Orbit Fit and Astrometric record for 03QY111

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: 03QY111   
# Created Fri May  2 02:36:52 2008
# Orbit generated from Bernstein formalism
# Fitting   10 observations of   10
# Arc:   1.13y
# First observation: 2003/08/25
#  Last observation: 2004/10/11
Preliminary a, adot, b, bdot, g, gdot:
  -0.000011   0.023811   0.000000  -0.000203   0.024227   0.000000
# Chi-squared of fit:    12.28 DOF:   14 RMS:  0.20
# Min/Max residuals:    -0.58    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.461390E-05  2.385805E-02 -4.659088E-07 -2.026251E-04  2.429215E-02  8.228398E-04
# Covariance matrix:
  4.4433E-13  4.0308E-13  4.5177E-16 -8.2120E-15  7.2045E-13  3.6699E-11
  4.0308E-13  4.9472E-12  3.3100E-15 -5.1221E-14  3.2899E-12  2.4055E-10
  4.5177E-16  3.3100E-15  2.7406E-13 -2.7881E-13  2.2903E-15  1.8491E-13
 -8.2120E-15 -5.1221E-14 -2.7881E-13  6.1285E-13 -3.9374E-14 -2.8395E-12
  7.2045E-13  3.2899E-12  2.2903E-15 -3.9374E-14  3.1506E-12  1.7890E-10
  3.6699E-11  2.4055E-10  1.8491E-13 -2.8395E-12  1.7890E-10  1.3368E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.968394   -3.582584    0.427292   -0.047627   -0.919600  2452876.779843
# Heliocentric elements and errors
Epoch:              2452870.5000  =  2003/08/19
Mean Anomaly:           41.04394 +/-     5.485
Argument of Peri:      216.16476 +/-     6.034
Long of Asc Node:       96.01010 +/-     0.037
Inclination:             2.94985 +/-     0.000
Eccentricity:         0.03362429 +/-    0.0035
Semi-Major Axis:     43.15647166 +/-    0.0129
Time of Perihelion: 2441064.1990 +/-    1577.7
Perihelion:          41.70536612 +/-    0.1514
Aphelion:            44.60757719 +/-    0.1514
Period (y)              283.5157 +/-      0.13
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.91953929 +/-    0.0030
Ecliptic Y           -3.04864372 +/-    0.0002
Ecliptic Z           -2.13179927 +/-    0.0002
Ecliptic XDOT         0.00025403 +/-    0.0000
Ecliptic YDOT         0.00267223 +/-    0.0000
Ecliptic ZDOT        -0.00002744 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.08427938 +/-    0.0030
Geocenter to KBO     41.16556284 +/-    0.0030
# Hcoef:  6.53

The following table shows the complete astrometric record for 03QY111. 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 (03QY111) followed by the observatory code and reference code for the source of the astrometry.

2003 08  25.27910  23 51 34.52   -04 08 53.1   22.2R 03QY111   807  Ci4592      
2003 08  25.38190  23 51 34.12   -04 08 56.1         03QY111   807  Ci4592      
2003 09  03.13413  23 50 58.52   -04 13 02.3   23.0R 03QY111   304  Ci4592      
2003 09  03.20601  23 50 58.25   -04 13 04.0         03QY111   304  Ci4592      
2003 10  22.15921  23 47 30.57   -04 35 00.5   22.5R 03QY111   695  Cj4700      
2003 10  22.25323  23 47 30.23   -04 35 02.5         03QY111   695  Cj4700      
2004 08  13.30947  23 57 16.35   -03 32 05.9   21.5R 03QY111   807  Cl8405      
2004 08  13.38192  23 57 16.10   -03 32 07.5         03QY111   807  Cl8405      
2004 10  11.21987  23 53 12.16   -03 59 13.1   23.0R 03QY111   695  Cl8405      
2004 10  11.31032  23 53 11.82   -03 59 15.6         03QY111   695  Cl8405      

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     0.19       0.00     0.07
  2   0.0003     -6.68     0.23      -0.37    -0.15
  3   0.0242   -593.25    -0.58     -14.29     0.08
  4   0.0244   -597.63     0.08     -14.25     0.19
  5   0.1585  -3971.52    -0.02      11.79    -0.08
  6   0.1587  -3976.98     0.10      11.97    -0.15
  7   0.9693   5573.06     0.02     -16.30    -0.03
  8   0.9695   5568.99    -0.01     -16.27     0.15
  9   1.1306   1571.07    -0.23     -49.83     0.19
 10   1.1308   1565.41     0.21     -50.10    -0.27

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.

03QY111    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj       43.614    43.614    43.614
ecceobj        0.043     0.043     0.043
incobj         2.950     2.950     2.950
qmin          40.876    40.875    40.882
qmax          46.028    46.018    46.028
amean         43.373    43.373    43.373
amin          43.045    43.044    43.048
amax          43.718    43.718    43.714
emean          0.036     0.036     0.036
emin           0.017     0.017     0.017
emax           0.053     0.053     0.053
imean          1.354     1.354     1.354
imin           0.411     0.411     0.411
imax           2.057     2.057     2.057
fracstop       1.000     1.000     1.000
cjmean         3.092     3.092     3.092

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      171.2     171.0     171.1
kozaiamp       180.0     180.0     180.0