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: 149349
# Created Sun Dec 22 02:06:58 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 53 observations of 53
# Arc: 21.89y
# First observation: 2002/11/09
# Last observation: 2024/09/28
# Chi-squared of fit: 81.21 DOF: 100 RMS: 0.22
# Min/Max residuals: -0.87 0.53
# Exact a, adot, b, bdot, g, gdot:
1.454083E-05 2.514150E-02 -4.189796E-06 -2.984889E-03 2.558388E-02 -6.315865E-03
# 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
2.039617 27.762341 -0.314699 0.033290 -0.935619 2452587.704403
# Heliocentric elements and errors
Epoch: 2452588.5000 = 2002/11/10
Mean Anomaly: 296.98521 +/- 0.000
Argument of Peri: 254.24319 +/- 0.000
Long of Asc Node: 224.52945 +/- 0.000
Inclination: 7.05914 +/- 0.000
Eccentricity: 0.24323367 +/- 0.0000
Semi-Major Axis: 42.42147034 +/- 0.0000
Time of Perihelion: 2470253.6372 +/- 0.0
Perihelion: 32.10314036 +/- 0.0000
Aphelion: 52.73980032 +/- 0.0000
Period (y) 276.3037 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 35.24639606 +/- 0.0000
Ecliptic Y 18.91549752 +/- 0.0000
Ecliptic Z 1.39098146 +/- 0.0000
Ecliptic XDOT -0.00184833 +/- 0.0000
Ecliptic YDOT 0.00206800 +/- 0.0000
Ecliptic ZDOT -0.00034307 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.02563229 +/- 0.0000
Geocenter to KBO 39.08731164 +/- 0.0000
# Hcoef: 6.52
The following table shows the complete astrometric record for 149349. 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 (149349) followed by the observatory code and reference code for the source of the astrometry.
2002 11 09.20366 01 40 07.30 +12 34 52.3 22.2R 149349 695 Cg8319 2002 11 09.28734 01 40 06.92 +12 34 49.6 149349 695 Cg8319 2002 11 30.27880 01 38 42.46 +12 25 35.4 22.6R 149349 568 Cg8319 2002 11 30.34751 01 38 42.22 +12 25 33.8 149349 568 Cg8319 2002 12 01.27244 01 38 39.10 +12 25 12.2 149349 568 Cg8319 2003 10 23.18473 01 47 18.51 +13 04 45.0 21.9R 149349 695 Cj4694 2003 10 23.27963 01 47 18.04 +13 04 42.2 149349 695 Cj4694 2003 11 24.15715 01 44 51.95 +12 49 40.9 21.8R 149349 695 Cj4694 2003 11 24.22581 01 44 51.67 +12 49 38.4 149349 695 Cj4694 2004 11 09.18308 01 51 46.24 +13 17 22.8 22.0R 149349 695 Cl9844 2004 11 10.25916 01 51 41.17 +13 16 52.2 149349 695 Cl9844 2005 09 30.33653 02 00 59.35 +13 56 52.3 22.6R 149349 688 Co3857 2005 09 30.42808 02 00 58.90 +13 56 50.2 149349 688 Co3857 2006 12 24.11328 02 01 03.73 +13 42 02.1 22.7R 149349 688 Ct2062 2006 12 24.22147 02 01 03.44 +13 