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: 16LJ106
# Created Tue Apr 1 01:10:49 2025
# Orbit generated from Bernstein formalism
# Fitting 9 observations of 9
# Arc: 80.87d
# First observation: 2016/03/16
# Last observation: 2016/06/05
Preliminary a, adot, b, bdot, g, gdot:
-0.000024 0.029393 -0.000010 -0.001083 0.025332 0.000000
# Chi-squared of fit: 1.12 DOF: 12 RMS: 0.06
# Min/Max residuals: -0.10 0.13
# Exact a, adot, b, bdot, g, gdot:
1.618306E-05 2.467260E-02 -2.994036E-07 -1.199998E-03 2.457979E-02 -1.559968E-03
# Covariance matrix:
4.9383E-13 8.8690E-12 -3.1932E-14 2.0204E-13 2.8268E-12 1.9803E-10
8.8690E-12 1.9899E-08 -5.0039E-11 4.9984E-10 3.2608E-09 -5.0236E-08
-3.1932E-14 -5.0039E-11 4.8647E-13 -3.2233E-12 -8.2459E-12 1.1822E-10
2.0204E-13 4.9984E-10 -3.2233E-12 3.2241E-11 8.1408E-11 -1.3876E-09
2.8268E-12 3.2608E-09 -8.2459E-12 8.1408E-11 5.4348E-10 -6.3860E-09
1.9803E-10 -5.0236E-08 1.1822E-10 -1.3876E-09 -6.3860E-09 5.2524E-07
# lat0 lon0 xBary yBary zBary JD0
9.566841 -151.850458 0.527170 0.139661 -0.827822 2457464.036129
# Heliocentric elements and errors
Epoch: 2457460.5000 = 2016/03/13
Mean Anomaly: 318.06097 +/- 7.157
Argument of Peri: 156.41062 +/- 9.943
Long of Asc Node: 101.35401 +/- 0.135
Inclination: 9.74600 +/- 0.007
Eccentricity: 0.10256714 +/- 0.0273
Semi-Major Axis: 44.69425795 +/- 0.5234
Time of Perihelion: 2470174.7826 +/- 2158.3
Perihelion: 40.11009591 +/- 1.3063
Aphelion: 49.27842000 +/- 1.3486
Period (y) 298.8036 +/- 5.25
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -36.36521368 +/- 0.0335
Ecliptic Y -18.86041184 +/- 0.0179
Ecliptic Z 6.76158908 +/- 0.0064
Ecliptic XDOT 0.00142797 +/- 0.0001
Ecliptic YDOT -0.00235975 +/- 0.0000
Ecliptic ZDOT -0.00016067 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 41.51942904 +/- 0.0305
Geocenter to KBO 40.68382795 +/- 0.0386
# Hcoef: 7.25
The following table shows the complete astrometric record for 16LJ106. 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 (16LJ106) followed by the observatory code and reference code for the source of the astrometry.
2016 03 16.53534 13 58 12.21 -01 51 58.7 23.3z 16LJ106 T09 C~89Tk 2016 03 16.55726 13 58 12.14 -01 51 57.9 23.2z 16LJ106 T09 C~89Tk 2016 03 16.58177 13 58 12.05 -01 51 57.4 22.9z 16LJ106 T09 C~89Tk 2016 04 15.50963 13 56 06.95 -01 38 13.0 23.0y 16LJ106 T09 C~89Tk 2016 04 15.52318 13 56 06.88 -01 38 12.6 23.0y 16LJ106 T09 C~89Tk 2016 04 15.53670 13 56 06.82 -01 38 12.3 22.6y 16LJ106 T09 C~89Tk 2016 06 05.36153 13 52 38.75 -01 23 54.7 23.9r 16LJ106 T09 C~89Tk 2016 06 05.39286 13 52 38.66 -01 23 54.5 23.7r 16LJ106 T09 C~89Tk 2016 06 05.40348 13 52 38.62 -01 23 54.3 23.8r 16LJ106 T09 C~89Tk
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 -0.06 0.00 -0.10
2 0.0001 -1.26 0.01 0.38 0.13
3 0.0001 -2.70 0.06 0.38 -0.04
4 0.0821 -2048.43 0.06 113.88 0.00
5 0.0821 -2049.55 -0.06 113.89 0.01
6 0.0821 -2050.50 -0.00 113.85 -0.02
7 0.2213 -5273.93 0.01 -179.56 -0.08
8 0.2214 -5275.26 0.08 -179.84 -0.01
9 0.2214 -5275.90 -0.08 -179.87 0.09
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.
16LJ106 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.153 45.841 42.858 ecceobj 0.096 0.167 0.042 incobj 9.746 9.732 9.763 qmin 39.483 37.811 40.706 qmax 49.717 55.033 45.764 amean 44.460 46.189 43.143 amin 44.099 45.779 42.812 amax 44.845 46.650 43.481 emean 0.094 0.166 0.038 emin 0.078 0.154 0.022 emax 0.109 0.180 0.053 imean 7.860 7.836 7.990 imin 7.269 7.324 7.290 imax 8.474 8.481 8.674 excite_mean 0.166 0.215 0.144 fracstop 1.000 1.000 1.000 cjmean 3.074 3.072 3.067 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 185.2 180.9 180.6 kozaiamp 180.0 179.9 180.0