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: 00CL104
# Created Thu Nov 21 02:08:04 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 36 observations of 36
# Arc: 19.99y
# First observation: 2000/02/05
# Last observation: 2020/02/01
# Chi-squared of fit: 103.43 DOF: 66 RMS: 0.30
# Min/Max residuals: -0.49 0.71
# Exact a, adot, b, bdot, g, gdot:
1.656988E-05 2.354295E-02 2.536682E-07 5.035267E-04 2.401849E-02 1.669470E-03
# Covariance matrix:
1.3431E-13 -4.0111E-14 1.2556E-15 -7.9264E-16 1.4831E-14 -7.7925E-14
-4.0111E-14 2.7942E-14 -9.1904E-16 5.9029E-16 2.7156E-14 5.7622E-14
1.2556E-15 -9.1904E-16 7.2884E-14 -4.7846E-15 -7.1172E-16 -1.9561E-15
-7.9264E-16 5.9029E-16 -4.7846E-15 7.0132E-16 5.0142E-16 1.2536E-15
1.4831E-14 2.7156E-14 -7.1172E-16 5.0142E-16 1.8750E-13 4.7182E-14
-7.7925E-14 5.7622E-14 -1.9561E-15 1.2536E-15 4.7182E-14 1.2248E-13
# lat0 lon0 xBary yBary zBary JD0
0.214017 150.916532 0.249716 0.003354 -0.956801 2451579.890013
# Heliocentric elements and errors
Epoch: 2451580.5000 = 2000/02/06
Mean Anomaly: 55.62620 +/- 0.028
Argument of Peri: 306.17178 +/- 0.033
Long of Asc Node: 140.91495 +/- 0.001
Inclination: 1.24711 +/- 0.000
Eccentricity: 0.07879142 +/- 0.0000
Semi-Major Axis: 44.36077788 +/- 0.0032
Time of Perihelion: 2434905.1852 +/- 8.5
Perihelion: 40.86552928 +/- 0.0032
Aphelion: 47.85602648 +/- 0.0036
Period (y) 295.4656 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -37.09290835 +/- 0.0007
Ecliptic Y 20.92349946 +/- 0.0004
Ecliptic Z 0.15554468 +/- 0.0000
Ecliptic XDOT -0.00147626 +/- 0.0000
Ecliptic YDOT -0.00224573 +/- 0.0000
Ecliptic ZDOT 0.00005821 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 42.58752334 +/- 0.0006
Geocenter to KBO 41.63457708 +/- 0.0008
# Hcoef: 6.40
The following table shows the complete astrometric record for 00CL104. 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 (00CL104) followed by the observatory code and reference code for the source of the astrometry.
2000 02 05.38927 10 12 09.92 +11 20 55.1 22.0R 00CL104 695 Cb1114 2000 02 05.49428 10 12 09.46 +11 20 57.9 00CL104 695 Cb1114 2000 03 01.16806 10 10 16.35 +11 31 35.5 22.2R 00CL104 695 Cb1114 2000 03 01.24778 10 10 16.01 +11 31 37.4 00CL104 695 Cb1114 2000 12 21.64373 10 19 45.45 +10 39 34.1 00CL104 568 Cc3758 2000 12 22.59385 10 19 43.86 +10 39 43.8 22.8R 00CL104 568 Cc3758 2000 12 22.66463 10 19 43.72 +10 39 44.7 00CL104 568 Cc3758 2001 02 21.18226 10 16 05.03 +11 00 54.4 22.0R 00CL104 688 Cc6636 2001 02 21.22867 10 16 04.80 +11 00 55.5 00CL104 688 Cc6636 2001 03 24.08038 10 13 51.31 +11 13 31.6 22.3 00CL104 304 Ce8743 2001 03 24.09363 10 13 51.26 +11 13 32.0 00CL104 304 Ce8743 2001 04 27.29029 10 12 19.69 +11 22 04.5 22.5R 00CL104 568 Cd0809 2001 04 27.40763 10 12 19.52 +11 22 04.9 00CL104 568 Cd0809 2002 02 04.55225 10 22 30.10 +10 26 07.5 22.0R 00CL104 568 Cf1711 2002 02 04.60598 10 22 29.87 +10 26 08.9 00CL104 568 Cf1711 2002 02 06.52553 10 22 21.55 +10 26 57.6 00CL104 568 Cf1711 2002 02 06.57394 10 22 21.34 +10 26 58.7 00CL104 568 Cf1711 