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: 13MR18 # Created Sat Apr 20 01:14:40 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 132 observations of 132 # Arc: 11.13y # First observation: 2011/04/14 # Last observation: 2022/06/02 # Chi-squared of fit: 126.40 DOF: 258 RMS: 0.17 # Min/Max residuals: -0.69 0.60 # Exact a, adot, b, bdot, g, gdot: 1.857341E-05 3.950696E-02 6.826253E-06 1.425758E-02 3.409534E-02 -1.053753E-02 # Covariance matrix: 1.9745E-13 -5.5612E-14 4.4233E-14 -1.6756E-14 -2.1962E-14 -8.1174E-14 -5.5612E-14 1.9240E-14 -1.7014E-14 6.5046E-15 1.1267E-14 3.1236E-14 4.4233E-14 -1.7014E-14 9.6596E-14 -1.6525E-14 -7.4687E-15 -3.0585E-14 -1.6756E-14 6.5046E-15 -1.6525E-14 3.8696E-15 3.5274E-15 1.1558E-14 -2.1962E-14 1.1267E-14 -7.4687E-15 3.5274E-15 3.6822E-14 1.3852E-14 -8.1174E-14 3.1236E-14 -3.0585E-14 1.1558E-14 1.3852E-14 5.6122E-14 # lat0 lon0 xBary yBary zBary JD0 25.205957 -142.415098 0.237015 0.416572 -0.885156 2455666.018179 # Heliocentric elements and errors Epoch: 2455666.5000 = 2011/04/15 Mean Anomaly: 327.18182 +/- 0.002 Argument of Peri: 116.72820 +/- 0.002 Long of Asc Node: 168.37527 +/- 0.000 Inclination: 31.13654 +/- 0.000 Eccentricity: 0.33983718 +/- 0.0000 Semi-Major Axis: 39.31385520 +/- 0.0012 Time of Perihelion: 2463874.3395 +/- 3.7 Perihelion: 25.95354538 +/- 0.0009 Aphelion: 52.67416502 +/- 0.0016 Period (y) 246.5055 +/- 0.01 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -21.94449448 +/- 0.0001 Ecliptic Y -16.59511589 +/- 0.0001 Ecliptic Z 12.49088521 +/- 0.0001 Ecliptic XDOT 0.00292628 +/- 0.0000 Ecliptic YDOT -0.00174365 +/- 0.0000 Ecliptic ZDOT 0.00067554 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 30.21572397 +/- 0.0001 Geocenter to KBO 29.32970169 +/- 0.0002 # Hcoef: 7.89
The following table shows the complete astrometric record for 13MR18. 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 (13MR18) followed by the observatory code and reference code for the source of the astrometry.
2011 04 14.517413 14 53 12.629 +09 51 30.26 23.1G 13MR18 F51 C~435k 2011 04 14.528896 14 53 12.566 +09 51 31.01 22.3G 13MR18 F51 C~435k 2011 04 14.541736 14 53 12.494 +09 51 31.78 21.9G 13MR18 F51 C~435k 2011 04 14.552397 14 53 12.387 +09 51 31.47 21.3G 13MR18 F51 C~435k 2013 06 16.267989 15 06 55.841 +10 20 52.41 22.0G 13MR18 F51 C~435k 2013 06 16.277975 15 06 55.777 +10 20 52.94 22.5G 13MR18 F51 C~435k 2013 06 17.283300 15 06 51.036 +10 20 43.03 22.5G 13MR18 F51 C~435k 2014 04 28.522185 15 22 03.663 +10 07 28.25 22.4G 13MR18 F51 C~435k 2014 04 28.534020 15 22 03.620 +10 07 29.11 21.9G 13MR18 F51 C~435k 2014 04 28.545869 15 22 03.519 +10 07 29.16 