Orbit Fit and Astrometric record for 00SP331

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: 00SP331   
# 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:     0.81 DOF:    8 RMS:  0.06
# Min/Max residuals:    -0.09    0.11
# Exact a, adot, b, bdot, g, gdot:
  1.595969E-05  2.583129E-02 -1.814424E-07  4.510921E-04  2.566564E-02  0.000000E+00
# Covariance matrix:
  1.2125E-10  1.9522E-07  9.1160E-12  1.5212E-08  5.9924E-08  0.0000E+00
  1.9522E-07  3.1575E-04  1.4730E-08  2.4580E-05  9.6826E-05  0.0000E+00
  9.1160E-12  1.4730E-08  1.0439E-12  1.0283E-09  4.5187E-09  0.0000E+00
  1.5212E-08  2.4580E-05  1.0283E-09  2.0406E-06  7.5406E-06  0.0000E+00
  5.9924E-08  9.6826E-05  4.5187E-09  7.5406E-06  2.9704E-05  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  2.2247E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.731888   60.775867    0.867009   -0.023728   -0.493454  2451810.946003
# Heliocentric elements and errors
Epoch:              2451810.5000  =  2000/09/23
Mean Anomaly:          313.52613 +/-   191.400
Argument of Peri:      338.21578 +/-   224.827
Long of Asc Node:      130.24875 +/-    47.437
Inclination:             2.85628 +/-     0.813
Eccentricity:         0.02935719 +/-    0.6649
Semi-Major Axis:     40.26751392 +/-   22.5739
Time of Perihelion: 2463859.1111 +/-  329461.7
Perihelion:          39.08537298 +/-   34.5960
Aphelion:            41.44965487 +/-   35.4503
Period (y)              255.5291 +/-    214.87
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           20.00370303 +/-    4.0351
Ecliptic Y           33.97727970 +/-    7.2123
Ecliptic Z           -1.85704700 +/-    0.3944
Ecliptic XDOT        -0.00241113 +/-    0.0014
Ecliptic YDOT         0.00135238 +/-    0.0015
Ecliptic ZDOT         0.00004822 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   39.47217114 +/-    6.5364
Geocenter to KBO     38.96260067 +/-    8.2737
# Hcoef:  7.99

The following table shows the complete astrometric record for 00SP331. 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 (00SP331) followed by the observatory code and reference code for the source of the astrometry.

2000 09  23.44526  03 56 52.97   +17 38 21.3   23.8R 00SP331   568  Cc1430      
2000 09  23.50233  03 56 52.85   +17 38 20.6   24.0R 00SP331   568  Cc1430      
2000 09  23.57560  03 56 52.68   +17 38 19.9         00SP331   568  Cc1430      
2000 09  24.46410  03 56 50.75   +17 38 11.0   23.5R 00SP331   568  Cc1430      
2000 09  24.51465  03 56 50.62   +17 38 10.6   23.5R 00SP331   568  Cc1430      
2000 09  24.57914  03 56 50.48   +17 38 09.8   23.7R 00SP331   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     0.09
  2   0.0002     -1.82     0.04      -0.34    -0.07
  3   0.0004     -4.34    -0.04      -0.53    -0.04
  4   0.0028    -33.17     0.07      -3.62    -0.03
  5   0.0029    -35.07    -0.09      -3.63     0.11
  6   0.0031    -37.19     0.02      -4.00    -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.

00SP331    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj       42.973    42.973    42.973
ecceobj        0.102     0.102     0.102
incobj         2.945     2.945     2.945
qmin          33.675    33.624    33.716
qmax          52.103    52.045    52.133
amean         42.652    42.651    42.651
amin          42.203    42.205    42.208
amax          43.103    43.091    43.118
emean          0.158     0.158     0.158
emin           0.088     0.088     0.088
emax           0.211     0.209     0.209
imean          5.934     5.934     5.934
imin           1.123     1.123     1.123
imax          10.728    10.719    10.717
fracstop       1.000     1.000     1.000
cjmean         3.037     3.037     3.037

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      180.0     179.8     179.9
kozaiamp       179.9     180.0     179.9