Orbit Fit and Astrometric record for 00YB29

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: 00YB29    
# Created Wed Nov 27 02:08:09 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:  11.02d
# First observation: 2000/12/21
#  Last observation: 2001/01/01
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.031909  -0.000001  -0.000432   0.027417   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     0.70 DOF:      7 RMS:  0.06
# Min/Max residuals:    -0.12    0.07
# Exact a, adot, b, bdot, g, gdot:
  1.794121E-05  3.201521E-02 -4.824043E-07 -2.303612E-04  2.781283E-02  1.040292E-03
# Covariance matrix:
  8.0157E-13 -8.1163E-11  1.0719E-13  1.7927E-10  2.1364E-10  4.0884E-10
 -8.1163E-11  1.2190E-08 -1.5634E-11 -2.7496E-08 -3.2470E-08  2.7594E-07
  1.0719E-13 -1.5634E-11  4.3839E-13  2.9988E-11  6.0523E-11  1.5608E-09
  1.7927E-10 -2.7496E-08  2.9988E-11  8.3882E-08  9.7433E-08  6.1287E-07
  2.1364E-10 -3.2470E-08  6.0523E-11  9.7433E-08  1.1695E-07  1.1712E-06
  4.0884E-10  2.7594E-07  1.5608E-09  6.1287E-07  1.1712E-06  5.0227E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.623103    3.083352   -0.977416    0.006910   -0.052815  2451899.768363
# Heliocentric elements and errors
Epoch:              2451890.5000  =  2000/12/12
Mean Anomaly:           11.42216 +/-   129.744
Argument of Peri:       76.18055 +/-   212.682
Long of Asc Node:      270.14862 +/-     3.884
Inclination:             7.63130 +/-     0.040
Eccentricity:         0.22099781 +/-    0.2214
Semi-Major Axis:     45.82309745 +/-    4.3835
Time of Perihelion: 2448295.7321 +/-   40829.6
Perihelion:          35.69629323 +/-   10.7031
Aphelion:            55.94990167 +/-   11.4692
Period (y)              310.1951 +/-     44.51
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           35.59057643 +/-    0.4375
Ecliptic Y            2.90124963 +/-    0.0236
Ecliptic Z            4.76958146 +/-    0.0586
Ecliptic XDOT        -0.00007322 +/-    0.0022
Ecliptic YDOT         0.00315669 +/-    0.0001
Ecliptic ZDOT        -0.00000871 +/-    0.0003
# Distances at JD0 (AU)
Heliocenter to KBO   36.02575866 +/-    0.4323
Geocenter to KBO     35.95462555 +/-    0.4421
# Hcoef:  7.73

The following table shows the complete astrometric record for 00YB29. 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 (00YB29) followed by the observatory code and reference code for the source of the astrometry.

2000 12  21.26762  23 59 06.46   +08 12 59.9   23.1R 00YB29    568  Cc4155      
2000 12  22.23942  23 59 07.61   +08 12 53.1         00YB29    568  Cc4155      
2000 12  22.30697  23 59 07.69   +08 12 52.6         00YB29    568  Cc4155      
2000 12  24.22544  23 59 10.29   +08 12 41.4         00YB29    568  Cc4155      
2000 12  24.33879  23 59 10.45   +08 12 40.7         00YB29    568  Cc4155      
2001 01  01.28435  23 59 25.44   +08 12 22.9         00YB29    568  Cc4155      

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     0.05       0.00     0.07
     2   0.0027     12.91    -0.05     -13.08     0.04
     3   0.0028     13.80    -0.05     -14.01    -0.01
     4   0.0081     44.66     0.03     -39.76    -0.01
     5   0.0084     46.55     0.03     -41.36    -0.12
     6   0.0302    243.26    -0.00    -146.95     0.03

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.

00YB29    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