22.4G 13MR18 F51 C~435k 2014 04 28.557891 15 22 03.479 +10 07 29.38 22.4G 13MR18 F51 C~435k 2014 05 17.492657 15 20 03.700 +10 18 11.44 22.6G 13MR18 F51 C~435k 2014 05 17.530413 15 20 03.480 +10 18 12.34 22.2G 13MR18 F51 C~435k 2014 05 24.457344 15 19 19.668 +10 20 36.09 22.7G 13MR18 F51 C~435k 2014 05 24.470072 15 19 19.576 +10 20 36.21 22.5G 13MR18 F51 C~435k 2014 05 24.482753 15 19 19.502 +10 20 36.39 22.6G 13MR18 F51 C~435k 2015 02 17.587946 15 35 56.436 +08 57 09.69 22.3G 13MR18 F51 C~435k 2015 02 17.600227 15 35 56.443 +08 57 10.16 22.6G 13MR18 F51 C~435k 2015 02 17.612632 15 35 56.463 +08 57 11.27 22.4G 13MR18 F51 C~435k 2015 02 17.624996 15 35 56.491 +08 57 11.89 22.5G 13MR18 F51 C~435k 2015 02 18.586707 15 35 57.863 +08 58 08.92 23.1G 13MR18 F51 C~435k 2015 02 18.599019 15 35 57.877 +08 58 09.85 22.1G 13MR18 F51 C~435k 2015 02 18.611388 15 35 57.886 +08 58 10.41 21.9G 13MR18 F51 C~435k 2015 02 18.623797 15 35 57.898 +08 58 11.29 22.2G 13MR18 F51 C~435k 2015 03 31.492028 15 35 00.696 +09 41 26.75 21.6G 13MR18 F51 C~435k 2015 06 05.432519 15 28 37.310 +10 22 43.62 22.4G 13MR18 F51 C~435k 2015 06 05.445483 15 28 37.228 +10 22 43.67 22.2G 13MR18 F51 C~435k 2015 06 05.458391 15 28 37.131 +10 22 43.48 22.5G 13MR18 F51 C~435k 2015 06 05.471368 15 28 37.096 +10 22 43.84 22.4G 13MR18 F51 C~435k 2016 04 09.595967 15 45 00.055 +09 49 03.05 21.4G 13MR18 F51 C~435k 2016 04 09.605904 15 44 59.999 +09 49 03.77 21.9G 13MR18 F51 C~435k 2016 04 09.615815 15 44 59.929 +09 49 04.43 22.2G 13MR18 F51 C~435k 2016 04 09.625718 15 44 59.888 +09 49 05.12 22.3G 13MR18 F51 C~435k 2016 04 15.587525 15 44 30.434 +09 54 40.99 21.8G 13MR18 F51 C~435k 2016 04 15.599367 15 44 30.372 +09 54 41.78 22.1G 13MR18 F51 C~435k 2016 04 16.590374 15 44 25.170 +09 55 35.50 22.6G 13MR18 F51 C~435k 2016 04 16.600249 15 44 25.130 +09 55 36.21 21.8G 13MR18 F51 C~435k 2016 04 16.610146 15 44 25.057 +09 55 36.55 22.5G 13MR18 F51 C~435k 2016 04 16.620042 15 44 24.997 +09 55 37.12 23.1G 13MR18 F51 C~435k 2016 06 03.310724 15 39 28.220 +10 21 25.08 22.5G 13MR18 F51 C~435k 2016 06 03.312108 15 39 28.208 +10 21 24.96 21.9G 13MR18 F51 C~435k 2016 06 03.322186 15 39 28.133 +10 21 25.33 22.5G 13MR18 F51 C~435k 2016 06 03.323636 15 39 28.138 +10 21 24.86 21.7G 13MR18 F51 C~435k 2016 06 03.333694 15 39 28.082 +10 21 25.06 22.7G 13MR18 F51 C~435k 2016 06 03.335101 15 39 28.078 +10 21 25.23 22.8G 13MR18 F51 C~435k 2016 06 03.345199 15 39 27.987 +10 21 25.79 22.6G 13MR18 F51 C~435k 2016 06 03.346630 15 39 27.985 +10 21 25.21 22.8G 13MR18 F51 C~435k 2016 06 10.303609 15 38 45.856 +10 21 47.68 22.1G 13MR18 F51 C~435k 2016 06 10.314730 15 38 45.785 +10 21 