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: 00GF147
# Created Sat Apr 27 01:10:06 2024
# Orbit generated from Bernstein formalism
# Fitting 8 observations of 8
# Arc: 28.97d
# First observation: 2000/04/05
# Last observation: 2000/05/04
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# Chi-squared of fit: 6.03 DOF: 12 RMS: 0.15
# Min/Max residuals: -0.22 0.22
# Exact a, adot, b, bdot, g, gdot:
1.463668E-05 2.513597E-02 -5.588812E-07 -2.116936E-03 2.529037E-02 0.000000E+00
# Covariance matrix:
3.3061E-11 5.2748E-08 -1.2695E-14 6.6544E-13 8.5277E-09 0.0000E+00
5.2748E-08 8.5137E-05 -2.0488E-11 1.0739E-09 1.3763E-05 0.0000E+00
-1.2695E-14 -2.0488E-11 3.7405E-13 -4.7992E-12 -3.3119E-12 0.0000E+00
6.6544E-13 1.0739E-09 -4.7992E-12 1.2101E-10 1.7361E-10 0.0000E+00
8.5277E-09 1.3763E-05 -3.3119E-12 1.7361E-10 2.2248E-06 0.0000E+00
0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 2.1286E-04
# lat0 lon0 xBary yBary zBary JD0
0.029813 -153.005413 0.189235 0.000287 -0.990053 2451640.078373
# Heliocentric elements and errors
Epoch: 2451640.5000 = 2000/04/06
Mean Anomaly: 345.96662 +/- 355.900
Argument of Peri: 194.11800 +/- 63.297
Long of Asc Node: 27.07236 +/- 0.111
Inclination: 4.82704 +/- 1.769
Eccentricity: 0.01515113 +/- 0.5645
Semi-Major Axis: 41.12774713 +/- 21.1583
Time of Perihelion: 2455395.9379 +/- 576927.7
Perihelion: 40.50461527 +/- 31.1958
Aphelion: 41.75087900 +/- 31.6277
Period (y) 263.7610 +/- 203.54
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -36.19397474 +/- 2.0780
Ecliptic Y -18.22561114 +/- 1.0583
Ecliptic Z 0.02058466 +/- 0.0012
Ecliptic XDOT 0.00122885 +/- 0.0015
Ecliptic YDOT -0.00241803 +/- 0.0010
Ecliptic ZDOT -0.00022905 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.52378478 +/- 1.9161
Geocenter to KBO 39.54073517 +/- 2.3320
# Hcoef: 8.21
The following table shows the complete astrometric record for 00GF147. 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 (00GF147) followed by the observatory code and reference code for the source of the astrometry.
2000 04 05.57763 13 40 14.63 -10 22 27.1 24.1R 00GF147 568 Cb4443 2000 04 05.61785 13 40 14.43 -10 22 25.7 24.0R 00GF147 568 Cb4443 2000 04 06.52278 13 40 10.18 -10 22 02.9 24.0R 00GF147 568 Cb4443 2000 04 06.56934 13 40 09.96 -10 22 01.4 23.5R 00GF147 568 Cb4443 2000 05 04.511254 13 37 58.23 -10 10 04.5 00GF147 568 C~5V7b 2000 05 04.516228 13 37 58.20 -10 10 04.4 00GF147 568 C~5V7b 2000 05 04.540832 13 37 58.11 -10 10 03.5 00GF147 568 C~5V7b 2000 05 04.546674 13 37 58.06 -10 10 03.2 00GF147 568 C~5V7b
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 -0.16
2 0.0001 -3.26 -0.04 0.24 0.14
3 0.0026 -69.97 -0.06 -1.09 -0.14
4 0.0027 -73.54 -0.13 -0.86 0.16
5 0.0792 -2145.60 0.07 -34.61 -0.16
6 0.0792 -2146.05 -0.03 -34.68 -0.22
7 0.0793 -2147.62 0.17 -34.32 0.17
8 0.0793 -2148.41 -0.21 -34.31 0.19
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.
00GF147 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0