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: 04OJ14 # Created Thu Apr 25 01:11:54 2024 # Orbit generated from Bernstein formalism # Fitting 13 observations of 13 # Arc: 2.98y # First observation: 2004/07/17 # Last observation: 2007/07/11 Preliminary a, adot, b, bdot, g, gdot: 0.000047 0.021397 -0.000021 -0.008676 0.022950 0.000000 # Chi-squared of fit: 47.42 DOF: 20 RMS: 0.34 # Min/Max residuals: -1.17 0.64 # Exact a, adot, b, bdot, g, gdot: 1.490136E-05 2.170042E-02 -5.488817E-06 -8.796993E-03 2.314727E-02 5.162541E-03 # Covariance matrix: 3.4469E-13 -4.0052E-13 -3.2171E-14 1.0410E-13 2.0594E-13 -4.0300E-12 -4.0052E-13 1.0706E-12 1.0539E-13 -3.6785E-13 -6.4222E-14 1.4339E-11 -3.2171E-14 1.0539E-13 2.1437E-13 -1.4227E-13 -3.7154E-15 1.5928E-12 1.0410E-13 -3.6785E-13 -1.4227E-13 2.6123E-13 -1.8576E-14 -5.6383E-12 2.0594E-13 -6.4222E-14 -3.7154E-15 -1.8576E-14 7.2070E-13 8.3183E-13 -4.0300E-12 1.4339E-11 1.5928E-12 -5.6383E-12 8.3183E-13 2.2006E-10 # lat0 lon0 xBary yBary zBary JD0 -4.305212 -65.562701 -0.010394 -0.076443 -1.016553 2453203.658163 # Heliocentric elements and errors Epoch: 2453200.5000 = 2004/07/14 Mean Anomaly: 34.71218 +/- 0.033 Argument of Peri: 130.35135 +/- 0.059 Long of Asc Node: 104.21521 +/- 0.000 Inclination: 22.49183 +/- 0.001 Eccentricity: 0.29124666 +/- 0.0007 Semi-Major Axis: 55.19878873 +/- 0.0310 Time of Perihelion: 2438757.0109 +/- 5.9 Perihelion: 39.12232585 +/- 0.0441 Aphelion: 71.27525162 +/- 0.0553 Period (y) 410.1120 +/- 0.35 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 18.24968353 +/- 0.0006 Ecliptic Y -40.14243971 +/- 0.0014 Ecliptic Z -3.24335706 +/- 0.0001 Ecliptic XDOT 0.00255420 +/- 0.0000 Ecliptic YDOT 0.00057162 +/- 0.0000 Ecliptic ZDOT -0.00108330 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 44.21522113 +/- 0.0013 Geocenter to KBO 43.20163713 +/- 0.0016 # Hcoef: 6.37
The following table shows the complete astrometric record for 04OJ14. 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 (04OJ14) followed by the observatory code and reference code for the source of the astrometry.
2004 07 17.15742 19 48 45.39 -25 28 02.1 22.3R 04OJ14 807 Cl2727 2004 07 17.23516 19 48 45.01 -25 28 03.6 04OJ14 807 Cl2727 2004 08 12.07787 19 46 42.83 -25 34 40.7 21.7R 04OJ14 807 Cl2727 2004 08 12.18501 19 46 42.27 -25 34 41.7 04OJ14 807 Cl2727 2004 09 11.02082 19 44 58.58 -25 39 24.6 23.9R 04OJ14 304 Cl4371 2004 09 11.04811 19 44 58.51 -25 39 25.3 04OJ14 304 Cl4371 2005 06 09.23005 19 57 21.85 -25 31 35.6 22.3R 04OJ14 304 Co3996 2005 06 09.26214 19 57 21.70 -25 31 36.2 04OJ14 304 Co3996 2005 08 08.05524 19 52 49.69 -25 49 32.6 22.3R 04OJ14 807 Co3996 2005 08 08.17171 19 52 49.17 -25 49 34.1 04OJ14 807 Co3996 2005 08 09.06123 19 52 45.14 -25 49 46.6 04OJ14 807 Co3996 2007 07 11.33756 20 06 35.27 -26 09 42.0 04OJ14 304 Cv1992 2007 07 11.38898 20 06 35.01 -26 09 43.3 04OJ14 304 Cv1992
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 -0.02 0.00 -0.11
2 0.0002 -5.33 0.07 -0.54 -0.28
3 0.0710 -1703.72 -0.11 -92.81 -0.14
4 0.0713 -1711.36 -1.17 -92.44 0.45
5 0.1529 -3141.95 0.64 -122.83 0.27
6 0.1530 -3143.00 0.52 -123.35 -0.26
7 0.8955 6826.69 0.45 -1540.20 -0.14
8 0.8956 6824.58 0.00 -1540.39 -0.05
9 1.0593 3006.01 -0.29 -1882.73 -0.04
10 1.0596 2998.83 0.00 -1882.87 0.09
11 1.0620 2943.02 -0.04 -1884.81 0.25
12 2.9820 13683.55 0.10 -5331.01 0.09
13 2.9822 13679.84 -0.15 -5331.52 -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.
04OJ14 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 55.167 55.258 55.077 ecceobj 0.288 0.290 0.286 incobj 22.489 22.489 22.489 qmin 38.178 37.749 38.407 qmax 73.155 74.338 72.820 amean 55.265 55.557 55.198 amin 54.678 54.685 54.617 amax 56.058 56.419 55.937 emean 0.286 0.296 0.286 emin 0.268 0.270 0.269 emax 0.307 0.319 0.303 imean 20.842 20.757 20.807 imin 20.135 19.903 20.188 imax 21.466 21.506 21.306 excite_mean 0.457 0.462 0.456 fracstop 1.000 1.000 1.000 cjmean 2.971 2.969 2.971 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 186.3 184.2 181.1 kozaiamp 179.9 179.9 180.0