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: 16FX59 # Created Fri Nov 1 01:10:21 2024 # Orbit generated from Bernstein formalism # Fitting 9 observations of 9 # Arc: 2.06d # First observation: 2016/03/29 # Last observation: 2016/03/31 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution # Chi-squared of fit: 31.84 DOF: 14 RMS: 0.33 # Min/Max residuals: -0.65 0.72 # Exact a, adot, b, bdot, g, gdot: 1.567287E-05 2.213280E-02 6.176577E-06 1.137836E-02 2.493343E-02 0.000000E+00 # Covariance matrix: 4.4278E-11 6.9083E-08 3.0416E-13 2.0819E-10 1.1002E-08 0.0000E+00 6.9083E-08 1.0880E-04 4.7852E-10 3.2742E-07 1.7305E-05 0.0000E+00 3.0416E-13 4.7852E-10 3.1625E-13 -6.7109E-11 7.6126E-11 0.0000E+00 2.0819E-10 3.2742E-07 -6.7109E-11 3.2121E-08 5.2093E-08 0.0000E+00 1.1002E-08 1.7305E-05 7.6126E-11 5.2093E-08 2.7531E-06 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 2.0397E-04 # lat0 lon0 xBary yBary zBary JD0 -12.027107 -170.324643 0.017113 -0.207033 -0.972558 2457476.763059 # Heliocentric elements and errors Epoch: 2457470.5000 = 2016/03/23 Mean Anomaly: 3.11906 +/- 35.427 Argument of Peri: 332.09799 +/- 101.427 Long of Asc Node: 211.29703 +/- 9.155 Inclination: 29.39223 +/- 9.908 Eccentricity: 0.04158195 +/- 0.5704 Semi-Major Axis: 42.86323887 +/- 22.7267 Time of Perihelion: 2456582.4290 +/- 215086.8 Perihelion: 41.08090163 +/- 32.7454 Aphelion: 44.64557611 +/- 34.0319 Period (y) 280.6310 +/- 223.19 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -39.65525114 +/- 2.5733 Ecliptic Y -6.74549480 +/- 0.4385 Ecliptic Z -8.35699319 +/- 0.5561 Ecliptic XDOT 0.00015188 +/- 0.0015 Ecliptic YDOT -0.00244649 +/- 0.0010 Ecliptic ZDOT 0.00122200 +/- 0.0003 # Distances at JD0 (AU) Heliocenter to KBO 41.08381650 +/- 2.4875 Geocenter to KBO 40.10679500 +/- 2.6690 # Hcoef: 8.04
The following table shows the complete astrometric record for 16FX59. 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 (16FX59) followed by the observatory code and reference code for the source of the astrometry.
2016 03 29.26227 12 16 07.19 -14 51 58.8 24.2V 16FX59 W84 C~1qoK 2016 03 29.26921 12 16 07.17 -14 51 58.9 16FX59 W84 C~1qoK 2016 03 29.27615 12 16 07.17 -14 51 58.8 16FX59 W84 C~1qoK 2016 03 30.30064 12 16 02.36 -14 51 21.3 16FX59 W84 C~1qoK 2016 03 30.30758 12 16 02.36 -14 51 21.2 16FX59 W84 C~1qoK 2016 03 30.31452 12 16 02.36 -14 51 21.3 16FX59 W84 C~1qoK 2016 03 31.31045 12 15 57.70 -14 50 44.1 16FX59 W84 C~1qoK 2016 03 31.31739 12 15 57.71 -14 50 44.1 16FX59 W84 C~1qoK 2016 03 31.32433 12 15 57.72 -14 50 44.2 16FX59 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 -0.34 0.00 0.21 2 0.0000 -0.22 -0.03 -0.21 -0.03 3 0.0000 -0.27 0.47 -0.12 0.02 4 0.0028 -79.22 -0.58 5.86 -0.13 5 0.0029 -79.26 -0.09 5.95 -0.08 6 0.0029 -79.22 0.48 5.86 -0.21 7 0.0056 -156.07 -0.65 12.44 0.09 8 0.0056 -155.93 0.01 12.50 0.10 9 0.0056 -155.76 0.72 12.47 0.02
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.
16FX59 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