Orbit Fit and Astrometric record for 729736

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: 729736    
# Created Sun Nov 24 02:07:51 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     82 observations of     82
# Arc:  12.37y
# First observation: 2010/07/19
#  Last observation: 2022/12/02
# Chi-squared of fit:   207.51 DOF:    158 RMS:  0.28
# Min/Max residuals:    -0.88    1.05
# Exact a, adot, b, bdot, g, gdot:
  3.369606E-05  2.753600E-01  1.004963E-05  9.040030E-02  1.325860E-01 -4.047378E-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
   -8.104981  -64.703844   -0.018228   -0.142837   -1.002536  2455396.911706
# Heliocentric elements and errors
Epoch:              2455396.5000  =  2010/07/19
Mean Anomaly:          300.72843 +/-     0.000
Argument of Peri:       52.78249 +/-     0.000
Long of Asc Node:      316.05532 +/-     0.000
Inclination:            19.59579 +/-     0.000
Eccentricity:         0.14286128 +/-    0.0000
Semi-Major Axis:      9.05967673 +/-    0.0000
Time of Perihelion: 2457036.3776 +/-       0.0
Perihelion:           7.76539974 +/-    0.0000
Aphelion:            10.35395372 +/-    0.0000
Period (y)               27.2695 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            3.64417713 +/-    0.0000
Ecliptic Y           -7.66036676 +/-    0.0000
Ecliptic Z           -1.06323899 +/-    0.0000
Ecliptic XDOT         0.00490086 +/-    0.0000
Ecliptic YDOT         0.00294596 +/-    0.0000
Ecliptic ZDOT         0.00196589 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO    8.54940377 +/-    0.0000
Geocenter to KBO      7.54234042 +/-    0.0000
# Hcoef: 12.71

The following table shows the complete astrometric record for 729736. 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 (729736) followed by the observatory code and reference code for the source of the astrometry.

2010 07  19.41094  19 55 44.948  -29 02 18.28  21.3G 729736    F51  C~2jgy      
2010 07  19.42193  19 55 44.694  -29 02 18.34  21.8G 729736    F51  C~2jgy      
2010 07  20.38650  19 55 21.825  -29 02 25.31  21.1G 729736    F51  C~2jgy      
2010 07  20.39769  19 55 21.549  -29 02 25.70  21.8G 729736    F51  C~2jgy      
2010 08  01.37207  19 50 41.190  -29 01 58.73  21.7G 729736    F51  C~2jgy      
2010 08  01.38419  19 50 40.902  -29 01 58.37  21.8G 729736    F51  C~2jgy      
2011 07  26.44014  20 57 03.762  -19 44 58.92  21.6w 729736    F51  C~0XJW      
2011 07  26.45390  20 57 03.442  -19 44 59.38  21.7w 729736    F51  C~0XJW      
2011 07  26.46766  20 57 03.134  -19 44 59.91  21.6w 729736    F51  C~0XJW      
2011 07  26.48142  20 57 02.825  -19 45 00.35  21.6w 729736    F51  C~0XJW      
2011 07  27.43307  20 56 41.627  -19 45 31.17  21.7G 729736    F51  C~2jgy      
2011 07  27.44273  20 56 41.432  -19 45 31.66  22.0G 729736    F51  C~2jgy      
2011 07  27.45325  20 56 41.176  -19 45 32.04  21.8G 729736    F51  C~2jgy      
2011 07  27.46250  20 56 40.963  -19 45 32.29  21.2G 729736    F51  C~2jgy      
2011 07  29.431908 20 55 56.812  -19 46 35.38  21.3R 729736    568  C~0XJW      
2011 07  29.433242 20 55 56.780  -19 46 35.46  21.2R 729736    568  C~0XJW      
2011 07  29.434731 20 55 56.749  -19 46 35.50  21.2R 729736    568  C~0XJW      
