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: 612085
# Created Fri Nov 22 02:07:40 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 86 observations of 86
# Arc: 21.86y
# First observation: 1999/02/11
# Last observation: 2020/12/22
# Chi-squared of fit: 146.12 DOF: 166 RMS: 0.23
# Min/Max residuals: -0.71 0.87
# Exact a, adot, b, bdot, g, gdot:
1.212960E-05 1.847322E-02 6.195951E-06 7.952436E-03 2.184122E-02 -2.306532E-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
0.594155 126.177740 -0.277735 0.009672 -0.953815 2451220.795213
# Heliocentric elements and errors
Epoch: 2451220.5000 = 1999/02/11
Mean Anomaly: 288.70460 +/- 0.000
Argument of Peri: 73.10293 +/- 0.000
Long of Asc Node: 125.15992 +/- 0.000
Inclination: 23.32760 +/- 0.000
Eccentricity: 0.00310551 +/- 0.0000
Semi-Major Axis: 46.78095211 +/- 0.0000
Time of Perihelion: 2474365.7044 +/- 0.0
Perihelion: 46.63567330 +/- 0.0000
Aphelion: 46.92623092 +/- 0.0000
Period (y) 319.9719 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -27.80446826 +/- 0.0000
Ecliptic Y 37.56093998 +/- 0.0000
Ecliptic Z 0.47506092 +/- 0.0000
Ecliptic XDOT -0.00184770 +/- 0.0000
Ecliptic YDOT -0.00138959 +/- 0.0000
Ecliptic ZDOT 0.00099651 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 46.73476793 +/- 0.0000
Geocenter to KBO 45.78503751 +/- 0.0000
# Hcoef: 6.09
The following table shows the complete astrometric record for 612085. 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 (612085) followed by the observatory code and reference code for the source of the astrometry.
1999 02 11.29447 08 34 51.17 +19 18 14.0 22.3R 612085 568 Ca4178 1999 02 11.37670 08 34 50.80 +19 18 15.6 22.3R 612085 568 Ca4178 1999 02 17.26347 08 34 25.46 +19 20 13.3 22.3R 612085 568 Ca4178 1999 02 17.30662 08 34 25.28 +19 20 14.5 22.3R 612085 568 Ca4178 1999 03 10.38367 08 33 06.89 +19 26 25.5 22.3R 612085 568 Ca4506 1999 03 10.39741 08 33 06.84 +19 26 25.7 22.3R 612085 568 Ca4506 1999 04 09.34053 08 32 06.43 +19 31 57.2 22.6R 612085 568 Ca4506 1999 04 11.29882 08 32 05.04 +19 32 09.5 22.6R 612085 568 Ca4506 1999 12 28.41958 08 42 58.13 +19 12 38.4 22.1R 612085 695 Ca8502 1999 12 28.49390 08 42 57.85 +19 12 40.2 22.7R 612085 695 Ca8502 1999 12 28.55970 08 42 57.61 +19 12 41.1 21.9R 612085 695 Ca8502 1999 12 29.44564 08 42 54.25 +19 12 59.0 22.3R 612085 695 Ca8502 1999 12 29.50881 08 42 54.02 +19 13 00.1 22.5R 612085 695 Ca8502 1999 12 30.62664 08 42 49.69 +19 13 21.7 612085 568 Ca8502 1999 12 31.60211 08 42 45.90 +19 13 41.2 612085 568 Ca8502 1999 12 31.62312 08 42 45.81 +19 13 41.8 612085 568 Ca8502 2001 03 11.06043 08 42 41.14 +19 47 23.2 22.2 612085 304 Ce8574 2001 