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: 471150
# Created Mon May 21 01:36:58 2018
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 85 observations of 85
# Arc: 12.45y
# First observation: 2002/12/11
# Last observation: 2015/05/23
# Chi-squared of fit: 201.86 DOF: 164 RMS: 0.27
# Min/Max residuals: -0.73 1.09
# Exact a, adot, b, bdot, g, gdot:
1.300310E-05 1.868193E-02 -8.745764E-06 -1.528409E-02 2.479015E-02 -4.890258E-04
# 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
7.596943 173.917859 0.976665 -0.010927 0.081801 2452619.974848
# Heliocentric elements and errors
Epoch: 2452620.5000 = 2002/12/12
Mean Anomaly: 233.09664 +/- 0.000
Argument of Peri: 299.11344 +/- 0.000
Long of Asc Node: 1.77263 +/- 0.000
Inclination: 39.69169 +/- 0.000
Eccentricity: 0.04721592 +/- 0.0000
Semi-Major Axis: 39.10819899 +/- 0.0000
Time of Perihelion: 2484110.3623 +/- 0.0
Perihelion: 37.26166946 +/- 0.0000
Aphelion: 40.95472852 +/- 0.0000
Period (y) 244.5738 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -39.57522621 +/- 0.0000
Ecliptic Y 5.20329846 +/- 0.0000
Ecliptic Z 5.33256193 +/- 0.0000
Ecliptic XDOT -0.00039454 +/- 0.0000
Ecliptic YDOT -0.00203748 +/- 0.0000
Ecliptic ZDOT -0.00168011 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.27047174 +/- 0.0000
Geocenter to KBO 40.33862665 +/- 0.0000
# Hcoef: 5.77
The following table shows the complete astrometric record for 471150. 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 (471150) followed by the observatory code and reference code for the source of the astrometry.
2002 12 11.474105 11 49 49.75 +09 23 06.6 21.8V 471150 645 C~1Q3z 2002 12 11.474934 11 49 49.75 +09 23 06.6 21.5V 471150 645 C~1Q3z 2002 12 11.477422 11 49 49.76 +09 23 06.6 22.4V 471150 645 C~1Q3z 2006 01 06.506513 11 57 31.09 +05 39 43.6 21.9V 471150 645 C~1Q3z 2006 01 06.507342 11 57 31.09 +05 39 43.6 21.6V 471150 645 C~1Q3z 2006 01 06.509830 11 57 31.09 +05 39 43.6 22.2V 471150 645 C~1Q3z 2007 04 15.208975 11 53 25.86 +04 55 28.5 21.8V 471150 645 C~2Pie 2007 04 15.209804 11 53 25.86 +04 55 28.6 21.5V 471150 645 C~2Pie 2007 04 15.212292 11 53 25.85 +04 55 28.6 22.4V 471150 645 C~2Pie 2010 03 18.06536 12 03 32.128 +00 55 07.28 21.0R 471150 809 C~0FoM 2010 03 18.14874 12 03 31.721 +00 55 09.40 21.3R 471150 809 C~0FoM 2010 03 18.23281 12 03 31.263 +00 55 12.57 21.2R 471150 809 C~0FoM 2010 03 19.06431 12 03 27.031 +00 55 30.57 471150 809 C~0FoM 2010 03 19.14753 12 03 26.602 +00 55 33.02 21.1R 471150 809 C~0FoM 2010 03 19.23185 12 03 26.144 +00 55 34.86 21.1R 471150 809 C~0FoM 2010 03 20.05904 12 03 21.877 +00 55 54.76 21.0R 471150 809 C~0FoM 2010 03 20.14266 