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: 437313 # Created Fri Nov 22 02:07:05 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 99 observations of 99 # Arc: 3.31y # First observation: 2012/02/22 # Last observation: 2015/06/15 # Chi-squared of fit: 297.70 DOF: 192 RMS: 0.31 # Min/Max residuals: -1.07 1.05 # Exact a, adot, b, bdot, g, gdot: 4.323238E-05 5.263492E-01 7.141212E-06 8.402680E-02 1.865333E-01 -2.125812E-01 # 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 -0.638687 135.079550 -0.307910 -0.010488 -0.942061 2455979.924656 # Heliocentric elements and errors Epoch: 2455980.5000 = 2012/02/23 Mean Anomaly: 347.40414 +/- 0.000 Argument of Peri: 49.33551 +/- 0.000 Long of Asc Node: 141.28029 +/- 0.000 Inclination: 8.99008 +/- 0.000 Eccentricity: 0.58296504 +/- 0.0000 Semi-Major Axis: 12.92544184 +/- 0.0000 Time of Perihelion: 2456574.3706 +/- 0.0 Perihelion: 5.39036108 +/- 0.0000 Aphelion: 20.46052259 +/- 0.0000 Period (y) 46.4704 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -4.67748699 +/- 0.0000 Ecliptic Y 4.23390443 +/- 0.0000 Ecliptic Z -0.05972903 +/- 0.0000 Ecliptic XDOT -0.00326038 +/- 0.0000 Ecliptic YDOT -0.00765955 +/- 0.0000 Ecliptic ZDOT 0.00126811 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 6.30947232 +/- 0.0000 Geocenter to KBO 5.36111289 +/- 0.0000 # Hcoef: 12.99
The following table shows the complete astrometric record for 437313. 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 (437313) followed by the observatory code and reference code for the source of the astrometry.
2012 02 22.42389 09 09 23.693 +15 42 07.52 21.2w 437313 F51 C~1w0Y 2012 02 22.44073 09 09 23.307 +15 42 10.42 21.1w 437313 F51 C~1w0Y 2012 02 22.45753 09 09 22.941 +15 42 12.48 21.2w 437313 F51 C~1w0Y 2012 02 22.47431 09 09 22.562 +15 42 15.09 21.2w 437313 F51 C~1w0Y 2012 02 24.22522 09 08 45.16 +15 46 30.9 20.9V 437313 G96 C~0qCg 2012 02 24.23377 09 08 44.95 +15 46 32.7 21.0V 437313 G96 C~0qCg 2012 02 24.24234 09 08 44.77 +15 46 33.5 21.2V 437313 G96 C~0qCg 2012 02 24.25096 09 08 44.52 +15 46 35.1 20.6V 437313 G96 C~0qCg 2012 03 17.17921 09 02 32.02 +16 32 32.4 21.1V 437313 G96 C~0qCg 2012 03 17.18722 09 02 31.95 +16 32 33.2 21.2V 437313 G96 C~0qCg 2012 03 17.19532 09 02 31.84 +16 32 33.9 21.0V 437313 G96 C~0qCg 2012 03 17.20340 09 02 31.74 +16 32 34.9 21.3V 437313 G96 C~0qCg 2013 