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: 03FL127 # Created Sat Oct 20 01:08:02 2018 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 20 observations of 20 # Arc: 12.06y # First observation: 2001/02/20 # Last observation: 2013/03/14 # Chi-squared of fit: 40.09 DOF: 34 RMS: 0.25 # Min/Max residuals: -0.40 0.64 # Exact a, adot, b, bdot, g, gdot: 1.326201E-05 1.780866E-02 9.319606E-07 -9.570612E-04 2.181529E-02 2.560909E-03 # Covariance matrix: 4.5953E-13 -1.6125E-13 -1.3912E-14 7.8396E-15 1.2950E-13 -6.2314E-13 -1.6125E-13 1.0773E-13 9.0841E-15 -5.6598E-15 8.5716E-14 4.5677E-13 -1.3912E-14 9.0841E-15 1.5426E-13 -2.1321E-14 4.4824E-15 4.0531E-14 7.8396E-15 -5.6598E-15 -2.1321E-14 5.8054E-15 -4.6019E-15 -2.5284E-14 1.2950E-13 8.5716E-14 4.4824E-15 -4.6019E-15 6.1180E-13 3.9223E-13 -6.2314E-13 4.5677E-13 4.0531E-14 -2.5284E-14 3.9223E-13 2.0409E-12 # lat0 lon0 xBary yBary zBary JD0 -1.676565 162.451629 0.176391 -0.028679 -0.974007 2451960.908107 # Heliocentric elements and errors Epoch: 2451960.5000 = 2001/02/20 Mean Anomaly: 135.80702 +/- 0.029 Argument of Peri: 56.92239 +/- 0.017 Long of Asc Node: 314.16130 +/- 0.002 Inclination: 3.48575 +/- 0.000 Eccentricity: 0.23630701 +/- 0.0001 Semi-Major Axis: 39.31408376 +/- 0.0040 Time of Perihelion: 2417994.8157 +/- 8.9 Perihelion: 30.02389002 +/- 0.0041 Aphelion: 48.60427751 +/- 0.0057 Period (y) 246.5077 +/- 0.04 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -44.55933201 +/- 0.0016 Ecliptic Y 14.28167577 +/- 0.0005 Ecliptic Z -1.34107584 +/- 0.0001 Ecliptic XDOT -0.00098515 +/- 0.0000 Ecliptic YDOT -0.00203191 +/- 0.0000 Ecliptic ZDOT -0.00012928 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 46.81122589 +/- 0.0015 Geocenter to KBO 45.83936335 +/- 0.0016 # Hcoef: 6.22
The following table shows the complete astrometric record for 03FL127. 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 (03FL127) followed by the observatory code and reference code for the source of the astrometry.
2001 02 20.407364 10 52 42.63 +05 20 18.6 03FL127 645 C~1S6p 2001 02 20.408193 10 52 42.63 +05 20 18.6 03FL127 645 C~1S6p 2001 02 20.410681 10 52 42.62 +05 20 18.6 03FL127 645 C~1S6p 2003 03 31.24892 10 57 29.60 +04 43 35.2 22.8R 03FL127 695 Ch8427 2003 04 01.20889 10 57 26.08 +04 43 57.7 03FL127 695 Ch8427 2003 04 01.30535 10 57 25.75 +04 44 00.1 03FL127 695 Ch8427 2003 04 20.98248 10 56 23.59 +04 50 43.7 21.1R 03FL127 304 Ch8427 2003 04 21.04435 10 56 23.45 +04 50 45.2 03FL127 304 Ch8427 2003 05 31.28477 10 55 34.42 +04 56 55.4 23.4R 03FL127 568 Ci1570 2003 06 01.27935 10 55 34.73 +04 56 55.2 03FL127 568 Ci1570 2004 02 22.34802 11 03 40.16 +04 01 50.2 22.7R 03FL127 695 Ck4311 2004 02 22.39985 11 03 39.94 +04 01 51.4 03FL127 695 Ck4311 2004 03 16.21639 11 02 05.34 +04 11 28.5 22.7R 03FL127 695 Ck4311 2004 03 16.28074 11 02 05.09 +04 11 30.3 03FL127 695 Ck4311 2005 03 09.30108 11 06 13.79 +03 42 09.9 22.7R 03FL127 695 Cn0206 2005 03 10.29166 11 06 09.68 +03 42 35.6 03FL127 695 Cn0206 2005 03 10.39291 11 06 09.24 +03 42 37.9 03FL127 695 Cn0206 2013 03 13.35452 11 34 25.72 +00 16 39.4 22.9R 03FL127 695 C~0ud4 2013 03 14.33104 11 34 21.74 +00 17 04.9 03FL127 695 C~0ud4 2013 03 14.43968 11 34 21.31 +00 17 07.8 03FL127 695 C~0ud4
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 -0.15 0.00 -0.30 2 0.0000 0.00 -0.10 0.00 -0.32 3 0.0000 0.00 -0.09 0.00 -0.38 4 2.1050 0.00 0.03 0.00 0.15 5 2.1076 0.00 -0.23 0.00 0.37 6 2.1079 0.00 0.17 0.00 0.54 7 2.1617 0.00 0.24 0.00 -0.01 8 2.1619 0.00 0.64 0.00 0.40 9 2.2721 0.00 -0.01 0.00 -0.33 10 2.2748 0.00 -0.40 0.00 -0.36 11 3.0033 0.00 0.32 0.00 0.01 12 3.0034 0.00 0.24 0.00 -0.06 13 3.0659 0.00 -0.14 0.00 0.02 14 3.0660 0.00 0.12 0.00 0.18 15 4.0463 0.00 -0.00 0.00 -0.05 16 4.0490 0.00 0.10 0.00 0.22 17 4.0492 0.00 -0.10 0.00 -0.08 18 12.0574 0.00 -0.15 0.00 -0.34 19 12.0600 0.00 -0.06 0.00 -0.03 20 12.0603 0.00 0.24 0.00 0.07
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.
03FL127 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.197 39.197 39.197 ecceobj 0.239 0.239 0.239 incobj 3.495 3.495 3.495 qmin 29.237 29.243 29.232 qmax 50.279 50.303 50.247 amean 39.455 39.455 39.455 amin 39.016 39.019 39.023 amax 39.945 39.952 39.951 emean 0.240 0.240 0.240 emin 0.221 0.221 0.220 emax 0.259 0.259 0.259 imean 3.920 3.918 3.921 imin 2.784 2.782 2.785 imax 5.574 5.576 5.579 excite_mean 0.250 0.250 0.250 fracstop 1.000 1.000 1.000 cjmean 2.980 2.980 2.980 libcent 0 180.3 180.1 179.9 libamp 0 72.1 71.7 71.9 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 91.8 91.8 91.8 kozaiamp 46.7 46.7 46.7