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: 523899
# Created Wed Apr 24 01:08:28 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 66 observations of 66
# Arc: 22.16y
# First observation: 1997/02/06
# Last observation: 2019/04/05
# Chi-squared of fit: 485.14 DOF: 126 RMS: 0.48
# Min/Max residuals: -1.43 1.09
# Exact a, adot, b, bdot, g, gdot:
1.491326E-05 2.551356E-02 3.502426E-07 3.459114E-03 2.543952E-02 -3.309919E-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
2.262878 137.068626 -0.011977 0.039125 -0.994093 2450485.970540
# Heliocentric elements and errors
Epoch: 2450486.5000 = 1997/02/07
Mean Anomaly: 342.65224 +/- 0.000
Argument of Peri: 34.81498 +/- 0.000
Long of Asc Node: 121.26270 +/- 0.000
Inclination: 8.04645 +/- 0.000
Eccentricity: 0.04151538 +/- 0.0000
Semi-Major Axis: 41.94984707 +/- 0.0000
Time of Perihelion: 2455268.7792 +/- 0.0
Perihelion: 40.20828340 +/- 0.0000
Aphelion: 43.69141073 +/- 0.0000
Period (y) 271.7088 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -29.48893443 +/- 0.0000
Ecliptic Y 27.41584416 +/- 0.0000
Ecliptic Z 1.55210997 +/- 0.0000
Ecliptic XDOT -0.00182737 +/- 0.0000
Ecliptic YDOT -0.00203890 +/- 0.0000
Ecliptic ZDOT 0.00037040 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.29436015 +/- 0.0000
Geocenter to KBO 39.30897209 +/- 0.0000
# Hcoef: 7.37
The following table shows the complete astrometric record for 523899. 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 (523899) followed by the observatory code and reference code for the source of the astrometry.
1997 02 06.46982 09 20 57.12 +17 52 31.8 22.8R 523899 568 C30145 1997 02 06.50517 09 20 56.92 +17 52 32.5 523899 568 C30145 1997 02 06.54095 09 20 56.78 +17 52 33.8 523899 568 C30145 1997 02 07.43281 09 20 52.20 +17 52 56.3 523899 568 C30145 1997 02 07.47111 09 20 52.00 +17 52 57.2 523899 568 C30145 1997 02 09.38100 09 20 42.22 +17 53 45.5 523899 568 C30145 1997 02 09.41839 09 20 42.06 +17 53 46.6 523899 568 C30145 1997 02 09.45591 09 20 41.82 +17 53 47.6 523899 568 C30145 1997 02 09.54990 09 20 41.38 +17 53 50.0 523899 568 C30145 1997 04 07.89249 09 16 55.40 +18 11 04.6 523899 950 C30242 1997 04 07.93019 09 16 55.33 +18 11 04.8 523899 950 C30242 1998 02 16.48182 09 26 12.45 +17 40 53.2 523899 568 Ca0526 1998 02 16.54732 09 26 12.13 +17 40 54.8 523899 568 Ca0526 1998 02 16.58885 09 26 11.90 +17 40 56.2 523899 568 Ca0526 1998 02 17.50192 09 26 07.35 +17 41 18.4 523899 568 Ca0526 1998 02 17.59559 09 26 06.86 +17 41 20.0 523899 568 Ca0526 1998 02 18.49820 09 26 02.37 +17 41 43.1 523899 568 Ca0526 1998 02 18.54722 09 26 02.12 +17 41 43.9 523899 568 Ca0526 1998 12 18.20884 09 36 33.56 +16 59 57.6 523899 950 Ca3586 1998 12 18.23825 09 36 33.47 +16 59 58.0 523899 950 Ca3586 1998 12 18.26209 