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: 184314 # Created Thu Nov 21 02:06:59 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 25 observations of 25 # Arc: 13.19y # First observation: 2005/03/11 # Last observation: 2018/05/19 # Chi-squared of fit: 54.04 DOF: 44 RMS: 0.26 # Min/Max residuals: -0.82 0.59 # Exact a, adot, b, bdot, g, gdot: 1.646594E-05 2.366402E-02 -1.163531E-06 -2.268985E-03 2.407383E-02 -2.754945E-03 # Covariance matrix: 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 # lat0 lon0 xBary yBary zBary JD0 -1.786459 -161.356701 0.462479 -0.027180 -0.874154 2453440.877673 # Heliocentric elements and errors Epoch: 2453440.5000 = 2005/03/11 Mean Anomaly: 305.38187 +/- 0.000 Argument of Peri: 266.89913 +/- 0.000 Long of Asc Node: 0.37382 +/- 0.000 Inclination: 5.75404 +/- 0.000 Eccentricity: 0.14144933 +/- 0.0000 Semi-Major Axis: 45.46285010 +/- 0.0000 Time of Perihelion: 2470427.5425 +/- 0.0 Perihelion: 39.03216035 +/- 0.0000 Aphelion: 51.89353986 +/- 0.0000 Period (y) 306.5443 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -40.32071006 +/- 0.0000 Ecliptic Y -13.11472408 +/- 0.0000 Ecliptic Z -1.29498075 +/- 0.0000 Ecliptic XDOT 0.00116477 +/- 0.0000 Ecliptic YDOT -0.00245449 +/- 0.0000 Ecliptic ZDOT -0.00024809 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 42.41980122 +/- 0.0000 Geocenter to KBO 41.53898453 +/- 0.0000 # Hcoef: 6.38
The following table shows the complete astrometric record for 184314. 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 (184314) followed by the observatory code and reference code for the source of the astrometry.
2005 03 11.37693 13 06 02.93 -08 57 26.6 22.2R 184314 695 Cn0311 2005 03 11.47979 13 06 02.53 -08 57 24.4 184314 695 Cn0311 2005 03 12.41944 13 05 58.79 -08 57 04.3 184314 695 Cn0311 2005 04 11.41433 13 03 47.66 -08 44 41.2 21.6R 184314 695 Cn3133 2005 04 11.45325 13 03 47.50 -08 44 39.8 184314 695 Cn3133 2005 04 12.33541 13 03 43.50 -08 44 16.6 184314 695 Cn3133 2005 04 15.21094 13 03 30.59 -08 43 01.1 21.4R 184314 304 Cn3360 2005 04 15.24975 13 03 30.43 -08 42 59.8 184314 304 Cn3360 2005 06 07.04591 13 00 28.39 -08 24 12.6 22.8R 184314 304 Cn6541 2005 06 07.13792 13 00 28.22 -08 24 11.5 184314 304 Cn6541 2005 07 10.98341 13 00 13.25 -08 21 55.0 22.8R 184314 304 Cn8898 2005 07 11.06000 13 00 13.30 -08 21 55.3 184314 304 Cn8898 2006 02 22.34826 13 11 56.78 -09 40 46.3 22.6R 184314 304 Cr0850 2006 02 22.38319 13 11 56.67 -09 40 45.8 184314 304 Cr0850 2006 05 02.25206 13 07 12.28 -09 14 18.6 23.1r 184314 695 Cr0850 2006 05 02.31530 13 07 11.99 -09 14 17.7 22.2r 184314 695 Cr0850 2007 04 21.07968 13 12 58.43 -09 57 40.8 21.2R 184314 807 Cv1537 2007 04 21.26898 13 12 57.56 -09 57 36.3 184314 807 Cv1537 2008 03 03.36547 13 21 22.79 -10 54 30.4 184314 695 Cy7595 2008 03 03.49173 13 21 22.38 -10 54 28.5 184314 695 Cy7595 2008 03 05.44424 13 21 15.65 -10 53 56.0 184314 695 Cy7595 2008 03 05.49806 13 21 15.46 -10 53 55.0 184314 695 Cy7595 2018 05 19.151490 14 08 43.03 -16 40 38.0 22.8G 184314 705 C~2rR1 2018 05 19.201840 14 08 42.82 -16 40 36.8 22.7G 184314 705 C~2rR1 2018 05 19.244280 14 08 42.61 -16 40 35.9 22.8G 184314 705 C~2rR1
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 -0.20 0.00 0.01
2 0.0003 0.00 -0.01 0.00 0.01
3 0.0029 0.00 -0.33 0.00 -0.07
4 0.0850 0.00 -0.15 0.00 -0.22
5 0.0851 0.00 0.12 0.00 0.15
6 0.0875 0.00 -0.25 0.00 -0.00
7 0.0954 0.00 -0.01 0.00 -0.82
8 0.0955 0.00 0.24 0.00 -0.55
9 0.2400 0.00 0.05 0.00 0.04
10 0.2403 0.00 0.14 0.00 -0.01
11 0.3329 0.00 -0.02 0.00 -0.09
12 0.3332 0.00 -0.35 0.00 -0.03
13 0.9527 0.00 0.05 0.00 0.23
14 0.9528 0.00 -0.04 0.00 0.24
15 1.1413 0.00 0.05 0.00 0.16
16 1.1415 0.00 -0.34 0.00 -0.51
17 2.1101 0.00 0.12 0.00 0.42
18 2.1106 0.00 -0.00 0.00 -0.03
19 2.9788 0.00 0.07 0.00 0.59
20 2.9791 0.00 0.46 0.00 0.43
21 2.9844 0.00 0.20 0.00 0.20
22 2.9846 0.00 0.24 0.00 0.27
23 13.1876 0.00 -0.12 0.00 -0.11
24 13.1877 0.00 0.10 0.00 -0.09
25 13.1879 0.00 -0.20 0.00 -0.18
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.
184314 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.870 44.870 44.870 ecceobj 0.137 0.137 0.137 incobj 5.784 5.784 5.784 qmin 38.343 38.348 38.349 qmax 52.372 52.339 52.392 amean 45.199 45.198 45.198 amin 44.824 44.818 44.817 amax 45.615 45.617 45.619 emean 0.134 0.134 0.134 emin 0.119 0.119 0.120 emax 0.149 0.148 0.149 imean 6.207 6.207 6.207 imin 5.494 5.497 5.494 imax 6.831 6.845 6.831 excite_mean 0.172 0.172 0.172 fracstop 1.000 1.000 1.000 cjmean 3.079 3.079 3.079 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 178.0 178.1 177.9 kozaiamp 180.0 179.9 180.0