Orbit Fit and Astrometric record for 04PU107

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: 04PU107   
# Created Fri Apr 19 01:11:59 2024
# Orbit generated from Bernstein formalism
# Fitting      5 observations of      5
# Arc:  28.92d
# First observation: 2004/08/13
#  Last observation: 2004/09/11
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.021222  -0.000001   0.000629   0.022140   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     2.05 DOF:      5 RMS:  0.11
# Min/Max residuals:    -0.18    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.313113E-05  1.682248E-02 -4.606934E-07  7.591310E-04  2.143255E-02 -1.033000E-02
# Covariance matrix:
  3.2560E-11  3.9224E-08 -2.8989E-14 -1.1229E-09  6.8178E-09  3.3861E-08
  3.9224E-08  4.8004E-05 -3.5363E-11 -1.3742E-06  8.3413E-06  4.0473E-05
 -2.8989E-14 -3.5363E-11  4.9384E-13 -5.3263E-12 -6.1590E-12 -3.9572E-11
 -1.1229E-09 -1.3742E-06 -5.3263E-12  3.9540E-08 -2.3877E-07 -1.1505E-06
  6.8178E-09  8.3413E-06 -6.1590E-12 -2.3877E-07  1.4496E-06  7.1577E-06
  3.3861E-08  4.0473E-05 -3.9572E-11 -1.1505E-06  7.1577E-06  1.1902E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -4.693242  -43.797166   -0.080885   -0.082868   -1.010556  2453230.654713
# Heliocentric elements and errors
Epoch:              2453230.5000  =  2004/08/13
Mean Anomaly:          302.07101 +/-    54.498
Argument of Peri:       59.64447 +/-    59.259
Long of Asc Node:       16.11006 +/-    16.814
Inclination:             5.31090 +/-     0.908
Eccentricity:         0.52182020 +/-    0.5109
Semi-Major Axis:     48.63702703 +/-   25.1275
Time of Perihelion: 2473166.7023 +/-   10633.7
Perihelion:          23.25724363 +/-   27.5994
Aphelion:            74.01681043 +/-   45.6028
Period (y)              339.2023 +/-    262.86
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           34.34872306 +/-    1.8853
Ecliptic Y          -32.82570703 +/-    1.8081
Ecliptic Z           -3.81762772 +/-    0.2145
Ecliptic XDOT         0.00054182 +/-    0.0014
Ecliptic YDOT         0.00244884 +/-    0.0008
Ecliptic ZDOT         0.00020473 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   47.66483084 +/-    1.8430
Geocenter to KBO     46.65800155 +/-    2.6210
# Hcoef:  6.63

The following table shows the complete astrometric record for 04PU107. 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 (04PU107) followed by the observatory code and reference code for the source of the astrometry.

2004 08  13.15397  21 20 37.17   -20 27 13.4   22.5R 04PU107   807  Cl2777      
2004 08  13.26006  21 20 36.72   -20 27 15.7         04PU107   807  Cl2777      
2004 08  14.22746  21 20 32.41   -20 27 34.0         04PU107   807  Cl2777      
2004 09  11.04183  21 18 36.66   -20 35 02.2   23.6R 04PU107   304  Cl4404      
2004 09  11.06976  21 18 36.55   -20 35 02.5         04PU107   304  Cl4404      

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    -0.15       0.00     0.21
     2   0.0003     -6.72     0.16      -0.25    -0.18
     3   0.0029    -69.99    -0.01       0.89    -0.03
     4   0.0791  -1755.33     0.02      69.84    -0.04
     5   0.0792  -1756.89    -0.02      70.02     0.04

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.

04PU107    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