03 11.08751 08 42 41.05 +19 47 23.6 612085 304 Ce8574 2002 02 03.61294 08 49 57.11 +19 45 21.1 22.2R 612085 568 Cf1463 2002 02 04.48508 08 49 53.14 +19 45 40.2 612085 568 Cf1463 2004 12 13.395013 09 07 56.14 +19 50 44.8 22.6V 612085 645 C~1BPS 2004 12 13.395843 09 07 56.14 +19 50 44.8 22.6V 612085 645 C~1BPS 2004 12 13.398330 09 07 56.13 +19 50 44.8 23.4V 612085 645 C~1BPS 2007 02 15.21330 09 13 34.40 +20 29 28.3 22.2R 612085 688 Cu2274 2007 02 15.31115 09 13 33.97 +20 29 29.5 612085 688 Cu2274 2011 01 08.33423 09 35 54.57 +20 35 43.4 22.4R 612085 695 C~0U2H 2011 01 08.47828 09 35 54.07 +20 35 47.2 612085 695 C~0U2H 2011 01 08.54482 09 35 53.77 +20 35 48.5 612085 695 C~0U2H 2011 01 30.53464 09 34 24.380 +20 45 44.78 22.6G 612085 F51 C~2r77 2011 01 30.56722 09 34 24.227 +20 45 45.64 22.6G 612085 F51 C~2r77 2011 01 30.58235 09 34 24.152 +20 45 46.09 22.5G 612085 F51 C~2r77 2012 02 15.34682 09 38 10.865 +20 56 58.52 22.3G 612085 F51 C~2r77 2012 02 15.36070 09 38 10.808 +20 56 58.54 22.4G 612085 F51 C~2r77 2012 02 15.37457 09 38 10.734 +20 56 59.05 22.4G 612085 F51 C~2r77 2012 02 15.38848 09 38 10.665 +20 56 59.49 22.2G 612085 F51 C~2r77 2014 01 24.38251 09 49 39.184 +20 54 10.78 22.3G 612085 F51 C~2r77 2014 01 24.39568 09 49 39.119 +20 54 11.68 23.0G 612085 F51 C~2r77 2014 01 24.40887 09 49 39.036 +20 54 11.71 22.5G 612085 F51 C~2r77 2014 01 24.42211 09 49 38.981 +20 54 12.26 22.5G 612085 F51 C~2r77 2015 01 17.41571 09 55 04.868 +20 53 17.20 22.9G 612085 F51 C~2r77 2015 01 17.42773 09 55 04.819 +20 53 17.23 23.2G 612085 F51 C~2r77 2015 01 17.43975 09 55 04.794 +20 53 17.62 22.6G 612085 F51 C~2r77 2015 01 17.45182 09 55 04.730 +20 53 18.28 22.5G 612085 F51 C~2r77 2015 01 17.57681 09 55 04.255 +20 53 21.68 22.3G 612085 F51 C~2r77 2015 01 17.58915 09 55 04.215 +20 53 22.28 22.4G 612085 F51 C~2r77 2015 01 17.60150 09 55 04.164 +20 53 22.43 22.4G 612085 F51 C~2r77 2015 01 17.61387 09 55 04.120 +20 53 22.53 22.0G 612085 F51 C~2r77 2015 01 22.40263 09 54 45.537 +20 55 42.24 23.2G 612085 F51 C~2r77 2015 01 22.41481 09 54 45.488 +20 55 42.50 23.0G 612085 F51 C~2r77 2015 01 22.42696 09 54 45.429 +20 55 42.90 22.5G 612085 F51 C~2r77 2015 01 22.43914 09 54 45.382 +20 55 43.36 23.1G 612085 F51 C~2r77 2015 02 11.37068 09 53 20.238 +21 05 15.38 23.8G 612085 F51 C~2r77 2015 02 12.38723 09 53 15.667 +21 05 43.11 22.3G 612085 F51 C~2r77 2015 04 17.024722 09 49 29.37 +21 23 45.7 612085 W84 C~3i8v 2015 04 17.026221 09 49 29.35 +21 23 46.3 612085 W84 C~3i8v 2016 01 07.59910 10 00 36.480 +20 50 27.87 22.4G 612085 F51 C~2r77 2016 01 07.61396 10 00 36.438 +20 50 28.29 22.6G 612085 F51 C~2r77 2016 01 07.62887 10 00 36.376 +20 50 