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: 679338
# Created Wed May 8 01:09:39 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 85 observations of 85
# Arc: 10.40y
# First observation: 2013/09/14
# Last observation: 2024/02/09
# Chi-squared of fit: 82.67 DOF: 164 RMS: 0.17
# Min/Max residuals: -0.49 0.75
# Exact a, adot, b, bdot, g, gdot:
2.564470E-05 7.406112E-02 5.014526E-06 1.210200E-02 4.830555E-02 3.740385E-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
7.278911 104.515710 0.927140 -0.049546 0.388504 2456550.104856
# Heliocentric elements and errors
Epoch: 2456550.5000 = 2013/09/15
Mean Anomaly: 0.87038 +/- 0.000
Argument of Peri: 36.48755 +/- 0.000
Long of Asc Node: 64.52262 +/- 0.000
Inclination: 12.09790 +/- 0.000
Eccentricity: 0.25006198 +/- 0.0000
Semi-Major Axis: 27.11600364 +/- 0.0000
Time of Perihelion: 2456425.8065 +/- 0.0
Perihelion: 20.33532209 +/- 0.0000
Aphelion: 33.89668519 +/- 0.0000
Period (y) 141.2039 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -4.15205605 +/- 0.0000
Ecliptic Y 19.73479007 +/- 0.0000
Ecliptic Z 2.62298177 +/- 0.0000
Ecliptic XDOT -0.00410073 +/- 0.0000
Ecliptic YDOT -0.00093387 +/- 0.0000
Ecliptic ZDOT 0.00070739 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 20.33670166 +/- 0.0000
Geocenter to KBO 20.70154780 +/- 0.0000
# Hcoef: 9.43
The following table shows the complete astrometric record for 679338. 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 (679338) followed by the observatory code and reference code for the source of the astrometry.
2013 09 14.604078 07 06 39.218 +29 52 56.52 22.4G 679338 F51 C~2sdL 2013 09 14.609670 07 06 39.291 +29 52 56.83 22.7G 679338 F51 C~2sdL 2013 09 14.615293 07 06 39.326 +29 52 56.71 22.3G 679338 F51 C~2sdL 2013 09 14.620899 07 06 39.375 +29 52 56.92 22.1G 679338 F51 C~2sdL 2013 11 25.533406 07 07 18.674 +30 25 58.93 22.4G 679338 F51 C~2sdL 2013 11 25.546275 07 07 18.564 +30 25 59.58 22.8G 679338 F51 C~2sdL 2013 11 27.606615 07 07 03.608 +30 27 10.01 23.6G 679338 F51 C~2sdL 2013 11 28.549352 07 06 56.598 +30 27 42.52 22.8G 679338 F51 C~2sdL 2013 12 04.429716 07 06 09.332 +30 31 00.70 23.2G 679338 F51 C~2sdL 2013 12 04.443666 07 06 09.229 +30 31 01.30 22.7G 679338 F51 C~2sdL 2013 12 04.457661 07 06 09.094 +30 31 01.75 22.7G 679338 F51 C~2sdL 2013 12 04.471646 07 06 08.996 +30 31 02.25 22.9G 679338 F51 C~2sdL 2013 12 26.374313 07 02 35.763 +30 42 05.90 22.1G 679338 F51 C~2sdL 2013 12 26.389732 07 02 35.603 +30 42 06.35 22.2G 679338 F51 C~2sdL 2013 12 26.405170 07 02 35.423 +30 42 06.57 22.0G 679338 F51 C~2sdL 2015 01 18.292597 07 19 57.459 +31 01 03.34 22.4G 679338 F51 C~2sdL 2015 01 18.319164 