12 03 21.453 +00 55 56.96 21.4R 471150 809 C~0FoM 2010 03 20.22531 12 03 21.031 +00 55 59.95 21.0R 471150 809 C~0FoM 2010 03 21.05796 12 03 16.721 +00 56 18.52 21.0R 471150 809 C~0FoM 2010 03 21.14213 12 03 16.289 +00 56 20.22 21.0R 471150 809 C~0FoM 2010 03 21.22492 12 03 15.842 +00 56 23.71 20.8R 471150 809 C~0FoM 2010 04 06.05953 12 01 55.196 +01 02 26.90 21.4R 471150 807 C~0GDt 2010 04 06.12183 12 01 54.859 +01 02 28.61 21.7R 471150 807 C~0GDt 2010 04 21.08801 12 00 44.483 +01 07 26.69 21.7R 471150 807 C~0Gu2 2010 04 21.15025 12 00 44.191 +01 07 27.86 21.6R 471150 807 C~0Gu2 2010 06 05.03169 11 58 35.609 +01 13 04.26 21.6R 471150 807 C~0IRp 2010 06 05.11109 11 58 35.511 +01 13 03.57 21.8R 471150 807 C~0IRp 2011 01 10.43322 12 10 12.86 -00 38 03.5 21.7R 471150 695 C~0UtK 2011 01 10.49169 12 10 12.80 -00 38 03.6 471150 695 C~0UtK 2011 01 10.53951 12 10 12.72 -00 38 03.4 471150 695 C~0UtK 2011 03 09.41964 12 06 52.99 -00 25 30.3 21.4R 471150 688 C~0UtK 2011 03 09.46458 12 06 52.78 -00 25 29.4 471150 688 C~0UtK 2011 12 02.61493 12 12 17.433 -01 44 07.84 21.9w 471150 F51 C~1vWC 2011 12 02.62089 12 12 17.434 -01 44 07.88 22.1w 471150 F51 C~1vWC 2011 12 02.62683 12 12 17.459 -01 44 08.09 22.0w 471150 F51 C~1vWC 2011 12 02.63277 12 12 17.475 -01 44 07.94 21.8w 471150 F51 C~1vWC 2012 02 24.54562 12 10 31.890 -01 47 21.20 21.5r 471150 F51 C~1vWC 2012 02 24.55552 12 10 31.844 -01 47 21.31 21.8r 471150 F51 C~1vWC 2012 02 24.56591 12 10 31.787 -01 47 20.89 22.0g 471150 F51 C~1vWC 2012 02 27.46871 12 10 18.484 -01 46 24.55 21.6w 471150 F51 C~1vWC 2012 02 27.48346 12 10 18.415 -01 46 24.19 21.8w 471150 F51 C~1vWC 2012 02 27.49827 12 10 18.341 -01 46 23.92 21.8w 471150 F51 C~1vWC 2012 02 27.51304 12 10 18.277 -01 46 23.72 21.9w 471150 F51 C~1vWC 2012 04 14.33434 12 06 23.630 -01 28 46.03 21.9w 471150 F51 C@0612 2012 04 14.34920 12 06 23.554 -01 28 45.71 21.6w 471150 F51 C@0612 2012 04 14.36405 12 06 23.484 -01 28 45.35 21.7w 471150 F51 C@0612 2012 04 14.37888 12 06 23.417 -01 28 45.07 21.8w 471150 F51 C@0612 2013 03 06.42554 12 12 18.446 -03 01 11.67 21.8w 471150 F51 C~1vWC 2013 03 06.44012 12 12 18.363 -03 01 11.37 21.8w 471150 F51 C~1vWC 2013 03 06.45472 12 12 18.291 -03 01 11.07 21.8w 471150 F51 C~1vWC 2013 03 06.46937 12 12 18.223 -03 01 10.62 21.8w 471150 F51 C~1vWC 2013 04 05.33872 12 09 45.558 -02 49 42.85 21.7w 471150 F51 C~1vWC 2013 04 05.35306 12 09 45.475 -02 49 42.67 21.7w 471150 F51 C~1vWC 2013 04 05.36743 12 09 45.401 -02 49 42.28 22.0w 471150 F51 C~1vWC 2013 04 05.38186 12 09 45.337 -02 49 41.88 21.6w 471150 F51 C~1vWC 2013 12 10.63704 12 17 41.738 -04 17 53.39 21.9w 471150 F51 C~1vWC 2013 