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: 06HB123
# Created Fri Apr 26 01:12:38 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 15 observations of 15
# Arc: 7.11y
# First observation: 2006/04/28
# Last observation: 2013/06/07
# Chi-squared of fit: 29.33 DOF: 24 RMS: 0.25
# Min/Max residuals: -0.87 0.44
# Exact a, adot, b, bdot, g, gdot:
1.685001E-05 2.638520E-02 1.546809E-08 -3.581949E-04 2.550285E-02 -2.728974E-04
# Covariance matrix:
2.6556E-13 -2.0661E-13 2.4799E-16 2.6717E-15 1.1200E-13 -1.0419E-12
-2.0661E-13 7.5079E-13 5.7401E-15 -1.1169E-14 2.3209E-13 4.0621E-12
2.4799E-16 5.7401E-15 1.4277E-13 -2.4160E-14 5.4447E-15 3.0822E-14
2.6717E-15 -1.1169E-14 -2.4160E-14 1.3311E-14 -3.7153E-15 -6.1462E-14
1.1200E-13 2.3209E-13 5.4447E-15 -3.7153E-15 4.4254E-13 1.1981E-12
-1.0419E-12 4.0621E-12 3.0822E-14 -6.1462E-14 1.1981E-12 2.2387E-11
# lat0 lon0 xBary yBary zBary JD0
1.670347 -128.658571 0.236182 0.028508 -0.973631 2453853.732894
# Heliocentric elements and errors
Epoch: 2453854.5000 = 2006/04/29
Mean Anomaly: 351.68805 +/- 0.098
Argument of Peri: 125.36791 +/- 0.119
Long of Asc Node: 115.74994 +/- 0.007
Inclination: 1.80177 +/- 0.000
Eccentricity: 0.09630876 +/- 0.0001
Semi-Major Axis: 44.41242632 +/- 0.0050
Time of Perihelion: 2456350.5627 +/- 34.3
Perihelion: 40.13512061 +/- 0.0056
Aphelion: 48.68973202 +/- 0.0064
Period (y) 295.9818 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -25.27991405 +/- 0.0006
Ecliptic Y -31.22280717 +/- 0.0008
Ecliptic Z 1.14296830 +/- 0.0000
Ecliptic XDOT 0.00223332 +/- 0.0000
Ecliptic YDOT -0.00175316 +/- 0.0000
Ecliptic ZDOT -0.00003932 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.19010967 +/- 0.0007
Geocenter to KBO 39.21134634 +/- 0.0010
# Hcoef: 7.04
The following table shows the complete astrometric record for 06HB123. 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 (06HB123) followed by the observatory code and reference code for the source of the astrometry.
2006 04 28.23214 15 17 28.73 -16 29 01.1 21.9R 06HB123 807 Cr3609 2006 04 28.29620 15 17 28.42 -16 28 59.7 06HB123 807 Cr3609 2006 05 01.36669 15 17 13.47 -16 28 00.8 23.3R 06HB123 695 Cr3609 2006 05 01.43896 15 17 13.11 -16 27 59.7 06HB123 695 Cr3609 2006 05 02.45601 15 17 08.09 -16 27 40.9 06HB123 695 Cr3609 2006 08 21.05302 15 12 10.93 -16 11 29.6 22.6R 06HB123 807 Cs2782 2006 08 22.04878 15 12 12.73 -16 11 39.8 06HB123 807 Cs2782 2006 08 23.05024 15 12 14.66 -16 11 50.0 06HB123 807 Cs2782 2007 04 22.27105 15 24 03.89 -16 55 19.2 22.6R 06HB123 807 Cv2001 2007 04 22.33864 15 24 03.54 -16 55 18.4 06HB123 807 Cv2001 2007 07 12.01225 15 18 18.58 -16 34 53.0 06HB123 304 Cv2001 2007 07 12.09877 15 18 18.38 -16 34 52.5 06HB123 304 Cv2001 2013 06 07.00319 15 57 18.95 -18 55 11.2 23.3R 06HB123 304 C~0sns 2013 06 07.13100 15 57 18.28 -18 55 09.8 06HB123 304 C~0sns 2013 06 07.31047 15 57 17.35 -18 55 07.3 06HB123 304 C~0sns
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 -0.12 0.00 -0.02
2 0.0002 0.00 -0.04 0.00 0.15
3 0.0086 0.00 0.11 0.00 0.27
4 0.0088 0.00 0.11 0.00 -0.03
5 0.0116 0.00 -0.15 0.00 -0.87
6 0.3144 0.00 0.13 0.00 0.33
7 0.3171 0.00 -0.11 0.00 0.05
8 0.3198 0.00 -0.00 0.00 0.20
9 0.9830 0.00 0.21 0.00 0.23
10 0.9832 0.00 -0.29 0.00 -0.18
11 1.2041 0.00 0.05 0.00 -0.02
12 1.2043 0.00 0.02 0.00 -0.05
13 7.1096 0.00 0.44 0.00 0.20
14 7.1099 0.00 0.01 0.00 -0.12
15 7.1104 0.00 -0.43 0.00 -0.10
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.
06HB123 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.804 43.804 43.804 ecceobj 0.085 0.085 0.085 incobj 1.802 1.802 1.802 qmin 39.634 39.653 39.622 qmax 48.916 48.918 48.899 amean 44.146 44.146 44.147 amin 43.796 43.797 43.797 amax 44.536 44.540 44.526 emean 0.082 0.082 0.082 emin 0.066 0.066 0.066 emax 0.099 0.099 0.098 imean 1.027 1.027 1.027 imin 0.257 0.257 0.257 imax 1.630 1.630 1.629 excite_mean 0.084 0.084 0.084 fracstop 1.000 1.000 1.000 cjmean 3.095 3.095 3.095 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 163.5 163.5 163.4 kozaiamp 180.0 179.9 180.0