Orbit Fit and Astrometric record for 04VU130

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: 04VU130   
# Created Thu May 24 01:37:29 2012
# Orbit generated from Bernstein formalism
# Fitting   23 observations of   23
# Arc:   4.07y
# First observation: 2004/11/09
#  Last observation: 2008/12/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000213   0.017813   0.000034   0.002508   0.020349   0.000000
# Chi-squared of fit:    36.81 DOF:   40 RMS:  0.22
# Min/Max residuals:    -0.47    0.52
# Exact a, adot, b, bdot, g, gdot:
  1.373120E-05  1.835514E-02  4.249968E-06  2.585443E-03  2.053526E-02  7.709625E-03
# Covariance matrix:
  2.1682E-13 -2.2256E-13  1.0048E-14 -2.4322E-14  3.4023E-14 -2.5718E-12
 -2.2256E-13  5.1658E-13 -2.9366E-14  7.0995E-14 -2.5898E-14  7.5037E-12
  1.0048E-14 -2.9366E-14  1.5944E-13 -6.0670E-14  5.1877E-16 -4.5778E-13
 -2.4322E-14  7.0995E-14 -6.0670E-14  4.5006E-14 -1.6678E-15  1.1065E-12
  3.4023E-14 -2.5898E-14  5.1877E-16 -1.6678E-15  3.4095E-13 -1.9193E-13
 -2.5718E-12  7.5037E-12 -4.5778E-13  1.1065E-12 -1.9193E-13  1.1694E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.209426   41.389101   -0.097915   -0.003507   -0.987988  2453318.888263
# Heliocentric elements and errors
Epoch:              2453310.5000  =  2004/11/01
Mean Anomaly:           40.78302 +/-     0.050
Argument of Peri:      271.21602 +/-     0.014
Long of Asc Node:       42.95794 +/-     0.000
Inclination:             8.04235 +/-     0.001
Eccentricity:         0.42556653 +/-    0.0006
Semi-Major Axis:     61.87783274 +/-    0.0455
Time of Perihelion: 2433169.6414 +/-      11.3
Perihelion:          35.54469804 +/-    0.0463
Aphelion:            88.21096745 +/-    0.0753
Period (y)              486.7555 +/-      0.54
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           37.20563957 +/-    0.0010
Ecliptic Y           32.92443604 +/-    0.0009
Ecliptic Z           -0.17779328 +/-    0.0000
Ecliptic XDOT        -0.00084708 +/-    0.0000
Ecliptic YDOT         0.00250922 +/-    0.0000
Ecliptic ZDOT         0.00034103 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   49.68208646 +/-    0.0010
Geocenter to KBO     48.69673438 +/-    0.0014
# Hcoef:  7.09

The following table shows the complete astrometric record for 04VU130. 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 (04VU130) followed by the observatory code and reference code for the source of the astrometry.

