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: 16FY59 # Created Fri Nov 1 01:10:21 2024 # Orbit generated from Bernstein formalism # Fitting 9 observations of 9 # Arc: 3.04d # First observation: 2016/03/29 # Last observation: 2016/04/01 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # Chi-squared of fit: 30.39 DOF: 14 RMS: 0.32 # Min/Max residuals: -0.69 0.73 # Exact a, adot, b, bdot, g, gdot: 1.620004E-05 2.268031E-02 8.191578E-06 1.391344E-02 2.619875E-02 0.000000E+00 # Covariance matrix: 5.5272E-11 9.0808E-08 6.5899E-13 7.3470E-10 1.4469E-08 0.0000E+00 9.0808E-08 1.5044E-04 1.0910E-09 1.2163E-06 2.3954E-05 0.0000E+00 6.5899E-13 1.0910E-09 3.9307E-13 -4.6419E-11 1.7373E-10 0.0000E+00 7.3470E-10 1.2163E-06 -4.6419E-11 2.3583E-08 1.9368E-07 0.0000E+00 1.4469E-08 2.3954E-05 1.7373E-10 1.9368E-07 3.8144E-06 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 2.3663E-04 # lat0 lon0 xBary yBary zBary JD0 -10.322519 -168.110636 0.054390 -0.177777 -0.976974 2457476.827779 # Heliocentric elements and errors Epoch: 2457470.5000 = 2016/03/23 Mean Anomaly: 3.47907 +/- 92.057 Argument of Peri: 337.51474 +/- 158.308 Long of Asc Node: 207.75541 +/- 8.026 Inclination: 32.85664 +/- 12.863 Eccentricity: 0.02741774 +/- 0.5827 Semi-Major Axis: 40.25264975 +/- 21.1908 Time of Perihelion: 2456569.0318 +/- 303693.4 Perihelion: 39.14901322 +/- 31.2223 Aphelion: 41.35628629 +/- 32.0013 Period (y) 255.3877 +/- 201.67 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -37.73300047 +/- 2.7394 Ecliptic Y -7.89054745 +/- 0.5765 Ecliptic Z -6.83929092 +/- 0.5099 Ecliptic XDOT 0.00023343 +/- 0.0016 Ecliptic YDOT -0.00237997 +/- 0.0011 Ecliptic ZDOT 0.00143047 +/- 0.0003 # Distances at JD0 (AU) Heliocenter to KBO 39.15119364 +/- 2.6442 Geocenter to KBO 38.16976514 +/- 2.8455 # Hcoef: 7.86
The following table shows the complete astrometric record for 16FY59. 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 (16FY59) followed by the observatory code and reference code for the source of the astrometry.
2016 03 29.32699 12 27 10.44 -14 11 00.4 23.8V 16FY59 W84 C~1qoK 2016 03 29.33393 12 27 10.43 -14 11 00.4 16FY59 W84 C~1qoK 2016 03 29.34087 12 27 10.43 -14 11 00.3 16FY59 W84 C~1qoK 2016 03 31.34235 12 27 00.68 -14 09 42.6 16FY59 W84 C~1qoK 2016 03 31.34929 12 27 00.67 -14 09 42.8 16FY59 W84 C~1qoK 2016 03 31.35623 12 27 00.67 -14 09 42.8 16FY59 W84 C~1qoK 2016 04 01.35452 12 26 55.75 -14 09 03.2 16FY59 W84 C~1qoK 2016 04 01.36146 12 26 55.75 -14 09 03.2 16FY59 W84 C~1qoK 2016 04 01.36840 12 26 55.75 -14 09 03.2 16FY59 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 -0.52 0.00 0.04
2 0.0000 -0.13 -0.09 -0.06 -0.06
3 0.0000 -0.17 0.43 0.03 -0.02
4 0.0055 -161.24 -0.34 14.25 0.25
5 0.0055 -161.29 0.17 14.01 -0.05
6 0.0056 -161.29 0.73 14.01 -0.10
7 0.0083 -242.73 -0.69 21.53 0.03
8 0.0083 -242.73 -0.13 21.53 -0.02
9 0.0083 -242.73 0.44 21.53 -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.
16FY59 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