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: 511553
# Created Wed Dec 25 02:07:12 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 44 observations of 44
# Arc: 7.03y
# First observation: 2013/11/29
# Last observation: 2020/12/09
# Chi-squared of fit: 5.60 DOF: 82 RMS: 0.06
# Min/Max residuals: -0.22 0.18
# Exact a, adot, b, bdot, g, gdot:
1.697294E-05 2.848959E-02 -3.081595E-06 -4.819485E-03 2.677861E-02 -1.245619E-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
4.667812 27.533124 -0.624440 0.062053 -0.758709 2456625.760228
# Heliocentric elements and errors
Epoch: 2456626.5000 = 2013/11/30
Mean Anomaly: 348.99633 +/- 0.000
Argument of Peri: 168.89476 +/- 0.000
Long of Asc Node: 233.58365 +/- 0.000
Inclination: 10.67816 +/- 0.000
Eccentricity: 0.13007799 +/- 0.0000
Semi-Major Axis: 43.64762984 +/- 0.0000
Time of Perihelion: 2459845.8957 +/- 0.0
Perihelion: 37.97003404 +/- 0.0000
Aphelion: 49.32522564 +/- 0.0000
Period (y) 288.3694 +/- 0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 33.38935695 +/- 0.0000
Ecliptic Y 18.11360771 +/- 0.0000
Ecliptic Z 3.03880995 +/- 0.0000
Ecliptic XDOT -0.00142961 +/- 0.0000
Ecliptic YDOT 0.00254080 +/- 0.0000
Ecliptic ZDOT -0.00050133 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 38.10758058 +/- 0.0000
Geocenter to KBO 37.34331979 +/- 0.0000
# Hcoef: 7.50
The following table shows the complete astrometric record for 511553. 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 (511553) followed by the observatory code and reference code for the source of the astrometry.
2013 11 29.25945 01 35 18.978 +14 56 50.29 23.4r 511553 568 C~2WZw 2013 12 04.40602 01 35 01.902 +14 54 28.89 23.3r 511553 568 C~2WZw 2013 12 05.29920 01 34 59.158 +14 54 05.32 23.2r 511553 568 C~2WZw 2013 12 30.37920 01 34 11.446 +14 45 24.38 23.4r 511553 568 C~2WZw 2013 12 30.38523 01 34 11.461 +14 45 24.34 23.5r 511553 568 C~2WZw 2014 01 02.25325 01 34 09.948 +14 44 44.94 23.3r 511553 568 C~2WZw 2014 01 02.30801 01 34 09.923 +14 44 44.15 23.2r 511553 568 C~2WZw 2014 01 03.22327 01 34 09.638 +14 44 32.67 23.3r 511553 568 C~2WZw 2014 01 03.26568 01 34 09.620 +14 44 32.25 23.2r 511553 568 C~2WZw 2014 07 26.53368 01 49 20.222 +15 57 50.20 23.5r 511553 568 C~2WZw 2014 07 26.57688 01 49 20.243 +15 57 50.56 23.5r 511553 568 C~2WZw 2014 08 24.47423 01 48 57.897 +15 57 52.06 23.3r 511553 568 C~2WZw 2014 08 24.54416 01 48 57.739 +15 57 51.49 23.4r 511553 568 C~2WZw 2014 08 30.44950 01 48 43.502 +15 56 54.00 23.2r 511553 568 C~2WZw 2014 08 30.55610 01 48 43.213 +15 56 52.78 23.3r 511553 568 C~2WZw 2014 09 18.47464 01 47 38.925 +15 51 45.73 23.2r 511553 568 C~2WZw 2014 09 18.51736 01 47 38.751 +15 51 44.90 23.3r 511553 568 C~2WZw 2014 09 23.51567 01 47 17.769 +15 49 55.45 23.3r 511553 568 C~2WZw 2014 10 22.29873 01 44 58.339 +15 36 38.35 23.3r 511553 568 C~2Gdr 2014 10 22.34444 01 44 58.106 +15 36 36.91 23.2r 511553 568 C~2Gdr 2014 10 22.38820 01 44 57.873 +15 36 35.54 23.2r 511553 568 C~2Gdr 2014 10 23.48652 01 44 52.254 +15 36 01.25 22.9r 511553 568 C~2WZw 2014 10 25.50246 01 44 42.000 +15 34 57.68 23.0r 511553 568 C~2WZw 2014 11 20.23375 01 42 39.235 +15 21 23.24 23.2r 511553 568 C~2WZw 2014 11 20.37417 01 42 38.632 +15 21 19.00 23.2r 511553 568 C~2WZw 2014 11 21.27833 01 42 