2004 11  09.38752  02 36 05.92   +15 02 55.9   24.2r 04VU130   568  C~0D3L      
2004 11  09.41397  02 36 05.80   +15 02 55.5   23.8r 04VU130   568  C~0D3L      
2004 11  09.43995  02 36 05.69   +15 02 55.1   24.2r 04VU130   568  C~0D3L      
2004 11  10.30379  02 36 02.11   +15 02 39.5   24.3r 04VU130   568  C~0D3L      
2005 01  05.22568  02 33 08.33   +14 50 30.6   23.6i 04VU130   568  C~0WzI      
2005 01  05.28317  02 33 08.23   +14 50 30.2   23.7i 04VU130   568  C~0WzI      
2005 01  05.35171  02 33 08.14   +14 50 29.8   23.4i 04VU130   568  C~0WzI      
2005 10  25.50968  02 41 03.97   +15 34 57.3         04VU130   568  C~0WzI      
2005 10  25.54218  02 41 03.84   +15 34 57.0         04VU130   568  C~0WzI      
2005 10  25.57629  02 41 03.72   +15 34 56.1         04VU130   568  C~0WzI      
2005 10  26.54983  02 40 59.73   +15 34 39.1   23.2r 04VU130   568  C~0WzI      
2006 10  23.25324  02 45 06.56   +16 02 26.7         04VU130   675  C~0WzI      
2006 10  23.29181  02 45 06.42   +16 02 26.1   23. R 04VU130   675  C~0WzI      
2006 10  23.34180  02 45 06.21   +16 02 25.2         04VU130   675  C~0WzI      
2006 11  25.21958  02 42 52.08   +15 53 04.3         04VU130   695  C~0WzI      
2006 11  25.30950  02 42 51.71   +15 53 03.1         04VU130   695  C~0WzI      
2007 09  12.44494  02 51 06.80   +16 37 01.1   23.4r 04VU130   695  C~0WzI      
2007 09  12.48749  02 51 06.71   +16 37 00.6   23.3r 04VU130   695  C~0WzI      
2007 11  08.20228  02 47 52.23   +16 24 10.2   23.9r 04VU130   695  C~0WzI      
2007 11  08.26346  02 47 51.97   +16 24 09.2   24.0r 04VU130   695  C~0WzI      
2008 12  06.12735  02 49 47.77   +16 42 08.5         04VU130   675  C~0WzI      
2008 12  06.16505  02 49 47.65   +16 42 08.2   23.6R 04VU130   675  C~0WzI      
2008 12  06.21054  02 49 47.48   +16 42 07.9   23.8R 04VU130   675  C~0WzI      

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     0.08       0.00    -0.47
  2   0.0001     -1.78    -0.01       0.16    -0.36
  3   0.0001     -3.42     0.01       0.27    -0.29
  4   0.0025    -57.56    -0.11       1.46    -0.34
  5   0.1556  -2678.08     0.16      91.00     0.20
  6   0.1558  -2679.58    -0.05      91.08     0.16
  7   0.1560  -2680.95     0.12      91.10     0.06
  8   0.9586   4694.05    -0.29     508.30     0.23
  9   0.9587   4692.17    -0.14     508.58     0.46
 10   0.9588   4690.24     0.06     508.25     0.08
 11   0.9614   4630.12    -0.02     509.55    -0.01
 12   1.9517   8533.57    -0.10    1026.70     0.52
 13   1.9518   8531.46     0.15    1026.73     0.48
 14   1.9520   8528.30     0.05    1026.77     0.44
 15   2.0420   6512.05     0.07    1072.41    -0.19
 16   2.0422   6506.60    -0.08    1072.88     0.13
 17   2.8393  14117.88     0.15    1477.75    -0.19
 18   2.8394  14116.49     0.09    1477.65    -0.37
 19   2.9947  11205.64    -0.02    1562.70    -0.15
 20   2.9949  11201.75    -0.04    1562.85    -0.10
 21   4.0732  13117.70    -0.20    2105.23    -0.32
 22   4.0733  13115.96     0.06    2105.45    -0.16
 23   4.0734  13113.53     0.06    2105.88     0.20

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.

04VU130    quality flag:3

Type:          3:1EE     3:1EE     3:1EE

axisobj        62.980    63.120    62.840
ecceobj         0.432     0.434     0.430
incobj          8.000     8.000     8.000
qmin           35.487    35.278    35.463
qmax           90.857    90.826    91.091
amean          62.629    62.628    62.631
amin           62.158    62.275    62.030
amax           63.173    63.061    63.304
emean           0.432     0.433     0.431
emin            0.427     0.427     0.423
emax            0.438     0.440     0.439
imean           7.368     7.355     7.437
imin            7.244     7.209     7.092
imax            7.509     7.493     7.733
excite_mean     0.450     0.452     0.450
fracstop        1.000     1.000     1.000
cjmean          3.061     3.059     3.062

libcent 0       180.1     180.3     179.0
libamp  0       159.8     150.0     172.3
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       201.5     214.8     193.3
kozaiamp        179.9     180.0     180.0