09 36 33.41 +16 59 59.1 523899 950 Ca3800 1998 12 19.20130 09 36 31.10 +17 00 15.0 523899 950 Ca3586 1998 12 19.23795 09 36 31.01 +17 00 15.9 523899 950 Ca3800 1998 12 19.26487 09 36 30.93 +17 00 15.8 523899 950 Ca3586 1999 02 16.25676 09 32 19.10 +17 24 15.4 523899 568 Ca4120 1999 02 16.37498 09 32 18.43 +17 24 17.8 22.9R 523899 568 Ca3800 1999 02 16.41302 09 32 18.22 +17 24 18.8 523899 568 Ca3800 1999 02 16.45233 09 32 18.02 +17 24 19.8 523899 568 Ca3800 1999 02 17.31904 09 32 13.70 +17 24 41.9 523899 568 Ca3800 1999 02 17.35801 09 32 13.50 +17 24 42.8 523899 568 Ca3800 1999 02 17.39170 09 32 13.32 +17 24 43.7 523899 568 Ca3800 1999 03 23.25284 09 29 43.64 +17 36 44.6 523899 568 Ca4796 1999 03 23.33771 09 29 43.32 +17 36 45.8 523899 568 Ca4796 1999 05 09.98889 09 28 34.40 +17 40 49.0 23.4R 523899 807 Ca6670 1999 05 10.99861 09 28 35.27 +17 40 42.5 23.6R 523899 807 Ca6670 2000 03 30.26309 09 35 20.04 +17 21 54.8 523899 568 Cb1806 2000 03 30.26959 09 35 20.02 +17 21 54.8 523899 568 Cb1806 2000 03 30.27631 09 35 19.99 +17 21 54.8 523899 568 Cb1806 2000 03 30.28290 09 35 19.97 +17 21 55.1 523899 568 Cb1806 2000 03 30.29589 09 35 19.93 +17 21 55.2 523899 568 Cb1806 2000 03 30.30371 09 35 19.91 +17 21 55.4 523899 568 Cb1806 2000 03 30.31661 09 35 19.87 +17 21 55.6 523899 568 Cb1807 2000 03 30.32306 09 35 19.85 +17 21 55.6 523899 568 Cb1807 2000 03 30.33607 09 35 19.81 +17 21 55.9 523899 568 Cb1807 2001 02 17.06311 09 44 19.40 +16 49 49.1 22.8R 523899 950 Cc6334 2001 02 17.11487 09 44 19.13 +16 49 50.7 523899 950 Cc6334 2001 05 22.28375 09 40 40.32 +17 05 39.8 523899 568 Cd2185 2001 05 22.31663 09 40 40.38 +17 05 39.4 523899 568 Cd2185 2006 01 06.449485 10 17 21.09 +14 50 53.2 22.7V 523899 645 C~1cF1 2006 01 06.450314 10 17 21.09 +14 50 53.2 22.9V 523899 645 C~1cF1 2006 01 06.452802 10 17 21.08 +14 50 53.2 24.2V 523899 645 C~1cF1 2006 01 31.393088 10 15 44.21 +15 02 09.6 523899 645 C~1cF1 2006 01 31.393917 10 15 44.21 +15 02 09.6 523899 645 C~1cF1 2006 01 31.396405 10 15 44.20 +15 02 09.7 523899 645 C~1cF1 2008 03 05.26810 10 24 55.97 +14 34 43.3 523899 695 Cy7583 2008 03 05.35218 10 24 55.56 +14 34 45.6 523899 695 Cy7583 2013 03 13.34035 10 53 37.80 +12 40 29.7 22.8R 523899 695 C~0ucn 2013 03 14.31430 10 53 33.21 +12 40 57.2 523899 695 C~0ucn 2013 03 14.42440 10 53 32.71 +12 41 00.2 523899 695 C~0ucn 2017 04 22.005046 11 14 04.65 +11 12 45.2 523899 W84 C~3n9P 2017 04 22.021013 11 14 04.59 +11 12 45.2 523899 W84 C~3n9P 2019 03 07.195140 11 28 47.04 +10 00 03.4 23.4G 523899 705 C~31GV 2019 03 07.249990 11 28 46.77 +10 00 05.2 23.6G 523899 705 C~31GV 2019 03 07.288140 11 28 46.61 +10 00 06.3 23.4G 523899 705 C~31GV 2019 04 05.179510 11 26 34.273 +10 13 55.67 23.2G 523899 G37 C~34bV 2019 04 05.253110 11 26 33.948 +10 13 57.24 523899 G37 C~34bV
