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. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.

# Object: 00SP331   
# Created Wed Nov 27 02:08:07 2024
# 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  2.583130E-02 -1.814301E-07  4.510951E-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   -0.493453  2451810.946003
# Heliocentric elements and errors
Epoch:              2451810.5000  =  2000/09/23
Mean Anomaly:          313.52627 +/-   191.396
Argument of Peri:      338.21576 +/-   224.824
Long of Asc Node:      130.24862 +/-    47.437
Inclination:             2.85628 +/-     0.813
Eccentricity:         0.02935725 +/-    0.6649
Semi-Major Axis:     40.26751665 +/-   22.5739
Time of Perihelion: 2463859.0756 +/-  329460.8
Perihelion:          39.08537298 +/-   34.5960
Aphelion:            41.44966033 +/-   35.4503
Period (y)              255.5292 +/-    214.87
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           20.00370241 +/-    4.0351
Ecliptic Y           33.97727859 +/-    7.2123
Ecliptic Z           -1.85704694 +/-    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   39.47216986 +/-    6.5364
Geocenter to KBO     38.96259940 +/-    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: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