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: 04VE131 # Created Fri Nov 22 02:08:44 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 16 observations of 16 # Arc: 8.91y # First observation: 2004/11/09 # Last observation: 2013/10/07 # Chi-squared of fit: 19.95 DOF: 26 RMS: 0.20 # Min/Max residuals: -0.73 0.25 # Exact a, adot, b, bdot, g, gdot: 1.481792E-05 2.576793E-02 -2.225926E-06 -2.344716E-03 2.592846E-02 -6.743861E-03 # Covariance matrix: 3.0322E-13 -3.0737E-13 -1.2837E-14 2.2357E-14 3.1009E-13 -9.6516E-13 -3.0737E-13 4.8440E-13 2.1352E-14 -3.7232E-14 -4.5732E-13 1.6067E-12 -1.2837E-14 2.1352E-14 1.2792E-13 -2.1282E-14 -1.8157E-14 7.3089E-14 2.2357E-14 -3.7232E-14 -2.1282E-14 1.3151E-14 3.1135E-14 -1.2760E-13 3.1009E-13 -4.5732E-13 -1.8157E-14 3.1135E-14 1.0950E-12 -1.3503E-12 -9.6516E-13 1.6067E-12 7.3089E-14 -1.2760E-13 -1.3503E-12 5.5047E-12 # lat0 lon0 xBary yBary zBary JD0 -0.176401 40.926316 -0.105835 -0.002935 -0.987173 2453318.884993 # Heliocentric elements and errors Epoch: 2453318.5000 = 2004/11/09 Mean Anomaly: 298.51101 +/- 0.021 Argument of Peri: 272.83238 +/- 0.035 Long of Asc Node: 219.19485 +/- 0.000 Inclination: 5.20405 +/- 0.000 Eccentricity: 0.25912353 +/- 0.0001 Semi-Major Axis: 42.21998402 +/- 0.0078 Time of Perihelion: 2470433.2425 +/- 23.6 Perihelion: 31.27979292 +/- 0.0065 Aphelion: 53.16017512 +/- 0.0102 Period (y) 274.3376 +/- 0.08 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 29.81166753 +/- 0.0012 Ecliptic Y 25.99284998 +/- 0.0010 Ecliptic Z -0.11883215 +/- 0.0000 Ecliptic XDOT -0.00232220 +/- 0.0000 Ecliptic YDOT 0.00158161 +/- 0.0000 Ecliptic ZDOT -0.00024530 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 39.55237495 +/- 0.0011 Geocenter to KBO 38.56786172 +/- 0.0016 # Hcoef: 7.48
The following table shows the complete astrometric record for 04VE131. 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 (04VE131) followed by the observatory code and reference code for the source of the astrometry.
2004 11 09.38425 02 34 14.06 +14 56 12.4 24.0g 04VE131 568 C~0WzI 2004 11 09.41074 02 34 13.92 +14 56 11.6 24.0g 04VE131 568 C~0WzI 2004 11 09.43671 02 34 13.78 +14 56 10.9 23.7g 04VE131 568 C~0WzI 2004 11 10.30006 02 34 09.43 +14 55 49.1 23.8g 04VE131 568 C~0WzI 2005 01 05.21941 02 30 41.11 +14 38 06.0 23.4i 04VE131 568 C~0WzI 2005 01 05.27535 02 30 41.04 +14 38 05.7 23.3i 04VE131 568 C~0WzI 2005 01 05.34540 02 30 40.91 +14 38 05.1 23.2i 04VE131 568 C~0WzI 2005 10 25.50968 02 41 32.80 +15 22 11.9 23.2r 04VE131 568 C~0WzI 2005 10 25.54219 02 41 32.63 +15 22 11.1 23.4r 04VE131 568 C~0WzI 2005 10 25.57629 02 41 32.46 +15 22 10.2 23.6r 04VE131 568 C~0WzI 2005 10 26.54983 02 41 27.51 +15 21 45.5 23.3r 04VE131 568 C~0WzI 2006 10 21.98902 02 47 59.46 +15 42 55.0 04VE131 950 C~0WzI 2006 10 22.09446 02 47 58.94 +15 42 52.8 04VE131 950 C~0WzI 2006 10 22.17303 02 47 58.53 +15 42 50.9 04VE131 950 C~0WzI 2013 10 07.31065 03 35 00.45 +17 48 30.6 22.2R 04VE131 695 C~0zdg 2013 10 07.39584 03 35 00.13 +17 48 29.6 04VE131 695 C~0zdg
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 0.13 0.00 0.21
2 0.0001 0.00 0.08 0.00 0.09
3 0.0001 0.00 -0.01 0.00 0.05
4 0.0025 0.00 0.09 0.00 0.15
5 0.1556 0.00 -0.26 0.00 -0.00
6 0.1558 0.00 0.12 0.00 0.19
7 0.1560 0.00 -0.06 0.00 0.22
8 0.9586 0.00 0.02 0.00 -0.08
9 0.9587 0.00 -0.03 0.00 -0.07
10 0.9588 0.00 0.04 0.00 -0.12
11 0.9614 0.00 -0.38 0.00 -0.73
12 1.9483 0.00 0.06 0.00 -0.18
13 1.9486 0.00 0.25 0.00 0.12
14 1.9488 0.00 0.05 0.00 0.09
15 8.9088 0.00 -0.13 0.00 -0.15
16 8.9090 0.00 0.09 0.00 0.24
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.
04VE131 quality flag:3 Type: 5:3EE 5:3EE 5:3EE axisobj 42.640 42.640 42.640 ecceobj 0.258 0.258 0.258 incobj 5.177 5.177 5.177 qmin 30.893 30.893 30.893 qmax 54.268 54.268 54.268 amean 42.326 42.326 42.326 amin 41.919 41.919 41.919 amax 42.823 42.823 42.822 emean 0.253 0.253 0.253 emin 0.239 0.239 0.239 emax 0.268 0.268 0.268 imean 6.599 6.599 6.599 imin 5.941 5.941 5.941 imax 7.106 7.106 7.106 excite_mean 0.278 0.278 0.278 fracstop 1.000 1.000 1.000 cjmean 2.990 2.990 2.990 libcent 0 180.2 180.2 180.1 libamp 0 49.6 49.6 49.6 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 211.3 211.3 211.3 kozaiamp 61.3 61.3 61.2