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: 16QC135 # Created Sun Nov 24 02:10:41 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 13 observations of 13 # Arc: 6.17y # First observation: 2016/08/26 # Last observation: 2022/10/29 # Chi-squared of fit: 5.10 DOF: 20 RMS: 0.11 # Min/Max residuals: -0.22 0.21 # Exact a, adot, b, bdot, g, gdot: 1.303286E-05 1.763547E-02 -5.938889E-07 -2.054515E-03 2.086603E-02 1.461092E-03 # Covariance matrix: 4.2706E-13 -8.7985E-14 -4.6861E-15 1.0618E-14 3.0599E-13 -7.9143E-13 -8.7985E-14 3.5511E-13 2.5897E-14 -4.5178E-14 2.7864E-13 3.4239E-12 -4.6861E-15 2.5897E-14 2.0738E-13 -4.6911E-14 1.9595E-14 2.6685E-13 1.0618E-14 -4.5178E-14 -4.6911E-14 2.6603E-14 -3.0298E-14 -4.6931E-13 3.0599E-13 2.7864E-13 1.9595E-14 -3.0298E-14 7.7765E-13 2.3174E-12 -7.9143E-13 3.4239E-12 2.6685E-13 -4.6931E-13 2.3174E-12 3.5547E-11 # lat0 lon0 xBary yBary zBary JD0 -5.671733 9.779873 0.598847 -0.080507 -0.812343 2457626.816669 # Heliocentric elements and errors Epoch: 2457626.5000 = 2016/08/26 Mean Anomaly: 142.58786 +/- 0.128 Argument of Peri: 69.39815 +/- 0.123 Long of Asc Node: 149.62047 +/- 0.002 Inclination: 8.73655 +/- 0.000 Eccentricity: 0.12640072 +/- 0.0002 Semi-Major Axis: 44.08578954 +/- 0.0056 Time of Perihelion: 2415279.1321 +/- 38.9 Perihelion: 38.51331411 +/- 0.0084 Aphelion: 49.65826497 +/- 0.0093 Period (y) 292.7225 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 47.89953522 +/- 0.0020 Ecliptic Y 7.64687797 +/- 0.0003 Ecliptic Z -4.73638707 +/- 0.0002 Ecliptic XDOT -0.00022977 +/- 0.0000 Ecliptic YDOT 0.00230126 +/- 0.0000 Ecliptic ZDOT -0.00028723 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 48.73673348 +/- 0.0020 Geocenter to KBO 47.92476074 +/- 0.0020 # Hcoef: 6.94
The following table shows the complete astrometric record for 16QC135. 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 (16QC135) followed by the observatory code and reference code for the source of the astrometry.
2016 08 26.31588 00 44 51.007 -01 20 34.61 23.8i 16QC135 W84 C~55Zd 2016 08 26.31725 00 44 50.987 -01 20 34.57 23.0z 16QC135 W84 C~55Zd 2016 09 09.27780 00 44 06.213 -01 26 31.47 23.5r 16QC135 W84 C~55Zd 2016 11 06.18492 00 40 31.262 -01 49 47.24 23.7r 16QC135 W84 C~55Zd 2016 11 06.19115 00 40 31.240 -01 49 47.29 23.6i 16QC135 W84 C~55Zd 2017 09 27.22126 00 46 54.790 -01 17 10.23 23.9r 16QC135 W84 C~55Zd 2017 10 20.16631 00 45 25.785 -01 26 46.94 23.2i 16QC135 W84 C~55Zd 2018 09 14.32489 00 51 37.572 -00 54 02.91 23.9i 16QC135 W84 C~55Zd 2018 11 08.18087 00 48 13.257 -01 15 47.67 23.3i 16QC135 W84 C~55Zd 2018 11 27.08311 00 47 21.994 -01 19 46.19 24.6g 16QC135 W84 C~55Zd 2022 10 29.259020 01 04 18.757 -00 03 39.88 24.1G 16QC135 G37 C~5z9z 2022 10 29.297680 01 04 18.623 -00 03 40.69 16QC135 G37 C~5z9z 2022 10 29.336440 01 04 18.451 -00 03 41.66 16QC135 G37 C~5z9z
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 0.14 0.00 -0.16
2 0.0000 0.00 -0.10 0.00 -0.08
3 0.0382 0.00 0.06 0.00 0.09
4 0.1968 0.00 -0.03 0.00 0.01
5 0.1968 0.00 -0.06 0.00 0.06
6 1.0867 0.00 -0.10 0.00 -0.02
7 1.1495 0.00 0.21 0.00 0.12
8 2.0507 0.00 0.04 0.00 -0.10
9 2.2009 0.00 0.00 0.00 -0.02
10 2.2526 0.00 -0.12 0.00 0.17
11 6.1737 0.00 0.02 0.00 0.04
12 6.1738 0.00 0.19 0.00 0.04
13 6.1739 0.00 -0.22 0.00 -0.13
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.
16QC135 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.515 44.515 44.515 ecceobj 0.117 0.117 0.117 incobj 8.706 8.706 8.706 qmin 38.417 38.417 38.418 qmax 50.546 50.483 50.474 amean 44.304 44.299 44.303 amin 43.925 43.927 43.935 amax 44.714 44.712 44.711 emean 0.113 0.113 0.114 emin 0.097 0.098 0.097 emax 0.131 0.130 0.130 imean 7.901 7.908 7.893 imin 7.191 7.202 7.168 imax 8.648 8.650 8.658 excite_mean 0.178 0.178 0.178 fracstop 1.000 1.000 1.000 cjmean 3.067 3.067 3.067 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 183.1 183.8 183.5 kozaiamp 180.0 180.0 180.0