Orbit Fit and Astrometric record for 00SQ331

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: 00SQ331   
# Created Fri May  2 02:36:32 2008
# Orbit generated from Bernstein formalism
# Fitting    6 observations of    6
# Arc:   1.13d
# First observation: 2000/09/23
#  Last observation: 2000/09/24
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit:     0.72 DOF:    8 RMS:  0.06
# Min/Max residuals:    -0.07    0.12
# Exact a, adot, b, bdot, g, gdot:
  1.851999E-05  4.050576E-02  1.981664E-06  4.130671E-03  3.470512E-02  0.000000E+00
# Covariance matrix:
  4.7394E-10  1.0360E-06  3.3599E-11  7.6709E-08  3.2047E-07  0.0000E+00
  1.0360E-06  2.2674E-03  7.3518E-08  1.6785E-04  7.0123E-04  0.0000E+00
  3.3599E-11  7.3518E-08  2.7817E-12  5.3035E-09  2.2738E-08  0.0000E+00
  7.6709E-08  1.6785E-04  5.3035E-09  1.2552E-05  5.1913E-05  0.0000E+00
  3.2047E-07  7.0123E-04  2.2738E-08  5.1913E-05  2.1688E-04  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  5.5005E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.568715   61.092443    0.869726   -0.022107   -0.488726  2451810.946003
# Heliocentric elements and errors
Epoch:              2451810.5000  =  2000/09/23
Mean Anomaly:          315.48145 +/-   113.807
Argument of Peri:       24.09533 +/-   190.025
Long of Asc Node:       83.05585 +/-     6.361
Inclination:             6.26629 +/-     1.789
Eccentricity:         0.04051341 +/-    0.8772
Semi-Major Axis:     30.16851656 +/-   21.7286
Time of Perihelion: 2459295.0874 +/-  200543.3
Perihelion:          28.94628723 +/-   33.6907
Aphelion:            31.39074589 +/-   34.8076
Period (y)              165.7063 +/-    179.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           14.91751798 +/-    5.9050
Ecliptic Y           25.21119841 +/-   10.6927
Ecliptic Z           -1.29131378 +/-    0.5480
Ecliptic XDOT        -0.00279771 +/-    0.0023
Ecliptic YDOT         0.00156252 +/-    0.0020
Ecliptic ZDOT         0.00032569 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   29.32242076 +/-    9.6719
Geocenter to KBO     28.81419379 +/-   12.2271
# Hcoef:  9.15

The following table shows the complete astrometric record for 00SQ331. 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 (00SQ331) followed by the observatory code and reference code for the source of the astrometry.

2000 09  23.44526  03 58 02.66   +17 51 47.5   23.4R 00SQ331   568  Cc1430      
2000 09  23.50233  03 58 02.50   +17 51 46.9   24.3R 00SQ331   568  Cc1430      
2000 09  23.57560  03 58 02.30   +17 51 46.3   23.7R 00SQ331   568  Cc1430      
2000 09  24.46410  03 57 59.88   +17 51 36.8   23.1R 00SQ331   568  Cc1430      
2000 09  24.51465  03 57 59.72   +17 51 36.3   23.5R 00SQ331   568  Cc1430      
2000 09  24.57914  03 57 59.53   +17 51 35.7         00SQ331   568  Cc1430      

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    -0.01       0.00    -0.02
  2   0.0002     -2.36    -0.05      -0.13    -0.05
  3   0.0004     -5.28     0.06      -0.14     0.08
  4   0.0028    -41.03     0.12      -2.46    -0.07
  5   0.0029    -43.37    -0.06      -2.49    -0.01
  6   0.0031    -46.15    -0.05      -2.53     0.07

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.

00SQ331    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj       32.703    32.703    32.703
ecceobj        0.146     0.146     0.146
incobj         6.099     6.099     6.099
qmin          23.761    27.105    26.513
qmax          37.487    39.401    37.487
amean         30.990    32.782    31.325
amin          28.406    31.632    30.306
amax          32.703    33.816    32.703
emean          0.120     0.151     0.119
emin           0.061     0.137     0.075
emax           0.168     0.165     0.149
imean          5.106     3.638     5.454
imin           2.563     3.341     2.816
imax           7.741     4.702     7.923
fracstop       0.011     0.007     0.030
cjmean         2.977     2.976     2.977

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      162.2     249.6     133.4
kozaiamp       178.7     178.9     177.8