Orbit Fit and Astrometric record for 14FE72

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: 14FE72    
# Created Fri Nov 22 02:09:52 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:   6.98y
# First observation: 2014/03/26
#  Last observation: 2021/03/18
# Chi-squared of fit:    42.36 DOF:     34 RMS:  0.26
# Min/Max residuals:    -0.44    0.53
# Exact a, adot, b, bdot, g, gdot:
  1.259824E-05  1.448955E-02 -4.529056E-06 -4.581387E-03  1.705417E-02  1.221062E-02
# Covariance matrix:
  1.3452E-13 -6.9497E-14 -6.9182E-15  1.4328E-14  6.6268E-15 -5.4223E-13
 -6.9497E-14  1.3599E-13  1.4403E-14 -3.8399E-14  3.2653E-14  1.4614E-12
 -6.9182E-15  1.4403E-14  1.1949E-13 -2.9822E-14 -1.2972E-14  1.7656E-13
  1.4328E-14 -3.8399E-14 -2.9822E-14  2.8433E-14 -9.2965E-15 -4.6821E-13
  6.6268E-15  3.2653E-14 -1.2972E-14 -9.2965E-15  2.0844E-13  3.8659E-13
 -5.4223E-13  1.4614E-12  1.7656E-13 -4.6821E-13  3.8659E-13  1.7817E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -10.988660 -172.675342    0.035342   -0.189649   -0.977363  2456742.613198
# Heliocentric elements and errors
Epoch:              2456742.5000  =  2014/03/26
Mean Anomaly:            0.10878 +/-     0.005
Argument of Peri:      134.12619 +/-     0.005
Long of Asc Node:      336.76245 +/-     0.001
Inclination:            20.59560 +/-     0.000
Eccentricity:         0.98773791 +/-    0.0004
Semi-Major Axis:   2944.81399416 +/-   84.6914
Time of Perihelion: 2439104.7936 +/-    1077.8
Perihelion:          36.10957387 +/-    1.4738
Aphelion:          5853.51841445 +/-  168.3476
Period (y)           159806.7078 +/-   6893.95
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -58.08517927 +/-    0.0015
Ecliptic Y           -7.42917087 +/-    0.0002
Ecliptic Z          -11.17730118 +/-    0.0003
Ecliptic XDOT        -0.00147861 +/-    0.0000
Ecliptic YDOT        -0.00253779 +/-    0.0000
Ecliptic ZDOT        -0.00109553 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   59.61487768 +/-    0.0015
Geocenter to KBO     58.63607157 +/-    0.0016
# Hcoef:  6.11

The following table shows the complete astrometric record for 14FE72. 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 (14FE72) followed by the observatory code and reference code for the source of the astrometry.

2014 03  26.11242  12 09 10.566  -12 59 00.28        14FE72    807  C~1x8j      
2014 03  26.17955  12 09 10.350  -12 58 59.36  23.9r 14FE72    807  C~1x8j      
2014 03  26.17955  12 09 10.30   -12 58 59.3   24.3V 14FE72    W84  C~2J9u      
2014 03  26.24892  12 09 10.105  -12 58 58.12        14FE72    807  C~1x8j      
2014 03  26.24892  12 09 10.07   -12 58 58.1         14FE72    W84  C~2J9u      
2014 05  01.01810  12 07 20.554  -12 46 56.00        14FE72    304  C~1x8j      
2014 05  01.10303  12 07 20.334  -12 46 54.05  23.6r 14FE72    304  C~1x8j      
2014 05  02.12025  12 07 17.756  -12 46 33.52        14FE72    304  C~1x8j      
2014 07  19.97907  12 06 51.593  -12 33 19.07        14FE72    I11  C~1x8j      
2014 07  20.04487  12 06 51.719  -12 33 19.13  23.7r 14FE72    I11  C~1x8j      
2015 01  18.29839  12 14 42.953  -13 40 26.48        14FE72    I11  C~1x8j      
2015 01  21.28680  12 14 39.469  -13 40 47.50        14FE72    I11  C~1x8j      
2015 03  02.129842 12 13 08.91   -13 39 04.4         14FE72    W84  C~5ZZr      
2015 12  09.31751  12 17 06.518  -14 02 02.66        14FE72    304  C~1x8j      
2015 12  09.34646  12 17 06.536  -14 02 03.32        14FE72    304  C~1x8j      
2018 05  14.25498  12 17 12.347  -14 54 11.79  23.9r 14FE72    G37  C~2fC5      
2018 05  14.26226  12 17 12.332  -14 54 11.86  24.0r 14FE72    G37  C~2fC5      
2018 05  15.29040  12 17 10.309  -14 53 52.02        14FE72    G37  C~2fC5      
2021 03  18.247327 12 27 09.95   -16 41 41.1         14FE72    W84  C~5ZZr      
2021 03  18.250082 12 27 09.91   -16 41 41.0         14FE72    W84  C~5ZZr      

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     0.19       0.00    -0.02
     2   0.0002      0.00    -0.36       0.00    -0.26
     3   0.0002      0.00     0.39       0.00    -0.32
     4   0.0004      0.00    -0.25       0.00    -0.33
     5   0.0004      0.00     0.27       0.00    -0.35
     6   0.0983      0.00     0.21       0.00     0.08
     7   0.0985      0.00     0.20       0.00     0.31
     8   0.1013      0.00    -0.13       0.00     0.20
     9   0.3172      0.00    -0.00       0.00     0.30
    10   0.3174      0.00    -0.04       0.00     0.53
    11   0.8164      0.00    -0.04       0.00     0.14
    12   0.8246      0.00     0.29       0.00     0.17
    13   0.9337      0.00    -0.42       0.00    -0.17
    14   1.7062      0.00    -0.03       0.00     0.08
    15   1.7063      0.00    -0.42       0.00     0.12
    16   4.1345      0.00    -0.15       0.00    -0.23
    17   4.1346      0.00    -0.16       0.00    -0.44
    18   4.1374      0.00     0.12       0.00    -0.18
    19   6.9792      0.00     0.36       0.00     0.18
    20   6.9792      0.00    -0.11       0.00     0.24

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.

14FE72    quality flag:3

Type:       CENTAURS  CENTAURS  CENTAURS

axisobj      1994.681  1995.494  1993.869
ecceobj         0.982     0.982     0.982
incobj         20.663    20.663    20.663
qmin           19.909    20.350    19.894
qmax         6402.089  7160.836  6937.479
amean        2066.424  1891.003  2045.287
amin         1676.560  1487.309  1549.184
amax         3219.185  3598.501  3486.854
emean           0.982     0.981     0.982
emin            0.972     0.969     0.971
emax            0.991     0.990     0.991
imean          21.926    21.908    21.935
imin           18.316    18.589    18.297
imax           27.632    26.944    27.137
excite_mean     1.051     1.049     1.051
fracstop        1.000     1.000     1.000
cjmean          2.881     2.881     2.881

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       134.6     134.7     134.7
kozaiamp         11.1      10.6      11.1