Orbit Fit and Astrometric record for 14TG115

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: 14TG115   
# Created Tue Apr  1 01:10:07 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:  11.12y
# First observation: 2013/10/13
#  Last observation: 2024/11/24
# Chi-squared of fit:     6.87 DOF:     34 RMS:  0.10
# Min/Max residuals:    -0.24    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.440309E-05  1.871505E-02 -1.787027E-06 -2.343964E-03  2.141111E-02 -1.807838E-03
# Covariance matrix:
  4.7436E-13 -1.7553E-13 -3.3032E-14  1.8545E-14 -1.0016E-13 -6.4353E-13
 -1.7553E-13  9.0892E-14  2.0643E-14 -1.1016E-14  4.6282E-15  3.9030E-13
 -3.3032E-14  2.0643E-14  1.9533E-13 -3.0398E-14 -1.0283E-14  1.0044E-13
  1.8545E-14 -1.1016E-14 -3.0398E-14  7.9309E-15  2.1496E-15 -5.2136E-14
 -1.0016E-13  4.6282E-15 -1.0283E-14  2.1496E-15  3.3519E-13 -1.2538E-13
 -6.4353E-13  3.9030E-13  1.0044E-13 -5.2136E-14 -1.2538E-13  1.8688E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
   -8.458773   16.655070   -0.053133   -0.146384   -0.985160  2456578.721808
# Heliocentric elements and errors
Epoch:              2456578.5000  =  2013/10/13
Mean Anomaly:          246.87626 +/-     0.043
Argument of Peri:      353.66592 +/-     0.032
Long of Asc Node:      147.68527 +/-     0.001
Inclination:            10.91175 +/-     0.000
Eccentricity:         0.11060913 +/-    0.0001
Semi-Major Axis:     45.28619800 +/-    0.0044
Time of Perihelion: 2491556.7817 +/-      17.4
Perihelion:          40.27713084 +/-    0.0055
Aphelion:            50.29526516 +/-    0.0062
Period (y)              304.7593 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           45.19687002 +/-    0.0012
Ecliptic Y           13.57982554 +/-    0.0004
Ecliptic Z           -6.87028259 +/-    0.0002
Ecliptic XDOT        -0.00095335 +/-    0.0000
Ecliptic YDOT         0.00221309 +/-    0.0000
Ecliptic ZDOT        -0.00026232 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   47.69041358 +/-    0.0011
Geocenter to KBO     46.70482753 +/-    0.0013
# Hcoef:  6.87

The following table shows the complete astrometric record for 14TG115. 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 (14TG115) followed by the observatory code and reference code for the source of the astrometry.

2013 10  13.22103  01 14 20.079  -01 16 18.02  23.0i 14TG115   W84  C~52UG      
2014 10  02.31064  01 19 15.196  -00 54 18.09  23.5r 14TG115   W84  C~52UG      
2014 10  02.31200  01 19 15.191  -00 54 18.21  23.5i 14TG115   W84  C~52UG      
2014 10  28.24179  01 17 31.788  -01 05 02.82  22.9i 14TG115   W84  C~52UG      
2014 10  29.24597  01 17 27.878  -01 05 24.29  23.4r 14TG115   W84  C~52UG      
2015 09  04.30826  01 25 04.002  -00 24 21.16  23.7i 14TG115   W84  C~52UG      
2016 08  14.40444  01 29 58.620  +00 00 41.96  23.8r 14TG115   W84  C~52UG      
2016 08  30.34715  01 29 26.203  -00 05 24.71  24.1g 14TG115   W84  C~52UG      
2016 10  21.19058  01 26 20.504  -00 28 16.28  22.8z 14TG115   W84  C~52UG      
2017 08  22.39752  01 33 55.922  +00 15 02.28  23.2r 14TG115   W84  C~52UG      
2017 08  22.39889  01 33 55.906  +00 15 02.44  23.1i 14TG115   W84  C~52UG      
2017 08  27.34864  01 33 45.405  +00 13 06.31  23.2r 14TG115   W84  C~52UG      
2017 08  28.38199  01 33 43.007  +00 12 41.54  23.5i 14TG115   W84  C~52UG      
2018 11  02.29613  01 34 00.09   +00 02 00.5   24.7g 14TG115   T09  C~8H4B      
2018 11  02.30741  01 34 00.06   +00 02 00.3   24.6g 14TG115   T09  C~8H4B      
2018 11  02.34808  01 33 59.89   +00 01 59.3   24.5g 14TG115   T09  C~8H4B      
2018 11  29.10663  01 32 26.877  -00 04 45.25  23.6r 14TG115   W84  C~52UG      
2024 11  24.113620 01 58 21.907  +01 41 15.66  23.5G 14TG115   G37  C~8SSg      
2024 11  24.157220 01 58 21.774  +01 41 15.02        14TG115   G37  C~8SSg      
2024 11  24.200530 01 58 21.596  +01 41 14.45        14TG115   G37  C~8SSg      

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    -0.12       0.00    -0.04
     2   0.9694      0.00    -0.08       0.00     0.03
     3   0.9694      0.00    -0.07       0.00    -0.05
     4   1.0404      0.00     0.17       0.00     0.03
     5   1.0432      0.00     0.05       0.00     0.04
     6   1.8921      0.00    -0.02       0.00    -0.01
     7   2.8369      0.00     0.18       0.00     0.06
     8   2.8806      0.00     0.07       0.00     0.08
     9   3.0225      0.00     0.05       0.00     0.07
    10   3.8581      0.00     0.16       0.00    -0.18
    11   3.8581      0.00    -0.03       0.00     0.02
    12   3.8717      0.00    -0.01       0.00    -0.18
    13   3.8745      0.00    -0.07       0.00     0.02
    14   5.0543      0.00    -0.24       0.00     0.07
    15   5.0543      0.00    -0.01       0.00     0.10
    16   5.0544      0.00    -0.12       0.00    -0.06
    17   5.1277      0.00     0.16       0.00     0.02
    18  11.1154      0.00    -0.10       0.00     0.06
    19  11.1155      0.00     0.23       0.00    -0.02
    20  11.1156      0.00    -0.13       0.00    -0.04

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.

14TG115    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        45.524    45.524    45.524
ecceobj         0.106     0.106     0.106
incobj         10.886    10.886    10.886
qmin           39.443    39.463    39.461
qmax           51.396    51.364    51.321
amean          45.258    45.258    45.258
amin           44.884    44.900    44.892
amax           45.658    45.653    45.679
emean           0.112     0.112     0.112
emin            0.100     0.100     0.100
emax            0.126     0.125     0.125
imean           9.953     9.953     9.953
imin            9.482     9.482     9.481
imax           10.438    10.438    10.438
excite_mean     0.206     0.206     0.206
fracstop        1.000     1.000     1.000
cjmean          3.065     3.065     3.065

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       175.3     175.4     175.4
kozaiamp        180.0     180.0     180.0