Orbit Fit and Astrometric record for 523709

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: 523709    
# Created Sun Dec 22 02:07:20 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     79 observations of     79
# Arc:  12.24y
# First observation: 2012/06/14
#  Last observation: 2024/09/08
# Chi-squared of fit:    46.25 DOF:    152 RMS:  0.14
# Min/Max residuals:    -0.31    0.41
# Exact a, adot, b, bdot, g, gdot:
  1.841481E-05  5.636673E-02 -1.485995E-05 -4.543988E-02  4.960876E-02 -1.236289E-02
# Covariance matrix:
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.745519  -67.525982    0.492923   -0.027173   -0.890309  2456092.984286
# Heliocentric elements and errors
Epoch:              2456092.5000  =  2012/06/14
Mean Anomaly:          322.77965 +/-     0.000
Argument of Peri:      242.26622 +/-     0.000
Long of Asc Node:      109.08407 +/-     0.000
Inclination:            39.11857 +/-     0.000
Eccentricity:         0.25026630 +/-    0.0000
Semi-Major Axis:     25.30259263 +/-    0.0000
Time of Perihelion: 2460898.9448 +/-       0.0
Perihelion:          18.97020627 +/-    0.0000
Aphelion:            31.63497899 +/-    0.0000
Period (y)              127.2787 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            7.58979803 +/-    0.0000
Ecliptic Y          -19.62753842 +/-    0.0000
Ecliptic Z           -0.61425298 +/-    0.0000
Ecliptic XDOT         0.00257943 +/-    0.0000
Ecliptic YDOT         0.00189319 +/-    0.0000
Ecliptic ZDOT        -0.00248572 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   21.05294086 +/-    0.0000
Geocenter to KBO     20.15783270 +/-    0.0000
# Hcoef:  9.01

The following table shows the complete astrometric record for 523709. 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 (523709) followed by the observatory code and reference code for the source of the astrometry.

