Orbit Fit and Astrometric record for 00PG30

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: 00PG30    
# Created Wed Dec 25 02:08:04 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:  21.18y
# First observation: 1999/07/18
#  Last observation: 2020/09/21
# Chi-squared of fit:    90.58 DOF:     34 RMS:  0.38
# Min/Max residuals:    -0.68    0.73
# Exact a, adot, b, bdot, g, gdot:
  1.348288E-05  1.903868E-02  1.863712E-06 -1.530862E-03  2.155291E-02 -1.657034E-03
# Covariance matrix:
  3.4541E-13 -1.7760E-13 -1.9584E-14  1.4849E-14  9.2322E-14 -3.9837E-13
 -1.7760E-13  1.3159E-13  1.4572E-14 -1.1015E-14  9.0541E-15  2.9432E-13
 -1.9584E-14  1.4572E-14  9.8662E-14 -7.7918E-15 -7.7700E-16  3.3198E-14
  1.4849E-14 -1.1015E-14 -7.7918E-15  2.6149E-15  7.9078E-16 -2.5116E-14
  9.2322E-14  9.0541E-15 -7.7700E-16  7.9078E-16  4.6938E-13 -2.8377E-14
 -3.9837E-13  2.9432E-13  3.3198E-14 -2.5116E-14 -2.8377E-14  6.7184E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.574147  -56.596223    0.149280    0.009812   -1.003234  2451377.922683
# Heliocentric elements and errors
Epoch:              2451378.5000  =  1999/07/19
Mean Anomaly:          248.07237 +/-     0.057
Argument of Peri:      295.46916 +/-     0.043
Long of Asc Node:      130.19794 +/-     0.000
Inclination:             4.62540 +/-     0.000
Eccentricity:         0.10445311 +/-    0.0001
Semi-Major Axis:     45.24033444 +/-    0.0054
Time of Perihelion: 2485934.3802 +/-      22.3
Perihelion:          40.51484100 +/-    0.0057
Aphelion:            49.96582788 +/-    0.0067
Period (y)              304.2965 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           25.97829759 +/-    0.0008
Ecliptic Y          -39.64911799 +/-    0.0012
Ecliptic Z            0.46503940 +/-    0.0000
Ecliptic XDOT         0.00190074 +/-    0.0000
Ecliptic YDOT         0.00151405 +/-    0.0000
Ecliptic ZDOT        -0.00019652 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   47.40407690 +/-    0.0011
Geocenter to KBO     46.39753148 +/-    0.0015
# Hcoef:  7.64

The following table shows the complete astrometric record for 00PG30. 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 (00PG30) followed by the observatory code and reference code for the source of the astrometry.

1999 07  18.42194  20 22 16.13   -18 50 09.2   24.1R 00PG30    568  Cd3309      
1999 07  18.44903  20 22 16.00   -18 50 09.5   24.1R 00PG30    568  Cd3309      
1999 07  18.47601  20 22 15.88   -18 50 09.9   23.9R 00PG30    568  Cd3309      
2000 08  05.32068  20 25 28.74   -18 44 52.8   24.7R 00PG30    568  Cb8005      
2000 08  05.36494  20 25 28.54   -18 44 53.6         00PG30    568  Cb8005      
2000 08  05.41301  20 25 28.33   -18 44 54.6         00PG30    568  Cb8005      
2000 08  06.31144  20 25 24.52   -18 45 08.5   24.2R 00PG30    568  Cb8005      
2000 08  06.35730  20 25 24.32   -18 45 09.1         00PG30    568  Cb8005      
2000 08  06.39871  20 25 24.12   -18 45 09.8         00PG30    568  Cb8005      
2001 07  24.38191  20 30 56.75   -18 30 58.7         00PG30    568  Cd3309      
2001 07  24.42286  20 30 56.58   -18 30 59.4   23.7R 00PG30    568  Cd3309      
2001 07  24.46359  20 30 56.39   -18 31 00.1   23.4R 00PG30    568  Cd3309      
2001 07  25.50785  20 30 51.82   -18 31 17.4         00PG30    568  Cd3309      
2001 09  18.15341  20 27 25.36   -18 44 26.5         00PG30    675  Ce0222      
2001 09  18.20484  20 27 25.25   -18 44 27.0   24.1R 00PG30    675  Ce0222      
2001 09  19.17155  20 27 22.89   -18 44 36.7         00PG30    675  Ce0222      
2002 06  07.51887  20 38 23.75   -18 08 42.2         00PG30    568  Cf8836      
2002 06  07.57025  20 38 23.59   -18 08 42.7         00PG30    568  Cf8836      
2020 09  21.126070 21 55 06.449  -14 05 57.19  23.9G 00PG30    G37  C~49Jp      
2020 09  21.174850 21 55 06.261  -14 05 58.32        00PG30    G37  C~49Jp      

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     0.25       0.00    -0.58
     2   0.0001      0.00     0.11       0.00    -0.45
     3   0.0001      0.00     0.10       0.00    -0.44
     4   1.0511      0.00    -0.62       0.00     0.49
     5   1.0512      0.00    -0.68       0.00     0.40
     6   1.0513      0.00    -0.65       0.00     0.17
     7   1.0538      0.00     0.51       0.00     0.59
     8   1.0539      0.00     0.53       0.00     0.73
     9   1.0540      0.00     0.27       0.00     0.69
    10   2.0177      0.00    -0.34       0.00    -0.19
    11   2.0178      0.00    -0.14       0.00    -0.21
    12   2.0179      0.00    -0.26       0.00    -0.24
    13   2.0208      0.00     0.11       0.00    -0.24
    14   2.1704      0.00     0.03       0.00    -0.20
    15   2.1705      0.00     0.33       0.00    -0.19
    16   2.1732      0.00     0.15       0.00    -0.43
    17   2.8887      0.00     0.42       0.00     0.05
    18   2.8888      0.00    -0.03       0.00     0.05
    19  21.1792      0.00     0.08       0.00     0.11
    20  21.1793      0.00    -0.11       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.

00PG30    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        45.166    45.166    45.166
ecceobj         0.105     0.105     0.105
incobj          4.628     4.628     4.628
qmin           39.353    39.373    39.349
qmax           51.211    51.276    51.174
amean          45.156    45.157    45.156
amin           44.781    44.785    44.788
amax           45.553    45.582    45.557
emean           0.110     0.110     0.110
emin            0.095     0.095     0.095
emax            0.124     0.125     0.124
imean           3.570     3.570     3.570
imin            2.985     2.985     2.986
imax            4.192     4.193     4.192
excite_mean     0.126     0.126     0.126
fracstop        1.000     1.000     1.000
cjmean          3.096     3.096     3.096

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       175.5     175.5     175.5
kozaiamp        180.0     180.0     180.0