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: 01HA59
# Created Wed Jul 17 01:08:14 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 16 observations of 16
# Arc: 23.02y
# First observation: 2001/04/26
# Last observation: 2024/05/04
# Chi-squared of fit: 7.51 DOF: 26 RMS: 0.12
# Min/Max residuals: -0.29 0.22
# Exact a, adot, b, bdot, g, gdot:
1.439544E-05 2.103140E-02 5.925985E-07 1.414532E-04 2.275120E-02 1.212083E-03
# Covariance matrix:
2.0998E-13 -2.4901E-14 2.6952E-16 -1.1662E-16 2.0231E-13 -3.5589E-14
-2.4901E-14 2.1088E-14 -1.6120E-16 1.3531E-16 1.0266E-13 3.9452E-14
2.6952E-16 -1.6120E-16 1.5654E-13 -8.4892E-15 1.5841E-16 -3.2864E-16
-1.1662E-16 1.3531E-16 -8.4892E-15 1.0523E-15 6.5192E-16 2.6689E-16
2.0231E-13 1.0266E-13 1.5841E-16 6.5192E-16 2.5768E-12 1.7871E-13
-3.5589E-14 3.9452E-14 -3.2864E-16 2.6689E-16 1.7871E-13 7.7946E-14
# lat0 lon0 xBary yBary zBary JD0
0.958107 -143.082549 0.015448 0.016808 -1.012181 2452025.608023
# Heliocentric elements and errors
Epoch: 2452026.5000 = 2001/04/27
Mean Anomaly: 112.42357 +/- 0.183
Argument of Peri: 308.19801 +/- 0.154
Long of Asc Node: 149.52734 +/- 0.005
Inclination: 1.01481 +/- 0.000
Eccentricity: 0.06591052 +/- 0.0001
Semi-Major Axis: 43.70513905 +/- 0.0114
Time of Perihelion: 2419069.1681 +/- 55.2
Perihelion: 40.82451072 +/- 0.0114
Aphelion: 46.58576738 +/- 0.0128
Period (y) 288.9395 +/- 0.11
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -35.95073008 +/- 0.0025
Ecliptic Y -26.98863781 +/- 0.0019
Ecliptic Z 0.73497710 +/- 0.0001
Ecliptic XDOT 0.00139547 +/- 0.0000
Ecliptic YDOT -0.00210833 +/- 0.0000
Ecliptic ZDOT 0.00001965 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 44.95974132 +/- 0.0023
Geocenter to KBO 43.95371275 +/- 0.0031
# Hcoef: 6.64
The following table shows the complete astrometric record for 01HA59. 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 (01HA59) followed by the observatory code and reference code for the source of the astrometry.
2001 04 26.10728 14 19 36.12 -12 55 04.6 22.7R 01HA59 809 Cd0940 2001 04 26.23149 14 19 35.56 -12 55 01.8 01HA59 809 Cd0940 2001 04 26.31921 14 19 35.16 -12 54 59.9 01HA59 809 Cd0940 2001 04 27.28576 14 19 30.91 -12 54 38.1 01HA59 809 Cd0940 2001 04 27.33379 14 19 30.70 -12 54 36.9 01HA59 809 Cd0940 2001 05 24.03924 14 17 37.71 -12 45 10.4 22.6R 01HA59 807 Cd1742 2001 05 24.14782 14 17 37.28 -12 45 08.3 01HA59 807 Cd1742 2006 04 28.21308 14 42 56.73 -14 45 20.8 22.2R 01HA59 807 Cr3558 2006 04 28.28102 14 42 56.42 -14 45 19.6 01HA59 807 Cr3558 2006 05 01.35511 14 42 42.74 -14 44 16.3 22.9R 01HA59 695 Cr3558 2006 05 01.42643 14 42 42.41 -14 44 15.1 01HA59 695 Cr3558 2016 05 29.24617 15 27 52.410 -17 47 25.77 23.0R 01HA59 G37 C~2bkQ 2016 05 29.31567 15 27 52.086 -17 47 24.55 01HA59 G37 C~2bkQ 2024 05 04.353580 16 08 00.782 -19 53 49.58 23.6G 01HA59 G37 C~82lx 2024 05 04.388630 16 08 00.628 -19 53 49.20 01HA59 G37 C~82lx 2024 05 04.423040 16 08 00.489 -19 53 48.65 01HA59 G37 C~82lx
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 0.01 0.00 -0.11
2 0.0003 0.00 -0.03 0.00 -0.09
3 0.0006 0.00 -0.13 0.00 -0.17
4 0.0032 0.00 0.15 0.00 -0.03
5 0.0034 0.00 0.22 0.00 0.09
6 0.0765 0.00 -0.04 0.00 0.08
7 0.0768 0.00 -0.07 0.00 0.11
8 5.0051 0.00 0.17 0.00 0.11
9 5.0053 0.00 0.11 0.00 -0.09
10 5.0137 0.00 -0.17 0.00 0.18
11 5.0139 0.00 -0.29 0.00 -0.09
12 15.0914 0.00 0.17 0.00 -0.04
13 15.0916 0.00 -0.04 0.00 0.10
14 23.0233 0.00 -0.06 0.00 -0.04
15 23.0234 0.00 -0.07 0.00 -0.08
16 23.0235 0.00 0.10 0.00 0.05
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.
01HA59 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.624 43.625 43.624 ecceobj 0.065 0.065 0.065 incobj 1.015 1.015 1.015 qmin 39.987 39.975 39.999 qmax 48.098 48.099 48.081 amean 43.938 43.938 43.938 amin 43.595 43.591 43.590 amax 44.313 44.312 44.316 emean 0.070 0.070 0.070 emin 0.053 0.053 0.053 emax 0.086 0.086 0.086 imean 1.569 1.569 1.569 imin 0.673 0.673 0.673 imax 2.312 2.312 2.312 excite_mean 0.076 0.076 0.076 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 193.9 193.9 193.9 kozaiamp 180.0 180.0 180.0