2011 07  29.435954 20 55 56.719  -19 46 35.54  21.1R 729736    568  C~0XJW      
2011 07  31.240885 20 55 16.07   -19 47 33.5   21.5V 729736    H21  C~0XJW      
2011 07  31.246815 20 55 15.86   -19 47 33.4   21.3V 729736    H21  C~0XJW      
2011 07  31.252745 20 55 15.76   -19 47 34.0   21.4V 729736    H21  C~0XJW      
2011 07  31.259697 20 55 15.60   -19 47 34.1   21.2V 729736    H21  C~0XJW      
2011 08  01.370730 20 54 50.472  -19 48 07.54  21.3R 729736    568  C~0XJW      
2011 08  01.372147 20 54 50.444  -19 48 07.65  21.3R 729736    568  C~0XJW      
2011 08  01.373558 20 54 50.408  -19 48 07.66  21.2R 729736    568  C~0XJW      
2011 08  02.41027  20 54 26.908  -19 48 39.48  21.5G 729736    F51  C~2jgy      
2011 08  02.42064  20 54 26.661  -19 48 39.83  21.5G 729736    F51  C~2jgy      
2011 08  02.43273  20 54 26.382  -19 48 40.31  21.7G 729736    F51  C~2jgy      
2011 08  02.44267  20 54 26.161  -19 48 40.55  21.4G 729736    F51  C~2jgy      
2011 08  07.347039 20 52 34.949  -19 51 02.82  21.3R 729736    568  C~0XJW      
2011 08  07.350769 20 52 34.876  -19 51 02.92  21.3R 729736    568  C~0XJW      
2011 08  10.42919  20 51 25.42   -19 52 25.1   20.5R 729736    F65  C~0XJW      
2011 08  10.43387  20 51 25.32   -19 52 24.9   20.4R 729736    F65  C~0XJW      
2011 08  16.39995  20 49 13.155  -19 54 41.06  22.1G 729736    F51  C~2jgy      
2011 08  16.41004  20 49 12.940  -19 54 41.08  22.4G 729736    F51  C~2jgy      
2011 08  17.34826  20 48 52.584  -19 54 59.49  21.6G 729736    F51  C~2jgy      
2011 08  17.35889  20 48 52.345  -19 54 59.82  21.3G 729736    F51  C~2jgy      
2011 08  19.508132 20 48 06.123  -19 55 38.50  21.4R 729736    568  C~0Xc0      
2011 08  19.509566 20 48 06.086  -19 55 38.50  21.5R 729736    568  C~0Xc0      
2011 09  04.20725  20 43 01.09   -19 57 36.0         729736    291  C~0Y0E      
2011 09  04.22362  20 43 00.92   -19 57 36.0         729736    291  C~0Y0E      
2011 09  04.23629  20 43 00.62   -19 57 36.0         729736    291  C~0Y0E      
2011 10  01.25263  20 37 46.086  -19 46 39.94  22.6G 729736    F51  C~2jgy      
2011 10  01.26371  20 37 46.035  -19 46 40.05  21.3G 729736    F51  C~2jgy      
2012 06  16.60322  22 05 05.326  -08 41 53.98  21.8G 729736    F51  C~2jgy      
2012 08  06.40544  21 53 22.898  -08 36 40.01  21.6G 729736    F51  C~2jgy      
2012 08  26.35158  21 46 09.908  -08 52 27.83  21.4G 729736    F51  C~2jgy      
2012 08  26.36328  21 46 09.666  -08 52 28.36  21.4G 729736    F51  C~2jgy      
2013 08  14.06427  22 50 50.67   +03 42 01.7         729736    621  C~0tvy      
2013 08  14.10122  22 50 49.94   +03 42 00.1   21.8R 729736    621  C~0tvy      
2013 08  15.04366  22 50 31.47   +03 41 39.5         729736    621  C~0tvy      
2013 08  15.10097  22 50 30.35   +03 41 39.0   21.7R 729736    621  C~0tvy      
2013 08  18.49184  22 49 22.463  +03 40 01.31  22.1G 729736    F51  C~2jgy      
2013 08  18.50432  22 49 22.204  +03 40 00.83  21.8G 729736    F51  C~2jgy      
2013 08  28.93731  22 45 42.84   +03 32 06.0         729736    621  C~0tvy      
2013 08  28.97425  22 45 41.97   +03 32 04.5   22.3R 729736    621  C~0tvy      
2013 08  29.95027  22 45 20.88   +03 31 07.9         729736    621  C~0tvy      
2013 08  29.98721  22 45 20.14   +03 31 05.7   22.6R 729736    621  C~0tvy      
