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: 00AB255 # Created Tue May 7 01:09:54 2024 # Orbit generated from Bernstein formalism # Fitting 44 observations of 44 # Arc: 1.16d # First observation: 2000/01/01 # Last observation: 2000/01/02 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution # Chi-squared of fit: 25.11 DOF: 84 RMS: 0.13 # Min/Max residuals: -0.51 0.27 # Exact a, adot, b, bdot, g, gdot: 1.714773E-05 2.597945E-02 9.402133E-07 1.774610E-03 2.605942E-02 0.000000E+00 # Covariance matrix: 3.9605E-11 6.4623E-08 -5.7432E-12 -9.5232E-09 1.0976E-08 0.0000E+00 6.4623E-08 1.0560E-04 -9.3811E-09 -1.5556E-05 1.7929E-05 0.0000E+00 -5.7432E-12 -9.3811E-09 8.7056E-13 1.3730E-09 -1.5931E-09 0.0000E+00 -9.5232E-09 -1.5556E-05 1.3730E-09 2.3163E-06 -2.6417E-06 0.0000E+00 1.0976E-08 1.7929E-05 -1.5931E-09 -2.6417E-06 3.0447E-06 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 2.3287E-04 # lat0 lon0 xBary yBary zBary JD0 -20.597615 78.104882 -0.376054 -0.319287 -0.848982 2451544.812233 # Heliocentric elements and errors Epoch: 2451540.5000 = 1999/12/28 Mean Anomaly: 101.92440 +/- 208.100 Argument of Peri: 177.82614 +/- 136.902 Long of Asc Node: 156.79613 +/- 13.642 Inclination: 20.53288 +/- 0.972 Eccentricity: 0.01236202 +/- 0.5837 Semi-Major Axis: 39.12411430 +/- 19.9446 Time of Perihelion: 2426233.4884 +/- 677089.0 Perihelion: 38.64046109 +/- 30.1594 Aphelion: 39.60776751 +/- 30.4838 Period (y) 244.7231 +/- 187.13 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 7.22949402 +/- 0.4960 Ecliptic Y 36.11743370 +/- 2.3536 Ecliptic Z -13.49999089 +/- 0.9039 Ecliptic XDOT -0.00266270 +/- 0.0009 Ecliptic YDOT 0.00063419 +/- 0.0015 Ecliptic ZDOT 0.00017462 +/- 0.0006 # Distances at JD0 (AU) Heliocenter to KBO 39.22989109 +/- 2.1909 Geocenter to KBO 38.37384145 +/- 2.5695 # Hcoef: 8.87
The following table shows the complete astrometric record for 00AB255. 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 (00AB255) followed by the observatory code and reference code for the source of the astrometry.
2000 01 01.31149 05 15 27.74 +02 22 59.1 24.6R 00AB255 568 Cb9120 2000 01 01.31809 05 15 27.73 +02 22 59.1 00AB255 568 Cb9120 2000 01 01.32464 05 15 27.69 +02 22 59.2 00AB255 568 Cb9120 2000 01 01.33118 05 15 27.65 +02 22 59.2 24.9R 00AB255 568 Cb9120 2000 01 01.33767 05 15 27.63 +02 22 59.3 24.5R 00AB255 568 Cb9120 2000 01 01.34422 05 15 27.59 +02 22 59.5 24.5R 00AB255 568 Cb9120 2000 01 01.35081 05 15 27.56 +02 22 59.3 24.3R 00AB255 568 Cb9120 2000 01 01.35739 05 15 27.52 +02 22 59.4 00AB255 568 Cb9120 2000 01 01.36394 05 15 27.48 +02 22 59.6 00AB255 568 Cb9120 2000 01 01.37054 05 15 27.46 +02 22 59.6 00AB255 568 Cb9120 2000 01 01.37708 05 15 27.42 +02 22 59.6 24.5R 00AB255 568 Cb9120 2000 01 01.38365 05 15 27.40 +02 22 59.7 00AB255 568 Cb9120 2000 01 01.39026 05 15 27.37 +02 22 59.7 00AB255 568 Cb9120 2000 01 01.39682 05 15 27.33 +02 22 59.7 00AB255 568 Cb9120 2000 01 01.40336 05 15 27.30 +02 22 59.8 00AB255 568 Cb9120 2000 01 01.40994 05 15 27.26 +02 22 59.8 00AB255 568 Cb9120 2000 01 01.41649 05 15 27.24 +02 22 59.9 00AB255 568 Cb9120 2000 01 01.42304 05 15 27.21 +02 23 00.1 00AB255 568 Cb9120 2000 01 