Orbit Fit and Astrometric record for 16GS391

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: 16GS391   
# Created Sun Oct 19 01:11:28 2025
# Orbit generated from Bernstein formalism
# Fitting     23 observations of     23
# Arc:   1.84y
# First observation: 2015/03/25
#  Last observation: 2017/01/26
Preliminary a, adot, b, bdot, g, gdot:
  -0.000006   0.023688  -0.000001  -0.000449   0.023893   0.000000
# Chi-squared of fit:    10.77 DOF:     40 RMS:  0.12
# Min/Max residuals:    -0.28    0.32
# Exact a, adot, b, bdot, g, gdot:
  1.546263E-05  2.378102E-02 -4.646521E-07 -4.512448E-04  2.431634E-02 -6.792019E-04
# Covariance matrix:
  2.6660E-13  7.3550E-14  5.1641E-16 -4.4331E-15  7.4637E-13  8.6708E-12
  7.3550E-14  7.0132E-12  2.2524E-14 -1.3049E-13  1.3511E-11  2.0605E-10
  5.1641E-16  2.2524E-14  2.0478E-13 -1.5591E-13  4.3194E-14  6.7064E-13
 -4.4331E-15 -1.3049E-13 -1.5591E-13  1.7437E-13 -2.5806E-13 -3.9324E-12
  7.4637E-13  1.3511E-11  4.3194E-14 -2.5806E-13  2.8277E-11  4.1655E-10
  8.6708E-12  2.0605E-10  6.7064E-13 -3.9324E-12  4.1655E-10  6.2641E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.824651 -178.184705   -0.043430    0.031743   -0.992678  2457106.972828
# Heliocentric elements and errors
Epoch:              2457100.5000  =  2015/03/19
Mean Anomaly:          316.33569 +/-     2.826
Argument of Peri:      168.06354 +/-     3.156
Long of Asc Node:       60.44797 +/-     0.023
Inclination:             2.08751 +/-     0.001
Eccentricity:         0.03683472 +/-    0.0028
Semi-Major Axis:     43.24407796 +/-    0.0373
Time of Perihelion: 2469698.8170 +/-     815.1
Perihelion:          41.65119465 +/-    0.1260
Aphelion:            44.83696126 +/-    0.1268
Period (y)              284.3794 +/-      0.37
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.07756122 +/-    0.0090
Ecliptic Y           -1.37717853 +/-    0.0003
Ecliptic Z            1.30944676 +/-    0.0003
Ecliptic XDOT         0.00015624 +/-    0.0000
Ecliptic YDOT        -0.00267968 +/-    0.0000
Ecliptic ZDOT        -0.00005313 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.12045145 +/-    0.0090
Geocenter to KBO     41.12460190 +/-    0.0090
# Hcoef:  8.03

The following table shows the complete astrometric record for 16GS391. 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 (16GS391) followed by the observatory code and reference code for the source of the astrometry.