2013 09  04.21019  22 43 26.93   +03 25 32.3   21.7R 729736    H36  C~0tvy      
2013 09  04.23447  22 43 26.41   +03 25 30.6   20.8R 729736    H36  C~0tvy      
2013 09  04.24610  22 43 26.22   +03 25 29.7   21.6R 729736    H36  C~0tvy      
2014 07  29.40615  23 56 33.78   +15 40 27.4   21.7R 729736    G37  C~16ck      
2014 07  29.45401  23 56 33.36   +15 40 32.6         729736    G37  C~16ck      
2014 08  28.55478  23 49 22.261  +16 06 14.90  21.6w 729736    F51  C~17ll      
2014 08  28.56669  23 49 22.021  +16 06 14.84  21.5w 729736    F51  C~17ll      
2014 08  28.57858  23 49 21.772  +16 06 14.93  21.6w 729736    F51  C~17ll      
2014 11  20.30977  23 26 27.545  +13 53 17.64  21.6G 729736    F51  C~2jgy      
2014 11  20.32294  23 26 27.515  +13 53 16.39  21.8G 729736    F51  C~2jgy      
2014 11  20.33611  23 26 27.478  +13 53 15.07  22.1G 729736    F51  C~2jgy      
2014 11  20.34935  23 26 27.443  +13 53 13.71  21.8G 729736    F51  C~2jgy      
2015 09  09.62651  00 56 09.621  +27 24 58.74  21.6G 729736    F51  C~2jgy      
2015 10  23.28722  00 40 08.563  +26 40 09.89  21.6G 729736    F51  C~2jgy      
2016 11  29.31191  01 48 05.221  +34 41 34.96  21.7G 729736    F51  C~2jgy      
2016 11  29.32381  01 48 05.015  +34 41 33.08  21.8G 729736    F51  C~2jgy      
2022 01  07.375024 08 15 12.247  +26 45 24.82  21.8w 729736    F52  C~5LhP      
2022 01  07.387243 08 15 11.970  +26 45 25.03  22.0w 729736    F52  C~5LhP      
2022 01  07.399477 08 15 11.685  +26 45 25.73  22.1w 729736    F52  C~5LhP      
2022 01  07.411648 08 15 11.415  +26 45 25.95  22.0w 729736    F52  C~5LhP      
2022 12  02.518353 09 10 43.029  +18 58 44.68  22.7w 729736    F51  C~672G      
2022 12  02.532925 09 10 42.947  +18 58 44.97  22.7w 729736    F51  C~672G      
2022 12  02.547507 09 10 42.851  +18 58 44.82  22.5w 729736    F51  C~672G      
2022 12  02.562138 09 10 42.790  +18 58 44.66  22.6w 729736    F51  C~672G      

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    -0.23       0.00     0.11
     2   0.0000      0.00    -0.04       0.00     0.15
     3   0.0027      0.00     0.31       0.00     0.22
     4   0.0027      0.00     0.24       0.00    -0.08
     5   0.0355      0.00     0.08       0.00    -0.03
     6   0.0355      0.00     0.00       0.00     0.20
     7   1.0186      0.00     0.10       0.00     0.23
     8   1.0186      0.00    -0.00       0.00     0.22
     9   1.0186      0.00     0.07       0.00     0.14
    10   1.0187      0.00     0.13       0.00     0.14
    11   1.0213      0.00    -0.14       0.00     0.16
    12   1.0213      0.00     0.24       0.00    -0.02
    13   1.0213      0.00     0.01       0.00    -0.05
    14   1.0214      0.00    -0.02       0.00    -0.00
    15   1.0268      0.00    -0.22       0.00     0.12
    16   1.0268      0.00    -0.24       0.00     0.08
    17   1.0268      0.00    -0.19       0.00     0.09
    18   1.0268      0.00    -0.21       0.00     0.09
    19   1.0317      0.00     0.69       0.00    -0.60
    20   1.0317      0.00    -0.41       0.00    -0.31
    21   1.0317      0.00     0.14       0.00    -0.73
    22   1.0318      0.00     0.14       0.00    -0.61
    23   1.0348      0.00    -0.17       0.00     0.15
