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: 16FZ59 # Created Wed Nov 27 02:10:36 2024 # Orbit generated from Bernstein formalism # Fitting 9 observations of 9 # Arc: 2.09d # First observation: 2016/03/30 # Last observation: 2016/04/01 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution # Chi-squared of fit: 41.24 DOF: 14 RMS: 0.38 # Min/Max residuals: -0.86 0.88 # Exact a, adot, b, bdot, g, gdot: 1.784669E-05 2.822458E-02 -2.440814E-06 -4.158144E-03 2.724438E-02 0.000000E+00 # Covariance matrix: 3.6006E-11 6.1136E-08 -1.0056E-12 -2.0417E-09 9.7870E-09 0.0000E+00 6.1136E-08 1.0502E-04 -1.7249E-09 -3.5021E-06 1.6787E-05 0.0000E+00 -1.0056E-12 -1.7249E-09 3.5175E-13 -1.2285E-11 -2.7582E-10 0.0000E+00 -2.0417E-09 -3.5021E-06 -1.2285E-11 1.4726E-07 -5.5999E-07 0.0000E+00 9.7870E-09 1.6787E-05 -2.7582E-10 -5.5999E-07 2.6843E-06 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 2.6611E-04 # lat0 lon0 xBary yBary zBary JD0 -19.462755 -176.150166 -0.097837 -0.329651 -0.933381 2457477.576979 # Heliocentric elements and errors Epoch: 2457470.5000 = 2016/03/23 Mean Anomaly: 1.56432 +/- 251.639 Argument of Peri: 245.42997 +/- 318.695 Long of Asc Node: 298.20589 +/- 6.121 Inclination: 20.63669 +/- 0.940 Eccentricity: 0.05065690 +/- 0.5610 Semi-Major Axis: 39.65114577 +/- 21.1064 Time of Perihelion: 2457074.2173 +/- 154943.7 Perihelion: 37.64254174 +/- 29.9388 Aphelion: 41.65974981 +/- 31.4102 Period (y) 249.6846 +/- 199.36 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -35.51411986 +/- 2.0765 Ecliptic Y -2.49035604 +/- 0.1396 Ecliptic Z -12.22992851 +/- 0.7355 Ecliptic XDOT 0.00032943 +/- 0.0015 Ecliptic YDOT -0.00282758 +/- 0.0009 Ecliptic ZDOT -0.00039398 +/- 0.0005 # Distances at JD0 (AU) Heliocenter to KBO 37.64340226 +/- 1.9736 Geocenter to KBO 36.70481101 +/- 2.2073 # Hcoef: 8.69
The following table shows the complete astrometric record for 16FZ59. 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 (16FZ59) followed by the observatory code and reference code for the source of the astrometry.
2016 03 30.07619 11 41 53.92 -19 19 20.1 24.5V 16FZ59 W84 C~1qoK 2016 03 30.08313 11 41 53.91 -19 19 20.0 16FZ59 W84 C~1qoK 2016 03 30.09007 11 41 53.91 -19 19 20.1 16FZ59 W84 C~1qoK 2016 03 31.13339 11 41 48.45 -19 18 43.6 16FZ59 W84 C~1qoK 2016 03 31.14033 11 41 48.45 -19 18 43.5 16FZ59 W84 C~1qoK 2016 03 31.14727 11 41 48.45 -19 18 43.5 16FZ59 W84 C~1qoK 2016 04 01.14784 11 41 43.30 -19 18 08.3 16FZ59 W84 C~1qoK 2016 04 01.15478 11 41 43.30 -19 18 08.4 16FZ59 W84 C~1qoK 2016 04 01.16172 11 41 43.31 -19 18 08.6 16FZ59 W84 C~1qoK
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 -0.30 0.00 0.01
2 0.0000 -0.17 0.09 0.03 0.04
3 0.0000 -0.13 0.70 -0.06 -0.05
4 0.0029 -85.60 -0.86 0.54 -0.06
5 0.0029 -85.64 -0.34 0.64 0.03
6 0.0029 -85.64 0.22 0.64 0.03
7 0.0057 -166.59 -0.50 1.89 0.11
8 0.0057 -166.55 0.11 1.80 0.01
9 0.0057 -166.34 0.88 1.68 -0.12
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.
16FZ59 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