12 10.64164 12 17 41.753 -04 17 53.35 22.1w 471150 F51 C~1vWC 2013 12 10.64627 12 17 41.779 -04 17 53.40 21.9w 471150 F51 C~1vWC 2014 02 26.50983 12 15 35.327 -04 21 25.24 21.7w 471150 F51 C~1vWC 2014 02 26.52220 12 15 35.271 -04 21 24.82 21.7w 471150 F51 C~1vWC 2014 02 26.53456 12 15 35.217 -04 21 24.76 21.8w 471150 F51 C~1vWC 2014 02 26.54693 12 15 35.157 -04 21 24.49 21.7w 471150 F51 C~1vWC 2014 03 27.11144 12 13 12.15 -04 11 12.3 22.1V 471150 W84 C~2Jbr 2014 03 27.18581 12 13 11.76 -04 11 10.5 471150 W84 C~2Jbr 2014 03 27.24898 12 13 11.43 -04 11 09.1 471150 W84 C~2Jbr 2014 05 25.32971 12 09 08.646 -03 52 34.31 21.8w 471150 F51 C~1vWC 2014 05 25.34113 12 09 08.608 -03 52 34.19 22.0w 471150 F51 C~1vWC 2014 05 25.35257 12 09 08.590 -03 52 34.15 21.8w 471150 F51 C~1vWC 2014 05 25.36403 12 09 08.563 -03 52 34.04 21.8w 471150 F51 C~1vWC 2014 06 16.26716 12 08 40.303 -03 51 33.10 22.1w 471150 F51 C~1vWC 2014 06 16.27925 12 08 40.297 -03 51 33.61 22.1w 471150 F51 C~1vWC 2014 06 16.29100 12 08 40.270 -03 51 33.21 22.1w 471150 F51 C~1vWC 2014 06 16.30244 12 08 40.288 -03 51 33.53 22.1w 471150 F51 C~1vWC 2015 01 23.53849 12 20 13.398 -05 43 51.76 22.0w 471150 F51 C~1vWC 2015 01 23.55383 12 20 13.362 -05 43 51.82 22.0w 471150 F51 C~1vWC 2015 01 23.56921 12 20 13.324 -05 43 51.78 21.9w 471150 F51 C~1vWC 2015 01 23.58462 12 20 13.295 -05 43 51.86 21.9w 471150 F51 C~1vWC 2015 02 16.50041 12 18 58.632 -05 41 33.85 21.8w 471150 F51 C~1vWC 2015 02 16.51313 12 18 58.573 -05 41 33.69 21.8w 471150 F51 C~1vWC 2015 02 16.52582 12 18 58.514 -05 41 33.46 21.7w 471150 F51 C~1vWC 2015 02 16.53850 12 18 58.478 -05 41 33.33 21.9w 471150 F51 C~1vWC 2015 05 23.26508 12 11 50.825 -05 10 03.19 21.6i 471150 F51 C~1vWC 2015 05 23.27717 12 11 50.783 -05 10 03.05 21.4i 471150 F51 C~1vWC 2015 05 23.28926 12 11 50.774 -05 10 02.74 21.3i 471150 F51 C~1vWC 2015 05 23.30136 12 11 50.735 -05 10 02.82 21.5i 471150 F51 C~1vWC
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 -0.11 0.00 0.47 2 0.0000 0.00 -0.32 0.00 -0.09 3 0.0000 0.00 -0.21 0.00 -0.08 4 3.0720 0.00 0.06 0.00 0.10 5 3.0720 0.00 0.08 0.00 0.09 6 3.0720 0.00 0.13 0.00 0.08 7 4.3415 0.00 -0.21 0.00 -0.21 8 4.3415 0.00 -0.15 0.00 -0.13 9 4.3415 0.00 -0.13 0.00 -0.17 10 7.2651 0.00 -0.36 0.00 -0.27 11 7.2654 0.00 0.07 0.00 -0.14 12 7.2656 0.00 -0.20 0.00 1.03 13 7.2679 0.00 0.47 0.00 -0.73 14 7.2681 0.00 0.56 0.00 -0.26 15 7.2683 0.00 0.32 0.00 -0.42 16 7.2706 0.00 0.18 0.00 -0.18 17 7.2708 0.00 0.38 0.00 0.03 18 7.2711 0.00 0.55 0.00 1.06 19 7.2733 0.00 0.23 0.00 -0.14 20 7.2736 0.00 0.35 0.00 -0.43 21 7.2738 0.00 0.16 0.00 1.09 22 7.3171 0.00 1.04 0.00 -0.03 23 7.3173 