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: 01FL185
# Created Wed Apr 24 01:10:22 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 43 observations of 43
# Arc: 21.02y
# First observation: 2001/03/26
# Last observation: 2022/04/01
# Chi-squared of fit: 339.68 DOF: 80 RMS: 0.50
# Min/Max residuals: -0.84 1.40
# Exact a, adot, b, bdot, g, gdot:
1.462453E-05 2.543364E-02 -9.002236E-07 1.747669E-04 2.498812E-02 2.064468E-04
# Covariance matrix:
1.4862E-13 -3.2813E-14 9.0664E-16 -1.9303E-16 1.2653E-14 -4.9304E-14
-3.2813E-14 1.3906E-14 -8.6997E-16 1.0914E-16 -2.5008E-14 2.4911E-14
9.0664E-16 -8.6997E-16 8.4965E-14 -6.8935E-15 4.3253E-15 -1.7160E-15
-1.9303E-16 1.0914E-16 -6.8935E-15 9.6234E-16 -2.9181E-16 2.1132E-16
1.2653E-14 -2.5008E-14 4.3253E-15 -2.9181E-16 1.6676E-13 -4.9999E-14
-4.9304E-14 2.4911E-14 -1.7160E-15 2.1132E-16 -4.9999E-14 4.7967E-14
# lat0 lon0 xBary yBary zBary JD0
3.621012 159.196379 -0.448767 0.056435 -0.894189 2451994.643133
# Heliocentric elements and errors
Epoch: 2451994.5000 = 2001/03/26
Mean Anomaly: 15.30358 +/- 0.008
Argument of Peri: 66.50497 +/- 0.010
Long of Asc Node: 75.44407 +/- 0.001
Inclination: 3.55878 +/- 0.000
Eccentricity: 0.07728578 +/- 0.0001
Semi-Major Axis: 44.18707668 +/- 0.0035
Time of Perihelion: 2447433.7972 +/- 2.5
Perihelion: 40.77204390 +/- 0.0041
Aphelion: 47.60210947 +/- 0.0045
Period (y) 293.7319 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -38.32843336 +/- 0.0006
Ecliptic Y 14.08839287 +/- 0.0002
Ecliptic Z 2.52743794 +/- 0.0000
Ecliptic XDOT -0.00101804 +/- 0.0000
Ecliptic YDOT -0.00259451 +/- 0.0000
Ecliptic ZDOT 0.00002073 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 40.91379228 +/- 0.0006
Geocenter to KBO 40.01904626 +/- 0.0007
# Hcoef: 7.14
The following table shows the complete astrometric record for 01FL185. 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 (01FL185) followed by the observatory code and reference code for the source of the astrometry.
2001 03 26.14239 10 48 40.62 +11 28 29.9 23.6R 01FL185 695 Cd1722 2001 03 26.24763 10 48 40.17 +11 28 32.3 01FL185 695 Cd1722 2001 04 24.15627 10 47 01.85 +11 36 37.7 22.8R 01FL185 688 Cd1722 2001 04 24.25675 10 47 01.59 +11 36 39.0 01FL185 688 Cd1722 2002 03 15.05648 10 55 01.55 +10 50 53.7 22.5R 01FL185 950 Cf7155 2002 03 15.09496 10 55 01.38 +10 50 54.7 23.1R 01FL185 950 Cf7155 2002 03 15.13281 10 55 01.20 +10 50 55.7 22.7R 01FL185 950 Cf7155 2002 05 11.90846 10 51 58.34 +11 05 53.9 01FL185 950 Cf7155 2002 05 11.95564 10 51 58.33 +11 05 54.0 01FL185 950 Cf7156 2002 05 12.90790 10 51 57.32 +11 05 54.9 01FL185 950 Cf7156 2002 05 12.96976 10 51 57.25 +11 05 54.9 01FL185 950 Cf7156 2003 03 07.30997 11 01 08.58 +10 13 51.8 21.7R 01FL185 662 Ch5853 2003 03 07.40852 11 01 08.06 +10 13 54.4 01FL185 662 Ch5853 2006 01 24.41284 11 20 18.71 +08 12 35.1 23.5R 01FL185 250 S~06AO 2006 01 24.41724 11 20 18.69 +08 12 35.3 01FL185 250 S~06AO 2006 01 24.42164 11 20 18.68 +08 12 35.3 01FL185 250 S~06AO 2007 11 14.18307 11 30 34.62 +06 59 57.6 23.4R 01FL185 250 S~06AO 2007 11 14.19071 11 30 34.64 +06 59 57.5 01FL185 250 S~06AO 2007 11 14.19835 11 30 34.67 +06 59 57.3 01FL185 250 S~06AO 2007 11 14.20599 11 30 34.70 +06 59 57.2 01FL185 250 S~06AO 2007 11 17.98307 11 30 47.29 +06 58 55.2 01FL185 250 S~06AO 2007 11 17.99071 11 30 47.31 +06 58 