Orbit Fit and Astrometric record for 16TS94

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: 16TS94    
# Created Sun Dec 22 02:10:53 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     36 observations of     36
# Arc:   6.07y
# First observation: 2014/12/16
#  Last observation: 2021/01/11
# Chi-squared of fit:    38.41 DOF:     66 RMS:  0.18
# Min/Max residuals:    -0.46    0.45
# Exact a, adot, b, bdot, g, gdot:
  1.653772E-05  3.103826E-02 -7.443920E-06 -1.317274E-02  2.965668E-02  3.657773E-03
# Covariance matrix:
  1.8928E-13 -1.2631E-13 -2.7814E-14  3.7147E-14 -1.4476E-14 -5.3560E-13
 -1.2631E-13  1.5361E-13  4.1872E-14 -5.5177E-14 -2.6598E-14  7.9224E-13
 -2.7814E-14  4.1872E-14  1.3344E-13 -5.0790E-14 -8.2811E-15  2.3941E-13
  3.7147E-14 -5.5177E-14 -5.0790E-14  3.7087E-14  8.6818E-15 -3.1607E-13
 -1.4476E-14 -2.6598E-14 -8.2811E-15  8.6818E-15  1.4998E-13 -1.1456E-13
 -5.3560E-13  7.9224E-13  2.3941E-13 -3.1607E-13 -1.1456E-13  4.5407E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
  -30.360119   26.049372   -0.831370   -0.265505   -0.453664  2457007.683328
# Heliocentric elements and errors
Epoch:              2457008.5000  =  2014/12/17
Mean Anomaly:           36.41011 +/-     0.009
Argument of Peri:      185.28568 +/-     0.012
Long of Asc Node:      157.19696 +/-     0.000
Inclination:            36.71561 +/-     0.000
Eccentricity:         0.18068456 +/-    0.0001
Semi-Major Axis:     39.33427003 +/-    0.0034
Time of Perihelion: 2447895.2234 +/-       2.5
Perihelion:          32.22717462 +/-    0.0043
Aphelion:            46.44136544 +/-    0.0051
Period (y)              246.6976 +/-      0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           26.24357053 +/-    0.0003
Ecliptic Y           13.75613925 +/-    0.0002
Ecliptic Z          -17.04309592 +/-    0.0002
Ecliptic XDOT        -0.00155284 +/-    0.0000
Ecliptic YDOT         0.00242721 +/-    0.0000
Ecliptic ZDOT        -0.00121989 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   34.18213379 +/-    0.0003
Geocenter to KBO     33.71919156 +/-    0.0004
# Hcoef:  7.40

The following table shows the complete astrometric record for 16TS94. 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 (16TS94) followed by the observatory code and reference code for the source of the astrometry.

2014 12  16.18255  02 21 09.926  -18 14 24.17  23.7g 16TS94    W84  C~4ycG      
2014 12  16.19078  02 21 09.901  -18 14 24.03  23.0r 16TS94    W84  C~4ycG      
2014 12  23.10167  02 20 47.694  -18 11 34.33  23.1r 16TS94    W84  C~4ycG      
2014 12  23.10304  02 20 47.697  -18 11 34.26  22.9i 16TS94    W84  C~4ycG      
2014 12  24.16332  02 20 44.707  -18 11 03.99  23.4g 16TS94    W84  C~4ycG      
2015 01  08.12518  02 20 15.572  -18 02 06.57  22.3z 16TS94    W84  C~4ycG      
2015 11  15.28381  02 31 46.468  -18 17 19.99  22.3i 16TS94    W84  C~4ycG      
2015 11  20.27054  02 31 18.838  -18 18 18.09  23.0g 16TS94    W84  C~4ycG      
2015 12  14.18968  02 29 24.323  -18 16 27.40  22.8r 16TS94    W84  C~4ycG      
2015 12  14.19108  02 29 24.325  -18 16 27.31  23.2g 16TS94    W84  C~4ycG      
2016 02  06.04408  02 28 26.348  -17 39 08.85  22.4i 16TS94    W84  C~4ycG      
2016 02  06.04957  02 28 26.371  -17 39 08.39  22.3r 16TS94    W84  C~4ycG      
2016 02  06.05094  02 28 26.379  -17 39 08.35  22.2g 16TS94    W84  C~4ycG      
2016 10  06.25664  02 43 29.497  -17 54 09.84  23.0r 16TS94    807  C~2AEF      
2016 10  06.37433  02 43 28.889  -17 54 15.60  23.2r 16TS94    807  C~2AEF      
2016 10  07.32498  02 43 24.269  -17 55 04.19  23.0r 16TS94    807  C~2AEF      
2016 10  07.33492  02 43 24.227  -17 55 04.04  22.9r 16TS94    807  C~2AEF      
2016 10  08.26721  02 43 19.617  -17 55 51.08  22.7r 16TS94    807  C~2AEF      
2017 01  22.08314  02 36 02.221  -17 52 37.91  23.4i 16TS94    W84  C~4ycG      
2017 01  22.08452  02 36 02.225  -17 52 37.93  23.1r 16TS94    W84  C~4ycG      
2017 10  30.33182  02 49 21.811  -18 09 10.84  23.0r 16TS94    W84  C~4ycG      
2017 10  30.33318  02 49 21.790  -18 09 10.89  22.6i 16TS94    W84  C~4ycG      
2017 10  30.33455  02 49 21.788  -18 09 10.88  23.3g 16TS94    W84  C~4ycG      
2017 11  01.22992  02 49 10.910  -18 10 10.91  21.8z 16TS94    W84  C~4ycG      
2017 11  01.23129  02 49 10.904  -18 10 10.59  22.3z 16TS94    W84  C~4ycG      
2017 11  10.22903  02 48 18.880  -18 14 04.09  22.9i 16TS94    W84  C~4ycG      
2018 01  16.11752  02 43 54.546  -17 56 57.13  23.1r 16TS94    W84  C~4ycG      
2018 01  16.11890  02 43 54.542  -17 56 56.90  22.9i 16TS94    W84  C~4ycG      
2018 01  16.12027  02 43 54.558  -17 56 57.03  23.3g 16TS94    W84  C~4ycG      
2018 09  22.37823  03 00 20.570  -17 35 32.47  22.7z 16TS94    W84  C~4ycG      
2018 10  18.31358  02 58 25.546  -17 58 16.35  22.5r 16TS94    W84  C~4ycG      
2018 10  18.33582  02 58 25.440  -17 58 17.28  22.5i 16TS94    W84  C~4ycG      
2018 10  18.33719  02 58 25.435  -17 58 17.36  22.8g 16TS94    W84  C~4ycG      
2021 01  11.119670 03 07 11.966  -17 50 52.32  22.8G 16TS94    G37  C~4UMi      
2021 01  11.184670 03 07 11.829  -17 50 49.49        16TS94    G37  C~4UMi      
2021 01  11.226110 03 07 11.780  -17 50 47.80        16TS94    G37  C~4UMi      

