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: 14QJ562 # Created Fri Nov 22 02:09:58 2024 # Orbit generated from Bernstein formalism # Fitting 13 observations of 13 # Arc: 2.15y # First observation: 2014/08/17 # Last observation: 2016/10/10 Preliminary a, adot, b, bdot, g, gdot: -0.000033 0.028193 0.000004 0.002276 0.027042 0.000000 # Chi-squared of fit: 5.84 DOF: 20 RMS: 0.12 # Min/Max residuals: -0.30 0.29 # Exact a, adot, b, bdot, g, gdot: 1.612611E-05 2.862387E-02 1.367808E-06 2.296718E-03 2.757403E-02 1.088279E-03 # Covariance matrix: 4.6988E-13 -3.3652E-13 -1.0316E-13 -8.3550E-14 4.7934E-13 -7.0459E-12 -3.3652E-13 5.1474E-12 -3.4489E-13 1.2261E-12 1.3587E-12 1.1657E-10 -1.0316E-13 -3.4489E-13 2.3235E-13 -2.0050E-13 -3.1067E-13 -7.6205E-12 -8.3550E-14 1.2261E-12 -2.0050E-13 6.5867E-13 2.9391E-13 2.9933E-11 4.7934E-13 1.3587E-12 -3.1067E-13 2.9391E-13 1.3551E-12 2.9560E-11 -7.0459E-12 1.1657E-10 -7.6205E-12 2.9933E-11 2.9560E-11 2.8402E-09 # lat0 lon0 xBary yBary zBary JD0 -27.026836 -45.120115 -0.161620 -0.455325 -0.892847 2456886.712198 # Heliocentric elements and errors Epoch: 2456880.5000 = 2014/08/11 Mean Anomaly: 65.18552 +/- 0.521 Argument of Peri: 209.21568 +/- 0.712 Long of Asc Node: 34.66958 +/- 0.003 Inclination: 26.71179 +/- 0.000 Eccentricity: 0.04659748 +/- 0.0018 Semi-Major Axis: 37.82897630 +/- 0.0102 Time of Perihelion: 2441492.4373 +/- 122.8 Perihelion: 36.06624123 +/- 0.0690 Aphelion: 39.59171137 +/- 0.0691 Period (y) 232.6725 +/- 0.09 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 23.61545206 +/- 0.0010 Ecliptic Y -23.48553206 +/- 0.0010 Ecliptic Z -16.47950686 +/- 0.0007 Ecliptic XDOT 0.00215001 +/- 0.0000 Ecliptic YDOT 0.00185954 +/- 0.0000 Ecliptic ZDOT 0.00015416 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.15957398 +/- 0.0009 Geocenter to KBO 36.26601039 +/- 0.0015 # Hcoef: 7.28
The following table shows the complete astrometric record for 14QJ562. 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 (14QJ562) followed by the observatory code and reference code for the source of the astrometry.
2014 08 17.21142 21 50 32.308 -41 54 43.66 23.3r 14QJ562 W84 C~52Tr 2014 08 20.20634 21 50 11.758 -41 55 45.14 24.1g 14QJ562 W84 C~52Tr 2014 08 22.20417 21 49 58.060 -41 56 21.90 23.4r 14QJ562 W84 C~52Tr 2014 09 26.07221 21 46 22.590 -41 57 22.38 24.1g 14QJ562 W84 C~52Tr 2014 10 21.16602 21 44 49.529 -41 46 39.18 24.0g 14QJ562 W84 C~52Tr 2014 10 21.16740 21 44 49.499 -41 46 39.07 22.8i 14QJ562 W84 C~52Tr 2014 10 23.14995 21 44 45.346 -41 45 26.01 22.2z 14QJ562 W84 C~52Tr 2014 10 26.05693 21 44 40.165 -41 43 33.89 23.2i 14QJ562 W84 C~52Tr 2014 10 28.03643 21 44 37.291 -41 42 13.93 23.5r 14QJ562 W84 C~52Tr 2014 10 29.01513 21 44 36.041 -41 41 33.59 22.5z 14QJ562 W84 C~52Tr 2014 11 04.02629 21 44 31.378 -41 37 11.08 22.7z 14QJ562 W84 C~52Tr 2015 09 22.09812 21 54 31.625 -41 14 12.73 21.1z 14QJ562 W84 C~52Tr 2016 10 10.99880 22 00 34.287 -40 23 14.27 22.6z 14QJ562 W84 C~52Tr
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 0.06 0.00 -0.01
2 0.0082 -235.62 0.00 29.45 -0.05
3 0.0137 -391.08 -0.03 52.85 0.03
4 0.1091 -2646.17 0.00 888.02 0.02
5 0.1778 -3380.68 0.25 1865.52 -0.24
6 0.1778 -3380.96 -0.01 1865.74 -0.08
7 0.1833 -3397.87 0.14 1950.68 0.00
8 0.1912 -3411.43 -0.05 2076.21 0.01
9 0.1966 -3412.56 0.01 2162.42 0.09
10 0.1993 -3411.05 -0.30 2205.10 0.05
11 0.2158 -3365.02 -0.07 2468.84 0.01
12 1.0976 3411.43 -0.04 1218.88 0.29
13 2.1514 8407.57 0.02 2399.12 -0.14
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.
14QJ562 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 37.941 37.979 37.904 ecceobj 0.046 0.051 0.042 incobj 26.728 26.728 26.728 qmin 35.449 35.306 35.766 qmax 40.771 40.974 40.322 amean 38.022 38.057 37.979 amin 37.741 37.757 37.694 amax 38.310 38.352 38.265 emean 0.051 0.055 0.044 emin 0.038 0.042 0.033 emax 0.065 0.069 0.054 imean 25.643 25.647 25.651 imin 24.915 24.907 24.959 imax 26.366 26.358 26.357 excite_mean 0.436 0.436 0.435 fracstop 1.000 1.000 1.000 cjmean 2.816 2.815 2.816 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 179.7 179.8 182.6 kozaiamp 180.0 180.0 179.9