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: 01DB106
# Created Wed May 21 01:08:16 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 34 observations of 34
# Arc: 24.15y
# First observation: 2001/02/28
# Last observation: 2025/04/23
# Chi-squared of fit: 92.40 DOF: 62 RMS: 0.29
# Min/Max residuals: -0.94 0.58
# Exact a, adot, b, bdot, g, gdot:
1.307647E-05 2.129609E-02 -2.116433E-06 1.230667E-03 2.299494E-02 4.120436E-04
# Covariance matrix:
1.3591E-13 -1.9352E-14 1.0544E-15 -7.2635E-16 -3.0084E-14 -2.7277E-14
-1.9352E-14 8.9330E-15 -7.7044E-16 4.8889E-16 6.2507E-16 1.8606E-14
1.0544E-15 -7.7044E-16 1.1157E-13 -6.4109E-15 9.2937E-16 -1.7715E-15
-7.2635E-16 4.8889E-16 -6.4109E-15 6.0694E-16 -1.9494E-16 1.1018E-15
-3.0084E-14 6.2507E-16 9.2937E-16 -1.9494E-16 2.0064E-13 -9.9424E-15
-2.7277E-14 1.8606E-14 -1.7715E-15 1.1018E-15 -9.9424E-15 4.2074E-14
# lat0 lon0 xBary yBary zBary JD0
1.898620 159.331433 -0.009468 0.032777 -0.992198 2451968.562653
# Heliocentric elements and errors
Epoch: 2451968.5000 = 2001/02/28
Mean Anomaly: 141.35353 +/- 0.062
Argument of Peri: 245.38265 +/- 0.056
Long of Asc Node: 130.05399 +/- 0.001
Inclination: 3.79078 +/- 0.000
Eccentricity: 0.03767463 +/- 0.0000
Semi-Major Axis: 43.18439459 +/- 0.0032
Time of Perihelion: 2411268.6462 +/- 18.5
Perihelion: 41.55743863 +/- 0.0036
Aphelion: 44.81135055 +/- 0.0038
Period (y) 283.7909 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -41.59475227 +/- 0.0008
Ecliptic Y 15.68724626 +/- 0.0003
Ecliptic Z 1.44067721 +/- 0.0000
Ecliptic XDOT -0.00094461 +/- 0.0000
Ecliptic YDOT -0.00235360 +/- 0.0000
Ecliptic ZDOT 0.00014826 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 44.47794250 +/- 0.0007
Geocenter to KBO 43.48783224 +/- 0.0008
# Hcoef: 6.69
The following table shows the complete astrometric record for 01DB106. 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 (01DB106) followed by the observatory code and reference code for the source of the astrometry.
2001 02 28.06191 10 46 31.88 +09 49 46.9 22.7R 01DB106 809 Cd0833 2001 02 28.15915 10 46 31.45 +09 49 49.5 01DB106 809 Cd0833 2001 03 02.13176 10 46 22.77 +09 50 42.7 01DB106 809 Cd0833 2001 03 02.23827 10 46 22.29 +09 50 46.0 01DB106 809 Cd0833 2002 01 14.20030 10 54 02.75 +09 07 11.2 22.9R 01DB106 950 Ce9334 2002 01 14.23341 10 54 02.68 +09 07 11.9 01DB106 950 Ce9334 2002 01 14.26966 10 54 02.57 +09 07 12.6 01DB106 950 Ce9334 2002 02 06.37090 10 52 45.57 +09 16 00.8 22.2R 01DB106 695 Ce9334 2002 02 06.46772 10 52 45.18 +09 16 02.5 01DB106 695 Ce9334 2002 02 08.53339 10 52 36.96 +09 16 57.0 01DB106 695 Ce9334 2002 02 09.21900 10 52 34.21 +09 17 15.5 01DB106 304 Ce9334 2002 02 09.25869 10 52 34.06 +09 17 16.6 22.8R 01DB106 304 Ce9334 2003 03 31.19847 10 53 46.12 +09 14 52.8 22.2R 01DB106 695 Ch8065 2003 04 01.17721 10 53 42.47 +09 15 14.7 01DB106 695 Ch8065 2003 04 01.27308 10 53 42.12 +09 15 16.6 01DB106 695 Ch8065 2015 02 18.29448 11 51 42.54 +03 55 37.9 22.9R 01DB106 695 C~1M60 2015 02 18.38762 11 51 42.20 +03 55 40.5 01DB106 695 C~1M60 2015 02 18.47664 11 51 41.87 +03 55 43.0 01DB106 695 C~1M60 2015 04 15.20534 11 47 55.88 +04 20 41.6 22.8R 01DB106 695 C~1RHM 2015 04 15.28229 11 47 55.60 +04 20 43.4 01DB106 695 C~1RHM 2015 04 15.35550 11 47 55.31 +04 20 44.9 01DB106 695 C~1RHM 2019 02 05.53446 12 10 27.43 +02 06 44.5 22.8i 01DB106 T09 C~7wJY 2019 02 05.58442 12 10 27.30 +02 06 45.6 22.9i 01DB106 T09 C~7wJY 2019 02 05.62497 12 10 27.19 +02 06 46.3 22.9i 01DB106 T09 C~7wJY 2019 02 05.66520 12 10 27.07 +02 06 47.3 23.1i 01DB106 T09 C~7wJY 2019 03 03.52564 12 08 59.72 +02 17 33.5 22.9z 01DB106 T09 C~7b9y 2019 03 03.56606 12 08 59.57 +02 17 34.6 22.8z 01DB106 T09 C~7b9y 2019 03 03.61973 12 08 59.35 +02 17 35.9 22.8z 01DB106 T09 C~7b9y 2019 03 03.62241 12 08 59.34 +02 17 35.9 22.9z 01DB106 T09 C~7b9y 2019 04 04.44671 12 06 46.73 +02 32 24.4 24.1g 01DB106 T09 C~8GhF 2019 04 04.45724 12 06 46.68 +02 32 24.6 24.2g 01DB106 T09 C~8GhF 2019 04 04.51189 12 06 46.45 +02 32 26.1 24.2g 01DB106 T09 C~8GhF 2025 04 23.273960 12 32 29.791 +00 03 51.91 23.3G 01DB106 G37 C~8srl 2025 04 23.311490 12 32 29.635 +00 03 52.99 01DB106 G37 C~8srl
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 0.54 0.00 0.44
2 0.0003 0.00 0.58 0.00 0.38
3 0.0057 0.00 0.19 0.00 -0.03
4 0.0060 0.00 0.12 0.00 0.38
5 0.8765 0.00 -0.07 0.00 -0.06
6 0.8766 0.00 0.23 0.00 0.00
7 0.8767 0.00 0.06 0.00 0.01
8 0.9399 0.00 0.56 0.00 -0.14
9 0.9402 0.00 0.49 0.00 -0.94
10 0.9458 0.00 -0.38 0.00 -0.17
11 0.9477 0.00 -0.69 0.00 0.12
12 0.9478 0.00 -0.51 0.00 0.17
13 2.0839 0.00 -0.71 0.00 -0.22
14 2.0866 0.00 -0.55 0.00 0.04
15 2.0868 0.00 -0.35 0.00 -0.16
16 13.9719 0.00 0.16 0.00 -0.12
17 13.9721 0.00 0.24 0.00 0.03
18 13.9724 0.00 0.25 0.00 0.19
19 14.1250 0.00 0.31 0.00 0.09
20 14.1252 0.00 0.43 0.00 0.17
21 14.1254 0.00 0.17 0.00 0.04
22 17.9370 0.00 -0.24 0.00 0.07
23 17.9371 0.00 -0.13 0.00 0.11
24 17.9372 0.00 -0.11 0.00 -0.05
25 17.9373 0.00 -0.26 0.00 0.09
26 18.0081 0.00 -0.18 0.00 0.12
27 18.0082 0.00 0.00 0.00 0.10
28 18.0084 0.00 -0.08 0.00 -0.09
29 18.0084 0.00 -0.06 0.00 -0.16
30 18.0955 0.00 -0.08 0.00 -0.08
31 18.0955 0.00 -0.17 0.00 -0.15
32 18.0957 0.00 -0.18 0.00 -0.09
33 24.1484 0.00 0.24 0.00 -0.13
34 24.1485 0.00 0.08 0.00 0.09
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.
01DB106 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.024 43.024 43.024 ecceobj 0.041 0.041 0.041 incobj 3.795 3.795 3.795 qmin 40.258 40.271 40.254 qmax 46.318 46.292 46.342 amean 43.189 43.189 43.188 amin 42.854 42.855 42.852 amax 43.531 43.532 43.532 emean 0.047 0.047 0.047 emin 0.027 0.027 0.027 emax 0.065 0.064 0.065 imean 3.117 3.117 3.117 imin 2.077 2.077 2.077 imax 3.998 3.997 3.999 excite_mean 0.072 0.072 0.072 fracstop 1.000 1.000 1.000 cjmean 3.085 3.085 3.085 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 178.1 178.4 178.1 kozaiamp 180.0 180.0 180.0