Orbit Fit and Astrometric record for 00SM331

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: 00SM331   
# 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
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:     1.46 DOF:    8 RMS:  0.09
# Min/Max residuals:    -0.18    0.12
# Exact a, adot, b, bdot, g, gdot:
  1.618923E-05  2.747720E-02  4.838098E-06  7.416194E-03  2.744720E-02  0.000000E+00
# Covariance matrix:
  1.6605E-10  2.8566E-07  1.2827E-11  2.3128E-08  8.6881E-08  0.0000E+00
  2.8566E-07  4.9322E-04  2.2131E-08  3.9901E-05  1.4989E-04  0.0000E+00
  1.2827E-11  2.2131E-08  1.3850E-12  1.6481E-09  6.7274E-09  0.0000E+00
  2.3128E-08  3.9901E-05  1.6481E-09  3.3673E-06  1.2129E-05  0.0000E+00
  8.6881E-08  1.4989E-04  6.7274E-09  1.2129E-05  4.5566E-05  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  2.7209E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.874537   60.419605    0.864118   -0.025212   -0.498442  2451810.924063
# Heliocentric elements and errors
Epoch:              2451810.5000  =  2000/09/23
Mean Anomaly:          300.71131 +/-   208.196
Argument of Peri:       51.00984 +/-   284.377
Long of Asc Node:       69.53129 +/-     5.467
Inclination:            15.25773 +/-     8.018
Eccentricity:         0.02549597 +/-    0.6456
Semi-Major Axis:     37.41767015 +/-   21.7270
Time of Perihelion: 2465578.8827 +/-  382566.2
Perihelion:          36.46367047 +/-   32.1230
Aphelion:            38.37166982 +/-   32.8638
Period (y)              228.8882 +/-    199.36
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           18.96536866 +/-    4.4179
Ecliptic Y           31.65734614 +/-    7.7825
Ecliptic Z           -1.82692327 +/-    0.4493
Ecliptic XDOT        -0.00237276 +/-    0.0016
Ecliptic YDOT         0.00139032 +/-    0.0016
Ecliptic ZDOT         0.00073899 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   36.94875400 +/-    7.0431
Geocenter to KBO     36.43359306 +/-    8.9603
# Hcoef:  8.47

The following table shows the complete astrometric record for 00SM331. 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 (00SM331) followed by the observatory code and reference code for the source of the astrometry.

2000 09  23.42332  03 55 32.66   +17 25 36.3   24.0R 00SM331   568  Cc1430      
2000 09  23.54753  03 55 32.36   +17 25 35.7   23.9R 00SM331   568  Cc1430      
2000 09  23.61663  03 55 32.19   +17 25 35.1         00SM331   568  Cc1430      
2000 09  24.42582  03 55 30.22   +17 25 29.2   24.0R 00SM331   568  Cc1430      
2000 09  24.49186  03 55 30.07   +17 25 28.7   23.8R 00SM331   568  Cc1430      
2000 09  24.55453  03 55 29.91   +17 25 28.2   23.8R 00SM331   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    -0.07       0.00    -0.12
  2   0.0003     -4.33     0.05       0.30     0.12
  3   0.0005     -6.83     0.06       0.21     0.01
  4   0.0027    -35.63    -0.18       0.24     0.07
  5   0.0029    -37.84     0.07       0.19    -0.01
  6   0.0031    -40.18     0.08       0.17    -0.06

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.

00SM331    quality flag:3

Type:       SCATNEAR  SCATNEAR  SCATNEAR

axisobj       38.161    38.161    38.161
ecceobj        0.040     0.040     0.040
incobj        14.995    14.995    14.995
qmin          30.880    31.896    32.263
qmax          44.271    44.371    44.061
amean         37.799    37.908    37.903
amin          36.687    37.529    37.513
amax          38.212    38.367    38.425
emean          0.093     0.096     0.091
emin           0.026     0.026     0.026
emax           0.163     0.159     0.149
imean         16.244    16.287    16.145
imin          12.509    12.505    12.515
imax          21.677    21.278    20.749
fracstop       1.000     1.000     1.000
cjmean         2.930     2.930     2.932

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      176.8     178.2     178.3
kozaiamp       179.9     180.0     180.0