01.42969 05 15 27.18 +02 23 00.1 00AB255 568 Cb9120 2000 01 01.43628 05 15 27.15 +02 23 00.0 00AB255 568 Cb9120 2000 01 01.44281 05 15 27.11 +02 23 00.0 00AB255 568 Cb9120 2000 01 01.44939 05 15 27.08 +02 23 00.0 00AB255 568 Cb9120 2000 01 01.45652 05 15 27.05 +02 23 00.0 00AB255 568 Cb9120 2000 01 01.46321 05 15 27.01 +02 23 00.3 24.7R 00AB255 568 Cb9120 2000 01 01.46976 05 15 26.97 +02 23 00.3 24.5R 00AB255 568 Cb9120 2000 01 01.47634 05 15 26.95 +02 23 00.3 24.7R 00AB255 568 Cb9120 2000 01 01.48362 05 15 26.91 +02 23 00.4 24.3R 00AB255 568 Cb9120 2000 01 01.49018 05 15 26.88 +02 23 00.4 24.1R 00AB255 568 Cb9120 2000 01 01.49668 05 15 26.84 +02 23 00.5 24.3R 00AB255 568 Cb9120 2000 01 01.50318 05 15 26.82 +02 23 00.4 24.5R 00AB255 568 Cb9120 2000 01 01.50972 05 15 26.79 +02 23 00.7 24.3R 00AB255 568 Cb9120 2000 01 01.51635 05 15 26.75 +02 23 00.6 00AB255 568 Cb9120 2000 01 02.27831 05 15 23.04 +02 23 06.6 00AB255 568 Cb9120 2000 01 02.29311 05 15 22.95 +02 23 06.5 00AB255 568 Cb9120 2000 01 02.30651 05 15 22.88 +02 23 06.8 00AB255 568 Cb9120 2000 01 02.31965 05 15 22.85 +02 23 07.0 00AB255 568 Cb9120 2000 01 02.32638 05 15 22.82 +02 23 07.0 00AB255 568 Cb9120 2000 01 02.35243 05 15 22.70 +02 23 07.2 00AB255 568 Cb9120 2000 01 02.36549 05 15 22.63 +02 23 07.2 00AB255 568 Cb9120 2000 01 02.38565 05 15 22.53 +02 23 07.6 00AB255 568 Cb9120 2000 01 02.40519 05 15 22.42 +02 23 07.7 00AB255 568 Cb9120 2000 01 02.43962 05 15 22.27 +02 23 07.8 00AB255 568 Cb9120 2000 01 02.45277 05 15 22.21 +02 23 08.1 00AB255 568 Cb9120 2000 01 02.47221 05 15 22.10 +02 23 08.2 00AB255 568 Cb9120
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 -0.29 0.00 0.03
2 0.0000 -0.15 0.05 0.01 -0.05
3 0.0000 -0.74 -0.06 0.16 0.01
4 0.0001 -1.34 -0.17 0.21 -0.03
5 0.0001 -1.63 0.02 0.33 0.01
6 0.0001 -2.21 -0.08 0.58 0.17
7 0.0001 -2.67 -0.06 0.42 -0.09
8 0.0001 -3.26 -0.16 0.57 -0.03
9 0.0001 -3.84 -0.26 0.82 0.13
10 0.0002 -4.14 -0.07 0.84 0.07
11 0.0002 -4.74 -0.19 0.89 0.03
12 0.0002 -5.03 0.01 1.02 0.06
13 0.0002 -5.48 0.04 1.05 0.01
14 0.0002 -6.07 -0.07 1.10 -0.03
15 0.0003 -6.51 -0.03 1.24 0.02
16 0.0003 -7.11 -0.14 1.29 -0.02
17 0.0003 -7.40 0.05 1.41 0.01
18 0.0003 -7.83 0.10 1.65 0.16
19 0.0003 -8.28 0.14 1.69 0.11
20 0.0003 -8.74 0.17 1.62 -0.05
21 0.0004 -9.34 0.06 1.67 -0.09
22 0.0004 -9.78 0.09 1.71 -0.14
23 0.0004 -10.23 0.17 1.75 -0.20
24 0.0004 -10.81 0.09 2.09 0.06
25 0.0004 -11.40 -0.03 2.14 0.02
26 0.0005 -11.70 0.15 2.17 -0.05
27 0.0005 -12.29 0.10 2.32 0.00
28 0.0005 -12.74 0.13 2.35 -0.05
29 0.0005 -13.33 0.02 2.50 0.01
30 0.0005 -13.63 0.19 2.43 -0.15
31 0.0005 -14.06 0.24 2.76 0.09
32 0.0006 -14.66 0.12 2.71 -0.05
33 0.0026 -69.59 -0.20 13.26 0.02
34 0.0027 -70.94 -0.47 13.27 -0.18
35 0.0027 -71.96 -0.51 13.65 0.02
36 0.0028 -72.39 0.02 13.89 0.07
37 0.0028 -72.84 0.06 13.92 0.01
38 0.0028 -74.61 0.19 14.27 -0.01
39 0.0029 -75.66 0.10 14.36 -0.11
40 0.0029 -77.12 0.11 14.88 0.13
41 0.0030 -78.76 -0.10 15.11 0.09
42 0.0031 -80.99 0.18 15.40 -0.12
43 0.0031 -81.86 0.27 15.77 0.07
44 0.0032 -83.49 0.05 16.01 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.
00AB255 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