02 05.42399 11 39 44.61 +07 07 59.4 20.7V 437313 691 C~0qCg 2013 02 05.44167 11 39 44.41 +07 08 02.2 20.5V 437313 691 C~0qCg 2013 02 05.45933 11 39 44.20 +07 08 05.1 20.5V 437313 691 C~0qCg 2013 02 12.17100 11 38 18.23 +07 27 55.8 20.5R 437313 J04 C~0qCg 2013 02 12.18257 11 38 18.05 +07 27 57.6 20.4R 437313 J04 C~0qCg 2013 02 12.19415 11 38 17.87 +07 28 00.0 20.7R 437313 J04 C~0qCg 2013 02 12.20572 11 38 17.72 +07 28 02.2 20.5R 437313 J04 C~0qCh 2013 03 03.21404 11 32 31.39 +08 31 40.0 437313 691 C~0qCh 2013 03 03.23173 11 32 30.99 +08 31 43.5 437313 691 C~0qCh 2013 03 03.24943 11 32 30.66 +08 31 47.1 437313 691 C~0qCh 2013 03 07.42211 11 31 01.48 +08 46 12.1 19.9V 437313 G96 C~0ptK 2013 03 07.42953 11 31 01.34 +08 46 13.8 20.2V 437313 G96 C~0ptK 2013 03 07.43707 11 31 01.20 +08 46 15.1 20.1V 437313 G96 C~0ptK 2013 03 07.44459 11 31 00.98 +08 46 17.1 20.1V 437313 G96 C~0ptK 2013 03 14.34885 11 28 30.21 +09 09 37.2 19.9V 437313 G96 C~0ptK 2013 03 14.35470 11 28 30.10 +09 09 38.3 20.1V 437313 G96 C~0ptK 2013 03 14.36063 11 28 29.96 +09 09 39.4 20.0V 437313 G96 C~0ptK 2013 03 14.36654 11 28 29.82 +09 09 40.4 20.2V 437313 G96 C~0ptK 2013 04 04.21436 11 21 26.94 +10 09 32.1 437313 H06 C~0rVe 2013 04 04.21679 11 21 26.89 +10 09 32.4 437313 H06 C~0rVe 2013 04 04.21922 11 21 26.83 +10 09 32.3 20.1V 437313 H06 C~0rVe 2014 02 14.47346 14 14 00.11 -04 16 34.2 20.4R 437313 926 C~10rX 2014 02 14.49876 14 14 00.37 -04 16 32.3 20.6R 437313 926 C~10rX 2014 02 14.53487 14 14 00.58 -04 16 28.3 20.8R 437313 926 C~10rX 2014 03 09.43584 14 14 24.51 -03 32 20.5 20.2R 437313 H36 C~11qu 2014 03 09.44705 14 14 24.45 -03 32 19.4 20.3R 437313 H36 C~11qu 2014 03 29.27426 14 10 20.57 -02 38 17.6 20.4r 437313 G45 C~196q 2014 03 29.28568 14 10 20.41 -02 38 15.2 20.5r 437313 G45 C~196q 2014 03 29.30185 14 10 20.10 -02 38 12.0 20.6r 437313 G45 C~196q 2014 03 29.31470 14 10 19.88 -02 38 09.8 20.6r 437313 G45 C~196q 2014 03 29.32608 14 10 19.64 -02 38 08.6 20.9r 437313 G45 C~196q 2014 03 29.32615 14 10 19.59 -02 38 09.0 20.2r 437313 G45 C~196q 2014 03 29.33889 14 10 19.42 -02 38 06.1 20.4r 437313 G45 C~196q 2014 03 29.36174 14 10 19.05 -02 38 01.5 20.2r 437313 G45 C~196q 2014 03 30.28046 14 10 02.99 -02 35 24.1 20.2r 437313 G45 C~196q 2014 03 30.29195 14 10 02.78 -02 35 20.4 20.1r 437313 G45 C~196q 2014 03 30.30914 14 10 02.45 -02 35 18.1 20.3r 