0.00 0.69 0.00 0.32 24 7.3583 0.00 -0.07 0.00 -0.00 25 7.3585 0.00 -0.28 0.00 0.07 26 7.4813 0.00 0.73 0.00 0.45 27 7.4816 0.00 0.61 0.00 0.11 28 8.0820 0.00 -0.06 0.00 -0.23 29 8.0822 0.00 0.15 0.00 -0.25 30 8.0823 0.00 -0.14 0.00 0.01 31 8.2408 0.00 -0.61 0.00 0.37 32 8.2409 0.00 -0.34 0.00 0.24 33 8.9751 0.00 -0.16 0.00 -0.28 34 8.9751 0.00 -0.37 0.00 -0.16 35 8.9751 0.00 -0.22 0.00 -0.21 36 8.9751 0.00 -0.20 0.00 0.09 37 9.2049 0.00 0.17 0.00 -0.03 38 9.2049 0.00 0.17 0.00 -0.33 39 9.2049 0.00 0.03 0.00 -0.11 40 9.2129 0.00 0.16 0.00 -0.07 41 9.2129 0.00 0.17 0.00 -0.00 42 9.2129 0.00 0.11 0.00 -0.02 43 9.2130 0.00 0.20 0.00 -0.12 44 9.3412 0.00 0.03 0.00 -0.10 45 9.3412 0.00 -0.04 0.00 -0.10 46 9.3412 0.00 -0.01 0.00 -0.06 47 9.3413 0.00 0.05 0.00 -0.09 48 10.2340 0.00 0.10 0.00 -0.18 49 10.2340 0.00 -0.05 0.00 -0.18 50 10.2340 0.00 -0.04 0.00 -0.19 51 10.2341 0.00 0.04 0.00 -0.05 52 10.3159 0.00 -0.08 0.00 -0.01 53 10.3159 0.00 -0.23 0.00 -0.17 54 10.3159 0.00 -0.23 0.00 -0.11 55 10.3160 0.00 -0.08 0.00 -0.05 56 10.9984 0.00 -0.21 0.00 -0.05 57 10.9984 0.00 -0.11 0.00 0.11 58 10.9984 0.00 0.15 0.00 0.17 59 11.2116 0.00 -0.02 0.00 -0.07 60 11.2116 0.00 0.01 0.00 0.13 61 11.2117 0.00 0.07 0.00 -0.03 62 11.2117 0.00 0.03 0.00 0.03 63 11.2899 0.00 -0.12 0.00 -0.14 64 11.2901 0.00 -0.09 0.00 -0.10 65 11.2903 0.00 -0.05 0.00 -0.20 66 11.4520 0.00 -0.05 0.00 -0.00 67 11.4521 0.00 -0.22 0.00 0.02 68 11.4521 0.00 -0.09 0.00 -0.04 69 11.4521 0.00 -0.10 0.00 -0.03 70 11.5121 0.00 0.07 0.00 0.48 71 11.5121 0.00 0.05 0.00 0.01 72 11.5122 0.00 -0.29 0.00 0.45 73 11.5122 0.00 0.05 0.00 0.17 74 12.1179 0.00 0.21 0.00 0.02 75 12.1179 0.00 0.18 0.00 -0.02 76 12.1180 0.00 0.12 0.00 0.04 77 12.1180 0.00 0.20 0.00 -0.02 78 12.1835 0.00 0.19 0.00 0.00 79 12.1835 0.00 0.09 0.00 0.01 80 12.1836 0.00 -0.02 0.00 0.08 81 12.1836 0.00 0.22 0.00 0.06 82 12.4457 0.00 -0.03 0.00 -0.16 83 12.4457 0.00 -0.19 0.00 -0.15 84 12.4458 0.00 0.15 0.00 0.02 85 12.4458 0.00 0.03 0.00 -0.20
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.
471150 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 38.865 38.865 38.865 ecceobj 0.052 0.052 0.052 incobj 39.842 39.842 39.842 qmin 36.545 36.549 36.556 qmax 41.622 41.633 41.627 amean 39.002 39.001 39.002 amin 38.721 38.729 38.707 amax 39.307 39.302 39.294 emean 0.050 0.050 0.050 emin 0.040 0.040 0.040 emax 0.059 0.060 0.060 imean 40.087 40.087 40.087 imin 39.807 39.805 39.807 imax 40.355 40.346 40.348 excite_mean 0.646 0.646 0.646 fracstop 1.000 1.000 1.000 cjmean 2.510 2.510 2.510 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 175.4 175.2 175.2 kozaiamp 180.0 179.9 179.9