Orbit Fit and Astrometric record for 11HD103

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: 11HD103   
# Created Sat Apr 27 01:13:46 2024
# Orbit generated from Bernstein formalism
# Fitting     24 observations of     24
# Arc:   0.98y
# First observation: 2011/04/28
#  Last observation: 2012/04/20
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.014643  -0.000000  -0.001341   0.019177   0.000000
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# Chi-squared of fit:     2.66 DOF:     43 RMS:  0.06
# Min/Max residuals:    -0.15    0.13
# Exact a, adot, b, bdot, g, gdot:
  1.228171E-05  1.455260E-02 -1.169510E-06 -1.333129E-03  1.912810E-02 -7.927484E-03
# Covariance matrix:
  2.3103E-13  1.3503E-11 -8.9113E-15 -1.2480E-12  1.0067E-11  9.2882E-10
  1.3503E-11  1.7569E-08  1.8717E-12 -1.6090E-09  5.6233E-09  1.1648E-06
 -8.9113E-15  1.8717E-12  7.1831E-14 -2.4723E-13  2.0308E-13  1.2212E-10
 -1.2480E-12 -1.6090E-09 -2.4723E-13  1.4795E-10 -5.1518E-10 -1.0668E-07
  1.0067E-11  5.6233E-09  2.0308E-13 -5.1518E-10  2.0186E-09  3.7392E-07
  9.2882E-10  1.1648E-06  1.2212E-10 -1.0668E-07  3.7392E-07  7.7235E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.389595  -82.230223    0.878522    0.020745   -0.497689  2455679.747046
# Heliocentric elements and errors
Epoch:              2455670.5000  =  2011/04/19
Mean Anomaly:          299.60946 +/-    57.640
Argument of Peri:      274.07021 +/-    22.587
Long of Asc Node:      121.01750 +/-     0.274
Inclination:             5.75784 +/-     0.061
Eccentricity:         0.49349638 +/-    0.4155
Semi-Major Axis:     53.41275643 +/-   27.3843
Time of Perihelion: 2479588.9103 +/-   13521.1
Perihelion:          27.05375468 +/-   26.1718
Aphelion:            79.77175818 +/-   46.5323
Period (y)              390.3693 +/-    300.21
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            6.26316096 +/-    0.0166
Ecliptic Y          -52.36633984 +/-    0.1216
Ecliptic Z            2.17968403 +/-    0.0051
Ecliptic XDOT         0.00190974 +/-    0.0002
Ecliptic YDOT         0.00140294 +/-    0.0012
Ecliptic ZDOT        -0.00023793 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   52.78457877 +/-    0.1206
Geocenter to KBO     52.27910772 +/-    0.1228
# Hcoef:  8.35

The following table shows the complete astrometric record for 11HD103. 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 (11HD103) followed by the observatory code and reference code for the source of the astrometry.

2011 04  28.24628  18 33 14.24   -20 49 33.1         11HD103   268  C~0pNK      
2011 04  28.24697  18 33 14.25   -20 49 33.1         11HD103   268  C~0pNK      
2011 04  28.34249  18 33 14.06   -20 49 33.1         11HD103   268  C~0pNK      
2011 04  28.34316  18 33 14.07   -20 49 33.2         11HD103   268  C~0pNK      
2011 04  28.41912  18 33 13.94   -20 49 33.1         11HD103   268  C~0pNK      
2011 04  28.41931  18 33 13.93   -20 49 33.0         11HD103   268  C~0pNK      
2011 04  30.32115  18 33 10.49   -20 49 32.6         11HD103   268  C~0pNK      
2011 04  30.41312  18 33 10.30   -20 49 32.7         11HD103   268  C~0pNK      
2011 05  01.31844  18 33 08.57   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  02.28342  18 33 06.65   -20 49 32.5         11HD103   268  C~0pNK      
2011 05  02.28856  18 33 06.64   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  02.30851  18 33 06.60   -20 49 32.5         11HD103   268  C~0pNK      
2011 05  02.32221  18 33 06.58   -20 49 32.5         11HD103   268  C~0pNK      
2011 05  02.33338  18 33 06.54   -20 49 32.4         11HD103   268  C~0pNK      
2011 05  02.35124  18 33 06.51   -20 49 32.5         11HD103   268  C~0pNK      
2011 05  03.28524  18 33 04.59   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  03.29159  18 33 04.58   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  03.30873  18 33 04.54   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  03.32834  18 33 04.50   -20 49 32.6         11HD103   268  C~0pNK      
2011 05  03.34419  18 33 04.46   -20 49 32.6   25.3R 11HD103   268  C~0pNK      
2011 05  03.36010  18 33 04.43   -20 49 32.5         11HD103   268  C~0pNK      
2012 04  20.32108  18 37 00.79   -20 51 10.4         11HD103   268  C~0pNK      
2012 04  20.36290  18 37 00.74   -20 51 10.3         11HD103   268  C~0pNK      
2012 04  20.40652  18 37 00.69   -20 51 10.2         11HD103   268  C~0pNK      

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    -0.05       0.00     0.01
     2   0.0000      0.14     0.11      -0.01     0.00
     3   0.0003     -2.52    -0.15       0.15     0.00
     4   0.0003     -2.39    -0.00       0.04    -0.10
     5   0.0005     -4.20     0.11       0.24    -0.04
     6   0.0005     -4.33    -0.02       0.35     0.07
     7   0.0057    -52.46     0.09       3.52     0.05
     8   0.0059    -55.12    -0.06       3.57    -0.06
     9   0.0084    -79.33     0.01       5.07    -0.05
    10   0.0111   -106.20    -0.03       6.71     0.02
    11   0.0111   -106.35    -0.02       6.62    -0.08
    12   0.0111   -106.90     0.00       6.75     0.02
    13   0.0112   -107.18     0.12       6.77     0.02
    14   0.0112   -107.74    -0.10       6.90     0.13
    15   0.0112   -108.16    -0.01       6.82     0.03
    16   0.0138   -135.04    -0.01       8.27    -0.03
    17   0.0138   -135.18     0.04       8.27    -0.03
    18   0.0139   -135.74    -0.00       8.31    -0.02
    19   0.0139   -136.30     0.03       8.34    -0.02
    20   0.0140   -136.86    -0.05       8.37    -0.01
    21   0.0140   -137.27     0.02       8.49     0.09
    22   0.9804   3164.49    -0.02    -289.16    -0.07
    23   0.9805   3163.80    -0.01    -289.02     0.00
    24   0.9806   3163.11     0.03    -288.88     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.

11HD103    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