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    -0.03       0.00     0.08
     2   0.0000      0.00     0.04       0.00     0.05
     3   0.0189      0.00    -0.03       0.00    -0.00
     4   0.0189      0.00     0.07       0.00     0.03
     5   0.0219      0.00     0.07       0.00    -0.03
     6   0.0628      0.00    -0.09       0.00    -0.11
     7   0.9147      0.00     0.16       0.00    -0.02
     8   0.9284      0.00     0.22       0.00     0.23
     9   0.9939      0.00    -0.03       0.00    -0.01
    10   0.9939      0.00     0.08       0.00     0.06
    11   1.1413      0.00    -0.06       0.00     0.00
    12   1.1413      0.00     0.12       0.00     0.14
    13   1.1413      0.00     0.20       0.00     0.10
    14   1.8072      0.00    -0.05       0.00    -0.37
    15   1.8075      0.00    -0.46       0.00    -0.10
    16   1.8101      0.00    -0.29       0.00    -0.20
    17   1.8101      0.00    -0.17       0.00     0.45
    18   1.8127      0.00    -0.42       0.00     0.37
    19   2.1024      0.00    -0.13       0.00     0.03
    20   2.1024      0.00    -0.07       0.00    -0.06
    21   2.8724      0.00     0.23       0.00    -0.05
    22   2.8724      0.00     0.03       0.00    -0.06
    23   2.8724      0.00     0.12       0.00    -0.00
    24   2.8776      0.00     0.11       0.00    -0.32
    25   2.8776      0.00     0.14       0.00     0.04
    26   2.9022      0.00     0.26       0.00    -0.04
    27   3.0854      0.00    -0.09       0.00    -0.03
    28   3.0854      0.00    -0.13       0.00     0.13
    29   3.0854      0.00     0.13       0.00    -0.06
    30   3.7678      0.00     0.23       0.00     0.05
    31   3.8388      0.00     0.00       0.00    -0.25
    32   3.8389      0.00     0.20       0.00    -0.21
    33   3.8389      0.00     0.23       0.00    -0.23
    34   6.0724      0.00    -0.36       0.00     0.14
    35   6.0726      0.00    -0.30       0.00     0.21
    36   6.0727      0.00     0.31       0.00     0.13

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.

16TS94    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.660    39.661    39.660
ecceobj         0.187     0.187     0.187
incobj         36.631    36.631    36.631
qmin           31.736    31.736    31.736
qmax           47.672    47.681    47.662
amean          39.454    39.454    39.454
amin           39.069    39.069    39.069
amax           39.878    39.877    39.879
emean           0.160     0.160     0.160
emin            0.113     0.113     0.113
emax            0.197     0.197     0.196
imean          36.012    36.012    36.012
imin           35.458    35.458    35.457
imax           36.606    36.606    36.606
excite_mean     0.610     0.610     0.610
fracstop        1.000     1.000     1.000
cjmean          2.591     2.591     2.591

libcent 0       179.7     179.7     179.7
libamp  0        90.2      90.2      90.1
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       180.2     180.2     180.1
kozaiamp        180.0     180.0     180.0