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: 135571 # Created Sat Apr 20 01:07:30 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 21 observations of 21 # Arc: 4.21y # First observation: 2002/04/08 # Last observation: 2006/06/22 # Chi-squared of fit: 63.27 DOF: 36 RMS: 0.31 # Min/Max residuals: -1.08 0.65 # Exact a, adot, b, bdot, g, gdot: 1.888578E-05 2.982464E-02 -6.430907E-06 -7.643406E-03 2.680595E-02 -5.098588E-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 -2.818554 -132.933800 0.481684 -0.043345 -0.879493 2452372.644023 # Heliocentric elements and errors Epoch: 2452372.5000 = 2002/04/08 Mean Anomaly: 341.05545 +/- 0.000 Argument of Peri: 230.94337 +/- 0.000 Long of Asc Node: 35.77172 +/- 0.000 Inclination: 14.69833 +/- 0.000 Eccentricity: 0.34786132 +/- 0.0000 Semi-Major Axis: 55.01083831 +/- 0.0000 Time of Perihelion: 2460214.9650 +/- 0.0 Perihelion: 35.87469567 +/- 0.0000 Aphelion: 74.14698094 +/- 0.0000 Period (y) 408.0192 +/- 0.00 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -26.33098727 +/- 0.0000 Ecliptic Y -27.59114936 +/- 0.0000 Ecliptic Z -1.83466968 +/- 0.0000 Ecliptic XDOT 0.00260229 +/- 0.0000 Ecliptic YDOT -0.00166738 +/- 0.0000 Ecliptic ZDOT -0.00075390 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 38.18334063 +/- 0.0000 Geocenter to KBO 37.30528435 +/- 0.0000 # Hcoef: 7.10
The following table shows the complete astrometric record for 135571. 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 (135571) followed by the observatory code and reference code for the source of the astrometry.
2002 04 08.14328 14 55 00.85 -19 37 58.4 22.0R 135571 807 Cf5154 2002 04 09.25532 14 54 55.71 -19 37 44.9 135571 807 Cf5154 2002 04 09.31861 14 54 55.42 -19 37 44.2 135571 807 Cf5154 2002 06 18.18615 14 49 12.50 -19 17 49.7 23.0R 135571 695 Ck7379 2002 06 18.22597 14 49 12.39 -19 17 48.9 23.1R 135571 695 Ck7379 2002 06 19.20584 14 49 08.72 -19 17 34.7 135571 695 Ck7379 2002 08 09.05482 14 48 03.36 -19 12 55.1 22.2R 135571 807 Cg3254 2002 08 10.05266 14 48 04.67 -19 13 00.5 135571 807 Cg3254 2002 08 11.05696 14 48 06.11 -19 13 06.2 135571 807 Cg3254 2002 08 12.05154 14 48 07.64 -19 13 12.6 135571 807 Cg3254 2003 05 31.37512 14 56 55.59 -20 17 57.0 22.8R 135571 568 Ci1475 2003 05 31.42295 14 56 55.33 -20 17 56.2 135571 568 Ci1475 2003 06 01.39039 14 56 50.60 -20 17 38.9 135571 568 Ci1475 2004 04 16.46343 15 07 25.68 -21 24 54.7 135571 675 Ck7379 2004 04 16.48574 15 07 25.55 -21 24 54.6 135571 675 Ck7379 2006 05 03.35267 15 19 44.15 -23 08 49.3 22.2R 135571 250 S~06HK 2006 05 03.35707 15 19 44.12 -23 08 49.3 135571 250 S~06HK 2006 05 03.36146 15 19 44.10 -23 08 49.2 135571 250 S~06HK 2006 05 03.36586 15 19 44.07 -23 08 49.1 135571 250 S~06HK 2006 06 22.03630 15 15 27.36 -22 55 14.1 22.8R 135571 304 Cr4819 2006 06 22.06655 15 15 27.22 -22 55 13.4 135571 304 Cr4819
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 -0.15 0.00 0.46
2 0.0030 0.00 -0.26 0.00 -0.10
3 0.0032 0.00 -0.12 0.00 -0.21
4 0.1945 0.00 0.06 0.00 -0.10
5 0.1946 0.00 0.65 0.00 0.11
6 0.1973 0.00 -1.08 0.00 0.04
7 0.3365 0.00 0.15 0.00 -0.16
8 0.3392 0.00 0.05 0.00 -0.19
9 0.3420 0.00 0.21 0.00 -0.03
10 0.3447 0.00 0.36 0.00 -0.16
11 1.1451 0.00 0.33 0.00 0.32
12 1.1452 0.00 0.01 0.00 0.25
13 1.1478 0.00 -0.30 0.00 0.15
14 2.0241 0.00 0.30 0.00 -0.14
15 2.0242 0.00 0.04 0.00 -0.32
16 4.0690 0.00 0.31 0.00 -0.17
17 4.0690 0.00 0.23 0.00 -0.24
18 4.0690 0.00 0.29 0.00 -0.20
19 4.0691 0.00 0.20 0.00 -0.16
20 4.2050 0.00 -0.21 0.00 0.26
21 4.2051 0.00 -0.44 0.00 0.50
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.
135571 quality flag:3 Type: 5:2EEE 5:2EEE 5:2EEE Type: 5:2EII 5:2EII 5:2EII axisobj 54.855 54.855 54.856 ecceobj 0.347 0.347 0.348 incobj 14.725 14.725 14.725 qmin 35.411 35.412 35.411 qmax 76.664 76.664 76.662 amean 55.462 55.462 55.462 amin 54.833 54.833 54.834 amax 56.284 56.285 56.284 emean 0.324 0.324 0.324 emin 0.297 0.297 0.298 emax 0.362 0.362 0.362 imean 16.579 16.585 16.573 imin 14.214 14.214 14.214 imax 17.851 17.860 17.842 excite_mean 0.432 0.432 0.432 fracstop 1.000 1.000 1.000 cjmean 3.003 3.003 3.003 libcent 0 180.6 180.6 180.5 libamp 0 63.7 64.2 63.5 libcent 1 197.9 198.2 197.9 libamp 1 137.2 137.1 137.1 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 195.5 195.5 195.4 kozaiamp 43.0 42.9 43.0