Orbit Fit and Astrometric record for 13RR109

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: 13RR109   
# Created Wed Dec 25 02:09:27 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     50 observations of     50
# Arc:   9.15y
# First observation: 2013/09/05
#  Last observation: 2022/10/29
# Chi-squared of fit:    19.18 DOF:     94 RMS:  0.11
# Min/Max residuals:    -0.29    0.36
# Exact a, adot, b, bdot, g, gdot:
  1.574009E-05  2.165976E-02 -6.288912E-07 -8.617525E-04  2.259125E-02  4.911171E-04
# Covariance matrix:
  1.5114E-13 -5.9019E-14 -1.9568E-15  1.9302E-15  4.7676E-14 -2.6534E-13
 -5.9019E-14  3.6594E-14  1.6906E-15 -1.4261E-15 -9.9568E-15  1.9595E-13
 -1.9568E-15  1.6906E-15  8.7251E-14 -1.7632E-14  5.6181E-16  1.0431E-14
  1.9302E-15 -1.4261E-15 -1.7632E-14  5.4095E-15  6.0065E-16 -8.9649E-15
  4.7676E-14 -9.9568E-15  5.6181E-16  6.0065E-16  1.3558E-13 -8.2950E-14
 -2.6534E-13  1.9595E-13  1.0431E-14 -8.9649E-15 -8.2950E-14  1.2319E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.661409  -11.691622    0.103688    0.064189   -1.001903  2456540.632498
# Heliocentric elements and errors
Epoch:              2456540.5000  =  2013/09/05
Mean Anomaly:           17.56285 +/-     0.039
Argument of Peri:      102.52929 +/-     0.045
Long of Asc Node:      225.89421 +/-     0.002
Inclination:             4.23288 +/-     0.000
Eccentricity:         0.05724391 +/-    0.0001
Semi-Major Axis:     47.86283371 +/-    0.0037
Time of Perihelion: 2450640.0047 +/-      13.2
Perihelion:          45.12297815 +/-    0.0046
Aphelion:            50.60268927 +/-    0.0050
Period (y)              331.1356 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           44.22005973 +/-    0.0007
Ecliptic Y           -9.25354138 +/-    0.0002
Ecliptic Z            2.82673816 +/-    0.0000
Ecliptic XDOT         0.00059045 +/-    0.0000
Ecliptic YDOT         0.00255600 +/-    0.0000
Ecliptic ZDOT        -0.00010028 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.26622417 +/-    0.0007
Geocenter to KBO     44.26494584 +/-    0.0007
# Hcoef:  6.91

The following table shows the complete astrometric record for 13RR109. 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 (13RR109) followed by the observatory code and reference code for the source of the astrometry.