47.76 22.2G 13MR18 F51 C~435k 2016 06 10.325950 15 38 45.729 +10 21 47.69 22.5G 13MR18 F51 C~435k 2016 06 10.335940 15 38 45.665 +10 21 47.61 22.2G 13MR18 F51 C~435k 2017 04 20.585639 15 55 02.154 +09 55 36.17 22.6G 13MR18 F51 C~435k 2017 04 20.596215 15 55 02.112 +09 55 36.67 22.4G 13MR18 F51 C~435k 2017 04 20.603739 15 55 02.058 +09 55 36.96 22.2G 13MR18 F51 C~435k 2017 04 20.611334 15 55 02.014 +09 55 37.73 22.5G 13MR18 F51 C~435k 2017 05 17.463338 15 52 16.707 +10 13 50.42 22.1G 13MR18 F51 C~435k 2017 05 17.474755 15 52 16.621 +10 13 50.44 22.8G 13MR18 F51 C~435k 2017 05 17.486159 15 52 16.538 +10 13 50.99 22.0G 13MR18 F51 C~435k 2017 05 17.497544 15 52 16.443 +10 13 50.91 22.2G 13MR18 F51 C~435k 2017 05 31.478060 15 50 44.437 +10 18 26.93 22.2G 13MR18 F51 C~435k 2017 05 31.489071 15 50 44.385 +10 18 26.86 22.0G 13MR18 F51 C~435k 2017 05 31.500028 15 50 44.291 +10 18 27.18 21.7G 13MR18 F51 C~435k 2017 05 31.511050 15 50 44.235 +10 18 27.25 22.1G 13MR18 F51 C~435k 2018 06 14.434428 16 00 27.059 +10 15 42.65 22.6G 13MR18 F51 C~435k 2018 06 14.446528 16 00 27.002 +10 15 42.88 22.5G 13MR18 F51 C~435k 2018 06 14.458633 16 00 26.918 +10 15 42.45 22.3G 13MR18 F51 C~435k 2018 06 14.470712 16 00 26.838 +10 15 42.41 22.4G 13MR18 F51 C~435k 2019 05 09.540502 16 15 46.770 +09 59 32.92 23.1G 13MR18 F51 C~435k 2019 05 09.546948 16 15 46.742 +09 59 33.44 22.3G 13MR18 F51 C~435k 2019 05 09.553395 16 15 46.695 +09 59 33.59 22.3G 13MR18 F51 C~435k 2019 05 09.559838 16 15 46.664 +09 59 34.14 22.7G 13MR18 F51 C~435k 2019 05 12.527521 16 15 27.632 +10 01 23.81 22.0G 13MR18 F51 C~435k 2019 05 12.539693 16 15 27.560 +10 01 24.45 21.6G 13MR18 F51 C~435k 2019 05 12.551903 16 15 27.494 +10 01 24.60 21.8G 13MR18 F51 C~435k 2019 05 12.564162 16 15 27.392 +10 01 25.04 22.1G 13MR18 F51 C~435k 2019 06 01.461615 16 13 14.494 +10 09 35.24 22.8G 13MR18 F52 C~435k 2019 06 01.472657 16 13 14.424 +10 09 35.11 22.3G 13MR18 F52 C~435k 2019 06 01.483659 16 13 14.346 +10 09 35.43 21.9G 13MR18 F52 C~435k 2019 06 01.494782 16 13 14.269 +10 09 35.59 22.2G 13MR18 F52 C~435k 2019 06 07.473718 16 12 34.448 +10 10 33.42 22.7G 13MR18 F51 C~435k 2019 06 07.485681 16 12 34.381 +10 10 33.60 22.2G 13MR18 F51 C~435k 2019 06 07.497595 16 12 34.282 +10 10 33.46 22.8G 13MR18 F51 C~435k 2019 06 07.509498 16 12 34.211 +10 10 33.56 22.6G 13MR18 F51 C~435k 2019 06 30.409118 16 10 16.265 +10 07 42.46 22.1G 13MR18 F51 C~435k 2019 06 30.421190 16 10 16.197 +10 07 42.19 22.4G 13MR18 F51 C~435k 2019 06 30.433330 16 10 16.133 +10 07 41.94 22.4G 13MR18 F51 C~435k 2019 06 30.445439 16 10 16.062 +10 07 41.69 22.5G 13MR18 F51 C~435k 2019 07 06.377339 16 09 46.400 +10 05 18.88 22.1G 13MR18 F52 C~435k 2019 07 06.389646 16 09 46.340 +10 05 18.60 21.7G 13MR18 F52 C~435k 2019 07 25.329695 16 08 35.799 +09 53 42.32 22.0G 13MR18 F51 C~435k 2019 07 25.341820 16 08 35.766 +09 53 41.78 22.5G 13MR18 F51 C~435k 2019 07 25.353909 16 08 35.746 +09 53 41.24 22.1G 13MR18 F51 C~435k 2019 07 25.365970 16 08 35.703 +09 53 40.79 22.7G 13MR18 F51 C~435k 2019 08 22.252329 16 08 13.711 +09 27 59.51 21.9G 13MR18 F51 C~435k 2019 08 22.252969 16 08 13.686 +09 27 59.57 22.0G 13MR18 F51 C~435k 2019 08 22.264078 16 08 13.707 +09 27 58.72 22.3G 13MR18 F51 C~435k 2019 08 22.264716 16 08 13.723 +09 27 58.64 23.0G 13MR18 F51 C~435k 2019 08 22.275801 16 08 13.709 +09 27 58.17 22.2G 13MR18 F51 C~435k 2019 08 22.276441 16 08 13.738 +09 27 57.63 22.0G 13MR18 F51 C~435k 2019 08 22.287591 16 08 13.747 +09 27 57.78 22.2G 13MR18 F51 C~435k 2019 08 22.288228 16 08 13.725 +09 27 57.46 22.0G 13MR18 F51 C~435k 2020 04 27.587473 16 28 28.359 +09 44 11.71 22.0G 13MR18 F51 C~435k 2020 04 27.596322 16 28 28.309 +09 44 12.12 22.4G 13MR18 F51 C~435k 2020 04 27.605110 16 28 28.268 +09 44 12.67 22.3G 13MR18 F51 C~435k 2020 04 27.614040 16 28 28.206 +09 44 13.04 22.2G 13MR18 F51 C~435k 2020 05 03.558087 16 27 54.135 +09 48 54.17 21.9G 13MR18 F51 C~435k 2020 05 03.570566 16 27 54.079 +09 48 54.57 22.4G 13MR18 F51 C~435k 2020 05 03.583046 16 27 53.987 +09 48 54.94 23.2G 13MR18 F51 C~435k 2020 05 03.595502 16 27 53.900 +09 48 55.95 22.3G 13MR18 F51 C~435k 2020 05 17.382211 16 26 26.674 +09 57 38.31 22.8G 13MR18 F51 C~435k 2020 05 17.393837 16 26 26.626 +09 57 38.53 22.6G 13MR18 F51 C~435k 2020 05 17.405480 16 26 26.535 +09 57 38.79 22.9G 13MR18 F51 C~435k 2020 05 17.417219 16 26 26.411 +09 57 38.90 22.8G 13MR18 F51 C~435k 2020 05 19.501109 16 26 12.555 +09 58 40.83 22.1G 13MR18 F51 C~435k 2020 05 19.513001 16 26 12.475 +09 58 41.11 22.2G 13MR18 F51 C~435k 2020 05 19.524770 16 26 12.393 +09 58 41.41 22.3G 13MR18 F51 C~435k 2020 05 19.536555 16 26 12.307 +09 58 41.92 22.0G 13MR18 F51 C~435k 2020 05 23.514014 16 25 45.518 +10 00 25.88 21.9G 13MR18 F52 C~435k 2020 05 23.525888 16 25 45.389 +10 00 26.23 21.7G 13MR18 F52 C~435k 2020 05 28.508574 16 25 11.511 +10 02 10.77 22.2G 13MR18 F51 C~435k 2020 05 28.520380 16 25 11.424 +10 02 10.95 21.9G 13MR18 F51 C~435k 2020 05 28.532169 16 25 11.346 +10 02 11.19 21.6G 13MR18 F51 C~435k 2020 05 28.543912 16 25 11.279 +10 02 11.39 21.4G 13MR18 F51 C~435k 2021 07 09.230100 16 32 36.831 +09 50 14.58 22.3G 13MR18 G37 C~4uuK 2021 07 09.262630 16 32 36.666 +09 50 13.67 13MR18 G37 C~4uuK 2021 07 09.295530 16 32 36.491 +09 50 12.32 13MR18 G37 C~4uuK 2021 08 08.318809 16 30 55.357 +09 28 03.84 22.0w 13MR18 F51 C~4xR2 2021 08 08.331317 16 30 55.326 +09 28 03.25 22.5w 13MR18 F51 C~4xR2 2021 08 08.343928 16 30 55.300 +09 28 02.28 22.3w 13MR18 F51 C~4xR2 2022 06 02.356742 16 48 25.395 +09 45 52.61 22.0w 13MR18 F52 C~5fiq 2022 06 02.380156 16 48 25.242 +09 45 52.68 21.8w 13MR18 F52 C~5fiq 2022 06 02.391938 16 48 25.154 +09 45 52.88 22.1w 13MR18 F52 C~5fiq
