Orbit Fit and Astrometric record for 11UK413

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: 11UK413   
# Created Sun Dec 22 02:09:19 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     49 observations of     49
# Arc:  21.00y
# First observation: 2003/11/24
#  Last observation: 2024/11/24
# Chi-squared of fit:    55.11 DOF:     92 RMS:  0.19
# Min/Max residuals:    -0.72    0.59
# Exact a, adot, b, bdot, g, gdot:
  1.644930E-05  2.444592E-02 -4.914732E-06 -5.756043E-03  2.525291E-02  2.191827E-03
# Covariance matrix:
  5.9127E-13 -9.2079E-14 -7.8518E-14  1.6104E-14 -9.1697E-14 -1.2464E-13
 -9.2079E-14  1.6508E-14  1.5978E-14 -3.2771E-15  1.8258E-14  2.5365E-14
 -7.8518E-14  1.5978E-14  2.6231E-13 -2.5239E-14  1.6802E-14  2.8488E-14
  1.6104E-14 -3.2771E-15 -2.5239E-14  2.9250E-15 -3.4324E-15 -5.8438E-15
 -9.1697E-14  1.8258E-14  1.6802E-14 -3.4324E-15  1.1895E-13  2.6337E-14
 -1.2464E-13  2.5365E-14  2.8488E-14 -5.8438E-15  2.6337E-14  4.5246E-14
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.344425   62.942040    0.029114    0.057566   -0.984183  2452967.769583
# Heliocentric elements and errors
Epoch:              2452968.5000  =  2003/11/25
Mean Anomaly:           68.70642 +/-     0.020
Argument of Peri:       87.61904 +/-     0.024
Long of Asc Node:      256.52491 +/-     0.000
Inclination:            13.61205 +/-     0.000
Eccentricity:         0.08750473 +/-    0.0000
Semi-Major Axis:     41.61853834 +/-    0.0022
Time of Perihelion: 2434252.0510 +/-       5.5
Perihelion:          37.97671920 +/-    0.0021
Aphelion:            45.26035747 +/-    0.0024
Period (y)              268.4964 +/-      0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           18.45330798 +/-    0.0002
Ecliptic Y           36.07315733 +/-    0.0005
Ecliptic Z            2.30996100 +/-    0.0000
Ecliptic XDOT        -0.00224027 +/-    0.0000
Ecliptic YDOT         0.00144314 +/-    0.0000
Ecliptic ZDOT        -0.00060897 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.58483620 +/-    0.0004
Geocenter to KBO     39.59938768 +/-    0.0005
# Hcoef:  6.48

The following table shows the complete astrometric record for 11UK413. 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 (11UK413) followed by the observatory code and reference code for the source of the astrometry.