07 19 57.184 +31 01 03.71 22.7G 679338 F51 C~2sdL 2015 01 18.332524 07 19 57.038 +31 01 04.12 22.6G 679338 F51 C~2sdL 2016 01 02.569558 07 44 09.456 +30 50 32.27 22.8G 679338 F51 C~2sdL 2016 01 07.346094 07 43 19.516 +30 53 20.14 23.3G 679338 F51 C~2sdL 2016 01 07.356457 07 43 19.423 +30 53 20.82 22.4G 679338 F51 C~2sdL 2016 01 07.366801 07 43 19.314 +30 53 21.21 22.4G 679338 F51 C~2sdL 2016 01 07.377143 07 43 19.192 +30 53 21.37 22.7G 679338 F51 C~2sdL 2017 01 06.400837 08 04 29.504 +30 37 13.86 21.9G 679338 F51 C~2sdL 2017 01 06.443037 08 04 29.042 +30 37 15.62 22.8G 679338 F51 C~2sdL 2017 01 06.460291 08 04 28.884 +30 37 16.72 22.8G 679338 F51 C~2sdL 2017 01 06.519783 08 04 28.280 +30 37 18.70 22.6G 679338 F51 C~2sdL 2017 01 06.546014 08 04 28.006 +30 37 19.91 21.6G 679338 F51 C~2sdL 2017 01 06.576292 08 04 27.682 +30 37 21.01 22.5G 679338 F51 C~2sdL 2017 01 06.604641 08 04 27.393 +30 37 22.14 22.5G 679338 F51 C~2sdL 2017 01 08.344018 08 04 09.575 +30 38 31.42 21.8G 679338 F51 C~2sdL 2017 01 08.435984 08 04 08.676 +30 38 34.92 22.7G 679338 F51 C~2sdL 2017 01 08.533464 08 04 07.621 +30 38 38.68 22.1G 679338 F51 C~2sdL 2017 01 08.597479 08 04 06.908 +30 38 41.29 21.3G 679338 F51 C~2sdL 2017 01 08.641467 08 04 06.459 +30 38 42.57 22.1G 679338 F51 C~2sdL 2017 01 09.345690 08 03 59.213 +30 39 10.25 22.3G 679338 F51 C~2sdL 2017 01 09.434859 08 03 58.307 +30 39 13.93 21.7G 679338 F51 C~2sdL 2017 01 09.589535 08 03 56.681 +30 39 19.28 20.9G 679338 F51 C~2sdL 2017 01 09.607846 08 03 56.489 +30 39 20.28 22.2G 679338 F51 C~2sdL 2017 01 10.372472 08 03 48.581 +30 39 49.80 22.2G 679338 F51 C~2sdL 2017 01 10.395781 08 03 48.334 +30 39 50.70 21.9G 679338 F51 C~2sdL 2017 01 10.434791 08 03 47.928 +30 39 52.34 22.1G 679338 F51 C~2sdL 2017 01 10.452579 08 03 47.709 +30 39 52.84 22.4G 679338 F51 C~2sdL 2017 01 10.535969 08 03 46.855 +30 39 56.20 22.1G 679338 F51 C~2sdL 2017 01 10.562234 08 03 46.581 +30 39 56.61 20.4G 679338 F51 C~2sdL 2017 01 10.646303 08 03 45.675 +30 40 00.05 23.0G 679338 F51 C~2sdL 2017 01 18.337282 08 02 24.855 +30 44 36.71 21.5G 679338 F51 C~2sdL 2017 01 18.465181 08 02 23.474 +30 44 40.71 21.4G 679338 F51 C~2sdL 2017 01 18.486849 08 02 23.245 +30 44 41.93 22.2G 679338 F51 C~2sdL 2017 01 29.341447 08 00 29.361 +30 50 06.51 22.7G 679338 F51 C~2sdL 2017 01 29.353596 08 00 29.232 +30 50 06.83 22.2G 679338 F51 C~2sdL 2017 01 29.365646 08 00 29.126 +30 50 07.16 22.8G 679338 F51 C~2sdL 2017 11 21.533022 08 30 15.453 +29 32 51.53 22.9G 679338 F51 C~2sdL 2017 11 21.544488 08 30 15.435 +29 32 52.12 22.9G 679338 F51 C~2sdL 2017 11 21.555945 08 30 15.406 +29 32 52.52 22.6G 679338 F51 C~2sdL 2017 11 21.567440 08 