2015 03  25.47205  12 09 33.86   +00 57 08.1   24.9g 16GS391   T09  C~94sd      
2015 03  25.48280  12 09 33.82   +00 57 08.4   25.6g 16GS391   T09  C~94sd      
2015 03  25.49994  12 09 33.73   +00 57 08.9   25.1g 16GS391   T09  C~94sd      
2015 03  29.28550  12 09 16.83   +00 58 56.9   22.8y 16GS391   T09  C~94sd      
2015 03  29.29365  12 09 16.81   +00 58 57.3   23.0y 16GS391   T09  C~94sd      
2015 03  29.36170  12 09 16.48   +00 58 59.3   23.2y 16GS391   T09  C~94sd      
2016 04  02.39692  12 13 53.73   +00 27 11.8   23.8i 16GS391   T09  C~8HFu      
2016 04  02.49633  12 13 53.28   +00 27 14.5   23.7i 16GS391   T09  C~8HFu      
2016 04  02.49902  12 13 53.29   +00 27 14.5   23.7i 16GS391   T09  C~8HFu      
2016 04  02.52059  12 13 53.17   +00 27 15.4   23.7i 16GS391   T09  C~8HFu      
2016 04  04.34312  12 13 45.19   +00 28 05.9   25.0g 16GS391   T09  C~8HFu      
2016 04  04.35168  12 13 45.14   +00 28 06.1   25.3g 16GS391   T09  C~8HFu      
2016 04  04.36588  12 13 45.08   +00 28 06.4   25.5g 16GS391   T09  C~8HFu      
2016 04  04.39376  12 13 44.96   +00 28 07.3   25.2g 16GS391   T09  C~8HFu      
2016 04  04.41084  12 13 44.89   +00 28 07.8   25.4g 16GS391   T09  C~8HFu      
2016 04  15.35150  12 12 58.37   +00 32 57.4   23.7y 16GS391   T09  C~8HFu      
2016 04  15.37454  12 12 58.28   +00 32 57.7   23.6y 16GS391   T09  C~8HFu      
2016 04  15.40815  12 12 58.17   +00 32 58.7   23.5y 16GS391   T09  C~8HFu      
2016 04  15.45127  12 12 57.96   +00 32 59.7   23.6y 16GS391   T09  C~8HFu      
2017 01  26.62885  12 22 55.02   -00 34 02.5   24.5z 16GS391   T09  C~94sd      
2017 01  26.63421  12 22 55.00   -00 34 02.3   24.1z 16GS391   T09  C~94sd      
2017 01  26.64229  12 22 54.99   -00 34 02.3   23.9z 16GS391   T09  C~94sd      
2017 01  26.64766  12 22 54.98   -00 34 02.2   24.6z 16GS391   T09  C~94sd      

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     0.00       0.00     0.04
     2   0.0000     -0.67     0.13       0.04     0.08
     3   0.0001     -2.11    -0.04      -0.04     0.02
     4   0.0104   -277.62    -0.03      -1.73    -0.16
     5   0.0105   -278.05     0.14      -1.48     0.09
     6   0.0106   -283.39    -0.20      -1.61     0.02
     7   1.0238   4291.25    -0.11     -97.77    -0.03
     8   1.0240   4283.98    -0.12     -97.98    -0.12
     9   1.0240   4284.12     0.21     -97.92    -0.06
    10   1.0241   4282.11    -0.23     -97.81     0.08
    11   1.0291   4152.15     0.10     -99.10     0.13
    12   1.0291   4151.38    -0.05     -99.22     0.03
    13   1.0291   4150.44     0.03     -99.30    -0.04
    14   1.0292   4148.43     0.04     -99.19     0.11
    15   1.0293   4147.26     0.12     -99.15     0.18
    16   1.0592   3391.62    -0.22    -111.04    -0.06
    17   1.0593   3390.26    -0.03    -111.30    -0.28
    18   1.0594   3388.35     0.32    -111.04     0.04
    19   1.0595   3385.06    -0.06    -111.38    -0.22
    20   1.8430  13219.52     0.08    -238.51     0.02
    21   1.8430  13219.16    -0.10    -238.45     0.08
    22   1.8430  13219.03     0.02    -238.51     0.01
    23   1.8431  13218.85     0.01    -238.48     0.03

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.

16GS391    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        42.852    42.946    42.764
ecceobj         0.031     0.039     0.023
incobj          2.089     2.089     2.089
qmin           41.010    40.776    41.194
qmax           45.252    45.680    44.918
amean          43.052    43.148    42.961
amin           42.721    42.817    42.634
amax           43.397    43.484    43.293
emean           0.024     0.031     0.019
emin            0.005     0.013     0.000
emax            0.043     0.051     0.038
imean           1.006     0.996     1.023
imin            0.127     0.084     0.178
imax            1.618     1.615     1.619
excite_mean     0.030     0.036     0.027
fracstop        1.000     1.000     1.000
cjmean          3.089     3.090     3.088

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       179.7     184.5     169.5
kozaiamp        179.8     179.8     179.9