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: 16FV59 # Created Wed Apr 24 01:17:49 2024 # Orbit generated from Bernstein formalism # Fitting 16 observations of 16 # Arc: 28.66d # First observation: 2016/03/11 # Last observation: 2016/04/09 Preliminary a, adot, b, bdot, g, gdot: -0.000000 0.032323 0.000000 0.003802 0.026452 0.000000 # WARNING Fitting with energy constraint # Chi-squared of fit: 44.49 DOF: 27 RMS: 0.29 # Min/Max residuals: -0.71 0.70 # Exact a, adot, b, bdot, g, gdot: 1.661418E-05 2.645201E-02 2.070346E-06 3.783771E-03 2.550455E-02 -1.896513E-03 # Covariance matrix: 2.3984E-12 3.0722E-09 2.4730E-13 7.9626E-12 4.8816E-10 -3.3880E-09 3.0722E-09 4.9406E-06 3.9807E-10 1.2433E-08 7.8107E-07 -6.8817E-06 2.4730E-13 3.9807E-10 4.7575E-13 -7.0368E-12 6.2905E-11 -5.7790E-10 7.9626E-12 1.2433E-08 -7.0368E-12 2.1595E-10 1.9729E-09 -1.1758E-08 4.8816E-10 7.8107E-07 6.2905E-11 1.9729E-09 1.2353E-07 -1.0569E-06 -3.3880E-09 -6.8817E-06 -5.7790E-10 -1.1758E-08 -1.0569E-06 3.3357E-05 # lat0 lon0 xBary yBary zBary JD0 -4.963067 -176.625983 0.212554 -0.083522 -0.963485 2457458.993329 # Heliocentric elements and errors Epoch: 2457450.5000 = 2016/03/03 Mean Anomaly: 334.00894 +/- 45.805 Argument of Peri: 3.84705 +/- 65.881 Long of Asc Node: 213.72494 +/- 2.011 Inclination: 9.43601 +/- 0.553 Eccentricity: 0.14831150 +/- 0.2216 Semi-Major Axis: 46.08070302 +/- 7.8208 Time of Perihelion: 2465699.4475 +/- 14384.9 Perihelion: 39.24640467 +/- 12.1928 Aphelion: 52.91500137 +/- 13.5996 Period (y) 312.8145 +/- 79.64 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -39.97564709 +/- 0.5374 Ecliptic Y -2.14619952 +/- 0.0316 Ecliptic Z -3.39198649 +/- 0.0468 Ecliptic XDOT 0.00033441 +/- 0.0006 Ecliptic YDOT -0.00283175 +/- 0.0002 Ecliptic ZDOT 0.00042228 +/- 0.0001 # Distances at JD0 (AU) Heliocenter to KBO 40.17666120 +/- 0.5347 Geocenter to KBO 39.20869143 +/- 0.5403 # Hcoef: 7.31
The following table shows the complete astrometric record for 16FV59. 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 (16FV59) followed by the observatory code and reference code for the source of the astrometry.
2016 03 11.492540 12 04 27.95 -05 53 40.3 23.0r 16FV59 568 C~5SAz 2016 03 11.493580 12 04 27.95 -05 53 40.4 23.0r 16FV59 568 C~5SAz 2016 03 11.494617 12 04 27.94 -05 53 40.3 23.0r 16FV59 568 C~5SAz 2016 03 29.22817 12 03 06.60 -05 44 21.5 24.2V 16FV59 W84 C~1qoK 2016 03 29.23511 12 03 06.60 -05 44 21.4 16FV59 W84 C~1qoK 2016 03 29.24205 12 03 06.60 -05 44 21.4 16FV59 W84 C~1qoK 2016 03 30.25282 12 03 01.93 -05 43 47.9 16FV59 W84 C~1qoK 2016 03 30.25976 12 03 01.93 -05 43 47.8 16FV59 W84 C~1qoK 2016 03 30.26670 12 03 01.94 -05 43 47.9 16FV59 W84 C~1qoK 2016 03 31.21315 12 02 57.58 -05 43 16.2 16FV59 W84 C~1qoK 2016 03 31.22009 12 02 57.59 -05 43 16.4 16FV59 W84 C~1qoK 2016 03 31.22703 12 02 57.60 -05 43 16.4 16FV59 W84 C~1qoK 2016 04 01.22720 12 02 53.01 -05 42 43.4 16FV59 W84 C~1qoK 2016 04 01.23414 12 02 53.00 -05 42 43.3 16FV59 W84 C~1qoK 2016 04 01.24108 12 02 53.00 -05 42 43.3 16FV59 W84 C~1qoK 2016 04 09.156285 12 02 18.00 -05 38 23.6 23.1r 16FV59 W84 C~5SAz
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 -0.04 0.00 0.06
2 0.0000 0.04 0.07 -0.09 -0.03
3 0.0000 -0.14 -0.03 -0.06 -0.00
4 0.0486 -1336.14 -0.50 27.33 -0.11
5 0.0486 -1336.18 -0.01 27.42 -0.04
6 0.0486 -1336.18 0.53 27.42 -0.06
7 0.0514 -1413.47 -0.63 30.26 -0.04
8 0.0514 -1413.51 -0.14 30.36 0.03
9 0.0514 -1413.33 0.57 30.32 -0.02
10 0.0540 -1485.65 -0.71 33.36 0.23
11 0.0540 -1485.44 0.04 33.24 0.08
12 0.0540 -1485.30 0.70 33.30 0.13
13 0.0568 -1561.29 -0.35 36.16 -0.08
14 0.0568 -1561.47 -0.00 36.19 -0.07
15 0.0568 -1561.47 0.52 36.19 -0.09
16 0.0785 -2144.20 -0.03 65.27 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.
16FV59 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