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: 02TZ300 # Created Sat Apr 27 01:10:53 2024 # Orbit generated from Bernstein formalism # Fitting 73 observations of 73 # Arc: 59.01d # First observation: 2002/10/06 # Last observation: 2002/12/04 Preliminary a, adot, b, bdot, g, gdot: -0.000001 0.022856 0.000000 0.001049 0.023486 0.000000 # WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution # WARNING Fitting with energy constraint # WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution # Chi-squared of fit: 53.20 DOF: 141 RMS: 0.15 # Min/Max residuals: -0.54 0.40 # Exact a, adot, b, bdot, g, gdot: 9.244250E-06 1.375664E-02 8.835122E-07 1.109239E-03 2.199991E-02 -1.275850E-02 # Covariance matrix: 9.3862E-12 1.2574E-08 2.5299E-13 -7.9858E-11 2.1092E-09 -8.0570E-09 1.2574E-08 1.6939E-05 3.4074E-10 -1.0780E-07 2.8377E-06 -1.2020E-05 2.5299E-13 3.4074E-10 3.0113E-14 -2.3199E-12 5.7087E-11 -2.4028E-10 -7.9858E-11 -1.0780E-07 -2.3199E-12 6.9437E-10 -1.8044E-08 8.1420E-08 2.1092E-09 2.8377E-06 5.7087E-11 -1.8044E-08 4.7565E-07 -1.9312E-06 -8.0570E-09 -1.2020E-05 -2.4028E-10 8.1420E-08 -1.9312E-06 3.4301E-05 # lat0 lon0 xBary yBary zBary JD0 -1.566729 30.552957 0.306666 -0.026032 -0.950796 2452553.943653 # Heliocentric elements and errors Epoch: 2452550.5000 = 2002/10/03 Mean Anomaly: 297.43254 +/- 71.028 Argument of Peri: 123.28228 +/- 31.241 Long of Asc Node: 48.38714 +/- 5.450 Inclination: 4.90038 +/- 1.416 Eccentricity: 0.69239213 +/- 0.1238 Semi-Major Axis: 40.80570820 +/- 16.7710 Time of Perihelion: 2469097.7490 +/- 15773.6 Perihelion: 12.55215681 +/- 7.2211 Aphelion: 69.05925959 +/- 28.8293 Period (y) 260.6691 +/- 160.70 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 40.10318990 +/- 1.2267 Ecliptic Y 23.32243890 +/- 0.7240 Ecliptic Z -1.24274131 +/- 0.0390 Ecliptic XDOT -0.00224139 +/- 0.0007 Ecliptic YDOT 0.00066629 +/- 0.0004 Ecliptic ZDOT 0.00018161 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 46.40847339 +/- 1.1207 Geocenter to KBO 45.45472423 +/- 1.4249 # Hcoef: 7.48
The following table shows the complete astrometric record for 02TZ300. 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 (02TZ300) followed by the observatory code and reference code for the source of the astrometry.
2002 10 06.44291 01 55 59.01 +10 11 51.3 24.7R 02TZ300 568 Cg6275 2002 10 06.44796 01 55 58.97 +10 11 51.1 02TZ300 568 Cg6275 2002 10 06.45279 01 55 58.95 +10 11 51.1 02TZ300 568 Cg6275 2002 10 06.46244 01 55 58.90 +10 11 50.7 02TZ300 568 Cg6275 2002 10 06.46727 01 55 58.88 +10 11 50.6 02TZ300 568 Cg6275 2002 10 06.47210 01 55 58.86 +10 11 50.4 02TZ300 568 Cg6275 2002 10 06.47692 01 55 58.86 +10 11 50.5 02TZ300 568 Cg6275 2002 10 06.48179 01 55 58.85 +10 11 50.3 02TZ300 568 Cg6275 2002 10 06.48662 01 55 58.83 +10 11 50.3 02TZ300 568 Cg6275 2002 10 06.49145 01 55 58.80 +10 11 50.1 02TZ300 568 Cg6275 2002 10 06.49760 01 55 58.76 +10 11 49.9 02TZ300 568 Cg6275 2002 10 06.51691 01 55 58.67 +10 11 49.4 02TZ300 568 Cg6275 2002 10 06.52261 01 55 58.66 +10 11 49.3 02TZ300 568 Cg6275 2002 10 06.52743 01 55 58.65 +10 11 