Orbit Fit and Astrometric record for 02GH166

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: 02GH166   
# Created Thu May 24 01:37:12 2012
# Orbit generated from Bernstein formalism
# Fitting    5 observations of    5
# Arc:  35.04d
# First observation: 2002/04/03
#  Last observation: 2002/05/08
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.044303   0.000002  -0.005575   0.032661   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# Chi-squared of fit:     5.40 DOF:    5 RMS:  0.18
# Min/Max residuals:    -0.41    0.30
# Exact a, adot, b, bdot, g, gdot:
  1.720636E-05  3.378610E-02 -8.691965E-07 -5.594374E-03  3.098241E-02 -1.055281E-02
# Covariance matrix:
  5.0576E-12  6.1934E-09 -1.0496E-13  9.0750E-12  1.0004E-09 -2.6933E-08
  6.1934E-09  1.0486E-05 -2.1997E-10  2.0842E-08  1.6667E-06 -5.5111E-05
 -1.0496E-13 -2.1997E-10  6.1968E-13 -7.8166E-12 -3.4483E-11  1.3389E-09
  9.0750E-12  2.0842E-08 -7.8166E-12  2.2072E-10  3.2507E-09 -1.3320E-07
  1.0004E-09  1.6667E-06 -3.4483E-11  3.2507E-09  2.6521E-07 -8.6518E-06
 -2.6933E-08 -5.5111E-05  1.3389E-09 -1.3320E-07 -8.6518E-06  3.3083E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.142088 -168.377318   -0.036340   -0.002575   -1.001254  2452367.873603
# Heliocentric elements and errors
Epoch:              2452360.5000  =  2002/03/27
Mean Anomaly:          310.01750 +/-    50.537
Argument of Peri:      265.35173 +/-    16.795
Long of Asc Node:       10.84424 +/-     0.080
Inclination:             9.39545 +/-     0.902
Eccentricity:         0.31500142 +/-    0.5704
Semi-Major Axis:     38.05513748 +/-   19.6378
Time of Perihelion: 2464265.6229 +/-    7744.3
Perihelion:          26.06771522 +/-   25.5377
Aphelion:            50.04255973 +/-   33.7355
Period (y)              234.7622 +/-    181.72
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -32.58701037 +/-    0.5255
Ecliptic Y           -6.73490343 +/-    0.1080
Ecliptic Z           -0.08004039 +/-    0.0013
Ecliptic XDOT         0.00150773 +/-    0.0016
Ecliptic YDOT        -0.00273759 +/-    0.0001
Ecliptic ZDOT        -0.00049183 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   33.27579564 +/-    0.5151
Geocenter to KBO     32.27637756 +/-    0.5365
# Hcoef:  6.46

The following table shows the complete astrometric record for 02GH166. 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 (02GH166) followed by the observatory code and reference code for the source of the astrometry.

2002 04  03.37286  12 42 31.42   -04 43 38.3   21.5R 02GH166   644  Cl2691      
2002 04  09.04270  12 41 59.38   -04 40 33.0   20.7R 02GH166   807  Cf7585      
2002 04  09.14504  12 41 58.81   -04 40 29.9         02GH166   807  Cf7585      
2002 05  08.34585  12 39 29.86   -04 26 19.4   21.7R 02GH166   568  Cf7585      
2002 05  08.41063  12 39 29.57   -04 26 17.8         02GH166   568  Cf7585      

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    -0.41
  2   0.0155   -513.30    -0.14     -16.76     0.30
  3   0.0158   -522.36     0.13     -17.24     0.19
  4   0.0958  -2904.93     0.03    -106.65    -0.04
  5   0.0959  -2909.54    -0.03    -106.88    -0.04

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.

02GH166    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