30 15.388 +29 32 53.06 22.9G 679338 F51 C~2sdL 2018 01 11.554693 08 24 26.724 +30 12 39.38 22.6G 679338 F51 C~2sdL 2018 01 11.566295 08 24 26.594 +30 12 40.21 22.0G 679338 F51 C~2sdL 2018 01 13.398902 08 24 08.144 +30 13 58.94 22.6G 679338 F51 C~2sdL 2018 01 13.410582 08 24 08.006 +30 13 59.58 22.3G 679338 F51 C~2sdL 2018 01 13.422334 08 24 07.881 +30 13 59.94 22.4G 679338 F51 C~2sdL 2018 01 13.434175 08 24 07.761 +30 14 00.29 22.4G 679338 F51 C~2sdL 2018 02 13.273632 08 18 54.094 +30 30 41.38 22.6G 679338 F51 C~2sdL 2018 02 13.296473 08 18 53.903 +30 30 42.05 23.5G 679338 F51 C~2sdL 2018 12 14.61455 08 48 28.859 +29 09 29.43 23.1G 679338 F51 C~2sJf 2018 12 14.62615 08 48 28.777 +29 09 29.90 22.2G 679338 F51 C~2sJf 2018 12 14.63781 08 48 28.688 +29 09 30.60 22.1G 679338 F51 C~2sJf 2018 12 14.64946 08 48 28.618 +29 09 31.27 22.1G 679338 F51 C~2sJf 2018 12 31.42620 08 46 28.222 +29 23 54.37 22.1G 679338 F51 C~2sJf 2018 12 31.43858 08 46 28.131 +29 23 55.07 22.4G 679338 F51 C~2sJf 2018 12 31.45099 08 46 27.994 +29 23 55.63 22.1G 679338 F51 C~2sJf 2018 12 31.46351 08 46 27.881 +29 23 56.34 22.3G 679338 F51 C~2sJf 2019 01 08.53073 08 45 16.346 +29 30 44.43 22.4w 679338 F51 C~2sJf 2019 01 08.54278 08 45 16.231 +29 30 45.07 23.0w 679338 F51 C~2sJf 2019 01 08.55483 08 45 16.133 +29 30 45.70 22.6w 679338 F51 C~2sJf 2019 01 08.56695 08 45 16.016 +29 30 46.12 22.9w 679338 F51 C~2sJf 2019 01 09.508957 08 45 07.226 +29 31 32.77 22.5G 679338 568 C~2sJf 2019 01 09.510157 08 45 07.213 +29 31 32.83 22.4G 679338 568 C~2sJf 2019 01 09.511343 08 45 07.203 +29 31 32.91 22.5G 679338 568 C~2sJf 2020 12 23.49408 09 25 46.430 +27 27 07.75 22.5w 679338 F51 C~4OHE 2020 12 23.50534 09 25 46.364 +27 27 08.44 22.7w 679338 F51 C~4OHE 2020 12 23.52743 09 25 46.222 +27 27 09.82 22.3w 679338 F51 C~4OHE 2024 02 09.396880 10 12 47.792 +24 29 45.81 22.4w 679338 F52 C~7n6c 2024 02 09.409799 10 12 47.666 +24 29 46.90 22.2w 679338 F52 C~7n6c 2024 02 09.422730 10 12 47.557 +24 29 47.40 22.4w 679338 F52 C~7n6c
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 -0.36 0.00 -0.18
2 0.0000 0.00 0.05 0.00 0.04
3 0.0000 0.00 -0.11 0.00 -0.17
4 0.0000 0.00 -0.06 0.00 -0.04
5 0.1969 0.00 0.31 0.00 0.05
6 0.1970 0.00 0.06 0.00 0.26
7 0.2026 0.00 -0.49 0.00 -0.01
8 0.2052 0.00 0.12 0.00 0.25
9 0.2213 0.00 -0.12 0.00 -0.12
10 0.2213 0.00 0.15 0.00 0.01
11 0.2214 0.00 -0.05 0.00 -0.02
12 0.2214 0.00 0.30 0.00 0.01
13 0.2814 0.00 0.04 0.00 0.02
14 0.2814 0.00 0.14 0.00 0.06
15 0.2815 0.00 -0.05 0.00 -0.14
16 1.3434 0.00 -0.09 0.00 0.11
17 1.3435 0.00 0.08 0.00 -0.10
18 1.3435 0.00 0.06 0.00 0.02
19 2.2997 0.00 0.02 0.00 -0.07
20 2.3128 0.00 -0.07 0.00 -0.20
