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: 11UA411
# Created Fri Nov 22 02:09:14 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 37 observations of 37
# Arc: 11.32y
# First observation: 2011/08/30
# Last observation: 2022/12/26
# Chi-squared of fit: 20.09 DOF: 68 RMS: 0.13
# Min/Max residuals: -0.48 0.36
# Exact a, adot, b, bdot, g, gdot:
1.937189E-05 4.339682E-02 -2.268119E-06 -5.933383E-03 3.418373E-02 -1.028478E-03
# Covariance matrix:
1.3264E-13 -1.9188E-14 -3.1910E-15 3.8266E-15 9.8150E-14 -5.3527E-14
-1.9188E-14 5.9344E-14 3.8660E-15 -8.3355E-15 2.1210E-14 1.2427E-13
-3.1910E-15 3.8660E-15 4.9836E-14 -7.3367E-15 -1.4852E-15 9.4310E-15
3.8266E-15 -8.3355E-15 -7.3367E-15 5.4107E-15 -7.1162E-16 -1.9367E-14
9.8150E-14 2.1210E-14 -1.4852E-15 -7.1162E-16 1.4010E-13 1.5125E-14
-5.3527E-14 1.2427E-13 9.4310E-15 -1.9367E-14 1.5125E-14 2.8763E-13
# lat0 lon0 xBary yBary zBary JD0
4.051789 32.379968 0.833582 0.039848 -0.563024 2455803.980326
# Heliocentric elements and errors
Epoch: 2455804.5000 = 2011/08/31
Mean Anomaly: 351.47872 +/- 0.003
Argument of Peri: 167.13637 +/- 0.004
Long of Asc Node: 238.00054 +/- 0.000
Inclination: 8.63192 +/- 0.000
Eccentricity: 0.25063627 +/- 0.0000
Semi-Major Axis: 39.55097053 +/- 0.0025
Time of Perihelion: 2457954.9854 +/- 8.4
Perihelion: 29.63806266 +/- 0.0024
Aphelion: 49.46387840 +/- 0.0035
Period (y) 248.7390 +/- 0.02
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 25.56991691 +/- 0.0003
Ecliptic Y 15.22660355 +/- 0.0002
Ecliptic Z 2.06697047 +/- 0.0000
Ecliptic XDOT -0.00190557 +/- 0.0000
Ecliptic YDOT 0.00291470 +/- 0.0000
Ecliptic ZDOT -0.00047979 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 29.83193370 +/- 0.0002
Geocenter to KBO 29.25372603 +/- 0.0003
# Hcoef: 9.23
The following table shows the complete astrometric record for 11UA411. 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 (11UA411) followed by the observatory code and reference code for the source of the astrometry.
2011 08 30.47956 01 54 58.086 +16 06 00.58 23.7r 11UA411 568 C~1C6M 2011 08 30.53207 01 54 57.916 +16 05 59.88 23.9r 11UA411 568 C~1C6M 2011 08 30.57849 01 54 57.778 +16 05 59.30 24.0r 11UA411 568 C~1C6M 2011 09 05.58010 01 54 37.931 +16 04 34.09 24.4r 11UA411 568 C~1C6M 2011 10 25.32951 01 50 08.155 +15 40 13.54 11UA411 568 C~1C6M 2011 10 25.32951 01 50 08.17 +15 40 13.6 23.3r 11UA411 568 C~3j8g 2011 10 25.37276 01 50 07.878 +15 40 11.94 24.0r 11UA411 568 C~1C6M 2011 10 25.37795 01 50 07.853 +15 40 11.79 23.9r 11UA411 568 C~1C6M 2011 10 25.42724 01 50 07.526 +15 40 09.69 23.6r 11UA411 568 C~1C6M 2011 10 25.42724 01 50 07.53 +15 40 10.0 23.8r 11UA411 568 C~3j8g 2011 10 25.48711 01 50 07.141 +15 40 07.47 24.0r 11UA411 568 C~1C6M 2011 10 25.48711 01 50 07.15 +15 40 07.7 24.4r 11UA411 568 C~3j8g 2011 10 26.27825 01 50 02.172 +15 39 37.12 23.6r 11UA411 568 C~1C6M 2011 10 26.33093 01 50 01.834 +15 39 35.11 23.7r 11UA411 568 C~1C6M 2011 10 26.33093 01 50 01.83 +15 39 35.3 23.6r 11UA411 568 C~3j8g 2011 10 26.37414 01 50 01.554 +15 39 33.52 23.9r 11UA411 568 C~1C6M 2011 10 31.27710 01 49 30.767 +15 36 23.77 11UA411 568 C~1C6M 2011 10 31.37984 01 49 