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: 594994
# Created Fri Apr 26 01:09:01 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 38 observations of 38
# Arc: 21.11y
# First observation: 2000/08/25
# Last observation: 2021/10/03
# Chi-squared of fit: 22.05 DOF: 70 RMS: 0.13
# Min/Max residuals: -0.32 0.84
# Exact a, adot, b, bdot, g, gdot:
1.375150E-05 2.029696E-02 -7.226852E-07 -2.229751E-04 2.317868E-02 3.606375E-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
1.497627 -8.575759 0.334891 0.024687 -0.950214 2451781.794373
# Heliocentric elements and errors
Epoch: 2451782.5000 = 2000/08/26
Mean Anomaly: 115.69093 +/- 0.000
Argument of Peri: 338.41224 +/- 0.000
Long of Asc Node: 238.64478 +/- 0.000
Inclination: 1.58403 +/- 0.000
Eccentricity: 0.19909427 +/- 0.0000
Semi-Major Axis: 39.57669073 +/- 0.0000
Time of Perihelion: 2422557.5039 +/- 0.0
Perihelion: 31.69719826 +/- 0.0000
Aphelion: 47.45618320 +/- 0.0000
Period (y) 248.9817 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 43.54184992 +/- 0.0000
Ecliptic Y -6.89915280 +/- 0.0000
Ecliptic Z 1.12751668 +/- 0.0000
Ecliptic XDOT 0.00077198 +/- 0.0000
Ecliptic YDOT 0.00231238 +/- 0.0000
Ecliptic ZDOT -0.00001504 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 44.09935976 +/- 0.0000
Geocenter to KBO 43.14302406 +/- 0.0000
# Hcoef: 7.11
The following table shows the complete astrometric record for 594994. 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 (594994) followed by the observatory code and reference code for the source of the astrometry.
2000 08 25.29363 23 26 07.73 -02 01 26.0 23.1R 594994 807 Cc1045 2000 08 26.28602 23 26 03.68 -02 01 51.5 594994 807 Cc1045 2000 08 26.35777 23 26 03.39 -02 01 53.2 594994 807 Cc1045 2003 10 22.16381 23 35 02.31 -01 07 03.8 22.8R 594994 695 C~2lRJ 2003 10 22.24392 23 35 01.97 -01 07 05.9 594994 695 C~2lRJ 2015 07 14.59595 00 29 04.875 +04 29 35.47 23.8r 594994 568 C~2lRJ 2015 07 19.57506 00 29 01.507 +04 29 21.50 23.7r 594994 568 C~2lRJ 2015 08 11.48002 00 28 22.649 +04 25 43.41 23.8r 594994 568 C~2lRJ 2015 08 11.52446 00 28 22.535 +04 25 42.53 23.8r 594994 568 C~2lRJ 2015 09 08.38855 00 26 52.757 +04 16 29.44 23.7r 594994 568 C~2lRJ 2015 09 08.49278 00 26 52.343 +04 16 26.97 23.7r 594994 568 C~2lRJ 2015 09 08.53500 00 26 52.181 +04 16 25.94 23.8r 594994 568 C~2lRJ 2015 09 09.51188 00 26 48.420 +04 16 02.26 23.9w 594994 568 C~2lRJ 2015 09 10.45287 00 26 44.778 +04 15 39.20 23.9w 594994 568 C~2lRJ 2015 09 16.43732 00 26 21.036 +04 13 08.47 23.9w 594994 568 C~2lRJ 2015 10 03.36404 00 25 10.941 +04 05 36.55 23.9w 594994 568 C~2lRJ 2015 11 10.35840 00 22 48.830 +03 49 46.30 23.9w 594994 568 C~2lRJ 2016 01 01.23433 00 21 51.460 +03 42 00.02 24.0w 594994 568 C~2lRJ 2016 09 05.47023 00 30 57.688 +04 41 27.24 23.9w 594994 568 C~2lRJ 2016 09 06.42437 00 30 54.132 +04 41 04.84 24.0w 594994 568 C~2lRJ 2016 09 06.46487 00 30 53.976 +04 41 03.91 24.1w 594994 568 C~2lRJ 2016 09 25.31706 00 29 38.702 +04 33 05.68 23.7w 594994 568 C~2lRJ 