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: 11UE411
# Created Fri Apr 19 01:13:51 2024
# Orbit generated from Bernstein formalism
# Fitting 14 observations of 14
# Arc: 1.38y
# First observation: 2011/08/29
# Last observation: 2013/01/14
Preliminary a, adot, b, bdot, g, gdot:
-0.000134 0.031358 0.000002 0.004942 0.027839 0.000000
# Chi-squared of fit: 6.01 DOF: 22 RMS: 0.12
# Min/Max residuals: -0.27 0.28
# Exact a, adot, b, bdot, g, gdot:
1.785026E-05 3.097357E-02 2.783563E-06 4.873121E-03 2.775670E-02 -6.537990E-03
# Covariance matrix:
6.2847E-13 3.9469E-13 -3.5365E-14 2.1083E-13 7.8075E-13 3.0669E-11
3.9469E-13 1.8005E-12 -8.5915E-14 5.6134E-13 1.3685E-12 8.1857E-11
-3.5365E-14 -8.5915E-14 2.0592E-13 -2.4473E-13 -8.3676E-14 -5.2940E-12
2.1083E-13 5.6134E-13 -2.4473E-13 6.8753E-13 5.2495E-13 3.5320E-11
7.8075E-13 1.3685E-12 -8.3676E-14 5.2495E-13 1.5667E-12 7.6471E-11
3.0669E-11 8.1857E-11 -5.2940E-12 3.5320E-11 7.6471E-11 5.1532E-09
# lat0 lon0 xBary yBary zBary JD0
2.467496 33.366806 0.851707 0.023098 -0.536619 2455803.072836
# Heliocentric elements and errors
Epoch: 2455800.5000 = 2011/08/27
Mean Anomaly: 329.91827 +/- 0.105
Argument of Peri: 72.47501 +/- 0.270
Long of Asc Node: 17.07099 +/- 0.002
Inclination: 9.33812 +/- 0.001
Eccentricity: 0.32419191 +/- 0.0022
Semi-Major Axis: 48.02704400 +/- 0.0764
Time of Perihelion: 2465958.9530 +/- 25.9
Perihelion: 32.45706490 +/- 0.1190
Aphelion: 63.59702310 +/- 0.1474
Period (y) 332.8411 +/- 0.79
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 30.98129951 +/- 0.0014
Ecliptic Y 19.38188920 +/- 0.0009
Ecliptic Z 1.55118959 +/- 0.0001
Ecliptic XDOT -0.00223885 +/- 0.0000
Ecliptic YDOT 0.00219123 +/- 0.0000
Ecliptic ZDOT 0.00045252 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 36.57738014 +/- 0.0012
Geocenter to KBO 36.02734220 +/- 0.0016
# Hcoef: 9.32
The following table shows the complete astrometric record for 11UE411. 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 (11UE411) followed by the observatory code and reference code for the source of the astrometry.
2011 08 29.57207 02 01 05.114 +14 57 20.79 25.4r 11UE411 568 C~1C6N 2011 08 29.61903 02 01 04.998 +14 57 20.50 24.7r 11UE411 568 C~1C6N 2011 10 24.43755 01 57 01.267 +14 40 23.70 11UE411 568 C~1C6N 2011 10 24.48029 01 57 01.019 +14 40 22.40 24.5r 11UE411 568 C~1C6N 2011 10 24.52304 01 57 00.789 +14 40 21.29 24.6r 11UE411 568 C~1C6N 2011 10 30.55955 01 56 28.136 +14 37 42.79 24.9r 11UE411 568 C~1C6N 2011 10 31.54242 01 56 22.865 +14 37 16.83 11UE411 568 C~1C6N 2011 11 24.28350 01 54 23.729 +14 27 08.93 25.1r 11UE411 568 C~1C6N 2011 11 30.32972 01 53 57.750 +14 24 49.97 24.8r 11UE411 568 C~1C6N 2012 01 27.32916 01 52 37.585 +14 16 26.41 24.4r 11UE411 568 C~1C6N 2012 10 21.32322 02 03 51.741 +15 34 52.74 24.5r 11UE411 568 C~1C6N 2012 10 21.34894 02 03 51.597 +15 34 52.00 24.8r 11UE411 568 C~1C6N 2012 10 21.37460 02 03 51.456 +15 34 51.48 25.3r 11UE411 568 C~1C6N 2013 01 14.34100 01 58 49.861 +15 08 16.37 25.3r 11UE411 568 C~1C6N
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 -0.00
2 0.0001 -1.68 0.03 0.31 -0.01
3 0.1530 -3670.01 0.22 269.23 0.00
4 0.1531 -3673.83 -0.01 269.26 -0.11
5 0.1532 -3677.35 0.06 269.38 -0.12
6 0.1697 -4176.93 -0.27 285.92 0.03
7 0.1724 -4257.72 -0.09 288.27 -0.02
8 0.2374 -6092.08 0.26 323.90 0.11
9 0.2540 -6494.60 -0.10 326.27 -0.12
10 0.4128 -7763.80 -0.05 264.90 0.28
11 1.1465 3036.71 0.02 1290.45 0.05
12 1.1465 3034.50 -0.04 1290.46 -0.04
13 1.1466 3032.41 0.02 1290.67 0.07
14 1.3792 -1612.75 0.00 1291.40 -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.
11UE411 quality flag:3 Type: 2:1E 2:1E 2:1E axisobj 48.143 48.340 47.954 ecceobj 0.325 0.330 0.319 incobj 9.328 9.328 9.329 qmin 31.706 31.424 32.030 qmax 64.597 64.837 64.689 amean 47.797 47.797 47.796 amin 47.245 47.279 47.071 amax 48.472 48.451 48.648 emean 0.311 0.319 0.316 emin 0.287 0.294 0.299 emax 0.335 0.340 0.332 imean 10.274 9.873 9.253 imin 8.778 8.518 8.954 imax 11.753 11.263 9.540 excite_mean 0.359 0.363 0.354 fracstop 1.000 1.000 1.000 cjmean 2.986 2.982 2.990 libcent 0 74.1 71.7 179.4 libamp 0 28.6 22.4 155.7 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 170.0 160.7 180.7 kozaiamp 180.0 180.0 179.9