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: MB56169 # Created Wed Jun 4 01:12:11 2025 # Orbit generated from Bernstein formalism # Fitting 2 observations of 2 # Arc: 2.08h # First observation: 2002/04/08 # Last observation: 2002/04/08 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # Chi-squared of fit: 0.00 DOF: 0 RMS: 0.00 # Min/Max residuals: -0.00 0.00 # Exact a, adot, b, bdot, g, gdot: 1.750666E-05 3.793841E-02 -5.635058E-06 -1.221165E-02 3.426704E-02 0.000000E+00 # Covariance matrix: 8.6034E-11 1.7818E-07 5.3811E-12 1.5289E-08 3.5433E-08 0.0000E+00 1.7818E-07 3.7523E-04 1.1545E-08 3.2842E-05 7.2488E-05 0.0000E+00 5.3811E-12 1.1545E-08 6.9419E-12 1.8086E-08 2.0826E-09 0.0000E+00 1.5289E-08 3.2842E-05 1.8086E-08 5.2698E-05 5.8966E-06 0.0000E+00 3.5433E-08 7.2488E-05 2.0826E-09 5.8966E-06 1.5483E-05 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 5.2948E-04 # lat0 lon0 xBary yBary zBary JD0 -0.011023 -137.935429 0.403193 -0.000221 -0.919149 2452372.636773 # Heliocentric elements and errors Epoch: 2452370.5000 = 2002/04/06 Inclination: 17.86501 +/- 14.555 Eccentricity: 0.03048774 +/- 0.6074 Semi-Major Axis: 30.98598720 +/- 16.5911 Perihelion: 30.04129432 +/- 24.7583 Aphelion: 31.93068007 +/- 25.4272 Period (y) 172.4869 +/- 138.53 # Distances at JD0 (AU) Heliocenter to KBO 30.10023094 +/- 2.3852 Geocenter to KBO 29.18256434 +/- 3.3510 # Hcoef: 6.35
The following table shows the complete astrometric record for MB56169. 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 (MB56169) followed by the observatory code and reference code for the source of the astrometry.
2002 04 8.13603 14 38 28.927 -15 27 59.28 20.8R MB56169 807 2002 04 8.22273 14 38 28.399 -15 27 57.51 MB56169 807
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 0.00 0.00 -0.00
2 0.0002 -7.81 0.00 -0.65 -0.00
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.
MB56169 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0