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: 06HX122 # Created Wed Dec 25 02:08:48 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 18 observations of 18 # Arc: 15.13y # First observation: 2006/04/27 # Last observation: 2021/06/13 # Chi-squared of fit: 13.22 DOF: 30 RMS: 0.15 # Min/Max residuals: -0.28 0.39 # Exact a, adot, b, bdot, g, gdot: 1.379309E-05 1.715758E-02 4.025071E-06 3.781090E-03 1.974967E-02 8.327593E-03 # Covariance matrix: 3.3123E-13 -1.4153E-13 2.4686E-14 -2.9796E-14 2.0092E-13 -5.9165E-13 -1.4153E-13 1.0497E-13 -2.0618E-14 2.3358E-14 -8.3932E-14 4.6198E-13 2.4686E-14 -2.0618E-14 1.3296E-13 -1.7838E-14 1.3104E-14 -9.4779E-14 -2.9796E-14 2.3358E-14 -1.7838E-14 9.9342E-15 -1.9322E-14 1.0741E-13 2.0092E-13 -8.3932E-14 1.3104E-14 -1.9322E-14 2.9912E-13 -3.8787E-13 -5.9165E-13 4.6198E-13 -9.4779E-14 1.0741E-13 -3.8787E-13 2.1245E-12 # lat0 lon0 xBary yBary zBary JD0 -3.718798 -125.356456 0.307523 -0.061741 -0.951665 2453852.769434 # Heliocentric elements and errors Epoch: 2453852.5000 = 2006/04/27 Mean Anomaly: 32.83683 +/- 0.015 Argument of Peri: 258.61800 +/- 0.012 Long of Asc Node: 250.56202 +/- 0.000 Inclination: 12.83183 +/- 0.000 Eccentricity: 0.49006771 +/- 0.0001 Semi-Major Axis: 70.95533896 +/- 0.0206 Time of Perihelion: 2433939.5859 +/- 12.5 Perihelion: 36.18241822 +/- 0.0139 Aphelion: 105.72825970 +/- 0.0320 Period (y) 597.7035 +/- 0.26 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -30.04369947 +/- 0.0008 Ecliptic Y -41.81145183 +/- 0.0011 Ecliptic Z -3.28388395 +/- 0.0001 Ecliptic XDOT 0.00125735 +/- 0.0000 Ecliptic YDOT -0.00234933 +/- 0.0000 Ecliptic ZDOT 0.00044816 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 51.59041450 +/- 0.0010 Geocenter to KBO 50.63344594 +/- 0.0014 # Hcoef: 6.10
The following table shows the complete astrometric record for 06HX122. 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 (06HX122) followed by the observatory code and reference code for the source of the astrometry.
2006 04 27.26868 15 25 13.18 -22 32 04.0 22.0R 06HX122 807 Cr3609 2006 04 27.34068 15 25 12.89 -22 32 02.5 06HX122 807 Cr3609 2006 04 28.24437 15 25 09.36 -22 31 49.5 06HX122 807 Cr3609 2006 06 20.02220 15 21 44.37 -22 17 00.7 23.0R 06HX122 304 Cr4858 2006 06 20.11619 15 21 44.06 -22 16 59.1 06HX122 304 Cr4858 2006 08 21.06094 15 20 32.76 -22 06 25.7 23.1R 06HX122 807 Cs2782 2006 08 22.05630 15 20 34.01 -22 06 23.5 06HX122 807 Cs2782 2006 08 23.05962 15 20 35.30 -22 06 22.5 06HX122 807 Cs2782 2007 06 16.01531 15 26 18.80 -22 20 32.1 06HX122 304 Cz0452 2007 06 16.08909 15 26 18.55 -22 20 30.7 06HX122 304 Cz0452 2007 07 16.07986 15 25 00.08 -22 13 19.9 06HX122 568 Cz0452 2009 03 23.357900 15 39 45.421 -22 42 04.17 06HX122 250 S~839V 2009 03 23.364150 15 39 45.402 -22 42 04.16 06HX122 250 S~839V 2009 03 23.423872 15 39 45.286 -22 42 03.80 06HX122 250 S~839V 2009 03 23.430122 15 39 45.268 -22 42 03.78 06HX122 250 S~839V 2013 05 08.344967 15 53 22.25 -22 34 10.6 23.6r 06HX122 W84 C~839V 2021 06 13.038685 16 20 32.86 -22 13 23.8 24.2V 06HX122 W84 C~839V 2021 06 13.169331 16 20 32.36 -22 13 22.7 06HX122 W84 C~839V
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 -0.20
2 0.0002 0.00 -0.12 0.00 0.24
3 0.0027 0.00 0.14 0.00 -0.10
4 0.1472 0.00 0.05 0.00 -0.24
5 0.1474 0.00 -0.01 0.00 -0.17
6 0.3170 0.00 -0.12 0.00 0.15
7 0.3197 0.00 0.26 0.00 0.39
8 0.3225 0.00 -0.10 0.00 -0.28
9 1.1355 0.00 0.01 0.00 -0.02
10 1.1357 0.00 0.11 0.00 0.19
11 1.2178 0.00 -0.19 0.00 0.12
12 2.9051 0.00 0.15 0.00 0.02
13 2.9051 0.00 0.06 0.00 -0.00
14 2.9053 0.00 0.15 0.00 0.02
15 2.9053 0.00 0.07 0.00 0.00
16 7.0310 0.00 0.10 0.00 0.08
17 15.1287 0.00 0.11 0.00 0.11
18 15.1291 0.00 -0.13 0.00 -0.16
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.
06HX122 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 69.496 69.497 69.496 ecceobj 0.484 0.484 0.484 incobj 12.898 12.898 12.898 qmin 35.319 35.182 35.044 qmax 107.165 107.667 107.823 amean 70.163 70.388 70.258 amin 69.082 69.185 69.135 amax 71.724 72.007 71.768 emean 0.482 0.485 0.486 emin 0.468 0.471 0.471 emax 0.497 0.498 0.502 imean 14.540 14.575 14.434 imin 13.731 13.684 13.545 imax 15.465 15.329 15.339 excite_mean 0.544 0.546 0.546 fracstop 1.000 1.000 1.000 cjmean 3.017 3.016 3.014 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 179.0 185.5 184.2 kozaiamp 180.0 180.0 180.0