542889 F51 C~2j3i 2020 08 16.47945 22 49 44.889 -21 02 51.32 22.1w 542889 F51 C~46mO 2020 08 16.49107 22 49 44.825 -21 02 52.07 21.9w 542889 F51 C~46mO 2020 08 16.50271 22 49 44.740 -21 02 52.75 21.9w 542889 F51 C~46mO 2020 08 16.51432 22 49 44.645 -21 02 53.17 22.0w 542889 F51 C~46mO 2020 10 16.27320 22 42 51.064 -21 37 31.58 21.8w 542889 F51 C~4InD 2020 10 16.28485 22 42 51.018 -21 37 31.62 22.3w 542889 F51 C~4InD 2020 10 16.30814 22 42 50.890 -21 37 31.76 22.2w 542889 F51 C~4InD 2021 08 05.526488 23 06 42.275 -19 50 09.19 22.1w 542889 F51 C~4yBb 2021 08 05.536892 23 06 42.230 -19 50 09.57 22.0w 542889 F51 C~4yBb 2021 08 05.557666 23 06 42.088 -19 50 10.89 21.9w 542889 F51 C~4yBb
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 -0.06
2 0.0110 0.00 -0.00 0.00 0.31
3 0.9640 0.00 -0.07 0.00 0.23
4 0.9695 0.00 0.23 0.00 -0.64
5 0.9884 0.00 -0.07 0.00 -0.19
6 0.9884 0.00 -0.14 0.00 -0.02
7 0.9966 0.00 0.00 0.00 0.19
8 0.9967 0.00 -0.09 0.00 -0.11
9 0.9968 0.00 0.10 0.00 -0.00
10 0.9993 0.00 0.14 0.00 -0.27
11 1.0404 0.00 0.26 0.00 0.07
12 1.8759 0.00 0.05 0.00 0.14
13 1.8759 0.00 -0.02 0.00 0.06
14 1.8760 0.00 0.11 0.00 -0.01
15 1.9906 0.00 -0.17 0.00 0.07
16 2.0287 0.00 -0.36 0.00 -0.08
17 2.9134 0.00 0.09 0.00 0.07
18 2.9134 0.00 0.19 0.00 0.05
19 2.9134 0.00 0.18 0.00 -0.00
20 2.9134 0.00 -0.11 0.00 -0.05
21 2.9353 0.00 -0.32 0.00 -0.16
22 2.9489 0.00 -0.01 0.00 -0.02
23 2.9490 0.00 0.05 0.00 -0.04
24 2.9490 0.00 0.21 0.00 -0.06
25 2.9517 0.00 0.10 0.00 0.05
26 2.9599 0.00 0.10 0.00 -0.03
27 2.9599 0.00 0.04 0.00 -0.01
28 2.9626 0.00 0.01 0.00 -0.05
29 2.9626 0.00 0.11 0.00 0.07
30 3.0035 0.00 0.06 0.00 -0.01
31 3.0035 0.00 0.04 0.00 -0.04
32 3.0036 0.00 -0.07 0.00 -0.30
33 3.0036 0.00 0.01 0.00 0.03
34 3.0610 0.00 0.09 0.00 -0.09
35 3.0690 0.00 -0.11 0.00 -0.38
36 3.8664 0.00 0.01 0.00 0.25
37 3.9865 0.00 -0.06 0.00 -0.04
38 3.9865 0.00 -0.11 0.00 -0.06
39 3.9865 0.00 -0.08 0.00 0.03
40 3.9866 0.00 0.05 0.00 0.01
41 3.9920 0.00 -0.08 0.00 -0.19
42 3.9920 0.00 -0.03 0.00 0.14
43 3.9920 0.00 -0.06 0.00 0.00
44 3.9921 0.00 -0.08 0.00 -0.04
45 3.9946 0.00 0.02 0.00 0.02
46 3.9946 0.00 0.03 0.00 0.03
47 3.9946 0.00 -0.11 0.00 0.05
48 3.9947 0.00 0.10 0.00 0.05
49 3.9948 0.00 0.11 0.00 0.16
50 3.9948 0.00 -0.00 0.00 0.12
51 3.9948 0.00 -0.12 0.00 0.06
52 3.9949 0.00 -0.11 0.00 0.04
53 4.0575 0.00 -0.25 0.00 0.01
54 4.0575 0.00 -0.10 0.00 0.10
55 4.0576 0.00 -0.04 0.00 0.11
56 4.0576 0.00 -0.10 0.00 0.05
57 4.1175 0.00 0.04 0.00 0.19
58 4.1175 0.00 0.18 0.00 0.19
59 4.1585 0.00 0.11 0.00 0.19
60 4.1585 0.00 -0.15 0.00 0.10
61 4.1585 0.00 -0.04 0.00 0.12
62 4.1586 0.00 -0.22 0.00 0.16
63 4.9094 0.00 0.03 0.00 0.04
64 4.9095 0.00 0.09 0.00 0.21
65 4.9095 0.00 -0.03 0.00 0.20
66 4.9122 0.00 0.08 0.00 -0.11
67 5.0404 0.00 0.14 0.00 -0.08
68 5.9360 0.00 -0.35 0.00 -0.37
69 5.9361 0.00 -0.05 0.00 0.00
70 5.9361 0.00 -0.05 0.00 -0.20
71 6.0262 0.00 -0.00 0.00 -0.05
72 6.0262 0.00 0.18 0.00 -0.04
73 6.0262 0.00 0.05 0.00 0.14
74 6.0262 0.00 0.25 0.00 -0.03
75 6.9818 0.00 0.23 0.00 0.13
76 6.9818 0.00 0.00 0.00 0.06
77 6.9818 0.00 -0.03 0.00 -0.10
78 6.9818 0.00 -0.03 0.00 0.20
79 7.0474 0.00 0.10 0.00 -0.11
80 7.0474 0.00 0.01 0.00 -0.08
81 7.0474 0.00 0.16 0.00 0.01
82 7.0475 0.00 0.34 0.00 0.16
83 7.1539 0.00 0.23 0.00 0.03
84 7.3534 0.00 -0.14 0.00 -0.04
85 8.0331 0.00 0.29 0.00 0.01
86 8.0332 0.00 -0.18 0.00 -0.12
87 8.0332 0.00 -0.34 0.00 -0.09
88 10.0427 0.00 -0.17 0.00 -0.04
89 10.0427 0.00 0.14 0.00 -0.16
90 10.0428 0.00 0.14 0.00 -0.20
91 10.0428 0.00 -0.02 0.00 0.02
92 10.2092 0.00 -0.01 0.00 -0.07
93 10.2092 0.00 0.14 0.00 -0.05
94 10.2093 0.00 -0.12 0.00 -0.07
95 11.0120 0.00 -0.17 0.00 -0.00
96 11.0121 0.00 0.09 0.00 0.21
97 11.0121 0.00 -0.18 0.00 0.07
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.
542889 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 51.659 51.658 51.659 ecceobj 0.584 0.584 0.584 incobj 14.519 14.519 14.519 qmin 21.314 21.314 21.314 qmax 85.262 85.810 87.634 amean 51.614 51.897 53.033 amin 50.227 50.511 51.588 amax 53.434 54.256 55.049 emean 0.576 0.572 0.586 emin 0.553 0.556 0.573 emax 0.596 0.597 0.598 imean 14.161 14.824 14.193 imin 12.860 12.860 12.861 imax 16.074 15.800 15.959 excite_mean 0.626 0.627 0.636 fracstop 0.040 0.083 0.043 cjmean 2.658 2.663 2.651 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 220.5 241.5 222.9 kozaiamp 23.9 43.0 25.6