49.3 02TZ300 568 Cg6275 2002 10 06.53226 01 55 58.62 +10 11 49.2 02TZ300 568 Cg6275 2002 10 06.53708 01 55 58.61 +10 11 49.1 02TZ300 568 Cg6275 2002 10 06.54193 01 55 58.58 +10 11 48.8 02TZ300 568 Cg6275 2002 10 06.54678 01 55 58.55 +10 11 48.8 02TZ300 568 Cg6275 2002 10 06.56757 01 55 58.46 +10 11 48.3 02TZ300 568 Cg6275 2002 10 06.57240 01 55 58.44 +10 11 48.2 02TZ300 568 Cg6275 2002 10 06.57722 01 55 58.42 +10 11 48.2 02TZ300 568 Cg6275 2002 10 06.58205 01 55 58.41 +10 11 48.4 02TZ300 568 Cg6275 2002 10 06.58688 01 55 58.38 +10 11 48.0 02TZ300 568 Cg6275 2002 10 06.59170 01 55 58.37 +10 11 47.8 02TZ300 568 Cg6275 2002 10 06.59653 01 55 58.32 +10 11 47.7 02TZ300 568 Cg6275 2002 10 06.61671 01 55 58.25 +10 11 47.2 02TZ300 568 Cg6275 2002 10 07.29978 01 55 55.36 +10 11 31.2 02TZ300 568 Cg6275 2002 10 07.30461 01 55 55.30 +10 11 31.1 02TZ300 568 Cg6275 2002 10 07.30943 01 55 55.31 +10 11 30.9 02TZ300 568 Cg6275 2002 10 07.31635 01 55 55.24 +10 11 30.8 02TZ300 568 Cg6275 2002 10 07.32117 01 55 55.23 +10 11 30.5 02TZ300 568 Cg6275 2002 10 07.32603 01 55 55.26 +10 11 30.8 02TZ300 568 Cg6275 2002 10 07.38074 01 55 55.00 +10 11 29.3 02TZ300 568 Cg6275 2002 10 07.38557 01 55 55.00 +10 11 29.3 02TZ300 568 Cg6275 2002 10 07.39039 01 55 54.95 +10 11 29.1 02TZ300 568 Cg6275 2002 10 07.39522 01 55 54.94 +10 11 29.0 02TZ300 568 Cg6275 2002 10 07.40007 01 55 54.91 +10 11 29.0 02TZ300 568 Cg6275 2002 10 07.42934 01 55 54.78 +10 11 28.1 02TZ300 568 Cg6275 2002 10 07.43417 01 55 54.76 +10 11 28.2 02TZ300 568 Cg6275 2002 10 07.43899 01 55 54.75 +10 11 27.9 02TZ300 568 Cg6275 2002 10 07.44382 01 55 54.73 +10 11 27.9 02TZ300 568 Cg6275 2002 10 07.44865 01 55 54.68 +10 11 27.9 02TZ300 568 Cg6275 2002 10 07.46854 01 55 54.61 +10 11 27.2 02TZ300 568 Cg6275 2002 10 07.48301 01 55 54.54 +10 11 26.7 02TZ300 568 Cg6275 2002 10 07.48784 01 55 54.52 +10 11 26.7 02TZ300 568 Cg6275 2002 10 07.49266 01 55 54.52 +10 11 26.7 02TZ300 568 Cg6275 2002 10 07.49749 01 55 54.50 +10 11 26.6 02TZ300 568 Cg6275 2002 10 07.50232 01 55 54.47 +10 11 26.5 02TZ300 568 Cg6275 2002 10 07.50714 01 55 54.46 +10 11 26.6 02TZ300 568 Cg6275 2002 10 07.51197 01 55 54.42 +10 11 26.3 02TZ300 568 Cg6275 2002 10 07.51720 01 55 54.40 +10 11 25.8 02TZ300 568 Cg6275 2002 10 07.53167 01 55 54.32 +10 11 25.7 02TZ300 568 Cg6275 2002 10 07.55497 01 55 54.24 +10 11 25.2 02TZ300 568 Cg6275 2002 10 07.56462 01 55 54.21 +10 11 25.0 02TZ300 568 Cg6275 2002 10 07.56945 01 55 54.18 +10 11 25.2 02TZ300 568 Cg6275 2002 10 07.57427 01 55 54.16 +10 11 24.8 02TZ300 568 Cg6275 2002 10 07.57910 01 55 54.14 +10 11 24.9 02TZ300 568 Cg6275 2002 10 07.58393 01 55 54.10 +10 11 24.7 02TZ300 568 Cg6275 2002 10 07.59288 01 55 54.06 +10 11 24.3 02TZ300 568 Cg6275 2002 10 07.60735 01 55 54.01 +10 11 24.0 02TZ300 568 Cg6275 2002 10 07.61218 01 55 54.01 +10 11 24.1 02TZ300 568 Cg6275 2002 10 07.61700 01 55 53.97 +10 11 23.8 02TZ300 568 Cg6275 2002 10 07.62183 01 55 53.96 +10 11 23.7 02TZ300 568 Cg6275 2002 10 07.62666 01 55 53.93 +10 11 23.7 02TZ300 568 Cg6275 2002 12 04.199878 01 51 53.13 +09 50 23.6 23.7R 02TZ300 568 