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 -0.03
2 0.0000 0.00 -0.02 0.00 0.15
3 0.0001 0.00 -0.00 0.00 0.28
4 0.0001 0.00 -0.69 0.00 -0.56
5 2.1732 0.00 0.44 0.00 -0.28
6 2.1732 0.00 0.21 0.00 0.34
7 2.1760 0.00 0.18 0.00 -0.05
8 3.0390 0.00 0.02 0.00 0.09
9 3.0391 0.00 0.48 0.00 0.44
10 3.0391 0.00 0.07 0.00 -0.01
11 3.0391 0.00 0.60 0.00 -0.30
12 3.0910 0.00 -0.13 0.00 0.09
13 3.0911 0.00 0.24 0.00 0.07
14 3.1100 0.00 0.05 0.00 0.08
15 3.1101 0.00 -0.12 0.00 -0.02
16 3.1101 0.00 -0.02 0.00 -0.05
17 3.8469 0.00 0.08 0.00 0.00
18 3.8469 0.00 -0.07 0.00 -0.25
19 3.8469 0.00 -0.03 0.00 0.12
20 3.8470 0.00 0.13 0.00 0.01
21 3.8496 0.00 0.07 0.00 -0.11
22 3.8496 0.00 0.04 0.00 0.08
23 3.8497 0.00 -0.05 0.00 -0.10
24 3.8497 0.00 -0.10 0.00 0.04
25 3.9616 0.00 0.21 0.00 -0.00
26 4.1421 0.00 -0.06 0.00 0.05
27 4.1422 0.00 -0.11 0.00 0.04
28 4.1422 0.00 -0.39 0.00 -0.21
29 4.1422 0.00 0.27 0.00 0.09
30 4.9886 0.00 0.11 0.00 -0.05
31 4.9886 0.00 -0.02 0.00 0.09
32 4.9886 0.00 -0.35 0.00 0.18
33 4.9887 0.00 -0.26 0.00 0.29
34 5.0050 0.00 0.16 0.00 -0.23
35 5.0050 0.00 0.17 0.00 -0.09
36 5.0077 0.00 -0.03 0.00 -0.09
37 5.0078 0.00 0.16 0.00 0.09
38 5.0078 0.00 -0.13 0.00 -0.11
39 5.0078 0.00 -0.23 0.00 -0.07
40 5.1384 0.00 -0.04 0.00 0.06
41 5.1384 0.00 -0.09 0.00 -0.07
42 5.1384 0.00 -0.26 0.00 0.23
43 5.1384 0.00 -0.04 0.00 -0.26
44 5.1384 0.00 0.07 0.00 -0.13
45 5.1384 0.00 0.15 0.00 0.03
46 5.1385 0.00 -0.26 0.00 0.52
47 5.1385 0.00 -0.15 0.00 -0.07
48 5.1575 0.00 -0.02 0.00 0.05
49 5.1576 0.00 -0.09 0.00 0.14
50 5.1576 0.00 0.08 0.00 0.08
51 5.1576 0.00 0.02 0.00 0.00
52 6.0180 0.00 -0.11 0.00 -0.07
53 6.0180 0.00 0.14 0.00 -0.12
54 6.0180 0.00 -0.05 0.00 -0.22
55 6.0181 0.00 -0.08 0.00 0.15
56 6.0916 0.00 0.13 0.00 0.06
57 6.0916 0.00 -0.01 0.00 -0.23
58 6.0916 0.00 -0.10 0.00 0.01
59 6.0917 0.00 -0.38 0.00 -0.39
60 6.1299 0.00 -0.16 0.00 0.18
61 6.1300 0.00 0.15 0.00 -0.02
62 6.1300 0.00 -0.18 0.00 0.17
63 6.1300 0.00 0.07 0.00 0.12
64 7.1675 0.00 -0.10 0.00 0.00
65 7.1675 0.00 0.17 0.00 0.27
66 7.1675 0.00 0.04 0.00 -0.11
67 7.1676 0.00 -0.03 0.00 -0.11
68 8.0685 0.00 -0.22 0.00 -0.22
69 8.0685 0.00 -0.01 0.00 0.06
70 8.0685 0.00 -0.09 0.00 -0.04
71 8.0686 0.00 0.07 0.00 0.26
72 8.0767 0.00 -0.16 0.00 0.05
73 8.0767 0.00 -0.04 0.00 0.26
