Orbit Fit and Astrometric record for 00QL226

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory.

# Object: 00QL226   
# Created Fri May  2 02:36:32 2008
# Orbit generated from Bernstein formalism
# Fitting    7 observations of    7
# Arc:   1.24d
# First observation: 2000/08/29
#  Last observation: 2000/08/30
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:     4.32 DOF:   10 RMS:  0.14
# Min/Max residuals:    -0.22    0.18
# Exact a, adot, b, bdot, g, gdot:
  1.615035E-05  2.863931E-02 -1.110430E-06 -1.060402E-03  2.736088E-02  0.000000E+00
# Covariance matrix:
  3.6853E-11  6.2180E-08 -5.3671E-14 -3.9997E-11  1.0029E-08  0.0000E+00
  6.2180E-08  1.0721E-04 -9.2215E-11 -6.8637E-08  1.7220E-05  0.0000E+00
 -5.3671E-14 -9.2215E-11  5.2788E-13 -1.9139E-10 -1.4826E-11  0.0000E+00
 -3.9997E-11 -6.8637E-08 -1.9139E-10  1.1532E-07 -1.1038E-08  0.0000E+00
  1.0029E-08  1.7220E-05 -1.4826E-11 -1.1038E-08  2.7690E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  2.6953E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.393354  -21.187404    0.053730    0.006736   -1.005119  2451785.653693
# Heliocentric elements and errors
Epoch:              2451780.5000  =  2000/08/24
Mean Anomaly:          354.84630 +/-   324.194
Argument of Peri:      175.36601 +/-    30.928
Long of Asc Node:      168.99708 +/-     4.790
Inclination:             2.14845 +/-     0.995
Eccentricity:         0.04565803 +/-    0.5658
Semi-Major Axis:     39.34587286 +/-   20.9844
Time of Perihelion: 2453071.0180 +/-  171323.2
Perihelion:          37.54941774 +/-   29.9449
Aphelion:            41.14232797 +/-   31.2589
Period (y)              246.8067 +/-    197.44
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           35.00075374 +/-    2.0724
Ecliptic Y          -13.61752876 +/-    0.8035
Ecliptic Z            0.25086339 +/-    0.0153
Ecliptic XDOT         0.00102912 +/-    0.0016
Ecliptic YDOT         0.00267708 +/-    0.0010
Ecliptic ZDOT        -0.00010595 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   37.55732664 +/-    1.9532
Geocenter to KBO     36.54852761 +/-    2.2228
# Hcoef:  8.39

The following table shows the complete astrometric record for 00QL226. 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 (00QL226) followed by the observatory code and reference code for the source of the astrometry.

2000 08  29.15295  22 41 05.75   -07 54 03.7         00QL226   809  Cb8401      
2000 08  29.25209  22 41 05.24   -07 54 07.0         00QL226   809  Cb8401      
2000 08  30.13214  22 41 00.88   -07 54 33.5         00QL226   809  Cb8401      
2000 08  30.21740  22 41 00.46   -07 54 36.4   23.7R 00QL226   809  Cb8401      
2000 08  30.30047  22 41 00.02   -07 54 38.7         00QL226   809  Cb8401      
2000 08  30.34795  22 40 59.78   -07 54 40.5         00QL226   809  Cb8401      
2000 08  30.39124  22 40 59.56   -07 54 41.4         00QL226   809  Cb8401      

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     0.10
  2   0.0003     -8.26    -0.13      -0.22    -0.11
  3   0.0027    -78.25     0.11      -0.54     0.13
  4   0.0029    -85.12     0.16      -0.89    -0.21
  5   0.0031    -92.05    -0.02      -0.58     0.11
  6   0.0033    -96.03    -0.16      -0.91    -0.22
  7   0.0034    -99.39    -0.04      -0.52     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.

00QL226    quality flag:2

Type:      CLASSICAL   10:7EEE CLASSICAL

axisobj       38.352    38.352    38.352
ecceobj        0.066     0.066     0.066
incobj         2.193     2.193     2.193
qmin          33.651    34.106    33.506
qmax          43.024    42.784    43.377
amean         38.143    38.194    38.157
amin          37.788    37.816    37.659
amax          38.603    38.591    38.680
emean          0.087     0.086     0.089
emin           0.058     0.045     0.051
emax           0.118     0.109     0.123
imean          1.290     1.488     1.295
imin           0.086     0.028     0.172
imax           2.137     2.449     2.209
fracstop       1.000     1.000     1.000
cjmean         3.031     3.032     3.031

libcent 0     -180.0     176.0    -180.0
libamp  0     -180.0     170.8    -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      167.7     149.1     172.7
kozaiamp       180.0     180.0     180.0