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: 11HZ102
# Created Wed Apr 24 01:13:43 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 91 observations of 91
# Arc: 6.23y
# First observation: 2011/04/28
# Last observation: 2017/07/21
# Chi-squared of fit: 47.82 DOF: 176 RMS: 0.13
# Min/Max residuals: -0.64 0.33
# Exact a, adot, b, bdot, g, gdot:
1.542593E-05 2.251254E-02 -1.454631E-06 -5.141592E-04 2.348727E-02 6.352242E-04
# Covariance matrix:
4.2125E-14 -2.9726E-14 -2.9840E-16 5.8315E-16 7.3689E-15 -2.1935E-13
-2.9726E-14 6.4170E-14 6.2574E-16 -1.4538E-15 2.5545E-14 5.1311E-13
-2.9840E-16 6.2574E-16 2.7360E-14 -6.1968E-15 9.1637E-17 5.4854E-15
5.8315E-16 -1.4538E-15 -6.1968E-15 3.3996E-15 -5.4906E-16 -1.2342E-14
7.3689E-15 2.5545E-14 9.1637E-17 -5.4906E-16 6.3412E-14 1.5249E-13
-2.1935E-13 5.1311E-13 5.4854E-15 -1.2342E-14 1.5249E-13 4.4054E-12
# lat0 lon0 xBary yBary zBary JD0
2.058492 -82.291730 0.877986 0.017903 -0.498743 2455679.747046
# Heliocentric elements and errors
Epoch: 2455680.5000 = 2011/04/29
Mean Anomaly: 61.26075 +/- 0.336
Argument of Peri: 59.88180 +/- 0.346
Long of Asc Node: 154.73941 +/- 0.003
Inclination: 2.39319 +/- 0.000
Eccentricity: 0.00638821 +/- 0.0001
Semi-Major Axis: 43.21578222 +/- 0.0018
Time of Perihelion: 2438022.4877 +/- 96.9
Perihelion: 42.93971086 +/- 0.0043
Aphelion: 43.49185357 +/- 0.0043
Period (y) 284.1004 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 4.90858931 +/- 0.0001
Ecliptic Y -42.77653390 +/- 0.0005
Ecliptic Z 1.52927520 +/- 0.0000
Ecliptic XDOT 0.00260884 +/- 0.0000
Ecliptic YDOT 0.00028247 +/- 0.0000
Ecliptic ZDOT -0.00005720 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 43.08438781 +/- 0.0004
Geocenter to KBO 42.57625714 +/- 0.0005
# Hcoef: 8.50
The following table shows the complete astrometric record for 11HZ102. 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 (11HZ102) followed by the observatory code and reference code for the source of the astrometry.
2011 04 28.24628 18 33 03.35 -21 09 35.8 11HZ102 268 C~0ljU 2011 04 28.24697 18 33 03.36 -21 09 35.9 11HZ102 268 C~0ljU 2011 04 28.34249 18 33 03.16 -21 09 35.8 11HZ102 268 C~0ljU 2011 04 28.34316 18 33 03.17 -21 09 35.9 11HZ102 268 C~0ljU 2011 04 28.41912 18 33 03.01 -21 09 35.8 11HZ102 268 C~0ljU 2011 04 28.41931 18 33 03.00 -21 09 35.8 11HZ102 268 C~0ljU 2011 04 30.32047 18 32 59.11 -21 09 34.6 11HZ102 268 C~0ljU 2011 04 30.32115 18 32 59.11 -21 09 34.7 11HZ102 268 C~0ljU 2011 04 30.41312 18 32 58.90 -21 09 34.5 11HZ102 268 C~0ljU 2011 05 01.31844 18 32 56.93 -21 09 34.3 11HZ102 268 C~0ljU 2011 05 03.28524 18 32 52.38 -21 09 33.3 11HZ102 268 C~0ljU 2011 05 03.29159 18 32 52.38 -21 09 33.4 11HZ102 268 C~0ljU 2011 05 03.32763 18 32 52.29 -21 09 33.4 11HZ102 268 C~0ljU 2011 05 03.36010 18 32 52.20 -21 09 33.4 11HZ102 268 C~0ljU 2011 05 03.36568 18 32 52.19 -21 09 33.3 11HZ102 268 C~0ljU 2011 05 27.25954 18 31 33.29 -21 09 52.5 11HZ102 268 C~0ljU 2011 05 27.26022 18 31 33.31 -21 09 52.4 11HZ102 268 C~0ljU 2011 05 27.30855 18 31 33.10 -21 09 52.6 11HZ102 268 C~0ljU 2011 05 27.30878 18 31 33.08 -21 09 52.6 11HZ102 268 C~0ljU 2011 05 27.35948 18 31 32.88 -21 09 52.6 11HZ102 268 C~0ljU 2011 05 27.35998 18 31 32.88 -21 09 52.5 11HZ102 268 C~0ljU 2011 05 28.31539 18 31 28.96 -21 09 54.5 11HZ102 268 C~0ljU 2011 05 28.31912 18 31 28.92 -21 09 54.6 25.4R 11HZ102 268 C~0ljU 2011 05 28.34773 18 31 28.82 -21 09 54.4 11HZ102 268 C~0ljU 2011 06 01.43469 18 31 11.48 -21 10 03.1 11HZ102 266 C~0ljU 2011 06 01.51361 18 31 11.12 -21 10 03.3 11HZ102 266 C~0ljU 2011 06 04.10625 18 30 59.69 -21 10 09.2 11HZ102 268 C~0ljU 2011 07 01.10007 18 28 49.07 -21 11 35.6 11HZ102 269 C~0ljU 2011 07 01.12040 18 28 48.94 -21 11 35.8 11HZ102 269 C~0ljU 2011 07 01.18502 18 28 48.64 -21 11 36.0 11HZ102 269 C~0ljU 2011 07 01.20571 18 28 48.50 -21 11 36.0 11HZ102 269 C~0ljU 2011 07 01.27016 18 28 48.21 -21 11 36.3 11HZ102 269 C~0ljU 2011 07 01.29082 18 28 48.07 -21 11 36.5 11HZ102 269 C~0ljU 2012 04 17.34023 18 38 48.54 -21 06 47.2 11HZ102 268 C~0ljU 2012 04 17.34199 18 38 48.54 -21 06 47.3 11HZ102 268 C~0ljU 2012 04 17.38698 18 38 48.49 -21 06 47.2 11HZ102 268 C~0ljU 2012 04 17.38720 18 38 48.49 -21 06 47.2 11HZ102 268 C~0ljU 2012 04 17.41592 18 38 48.46 -21 06 47.1 11HZ102 268 C~0ljU 2012 04 17.41654 18 38 48.46 -21 06 47.2 11HZ102 268 C~0ljU 2012 04 18.26734 18 38 47.68 -21 06 45.8 11HZ102 268 C~0ljU 2012 04 18.26755 18 38 47.67 -21 06 45.8 11HZ102 268 C~0ljU 2012 04 18.31485 18 38 47.63 -21 06 45.7 11HZ102 268 C~0ljU 2012 04 18.31552 18 38 47.62 -21 06 45.6 11HZ102 268 C~0ljU 2012 04 18.36209 18 38 47.57 -21 06 45.6 11HZ102 268 C~0ljU 2012 04 18.36265 18 38 47.57 -21 06 45.6 11HZ102 268 C~0ljU 2012 04 18.40528 18 38 47.53 -21 06 45.6 11HZ102 268 C~0ljU 2012 04 18.40586 18 38 47.52 -21 06 45.6 11HZ102 268 C~0ljU 2012 04 19.30535 18 38 46.60 -21 06 44.2 11HZ102 268 C~0ljU 2012 04 19.30696 18 38 46.60 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.31725 18 38 46.59 -21 06 44.2 11HZ102 268 C~0ljU 2012 04 19.33912 18 38 46.57 -21 06 44.2 11HZ102 268 C~0ljU 2012 04 19.35214 18 38 46.55 -21 06 44.2 11HZ102 268 C~0ljU 2012 04 19.36183 18 38 46.54 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.36529 18 38 46.54 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.39518 18 38 46.50 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.39905 18 38 46.49 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.40424 18 38 46.49 -21 06 44.1 11HZ102 268 C~0ljU 2012 04 19.41581 18 38 46.47 -21 06 44.0 11HZ102 268 C~0ljU 2012 09 17.71791 18 30 04.92 -21 15 07.7 25.2R 