Orbit Fit and Astrometric record for 02CB225

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: 02CB225   
# Created Fri Mar 29 01:10:46 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     37 observations of     37
# Arc:  19.11y
# First observation: 2002/02/07
#  Last observation: 2021/03/20
# Chi-squared of fit:    45.13 DOF:     68 RMS:  0.20
# Min/Max residuals:    -0.52    0.70
# Exact a, adot, b, bdot, g, gdot:
  1.422918E-05  2.405700E-02  1.078655E-06  8.576850E-04  2.432283E-02 -1.400138E-03
# Covariance matrix:
  1.8349E-13 -3.0471E-14  3.3628E-15 -1.0530E-15  1.1454E-13 -5.8797E-14
 -3.0471E-14  1.2269E-14 -9.4374E-16  4.5408E-16 -1.4442E-14  2.6255E-14
  3.3628E-15 -9.4374E-16  9.3863E-14 -6.1445E-15  4.1887E-15 -2.2662E-15
 -1.0530E-15  4.5408E-16 -6.1445E-15  6.6391E-16 -7.8429E-16  1.0355E-15
  1.1454E-13 -1.4442E-14  4.1887E-15 -7.8429E-16  2.0153E-13 -4.0802E-14
 -5.8797E-14  2.6255E-14 -2.2662E-15  1.0355E-15 -4.0802E-14  5.9673E-14
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.241616  157.857783    0.323645    0.052438   -0.927338  2452312.848143
# Heliocentric elements and errors
Epoch:              2452312.5000  =  2002/02/07
Mean Anomaly:          311.68637 +/-     0.031
Argument of Peri:      112.68583 +/-     0.037
Long of Asc Node:      100.40333 +/-     0.001
Inclination:             3.77785 +/-     0.000
Eccentricity:         0.07998417 +/-    0.0000
Semi-Major Axis:     44.22492569 +/-    0.0036
Time of Perihelion: 2466729.2118 +/-      14.7
Perihelion:          40.68763164 +/-    0.0036
Aphelion:            47.76221975 +/-    0.0042
Period (y)              294.1094 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -38.75794809 +/-    0.0007
Ecliptic Y           16.12609967 +/-    0.0003
Ecliptic Z            2.32489367 +/-    0.0000
Ecliptic XDOT        -0.00087833 +/-    0.0000
Ecliptic YDOT        -0.00257028 +/-    0.0000
Ecliptic ZDOT         0.00008769 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.04328925 +/-    0.0007
Geocenter to KBO     41.11369960 +/-    0.0008
# Hcoef:  7.41

The following table shows the complete astrometric record for 02CB225. 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 (02CB225) followed by the observatory code and reference code for the source of the astrometry.

2002 02  07.34740  10 43 02.45   +11 37 42.7   22.6R 02CB225   695  Cf0409      
2002 02  07.44282  10 43 02.03   +11 37 45.7         02CB225   695  Cf0409      
2002 02  08.38954  10 42 57.97   +11 38 11.8         02CB225   695  Cf0409      
2002 03  09.41141  10 40 45.81   +11 51 44.9   22.5R 02CB225   568  Cf2752      
2002 03  09.48148  10 40 45.47   +11 51 46.7         02CB225   568  Cf2752      
2002 05  11.91582  10 37 33.63   +12 07 44.5         02CB225   950  Cf7296      
2002 05  11.96296  10 37 33.59   +12 07 44.4         02CB225   950  Cf7296      
2002 05  12.91539  10 37 32.93   +12 07 44.3         02CB225   950  Cf7296      
2002 05  12.97708  10 37 32.88   +12 07 44.1         02CB225   950  Cf7296      
2003 03  05.31613  10 46 24.48   +11 21 14.6   22.8R 02CB225   662  Ch6137      
2003 03  05.39992  10 46 24.07   +11 21 16.9         02CB225   662  Ch6137      
2003 03  06.23876  10 46 20.21   +11 21 39.6   22.4R 02CB225   662  Ch6137      
2003 03  06.34313  10 46 19.73   +11 21 42.5         02CB225   662  Ch6137      
2004 03  20.24115  10 50 32.85   +10 59 12.1   22.8R 02CB225   662  Ck2152      
2004 03  20.36851  10 50 32.24   +10 59 15.1         02CB225   662  Ck2152      
2008 11  28.19958  11 21 24.93   +07 54 03.4   25.3R 02CB225   250  S~06AT      
2008 11  28.20583  11 21 24.94   +07 54 03.4         02CB225   250  S~06AT      
2008 11  28.21277  11 21 24.96   +07 54 03.3         02CB225   250  S~06AT      
2008 11  28.21902  11 21 24.97   +07 54 03.3         02CB225   250  S~06AT      
2013 03  13.35725  11 38 47.94   +06 18 40.4   23.0R 02CB225   695  C~0ucs      
2013 03  14.33406  11 38 43.46   +06 19 09.4         02CB225   695  C~0ucs      
2013 03  14.44273  11 38 42.95   +06 19 12.6         02CB225   695  C~0ucs      
2015 03  23.18015  11 48 43.99   +05 17 56.9   22.9R 02CB225   695  C~1Q3B      
2015 03  23.24427  11 48 43.69   +05 17 58.6         02CB225   695  C~1Q3B      
2015 03  23.30353  11 48 43.41   +05 18 00.2         02CB225   695  C~1Q3B      
2019 04  04.44671  12 09 09.64   +03 10 24.7   24.2g 02CB225   T09  C~7bAA      
2019 04  04.45934  12 09 09.58   +03 10 24.7   24.0g 02CB225   T09  C~7bAA      
2019 04  04.46994  12 09 09.54   +03 10 25.4   24.4g 02CB225   T09  C~7bAA      
2019 04  04.49303  12 09 09.43   +03 10 25.9   24.5g 02CB225   T09  C~7bAA      
2019 04  04.51189  12 09 09.35   +03 10 26.4   24.6g 02CB225   T09  C~7bAA      
2019 04  05.52240  12 09 04.86   +03 10 53.7   23.2r 02CB225   T09  C~7bAA      
2019 04  05.53288  12 09 04.81   +03 10 54.4   23.3r 02CB225   T09  C~7bAA      
2019 04  05.55592  12 09 04.72   +03 10 55.1   23.4r 02CB225   T09  C~7bAA      
2019 04  05.57477  12 09 04.62   +03 10 55.4   23.3r 02CB225   T09  C~7bAA      
2021 03  20.290520 12 20 57.091  +01 55 39.41  23.5G 02CB225   G37  C~4hhn      
2021 03  20.323090 12 20 56.950  +01 55 40.38        02CB225   G37  C~4hhn      
2021 03  20.350400 12 20 56.825  +01 55 41.25        02CB225   G37  C~4hhn      