437313 G45 C~196q 2014 03 30.33195 14 10 02.07 -02 35 14.6 20.3r 437313 G45 C~196q 2014 03 30.33202 14 10 02.02 -02 35 15.3 19.7r 437313 G45 C~196q 2014 03 30.33336 14 10 02.07 -02 35 14.1 20.1r 437313 G45 C~196q 2014 03 30.35617 14 10 01.64 -02 35 09.7 20.4r 437313 G45 C~196q 2014 04 04.49286 14 08 25.627 -02 20 22.77 20.5w 437313 F51 C@0614 2014 04 04.50622 14 08 25.356 -02 20 20.54 20.5w 437313 F51 C@0614 2014 04 04.51959 14 08 25.084 -02 20 18.16 20.4w 437313 F51 C@0614 2014 04 04.53301 14 08 24.810 -02 20 15.92 20.4w 437313 F51 C@0614 2014 04 24.38276 14 01 17.65 -01 27 44.4 19.7V 437313 G96 C~13Lh 2014 04 24.39180 14 01 17.43 -01 27 43.0 19.8V 437313 G96 C~13Lh 2014 04 24.40083 14 01 17.22 -01 27 41.8 19.8V 437313 G96 C~13Lh 2014 04 24.40986 14 01 17.01 -01 27 40.6 19.7V 437313 G96 C~13Lh 2014 04 29.35088 13 59 27.738 -01 16 51.06 20.4w 437313 F51 C@0614 2014 04 29.36344 13 59 27.454 -01 16 49.48 20.4w 437313 F51 C@0614 2014 04 29.37600 13 59 27.174 -01 16 47.98 20.4w 437313 F51 C@0614 2014 04 29.38859 13 59 26.888 -01 16 46.38 20.4w 437313 F51 C@0614 2014 05 03.26896 13 58 03.13 -01 09 11.7 20.1V 437313 G96 C~143c 2014 05 03.27404 13 58 03.01 -01 09 11.1 19.9V 437313 G96 C~143c 2014 05 03.27911 13 58 02.90 -01 09 10.6 19.9V 437313 G96 C~143c 2014 05 03.28416 13 58 02.80 -01 09 10.0 19.9V 437313 G96 C~143c 2014 05 04.35894 13 57 40.169 -01 07 12.87 20.5w 437313 F51 C@0614 2014 05 04.37028 13 57 39.920 -01 07 11.64 20.4w 437313 F51 C@0614 2014 05 04.38164 13 57 39.678 -01 07 10.48 20.5w 437313 F51 C@0614 2014 05 04.39302 13 57 39.430 -01 07 09.20 20.4w 437313 F51 C@0614 2014 05 18.28770 13 53 16.278 -00 48 42.07 20.6w 437313 F51 C@0614 2014 05 18.29896 13 53 16.083 -00 48 41.45 20.6w 437313 F51 C@0614 2014 05 18.31020 13 53 15.893 -00 48 40.87 20.6w 437313 F51 C@0614 2014 05 18.32146 13 53 15.697 -00 48 40.26 20.6w 437313 F51 C@0614 2015 02 27.59639 16 24 33.018 -12 23 23.54 21.7w 437313 F51 C~1w0Y 2015 02 27.60769 16 24 33.218 -12 23 23.03 21.6w 437313 F51 C@0614 2015 02 27.61900 16 24 33.424 -12 23 22.77 21.7w 437313 F51 C@0614 2015 02 27.63031 16 24 33.610 -12 23 22.26 21.5w 437313 F51 C@0614 2015 04 23.55405 16 25 01.655 -11 14 25.13 21.2w 437313 F51 C~1QeM 2015 04 23.56677 16 25 01.457 -11 14 24.15 21.2w 437313 F51 C~1QeM 2015 04 23.57941 16 25 01.241 -11 14 22.94 21.2w 437313 F51 C~1QeM 2015 04 