Orbit Fit and Astrometric record for 14JE80

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: 14JE80    
# Created Fri Mar 29 01:16:40 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     64 observations of     64
# Arc:   6.32y
# First observation: 2011/04/13
#  Last observation: 2017/08/08
# Chi-squared of fit:    43.35 DOF:    122 RMS:  0.15
# Min/Max residuals:    -0.44    0.40
# Exact a, adot, b, bdot, g, gdot:
  2.678471E-05  8.746284E-02 -2.595203E-06 -9.035876E-03  5.056346E-02 -3.069876E-02
# Covariance matrix:
  4.6608E-13 -2.0020E-13 -4.0241E-14  2.0080E-14 -2.8091E-14 -1.8955E-13
 -2.0020E-13  1.0240E-13  2.1355E-14 -1.0373E-14  3.6680E-14  1.0265E-13
 -4.0241E-14  2.1355E-14  1.5401E-13 -3.3568E-14  3.0798E-15  2.4014E-14
  2.0080E-14 -1.0373E-14 -3.3568E-14  8.5162E-15 -2.9096E-16 -1.1894E-14
 -2.8091E-14  3.6680E-14  3.0798E-15 -2.9096E-16  9.7853E-14  2.3562E-14
 -1.8955E-13  1.0265E-13  2.4014E-14 -1.1894E-14  2.3562E-14  1.1375E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
   28.852498 -140.041331    0.295968    0.464082   -0.842424  2455664.881776
# Heliocentric elements and errors
Epoch:              2455664.5000  =  2011/04/13
Mean Anomaly:          356.66226 +/-     0.001
Argument of Peri:      146.46341 +/-     0.001
Long of Asc Node:      116.36119 +/-     0.000
Inclination:            28.14829 +/-     0.000
Eccentricity:         0.79944813 +/-    0.0000
Semi-Major Axis:     89.31823061 +/-    0.0121
Time of Perihelion: 2458523.1301 +/-      62.1
Perihelion:          17.91293783 +/-    0.0033
Aphelion:           160.72352338 +/-    0.0219
Period (y)              844.1476 +/-      0.17
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -14.20045904 +/-    0.0001
Ecliptic Y          -11.51619843 +/-    0.0001
Ecliptic Z            9.54356377 +/-    0.0001
Ecliptic XDOT         0.00397476 +/-    0.0000
Ecliptic YDOT        -0.00284069 +/-    0.0000
Ecliptic ZDOT        -0.00123063 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   20.62434296 +/-    0.0001
Geocenter to KBO     19.77734261 +/-    0.0001
# Hcoef:  9.66

The following table shows the complete astrometric record for 14JE80. 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 (14JE80) followed by the observatory code and reference code for the source of the astrometry.

