Orbit Fit and Astrometric record for 06QG181

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: 06QG181   
# Created Fri May  2 02:36:57 2008
# Orbit generated from Bernstein formalism
# Fitting    9 observations of    9
# Arc:  60.03d
# First observation: 2006/08/21
#  Last observation: 2006/10/20
Preliminary a, adot, b, bdot, g, gdot:
  -0.000002   0.064392   0.000000   0.008179   0.043311   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     2.76 DOF:   13 RMS:  0.10
# Min/Max residuals:    -0.19    0.22
# Exact a, adot, b, bdot, g, gdot:
  2.321255E-05  6.171987E-02  3.903122E-06  7.936241E-03  4.182453E-02  3.625069E-03
# Covariance matrix:
  8.7018E-13 -3.1419E-10  2.1898E-14 -1.4214E-12 -9.4775E-11 -4.2308E-09
 -3.1419E-10  3.0943E-07 -3.5477E-11  6.2715E-09  1.0852E-07  7.4929E-06
  2.1898E-14 -3.5477E-11  5.1071E-13 -5.0675E-12 -1.6081E-11 -1.6975E-09
 -1.4214E-12  6.2715E-09 -5.0675E-12  5.9469E-10  3.4898E-09  4.4921E-07
 -9.4775E-11  1.0852E-07 -1.6081E-11  3.4898E-09  4.1846E-08  3.5005E-06
 -4.2308E-09  7.4929E-06 -1.6975E-09  4.4921E-07  3.5005E-06  3.8253E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.710527   46.784312    0.992010    0.002640   -0.202262  2453968.832664
# Heliocentric elements and errors
Epoch:              2453960.5000  =  2006/08/13
Mean Anomaly:            1.66848 +/-    30.437
Argument of Peri:        1.67042 +/-    68.184
Long of Asc Node:       38.99001 +/-     0.106
Inclination:             7.39000 +/-     0.127
Eccentricity:         0.35349767 +/-    0.0626
Semi-Major Axis:     37.29836972 +/-    2.6761
Time of Perihelion: 2453574.8875 +/-    7034.3
Perihelion:          24.11348275 +/-    2.9066
Aphelion:            50.48325670 +/-    4.3099
Period (y)              227.7944 +/-     24.52
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           17.22868094 +/-    0.0801
Ecliptic Y           16.88838931 +/-    0.0852
Ecliptic Z            0.29656800 +/-    0.0015
Ecliptic XDOT        -0.00278183 +/-    0.0009
Ecliptic YDOT         0.00292985 +/-    0.0009
Ecliptic ZDOT         0.00052237 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   24.12743444 +/-    0.0826
Geocenter to KBO     23.90941333 +/-    0.1169
# Hcoef:  8.43

The following table shows the complete astrometric record for 06QG181. 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 (06QG181) followed by the observatory code and reference code for the source of the astrometry.

2006 08  21.33191  02 56 25.50   +17 31 57.2   21.6R 06QG181   807  Cs5502      
2006 08  22.31581  02 56 25.58   +17 32 04.3         06QG181   807  Cs5502      
2006 08  23.30379  02 56 25.52   +17 32 10.4         06QG181   807  Cs5502      
2006 10  19.29748  02 52 23.03   +17 20 41.6   22.4R 06QG181   695  Ct0530      
2006 10  19.30906  02 52 22.94   +17 20 41.3         06QG181   695  Ct0530      
2006 10  20.22801  02 52 16.12   +17 20 16.7         06QG181   695  Ct0530      
2006 10  20.23969  02 52 16.03   +17 20 16.4         06QG181   695  Ct0530      
2006 10  20.35183  02 52 15.17   +17 20 13.6         06QG181   695  Ct0530      
2006 10  20.36327  02 52 15.10   +17 20 13.0         06QG181   695  Ct0530      

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     0.03       0.00    -0.19
  2   0.0027      3.12    -0.06       6.48     0.14
  3   0.0054      4.04     0.03      12.57     0.05
  4   0.1614  -3517.71     0.02     353.05    -0.04
  5   0.1615  -3519.03    -0.02     353.14    -0.03
  6   0.1640  -3619.65     0.00     358.00    -0.02
  7   0.1640  -3620.97    -0.01     358.09     0.00
  8   0.1643  -3633.57    -0.07     358.99     0.22
  9   0.1644  -3634.70     0.08     358.71    -0.13

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.

06QG181    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
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