28.75 22.4G 612085 F51 C~2r77 2016 01 07.64386 10 00 36.329 +20 50 29.17 22.9G 612085 F51 C~2r77 2016 01 31.38893 09 59 07.325 +21 02 04.11 23.2G 612085 F51 C~2r77 2016 02 05.38255 09 58 45.878 +21 04 30.08 23.1G 612085 F51 C~2r77 2016 02 06.55679 09 58 40.743 +21 05 04.05 22.8G 612085 F51 C~2r77 2016 02 06.56949 09 58 40.691 +21 05 04.37 22.6G 612085 F51 C~2r77 2016 02 06.58217 09 58 40.643 +21 05 04.76 22.4G 612085 F51 C~2r77 2016 02 06.59493 09 58 40.570 +21 05 05.22 23.1G 612085 F51 C~2r77 2016 03 03.29332 09 56 47.230 +21 16 19.33 22.7G 612085 F51 C~2r77 2016 03 03.30650 09 56 47.179 +21 16 19.92 22.5G 612085 F51 C~2r77 2016 03 03.31970 09 56 47.120 +21 16 20.31 22.2G 612085 F51 C~2r77 2016 03 03.33301 09 56 47.056 +21 16 20.68 22.6G 612085 F51 C~2r77 2016 04 22.32063 09 54 15.049 +21 26 35.89 22.6G 612085 F51 C~2r77 2017 02 18.35297 10 02 43.506 +21 12 38.55 22.6G 612085 F51 C~2r77 2017 02 19.36446 10 02 38.990 +21 13 05.92 22.3G 612085 F51 C~2r77 2017 02 24.50536 10 02 16.182 +21 15 20.39 23.3G 612085 F51 C~2r77 2017 02 24.50611 10 02 16.166 +21 15 20.35 22.7G 612085 F51 C~2r77 2017 02 24.51841 10 02 16.121 +21 15 20.74 23.0G 612085 F51 C~2r77 2017 02 24.51918 10 02 16.114 +21 15 20.88 22.9G 612085 F51 C~2r77 2017 02 24.53155 10 02 16.055 +21 15 21.09 22.0G 612085 F51 C~2r77 2017 02 24.53233 10 02 16.065 +21 15 21.17 22.6G 612085 F51 C~2r77 2017 03 06.079520 10 01 34.71 +21 19 09.9 612085 W84 C~3i8v 2017 03 06.082818 10 01 34.70 +21 19 10.0 612085 W84 C~3i8v 2017 04 16.38772 09 59 20.446 +21 28 29.79 23.1G 612085 F51 C~2r77 2020 01 31.447456 10 18 57.455 +21 05 30.55 22.6G 612085 T12 C~3i8v 2020 01 31.498039 10 18 57.249 +21 05 32.13 22.4G 612085 T12 C~3i8v 2020 12 22.53274 10 25 47.692 +20 45 32.90 22.7w 612085 F51 C~4NCX 2020 12 22.54489 10 25 47.687 +20 45 33.12 22.6w 612085 F51 C~4NCX 2020 12 22.55700 10 25 47.673 +20 45 33.78 22.4w 612085 F51 C~4NCX
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 0.24 0.00 -0.15
2 0.0002 0.00 0.20 0.00 -0.24
3 0.0163 0.00 0.23 0.00 -0.27
4 0.0165 0.00 0.29 0.00 0.07
5 0.0742 0.00 0.16 0.00 0.19
6 0.0742 0.00 0.07 0.00 0.18
7 0.1562 0.00 0.15 0.00 -0.10
8 0.1615 0.00 0.25 0.00 -0.05
9 0.8765 0.00 -0.15 0.00 0.20
10 0.8767 0.00 -0.09 0.00 0.54
11 0.8768 0.00 0.07 0.00 0.16
12 0.8793 0.00 -0.17 0.00 0.53
13 0.8794 0.00 0.05 0.00 0.39
14 0.8825 0.00 -0.58 0.00 -0.35
15 0.8852 0.00 -0.58 0.00 -0.47
16 0.8852 0.00 -0.68 0.00 -0.29
17 2.0774 0.00 0.05 0.00 0.15
18 2.0775 0.00 0.02 0.00 0.14
19 2.9797 0.00 0.16 0.00 -0.29
20 2.9820 0.00 0.04 0.00 -0.71
21 5.8374 0.00 0.16 0.00 -0.14
22 5.8374 0.00 0.19 0.00 -0.15
23 5.8374 0.00 0.13 0.00 -0.20
24 8.0107 0.00 -0.28 0.00 0.74
