Orbit Fit and Astrometric record for 00GM147

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: 00GM147   
# Created Wed Nov 27 02:08:04 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:  33.09d
# First observation: 2000/04/03
#  Last observation: 2000/05/06
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.039076  -0.000001   0.002924   0.028972   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     2.06 DOF:      9 RMS:  0.10
# Min/Max residuals:    -0.12    0.12
# Exact a, adot, b, bdot, g, gdot:
  1.924875E-05  3.392939E-02  6.136474E-07  1.996507E-03  2.818935E-02  5.404105E-03
# Covariance matrix:
  3.1111E-12  3.9673E-09 -7.6844E-14  6.9522E-10  7.2152E-10 -8.2786E-09
  3.9673E-09  5.7049E-06 -1.1667E-10  1.0004E-06  1.0274E-06 -1.6538E-05
 -7.6844E-14 -1.1667E-10  3.0140E-13 -2.3943E-11 -2.0435E-11  6.2664E-10
  6.9522E-10  1.0004E-06 -2.3943E-11  1.7559E-07  1.8002E-07 -2.9721E-06
  7.2152E-10  1.0274E-06 -2.0435E-11  1.8002E-07  1.8587E-07 -2.5513E-06
 -8.2786E-09 -1.6538E-05  6.2664E-10 -2.9721E-06 -2.5513E-06  2.6162E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   18.471913 -179.473681   -0.234649    0.310173   -0.929181  2451637.856713
# Heliocentric elements and errors
Epoch:              2451630.5000  =  2000/03/27
Mean Anomaly:           13.72440 +/-    29.332
Argument of Peri:       46.10273 +/-    80.926
Long of Asc Node:      101.50527 +/-     1.322
Inclination:            18.27771 +/-     0.067
Eccentricity:         0.39996733 +/-    0.3125
Semi-Major Axis:     57.72863492 +/-   16.7535
Time of Perihelion: 2445522.8219 +/-   12779.6
Perihelion:          34.63906699 +/-   20.6541
Aphelion:            80.81820285 +/-   29.5913
Period (y)              438.6268 +/-    190.94
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -34.61607434 +/-    0.5146
Ecliptic Y           -0.54994412 +/-    0.0047
Ecliptic Z           11.23973137 +/-    0.1719
Ecliptic XDOT        -0.00041227 +/-    0.0015
Ecliptic YDOT        -0.00329251 +/-    0.0002
Ecliptic ZDOT         0.00035034 +/-    0.0005
# Distances at JD0 (AU)
Heliocenter to KBO   36.39926651 +/-    0.4922
Geocenter to KBO     35.47439474 +/-    0.5425
# Hcoef:  8.04

The following table shows the complete astrometric record for 00GM147. 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 (00GM147) followed by the observatory code and reference code for the source of the astrometry.

2000 04  03.35597  12 32 10.39   +16 41 31.7   23.1R 00GM147   568  Cb4444      
2000 04  03.39060  12 32 10.21   +16 41 32.4   23.1R 00GM147   568  Cb4444      
2000 04  03.42646  12 32 10.03   +16 41 33.6   23.1R 00GM147   568  Cb4444      
2000 04  04.45475  12 32 04.73   +16 42 01.3   23.2R 00GM147   568  Cb4444      
2000 04  04.50881  12 32 04.45   +16 42 02.8   23.0R 00GM147   568  Cb4444      
2000 05  06.38902  12 29 37.88   +16 49 50.4   23.9R 00GM147   568  Cb5789      
2000 05  06.44318  12 29 37.67   +16 49 50.7   23.9R 00GM147   568  Cb5789      

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    -0.04       0.00     0.10
     2   0.0001     -2.64     0.08      -0.44    -0.12
     3   0.0002     -5.49     0.09      -0.42     0.12
     4   0.0030    -86.27    -0.07      -6.84    -0.09
     5   0.0032    -90.55    -0.07      -7.14    -0.02
     6   0.0904  -2200.57     0.05    -452.44    -0.09
     7   0.0906  -2203.44    -0.05    -453.41     0.10

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.

00GM147    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0