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: 434709
# Created Fri Nov 22 02:07:05 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 41 observations of 41
# Arc: 18.12y
# First observation: 2005/02/04
# Last observation: 2023/03/19
# Chi-squared of fit: 107.10 DOF: 76 RMS: 0.29
# Min/Max residuals: -0.62 0.69
# Exact a, adot, b, bdot, g, gdot:
1.686119E-05 3.078717E-02 7.661137E-06 9.948381E-03 2.893385E-02 -5.526903E-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
0.803391 132.778544 -0.042268 0.013871 -0.981783 2453405.714849
# Heliocentric elements and errors
Epoch: 2453406.5000 = 2005/02/05
Mean Anomaly: 323.95065 +/- 0.000
Argument of Peri: 58.63583 +/- 0.000
Long of Asc Node: 130.43042 +/- 0.000
Inclination: 17.88884 +/- 0.000
Eccentricity: 0.23291772 +/- 0.0000
Semi-Major Axis: 42.46926916 +/- 0.0000
Time of Perihelion: 2463529.4133 +/- 0.0
Perihelion: 32.57742386 +/- 0.0000
Aphelion: 52.36111447 +/- 0.0000
Period (y) 276.7709 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -24.17339337 +/- 0.0000
Ecliptic Y 26.05680667 +/- 0.0000
Ecliptic Z 0.48486677 +/- 0.0000
Ecliptic XDOT -0.00177438 +/- 0.0000
Ecliptic YDOT -0.00237927 +/- 0.0000
Ecliptic ZDOT 0.00093400 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 35.54648554 +/- 0.0000
Geocenter to KBO 34.56173987 +/- 0.0000
# Hcoef: 7.42
The following table shows the complete astrometric record for 434709. 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 (434709) followed by the observatory code and reference code for the source of the astrometry.
2005 02 04.214106 09 01 55.63 +17 44 45.6 22.4V 434709 645 C~1S6u 2005 02 04.214935 09 01 55.62 +17 44 45.6 22.0V 434709 645 C~1S6u 2005 02 04.217423 09 01 55.61 +17 44 45.7 24.0V 434709 645 C~1S6u 2005 02 10.29754 09 01 21.10 +17 47 46.3 23.9g 434709 568 C~0WzS 2005 02 10.38053 09 01 20.62 +17 47 49.2 23.7g 434709 568 C~0WzS 2005 02 10.41998 09 01 20.40 +17 47 50.1 23.4g 434709 568 C~0WzS 2005 04 11.28159 08 57 27.46 +18 08 53.5 23.4i 434709 568 C~0WzS 2005 04 11.30756 08 57 27.42 +18 08 53.6 23.5i 434709 568 C~0WzS 2005 04 11.33716 08 57 27.39 +18 08 53.8 23.3i 434709 568 C~0WzS 2006 02 03.46124 09 09 51.58 +17 46 24.9 22.2r 434709 568 C~0D42 2006 02 06.31183 09 09 35.31 +17 47 53.0 22.5r 434709 568 C~0D42 2006 02 06.35104 09 09 35.09 +17 47 54.1 23.1r 434709 568 C~0D42 2006 02 06.39104 09 09 34.86 +17 47 55.3 22.9r 434709 568 C~0D42 2006 11 23.49146 09 22 13.36 +17 17 25.7 434709 695 C~0WzS 2006 11 24.49089 09 22 12.99 +17 17 36.7 434709 695 C~0WzS 2007 02 14.48107 09 16 45.32 +17 53 06.9 22.8r 434709 568 C~0WzS 2007 02 14.51467 09 16 45.13 +17 53 08.0 22.7r 434709 568 C~0WzS 2007 02 14.54775 09 16 44.93 +17 53 08.9 434709 568 C~0WzS 2007 02 15.49201 09 16 39.59 +17 53 37.7 22.9r 434709 568 C~0WzS 2010 03 19.14502 09 38 05.97 +18 05 45.6 434709 675 C~0WzS 2010 03 20.13767 09 38 01.68 +18 06 08.1 434709 675 C~0WzS 2010 03 20.16850 09 38 01.54 +18 06 08.8 434709 675 C~0WzS 2015 03 23.13538 10 19 32.56 +17 37 36.1 22.3R 434709 695 C~1Q3P 2015 03 23.19935 10 19 32.25 +17 37 37.9 434709 695 C~1Q3P 2015 03 23.26284 10 19 