2011 04  13.38101  15 06 05.632  +12 38 57.47  23.2G 14JE80    F51  C~2qbE      
2011 04  14.51807  15 05 57.143  +12 40 03.02  23.5G 14JE80    F51  C~2qbE      
2012 05  20.49973  15 20 05.504  +10 52 08.12  22.6G 14JE80    F51  C~2qbE      
2012 08  11.27189  15 14 23.007  +09 37 25.21  22.4G 14JE80    F51  C~2qbE      
2014 04  23.57959  16 05 14.219  +05 44 39.53  21.5G 14JE80    F51  C~2qbE      
2014 05  04.41804  16 03 47.753  +05 52 10.89  22.6w 14JE80    F51  C~1vXS      
2014 05  04.43005  16 03 47.660  +05 52 11.49  22.4w 14JE80    F51  C~1vXS      
2014 05  04.44210  16 03 47.547  +05 52 11.85  22.4w 14JE80    F51  C~1vXS      
2014 05  08.37578  16 03 13.688  +05 54 22.15  21.3G 14JE80    F51  C~2qbE      
2014 05  08.38850  16 03 13.572  +05 54 22.40  22.7G 14JE80    F51  C~2qbE      
2014 05  08.40076  16 03 13.451  +05 54 22.72  22.6G 14JE80    F51  C~2qbE      
2014 05  08.41303  16 03 13.321  +05 54 23.06  22.0G 14JE80    F51  C~2qbE      
2014 05  09.40835  16 03 04.607  +05 54 52.69  22.3G 14JE80    F51  C~2qbE      
2014 05  09.42082  16 03 04.497  +05 54 52.87  21.6G 14JE80    F51  C~2qbE      
2014 05  09.43331  16 03 04.385  +05 54 53.45  22.0G 14JE80    F51  C~2qbE      
2014 05  09.44586  16 03 04.280  +05 54 53.81  22.2G 14JE80    F51  C~2qbE      
2014 05  09.53302  16 03 03.477  +05 54 56.32  22.4w 14JE80    F51  C~1vXS      
2014 05  09.54516  16 03 03.389  +05 54 56.48  22.3w 14JE80    F51  C~1vXS      
2014 05  09.55726  16 03 03.278  +05 54 57.12  22.5w 14JE80    F51  C~1vXS      
2014 05  09.56935  16 03 03.166  +05 54 57.48  22.3w 14JE80    F51  C~1vXS      
2014 05  10.37677  16 02 56.073  +05 55 20.48  22.2G 14JE80    F51  C~2qbE      
2014 05  10.38882  16 02 55.971  +05 55 20.68  21.5G 14JE80    F51  C~2qbE      
2014 05  10.40084  16 02 55.837  +05 55 21.05  22.2G 14JE80    F51  C~2qbE      
2014 05  10.41289  16 02 55.744  +05 55 21.42  22.0G 14JE80    F51  C~2qbE      
2014 05  28.33463  16 00 12.190  +05 59 58.84  22.5w 14JE80    F51  C~1vXS      
2014 05  28.34685  16 00 12.072  +05 59 59.21  22.2w 14JE80    F51  C~1vXS      
2014 05  28.35901  16 00 11.954  +05 59 59.00  22.3w 14JE80    F51  C~1vXS      
2014 06  15.45904  15 57 32.802  +05 56 25.93  22.8G 14JE80    F51  C~2qbE      
2014 07  01.36997  15 55 35.692  +05 46 20.82  22.5w 14JE80    F51  C~1vXS      
2014 07  01.38199  15 55 35.608  +05 46 20.34  22.5w 14JE80    F51  C~1vXS      
2014 07  01.39399  15 55 35.532  +05 46 19.59  22.5w 14JE80    F51  C~1vXS      
2014 07  01.40599  15 55 35.451  +05 46 19.21  22.6w 14JE80    F51  C~1vXS      
2015 03  23.56273  16 29 17.624  +02 34 23.10  18.7G 14JE80    F51  C~2qbE      
2015 05  13.50306  16 24 25.754  +03 13 39.53  22.3G 14JE80    F51  C~2qbE      
2015 06  20.31280  16 18 40.565  +03 12 25.80  22.3w 14JE80    F51  C~2HP5      
2015 06  20.32543  16 18 40.461  +03 12 25.27  22.8w 14JE80    F51  C~2HP5      
2015 06  20.33811  16 18 40.348  +03 12 24.98  22.5w 14JE80    F51  C~2HP5      
2015 06  20.35081  16 18 40.245  +03 12 24.66  22.2w 14JE80    F51  C~2HP5      
2015 06  21.46238  16 18 30.946  +03 11 51.17  22.4G 14JE80    F51  C~2qbE      
2015 08  17.27570  16 14 34.982  +02 08 21.39  22.5G 14JE80    F51  C~2qbE      
2016 04  03.59873  16 51 03.093  -00 02 03.99  22.3G 14JE80    F51  C~2qbE      
2016 05  06.52512  16 47 58.902  +00 20 19.35  22.5G 14JE80    F51  C~2qbE      
2016 05  06.53716  16 47 58.788  +00 20 19.71  23.0G 14JE80    F51  C~2qbE      
2016 05  29.58603  16 44 32.849  +00 26 19.57  22.1G 14JE80    F51  C~2qbE      
2016 06  03.47192  16 43 46.271  +00 26 12.95  21.9G 14JE80    F51  C~2qbE      
2016 06  03.48310  16 43 46.154  +00 26 12.82  22.1G 14JE80    F51  C~2qbE      
2016 06  03.49429  16 43 46.056  +00 26 12.78  22.3G 14JE80    F51  C~2qbE      
2016 06  03.50547  16 43 45.939  +00 26 12.51  22.2G 14JE80    F51  C~2qbE      
2016 06  23.43390  16 40 41.782  +00 20 10.20  22.8G 14JE80    F51  C~2qbE      
2016 07  05.39769  16 39 05.110  +00 12 16.12  22.4G 14JE80    F51  C~2qbE      
2016 07  05.40974  16 39 05.004  +00 12 15.37  22.4G 14JE80    F51  C~2qbE      
2016 07  05.42181  16 39 04.936  +00 12 15.00  22.3G 14JE80    F51  C~2qbE      
2017 05  06.57371  17 11 18.426  -02 34 36.51  21.9G 14JE80    F51  C~2qbE      
2017 05  26.36009  17 08 30.61   -02 29 50.0   22.3R 14JE80    G37  C~2HP5      
2017 05  26.42000  17 08 30.06   -02 29 49.9         14JE80    G37  C~2HP5      
2017 06  23.35807  17 04 03.710  -02 35 30.22  22.3G 14JE80    F51  C~2qbE      
2017 06  23.37201  17 04 03.591  -02 35 30.40  22.7G 14JE80    F51  C~2qbE      
2017 06  23.38595  17 04 03.472  -02 35 30.87  23.9G 14JE80    F51  C~2qbE      
2017 06  23.39985  17 04 03.326  -02 35 31.31  22.5G 14JE80    F51  C~2qbE      
2017 06  23.40342  17 04 03.296  -02 35 31.12  22.5G 14JE80    F51  C~2qbE      
2017 06  23.41430  17 04 03.189  -02 35 31.59  22.4G 14JE80    F51  C~2qbE      
2017 06  23.42519  17 04 03.091  -02 35 31.92  22.3G 14JE80    F51  C~2qbE      
2017 06  23.43607  17 04 02.991  -02 35 32.24  22.5G 14JE80    F51  C~2qbE      
2017 08  08.29193  16 59 04.218  -03 17 15.26  22.5G 14JE80    F51  C~2qbE      

