Orbit Fit and Astrometric record for 11UX412

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: 11UX412   
# Created Wed Nov 27 02:09:13 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:  36.89d
# First observation: 2011/10/24
#  Last observation: 2011/11/30
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.023354  -0.000001  -0.009422   0.022779   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     1.04 DOF:      9 RMS:  0.07
# Min/Max residuals:    -0.10    0.11
# Exact a, adot, b, bdot, g, gdot:
  1.272984E-05  1.732226E-02 -7.181346E-06 -9.545991E-03  2.182532E-02 -8.416487E-03
# Covariance matrix:
  1.1619E-12  9.2202E-10 -8.8270E-14  1.7736E-11  1.4868E-10 -3.8287E-09
  9.2202E-10  1.1803E-06 -1.2169E-10  2.4417E-08  1.8593E-07 -6.7877E-06
 -8.8270E-14 -1.2169E-10  3.5182E-13 -6.7857E-12 -1.8963E-11  8.1236E-10
  1.7736E-11  2.4417E-08 -6.7857E-12  6.6101E-10  3.8058E-09 -1.6263E-07
  1.4868E-10  1.8593E-07 -1.8963E-11  3.8058E-09  2.9371E-08 -1.0263E-06
 -3.8287E-09 -6.7877E-06  8.1236E-10 -1.6263E-07 -1.0263E-06  6.2352E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.856190   31.933288    0.023858    0.049385   -0.989740  2455858.938316
# Heliocentric elements and errors
Epoch:              2455850.5000  =  2011/10/16
Mean Anomaly:          313.91707 +/-    36.934
Argument of Peri:      267.22994 +/-    12.371
Long of Asc Node:      216.96954 +/-     0.322
Inclination:            28.93814 +/-     1.542
Eccentricity:         0.41597685 +/-    0.3944
Semi-Major Axis:     55.36850242 +/-   24.9265
Time of Perihelion: 2475113.7779 +/-    8315.6
Perihelion:          32.33648703 +/-   26.2452
Aphelion:            78.40051780 +/-   41.5048
Period (y)              412.0049 +/-    278.22
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           39.69294483 +/-    0.3050
Ecliptic Y           24.71007140 +/-    0.1900
Ecliptic Z            2.28275691 +/-    0.0179
Ecliptic XDOT        -0.00199725 +/-    0.0009
Ecliptic YDOT         0.00132304 +/-    0.0004
Ecliptic ZDOT        -0.00124854 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.81162758 +/-    0.2774
Geocenter to KBO     45.81835098 +/-    0.3598
# Hcoef:  8.11

The following table shows the complete astrometric record for 11UX412. 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 (11UX412) followed by the observatory code and reference code for the source of the astrometry.

2011 10  24.43755  01 54 58.085  +14 49 26.88  24.3r 11UX412   568  C~1CKy      
2011 10  24.48029  01 54 57.904  +14 49 25.60  24.9r 11UX412   568  C~1CKy      
2011 10  24.52304  01 54 57.717  +14 49 24.26  24.7r 11UX412   568  C~1CKy      
2011 10  30.55955  01 54 31.992  +14 46 29.54  24.8r 11UX412   568  C~1CKy      
2011 10  31.54242  01 54 27.835  +14 46 00.81  24.5r 11UX412   568  C~1CKy      
2011 11  24.28350  01 52 53.984  +14 34 43.93  24.9r 11UX412   568  C~1CKy      
2011 11  30.32972  01 52 33.519  +14 32 04.37  24.7r 11UX412   568  C~1CKy      

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    -0.04       0.00     0.05
     2   0.0001     -2.91     0.01      -0.28    -0.01
     3   0.0002     -5.92    -0.05      -0.59    -0.10
     4   0.0168   -416.53     0.03     -33.93     0.11
     5   0.0195   -483.06     0.08     -39.76    -0.02
     6   0.0845  -1995.84    -0.08    -196.32    -0.10
     7   0.1010  -2330.12     0.05    -241.25     0.07

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.

11UX412    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