Orbit Fit and Astrometric record for 04VV75

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: 04VV75    
# Created Wed Dec  4 02:08:41 2024
# Orbit generated from Bernstein formalism
# Fitting      5 observations of      5
# Arc:   9.15d
# First observation: 2004/11/09
#  Last observation: 2004/11/18
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.088078   0.000000   0.008704   0.043063   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:     4.39 DOF:      5 RMS:  0.17
# Min/Max residuals:    -0.27    0.22
# Exact a, adot, b, bdot, g, gdot:
  2.044189E-05  4.736087E-02  3.952492E-06  8.145075E-03  3.640188E-02  8.291635E-03
# Covariance matrix:
  4.3266E-11  9.4149E-08  1.9456E-13  1.3164E-09  1.5492E-08 -8.6850E-08
  9.4149E-08  2.0749E-04  4.2896E-10  2.8992E-06  3.4130E-05 -1.9780E-04
  1.9456E-13  4.2896E-10  5.1561E-13 -1.5662E-11  7.0538E-11 -4.3968E-10
  1.3164E-09  2.8992E-06 -1.5662E-11  4.2663E-08  4.7700E-07 -2.6281E-06
  1.5492E-08  3.4130E-05  7.0538E-11  4.7700E-07  5.6145E-06 -3.2018E-05
 -8.6850E-08 -1.9780E-04 -4.3968E-10 -2.6281E-06 -3.2018E-05  9.0169E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.609526   35.286742   -0.199005    0.044377   -0.971722  2453318.689463
# Heliocentric elements and errors
Epoch:              2453310.5000  =  2004/11/01
Mean Anomaly:           20.53347 +/-    61.612
Argument of Peri:      332.71774 +/-   137.564
Long of Asc Node:       21.39041 +/-     3.860
Inclination:            10.10272 +/-     2.654
Eccentricity:         0.33418487 +/-    0.4805
Semi-Major Axis:     39.99174832 +/-   22.6439
Time of Perihelion: 2448041.6731 +/-   15162.9
Perihelion:          26.62711106 +/-   24.4246
Aphelion:            53.35638559 +/-   35.8046
Period (y)              252.9087 +/-    214.80
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           23.07510222 +/-    1.4582
Ecliptic Y           16.57824214 +/-    1.0318
Ecliptic Z            1.25085198 +/-    0.0814
Ecliptic XDOT        -0.00157313 +/-    0.0021
Ecliptic YDOT         0.00324422 +/-    0.0012
Ecliptic ZDOT         0.00064045 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   28.44051838 +/-    1.3272
Geocenter to KBO     27.47110905 +/-    1.7882
# Hcoef:  8.38

The following table shows the complete astrometric record for 04VV75. 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 (04VV75) followed by the observatory code and reference code for the source of the astrometry.

2004 11  09.18872  02 08 21.89   +15 44 33.6   22.1R 04VV75    695  Cm0643      
2004 11  09.28093  02 08 21.27   +15 44 31.1         04VV75    695  Cm0643      
2004 11  10.26483  02 08 14.74   +15 44 00.3         04VV75    695  Cm0643      
2004 11  18.29880  02 07 23.22   +15 39 57.3   23.0R 04VV75    568  Cm0643      
2004 11  18.33894  02 07 22.95   +15 39 55.8         04VV75    568  Cm0643      

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     0.03       0.00    -0.09
     2   0.0003     -9.27     0.18       0.67     0.22
     3   0.0029   -108.41    -0.27       3.48    -0.15
     4   0.0249   -890.74     0.16      26.21     0.11
     5   0.0251   -894.91    -0.16      26.12    -0.10

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.

04VV75    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