Orbit Fit and Astrometric record for 00SE331

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: 00SE331   
# Created Fri Mar 29 01:10:21 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:     0.87 DOF:      8 RMS:  0.07
# Min/Max residuals:    -0.13    0.09
# Exact a, adot, b, bdot, g, gdot:
  1.578051E-05  2.237181E-02 -8.600134E-07 -1.814572E-03  2.336680E-02  0.000000E+00
# Covariance matrix:
  9.5133E-11  1.3886E-07  5.1544E-12  8.1295E-09  4.2443E-08  0.0000E+00
  1.3886E-07  2.0397E-04  7.5592E-09  1.1923E-05  6.2246E-05  0.0000E+00
  5.1544E-12  7.5592E-09  6.4522E-13  3.1322E-10  2.3085E-09  0.0000E+00
  8.1295E-09  1.1923E-05  3.1322E-10  8.3576E-07  3.6409E-06  0.0000E+00
  4.2443E-08  6.2246E-05  2.3085E-09  3.6409E-06  1.9009E-05  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  1.6789E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.051788   60.552968    0.865228   -0.017983   -0.496823  2451810.929573
# Heliocentric elements and errors
Epoch:              2451810.5000  =  2000/09/23
Mean Anomaly:          315.24518 +/-   227.118
Argument of Peri:      250.57345 +/-   278.355
Long of Asc Node:      215.93699 +/-    23.295
Inclination:             5.08008 +/-     4.701
Eccentricity:         0.02745272 +/-    0.6489
Semi-Major Axis:     44.15158532 +/-   24.0880
Time of Perihelion: 2465132.0625 +/-  388919.5
Perihelion:          42.93950400 +/-   37.0096
Aphelion:            45.36366664 +/-   37.8606
Period (y)              293.3781 +/-    240.09
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           22.02838605 +/-    3.9234
Ecliptic Y           37.25546378 +/-    6.9489
Ecliptic Z           -1.53223285 +/-    0.2859
Ecliptic XDOT        -0.00229383 +/-    0.0013
Ecliptic YDOT         0.00128709 +/-    0.0014
Ecliptic ZDOT        -0.00021232 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   43.30781813 +/-    6.3021
Geocenter to KBO     42.79575524 +/-    7.9851
# Hcoef:  7.91

The following table shows the complete astrometric record for 00SE331. 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 (00SE331) followed by the observatory code and reference code for the source of the astrometry.

2000 09  23.42883  03 55 22.83   +18 15 33.5   24.1R 00SE331   568  Cc1430      
2000 09  23.55431  03 55 22.58   +18 15 32.5   24.2R 00SE331   568  Cc1430      
2000 09  23.62225  03 55 22.44   +18 15 31.8         00SE331   568  Cc1430      
2000 09  24.43323  03 55 20.78   +18 15 23.7   23.8R 00SE331   568  Cc1430      
2000 09  24.49743  03 55 20.64   +18 15 23.2   24.1R 00SE331   568  Cc1430      
2000 09  24.56052  03 55 20.50   +18 15 22.6   23.9R 00SE331   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    -0.13       0.00    -0.08
     2   0.0003     -3.69     0.06      -0.25     0.07
     3   0.0005     -5.79     0.09      -0.52     0.02
     4   0.0027    -30.59    -0.00      -3.58    -0.10
     5   0.0029    -32.65     0.00      -3.65     0.03
     6   0.0031    -34.72    -0.03      -3.83     0.05

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.

00SE331    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