2012 06  14.48352  19 38 19.378  -23 17 14.62  23.1G 523709    F51  C~2kQ8      
2013 06  18.51850  19 53 59.808  -25 21 04.73  22.2w 523709    F51  C~1vXS      
2013 06  18.53163  19 53 59.699  -25 21 05.24  22.2w 523709    F51  C~1vXS      
2013 06  18.54474  19 53 59.592  -25 21 06.02  22.4w 523709    F51  C~1vXS      
2013 06  30.50586  19 52 12.711  -25 32 09.46  21.9G 523709    F51  C~2kQ8      
2013 07  04.44930  19 51 34.903  -25 35 47.16  22.1G 523709    F51  C~2kQ8      
2013 07  04.46187  19 51 34.764  -25 35 47.63  21.9G 523709    F51  C~2kQ8      
2013 07  04.47445  19 51 34.652  -25 35 48.41  22.4G 523709    F51  C~2kQ8      
2013 07  17.47978  19 49 24.856  -25 47 28.75  23.1G 523709    F51  C~2kQ8      
2014 05  09.59290  20 14 15.288  -26 39 11.91  22.2w 523709    F51  C~1vXS      
2014 05  09.60022  20 14 15.307  -26 39 12.63  22.2w 523709    F51  C~1vXS      
2014 05  09.60754  20 14 15.279  -26 39 12.66  22.0w 523709    F51  C~1vXS      
2014 05  23.57153  20 13 44.409  -26 51 22.93  22.5G 523709    F51  C~2kQ8      
2014 06  04.56414  20 12 47.858  -27 03 00.65  22.9G 523709    F51  C~2kQ8      
2014 06  04.58612  20 12 47.726  -27 03 01.78  22.5G 523709    F51  C~2kQ8      
2014 06  04.59721  20 12 47.641  -27 03 02.73  22.8G 523709    F51  C~2kQ8      
2014 06  10.54925  20 12 10.283  -27 09 05.74  22.3G 523709    F51  C~2kQ8      
2014 06  20.59241  20 10 55.085  -27 19 32.20  22.3G 523709    F51  C~2kQ8      
2014 06  30.49035  20 09 28.610  -27 29 53.95  21.9G 523709    F51  C~2kQ8      
2014 07  29.40701  20 04 38.923  -27 58 07.09  22.1w 523709    F51  C~1vXS      
2014 07  29.41827  20 04 38.797  -27 58 07.80  22.0w 523709    F51  C~1vXS      
2014 07  29.42952  20 04 38.680  -27 58 08.50  22.1w 523709    F51  C~1vXS      
2014 07  29.44076  20 04 38.569  -27 58 08.91  22.4w 523709    F51  C~1vXS      
2014 07  31.41890  20 04 18.435  -27 59 52.30  21.3G 523709    F51  C~2kQ8      
2014 08  15.36223  20 01 52.918  -28 11 35.22  22.2G 523709    F51  C~2kQ8      
2014 08  22.37761  20 00 51.090  -28 16 14.55  22.2w 523709    F51  C~1vXS      
2014 08  22.38909  20 00 50.986  -28 16 14.75  22.5w 523709    F51  C~1vXS      
2014 08  22.40057  20 00 50.880  -28 16 15.21  22.4w 523709    F51  C~1vXS      
2014 08  22.41202  20 00 50.792  -28 16 15.63  22.2w 523709    F51  C~1vXS      
2014 08  23.31669  20 00 43.257  -28 16 49.12  22.1w 523709    F51  C~1vXS      
2014 08  23.32800  20 00 43.184  -28 16 49.43  22.3w 523709    F51  C~1vXS      
2014 08  23.33934  20 00 43.052  -28 16 50.04  22.4w 523709    F51  C~1vXS      
2014 08  23.35063  20 00 42.967  -28 16 50.16  22.3w 523709    F51  C~1vXS      
2015 07  24.43556  20 23 51.118  -29 48 21.37  22.2w 523709    F51  C~1vXS      
2015 07  24.44587  20 23 51.003  -29 48 22.06  22.3w 523709    F51  C~1vXS      
2015 07  24.45618  20 23 50.895  -29 48 22.58  22.0w 523709    F51  C~1vXS      
2015 07  24.46650  20 23 50.794  -29 48 23.27  21.8w 523709    F51  C~1vXS      
2016 07  12.44642  20 45 13.056  -31 22 30.11  22.3G 523709    F51  C~2kQ8      
2016 07  12.45609  20 45 12.967  -31 22 30.68  23.0G 523709    F51  C~2kQ8      
2016 07  12.46577  20 45 12.875  -31 22 31.56  22.2G 523709    F51  C~2kQ8      