55.1 01FL185 250 S~06AO 2007 11 17.99835 11 30 47.34 +06 58 55.0 01FL185 250 S~06AO 2007 11 18.00599 11 30 47.36 +06 58 54.8 01FL185 250 S~06AO 2007 12 14.68793 11 31 42.13 +06 55 35.3 01FL185 250 S~06AO 2007 12 14.69557 11 31 42.13 +06 55 35.3 01FL185 250 S~06AO 2007 12 14.71154 11 31 42.15 +06 55 35.3 01FL185 250 S~06AO 2008 03 12.74823 11 27 46.78 +07 26 05.2 01FL185 250 S~06AO 2008 03 12.75448 11 27 46.75 +07 26 05.4 01FL185 250 S~06AO 2008 03 12.81629 11 27 46.46 +07 26 07.3 01FL185 250 S~06AO 2008 03 12.82601 11 27 46.41 +07 26 07.6 01FL185 250 S~06AO 2008 03 12.88295 11 27 46.15 +07 26 09.2 01FL185 250 S~06AO 2008 03 12.89198 11 27 46.11 +07 26 09.5 01FL185 250 S~06AO 2008 03 12.94893 11 27 45.85 +07 26 11.1 01FL185 250 S~06AO 2008 03 12.95518 11 27 45.82 +07 26 11.3 01FL185 250 S~06AO 2015 03 23.18927 12 04 01.00 +03 25 17.6 23.0R 01FL185 695 C~1Q3A 2015 03 23.25348 12 04 00.70 +03 25 19.6 01FL185 695 C~1Q3A 2015 03 23.31213 12 04 00.42 +03 25 21.4 01FL185 695 C~1Q3A 2018 04 10.18338 12 18 16.948 +01 47 26.24 22.9R 01FL185 G37 C~2bGP 2018 04 10.24883 12 18 16.639 +01 47 27.78 01FL185 G37 C~2bGP 2018 04 10.28614 12 18 16.465 +01 47 28.73 01FL185 G37 C~2bGP 2022 04 01.42114 12 39 30.39 -00 37 29.3 23.0R 01FL185 G37 C~5XSj 2022 04 01.43723 12 39 30.31 -00 37 28.8 23.0R 01FL185 G37 C~5XSj
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 0.37 0.00 0.08
2 0.0003 0.00 0.38 0.00 0.06
3 0.0794 0.00 0.36 0.00 0.68
4 0.0797 0.00 0.22 0.00 0.99
5 0.9690 0.00 -0.01 0.00 0.10
6 0.9691 0.00 0.14 0.00 0.07
7 0.9692 0.00 0.08 0.00 0.06
8 1.1274 0.00 -0.36 0.00 -0.00
9 1.1275 0.00 0.31 0.00 0.05
10 1.1301 0.00 -0.04 0.00 0.10
11 1.1303 0.00 -0.10 0.00 0.07
12 1.9471 0.00 0.33 0.00 0.50
13 1.9473 0.00 -0.42 0.00 0.27
14 4.8330 0.00 -0.21 0.00 -0.09
15 4.8331 0.00 -0.31 0.00 0.01
16 4.8331 0.00 -0.26 0.00 -0.10
17 6.6367 0.00 0.77 0.00 -0.19
18 6.6367 0.00 0.67 0.00 -0.16
19 6.6367 0.00 0.72 0.00 -0.23
20 6.6367 0.00 0.77 0.00 -0.19
21 6.6471 0.00 -0.46 0.00 -0.21
22 6.6471 0.00 -0.52 0.00 -0.19
23 6.6471 0.00 -0.44 0.00 -0.17
24 6.6471 0.00 -0.51 0.00 -0.26
25 6.7202 0.00 0.42 0.00 1.40
26 6.7202 0.00 0.33 0.00 1.39
27 6.7202 0.00 0.43 0.00 1.39
28 6.9640 0.00 -0.49 0.00 -0.84
29 6.9640 0.00 -0.50 0.00 -0.82
30 6.9642 0.00 -0.57 0.00 -0.73
31 6.9642 0.00 -0.64 0.00 -0.72
32 6.9644 0.00 -0.59 0.00 -0.78
33 6.9644 0.00 -0.57 0.00 -0.75
34 6.9646 0.00 -0.52 0.00 -0.81
35 6.9646 0.00 -0.54 0.00 -0.79
36 13.9905 0.00 0.30 0.00 0.23
37 13.9907 0.00 0.24 0.00 0.35
38 13.9909 0.00 0.11 0.00 0.44
39 17.0405 0.00 0.27 0.00 0.36
40 17.0407 0.00 -0.03 0.00 0.17
41 17.0408 0.00 -0.17 0.00 0.14
42 21.0165 0.00 0.13 0.00 0.14
43 21.0166 0.00 0.03 0.00 0.18
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.
01FL185 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.992 43.992 43.992 ecceobj 0.073 0.073 0.073 incobj 3.559 3.559 3.559 qmin 39.822 39.824 39.820 qmax 48.789 48.747 48.794 amean 44.174 44.172 44.174 amin 43.824 43.827 43.817 amax 44.549 44.546 44.553 emean 0.079 0.079 0.079 emin 0.062 0.062 0.062 emax 0.095 0.095 0.095 imean 2.055 2.055 2.055 imin 1.231 1.231 1.231 imax 2.750 2.751 2.750 excite_mean 0.087 0.087 0.087 fracstop 1.000 1.000 1.000 cjmean 3.094 3.094 3.094 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 173.5 173.7 173.6 kozaiamp 180.0 180.0 179.9