23.59209 16 25 01.028 -11 14 21.92 21.1w 437313 F51 C~1QeM 2015 05 13.37933 16 18 35.46 -10 47 23.3 20.7V 437313 G96 C~1S7Q 2015 05 13.39263 16 18 35.17 -10 47 22.4 20.6V 437313 G96 C~1S7Q 2015 05 13.40262 16 18 34.94 -10 47 21.4 20.7V 437313 G96 C~1S7Q 2015 05 13.41260 16 18 34.69 -10 47 20.9 20.7V 437313 G96 C~1S7Q 2015 05 21.47999 16 15 29.351 -10 38 36.20 21.0w 437313 F51 C~1SM7 2015 05 21.49236 16 15 29.055 -10 38 35.41 21.0w 437313 F51 C~1SM7 2015 05 21.50469 16 15 28.751 -10 38 34.80 20.9w 437313 F51 C~1SM7 2015 05 21.51707 16 15 28.457 -10 38 34.13 20.9w 437313 F51 C~1SM7 2015 05 22.50672 16 15 05.279 -10 37 37.35 21.1w 437313 F51 C~1Shb 2015 05 22.51926 16 15 04.967 -10 37 36.56 21.1w 437313 F51 C~1Shb 2015 06 15.34060 16 06 09.865 -10 25 08.80 21.1w 437313 F51 C~1TiV 2015 06 15.35314 16 06 09.612 -10 25 08.72 21.1w 437313 F51 C~1TiV 2015 06 15.36564 16 06 09.351 -10 25 08.90 21.1w 437313 F51 C~1TiV 2015 06 15.37816 16 06 09.089 -10 25 08.67 21.2w 437313 F51 C~1TiV
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 0.28 0.00 -0.09
2 0.0000 0.00 0.13 0.00 0.34
3 0.0001 0.00 0.25 0.00 -0.07
4 0.0001 0.00 0.16 0.00 0.09
5 0.0049 0.00 0.34 0.00 -0.21
6 0.0050 0.00 -0.02 0.00 0.34
7 0.0050 0.00 0.08 0.00 -0.11
8 0.0050 0.00 -0.85 0.00 0.24
9 0.0650 0.00 -0.40 0.00 -0.09
10 0.0651 0.00 0.04 0.00 -0.11
11 0.0651 0.00 -0.10 0.00 -0.24
12 0.0651 0.00 -0.09 0.00 -0.06
13 0.9555 0.00 0.01 0.00 -0.07
14 0.9556 0.00 0.11 0.00 -0.23
15 0.9556 0.00 0.05 0.00 -0.29
16 0.9740 0.00 0.23 0.00 0.37
17 0.9740 0.00 0.17 0.00 0.02
18 0.9740 0.00 0.11 0.00 0.28
19 0.9741 0.00 0.49 0.00 0.33
20 1.0261 0.00 -0.63 0.00 0.32
21 1.0262 0.00 -0.92 0.00 0.12
22 1.0262 0.00 -0.15 0.00 0.02
23 1.0376 0.00 -0.60 0.00 -0.13
24 1.0377 0.00 -0.23 0.00 0.05
25 1.0377 0.00 0.17 0.00 -0.20
26 1.0377 0.00 -0.63 0.00 0.25
27 1.0566 0.00 -0.13 0.00 0.16
28 1.0566 0.00 0.20 0.00 0.10
29 1.0566 0.00 0.11 0.00 0.03
30 1.0567 0.00 0.01 0.00 -0.14
31 1.1137 0.00 0.79 0.00 -0.27
32 1.1137 0.00 0.70 0.00 -0.30
33 1.1137 0.00 0.46 0.00 -0.74
34 1.9796 0.00 -0.09 0.00 -0.04
35 1.9797 0.00 0.65 0.00 -0.12
36 1.9798 0.00 -0.70 0.00 1.05
37 2.0425 0.00 0.11 0.00 0.75
38 2.0425 0.00 0.42 0.00 0.19
39 2.0968 0.00 -0.31 0.00 -0.39
40 2.0968 0.00 0.35 0.00 0.04
41 2.0969 0.00 0.04 0.00 0.44
42 2.0969 0.00 0.20 0.00 0.42
43 2.0969 0.00 -0.34 0.00 -0.34