    24   1.0348      0.00    -0.10       0.00     0.08
    25   1.0348      0.00    -0.15       0.00     0.12
    26   1.0376      0.00     0.11       0.00     0.08
    27   1.0377      0.00     0.01       0.00     0.04
    28   1.0377      0.00     0.03       0.00    -0.07
    29   1.0377      0.00     0.18       0.00    -0.00
    30   1.0512      0.00    -0.12       0.00     0.11
    31   1.0512      0.00     0.07       0.00     0.12
    32   1.0596      0.00     0.03       0.00    -0.48
    33   1.0596      0.00     0.14       0.00    -0.17
    34   1.0759      0.00    -0.00       0.00    -0.08
    35   1.0760      0.00     0.15       0.00     0.10
    36   1.0785      0.00     0.03       0.00     0.14
    37   1.0786      0.00    -0.02       0.00     0.02
    38   1.0845      0.00     0.01       0.00     0.15
    39   1.0845      0.00    -0.08       0.00     0.17
    40   1.1274      0.00    -0.88       0.00    -0.21
    41   1.1275      0.00     0.89       0.00    -0.26
    42   1.1275      0.00    -0.27       0.00    -0.30
    43   1.2015      0.00    -0.35       0.00     0.44
    44   1.2015      0.00    -0.12       0.00    -0.18
    45   1.9115      0.00     0.29       0.00    -0.04
    46   2.0506      0.00     0.15       0.00     0.02
    47   2.1052      0.00    -0.19       0.00     0.03
    48   2.1053      0.00     0.04       0.00     0.12
    49   3.0709      0.00    -0.14       0.00     0.06
    50   3.0710      0.00    -0.12       0.00    -0.74
    51   3.0736      0.00    -0.53       0.00     0.16
    52   3.0738      0.00    -0.12       0.00     1.04
    53   3.0830      0.00    -0.10       0.00    -0.10
    54   3.0831      0.00    -0.08       0.00    -0.16
    55   3.1116      0.00     1.05       0.00    -0.76
    56   3.1117      0.00     0.12       0.00    -0.15
    57   3.1144      0.00    -0.51       0.00    -0.11
    58   3.1145      0.00     0.54       0.00    -0.13
    59   3.1288      0.00    -0.76       0.00     0.54
    60   3.1289      0.00    -0.51       0.00     0.51
    61   3.1289      0.00     0.49       0.00     0.41
    62   4.0274      0.00     0.02       0.00     0.22
    63   4.0275      0.00    -0.02       0.00     0.30
    64   4.1099      0.00     0.20       0.00    -0.01
    65   4.1099      0.00     0.15       0.00     0.01
    66   4.1100      0.00    -0.06       0.00     0.18
    67   4.3392      0.00     0.11       0.00    -0.04
    68   4.3393      0.00     0.15       0.00    -0.08
    69   4.3393      0.00     0.08       0.00    -0.17
    70   4.3393      0.00     0.03       0.00    -0.31
    71   5.1423      0.00    -0.10       0.00    -0.29
    72   5.2618      0.00    -0.00       0.00    -0.10
    73   6.3652      0.00     0.10       0.00    -0.07
    74   6.3653      0.00     0.00       0.00     0.14
    75  11.4715      0.00     0.10       0.00     0.16
    76  11.4715      0.00     0.04       0.00    -0.06
    77  11.4716      0.00    -0.13       0.00     0.21
    78  11.4716      0.00    -0.10       0.00     0.01
    79  12.3726      0.00     0.27       0.00    -0.27
    80  12.3727      0.00     0.13       0.00     0.09
    81  12.3727      0.00    -0.21       0.00     0.02
    82  12.3728      0.00    -0.01       0.00    -0.06

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.