42 00.8 149349 688 Ct2062 2010 11 03.44841 02 29 38.054 +15 21 16.71 22.5w 149349 F51 C~1vqk 2010 11 03.47391 02 29 37.924 +15 21 16.05 22.1w 149349 F51 C~1vqk 2010 11 03.48655 02 29 37.857 +15 21 15.48 22.6w 149349 F51 C~1vqk 2012 12 07.23645 02 40 03.893 +15 44 01.86 22.3w 149349 F51 C~1vqk 2012 12 07.25146 02 40 03.821 +15 44 01.80 22.6w 149349 F51 C~1vqk 2012 12 07.26642 02 40 03.781 +15 44 01.43 22.4w 149349 F51 C~1vqk 2012 12 07.28150 02 40 03.697 +15 44 01.18 22.4w 149349 F51 C~1vqk 2013 10 05.51606 02 52 06.78 +16 27 38.5 21.9R 149349 695 C~0zw1 2013 10 06.35505 02 52 03.13 +16 27 20.7 149349 695 C~0zw1 2013 10 06.47497 02 52 02.62 +16 27 18.3 149349 695 C~0zw1 2013 11 24.29410 02 47 51.858 +16 07 07.03 22.3w 149349 F51 C~1vqk 2013 11 24.30739 02 47 51.784 +16 07 06.69 22.4w 149349 F51 C~1vqk 2013 11 24.32069 02 47 51.710 +16 07 06.24 22.5w 149349 F51 C~1vqk 2013 11 24.33403 02 47 51.655 +16 07 05.89 22.4w 149349 F51 C~1vqk 2014 07 28.60597 03 00 18.335 +16 52 39.66 22.4w 149349 F51 C~1vqk 2014 07 28.60861 03 00 18.351 +16 52 39.62 22.5w 149349 F51 C~1vqk 2014 07 28.61125 03 00 18.357 +16 52 40.04 22.5w 149349 F51 C~1vqk 2014 07 28.61387 03 00 18.368 +16 52 40.08 22.3w 149349 F51 C~1vqk 2014 11 17.46323 02 55 21.892 +16 27 18.09 22.4w 149349 F51 C~1vqk 2014 11 17.47689 02 55 21.790 +16 27 17.81 22.5w 149349 F51 C~1vqk 2014 11 17.49059 02 55 21.709 +16 27 17.70 22.4w 149349 F51 C~1vqk 2014 11 17.50426 02 55 21.651 +16 27 16.98 22.5w 149349 F51 C~1vqk 2014 12 13.34976 02 53 14.755 +16 17 17.34 22.5w 149349 F51 C~1vqk 2014 12 13.36267 02 53 14.702 +16 17 16.87 22.4w 149349 F51 C~1vqk 2014 12 13.37561 02 53 14.651 +16 17 16.61 22.4w 149349 F51 C~1vqk 2017 08 19.60939 03 21 40.556 +17 38 22.96 149349 568 C~2N74 2023 11 18.80420 04 02 04.90 +18 26 20.7 22.0w 149349 O18 C~7aHP 2023 11 18.80528 04 02 04.89 +18 26 20.4 22.4w 149349 O18 C~7aHP 2023 11 18.81068 04 02 04.85 +18 26 20.5 22.0w 149349 O18 C~7aHP 2023 11 18.81175 04 02 04.85 +18 26 20.5 22.5w 149349 O18 C~7aHP 2023 11 18.81707 04 02 04.82 +18 26 20.2 21.9w 149349 O18 C~7aHP 2023 11 18.81812 04 02 04.81 +18 26 20.1 22.3w 149349 O18 C~7aHP 2023 11 19.85147 04 01 58.73 +18 26 00.3 21.9w 149349 O18 C~7aHP 2023 11 19.85803 04 01 58.70 +18 26 00.2 21.6w 149349 O18 C~7aHP 2023 11 19.86458 04 01 58.65 +18 26 00.1 22.0w 149349 O18 C~7aHP 2024 09 28.484681 04 13 51.873 +18 48 30.55 22.4w 149349 F51 C~8K8F 2024 09 28.497199 04 13 51.827 +18 48 30.69 22.5w 149349 F51 C~8K8G 2024 09 28.522656 04 13 51.794 +18 48 30.25 22.3w 149349 F51 C~8K8G
