Orbit Fit and Astrometric record for 04UU10

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory.

# Object: 04UU10    
# Created Fri May  2 02:36:55 2008
# Orbit generated from Bernstein formalism
# Fitting    6 observations of    6
# Arc:  58.27d
# First observation: 2004/10/17
#  Last observation: 2004/12/14
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.022569   0.000001  -0.000731   0.022413   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# Chi-squared of fit:     4.51 DOF:    7 RMS:  0.15
# Min/Max residuals:    -0.30    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.443525E-05  2.005907E-02  1.846015E-08 -6.839974E-04  2.208303E-02 -5.187277E-03
# Covariance matrix:
  7.1442E-13  3.0128E-10 -3.9517E-15 -5.9624E-12  5.9244E-11 -3.7173E-09
  3.0128E-10  4.0729E-07 -5.2487E-12 -7.9453E-09  7.7238E-08 -5.7140E-06
 -3.9517E-15 -5.2487E-12  4.8585E-13 -2.9966E-12 -1.0336E-12  5.9718E-11
 -5.9624E-12 -7.9453E-09 -2.9966E-12  1.9594E-10 -1.5387E-09  9.9862E-08
  5.9244E-11  7.7238E-08 -1.0336E-12 -1.5387E-09  1.6655E-08 -3.5120E-07
 -3.7173E-09 -5.7140E-06  5.9718E-11  9.9862E-08 -3.5120E-07  3.4765E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.222397   10.141548   -0.236410   -0.020617   -0.971514  2453295.559443
# Heliocentric elements and errors
Epoch:              2453290.5000  =  2004/10/12
Mean Anomaly:          290.53552 +/-   101.757
Argument of Peri:      309.73195 +/-    37.836
Long of Asc Node:      158.80368 +/-     0.731
Inclination:             2.28103 +/-     0.047
Eccentricity:         0.24831181 +/-    0.8880
Semi-Major Axis:     47.57104839 +/-   24.1531
Time of Perihelion: 2476415.0245 +/-   28936.7
Perihelion:          35.75859536 +/-   45.9796
Aphelion:            59.38350143 +/-   51.8995
Period (y)              328.1121 +/-    249.89
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           45.47655646 +/-    0.2604
Ecliptic Y            8.37706418 +/-    0.0466
Ecliptic Z           -0.96606220 +/-    0.0056
Ecliptic XDOT        -0.00107401 +/-    0.0023
Ecliptic YDOT         0.00232739 +/-    0.0004
Ecliptic ZDOT        -0.00007097 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.25176394 +/-    0.2562
Geocenter to KBO     45.28363730 +/-    0.2646
# Hcoef:  8.73

The following table shows the complete astrometric record for 04UU10. 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 (04UU10) followed by the observatory code and reference code for the source of the astrometry.

2004 10  17.05870  00 39 12.10   +02 53 30.9         04UU10    304  Cn7976      
2004 10  17.09701  00 39 11.94   +02 53 30.2         04UU10    304  Cn7976      
2004 10  17.13526  00 39 11.79   +02 53 29.0         04UU10    304  Cn7976      
2004 12  12.31999  00 36 39.25   +02 37 57.2   25.2R 04UU10    568  Cn7976      
2004 12  13.33042  00 36 38.36   +02 37 53.3   25.1R 04UU10    568  Cn7976      
2004 12  14.32403  00 36 37.64   +02 37 49.7   25.1R 04UU10    568  Cn7976      

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    -0.01       0.00    -0.10
  2   0.0001     -2.48     0.02       0.30     0.17
  3   0.0002     -5.02    -0.01       0.07    -0.07
  4   0.1540  -2472.91     0.15      39.58    -0.21
  5   0.1568  -2486.71    -0.30      41.23     0.23
  6   0.1595  -2498.05     0.15      42.15    -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.

04UU10    quality flag:3

Type:           2:1E      2:1E      2:1E

axisobj       48.167    48.166    48.167
ecceobj        0.248     0.248     0.248
incobj         2.271     2.271     2.271
qmin          35.374    35.376    35.375
qmax          61.610    61.573    61.578
amean         47.801    47.800    47.799
amin          46.980    46.977    46.963
amax          48.723    48.715    48.724
emean          0.247     0.248     0.248
emin           0.231     0.231     0.230
emax           0.264     0.264     0.264
imean          2.321     2.312     2.291
imin           1.752     1.763     1.686
imax           2.869     2.826     2.826
fracstop       1.000     1.000     1.000
cjmean         3.069     3.069     3.069

libcent 0      180.2     179.9     179.9
libamp  0      169.1     169.3     169.4
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      170.7     175.0     171.9
kozaiamp       180.0     179.9     180.0