74 8.0768 0.00 0.18 0.00 -0.02
75 8.0768 0.00 -0.14 0.00 -0.01
76 8.1313 0.00 -0.08 0.00 0.16
77 8.1313 0.00 0.00 0.00 -0.11
78 8.1313 0.00 -0.04 0.00 0.06
79 8.1314 0.00 -0.05 0.00 0.08
80 8.1477 0.00 -0.05 0.00 0.01
81 8.1478 0.00 0.15 0.00 0.12
82 8.1478 0.00 -0.14 0.00 -0.09
83 8.1478 0.00 -0.01 0.00 -0.06
84 8.2105 0.00 0.03 0.00 -0.01
85 8.2106 0.00 -0.02 0.00 -0.03
86 8.2106 0.00 0.00 0.00 -0.02
87 8.2106 0.00 -0.09 0.00 -0.02
88 8.2269 0.00 -0.06 0.00 -0.08
89 8.2269 0.00 -0.06 0.00 -0.02
90 8.2787 0.00 -0.06 0.00 -0.10
91 8.2788 0.00 -0.05 0.00 -0.09
92 8.2788 0.00 0.15 0.00 -0.08
93 8.2788 0.00 -0.00 0.00 0.03
94 8.3552 0.00 0.21 0.00 -0.08
95 8.3552 0.00 -0.17 0.00 0.02
96 8.3552 0.00 -0.03 0.00 -0.13
97 8.3552 0.00 0.20 0.00 -0.17
98 8.3553 0.00 -0.17 0.00 0.06
99 8.3553 0.00 0.25 0.00 -0.44
100 8.3553 0.00 0.21 0.00 0.41
101 8.3553 0.00 -0.13 0.00 0.13
102 9.0378 0.00 0.09 0.00 -0.05
103 9.0379 0.00 0.09 0.00 -0.08
104 9.0379 0.00 0.21 0.00 0.03
105 9.0379 0.00 0.03 0.00 -0.04
106 9.0542 0.00 -0.01 0.00 -0.02
107 9.0542 0.00 0.29 0.00 -0.18
108 9.0543 0.00 0.04 0.00 -0.36
109 9.0543 0.00 -0.13 0.00 0.10
110 9.0920 0.00 -0.27 0.00 0.29
111 9.0921 0.00 0.19 0.00 0.15
112 9.0921 0.00 0.00 0.00 0.05
113 9.0921 0.00 -0.67 0.00 -0.21
114 9.0978 0.00 0.02 0.00 0.08
115 9.0979 0.00 0.04 0.00 0.02
116 9.0979 0.00 0.01 0.00 -0.01
117 9.0979 0.00 -0.08 0.00 0.17
118 9.1088 0.00 0.28 0.00 0.07
119 9.1089 0.00 -0.42 0.00 0.13
120 9.1225 0.00 0.05 0.00 -0.00
121 9.1225 0.00 -0.02 0.00 -0.04
122 9.1226 0.00 0.03 0.00 -0.01
123 9.1226 0.00 0.25 0.00 -0.02
124 10.2360 0.00 0.05 0.00 -0.04
125 10.2361 0.00 0.08 0.00 0.03
126 10.2362 0.00 -0.01 0.00 -0.33
127 10.3184 0.00 0.10 0.00 -0.00
128 10.3185 0.00 -0.07 0.00 0.12
129 10.3185 0.00 -0.15 0.00 -0.14
130 11.1344 0.00 -0.07 0.00 0.27
131 11.1345 0.00 0.12 0.00 -0.02
132 11.1345 0.00 0.05 0.00 0.00
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.
13MR18 quality flag:3 Type: 3:2E 3:2E 3:2E Type: 6:4II 6:4II 6:4II axisobj 39.174 39.174 39.175 ecceobj 0.338 0.338 0.338 incobj 31.164 31.164 31.164 qmin 24.984 24.985 24.983 qmax 54.511 54.510 54.512 amean 39.453 39.453 39.453 amin 39.108 39.109 39.108 amax 39.908 39.909 39.908 emean 0.282 0.282 0.282 emin 0.183 0.183 0.183 emax 0.366 0.366 0.366 imean 32.114 32.114 32.114 imin 29.595 29.595 29.595 imax 34.446 34.445 34.446 excite_mean 0.605 0.605 0.605 fracstop 1.000 1.000 1.000 cjmean 2.620 2.620 2.620 libcent 0 180.5 180.5 180.5 libamp 0 18.5 18.6 18.4 libcent 1 178.5 178.5 178.6 libamp 1 95.8 96.2 95.5 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 93.8 93.8 93.8 kozaiamp 48.0 48.0 48.0