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 0.02 0.00 0.53
2 0.0002 0.00 0.10 0.00 0.22
3 0.0577 0.00 0.32 0.00 -0.41
4 0.0579 0.00 0.33 0.00 -0.40
5 0.0604 0.00 0.25 0.00 -0.47
6 0.9527 0.00 -0.01 0.00 -0.10
7 0.9530 0.00 0.05 0.00 -0.14
8 1.0403 0.00 -0.32 0.00 0.22
9 1.0404 0.00 -0.37 0.00 -0.52
10 2.0013 0.00 0.51 0.00 0.12
11 2.0043 0.00 0.09 0.00 0.09
12 2.8915 0.00 0.07 0.00 0.05
13 2.8918 0.00 -0.48 0.00 0.19
14 4.1230 0.00 0.03 0.00 0.02
15 4.1233 0.00 -0.87 0.00 0.33
16 7.9842 0.00 0.04 0.00 -0.01
17 7.9843 0.00 0.13 0.00 0.03
18 7.9843 0.00 0.14 0.00 -0.19
19 10.0781 0.00 -0.08 0.00 -0.07
20 10.0782 0.00 -0.18 0.00 0.19
21 10.0782 0.00 0.20 0.00 0.15
22 10.0782 0.00 -0.06 0.00 0.23
23 10.9057 0.00 -0.28 0.00 0.25
24 10.9080 0.00 -0.43 0.00 0.18
25 10.9083 0.00 -0.04 0.00 0.34
26 11.0420 0.00 0.09 0.00 0.09
27 11.0420 0.00 0.01 0.00 0.07
28 11.0421 0.00 -0.06 0.00 -0.05
29 11.0421 0.00 0.15 0.00 -0.07
30 11.7164 0.00 -0.02 0.00 -0.12
31 11.7164 0.00 0.13 0.00 -0.18
32 11.7164 0.00 0.13 0.00 0.22
33 11.7164 0.00 0.20 0.00 0.24
34 12.0226 0.00 0.38 0.00 -0.27
35 12.0227 0.00 -0.03 0.00 -0.20
36 12.0227 0.00 -0.12 0.00 0.04
37 12.0227 0.00 0.13 0.00 -0.34
38 12.0935 0.00 -0.11 0.00 0.18
39 12.0935 0.00 -0.07 0.00 -0.03
40 12.0936 0.00 0.00 0.00 -0.02
41 14.7773 0.00 0.10 0.00 -0.06
42 21.0256 0.00 0.07 0.00 0.10
43 21.0256 0.00 0.02 0.00 -0.18
44 21.0256 0.00 -0.10 0.00 0.03
45 21.0256 0.00 -0.01 0.00 0.05
46 21.0256 0.00 0.02 0.00 -0.15
47 21.0256 0.00 -0.04 0.00 -0.23
48 21.0285 0.00 -0.00 0.00 -0.07
49 21.0285 0.00 0.13 0.00 -0.04
50 21.0285 0.00 -0.03 0.00 -0.01
51 21.8871 0.00 -0.07 0.00 -0.12
52 21.8872 0.00 -0.30 0.00 0.17
53 21.8873 0.00 0.14 0.00 0.03
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.
149349 quality flag:3 Type: 5:3EE 5:3EE 5:3EE axisobj 42.659 42.658 42.659 ecceobj 0.241 0.241 0.241 incobj 7.046 7.046 7.046 qmin 31.663 31.663 31.662 qmax 53.362 53.362 53.362 amean 42.326 42.327 42.326 amin 41.956 41.956 41.956 amax 42.772 42.772 42.772 emean 0.235 0.235 0.235 emin 0.221 0.221 0.221 emax 0.248 0.248 0.248 imean 8.299 8.299 8.299 imin 7.887 7.887 7.887 imax 8.610 8.610 8.610 excite_mean 0.276 0.276 0.276 fracstop 1.000 1.000 1.000 cjmean 2.992 2.992 2.992 libcent 0 180.7 180.7 180.8 libamp 0 14.9 14.8 15.1 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 189.2 189.2 189.3 kozaiamp 180.0 180.0 180.0