2003 11  24.26884  04 00 44.49   +24 01 35.6   21.6R 11UK413   695  C~1w3o      
2003 11  24.34422  04 00 44.10   +24 01 33.9         11UK413   695  C~1w3o      
2010 10  11.48971  04 47 01.143  +23 27 08.98  23.9G 11UK413   F51  C~345i      
2010 11  07.55785  04 45 18.606  +23 23 10.22  21.8G 11UK413   F51  C~345i      
2010 11  09.54329  04 45 09.186  +23 22 48.91  22.7w 11UK413   F51  C~1w3o      
2010 11  09.56142  04 45 09.089  +23 22 48.67  22.6w 11UK413   F51  C~1w3o      
2010 11  09.57966  04 45 09.021  +23 22 48.49  22.4w 11UK413   F51  C~1w3o      
2010 11  09.59782  04 45 08.930  +23 22 48.30  22.5w 11UK413   F51  C~1w3o      
2010 11  16.53919  04 44 34.423  +23 21 28.19  22.4G 11UK413   F51  C~345i      
2010 11  16.55074  04 44 34.364  +23 21 28.69  22.4i 11UK413   F51  C~1w3o      
2011 10  25.42693  04 52 15.700  +23 15 42.94  22.5w 11UK413   F51  C~1w3o      
2011 10  25.44144  04 52 15.648  +23 15 42.87  22.9w 11UK413   F51  C~1w3o      
2011 10  25.45588  04 52 15.605  +23 15 42.76  22.5w 11UK413   F51  C~1w3o      
2011 10  25.47033  04 52 15.535  +23 15 42.58  22.8w 11UK413   F51  C~1w3o      
2011 11  24.55209  04 49 55.644  +23 10 31.59  22.5r 11UK413   F51  C~1w3o      
2011 11  24.56387  04 49 55.573  +23 10 31.39  21.9r 11UK413   F51  C~1w3o      
2011 11  30.31306  04 49 24.780  +23 09 21.93  22.0i 11UK413   F51  C~1w3o      
2011 11  30.32565  04 49 24.705  +23 09 21.99  22.2i 11UK413   F51  C~1w3o      
2012 10  11.60692  04 58 53.141  +23 06 50.50  22.9G 11UK413   F51  C~345i      
2012 10  11.62097  04 58 53.097  +23 06 50.97  22.6G 11UK413   F51  C~345i      
2012 11  06.58702  04 57 20.163  +23 03 21.39  22.8G 11UK413   F51  C~345i      
2012 11  06.60051  04 57 20.111  +23 03 21.87  22.2G 11UK413   F51  C~345i      
2013 11  27.36249  05 01 34.964  +22 48 49.88  22.3w 11UK413   F51  C~1w3o      
2013 11  27.37773  05 01 34.895  +22 48 49.80  22.1w 11UK413   F51  C~1w3o      
2013 11  27.39294  05 01 34.805  +22 48 49.43  22.2w 11UK413   F51  C~1w3o      
2013 11  27.40829  05 01 34.730  +22 48 49.47  22.0w 11UK413   F51  C~1w3o      
2013 12  25.29191  04 59 05.579  +22 43 47.20  22.9G 11UK413   F51  C~345i      
2013 12  25.30506  04 59 05.546  +22 43 47.17  22.2G 11UK413   F51  C~345i      
2013 12  25.31829  04 59 05.489  +22 43 46.84  23.2G 11UK413   F51  C~345i      
2014 02  26.24589  04 56 00.690  +22 35 51.46  23.2G 11UK413   F51  C~345i      
2015 01  18.23213  05 03 11.183  +22 28 51.92  22.2G 11UK413   F51  C~345i      
2015 01  18.24608  05 03 11.143  +22 28 51.73  21.9G 11UK413   F51  C~345i      
2015 01  18.26002  05 03 11.074  +22 28 51.31  22.6G 11UK413   F51  C~345i      
2015 01  18.27400  05 03 11.003  +22 28 51.35  22.9G 11UK413   F51  C~345i      
2015 01  20.22615  05 03 03.631  +22 28 35.89  21.9G 11UK413   F51  C~345i      
2015 01  20.23971  05 03 03.561  +22 28 35.80  22.3G 11UK413   F51  C~345i      
2015 01  20.25328  05 03 03.529  +22 28 35.53  22.3G 11UK413   F51  C~345i      
2015 01  20.26680  05 03 03.460  +22 28 35.40  22.6G 11UK413   F51  C~345i      
2016 01  14.39821  05 09 18.049  +22 17 35.51  22.8G 11UK413   F51  C~345i      
2016 01  14.41220  05 09 17.995  +22 17 35.30  23.0G 11UK413   F51  C~345i      
2016 01  14.42609  05 09 17.930  +22 17 35.33  22.8G 11UK413   F51  C~345i      
2016 01  14.43998  05 09 17.880  +22 17 34.87  22.4G 11UK413   F51  C~345i      
2016 11  03.62098  05 20 58.361  +22 14 43.75  22.7G 11UK413   F51  C~345i      
2016 11  03.62747  05 20 58.353  +22 14 43.55  23.3G 11UK413   F51  C~345i      
2016 11  03.63394  05 20 58.297  +22 14 43.60  22.8G 11UK413   F51  C~345i      
2016 11  03.64041  05 20 58.268  +22 14 43.30  23.6G 11UK413   F51  C~345i      
2017 09  01.59519  05 27 41.134  +22 06 19.76  23.2G 11UK413   F51  C~345i      
2024 11  24.439040 06 04 11.757  +20 02 39.27  22.7G 11UK413   G37  C~8SMZ      
2024 11  24.489050 06 04 11.532  +20 02 39.08        11UK413   G37  C~8SMZ      

