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: 05EM303
# Created Fri Nov 22 02:08:46 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 18 observations of 18
# Arc: 14.15y
# First observation: 2005/03/11
# Last observation: 2019/05/07
# Chi-squared of fit: 41.40 DOF: 30 RMS: 0.27
# Min/Max residuals: -0.38 0.96
# Exact a, adot, b, bdot, g, gdot:
1.639884E-05 2.315388E-02 3.896651E-07 1.975670E-04 2.387094E-02 6.734447E-05
# Covariance matrix:
3.5361E-13 -8.5696E-16 6.4622E-16 -1.3010E-16 3.4592E-13 3.0813E-14
-8.5696E-16 1.1420E-13 -3.7482E-16 1.0202E-15 1.2045E-13 3.4125E-13
6.4622E-16 -3.7482E-16 1.4113E-13 -1.1012E-14 6.7432E-16 -1.1413E-15
-1.3010E-16 1.0202E-15 -1.1012E-14 2.1130E-15 7.4386E-16 3.1057E-15
3.4592E-13 1.2045E-13 6.7432E-16 7.4386E-16 6.5992E-13 3.6653E-13
3.0813E-14 3.4125E-13 -1.1413E-15 3.1057E-15 3.6653E-13 1.0388E-12
# lat0 lon0 xBary yBary zBary JD0
5.692382 -161.780836 0.455816 0.087177 -0.873731 2453440.889073
# Heliocentric elements and errors
Epoch: 2453440.5000 = 2005/03/11
Mean Anomaly: 344.61635 +/- 0.098
Argument of Peri: 100.62608 +/- 0.103
Long of Asc Node: 113.19244 +/- 0.001
Inclination: 5.60134 +/- 0.000
Eccentricity: 0.02565527 +/- 0.0001
Semi-Major Axis: 43.85504745 +/- 0.0057
Time of Perihelion: 2457973.4896 +/- 35.0
Perihelion: 42.72993441 +/- 0.0069
Aphelion: 44.98016048 +/- 0.0071
Period (y) 290.4274 +/- 0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -40.57623306 +/- 0.0014
Ecliptic Y -12.87545744 +/- 0.0004
Ecliptic Z 4.15519583 +/- 0.0001
Ecliptic XDOT 0.00082521 +/- 0.0000
Ecliptic YDOT -0.00253132 +/- 0.0000
Ecliptic ZDOT 0.00002338 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 42.77235240 +/- 0.0013
Geocenter to KBO 41.89196989 +/- 0.0014
# Hcoef: 7.56
The following table shows the complete astrometric record for 05EM303. 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 (05EM303) followed by the observatory code and reference code for the source of the astrometry.
2005 03 11.38833 13 15 52.72 -01 52 36.4 23.3R 05EM303 695 Cn0312 2005 03 11.48760 13 15 52.34 -01 52 33.9 05EM303 695 Cn0312 2005 03 12.41187 13 15 48.90 -01 52 08.8 05EM303 695 Cn0312 2005 04 15.21936 13 13 25.62 -01 36 30.7 24.3R 05EM303 304 Cn3361 2005 04 15.25873 13 13 25.49 -01 36 29.8 05EM303 304 Cn3361 2005 06 07.05035 13 10 21.60 -01 21 37.4 23.6R 05EM303 304 Cn6541 2005 06 07.14241 13 10 21.41 -01 21 36.8 05EM303 304 Cn6541 2006 04 26.08455 13 17 37.10 -02 01 44.2 22.6R 05EM303 807 Cr3594 2006 04 26.16780 13 17 36.71 -02 01 42.0 05EM303 807 Cr3594 2006 04 27.11423 13 17 32.70 -02 01 19.6 05EM303 807 Cr3594 2006 04 27.18598 13 17 32.39 -02 01 18.2 05EM303 807 Cr3594 2013 05 14.23195 13 51 04.25 -05 19 31.8 23.6R 05EM303 G37 C~0snm 2013 05 14.29607 13 51 04.04 -05 19 31.7 05EM303 G37 C~0snm 2019 04 05.320130 14 24 08.814 -08 24 30.50 23.5G 05EM303 G37 C~34bb 2019 04 05.399720 14 24 08.468 -08 24 28.55 05EM303 G37 C~34bb 2019 04 05.448630 14 24 08.259 -08 24 27.51 05EM303 G37 C~34bb 2019 05 06.357170 14 21 51.13 -08 12 26.9 23.7G 05EM303 705 C~39ng 2019 05 07.306300 14 21 46.85 -08 12 06.6 23.9G 05EM303 705 C~39ng
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 -0.22 0.00 0.03
2 0.0003 0.00 -0.27 0.00 -0.17
3 0.0028 0.00 0.07 0.00 -0.34
4 0.0954 0.00 -0.29 0.00 0.33
5 0.0955 0.00 0.40 0.00 0.20
6 0.2400 0.00 0.03 0.00 0.02
7 0.2403 0.00 0.02 0.00 0.17
8 1.1244 0.00 0.36 0.00 -0.38
9 1.1247 0.00 -0.09 0.00 -0.14
10 1.1272 0.00 -0.08 0.00 0.10
11 1.1274 0.00 -0.10 0.00 -0.17
12 8.1748 0.00 -0.27 0.00 0.96
13 8.1750 0.00 0.53 0.00 -0.15
14 14.0669 0.00 0.19 0.00 -0.12
15 14.0671 0.00 -0.01 0.00 -0.07
16 14.0672 0.00 -0.08 0.00 -0.19
17 14.1519 0.00 -0.05 0.00 -0.05
18 14.1545 0.00 -0.24 0.00 -0.00
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.
05EM303 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.315 43.315 43.315 ecceobj 0.014 0.014 0.014 incobj 5.602 5.602 5.602 qmin 42.234 42.231 42.239 qmax 45.131 45.132 45.130 amean 43.612 43.612 43.612 amin 43.279 43.277 43.280 amax 43.948 43.947 43.948 emean 0.014 0.014 0.014 emin 0.000 0.000 0.000 emax 0.027 0.028 0.027 imean 4.084 4.084 4.084 imin 3.420 3.420 3.420 imax 4.751 4.751 4.751 excite_mean 0.073 0.073 0.073 fracstop 1.000 1.000 1.000 cjmean 3.091 3.091 3.091 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 179.6 179.6 179.7 kozaiamp 180.0 180.0 180.0