2013 09  05.13172  23 11 16.635  -01 15 07.68  24.3g 13RR109   W84  C~4yQq      
2013 09  08.17151  23 11 04.111  -01 16 27.61  23.4g 13RR109   W84  C~4yQq      
2013 09  11.25883  23 10 51.385  -01 17 49.91  23.3g 13RR109   W84  C~4yQq      
2013 09  29.20901  23 09 39.234  -01 25 53.71  23.3r 13RR109   W84  C~4yQq      
2013 09  29.21180  23 09 39.226  -01 25 53.74  23.1i 13RR109   W84  C~4yQq      
2013 10  12.08076  23 08 52.807  -01 31 24.81  22.7i 13RR109   W84  C~4yQq      
2013 10  12.08921  23 08 52.792  -01 31 25.14  22.5z 13RR109   W84  C~4yQq      
2013 10  13.04683  23 08 49.623  -01 31 48.64  22.9z 13RR109   W84  C~4yQq      
2013 10  28.02795  23 08 06.376  -01 37 22.90  23.2r 13RR109   W84  C~4yQq      
2013 10  28.02934  23 08 06.364  -01 37 23.00  23.1i 13RR109   W84  C~4yQq      
2013 11  23.07047  23 07 27.556  -01 43 44.82  23.5r 13RR109   W84  C~4yQq      
2015 11  01.05271  23 17 10.245  -00 46 29.16  23.1r 13RR109   W84  C~4yQq      
2015 11  01.05410  23 17 10.259  -00 46 29.26  23.0i 13RR109   W84  C~4yQq      
2015 11  01.05547  23 17 10.253  -00 46 29.04  24.1g 13RR109   W84  C~4yQq      
2016 08  01.43571  23 27 14.05   +00 15 50.9   23.2z 13RR109   T09  C~7gpU      
2016 08  01.44598  23 27 14.03   +00 15 50.7   23.6z 13RR109   T09  C~7gpU      
2016 08  01.48420  23 27 13.91   +00 15 50.0   23.5z 13RR109   T09  C~7gpU      
2016 08  01.51671  23 27 13.80   +00 15 49.5   24.0z 13RR109   T09  C~7gpU      
2016 08  01.58729  23 27 13.59   +00 15 48.4   23.2z 13RR109   T09  C~7gpU      
2016 08  09.42245  23 26 49.53   +00 13 34.4   23.4y 13RR109   T09  C~7gpU      
2016 08  09.45205  23 26 49.42   +00 13 34.0   23.5y 13RR109   T09  C~7gpU      
2016 08  09.47657  23 26 49.35   +00 13 33.3   23.1y 13RR109   T09  C~7gpU      
2016 08  09.52904  23 26 49.17   +00 13 32.5   23.7y 13RR109   T09  C~7gpU      
2016 08  09.54843  23 26 49.09   +00 13 32.0   23.4y 13RR109   T09  C~7gpU      
2016 09  26.13353  23 23 43.648  -00 06 00.77  23.5r 13RR109   W84  C~4yQq      
2016 09  26.13489  23 23 43.639  -00 06 00.92  22.8i 13RR109   W84  C~4yQq      
2016 09  26.13627  23 23 43.640  -00 06 01.03  24.3g 13RR109   W84  C~4yQq      
2017 09  13.36589  23 29 14.02   +00 26 04.8   23.0y 13RR109   T09  C~85Dt      
2017 09  13.36941  23 29 14.00   +00 26 04.6   23.0y 13RR109   T09  C~85Dt      
2017 09  13.38367  23 29 13.94   +00 26 04.3   22.7y 13RR109   T09  C~85Dt      
2017 09  13.39746  23 29 13.89   +00 26 04.0   22.9y 13RR109   T09  C~85Dt      
2017 09  13.40105  23 29 13.87   +00 26 03.8   22.6y 13RR109   T09  C~85Dt      
2017 09  13.41178  23 29 13.83   +00 26 03.6   22.8y 13RR109   T09  C~85Dt      
2017 09  13.41536  23 29 13.82   +00 26 03.5   22.8y 13RR109   T09  C~85Dt      
2017 09  27.27630  23 28 17.32   +00 19 44.1   23.8z 13RR109   T09  C~7bI7      
2017 09  27.30436  23 28 17.20   +00 19 43.6   23.8z 13RR109   T09  C~7bI7      
2017 09  27.31840  23 28 17.13   +00 19 43.3   24.1z 13RR109   T09  C~7bI7      
2017 09  27.33246  23 28 17.08   +00 19 42.6   24.4z 13RR109   T09  C~7bI7      
2017 09  27.34659  23 28 17.02   +00 19 42.4   23.8z 13RR109   T09  C~7bI7      
2017 10  11.18778  23 27 24.305  +00 13 31.02  22.7i 13RR109   W84  C~4yQq      
2017 11  08.06827  23 26 04.182  +00 03 06.51  24.3g 13RR109   W84  C~4yQq      
2017 11  08.06964  23 26 04.167  +00 03 06.55  23.3r 13RR109   W84  C~4yQq      
2017 11  09.04198  23 26 02.257  +00 02 49.57  23.9g 13RR109   W84  C~4yQq      
2017 11  09.04336  23 26 02.245  +00 02 49.61  23.4r 13RR109   W84  C~4yQq      
2020 09  21.156020 23 42 33.313  +01 40 51.18  23.0G 13RR109   G37  C~49w4      
2020 09  21.193000 23 42 33.157  +01 40 49.97        13RR109   G37  C~49w4      
2020 09  21.261690 23 42 32.871  +01 40 48.15        13RR109   G37  C~49w4      
2022 10  29.096870 23 49 28.640  +02 16 27.23  23.4G 13RR109   G37  C~5z08      
2022 10  29.135190 23 49 28.533  +02 16 26.46        13RR109   G37  C~5z08      
2022 10  29.174000 23 49 28.407  +02 16 25.55        13RR109   G37  C~5z08      

