Orbit Fit and Astrometric record for 137294

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: 137294    
# Created Fri Apr 26 01:07:28 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     49 observations of     49
# Arc:  22.97y
# First observation: 1999/09/07
#  Last observation: 2022/08/27
# Chi-squared of fit:   110.35 DOF:     92 RMS:  0.27
# Min/Max residuals:    -0.64    0.96
# Exact a, adot, b, bdot, g, gdot:
  1.522549E-05  2.370095E-02 -2.031233E-07 -5.585438E-04  2.404613E-02  2.031271E-03
# 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
    0.027506  -32.252713   -0.280674    0.000221   -0.960837  2451428.809803
# Heliocentric elements and errors
Epoch:              2451428.5000  =  1999/09/07
Mean Anomaly:           51.44361 +/-     0.000
Argument of Peri:      117.05909 +/-     0.000
Long of Asc Node:      149.27761 +/-     0.000
Inclination:             1.34735 +/-     0.000
Eccentricity:         0.10655264 +/-    0.0000
Semi-Major Axis:     45.21022391 +/-    0.0000
Time of Perihelion: 2435561.9560 +/-       0.0
Perihelion:          40.39295498 +/-    0.0000
Aphelion:            50.02749284 +/-    0.0000
Period (y)              303.9927 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           36.14039714 +/-    0.0000
Ecliptic Y          -22.46592118 +/-    0.0000
Ecliptic Z            0.01998077 +/-    0.0000
Ecliptic XDOT         0.00163163 +/-    0.0000
Ecliptic YDOT         0.00216705 +/-    0.0000
Ecliptic ZDOT        -0.00006342 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.55398213 +/-    0.0000
Geocenter to KBO     41.58671335 +/-    0.0000
# Hcoef:  6.36

The following table shows the complete astrometric record for 137294. 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 (137294) followed by the observatory code and reference code for the source of the astrometry.

1999 09  07.30906  21 59 41.20   -12 13 47.7   22.4R 137294    568  Ca8546      
1999 09  07.34237  21 59 41.04   -12 13 48.7   22.4R 137294    568  Ca8546      
1999 09  07.37708  21 59 40.89   -12 13 49.5   22.4R 137294    568  Ca8546      
1999 10  09.27344  21 57 45.57   -12 24 18.9   22.6R 137294    568  Ca8546      
1999 10  09.32742  21 57 45.43   -12 24 19.9   22.6R 137294    568  Ca8546      
1999 11  09.25939  21 57 01.05   -12 28 27.5   22.6R 137294    568  Ca8546      
1999 11  10.23324  21 57 01.03   -12 28 28.0   22.7R 137294    568  Ca8546      
2000 05  30.58669  22 10 03.26   -11 18 39.9   22.8R 137294    568  Cb6506      
2000 05  31.59735  22 10 03.28   -11 18 40.2   22.9R 137294    568  Cb6506      
2000 06  01.58175  22 10 03.20   -11 18 40.8   23.0R 137294    568  Cb6506      
2000 08  26.09249  22 05 47.03   -11 42 40.9   22.4R 137294    807  Cc0856      
2000 08  26.17190  22 05 46.67   -11 42 43.0         137294    807  Cc0856      
2001 07  18.49744  22 13 41.277  -11 00 42.09        137294    568  Cl5166      
2001 07  19.49802  22 13 37.760  -11 01 02.26        137294    568  Cl5166      
2002 11  05.28485  22 12 25.34   -11 10 21.0   23.4R 137294    568  Cl8251      
2002 11  06.31805  22 12 24.55   -11 10 25.6         137294    568  Cl8251      
2006 08  21.18518  22 36 46.79   -08 57 35.5   21.1R 137294    807  Cs2409      
2006 08  21.27601  22 36 46.38   -08 57 38.0         137294    807  Cs2409      
2006 10  19.10839  22 32 58.49   -09 20 17.9   22.5R 137294    695  Ct0246      
2006 10  19.20218  22 32 58.26   -09 20 19.4         137294    695  Ct0246      
2006 10  20.11097  22 32 55.98   -09 20 32.8         137294    695  Ct0246      
2006 12  21.07730  22 33 01.89   -09 20 00.0   22.3R 137294    695  Ct6215      
2006 12  21.14614  22 33 02.05   -09 19 59.0         137294    695  Ct6215      
2007 06  27.41489  22 44 37.01   -08 12 11.3   22.9R 137294    250  S~06HN      
2007 06  27.42184  22 44 37.00   -08 12 11.4         137294    250  S~06HN      
2007 06  27.48017  22 44 36.92   -08 12 11.9         137294    250  S~06HN      
2007 06  27.48712  22 44 36.91   -08 12 12.0         137294    250  S~06HN      
2013 09  03.42331  23 10 00.562  -05 47 41.14  22.4w 137294    F51  C~1vpm      
2013 09  03.43820  23 10 00.494  -05 47 41.30  22.6w 137294    F51  C~1vpm      
2013 09  03.45310  23 10 00.427  -05 47 41.87  22.4w 137294    F51  C~1vpm      
2013 09  03.46799  23 10 00.373  -05 47 42.10  22.8w 137294    F51  C~1vpm      
2014 07  28.54385  23 17 03.315  -05 04 41.26  22.9w 137294    F51  C~1vpm      
2014 07  28.55527  23 17 03.273  -05 04 41.12  22.9w 137294    F51  C~1vpm      
2014 07  28.57802  23 17 03.212  -05 04 41.65  23.0w 137294    F51  C~1vpm      
2014 08  03.53401  23 16 45.007  -05 06 41.45  22.8w 137294    F51  C~1vpm      
2014 08  03.55662  23 16 44.934  -05 06 41.82  22.7w 137294    F51  C~1vpm      
2014 08  03.56794  23 16 44.903  -05 06 42.17  22.9w 137294    F51  C~1vpm      
2014 08  20.47528  23 15 43.855  -05 13 19.32  22.9w 137294    F51  C~1vpm      
2014 08  20.48745  23 15 43.806  -05 13 19.59  22.7w 137294    F51  C~1vpm      
2014 08  20.49962  23 15 43.764  -05 13 19.99  22.5w 137294    F51  C~1vpm      
2014 08  20.51181  23 15 43.720  -05 13 20.31  22.9w 137294    F51  C~1vpm      
2017 07  18.335671 23 31 23.12   -03 38 22.2         137294    W84  C~3fp3      
2017 07  18.388310 23 31 23.02   -03 38 23.0         137294    W84  C~3fp3      
2021 09  12.301040 23 46 37.997  -02 07 25.91  22.8G 137294    G37  C~57po      
2021 09  12.361120 23 46 37.751  -02 07 27.49        137294    G37  C~57po      
2021 09  12.421840 23 46 37.490  -02 07 29.11        137294    G37  C~57po      
2022 08  27.384530 23 52 15.863  -01 32 24.76  22.7G 137294    G37  C~5ngo      
2022 08  27.418090 23 52 15.734  -01 32 25.62        137294    G37  C~5ngo      
2022 08  27.453230 23 52 15.595  -01 32 26.54        137294    G37  C~5ngo      

