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: 03UV292 # Created Fri Nov 22 02:08:31 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 21 observations of 21 # Arc: 18.11y # First observation: 2003/10/24 # Last observation: 2021/12/01 # Chi-squared of fit: 16.73 DOF: 36 RMS: 0.16 # Min/Max residuals: -0.41 0.31 # Exact a, adot, b, bdot, g, gdot: 1.783904E-05 3.365405E-02 -3.339203E-06 -6.530162E-03 3.026844E-02 6.300386E-03 # Covariance matrix: 1.9399E-13 -2.5709E-14 -5.9470E-15 3.7111E-15 9.5032E-14 -3.5137E-14 -2.5709E-14 2.5672E-14 6.6213E-15 -4.5377E-15 4.1218E-14 4.1286E-14 -5.9470E-15 6.6213E-15 1.2352E-13 -1.1610E-14 8.4083E-15 1.1813E-14 3.7111E-15 -4.5377E-15 -1.1610E-14 2.9908E-15 -6.4759E-15 -8.0482E-15 9.5032E-14 4.1218E-14 8.4083E-15 -6.4759E-15 3.1080E-13 5.6235E-14 -3.5137E-14 4.1286E-14 1.1813E-14 -8.0482E-15 5.6235E-14 7.3406E-14 # lat0 lon0 xBary yBary zBary JD0 -0.482766 58.901724 0.477079 -0.007316 -0.874056 2452936.912813 # Heliocentric elements and errors Epoch: 2452936.5000 = 2003/10/24 Mean Anomaly: 40.24622 +/- 0.009 Argument of Peri: 122.71769 +/- 0.012 Long of Asc Node: 235.67592 +/- 0.000 Inclination: 10.96840 +/- 0.000 Eccentricity: 0.21438185 +/- 0.0000 Semi-Major Axis: 39.38888022 +/- 0.0033 Time of Perihelion: 2442842.0775 +/- 2.5 Perihelion: 30.94461909 +/- 0.0030 Aphelion: 47.83314134 +/- 0.0043 Period (y) 247.2115 +/- 0.03 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 17.91998736 +/- 0.0003 Ecliptic Y 28.79423738 +/- 0.0005 Ecliptic Z -0.27847749 +/- 0.0000 Ecliptic XDOT -0.00231955 +/- 0.0000 Ecliptic YDOT 0.00204996 +/- 0.0000 Ecliptic ZDOT -0.00059529 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 33.91614516 +/- 0.0005 Geocenter to KBO 33.03764367 +/- 0.0006 # Hcoef: 7.39
The following table shows the complete astrometric record for 03UV292. 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 (03UV292) followed by the observatory code and reference code for the source of the astrometry.
2003 10 24.41207 03 47 09.36 +19 26 34.4 22.2R 03UV292 695 Cj5825 2003 10 24.50482 03 47 08.87 +19 26 32.4 03UV292 695 Cj5825 2003 11 20.30028 03 44 32.78 +19 16 27.3 21.9R 03UV292 695 Cj5825 2003 11 20.37554 03 44 32.32 +19 16 25.6 03UV292 695 Cj5825 2004 03 16.13469 03 40 56.21 +18 58 56.8 22.4R 03UV292 695 Ck4313 2004 03 16.17543 03 40 56.40 +18 58 57.6 03UV292 695 Ck4313 2004 11 09.41846 03 53 52.72 +19 23 17.3 21.8R 03UV292 695 Cl9848 2004 11 10.36606 03 53 47.07 +19 22 56.5 03UV292 695 Cl9848 2004 11 10.44059 03 53 46.63 +19 22 54.9 03UV292 695 Cl9848 2005 12 02.22096 03 59 48.17 +19 16 48.6 21.8R 03UV292 695 Cp9890 2005 12 02.27438 03 59 47.83 +19 16 47.5 03UV292 695 Cp9890 2005 12 02.32705 03 59 47.52 +19 16 46.4 03UV292 695 Cp9890 2008 11 03.88152 04 26 34.79 +19 22 36.6 23.2R 03UV292 250 S~06Af 2008 11 03.88777 04 26 34.76 +19 22 36.5 03UV292 250 S~06Af 2008 11 03.89471 04 26 34.72 +19 22 36.4 03UV292 250 S~06Af 2008 11 03.90096 04 26 34.69 +19 22 36.2 03UV292 250 S~06Af 2015 02 18.11969 05 03 37.33 +18 31 09.7 23.0R 03UV292 695 C~1M69 2015 02 18.16392 05 03 37.28 +18 31 09.6 03UV292 695 C~1M69 2015 02 18.21187 05 03 37.23 +18 31 09.8 03UV292 695 C~1M69 2021 12 01.408760 05 57 36.966 +17 13 01.16 23.7G 03UV292 G37 C~5J1A 2021 12 01.487720 05 57 36.573 +17 13 00.57 03UV292 G37 C~5J1A
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 -0.05 0.00 -0.03
2 0.0003 0.00 0.01 0.00 -0.08
3 0.0736 0.00 -0.02 0.00 -0.03
4 0.0738 0.00 0.11 0.00 0.05
5 0.3935 0.00 0.18 0.00 -0.05
6 0.3936 0.00 0.26 0.00 0.26
7 1.0459 0.00 0.05 0.00 -0.06
8 1.0485 0.00 -0.17 0.00 -0.02
9 1.0487 0.00 0.01 0.00 0.04
10 2.1076 0.00 -0.23 0.00 -0.15
11 2.1078 0.00 -0.41 0.00 -0.15
12 2.1079 0.00 -0.20 0.00 -0.16
13 5.0307 0.00 0.01 0.00 0.16
14 5.0307 0.00 0.06 0.00 0.16
15 5.0308 0.00 0.01 0.00 0.18
16 5.0308 0.00 0.06 0.00 0.09
17 11.3202 0.00 -0.08 0.00 0.31
18 11.3203 0.00 -0.06 0.00 0.10
19 11.3205 0.00 0.02 0.00 0.18
20 18.1054 0.00 -0.28 0.00 -0.15
21 18.1056 0.00 0.24 0.00 -0.23
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.
03UV292 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.726 39.726 39.726 ecceobj 0.221 0.221 0.221 incobj 10.941 10.941 10.941 qmin 28.250 28.272 28.250 qmax 51.173 51.186 51.171 amean 39.455 39.455 39.455 amin 39.044 39.043 39.045 amax 39.980 39.937 39.979 emean 0.247 0.247 0.247 emin 0.197 0.197 0.197 emax 0.281 0.282 0.281 imean 9.832 9.836 9.832 imin 7.204 7.217 7.205 imax 12.819 12.819 12.818 excite_mean 0.302 0.302 0.302 fracstop 1.000 1.000 1.000 cjmean 2.947 2.947 2.947 libcent 0 179.5 179.3 179.4 libamp 0 60.2 60.4 60.2 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 81.3 81.4 81.3 kozaiamp 48.8 48.8 48.8