11HZ102 250 S~0sHu 2012 09 17.72638 18 30 04.92 -21 15 07.7 11HZ102 250 S~0sHu 2012 09 17.78014 18 30 04.91 -21 15 07.8 11HZ102 250 S~0sHu 2012 09 17.78861 18 30 04.91 -21 15 07.9 11HZ102 250 S~0sHu 2012 09 17.85075 18 30 04.89 -21 15 08.1 11HZ102 250 S~0sHu 2012 09 17.85921 18 30 04.89 -21 15 08.1 11HZ102 250 S~0sHv 2012 09 17.89891 18 30 04.88 -21 15 08.2 11HZ102 250 S~0sHv 2012 09 17.90738 18 30 04.88 -21 15 08.3 11HZ102 250 S~0sHv 2014 06 25.39941 18 46 01.126 -21 01 28.65 11HZ102 266 C~2Gt6 2014 06 25.45160 18 46 00.867 -21 01 28.91 11HZ102 266 C~2Gt6 2014 06 25.51748 18 46 00.531 -21 01 29.26 11HZ102 266 C~2Gt6 2014 06 25.54594 18 46 00.390 -21 01 29.38 11HZ102 266 C~2Gt6 2015 06 13.53486 18 52 33.14 -20 55 43.4 25.2r 11HZ102 568 C~1s2l 2015 06 13.53708 18 52 33.13 -20 55 43.4 25.6r 11HZ102 568 C~1s2l 2015 06 13.53928 18 52 33.12 -20 55 43.4 25.0r 11HZ102 568 C~1s2l 2015 06 13.58808 18 52 32.87 -20 55 43.7 25.6r 11HZ102 568 C~1s2l 2015 06 13.59038 18 52 32.84 -20 55 43.8 25.4r 11HZ102 568 C~1s2l 2015 06 13.59268 18 52 32.86 -20 55 43.5 25.5r 11HZ102 568 C~1s2l 2016 06 05.49974 18 58 38.559 -20 49 40.00 11HZ102 266 C~2Gt6 2016 06 05.52395 18 58 38.453 -20 49 40.11 11HZ102 266 C~2Gt6 2016 06 05.59476 18 58 38.143 -20 49 40.41 11HZ102 266 C~2Gt6 2017 07 20.25325 19 00 39.510 -20 48 49.72 24.5r 11HZ102 266 C~7ued 2017 07 20.27714 19 00 39.394 -20 48 49.97 24.3r 11HZ102 266 C~7ued 2017 07 20.39364 19 00 38.826 -20 48 50.87 24.5r 11HZ102 266 C~7ued 2017 07 20.41604 19 00 38.717 -20 48 51.10 24.3r 11HZ102 266 C~7ued 2017 07 20.53088 19 00 38.158 -20 48 51.95 24.5r 11HZ102 266 C~7ued 2017 07 20.55184 19 00 38.057 -20 48 52.16 24.3r 11HZ102 266 C~7ued 2017 07 21.24888 19 00 34.749 -20 48 57.67 24.2r 11HZ102 266 C~7ued 2017 07 21.26989 19 00 34.648 -20 48 57.77 24.2r 11HZ102 266 C~7ued 2017 07 21.39303 19 00 34.050 -20 48 58.78 24.2r 11HZ102 266 C~7ued 2017 07 21.40987 19 00 33.969 -20 48 58.99 24.2r 11HZ102 266 C~7ued 2017 07 21.50353 19 00 33.515 -20 48 59.72 24.2r 11HZ102 266 C~7ued 2017 07 21.52455 19 00 33.413 -20 48 59.81 24.2r 11HZ102 266 C~7ued
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 -0.07 0.00 0.23
2 0.0000 0.00 0.10 0.00 0.12
3 0.0003 0.00 0.01 0.00 0.17
4 0.0003 0.00 0.18 0.00 0.07
5 0.0005 0.00 0.11 0.00 0.11
6 0.0005 0.00 -0.03 0.00 0.11
7 0.0057 0.00 0.09 0.00 0.09
8 0.0057 0.00 0.11 0.00 -0.02
9 0.0059 0.00 0.03 0.00 0.13
10 0.0084 0.00 0.05 0.00 -0.12
11 0.0138 0.00 -0.09 0.00 0.15
12 0.0138 0.00 0.15 0.00 0.05
13 0.0139 0.00 0.13 0.00 0.04
14 0.0140 0.00 -0.01 0.00 0.03
15 0.0140 0.00 0.05 0.00 0.13
16 0.0794 0.00 -0.22 0.00 -0.10
17 0.0794 0.00 0.12 0.00 0.01
18 0.0796 0.00 -0.00 0.00 -0.11
19 0.0796 0.00 -0.29 0.00 -0.11
20 0.0797 0.00 -0.12 0.00 -0.02
21 0.0797 0.00 -0.09 0.00 0.08
22 0.0823 0.00 0.06 0.00 -0.15