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     0.08       0.00    -0.01
     2   0.0001      0.00    -0.12       0.00    -0.22
     3   0.0002      0.00    -0.09       0.00    -0.20
     4   0.0875      0.00    -0.01       0.00    -0.36
     5   0.0877      0.00     0.14       0.00    -0.57
     6   0.1723      0.00    -0.07       0.00    -0.27
     7   0.1750      0.00     0.05       0.00    -0.26
     8   0.7290      0.00     0.01       0.00    -0.06
     9   0.7318      0.00     0.00       0.00    -0.16
    10   0.7345      0.00    -0.23       0.00    -0.08
    11   0.9686      0.00     0.13       0.00     0.21
    12   0.9688      0.00     0.18       0.00     0.10
    13   1.8623      0.00     0.96       0.00     0.23
    14   1.8650      0.00     0.78       0.00     0.05
    15   3.1622      0.00    -0.04       0.00    -0.32
    16   3.1650      0.00    -0.41       0.00    -0.43
    17   6.9538      0.00     0.14       0.00     0.17
    18   6.9541      0.00    -0.01       0.00     0.04
    19   7.1151      0.00    -0.22       0.00     0.23
    20   7.1154      0.00     0.04       0.00     0.15
    21   7.1179      0.00     0.24       0.00     0.37
    22   7.2875      0.00     0.21       0.00     0.37
    23   7.2877      0.00    -0.23       0.00     0.23
    24   7.8032      0.00    -0.63       0.00     0.51
    25   7.8032      0.00    -0.64       0.00     0.48
    26   7.8033      0.00    -0.62       0.00     0.50
    27   7.8034      0.00    -0.62       0.00     0.47
    28  13.9907      0.00     0.01       0.00    -0.15
    29  13.9908      0.00    -0.04       0.00     0.10
    30  13.9908      0.00    -0.07       0.00    -0.07
    31  13.9909      0.00     0.09       0.00     0.11
    32  14.8891      0.00     0.14       0.00    -0.27
    33  14.8891      0.00     0.01       0.00     0.09
    34  14.8892      0.00     0.11       0.00    -0.01
    35  14.9055      0.00     0.19       0.00    -0.05
    36  14.9055      0.00     0.22       0.00     0.06
    37  14.9056      0.00     0.31       0.00    -0.05
    38  14.9519      0.00     0.01       0.00    -0.05
    39  14.9519      0.00     0.01       0.00    -0.01
    40  14.9519      0.00     0.12       0.00    -0.10
    41  14.9520      0.00     0.19       0.00    -0.11
    42  17.8618      0.00     0.10       0.00     0.09
    43  17.8620      0.00     0.20       0.00    -0.00
    44  22.0150      0.00    -0.10       0.00    -0.20
    45  22.0152      0.00     0.02       0.00    -0.14
    46  22.0154      0.00    -0.05       0.00    -0.10
    47  22.9708      0.00     0.02       0.00    -0.12
    48  22.9709      0.00     0.00       0.00    -0.14
    49  22.9710      0.00    -0.07       0.00    -0.18

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.

137294    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        45.153    45.154    45.153
ecceobj         0.106     0.106     0.106
incobj          1.347     1.347     1.347
qmin           39.723    39.730    39.688
qmax           50.651    50.688    50.694
amean          45.030    45.030    45.030
amin           44.662    44.658    44.669
amax           45.424    45.425    45.434
emean           0.101     0.101     0.101
emin            0.086     0.086     0.086
emax            0.115     0.116     0.116
imean           1.718     1.718     1.718
imin            1.062     1.062     1.062
imax            2.336     2.336     2.336
excite_mean     0.106     0.106     0.106
fracstop        1.000     1.000     1.000
cjmean          3.100     3.100     3.100

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       173.9     173.9     174.1
kozaiamp        180.0     180.0     180.0