30.115 +15 36 19.81 11UA411 568 C~1C6M 2011 11 28.42497 01 46 52.655 +15 18 39.63 23.9r 11UA411 568 C~1C6M 2011 11 30.31655 01 46 43.991 +15 17 34.68 24.3r 11UA411 568 C~1C6M 2012 01 25.31235 01 45 34.487 +15 00 35.19 24.4r 11UA411 568 C~1C6M 2012 01 26.29717 01 45 36.935 +15 00 36.73 24.1r 11UA411 568 C~1C6M 2012 01 27.23112 01 45 39.373 +15 00 38.91 11UA411 568 C~1C6M 2012 08 22.45359 02 05 29.689 +16 39 17.24 11UA411 568 C~1C6M 2012 08 23.52913 02 05 27.627 +16 39 10.77 24.2r 11UA411 568 C~1C6M 2012 08 24.56487 02 05 25.533 +16 39 03.75 23.7r 11UA411 568 C~1C6M 2012 10 21.32322 02 00 50.913 +16 15 50.55 11UA411 568 C~1C6M 2012 10 21.34894 02 00 50.749 +16 15 49.70 11UA411 568 C~1C6M 2012 10 21.37460 02 00 50.584 +16 15 48.65 23.7r 11UA411 568 C~1C6M 2013 02 06.29902 01 56 08.790 +15 34 41.82 23.7r 11UA411 568 C~1C6M 2013 10 05.57787 02 12 56.43 +16 56 22.0 11UA411 568 C~1CKy 2013 10 05.59819 02 12 56.31 +16 56 21.3 11UA411 568 C~1CKy 2013 10 05.61843 02 12 56.19 +16 56 20.7 11UA411 568 C~1CKy 2019 02 08.146680 02 57 12.919 +18 14 54.75 23.8G 11UA411 G37 C~2zmc 2019 02 08.246050 02 57 13.100 +18 14 55.54 11UA411 G37 C~2zmc 2022 12 26.133910 03 40 49.863 +19 29 41.40 24.0G 11UA411 G37 C~69Zk 2022 12 26.186630 03 40 49.593 +19 29 40.29 11UA411 G37 C~69Zk
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 0.18 0.00 -0.04
2 0.0001 0.00 0.06 0.00 -0.11
3 0.0003 0.00 0.15 0.00 -0.13
4 0.0167 0.00 0.36 0.00 0.07
5 0.1529 0.00 0.14 0.00 0.06
6 0.1529 0.00 -0.08 0.00 0.00
7 0.1530 0.00 -0.07 0.00 0.05
8 0.1530 0.00 0.06 0.00 0.10
9 0.1532 0.00 -0.08 0.00 -0.12
10 0.1532 0.00 -0.02 0.00 0.19
11 0.1533 0.00 0.06 0.00 0.19
12 0.1533 0.00 -0.08 0.00 -0.04
13 0.1555 0.00 -0.03 0.00 -0.03
14 0.1557 0.00 -0.09 0.00 0.16
15 0.1557 0.00 -0.03 0.00 -0.03
16 0.1558 0.00 -0.07 0.00 0.03
17 0.1692 0.00 -0.06 0.00 -0.02
18 0.1695 0.00 -0.06 0.00 -0.01
19 0.2463 0.00 -0.21 0.00 -0.13
20 0.2514 0.00 0.00 0.00 0.05
21 0.4047 0.00 0.06 0.00 0.10
22 0.4074 0.00 0.14 0.00 -0.04
23 0.4100 0.00 0.11 0.00 -0.14
24 0.9801 0.00 0.16 0.00 -0.14
25 0.9830 0.00 -0.05 0.00 -0.07
26 0.9859 0.00 0.05 0.00 -0.03
27 1.1440 0.00 -0.21 0.00 -0.08
28 1.1441 0.00 -0.17 0.00 0.01
29 1.1441 0.00 -0.16 0.00 -0.11
30 1.4396 0.00 -0.14 0.00 0.18
31 2.1002 0.00 -0.11 0.00 0.08
32 2.1003 0.00 -0.12 0.00 -0.00
33 2.1003 0.00 -0.14 0.00 0.01
34 7.4433 0.00 0.25 0.00 -0.48
35 7.4436 0.00 0.19 0.00 0.21
36 11.3228 0.00 -0.12 0.00 0.10
37 11.3229 0.00 -0.04 0.00 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.
11UA411 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.623 39.623 39.623 ecceobj 0.252 0.252 0.252 incobj 8.630 8.630 8.630 qmin 28.918 28.974 28.847 qmax 50.736 50.770 50.816 amean 39.456 39.456 39.456 amin 38.904 38.920 38.924 amax 40.081 40.095 40.078 emean 0.249 0.247 0.249 emin 0.225 0.225 0.225 emax 0.268 0.267 0.270 imean 9.489 9.581 9.478 imin 8.533 8.657 8.444 imax 10.709 10.707 10.711 excite_mean 0.298 0.298 0.299 fracstop 1.000 1.000 1.000 cjmean 2.950 2.950 2.950 libcent 0 181.2 181.7 182.3 libamp 0 125.4 125.6 125.2 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 186.2 180.1 180.0 kozaiamp 180.0 179.9 180.0