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    -0.21
     2   0.0003      0.00     0.16       0.00     0.14
     3   0.0029      0.00     0.13       0.00    -0.17
     4   0.0823      0.00     0.25       0.00    -0.04
     5   0.0825      0.00     0.02       0.00    -0.10
     6   0.2562      0.00    -0.13       0.00    -0.17
     7   0.2563      0.00    -0.15       0.00    -0.27
     8   0.2589      0.00    -0.18       0.00    -0.14
     9   0.2591      0.00    -0.27       0.00    -0.30
    10   1.0704      0.00     0.01       0.00     0.50
    11   1.0706      0.00    -0.25       0.00     0.47
    12   1.0729      0.00    -0.29       0.00    -0.07
    13   1.0732      0.00    -0.17       0.00    -0.06
    14   2.1133      0.00     0.70       0.00     0.26
    15   2.1137      0.00    -0.05       0.00     0.09
    16   6.8059      0.00    -0.05       0.00    -0.00
    17   6.8059      0.00    -0.09       0.00     0.04
    18   6.8059      0.00    -0.00       0.00    -0.01
    19   6.8059      0.00    -0.04       0.00     0.03
    20  11.0938      0.00     0.22       0.00     0.21
    21  11.0965      0.00    -0.07       0.00     0.11
    22  11.0968      0.00    -0.15       0.00     0.09
    23  13.1193      0.00     0.31       0.00     0.20
    24  13.1195      0.00     0.24       0.00     0.03
    25  13.1197      0.00     0.14       0.00    -0.09
    26  17.1529      0.00    -0.08       0.00     0.18
    27  17.1529      0.00    -0.12       0.00    -0.17
    28  17.1530      0.00    -0.00       0.00     0.24
    29  17.1530      0.00    -0.08       0.00     0.10
    30  17.1531      0.00    -0.01       0.00     0.07
    31  17.1559      0.00    -0.06       0.00    -0.52
    32  17.1559      0.00    -0.10       0.00    -0.11
    33  17.1559      0.00     0.10       0.00    -0.04
    34  17.1560      0.00    -0.14       0.00    -0.26
    35  19.1128      0.00    -0.08       0.00     0.02
    36  19.1129      0.00     0.06       0.00     0.01
    37  19.1129      0.00     0.08       0.00     0.05

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.

02CB225    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.915    43.915    43.915
ecceobj         0.076     0.076     0.076
incobj          3.780     3.780     3.780
qmin           40.027    40.052    40.018
qmax           48.419    48.410    48.398
amean          44.105    44.104    44.105
amin           43.761    43.752    43.761
amax           44.476    44.476    44.473
emean           0.073     0.073     0.073
emin            0.057     0.057     0.057
emax            0.089     0.089     0.089
imean           2.040     2.039     2.040
imin            1.326     1.325     1.326
imax            2.723     2.723     2.723
excite_mean     0.082     0.082     0.082
fracstop        1.000     1.000     1.000
cjmean          3.095     3.095     3.095

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       190.8     190.2     190.9
kozaiamp        180.0     180.0     180.0