2016 07  12.47544  20 45 12.758  -31 22 32.30  22.6G 523709    F51  C~2kQ8      
2016 08  07.39420  20 40 43.323  -31 51 17.30  22.0G 523709    F51  C~2kQ8      
2016 08  07.40516  20 40 43.206  -31 51 18.18  22.0G 523709    F51  C~2kQ8      
2016 08  07.41613  20 40 43.074  -31 51 18.80  22.4G 523709    F51  C~2kQ8      
2016 08  07.42711  20 40 42.969  -31 51 19.19  21.5G 523709    F51  C~2kQ8      
2016 08  10.36976  20 40 12.204  -31 54 02.41  22.2G 523709    F51  C~2kQ8      
2017 06  22.54924  21 08 31.567  -32 30 22.67  22.2G 523709    F51  C~2kQ8      
2017 06  22.56134  21 08 31.484  -32 30 23.69  21.9G 523709    F51  C~2kQ8      
2017 06  22.57343  21 08 31.399  -32 30 24.76  22.6G 523709    F51  C~2kQ8      
2017 06  22.58551  21 08 31.318  -32 30 25.90  22.0G 523709    F51  C~2kQ8      
2017 06  23.55089  21 08 24.901  -32 31 49.59  22.1G 523709    F51  C~2kQ8      
2017 06  23.56070  21 08 24.844  -32 31 50.49  22.3G 523709    F51  C~2kQ8      
2017 06  23.57049  21 08 24.766  -32 31 51.32  22.4G 523709    F51  C~2kQ8      
2017 06  23.58029  21 08 24.696  -32 31 51.97  22.1G 523709    F51  C~2kQ8      
2017 08  14.34968  21 00 09.465  -33 37 48.19  22.4G 523709    F51  C~2kQ8      
2017 08  14.35967  21 00 09.374  -33 37 48.65  22.2G 523709    F51  C~2kQ8      
2017 08  14.36965  21 00 09.244  -33 37 49.23  21.8G 523709    F51  C~2kQ8      
2017 08  14.37962  21 00 09.146  -33 37 49.88  21.6G 523709    F51  C~2kQ8      
2020 08  14.40717  22 08 58.382  -37 22 21.97  21.2w 523709    F51  C~46kk      
2020 08  14.41685  22 08 58.282  -37 22 22.77  21.5w 523709    F51  C~46kk      
2020 08  14.43613  22 08 58.067  -37 22 24.16  21.3w 523709    F51  C~46kk      
2022 07  26.484613 23 02 13.197  -37 51 43.90  21.6w 523709    F52  C~5kPj      
2022 07  26.494072 23 02 13.121  -37 51 44.66  21.7w 523709    F52  C~5kPj      
2022 07  26.503624 23 02 13.070  -37 51 45.80  21.6w 523709    F52  C~5kPj      
2022 07  26.513168 23 02 13.008  -37 51 46.73  21.8w 523709    F52  C~5kPj      
2022 08  05.521160 23 00 53.860  -38 10 18.40  21.7w 523709    F52  C~5kPj      
2022 08  05.530082 23 00 53.776  -38 10 19.40  21.8w 523709    F52  C~5kPj      
2022 08  05.538929 23 00 53.685  -38 10 20.46  21.6w 523709    F52  C~5kPj      
2023 08  20.438233 23 24 28.634  -38 37 05.96  21.3w 523709    F52  C~78vu      
2023 08  20.438912 23 24 28.620  -38 37 06.01  21.6w 523709    F52  C~78vu      
2023 08  20.447237 23 24 28.529  -38 37 06.56  21.4w 523709    F52  C~78vu      
2023 08  20.447905 23 24 28.526  -38 37 06.86  21.6w 523709    F52  C~78vu      
2023 08  20.456303 23 24 28.476  -38 37 07.75  21.5w 523709    F52  C~78vu      
2023 08  20.456975 23 24 28.458  -38 37 07.54  21.5w 523709    F52  C~78vu      
2023 08  20.465321 23 24 28.365  -38 37 08.32  21.7w 523709    F52  C~78vu      
2023 08  20.466006 23 24 28.362  -38 37 08.66  21.7w 523709    F52  C~78vu      
2024 09  08.407007 23 47 08.046  -38 49 03.11  21.3w 523709    F51  C~8Fil      
2024 09  08.417361 23 47 07.898  -38 49 03.97  21.5w 523709    F51  C~8Fil      
2024 09  08.427697 23 47 07.806  -38 49 04.52  21.1w 523709    F51  C~8Fil      