25 8.0110 0.00 -0.08 0.00 -0.33
26 11.9070 0.00 0.45 0.00 0.18
27 11.9074 0.00 0.87 0.00 0.18
28 11.9076 0.00 0.02 0.00 -0.27
29 11.9678 0.00 -0.15 0.00 0.14
30 11.9679 0.00 -0.25 0.00 0.12
31 11.9679 0.00 -0.36 0.00 0.17
32 13.0104 0.00 -0.17 0.00 0.19
33 13.0104 0.00 -0.07 0.00 -0.15
34 13.0105 0.00 -0.23 0.00 0.01
35 13.0105 0.00 -0.31 0.00 0.09
36 14.9516 0.00 0.41 0.00 -0.24
37 14.9517 0.00 0.26 0.00 0.28
38 14.9517 0.00 -0.15 0.00 -0.07
39 14.9518 0.00 -0.15 0.00 0.10
40 15.9319 0.00 -0.11 0.00 0.09
41 15.9319 0.00 -0.15 0.00 -0.23
42 15.9320 0.00 0.16 0.00 -0.19
43 15.9320 0.00 -0.10 0.00 0.12
44 15.9323 0.00 -0.02 0.00 -0.11
45 15.9324 0.00 0.10 0.00 0.14
46 15.9324 0.00 0.04 0.00 -0.07
47 15.9324 0.00 0.10 0.00 -0.32
48 15.9455 0.00 -0.05 0.00 0.03
49 15.9456 0.00 -0.04 0.00 -0.06
50 15.9456 0.00 -0.19 0.00 -0.02
51 15.9456 0.00 -0.15 0.00 0.08
52 16.0002 0.00 0.74 0.00 0.32
53 16.0030 0.00 0.21 0.00 0.08
54 16.1772 0.00 0.13 0.00 0.13
55 16.1772 0.00 -0.13 0.00 0.73
56 16.9043 0.00 0.11 0.00 -0.02
57 16.9044 0.00 0.19 0.00 -0.01
58 16.9044 0.00 -0.02 0.00 0.03
59 16.9044 0.00 -0.01 0.00 0.03
60 16.9695 0.00 0.07 0.00 -0.05
61 16.9831 0.00 -0.08 0.00 0.00
62 16.9863 0.00 -0.08 0.00 0.02
63 16.9864 0.00 -0.01 0.00 -0.03
64 16.9864 0.00 0.11 0.00 -0.00
65 16.9864 0.00 -0.14 0.00 0.09
66 17.0568 0.00 -0.20 0.00 -0.35
67 17.0568 0.00 -0.11 0.00 -0.06
68 17.0569 0.00 -0.13 0.00 0.02
69 17.0569 0.00 -0.23 0.00 0.09
70 17.1938 0.00 -0.13 0.00 0.13
71 18.0207 0.00 0.02 0.00 -0.20
72 18.0235 0.00 -0.13 0.00 -0.08
73 18.0375 0.00 0.11 0.00 -0.06
74 18.0375 0.00 -0.08 0.00 -0.12
75 18.0376 0.00 0.08 0.00 -0.04
76 18.0376 0.00 0.02 0.00 0.08
77 18.0376 0.00 -0.03 0.00 -0.02
78 18.0376 0.00 0.17 0.00 0.04
79 18.0638 0.00 -0.12 0.00 0.01
80 18.0638 0.00 -0.06 0.00 0.03
81 18.1768 0.00 0.01 0.00 -0.03
82 20.9696 0.00 0.05 0.00 -0.02
83 20.9698 0.00 0.09 0.00 -0.03
84 21.8624 0.00 -0.25 0.00 -0.19
85 21.8624 0.00 -0.04 0.00 -0.28
86 21.8625 0.00 0.04 0.00 0.07
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.
612085 quality flag:3 Type: SCATEXTD SCATEXTD SCATEXTD axisobj 46.916 46.916 46.916 ecceobj 0.005 0.005 0.005 incobj 23.294 23.294 23.294 qmin 46.022 46.021 46.023 qmax 48.034 48.033 48.034 amean 46.930 46.930 46.931 amin 46.573 46.573 46.573 amax 47.299 47.298 47.299 emean 0.007 0.007 0.007 emin 0.000 0.000 0.000 emax 0.016 0.016 0.016 imean 21.814 21.814 21.814 imin 21.600 21.600 21.600 imax 22.033 22.033 22.033 excite_mean 0.372 0.372 0.372 fracstop 1.000 1.000 1.000 cjmean 2.960 2.960 2.960 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 175.9 176.0 176.0 kozaiamp 179.9 179.9 180.0