31.94 +17 37 39.5 434709 695 C~1Q3P 2015 04 15.18266 10 18 01.46 +17 44 58.6 22.1R 434709 695 C~1RHb 2015 04 15.25488 10 18 01.25 +17 44 59.5 434709 695 C~1RHb 2015 04 15.33374 10 18 01.01 +17 45 00.4 434709 695 C~1RHb 2020 02 01.557945 11 07 14.993 +15 59 04.02 23.0G 434709 T12 C~3sZs 2022 01 27.29019 11 25 00.43 +15 18 17.6 22.0R 434709 G37 C~5RdQ 2022 01 27.31076 11 25 00.36 +15 18 18.4 22.1R 434709 G37 C~5RdQ 2022 01 27.38462 11 25 00.06 +15 18 21.8 22.5R 434709 G37 C~5RdQ 2022 01 27.43895 11 24 59.86 +15 18 24.1 22.5R 434709 G37 C~5RdQ 2022 01 27.462694 11 24 59.795 +15 18 24.94 22.5w 434709 F52 C~5Paz 2022 01 27.474872 11 24 59.754 +15 18 25.83 22.5w 434709 F52 C~5Paz 2022 01 27.487060 11 24 59.695 +15 18 26.17 22.1w 434709 F52 C~5Paz 2022 01 27.53897 11 24 59.49 +15 18 28.4 22.2R 434709 G37 C~5RdQ 2023 03 19.494536 11 29 29.672 +15 34 30.84 22.3w 434709 F52 C~6bkt 2023 03 19.507388 11 29 29.623 +15 34 31.24 22.6w 434709 F52 C~6bkt 2023 03 19.520265 11 29 29.562 +15 34 31.84 22.7w 434709 F52 C~6bkt 2023 03 19.533117 11 29 29.472 +15 34 32.10 22.5w 434709 F52 C~6bkt
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 -0.14 0.00 -0.44
2 0.0000 0.00 -0.22 0.00 -0.46
3 0.0000 0.00 -0.16 0.00 -0.44
4 0.0167 0.00 0.08 0.00 -0.36
5 0.0169 0.00 0.01 0.00 0.09
6 0.0170 0.00 0.11 0.00 -0.17
7 0.1809 0.00 0.29 0.00 0.69
8 0.1810 0.00 0.20 0.00 0.55
9 0.1810 0.00 0.33 0.00 0.48
10 0.9973 0.00 -0.43 0.00 -0.47
11 1.0051 0.00 -0.37 0.00 -0.46
12 1.0052 0.00 -0.26 0.00 -0.58
13 1.0053 0.00 -0.23 0.00 -0.62
14 1.7995 0.00 0.08 0.00 0.46
15 1.8023 0.00 0.12 0.00 0.60
16 2.0267 0.00 0.07 0.00 0.12
17 2.0268 0.00 0.12 0.00 0.19
18 2.0269 0.00 -0.04 0.00 0.08
19 2.0295 0.00 -0.35 0.00 -0.24
20 5.1169 0.00 0.40 0.00 0.54
21 5.1196 0.00 0.65 0.00 0.25
22 5.1197 0.00 0.57 0.00 0.24
23 10.1271 0.00 -0.22 0.00 0.10
24 10.1273 0.00 -0.17 0.00 0.22
25 10.1274 0.00 -0.15 0.00 0.17
26 10.1902 0.00 -0.24 0.00 0.05
27 10.1904 0.00 -0.08 0.00 0.10
28 10.1906 0.00 -0.10 0.00 0.09
29 14.9907 0.00 0.06 0.00 -0.08
30 16.9776 0.00 0.03 0.00 -0.08
31 16.9777 0.00 0.13 0.00 -0.17
32 16.9779 0.00 -0.20 0.00 0.03
33 16.9780 0.00 -0.11 0.00 -0.02
34 16.9781 0.00 0.07 0.00 -0.26
35 16.9781 0.00 0.15 0.00 0.10
36 16.9782 0.00 -0.04 0.00 -0.09
37 16.9783 0.00 0.02 0.00 -0.03
38 18.1171 0.00 -0.28 0.00 -0.01
39 18.1172 0.00 0.08 0.00 -0.08
40 18.1172 0.00 0.27 0.00 0.05
41 18.1172 0.00 0.02 0.00 -0.16
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.
434709 quality flag:3 Type: 5:3EE 5:3EE 5:3EE axisobj 42.191 42.190 42.191 ecceobj 0.226 0.226 0.226 incobj 17.922 17.922 17.922 qmin 30.312 30.298 30.621 qmax 55.000 55.054 54.636 amean 42.326 42.326 42.326 amin 41.890 41.852 41.866 amax 42.869 42.859 42.854 emean 0.249 0.249 0.247 emin 0.194 0.194 0.194 emax 0.284 0.285 0.276 imean 15.729 15.732 15.870 imin 14.165 14.176 14.828 imax 17.995 17.994 17.996 excite_mean 0.369 0.369 0.369 fracstop 1.000 1.000 1.000 cjmean 2.921 2.921 2.921 libcent 0 179.4 179.8 179.7 libamp 0 76.3 76.5 76.0 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 268.9 268.5 260.7 kozaiamp 180.0 180.0 180.0