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: 11HJ103
# Created Wed Dec 4 02:09:09 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 42 observations of 42
# Arc: 6.23y
# First observation: 2011/04/28
# Last observation: 2017/07/21
# Chi-squared of fit: 23.59 DOF: 78 RMS: 0.13
# Min/Max residuals: -0.44 0.28
# Exact a, adot, b, bdot, g, gdot:
1.576072E-05 2.597561E-02 -1.469502E-06 -2.123875E-03 2.493362E-02 -1.760505E-03
# Covariance matrix:
1.5468E-13 -1.0835E-14 -3.4859E-15 9.0738E-16 1.7726E-13 -6.9716E-14
-1.0835E-14 9.3970E-14 1.4318E-15 -7.8188E-15 6.0554E-14 6.3174E-13
-3.4859E-15 1.4318E-15 6.3986E-14 -1.2475E-14 -5.8358E-15 1.3269E-14
9.0738E-16 -7.8188E-15 -1.2475E-14 5.7278E-15 -3.3109E-15 -5.6451E-14
1.7726E-13 6.0554E-14 -5.8358E-15 -3.3109E-15 3.8327E-13 2.7450E-13
-6.9716E-14 6.3174E-13 1.3269E-14 -5.6451E-14 2.7450E-13 4.5580E-12
# lat0 lon0 xBary yBary zBary JD0
2.702638 -82.325212 0.877510 0.023547 -0.499352 2455679.768846
# Heliocentric elements and errors
Epoch: 2455680.5000 = 2011/04/29
Mean Anomaly: 330.16786 +/- 0.023
Argument of Peri: 190.50421 +/- 0.033
Long of Asc Node: 126.37679 +/- 0.001
Inclination: 5.33624 +/- 0.000
Eccentricity: 0.15709878 +/- 0.0001
Semi-Major Axis: 46.61474848 +/- 0.0054
Time of Perihelion: 2465313.5840 +/- 19.8
Perihelion: 39.29162844 +/- 0.0059
Aphelion: 53.93786852 +/- 0.0073
Period (y) 318.2682 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 4.55202501 +/- 0.0001
Ecliptic Y -40.31554738 +/- 0.0010
Ecliptic Z 1.89107062 +/- 0.0000
Ecliptic XDOT 0.00280050 +/- 0.0000
Ecliptic YDOT 0.00056733 +/- 0.0000
Ecliptic ZDOT -0.00024204 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.61582606 +/- 0.0010
Geocenter to KBO 40.10655993 +/- 0.0010
# Hcoef: 7.98
The following table shows the complete astrometric record for 11HJ103. 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 (11HJ103) followed by the observatory code and reference code for the source of the astrometry.
2011 04 28.26808 18 32 45.35 -20 31 07.5 11HJ103 268 C~113n 2011 04 28.36805 18 32 45.14 -20 31 07.4 11HJ103 268 C~113n 2011 04 30.39635 18 32 40.89 -20 31 06.0 11HJ103 268 C~113n 2011 05 06.36820 18 32 26.23 -20 31 04.2 11HJ103 268 C~113n 2011 05 29.48014 18 31 02.93 -20 31 32.8 11HJ103 266 C~113n 2011 05 29.56900 18 31 02.55 -20 31 33.1 11HJ103 266 C~113n 2011 05 30.48977 18 30 58.50 -20 31 35.7 11HJ103 266 C~113n 2011 05 30.52326 18 30 58.35 -20 31 35.7 11HJ103 266 C~113n 2011 05 31.48809 18 30 54.08 -20 31 38.0 11HJ103 266 C~113n 2011 05 31.52730 18 30 53.90 -20 31 38.2 11HJ103 266 C~113n 2011 05 31.56672 18 30 53.74 -20 31 38.1 11HJ103 266 C~113n 2011 06 01.53319 18 30 49.38 -20 31 40.8 11HJ103 266 C~113n 2011 06 01.59657 18 30 49.09 -20 31 41.1 11HJ103 266 C~113n 2011 06 04.29530 18 30 36.70 -20 31 48.7 11HJ103 268 C~113n 2011 06 04.39266 18 30 36.23 -20 31 48.8 11HJ103 268 C~113n 2011 07 02.03941 18 28 16.77 -20 33 40.9 11HJ103 269 C~113n 2011 07 02.14714 18 28 16.20 -20 33 41.3 11HJ103 269 C~113n 2011 07 02.25740 18 28 15.62 -20 33 41.8 11HJ103 269 C~113n 2011 07 02.28855 18 28 15.48 -20 33 42.2 11HJ103 266 C~113n 2011 07 02.35039 18 28 15.15 -20 33 42.6 25.0R 11HJ103 266 C~113n 2011 07 02.41278 18 28 14.82 -20 33 42.7 11HJ103 266 C~113n 2011 07 02.53920 18 28 14.16 -20 33 43.5 11HJ103 266 C~113n 2014 06 25.35303 18 48 18.321 -20 37 32.17 11HJ103 266 C~2Gt6 2014 06 25.39002 18 48 18.124 -20 37 32.36 11HJ103 266 C~2Gt6 2014 06 25.43230 18 48 17.902 -20 37 32.67 11HJ103 266 C~2Gt6 2014 06 25.51192 18 48 17.481 -20 37 33.21 11HJ103 266 C~2Gt6 2014 06 25.54572 18 48 17.304 -20 37 33.42 11HJ103 266 C~2Gt6 2014 06 27.35764 18 48 07.923 -20 37 45.91 11HJ103 266 C~2Gt6 2014 06 27.37087 18 48 07.862 -20 37 46.05 11HJ103 266 C~2Gt6 2016 06 05.46715 19 02 58.844 -20 33 28.63 11HJ103 266 C~2Gt6 2016 06 05.51228 19 02 58.645 -20 33 29.00 11HJ103 266 C~2Gt6 2016 06 05.53621 19 02 58.537 -20 33 28.99 11HJ103 266 C~2Gt6 2016 06 05.53960 19 02 58.515 -20 33 29.05 11HJ103 266 C~2Gt6 2017 05 20.49661 19 10 34.945 -20 29 26.85 23.2r 11HJ103 568 C~2cbA 2017 06 22.46305 19 08 15.494 -20 33 13.57 11HJ103 568 C~2cbA 2017 06 23.46091 19 08 10.473 -20 33 22.35 23.6r 11HJ103 568 C~2cbA 2017 07 20.27714 19 05 51.824 -20 37 41.68 23.9r 11HJ103 266 C~7ued 2017 07 20.41604 19 05 51.106 -20 37 43.10 23.9r 11HJ103 266 C~7ued 2017 07 20.55184 19 05 50.406 -20 37 44.44 23.9r 11HJ103 266 C~7ued 2017 07 21.26989 19 05 46.782 -20 37 51.70 23.8r 11HJ103 266 C~7ued 2017 07 21.38744 19 05 46.178 -20 37 52.91 23.8r 11HJ103 266 C~7ued 2017 07 21.48258 19 05 45.688 -20 37 53.86 23.8r 11HJ103 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 0.16 0.00 0.03
2 0.0003 0.00 0.11 0.00 0.06
3 0.0058 0.00 0.07 0.00 -0.01
4 0.0222 0.00 0.28 0.00 0.04
5 0.0855 0.00 -0.44 0.00 0.19
6 0.0857 0.00 -0.19 0.00 0.10
7 0.0882 0.00 -0.35 0.00 -0.23
8 0.0883 0.00 -0.33 0.00 -0.15
9 0.0910 0.00 -0.07 0.00 0.01
10 0.0911 0.00 -0.09 0.00 -0.08
11 0.0912 0.00 0.21 0.00 0.11
12 0.0938 0.00 0.01 0.00 -0.02
13 0.0940 0.00 0.05 0.00 -0.16
14 0.1014 0.00 0.03 0.00 -0.30
15 0.1016 0.00 -0.11 0.00 -0.13
16 0.1773 0.00 0.05 0.00 -0.12
17 0.1776 0.00 0.02 0.00 0.04
18 0.1779 0.00 0.07 0.00 0.09
19 0.1780 0.00 0.14 0.00 0.01
20 0.1782 0.00 0.09 0.00 -0.06
21 0.1784 0.00 0.09 0.00 0.16
22 0.1787 0.00 0.21 0.00 -0.03
23 3.1597 0.00 0.03 0.00 0.08
24 3.1598 0.00 -0.01 0.00 0.16
25 3.1599 0.00 0.00 0.00 0.14
26 3.1601 0.00 -0.02 0.00 0.14
27 3.1602 0.00 -0.01 0.00 0.16
28 3.1652 0.00 0.01 0.00 0.20
29 3.1652 0.00 0.14 0.00 0.15
30 5.1066 0.00 -0.00 0.00 -0.12
31 5.1068 0.00 0.04 0.00 -0.19
32 5.1068 0.00 0.03 0.00 -0.03
33 5.1068 0.00 -0.07 0.00 -0.07
34 6.0622 0.00 0.22 0.00 -0.11
35 6.1525 0.00 0.04 0.00 -0.14
36 6.1552 0.00 -0.06 0.00 -0.07
37 6.2286 0.00 0.02 0.00 0.03
38 6.2290 0.00 0.02 0.00 0.03
39 6.2294 0.00 0.02 0.00 0.03
40 6.2314 0.00 -0.11 0.00 0.02
41 6.2317 0.00 -0.10 0.00 0.02
42 6.2319 0.00 -0.11 0.00 0.02
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.
11HJ103 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 46.392 46.392 46.392 ecceobj 0.155 0.155 0.155 incobj 5.339 5.339 5.339 qmin 38.655 38.679 38.676 qmax 54.883 54.909 54.892 amean 46.594 46.597 46.596 amin 46.185 46.189 46.194 amax 47.044 47.075 47.059 emean 0.154 0.154 0.154 emin 0.140 0.140 0.140 emax 0.167 0.168 0.167 imean 4.002 4.005 4.001 imin 3.505 3.505 3.505 imax 4.509 4.510 4.502 excite_mean 0.169 0.169 0.169 fracstop 1.000 1.000 1.000 cjmean 3.098 3.098 3.098 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 184.1 184.3 184.1 kozaiamp 180.0 180.0 180.0