Orbit Fit and Astrometric record for 05QU182

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: 05QU182   
# Created Fri May  2 02:36:56 2008
# Orbit generated from Bernstein formalism
# Fitting    7 observations of    7
# Arc:  66.78d
# First observation: 2005/08/30
#  Last observation: 2005/11/05
Preliminary a, adot, b, bdot, g, gdot:
  -0.000006   0.028771   0.000005   0.001427   0.022867   0.000000
# Chi-squared of fit:     5.35 DOF:    8 RMS:  0.15
# Min/Max residuals:    -0.29    0.29
# Exact a, adot, b, bdot, g, gdot:
  1.735080E-05  2.421228E-02  1.360741E-06  1.528606E-03  2.215675E-02  6.784054E-03
# Covariance matrix:
  5.0387E-13  1.9150E-11  2.0429E-14 -3.9482E-13  4.0541E-12  1.0697E-10
  1.9150E-11  3.0920E-08  2.9535E-11 -6.7501E-10  4.7351E-09 -1.5500E-07
  2.0429E-14  2.9535E-11  4.8706E-13 -3.5730E-12  4.5124E-12 -1.5329E-10
 -3.9482E-13 -6.7501E-10 -3.5730E-12  4.9451E-11 -1.0148E-10  4.0392E-09
  4.0541E-12  4.7351E-09  4.5124E-12 -1.0148E-10  7.4126E-10 -1.8784E-08
  1.0697E-10 -1.5500E-07 -1.5329E-10  4.0392E-09 -1.8784E-08  2.3970E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
  -13.847554    3.832152    0.454681   -0.216551   -0.878866  2453612.853943
# Heliocentric elements and errors
Epoch:              2453610.5000  =  2005/08/28
Mean Anomaly:           11.34393 +/-     1.978
Argument of Peri:      240.31185 +/-     7.267
Long of Asc Node:       79.02668 +/-     0.125
Inclination:            13.99097 +/-     0.008
Eccentricity:         0.54923557 +/-    0.0563
Semi-Major Axis:     92.13203536 +/-    7.8726
Time of Perihelion: 2443432.1938 +/-    1203.5
Perihelion:          41.52984413 +/-    6.2852
Aphelion:           142.73422659 +/-   13.2539
Period (y)              884.3500 +/-    113.35
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           44.65257063 +/-    0.0537
Ecliptic Y            2.53494951 +/-    0.0036
Ecliptic Z          -10.80201258 +/-    0.0133
Ecliptic XDOT         0.00065902 +/-    0.0002
Ecliptic YDOT         0.00303585 +/-    0.0000
Ecliptic ZDOT        -0.00001722 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.01044999 +/-    0.0522
Geocenter to KBO     45.13297198 +/-    0.0555
# Hcoef:  3.67

The following table shows the complete astrometric record for 05QU182. 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 (05QU182) followed by the observatory code and reference code for the source of the astrometry.

2005 08  30.35320  00 36 18.04   -11 10 23.9   20.2R 05QU182   644  Cv4445      
2005 08  30.42829  00 36 17.80   -11 10 26.1   19.7R 05QU182   644  Cv4445      
2005 08  30.49423  00 36 17.55   -11 10 27.9   20.5R 05QU182   644  Cv4445      
2005 10  12.23332  00 33 31.75   -11 28 57.0         05QU182   644  Cv4445      
2005 10  12.30144  00 33 31.47   -11 28 57.7         05QU182   644  Cv4445      
2005 11  05.10313  00 32 03.70   -11 34 14.2   19.7R 05QU182   644  Cv4445      
2005 11  05.13332  00 32 03.60   -11 34 14.1   19.8R 05QU182   644  Cv4445      

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    -0.06
  2   0.0002     -4.12     0.17      -0.58    -0.12
  3   0.0004     -8.21    -0.15      -0.74     0.18
  4   0.1174  -2687.10    -0.11     -31.68    -0.29
  5   0.1176  -2691.15     0.11     -30.66     0.29
  6   0.1828  -3999.96    -0.06     197.86    -0.14
  7   0.1828  -4001.26     0.06     198.55     0.14

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.

05QU182    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