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     0.10       0.00    -0.08
     2   0.0031      0.00    -0.02       0.00    -0.04
     3   1.1037      0.00     0.02       0.00     0.04
     4   1.3303      0.00    -0.06       0.00    -0.20
     5   3.0286      0.00    -0.21       0.00     0.13
     6   3.0583      0.00    -0.09       0.00     0.04
     7   3.0583      0.00     0.08       0.00     0.21
     8   3.0583      0.00    -0.05       0.00     0.14
     9   3.0691      0.00     0.18       0.00     0.37
    10   3.0692      0.00     0.14       0.00     0.23
    11   3.0692      0.00    -0.04       0.00     0.17
    12   3.0692      0.00    -0.34       0.00     0.14
    13   3.0719      0.00    -0.05       0.00    -0.00
    14   3.0720      0.00    -0.02       0.00    -0.19
    15   3.0720      0.00    -0.02       0.00     0.02
    16   3.0720      0.00     0.10       0.00     0.02
    17   3.0723      0.00    -0.18       0.00    -0.01
    18   3.0723      0.00     0.14       0.00    -0.21
    19   3.0724      0.00     0.10       0.00     0.08
    20   3.0724      0.00     0.05       0.00     0.09
    21   3.0746      0.00     0.14       0.00     0.05
    22   3.0746      0.00     0.24       0.00    -0.09
    23   3.0747      0.00    -0.14       0.00    -0.05
    24   3.0747      0.00     0.10       0.00    -0.02
    25   3.1238      0.00     0.01       0.00    -0.26
    26   3.1238      0.00    -0.04       0.00     0.07
    27   3.1238      0.00    -0.11       0.00    -0.16
    28   3.1734      0.00    -0.25       0.00    -0.35
    29   3.2169      0.00     0.02       0.00    -0.10
    30   3.2170      0.00    -0.06       0.00     0.03
    31   3.2170      0.00    -0.02       0.00    -0.12
    32   3.2170      0.00    -0.05       0.00     0.10
    33   3.9430      0.00     0.15       0.00     0.09
    34   4.0825      0.00     0.19       0.00     0.05
    35   4.1860      0.00    -0.05       0.00     0.10
    36   4.1860      0.00     0.01       0.00    -0.06
    37   4.1861      0.00    -0.05       0.00     0.02
    38   4.1861      0.00     0.05       0.00     0.08
    39   4.1891      0.00     0.15       0.00     0.22
    40   4.3447      0.00     0.14       0.00     0.10
    41   4.9753      0.00     0.21       0.00     0.04
    42   5.0654      0.00    -0.00       0.00    -0.04
    43   5.0655      0.00    -0.23       0.00    -0.02
    44   5.1286      0.00    -0.02       0.00    -0.28
    45   5.1419      0.00     0.18       0.00     0.14
    46   5.1420      0.00     0.06       0.00     0.06
    47   5.1420      0.00     0.22       0.00     0.07
    48   5.1420      0.00     0.10       0.00    -0.14
    49   5.1966      0.00    -0.13       0.00    -0.04
    50   5.2293      0.00    -0.08       0.00    -0.14
    51   5.2294      0.00    -0.30       0.00    -0.32
    52   5.2294      0.00     0.06       0.00    -0.12
    53   6.0649      0.00    -0.04       0.00    -0.09
    54   6.1190      0.00    -0.44       0.00     0.40
    55   6.1192      0.00    -0.17       0.00     0.25
    56   6.1957      0.00    -0.14       0.00    -0.24
    57   6.1957      0.00     0.04       0.00    -0.01
    58   6.1958      0.00     0.23       0.00    -0.08
    59   6.1958      0.00    -0.00       0.00    -0.11
    60   6.1958      0.00     0.05       0.00     0.18
    61   6.1958      0.00    -0.02       0.00     0.03
    62   6.1959      0.00     0.05       0.00     0.01
    63   6.1959      0.00     0.09       0.00     0.01
    64   6.3215      0.00     0.05       0.00    -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.

14JE80    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        88.325    88.322    88.328
ecceobj         0.797     0.797     0.797
incobj         28.148    28.148    28.148
qmin           17.302    17.452    17.485
qmax          178.549   168.349   171.503
amean          93.548    85.902    92.764
amin           87.010    81.537    88.328
amax           98.172    93.151    94.736
emean           0.809     0.792     0.807
emin            0.792     0.778     0.797
emax            0.819     0.807     0.812
imean          26.265    26.658    26.479
imin           25.728    26.308    26.186
imax           26.911    26.936    26.745
excite_mean     0.922     0.910     0.922
fracstop        0.032     0.011     0.003
cjmean          2.185     2.198     2.185

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       151.2     148.0     147.1
kozaiamp          4.6       1.8       0.9