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    -0.04
     2   0.0083      0.00     0.03       0.00     0.10
     3   0.0168      0.00     0.36       0.00     0.10
     4   0.0659      0.00    -0.05       0.00     0.04
     5   0.0659      0.00    -0.01       0.00     0.09
     6   0.1012      0.00    -0.15       0.00     0.02
     7   0.1012      0.00     0.06       0.00    -0.10
     8   0.1038      0.00     0.11       0.00    -0.19
     9   0.1448      0.00    -0.05       0.00     0.03
    10   0.1448      0.00    -0.17       0.00    -0.05
    11   0.2161      0.00    -0.03       0.00    -0.06
    12   2.1545      0.00    -0.03       0.00    -0.07
    13   2.1545      0.00     0.23       0.00    -0.14
    14   2.1545      0.00     0.19       0.00     0.10
    15   2.9057      0.00     0.06       0.00     0.14
    16   2.9057      0.00     0.21       0.00     0.10
    17   2.9058      0.00     0.09       0.00    -0.01
    18   2.9059      0.00    -0.13       0.00    -0.01
    19   2.9061      0.00    -0.16       0.00    -0.01
    20   2.9276      0.00    -0.01       0.00     0.03
    21   2.9276      0.00    -0.18       0.00     0.18
    22   2.9277      0.00     0.00       0.00    -0.07
    23   2.9279      0.00    -0.06       0.00     0.11
    24   2.9279      0.00    -0.29       0.00    -0.02
    25   3.0582      0.00     0.12       0.00     0.06
    26   3.0582      0.00     0.06       0.00    -0.06
    27   3.0582      0.00     0.16       0.00    -0.13
    28   4.0225      0.00    -0.04       0.00     0.06
    29   4.0226      0.00    -0.12       0.00    -0.04
    30   4.0226      0.00    -0.13       0.00     0.04
    31   4.0226      0.00    -0.01       0.00     0.11
    32   4.0226      0.00    -0.08       0.00     0.01
    33   4.0227      0.00    -0.01       0.00     0.10
    34   4.0227      0.00     0.07       0.00     0.10
    35   4.0606      0.00     0.21       0.00    -0.21
    36   4.0607      0.00     0.12       0.00     0.06
    37   4.0607      0.00    -0.08       0.00     0.14
    38   4.0608      0.00     0.03       0.00    -0.17
    39   4.0608      0.00    -0.01       0.00     0.02
    40   4.0987      0.00     0.05       0.00    -0.12
    41   4.1750      0.00     0.01       0.00    -0.14
    42   4.1751      0.00    -0.17       0.00    -0.08
    43   4.1777      0.00     0.06       0.00     0.01
    44   4.1777      0.00    -0.07       0.00     0.07
    45   7.0446      0.00     0.09       0.00     0.12
    46   7.0447      0.00     0.05       0.00    -0.07
    47   7.0448      0.00     0.05       0.00    -0.01
    48   9.1471      0.00    -0.12       0.00    -0.10
    49   9.1472      0.00     0.06       0.00     0.02
    50   9.1473      0.00    -0.03       0.00     0.02

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.

13RR109    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        48.142    48.142    48.142
ecceobj         0.063     0.063     0.063
incobj          4.232     4.232     4.232
qmin           43.956    43.958    43.952
qmax           52.359    52.350    52.370
amean          47.973    47.973    47.973
amin           47.550    47.550    47.550
amax           48.406    48.405    48.406
emean           0.061     0.061     0.061
emin            0.039     0.039     0.039
emax            0.082     0.082     0.082
imean           5.373     5.373     5.373
imin            5.084     5.084     5.085
imax            5.681     5.681     5.681
excite_mean     0.112     0.112     0.112
fracstop        1.000     1.000     1.000
cjmean          3.136     3.136     3.136

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       180.6     180.7     180.7
kozaiamp        180.0     180.0     179.9