2016 09 25.34339 00 29 38.595 +04 33 04.96 23.9w 594994 568 C~2lRJ 2016 09 25.44037 00 29 38.178 +04 33 02.49 23.9w 594994 568 C~2lRJ 2016 09 26.42319 00 29 34.082 +04 32 36.09 24.0w 594994 568 C~2lRJ 2016 10 30.34865 00 27 18.676 +04 17 45.16 23.9w 594994 568 C~2lRJ 2016 11 03.30427 00 27 05.048 +04 16 12.80 23.9w 594994 568 C~2lRJ 2016 11 03.35669 00 27 04.867 +04 16 11.67 24.0w 594994 568 C~2lRJ 2016 12 24.27431 00 25 39.121 +04 05 31.78 24.1w 594994 568 C~2lRJ 2017 01 02.26396 00 25 45.077 +04 05 52.16 24.1w 594994 568 C~2lRJ 2017 01 29.22410 00 26 41.872 +04 11 07.54 24.0w 594994 568 C~2lRJ 2017 09 15.44482 00 34 16.342 +05 01 27.46 24.0w 594994 568 C~2lRJ 2017 09 22.50999 00 33 47.731 +04 58 25.94 23.9w 594994 568 C~2lRJ 2017 11 22.34219 00 30 06.469 +04 33 57.51 23.6w 594994 568 C~2lRJ 2017 11 22.36828 00 30 06.398 +04 33 57.09 24.0w 594994 568 C~2lRJ 2021 10 03.279620 00 48 45.054 +06 28 04.22 23.8G 594994 G37 C~552k 2021 10 03.316370 00 48 44.895 +06 28 03.19 594994 G37 C~552k 2021 10 03.353100 00 48 44.737 +06 28 02.06 594994 G37 C~552k
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 -0.03 0.00 0.12
2 0.0027 0.00 -0.32 0.00 -0.09
3 0.0029 0.00 -0.21 0.00 0.05
4 3.1564 0.00 0.84 0.00 0.19
5 3.1566 0.00 -0.15 0.00 -0.06
6 14.8838 0.00 0.06 0.00 -0.02
7 14.8974 0.00 0.04 0.00 -0.02
8 14.9601 0.00 -0.04 0.00 -0.02
9 14.9602 0.00 -0.05 0.00 -0.24
10 15.0365 0.00 0.17 0.00 -0.09
11 15.0368 0.00 0.05 0.00 -0.05
12 15.0369 0.00 0.10 0.00 -0.06
13 15.0396 0.00 -0.00 0.00 -0.04
14 15.0422 0.00 -0.01 0.00 -0.07
15 15.0586 0.00 0.01 0.00 -0.05
16 15.1049 0.00 0.05 0.00 -0.11
17 15.2089 0.00 0.06 0.00 -0.03
18 15.3510 0.00 -0.00 0.00 -0.05
19 16.0306 0.00 0.02 0.00 0.06
20 16.0332 0.00 0.02 0.00 -0.04
21 16.0333 0.00 0.01 0.00 -0.02
22 16.0849 0.00 0.08 0.00 -0.02
23 16.0850 0.00 0.14 0.00 -0.04
24 16.0853 0.00 0.04 0.00 0.08
25 16.0880 0.00 -0.04 0.00 0.01
26 16.1808 0.00 0.00 0.00 -0.02
27 16.1917 0.00 -0.04 0.00 -0.04
28 16.1918 0.00 -0.06 0.00 0.02
29 16.3312 0.00 -0.14 0.00 -0.03
30 16.3558 0.00 -0.05 0.00 -0.02
31 16.4297 0.00 -0.02 0.00 0.18
32 17.0572 0.00 -0.03 0.00 0.06
33 17.0766 0.00 -0.11 0.00 0.05
34 17.2431 0.00 -0.08 0.00 0.09
35 17.2432 0.00 -0.21 0.00 0.10
36 21.1061 0.00 0.09 0.00 0.21
37 21.1062 0.00 0.04 0.00 0.14
38 21.1063 0.00 0.00 0.00 -0.02
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.
594994 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.644 39.644 39.644 ecceobj 0.198 0.198 0.198 incobj 1.585 1.585 1.585 qmin 30.466 30.466 30.465 qmax 48.926 48.921 48.927 amean 39.455 39.455 39.455 amin 39.097 39.096 39.098 amax 39.887 39.885 39.887 emean 0.210 0.210 0.210 emin 0.193 0.193 0.193 emax 0.227 0.227 0.227 imean 2.960 2.960 2.960 imin 2.506 2.506 2.507 imax 3.672 3.672 3.673 excite_mean 0.216 0.216 0.216 fracstop 1.000 1.000 1.000 cjmean 2.998 2.998 2.998 libcent 0 180.1 180.1 180.7 libamp 0 37.1 37.6 37.7 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 180.4 180.4 180.4 kozaiamp 179.9 180.0 180.0