2002 02 14.19816 10 21 47.33 +10 30 17.2 21.3R 00CL104 304 f1711 2002 02 14.22052 10 21 47.22 +10 30 17.9 00CL104 304 f1711 2003 03 31.151014 10 23 43.24 +10 21 10.0 22.1V 00CL104 645 C~2FZD 2003 03 31.151843 10 23 43.25 +10 21 10.1 22.5V 00CL104 645 C~2FZD 2003 03 31.154330 10 23 43.25 +10 21 10.1 24.9V 00CL104 645 C~2FZD 2004 03 18.23124 10 29 36.06 +09 48 54.7 22.5R 00CL104 688 Ck2009 2004 03 18.33010 10 29 35.62 +09 48 57.1 00CL104 688 Ck2009 2007 02 15.37066 10 47 02.43 +08 10 20.4 22.2R 00CL104 688 Cu2276 2007 02 15.44552 10 47 02.14 +08 10 22.7 00CL104 688 Cu2276 2016 03 13.24257 11 28 54.42 +04 03 26.4 22.8R 00CL104 G37 C~1pPV 2016 03 13.29163 11 28 54.20 +04 03 27.8 00CL104 G37 C~1pPV 2018 04 24.35200 11 35 41.80 +03 22 45.8 22.5z 00CL104 T09 C~7b9t 2018 04 24.39881 11 35 41.64 +03 22 46.5 22.7z 00CL104 T09 C~7b9t 2018 04 24.44256 11 35 41.52 +03 22 47.5 22.3z 00CL104 T09 C~7b9t 2018 04 24.48268 11 35 41.35 +03 22 48.7 23.2z 00CL104 T09 C~7b9t 2019 03 08.38964 11 43 31.98 +02 33 38.7 23.1r 00CL104 T09 C~8CLS 2019 03 08.40222 11 43 31.91 +02 33 39.1 23.1r 00CL104 T09 C~8CLS 2019 03 08.43185 11 43 31.79 +02 33 39.7 23.1r 00CL104 T09 C~8CLS 2020 02 01.590290 11 50 21.470 +01 50 23.71 22.9G 00CL104 T12 C~3q9S
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 -0.20 0.00 0.09
2 0.0003 0.00 -0.00 0.00 0.26
3 0.0678 0.00 0.14 0.00 0.71
4 0.0681 0.00 0.55 0.00 0.58
5 0.8768 0.00 0.20 0.00 -0.44
6 0.8794 0.00 0.31 0.00 -0.46
7 0.8796 0.00 0.13 0.00 -0.30
8 1.0453 0.00 0.25 0.00 0.62
9 1.0454 0.00 0.05 0.00 0.49
10 1.1299 0.00 -0.18 0.00 0.09
11 1.1299 0.00 -0.17 0.00 0.21
12 1.2235 0.00 0.27 0.00 0.23
13 1.2239 0.00 0.28 0.00 -0.26
14 1.9991 0.00 -0.47 0.00 -0.49
15 1.9992 0.00 -0.39 0.00 -0.44
16 2.0045 0.00 -0.26 0.00 -0.35
17 2.0046 0.00 -0.18 0.00 -0.48
18 2.0255 0.00 -0.34 0.00 0.02
19 2.0255 0.00 -0.44 0.00 0.14
20 3.1479 0.00 -0.24 0.00 -0.40
21 3.1479 0.00 -0.04 0.00 -0.32
22 3.1479 0.00 0.09 0.00 -0.37
23 4.1146 0.00 0.44 0.00 0.23
24 4.1148 0.00 0.10 0.00 0.23
25 7.0280 0.00 -0.36 0.00 -0.06
26 7.0282 0.00 0.23 0.00 0.24
27 16.1009 0.00 0.29 0.00 0.20
28 16.1010 0.00 0.24 0.00 0.22
29 18.2148 0.00 0.10 0.00 -0.06
30 18.2149 0.00 -0.07 0.00 -0.27
31 18.2151 0.00 0.20 0.00 -0.12
32 18.2152 0.00 -0.46 0.00 0.30
33 19.0856 0.00 0.04 0.00 0.06
34 19.0856 0.00 -0.19 0.00 0.11
35 19.0857 0.00 -0.06 0.00 -0.13
36 19.9896 0.00 0.07 0.00 -0.08
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.
00CL104 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 44.346 44.346 44.346 ecceobj 0.079 0.079 0.079 incobj 1.247 1.247 1.247 qmin 39.859 39.874 39.844 qmax 49.328 49.329 49.313 amean 44.474 44.474 44.474 amin 44.116 44.118 44.118 amax 44.863 44.858 44.858 emean 0.084 0.084 0.084 emin 0.068 0.068 0.068 emax 0.100 0.100 0.100 imean 1.357 1.357 1.357 imin 0.586 0.586 0.586 imax 2.026 2.025 2.026 excite_mean 0.088 0.088 0.088 fracstop 1.000 1.000 1.000 cjmean 3.098 3.098 3.098 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 207.5 207.5 207.5 kozaiamp 179.9 180.0 180.0