34.825 +15 20 51.48 23.2r 511553 568 C~2WZw 2014 11 21.43358 01 42 34.153 +15 20 46.80 23.3r 511553 568 C~2WZw 2015 01 28.28328 01 41 08.257 +15 02 03.32 23.1r 511553 568 C~2WZw 2015 02 19.26046 01 42 19.072 +15 05 04.09 23.4r 511553 568 C~2WZw 2015 10 10.36050 01 52 48.463 +16 01 37.40 23.2r 511553 568 C~2WZw 2015 10 10.42692 01 52 48.128 +16 01 35.53 23.1r 511553 568 C~2WZw 2015 10 12.48210 01 52 37.895 +16 00 37.41 511553 568 C~2WZw 2015 10 12.54868 01 52 37.541 +16 00 35.63 511553 568 C~2WZw 2015 10 14.38671 01 52 28.344 +15 59 42.73 511553 568 C~2WZw 2015 10 14.39084 01 52 28.323 +15 59 42.68 511553 568 C~2WZw 2015 12 06.20482 01 48 24.662 +15 33 07.99 23.5r 511553 568 C~2WZw 2015 12 06.27161 01 48 24.426 +15 33 06.30 23.3r 511553 568 C~2WZw 2015 12 07.40375 01 48 20.710 +15 32 36.80 23.4w 511553 568 C~2WZw 2015 12 31.32052 01 47 29.172 +15 24 17.93 23.5w 511553 568 C~2WZw 2016 01 07.29206 01 47 24.728 +15 22 45.26 23.8w 511553 568 C~2WZw 2017 08 25.56297 02 09 11.673 +16 50 12.23 23.4w 511553 568 C~2WZw 2017 08 30.58559 02 09 01.416 +16 49 31.23 23.6w 511553 568 C~2WZw 2020 12 09.104930 02 22 17.616 +16 55 54.89 23.4G 511553 G37 C~4TsE 2020 12 09.160240 02 22 17.394 +16 55 53.34 511553 G37 C~4TsE
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 -0.05 0.00 0.03
2 0.0141 0.00 0.03 0.00 -0.04
3 0.0165 0.00 -0.04 0.00 -0.03
4 0.0852 0.00 -0.11 0.00 -0.00
5 0.0852 0.00 0.18 0.00 0.04
6 0.0931 0.00 -0.04 0.00 -0.05
7 0.0932 0.00 -0.04 0.00 -0.13
8 0.0957 0.00 -0.01 0.00 -0.07
9 0.0958 0.00 -0.04 0.00 0.04
10 0.6551 0.00 0.11 0.00 -0.02
11 0.6552 0.00 0.05 0.00 -0.02
12 0.7343 0.00 0.01 0.00 0.00
13 0.7345 0.00 -0.02 0.00 -0.01
14 0.7507 0.00 -0.02 0.00 0.01
15 0.7510 0.00 0.06 0.00 -0.02
16 0.8028 0.00 -0.03 0.00 -0.03
17 0.8029 0.00 0.02 0.00 0.02
18 0.8166 0.00 0.02 0.00 -0.03
19 0.8954 0.00 0.02 0.00 0.06
20 0.8955 0.00 0.08 0.00 0.04
21 0.8956 0.00 -0.01 0.00 0.03
22 0.8986 0.00 -0.14 0.00 0.06
23 0.9042 0.00 0.08 0.00 -0.11
24 0.9746 0.00 -0.00 0.00 0.02
25 0.9750 0.00 0.09 0.00 0.06
26 0.9775 0.00 0.04 0.00 0.02
27 0.9779 0.00 -0.07 0.00 0.05
28 1.1637 0.00 0.01 0.00 0.13
29 1.2238 0.00 -0.02 0.00 -0.03
30 1.8620 0.00 0.03 0.00 -0.03
31 1.8622 0.00 0.03 0.00 -0.05
32 1.8678 0.00 0.01 0.00 -0.11
33 1.8680 0.00 -0.22 0.00 0.01
34 1.8730 0.00 0.04 0.00 -0.02
35 1.8730 0.00 0.05 0.00 0.05
36 2.0176 0.00 0.09 0.00 -0.02
37 2.0178 0.00 -0.04 0.00 0.04
38 2.0209 0.00 -0.04 0.00 0.03
39 2.0864 0.00 0.05 0.00 0.01
40 2.1055 0.00 0.03 0.00 0.03
41 3.7380 0.00 -0.09 0.00 0.07
42 3.7517 0.00 -0.04 0.00 0.07
43 7.0276 0.00 0.09 0.00 0.05
44 7.0278 0.00 -0.04 0.00 -0.14
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.
511553 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.921 43.921 43.921 ecceobj 0.135 0.135 0.135 incobj 10.669 10.669 10.669 qmin 36.248 36.237 36.251 qmax 51.332 51.285 51.339 amean 43.602 43.601 43.602 amin 43.218 43.214 43.197 amax 44.028 44.020 44.053 emean 0.139 0.139 0.139 emin 0.112 0.112 0.112 emax 0.167 0.166 0.167 imean 11.892 11.892 11.891 imin 10.874 10.883 10.872 imax 13.015 13.018 13.015 excite_mean 0.249 0.249 0.249 fracstop 1.000 1.000 1.000 cjmean 3.022 3.022 3.022 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 180.8 180.8 180.7 kozaiamp 180.0 180.0 180.0