C~5bf3 2002 12 04.224009 01 51 53.04 +09 50 23.3 02TZ300 568 C~5bf3 2002 12 04.243316 01 51 52.98 +09 50 22.8 02TZ300 568 C~5bf3 2002 12 04.272553 01 51 52.89 +09 50 22.6 23.6R 02TZ300 568 C~5bf3 2002 12 04.291856 01 51 52.82 +09 50 22.1 02TZ300 568 C~5bf3 2002 12 04.317654 01 51 52.74 +09 50 21.9 02TZ300 568 C~5bf3 2002 12 04.341825 01 51 52.66 +09 50 21.3 02TZ300 568 C~5bf3 2002 12 04.365017 01 51 52.58 +09 50 21.0 02TZ300 568 C~5bf3 2002 12 04.452053 01 51 52.30 +09 50 19.6 23.3R 02TZ300 568 C~5bf3
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 0.13 0.00 -0.02
2 0.0000 -0.62 -0.15 0.02 -0.00
3 0.0000 -0.90 -0.09 0.12 0.10
4 0.0001 -1.73 -0.27 0.00 -0.02
5 0.0001 -2.04 -0.25 0.01 -0.02
6 0.0001 -2.39 -0.27 -0.07 -0.10
7 0.0001 -2.35 0.10 0.02 -0.01
8 0.0001 -2.56 0.22 -0.12 -0.15
9 0.0001 -2.84 0.27 -0.01 -0.05
10 0.0001 -3.32 0.12 -0.05 -0.08
11 0.0001 -3.95 -0.09 -0.03 -0.07
12 0.0002 -5.37 -0.19 -0.03 -0.08
13 0.0002 -5.54 0.03 -0.08 -0.13
14 0.0002 -5.68 0.22 -0.03 -0.08
15 0.0002 -6.13 0.09 0.04 -0.02
16 0.0003 -6.30 0.25 -0.01 -0.06
17 0.0003 -6.82 0.06 -0.13 -0.19
18 0.0003 -7.24 -0.02 0.02 -0.04
19 0.0003 -8.66 -0.03 0.01 -0.05
20 0.0004 -8.97 -0.01 0.02 -0.04
21 0.0004 -9.24 0.04 0.13 0.06
22 0.0004 -9.31 0.30 0.36 0.30
23 0.0004 -9.87 0.07 0.14 0.08
24 0.0004 -10.08 0.19 0.01 -0.06
25 0.0004 -10.80 -0.21 0.17 0.10
26 0.0005 -11.95 0.02 0.06 -0.01
27 0.0023 -57.51 0.14 -0.09 -0.07
28 0.0024 -58.38 -0.40 0.13 0.14
29 0.0024 -58.31 -0.00 -0.11 -0.10
30 0.0024 -59.31 -0.54 0.15 0.16
31 0.0024 -59.56 -0.45 -0.08 -0.07
32 0.0024 -59.04 0.40 0.05 0.06
33 0.0026 -63.16 0.01 -0.02 -0.04
34 0.0026 -63.16 0.34 -0.02 -0.04
35 0.0026 -63.92 -0.09 0.05 0.03
36 0.0026 -64.09 0.07 0.01 -0.02
37 0.0026 -64.51 -0.02 0.16 0.13
38 0.0027 -66.62 -0.13 -0.01 -0.06
39 0.0027 -66.86 -0.04 0.18 0.14
40 0.0027 -67.10 0.05 -0.05 -0.09
41 0.0027 -67.38 0.10 0.06 0.01
42 0.0028 -68.07 -0.26 0.31 0.26
43 0.0028 -69.28 -0.11 0.02 -0.05
44 0.0028 -70.43 -0.26 -0.09 -0.16
45 0.0029 -70.70 -0.20 0.01 -0.06
46 0.0029 -70.70 0.13 0.01 -0.06
47 0.0029 -71.02 0.15 0.02 -0.05
48 0.0029 -71.47 0.03 0.08 0.00
49 0.0029 -71.57 0.26 0.23 0.15
50 0.0029 -72.23 -0.07 0.15 0.07
51 0.0029 -72.68 -0.16 -0.22 -0.30
52 0.0030 -73.82 -0.31 0.10 0.01
53 0.0030 -75.10 0.00 0.04 -0.05
54 0.0031 -75.59 0.18 0.01 -0.09
55 0.0031 -75.93 0.16 0.35 0.25
56 0.0031 -76.35 0.08 0.08 -0.02
57 0.0031 -76.59 0.17 0.28 0.17
58 0.0031 -77.21 -0.13 0.29 0.19
59 0.0031 -77.91 -0.21 0.13 0.02
60 0.0032 -78.70 -0.01 0.10 -0.01
61 0.0032 -78.67 0.35 0.19 0.09
62 0.0032 -79.33 0.02 0.12 0.01
63 0.0032 -79.50 0.18 0.08 -0.03
64 0.0032 -79.91 0.09 0.23 0.12
65 0.1609 -3853.40 0.04 62.94 -0.02
66 0.1609 -3854.76 -0.08 63.13 0.10
67 0.1610 -3855.76 -0.09 62.97 -0.10
68 0.1611 -3857.08 0.09 63.25 0.11
69 0.1611 -3858.22 -0.06 63.14 -0.05
70 0.1612 -3859.40 0.08 63.37 0.12
71 0.1613 -3860.72 0.00 63.22 -0.09
72 0.1613 -3861.93 -0.02 63.36 -0.01
73 0.1616 -3866.30 0.05 63.50 -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.
02TZ300 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0