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    -0.11       0.00     0.06
     2   1.0104      0.00    -0.19       0.00    -0.12
     3   1.0104      0.00    -0.14       0.00     0.10
     4   1.0104      0.00    -0.07       0.00     0.04
     5   1.0432      0.00    -0.04       0.00    -0.16
     6   1.0540      0.00     0.14       0.00    -0.15
     7   1.0540      0.00    -0.08       0.00     0.07
     8   1.0540      0.00     0.11       0.00    -0.02
     9   1.0897      0.00     0.24       0.00    -0.15
    10   1.9004      0.00    -0.20       0.00     0.05
    11   1.9004      0.00     0.19       0.00    -0.31
    12   1.9004      0.00    -0.12       0.00     0.02
    13   1.9386      0.00    -0.13       0.00    -0.08
    14   1.9715      0.00     0.18       0.00    -0.01
    15   1.9715      0.00     0.17       0.00     0.18
    16   1.9716      0.00    -0.11       0.00    -0.10
    17   1.9879      0.00     0.28       0.00    -0.09
    18   2.0154      0.00    -0.05       0.00     0.02
    19   2.0425      0.00     0.16       0.00    -0.02
    20   2.1216      0.00    -0.01       0.00     0.22
    21   2.1217      0.00    -0.14       0.00     0.11
    22   2.1217      0.00    -0.14       0.00    -0.00
    23   2.1217      0.00    -0.05       0.00     0.18
    24   2.1271      0.00     0.29       0.00    -0.12
    25   2.1680      0.00     0.09       0.00     0.11
    26   2.1873      0.00    -0.03       0.00    -0.09
    27   2.1873      0.00    -0.11       0.00     0.14
    28   2.1873      0.00    -0.21       0.00     0.10
    29   2.1873      0.00    -0.06       0.00     0.10
    30   2.1898      0.00     0.06       0.00     0.03
    31   2.1899      0.00     0.41       0.00     0.14
    32   2.1899      0.00    -0.13       0.00    -0.06
    33   2.1899      0.00     0.03       0.00     0.24
    34   3.1073      0.00     0.04       0.00    -0.02
    35   3.1074      0.00    -0.04       0.00    -0.08
    36   3.1074      0.00    -0.01       0.00     0.03
    37   3.1074      0.00     0.12       0.00    -0.03
    38   4.0766      0.00     0.09       0.00    -0.12
    39   4.0766      0.00     0.20       0.00     0.03
    40   4.0766      0.00     0.28       0.00    -0.13
    41   4.0766      0.00    -0.03       0.00    -0.15
    42   4.1476      0.00    -0.07       0.00     0.20
    43   4.1476      0.00    -0.06       0.00    -0.05
    44   4.1477      0.00    -0.27       0.00    -0.05
    45   4.1477      0.00    -0.08       0.00     0.18
    46   4.1557      0.00     0.17       0.00    -0.07
    47   5.0214      0.00     0.08       0.00     0.04
    48   5.0214      0.00     0.06       0.00     0.07
    49   5.0215      0.00     0.02       0.00     0.05
    50   5.0215      0.00     0.03       0.00    -0.05
    51   5.0241      0.00    -0.10       0.00    -0.08
    52   5.0242      0.00     0.07       0.00    -0.13
    53   5.0242      0.00    -0.08       0.00    -0.11
    54   5.0242      0.00    -0.11       0.00     0.09
    55   5.1660      0.00    -0.08       0.00    -0.09
    56   5.1660      0.00     0.18       0.00     0.02
    57   5.1660      0.00    -0.16       0.00     0.00
    58   5.1660      0.00    -0.01       0.00    -0.08
    59   8.1668      0.00    -0.05       0.00    -0.05
    60   8.1668      0.00     0.05       0.00    -0.08
    61   8.1669      0.00     0.01       0.00     0.07
    62  10.1136      0.00    -0.13       0.00    -0.26
    63  10.1136      0.00    -0.24       0.00     0.07
    64  10.1137      0.00     0.04       0.00     0.03
    65  10.1137      0.00     0.16       0.00     0.19
    66  10.1411      0.00    -0.05       0.00     0.17
    67  10.1411      0.00    -0.12       0.00     0.12
    68  10.1412      0.00    -0.30       0.00     0.01
    69  11.1813      0.00     0.04       0.00    -0.14
    70  11.1813      0.00    -0.06       0.00    -0.13
    71  11.1813      0.00    -0.19       0.00     0.15
    72  11.1813      0.00    -0.14       0.00    -0.08
    73  11.1813      0.00     0.36       0.00    -0.14
    74  11.1813      0.00     0.19       0.00     0.14
    75  11.1813      0.00     0.04       0.00     0.18
    76  11.1813      0.00     0.09       0.00    -0.09
    77  12.2352      0.00     0.24       0.00    -0.06
    78  12.2353      0.00    -0.28       0.00    -0.12
    79  12.2353      0.00     0.04       0.00     0.11

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.

523709    quality flag:2

Type:       CENTAURR  CENTAURS  CENTAURR

axisobj        25.233    25.233    25.233
ecceobj         0.251     0.251     0.251
incobj         39.112    39.112    39.112
qmin           16.805    15.827    16.823
qmax           33.971    34.739    33.891
amean          25.133    25.176    25.092
amin           24.577    24.623    24.377
amax           25.525    25.537    25.534
emean           0.257     0.260     0.245
emin            0.138     0.112     0.146
emax            0.331     0.369     0.330
imean          36.903    37.054    37.187
imin           35.320    34.435    35.335
imax           38.956    39.817    39.113
excite_mean     0.656     0.659     0.654
fracstop        0.079     1.000     0.288
cjmean          2.600     2.601     2.602

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       265.4     270.6     243.2
kozaiamp        179.7     179.8     179.4