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: 07CR79
# Created Fri Apr 19 01:12:52 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 21 observations of 21
# Arc: 17.16y
# First observation: 2005/02/10
# Last observation: 2022/04/08
# Chi-squared of fit: 14.53 DOF: 36 RMS: 0.15
# Min/Max residuals: -0.19 0.40
# Exact a, adot, b, bdot, g, gdot:
1.600288E-05 2.954512E-02 5.572871E-06 1.183567E-02 2.785925E-02 5.743752E-04
# Covariance matrix:
2.0271E-13 -5.2403E-14 2.9664E-14 -1.8630E-14 7.5892E-14 -8.9376E-14
-5.2403E-14 2.7682E-14 -1.7073E-14 1.0989E-14 -1.5451E-14 5.2007E-14
2.9664E-14 -1.7073E-14 1.3380E-13 -1.7235E-14 1.7885E-14 -3.4919E-14
-1.8630E-14 1.0989E-14 -1.7235E-14 6.5117E-15 -9.2985E-15 2.2304E-14
7.5892E-14 -1.5451E-14 1.7885E-14 -9.2985E-15 2.5044E-13 -4.9781E-14
-8.9376E-14 5.2007E-14 -3.4919E-14 2.2304E-14 -4.9781E-14 1.0600E-13
# lat0 lon0 xBary yBary zBary JD0
1.392795 136.524240 -0.084238 0.023932 -0.979635 2453411.809733
# Heliocentric elements and errors
Epoch: 2453412.5000 = 2005/02/11
Mean Anomaly: 3.57226 +/- 0.002
Argument of Peri: 357.87024 +/- 0.003
Long of Asc Node: 133.27406 +/- 0.000
Inclination: 21.83601 +/- 0.000
Eccentricity: 0.22421196 +/- 0.0001
Semi-Major Axis: 47.49145061 +/- 0.0051
Time of Perihelion: 2452226.2883 +/- 0.6
Perihelion: 36.84329936 +/- 0.0051
Aphelion: 58.13960186 +/- 0.0070
Period (y) 327.2890 +/- 0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -26.81363137 +/- 0.0005
Ecliptic Y 25.30267818 +/- 0.0004
Ecliptic Z 0.87266594 +/- 0.0000
Ecliptic XDOT -0.00201838 +/- 0.0000
Ecliptic YDOT -0.00209480 +/- 0.0000
Ecliptic ZDOT 0.00116424 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 36.87759503 +/- 0.0005
Geocenter to KBO 35.89474555 +/- 0.0006
# Hcoef: 7.32
The following table shows the complete astrometric record for 07CR79. 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 (07CR79) followed by the observatory code and reference code for the source of the astrometry.
2005 02 10.30899 09 17 40.05 +17 12 43.5 23.4g 07CR79 568 C~0VEU 2005 02 10.39196 09 17 39.59 +17 12 45.9 23.5g 07CR79 568 C~0VEU 2005 02 10.43152 09 17 39.36 +17 12 47.3 23.4g 07CR79 568 C~0VEU 2005 04 11.30482 09 13 43.08 +17 36 02.0 23.3i 07CR79 568 C~0VEU 2005 04 11.33442 09 13 43.03 +17 36 02.4 23.3i 07CR79 568 C~0VEU 2005 04 11.35929 09 13 42.99 +17 36 02.7 23.4i 07CR79 568 C~0VEU 2007 02 14.45798 09 32 35.01 +17 28 40.4 23.0r 07CR79 568 C74770 2007 02 14.49571 09 32 34.80 +17 28 41.6 23.0r 07CR79 568 C74770 2007 02 14.52893 09 32 34.63 +17 28 42.7 23.0r 07CR79 568 C74770 2007 02 15.47269 09 32 29.57 +17 29 13.3 23.1r 07CR79 568 C74770 2007 11 08.51341 09 44 29.36 +16 55 10.2 22.0r 07CR79 695 C~0VEU 2007 11 09.49094 09 44 31.29 +16 55 12.8 22.1r 07CR79 695 C~0VEU 2008 05 04.16494 09 35 54.96 +17 59 00.0 07CR79 695 C~0VEU 2008 05 05.13645 09 35 55.33 +17 58 59.5 07CR79 695 C~0VEU 2008 05 05.13952 09 35 55.31 +17 58 59.2 07CR79 695 C~0VEU 2015 02 18.26506 10 32 34.73 +17 44 04.9 22.3R 07CR79 695 C~1M6T 2015 02 18.35525 10 32 34.26 +17 44 08.4 07CR79 695 C~1M6T 2015 02 18.44818 10 32 33.78 +17 44 11.7 07CR79 695 C~1M6T 2022 04 08.150950 11 19 33.080 +17 28 59.81 22.8G 07CR79 G37 C~5ZWP 2022 04 08.185850 11 19 32.948 +17 29 00.49 07CR79 G37 C~5ZWP 2022 04 08.220830 11 19 32.800 +17 29 01.01 07CR79 G37 C~5ZWP
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 0.23 0.00 0.18
2 0.0002 0.00 0.16 0.00 -0.04
3 0.0003 0.00 -0.03 0.00 0.12
4 0.1643 0.00 -0.14 0.00 -0.17
5 0.1643 0.00 -0.16 0.00 -0.11
6 0.1644 0.00 -0.15 0.00 -0.09
7 2.0100 0.00 -0.06 0.00 -0.10
8 2.0101 0.00 -0.12 0.00 -0.12
9 2.0102 0.00 0.04 0.00 -0.09
10 2.0128 0.00 -0.14 0.00 0.05
11 2.7411 0.00 0.09 0.00 0.13
12 2.7438 0.00 0.08 0.00 0.36
13 3.2275 0.00 -0.19 0.00 -0.16
14 3.2302 0.00 0.40 0.00 0.22
15 3.2302 0.00 0.09 0.00 -0.07
16 10.0204 0.00 -0.08 0.00 -0.10
17 10.0207 0.00 -0.07 0.00 0.04
18 10.0209 0.00 -0.01 0.00 -0.11
19 17.1549 0.00 -0.17 0.00 0.11
20 17.1550 0.00 0.10 0.00 0.07
21 17.1551 0.00 0.14 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.
07CR79 quality flag:3 Type: SCATNEAR SCATNEAR SCATNEAR axisobj 47.228 47.228 47.228 ecceobj 0.220 0.220 0.220 incobj 21.878 21.878 21.878 qmin 35.474 35.408 35.451 qmax 59.539 59.600 59.381 amean 47.191 47.192 47.192 amin 46.759 46.734 46.771 amax 47.753 47.782 47.732 emean 0.228 0.228 0.228 emin 0.210 0.210 0.210 emax 0.247 0.247 0.247 imean 20.240 20.241 20.238 imin 19.645 19.650 19.638 imax 20.758 20.756 20.764 excite_mean 0.414 0.414 0.415 fracstop 1.000 1.000 1.000 cjmean 2.926 2.926 2.926 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 168.6 168.4 168.8 kozaiamp 180.0 180.0 179.9