Orbit Fit and Astrometric record for 05TH173

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: 05TH173   
# Created Thu May 24 01:37:32 2012
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting    4 observations of    5
# Arc:  16.97d
# First observation: 2005/10/08
#  Last observation: 2005/10/25
# Chi-squared of fit:     1.09 DOF:    2 RMS:  0.09
# Min/Max residuals:    -0.08    0.20
# Exact a, adot, b, bdot, g, gdot:
  2.419634E-05  1.092183E-01 -7.554122E-06 -2.991658E-02  6.933485E-02 -1.398741E-04
# Covariance matrix:
  1.8253E-11  4.8801E-08 -4.7755E-14 -9.4433E-11  7.8680E-09  0.0000E+00
  4.8801E-08  1.3409E-04 -1.3119E-10 -2.5942E-07  2.1614E-05  0.0000E+00
 -4.7755E-14 -1.3119E-10  4.8445E-13 -1.0149E-11 -2.1146E-11  0.0000E+00
 -9.4433E-11 -2.5942E-07 -1.0149E-11  1.0712E-09 -4.1816E-08  0.0000E+00
  7.8680E-09  2.1614E-05 -2.1146E-11 -4.1816E-08  3.4840E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  1.1047E-03
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.669299   16.020669    0.018646   -0.011580   -1.003298  2453651.688943
# Heliocentric elements and errors
Epoch:              2453652.5000  =  2005/10/09
Mean Anomaly:          356.39672 +/-   351.289
Argument of Peri:      186.27886 +/-    58.134
Long of Asc Node:      193.66894 +/-     0.255
Inclination:            15.35474 +/-     5.939
Eccentricity:         0.03906887 +/-    0.4914
Semi-Major Axis:     16.04729167 +/-   13.8445
Time of Perihelion: 2453887.5155 +/-   37813.5
Perihelion:          15.42034212 +/-   15.4650
Aphelion:            16.67424122 +/-   16.4049
Period (y)               64.2852 +/-     83.19
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           14.82703146 +/-    0.9357
Ecliptic Y            4.23784616 +/-    0.2685
Ecliptic Z           -0.16860814 +/-    0.0114
Ecliptic XDOT        -0.00120674 +/-    0.0020
Ecliptic YDOT         0.00413337 +/-    0.0010
Ecliptic ZDOT        -0.00118117 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   15.42169445 +/-    0.9025
Geocenter to KBO     14.42279613 +/-    0.9735
# Hcoef: 11.07

The following table shows the complete astrometric record for 05TH173. 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 (05TH173) followed by the observatory code and reference code for the source of the astrometry.

2005 10  08.18820  01 00 04.20   +05 41 05.2   22.5R 05TH173   304  Co7771      
2005 10  08.22696  01 00 03.76   +05 41 01.5   22.4R 05TH173   304  Co7771      
2005 10  08.26516  01 00 03.33   +05 40 58.3   22.4R 05TH173   304  Co7771      
2005 10  25.15692  00 57 01.27   +05 17 04.2         05TH173   304  Co7771      
2005 10  25.20921  00 57 00.71   +05 17 00.1         05TH173   304  Co7771      

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 (  -0.44)      0.00 (  -3.41)
  2   0.0001      0.00     0.12       0.00    -0.08
  3   0.0002      0.00     0.09       0.00     0.03
  4   0.0465      0.00     0.20       0.00    -0.02
  5   0.0466      0.00     0.07       0.00     0.15

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.

05TH173    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        16.163    16.163    16.163
ecceobj         0.045     0.045     0.045
incobj         15.305    15.305    15.305
qmin           13.554    12.737    11.583
qmax           20.091    19.881    20.045
amean          16.351    16.161    15.966
amin           15.920    15.962    15.697
amax           17.450    16.742    16.466
emean           0.089     0.098     0.117
emin            0.021     0.041     0.041
emax            0.177     0.212     0.264
imean          15.431    15.330    15.642
imin           14.342    14.497    14.334
imax           17.559    16.563    16.844
excite_mean     0.282     0.284     0.296
fracstop        0.139     0.094     0.168
cjmean          3.256     3.268     3.277

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       181.7     184.3     182.4
kozaiamp        179.6     178.9     180.0