23 0.0823 0.00 -0.30 0.00 -0.24
24 0.0824 0.00 0.01 0.00 0.01
25 0.0936 0.00 0.26 0.00 -0.17
26 0.0938 0.00 0.11 0.00 -0.19
27 0.1009 0.00 0.12 0.00 -0.31
28 0.1748 0.00 0.06 0.00 -0.07
29 0.1749 0.00 -0.34 0.00 -0.19
30 0.1751 0.00 0.08 0.00 -0.13
31 0.1751 0.00 -0.44 0.00 -0.05
32 0.1753 0.00 0.12 0.00 -0.10
33 0.1753 0.00 -0.40 0.00 -0.23
34 0.9722 0.00 0.10 0.00 0.09
35 0.9722 0.00 0.12 0.00 -0.02
36 0.9723 0.00 0.03 0.00 0.01
37 0.9723 0.00 0.03 0.00 0.01
38 0.9724 0.00 0.00 0.00 0.07
39 0.9724 0.00 0.01 0.00 -0.04
40 0.9747 0.00 0.11 0.00 -0.02
41 0.9747 0.00 -0.04 0.00 -0.02
42 0.9749 0.00 0.10 0.00 0.02
43 0.9749 0.00 -0.04 0.00 0.12
44 0.9750 0.00 -0.05 0.00 0.06
45 0.9750 0.00 -0.04 0.00 0.06
46 0.9751 0.00 0.05 0.00 -0.01
47 0.9751 0.00 -0.09 0.00 -0.01
48 0.9776 0.00 -0.04 0.00 0.04
49 0.9776 0.00 -0.02 0.00 0.14
50 0.9776 0.00 0.01 0.00 0.03
51 0.9777 0.00 0.09 0.00 -0.00
52 0.9777 0.00 0.01 0.00 -0.02
53 0.9777 0.00 0.03 0.00 0.07
54 0.9777 0.00 0.09 0.00 0.06
55 0.9778 0.00 0.02 0.00 0.02
56 0.9778 0.00 -0.07 0.00 0.02
57 0.9778 0.00 0.03 0.00 0.01
58 0.9779 0.00 -0.07 0.00 0.09
59 1.3921 0.00 0.10 0.00 -0.13
60 1.3921 0.00 0.12 0.00 -0.11
61 1.3923 0.00 0.15 0.00 -0.03
62 1.3923 0.00 0.17 0.00 -0.10
63 1.3925 0.00 0.07 0.00 -0.10
64 1.3925 0.00 0.09 0.00 -0.07
65 1.3926 0.00 0.06 0.00 -0.04
66 1.3926 0.00 0.09 0.00 -0.12
67 3.1599 0.00 0.02 0.00 0.05
68 3.1600 0.00 0.07 0.00 0.08
69 3.1602 0.00 0.00 0.00 0.08
70 3.1603 0.00 0.03 0.00 0.11
71 4.1267 0.00 -0.05 0.00 -0.06
72 4.1267 0.00 -0.04 0.00 -0.05
73 4.1267 0.00 -0.04 0.00 -0.04
74 4.1269 0.00 -0.35 0.00 -0.10
75 4.1269 0.00 -0.64 0.00 -0.19
76 4.1269 0.00 -0.18 0.00 0.13
77 5.1068 0.00 0.33 0.00 0.09
78 5.1069 0.00 0.31 0.00 0.10
79 5.1070 0.00 0.25 0.00 0.15
80 6.2286 0.00 -0.02 0.00 -0.05
81 6.2287 0.00 -0.02 0.00 -0.10
82 6.2290 0.00 -0.02 0.00 -0.05
83 6.2291 0.00 -0.02 0.00 -0.10
84 6.2294 0.00 -0.02 0.00 -0.05
85 6.2294 0.00 -0.01 0.00 -0.10
86 6.2314 0.00 0.00 0.00 -0.01
87 6.2314 0.00 0.01 0.00 0.06
88 6.2318 0.00 -0.00 0.00 0.06
89 6.2318 0.00 0.01 0.00 -0.02
90 6.2321 0.00 0.01 0.00 -0.01
91 6.2321 0.00 -0.00 0.00 0.06
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.
11HZ102 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.037 43.037 43.037 ecceobj 0.005 0.005 0.005 incobj 2.394 2.394 2.394 qmin 41.994 41.993 41.996 qmax 44.618 44.618 44.619 amean 43.253 43.253 43.253 amin 42.925 42.924 42.925 amax 43.585 43.584 43.586 emean 0.011 0.011 0.011 emin 0.000 0.000 0.000 emax 0.024 0.024 0.024 imean 2.615 2.615 2.615 imin 1.740 1.740 1.740 imax 3.328 3.328 3.328 excite_mean 0.047 0.047 0.047 fracstop 1.000 1.000 1.000 cjmean 3.090 3.090 3.090 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 177.5 177.4 177.5 kozaiamp 180.0 180.0 180.0