44 2.0969 0.00 -1.07 0.00 -0.75
45 2.0970 0.00 -0.19 0.00 -0.06
46 2.0970 0.00 0.43 0.00 0.59
47 2.0995 0.00 0.04 0.00 -0.92
48 2.0996 0.00 0.04 0.00 0.79
49 2.0996 0.00 -0.19 0.00 0.12
50 2.0997 0.00 0.40 0.00 -0.32
51 2.0997 0.00 -0.33 0.00 -1.03
52 2.0997 0.00 0.78 0.00 -0.06
53 2.0997 0.00 0.63 0.00 0.39
54 2.1138 0.00 -0.19 0.00 -0.07
55 2.1138 0.00 -0.18 0.00 -0.13
56 2.1139 0.00 -0.18 0.00 -0.05
57 2.1139 0.00 -0.20 0.00 -0.12
58 2.1683 0.00 0.24 0.00 -0.05
59 2.1683 0.00 0.05 0.00 0.10
60 2.1683 0.00 -0.00 0.00 0.05
61 2.1683 0.00 -0.05 0.00 -0.00
62 2.1819 0.00 0.04 0.00 0.01
63 2.1819 0.00 0.04 0.00 0.04
64 2.1819 0.00 0.10 0.00 -0.02
65 2.1820 0.00 0.08 0.00 0.03
66 2.1926 0.00 -0.26 0.00 0.01
67 2.1926 0.00 -0.39 0.00 0.05
68 2.1926 0.00 -0.38 0.00 -0.01
69 2.1926 0.00 -0.22 0.00 0.03
70 2.1956 0.00 0.06 0.00 0.03
71 2.1956 0.00 0.02 0.00 0.05
72 2.1956 0.00 0.10 0.00 -0.00
73 2.1957 0.00 0.09 0.00 0.06
74 2.2337 0.00 0.06 0.00 -0.12
75 2.2337 0.00 0.03 0.00 -0.07
76 2.2338 0.00 0.07 0.00 -0.07
77 2.2338 0.00 0.03 0.00 -0.03
78 3.0148 0.00 0.01 0.00 0.03
79 3.0149 0.00 0.04 0.00 0.09
80 3.0149 0.00 0.16 0.00 -0.10
81 3.0149 0.00 -0.01 0.00 -0.05
82 3.1653 0.00 0.03 0.00 0.21
83 3.1653 0.00 0.18 0.00 0.06
84 3.1654 0.00 0.05 0.00 0.13
85 3.1654 0.00 -0.04 0.00 0.02
86 3.2196 0.00 -0.14 0.00 -0.19
87 3.2196 0.00 0.08 0.00 -0.25
88 3.2197 0.00 0.07 0.00 0.04
89 3.2197 0.00 -0.25 0.00 -0.18
90 3.2418 0.00 0.07 0.00 0.00
91 3.2418 0.00 0.09 0.00 0.06
92 3.2418 0.00 -0.03 0.00 -0.05
93 3.2419 0.00 0.02 0.00 -0.11
94 3.2446 0.00 0.08 0.00 -0.04
95 3.2446 0.00 -0.07 0.00 0.04
96 3.3098 0.00 -0.09 0.00 0.13
97 3.3099 0.00 0.01 0.00 0.17
98 3.3099 0.00 -0.02 0.00 -0.06
99 3.3099 0.00 -0.05 0.00 0.12
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.
437313 quality flag:3 Type: CENTAURR CENTAURR CENTAURR axisobj 12.930 12.930 12.930 ecceobj 0.579 0.579 0.579 incobj 8.983 8.983 8.983 qmin 5.439 5.235 5.393 qmax 21.790 21.105 21.259 amean 13.088 11.726 13.181 amin 12.459 10.192 12.930 amax 13.658 13.290 13.326 emean 0.582 0.538 0.588 emin 0.562 0.483 0.579 emax 0.595 0.588 0.595 imean 8.767 7.292 8.427 imin 7.718 6.249 7.718 imax 10.100 8.150 9.439 excite_mean 0.601 0.553 0.606 fracstop 0.000 0.000 0.000 cjmean 3.364 3.644 3.342 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 62.1 70.1 53.8 kozaiamp 10.3 27.6 4.3