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    -0.31       0.00     0.22
     2   0.0002      0.00     0.11       0.00    -0.10
     3   6.8808      0.00    -0.01       0.00     0.16
     4   6.9549      0.00    -0.29       0.00    -0.41
     5   6.9604      0.00     0.16       0.00     0.03
     6   6.9604      0.00     0.04       0.00    -0.01
     7   6.9605      0.00     0.36       0.00     0.02
     8   6.9605      0.00     0.33       0.00     0.03
     9   6.9795      0.00     0.19       0.00    -0.31
    10   6.9796      0.00     0.21       0.00     0.33
    11   7.9183      0.00    -0.20       0.00    -0.04
    12   7.9183      0.00    -0.15       0.00     0.01
    13   7.9184      0.00     0.03       0.00     0.02
    14   7.9184      0.00    -0.19       0.00    -0.04
    15   8.0008      0.00     0.13       0.00     0.11
    16   8.0008      0.00     0.02       0.00     0.06
    17   8.0165      0.00     0.15       0.00    -0.25
    18   8.0166      0.00     0.06       0.00    -0.04
    19   8.8825      0.00    -0.03       0.00    -0.14
    20   8.8826      0.00    -0.14       0.00     0.42
    21   8.9536      0.00     0.08       0.00    -0.02
    22   8.9537      0.00     0.23       0.00     0.59
    23  10.0098      0.00    -0.20       0.00     0.00
    24  10.0099      0.00    -0.00       0.00     0.08
    25  10.0099      0.00    -0.12       0.00    -0.13
    26  10.0100      0.00    -0.01       0.00     0.06
    27  10.0863      0.00    -0.72       0.00    -0.23
    28  10.0863      0.00    -0.19       0.00    -0.12
    29  10.0864      0.00    -0.01       0.00    -0.31
    30  10.2587      0.00     0.11       0.00     0.04
    31  11.1512      0.00    -0.03       0.00     0.15
    32  11.1512      0.00     0.19       0.00     0.07
    33  11.1512      0.00    -0.01       0.00    -0.24
    34  11.1513      0.00    -0.25       0.00    -0.09
    35  11.1566      0.00     0.21       0.00     0.12
    36  11.1567      0.00    -0.07       0.00     0.13
    37  11.1567      0.00     0.23       0.00    -0.03
    38  11.1567      0.00    -0.04       0.00    -0.06
    39  12.1400      0.00    -0.02       0.00     0.08
    40  12.1400      0.00     0.08       0.00    -0.02
    41  12.1401      0.00     0.00       0.00     0.12
    42  12.1401      0.00     0.15       0.00    -0.23
    43  12.9455      0.00    -0.08       0.00     0.06
    44  12.9455      0.00     0.19       0.00    -0.09
    45  12.9456      0.00    -0.25       0.00     0.01
    46  12.9456      0.00    -0.30       0.00    -0.24
    47  13.7723      0.00     0.03       0.00     0.01
    48  21.0025      0.00     0.05       0.00     0.07
    49  21.0027      0.00     0.12       0.00     0.13

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.

11UK413    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        41.897    41.898    41.897
ecceobj         0.093     0.093     0.093
incobj         13.594    13.594    13.594
qmin           37.265    37.278    37.237
qmax           46.156    46.173    46.238
amean          41.618    41.618    41.618
amin           41.270    41.277    41.272
amax           41.970    41.984    41.978
emean           0.089     0.088     0.090
emin            0.077     0.076     0.078
emax            0.101     0.101     0.102
imean          15.432    15.435    15.425
imin           14.640    14.638    14.615
imax           16.205    16.204    16.204
excite_mean     0.281     0.280     0.281
fracstop        1.000     1.000     1.000
cjmean          2.981     2.981     2.981

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       177.8     178.0     177.9
kozaiamp        180.0     180.0     180.0