21 2.3128 0.00 0.20 0.00 0.12
22 2.3128 0.00 0.24 0.00 0.15
23 2.3129 0.00 0.07 0.00 -0.05
24 3.3122 0.00 -0.05 0.00 -0.21
25 3.3124 0.00 -0.40 0.00 -0.16
26 3.3124 0.00 -0.07 0.00 0.24
27 3.3126 0.00 0.15 0.00 -0.16
28 3.3126 0.00 0.14 0.00 0.01
29 3.3127 0.00 -0.01 0.00 -0.08
30 3.3128 0.00 0.07 0.00 -0.06
31 3.3176 0.00 -0.23 0.00 0.26
32 3.3178 0.00 0.75 0.00 0.10
33 3.3181 0.00 0.30 0.00 0.05
34 3.3183 0.00 -0.33 0.00 0.21
35 3.3184 0.00 -0.17 0.00 -0.19
36 3.3203 0.00 -0.45 0.00 0.04
37 3.3205 0.00 0.05 0.00 0.21
38 3.3210 0.00 0.14 0.00 -0.36
39 3.3210 0.00 0.15 0.00 -0.05
40 3.3231 0.00 -0.06 0.00 0.05
41 3.3232 0.00 -0.07 0.00 0.05
42 3.3233 0.00 0.04 0.00 0.18
43 3.3233 0.00 -0.41 0.00 -0.00
44 3.3236 0.00 0.04 0.00 0.20
45 3.3236 0.00 0.10 0.00 -0.38
46 3.3239 0.00 -0.21 0.00 -0.05
47 3.3449 0.00 -0.27 0.00 0.05
48 3.3453 0.00 -0.32 0.00 -0.30
49 3.3453 0.00 -0.25 0.00 0.20
50 3.3751 0.00 -0.02 0.00 -0.05
51 3.3751 0.00 -0.04 0.00 -0.05
52 3.3751 0.00 0.27 0.00 -0.04
53 4.1860 0.00 -0.20 0.00 -0.03
54 4.1860 0.00 -0.05 0.00 0.08
55 4.1860 0.00 -0.06 0.00 -0.01
56 4.1861 0.00 0.09 0.00 0.05
57 4.3257 0.00 -0.11 0.00 -0.10
58 4.3257 0.00 -0.28 0.00 0.24
59 4.3307 0.00 0.41 0.00 0.06
60 4.3308 0.00 0.15 0.00 0.19
61 4.3308 0.00 0.10 0.00 0.05
62 4.3308 0.00 0.14 0.00 -0.11
63 4.4152 0.00 -0.38 0.00 -0.12
64 4.4153 0.00 0.04 0.00 0.07
65 5.2485 0.00 0.36 0.00 -0.02
66 5.2485 0.00 0.18 0.00 -0.13
67 5.2486 0.00 -0.11 0.00 -0.01
68 5.2486 0.00 -0.11 0.00 0.07
69 5.2945 0.00 0.14 0.00 0.00
70 5.2946 0.00 0.37 0.00 0.06
71 5.2946 0.00 -0.09 0.00 -0.02
72 5.2946 0.00 -0.17 0.00 0.04
73 5.3167 0.00 -0.05 0.00 -0.02
74 5.3167 0.00 -0.06 0.00 0.03
75 5.3168 0.00 0.19 0.00 0.06
76 5.3168 0.00 0.15 0.00 -0.11
77 5.3194 0.00 0.02 0.00 -0.03
78 5.3194 0.00 -0.00 0.00 -0.02
79 5.3194 0.00 0.02 0.00 -0.00
80 7.2742 0.00 0.09 0.00 -0.14
81 7.2742 0.00 0.08 0.00 -0.07
82 7.2743 0.00 -0.12 0.00 0.10
83 10.4033 0.00 0.01 0.00 -0.18
84 10.4033 0.00 -0.12 0.00 0.21
85 10.4033 0.00 0.01 0.00 0.01
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.
679338 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 27.147 27.147 27.147 ecceobj 0.249 0.249 0.249 incobj 12.087 12.087 12.087 qmin 19.026 19.401 18.837 qmax 34.704 34.740 35.207 amean 26.540 27.014 26.703 amin 25.955 26.452 26.101 amax 27.271 27.422 27.406 emean 0.262 0.262 0.271 emin 0.223 0.245 0.245 emax 0.277 0.276 0.287 imean 10.364 9.672 9.428 imin 9.357 8.726 8.242 imax 12.254 11.018 11.018 excite_mean 0.319 0.312 0.317 fracstop 0.009 0.007 0.007 cjmean 2.913 2.913 2.913 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 82.7 74.7 75.3 kozaiamp 46.9 37.9 44.2