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 0.31 0.00 0.29
2 0.0001 0.00 0.07 0.00 0.10
3 0.0002 0.00 0.75 0.00 0.49
4 0.0026 0.00 0.23 0.00 0.30
5 0.0027 0.00 0.21 0.00 0.23
6 0.0080 0.00 -0.41 0.00 0.20
7 0.0081 0.00 0.10 0.00 0.35
8 0.0082 0.00 -0.57 0.00 0.41
9 0.0084 0.00 0.13 0.00 0.46
10 0.1654 0.00 -0.70 0.00 0.96
11 0.1655 0.00 -0.60 0.00 0.88
12 1.0267 0.00 -0.05 0.00 0.29
13 1.0269 0.00 0.15 0.00 0.27
14 1.0270 0.00 -0.14 0.00 0.64
15 1.0295 0.00 0.15 0.00 0.11
16 1.0298 0.00 -0.09 0.00 -0.59
17 1.0322 0.00 0.07 0.00 0.18
18 1.0324 0.00 0.04 0.00 -0.22
19 1.8610 0.00 0.27 0.00 0.17
20 1.8611 0.00 0.02 0.00 0.06
21 1.8612 0.00 0.02 0.00 0.75
22 1.8637 0.00 0.05 0.00 0.13
23 1.8638 0.00 0.12 0.00 0.38
24 1.8639 0.00 -0.03 0.00 -0.20
25 2.0254 0.00 0.83 0.00 0.08
26 2.0257 0.00 -0.18 0.00 -0.58
27 2.0259 0.00 -0.41 0.00 -0.56
28 2.0260 0.00 -0.39 0.00 -0.57
29 2.0283 0.00 -0.08 0.00 -0.64
30 2.0284 0.00 -0.10 0.00 -0.74
31 2.0285 0.00 -0.22 0.00 -0.70
32 2.1212 0.00 -0.43 0.00 -1.29
33 2.1215 0.00 -0.66 0.00 -1.43
34 2.2519 0.00 1.06 0.00 0.91
35 2.2547 0.00 1.09 0.00 0.79
36 3.1425 0.00 -0.08 0.00 -0.84
37 3.1425 0.00 -0.08 0.00 -0.93
38 3.1425 0.00 -0.21 0.00 -1.02
39 3.1425 0.00 -0.20 0.00 -0.81
40 3.1426 0.00 -0.20 0.00 -0.88
41 3.1426 0.00 -0.13 0.00 -0.78
42 3.1426 0.00 -0.13 0.00 -0.75
43 3.1427 0.00 -0.13 0.00 -0.84
44 3.1427 0.00 -0.12 0.00 -0.71
45 4.0290 0.00 0.22 0.00 0.66
46 4.0291 0.00 0.12 0.00 0.88
47 4.2870 0.00 0.28 0.00 1.05
48 4.2871 0.00 0.35 0.00 1.03
49 8.9144 0.00 0.10 0.00 0.14
50 8.9144 0.00 0.14 0.00 0.12
51 8.9144 0.00 0.11 0.00 0.06
52 8.9827 0.00 0.01 0.00 0.38
53 8.9827 0.00 0.07 0.00 0.36
54 8.9827 0.00 0.09 0.00 0.39
55 11.0741 0.00 -0.13 0.00 0.47
56 11.0743 0.00 -0.13 0.00 0.45
57 16.0955 0.00 -0.05 0.00 0.12
58 16.0981 0.00 -0.37 0.00 0.11
59 16.0984 0.00 -0.02 0.00 0.03
60 20.2041 0.00 0.07 0.00 -0.01
61 20.2041 0.00 -0.06 0.00 -0.24
62 22.0773 0.00 -0.02 0.00 -0.13
63 22.0774 0.00 -0.16 0.00 -0.10
64 22.0775 0.00 0.17 0.00 -0.23
65 22.1566 0.00 0.15 0.00 0.15
66 22.1568 0.00 0.02 0.00 -0.04
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.
523899 quality flag:2 Type: CLASSICAL SCATNEAR SCATNEAR axisobj 42.151 42.151 42.151 ecceobj 0.045 0.045 0.045 incobj 8.027 8.027 8.027 qmin 38.791 38.111 38.645 qmax 46.274 47.136 46.398 amean 42.323 42.325 42.323 amin 41.920 41.918 41.927 amax 42.757 42.773 42.780 emean 0.057 0.067 0.060 emin 0.024 0.024 0.024 emax 0.083 0.103 0.085 imean 6.591 6.365 6.781 imin 5.415 5.054 5.403 imax 8.045 8.030 8.298 excite_mean 0.129 0.131 0.133 fracstop 1.000 1.000 1.000 cjmean 3.063 3.062 3.062 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 175.9 187.2 173.1 kozaiamp 180.0 180.0 180.0