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: 05BV49
# Created Fri Apr 26 01:12:18 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 45 observations of 45
# Arc: 20.14y
# First observation: 2002/01/10
# Last observation: 2022/03/02
# Chi-squared of fit: 56.84 DOF: 84 RMS: 0.20
# Min/Max residuals: -0.47 0.51
# Exact a, adot, b, bdot, g, gdot:
1.502283E-05 2.402443E-02 3.804233E-06 3.351998E-03 2.445369E-02 -2.894397E-04
# Covariance matrix:
2.5419E-13 -5.7614E-14 2.4495E-14 -7.2989E-15 -2.7071E-14 -9.1055E-14
-5.7614E-14 1.6276E-14 -7.3475E-15 2.1919E-15 1.0758E-14 2.7325E-14
2.4495E-14 -7.3475E-15 8.6518E-14 -7.1173E-15 -2.5006E-15 -1.3076E-14
-7.2989E-15 2.1919E-15 -7.1173E-15 1.0164E-15 8.7120E-16 3.8919E-15
-2.7071E-14 1.0758E-14 -2.5006E-15 8.7120E-16 1.3430E-13 9.9093E-15
-9.1055E-14 2.7325E-14 -1.3076E-14 3.8919E-15 9.9093E-15 4.8585E-14
# lat0 lon0 xBary yBary zBary JD0
0.755885 121.622354 0.195337 0.012581 -0.958970 2452284.874694
# Heliocentric elements and errors
Epoch: 2452284.5000 = 2002/01/10
Mean Anomaly: 343.78290 +/- 0.017
Argument of Peri: 23.30870 +/- 0.019
Long of Asc Node: 116.06109 +/- 0.000
Inclination: 7.96239 +/- 0.000
Eccentricity: 0.05140832 +/- 0.0000
Semi-Major Axis: 44.02024741 +/- 0.0027
Time of Perihelion: 2457090.1038 +/- 10.7
Perihelion: 41.75724061 +/- 0.0032
Aphelion: 46.28325422 +/- 0.0034
Period (y) 292.0700 +/- 0.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -21.77498145 +/- 0.0003
Ecliptic Y 35.74314645 +/- 0.0005
Ecliptic Z 0.53962746 +/- 0.0000
Ecliptic XDOT -0.00227938 +/- 0.0000
Ecliptic YDOT -0.00144249 +/- 0.0000
Ecliptic ZDOT 0.00037504 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 41.85707042 +/- 0.0005
Geocenter to KBO 40.89366419 +/- 0.0006
# Hcoef: 6.89
The following table shows the complete astrometric record for 05BV49. 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 (05BV49) followed by the observatory code and reference code for the source of the astrometry.
2002 01 10.373951 08 16 10.88 +20 32 08.4 05BV49 568 C~0sOv 2002 01 10.398200 08 16 10.76 +20 32 08.9 05BV49 568 C~0sOv 2002 01 10.419805 08 16 10.65 +20 32 09.4 05BV49 568 C~0sOv 2004 12 12.396499 08 35 56.27 +19 58 28.6 05BV49 645 C~1GH2 2004 12 12.397328 08 35 56.26 +19 58 28.6 05BV49 645 C~1GH2 2004 12 12.399816 08 35 56.25 +19 58 28.5 05BV49 645 C~1GH2 2005 01 16.33048 08 33 25.92 +20 09 12.9 23.8g 05BV49 568 C~0VDy 2005 01 16.37246 08 33 25.68 +20 09 13.9 24.3g 05BV49 568 C~0VDy 2005 01 16.41033 08 33 25.50 +20 09 14.9 24.2g 05BV49 568 C~0VDy 2005 04 05.30748 08 28 22.79 +20 28 18.2 22.5i 05BV49 568 C~0VDy 2005 04 06.25340 08 28 21.82 +20 28 21.6 23.0i 05BV49 568 C~0VDy 2005 04 06.31853 08 28 21.75 +20 28 21.8 23.1i 05BV49 568 C~0VDy 2006 01 31.37052 08 38 05.14 +20 04 36.1 22.2r 05BV49 568 C~0VDy 2006 02 01.40821 08 37 59.86 +20 04 57.3 05BV49 568 C~0VDy 2006 11 23.50318 08 48 19.37 +19 33 45.0 05BV49 568 C~0VDy 2006 11 24.49415 08 48 18.05 +19 33 54.0 22.4i 05BV49 568 C~0VDy 2006 11 24.54569 08 48 17.98 +19 33 54.5 22.7i 05BV49 568 C~0VDy 2006 11 24.59769 08 48 17.90 +19 33 55.1 23.3i 05BV49 568 C~0VDy 2007 01 19.31365 08 45 00.83 +19 49 54.3 22.9g 05BV49 568 C~0VDy 2007 01 19.35642 08 45 00.60 +19 49 55.1 23.5g 05BV49 568 C~0VDy 2007 01 19.38908 08 45 00.47 +19 49 55.7 05BV49 568 C~0VDy 2007 01 20.37704 08 44 55.53 +19 50 17.0 05BV49 568 C~0VDy 2007 01 20.40060 08 44 55.39 +19 50 17.8 05BV49 568 C~0VDy 2007 01 20.41290 08 44 55.37 +19 50 17.8 05BV49 568 C~0VDy 2008 01 06.359769 08 51 55.51 +19 33 59.7 22.9R 05BV49 568 C~0qjG 2008 01 06.426157 08 51 55.20 +19 34 01.3 22.7R 05BV49 568 C~0qjG 2008 01 07.510822 08 51 50.32 +19 34 24.0 22.9R 05BV49 568 C~0qjG 2008 01 07.539421 08 51 50.19 +19 34 24.7 22.8R 05BV49 568 C~0qjG 2008 01 07.567940 08 51 50.06 +19 34 25.1 23.1R 05BV49 568 C~0qjG 2010 01 21.35555 09 02 23.64 +19 15 15.9 05BV49 568 C~0VDy 2010 01 21.36818 09 02 23.57 +19 15 16.3 05BV49 568 C~0VDy 2010 01 21.40057 09 02 23.41 +19 15 17.0 05BV49 568 C~0VDy 2013 03 13.12705 09 15 53.07 +18 52 18.6 22.5R 05BV49 695 C~0udE 2013 03 13.20695 09 15 52.77 +18 52 19.8 05BV49 695 C~0udE 2013 03 14.14066 09 15 49.23 +18 52 35.1 05BV49 695 C~0udE 2019 02 08.339530 09 53 02.818 +16 59 54.85 23.0G 05BV49 G37 C~2zmb 2019 02 08.478120 09 53 02.127 +16 59 58.81 05BV49 G37 C~2zmb 2021 01 11.428030 10 06 20.687 +16 09 09.81 23.2G 05BV49 G37 C~4TyC 2021 01 11.468990 10 06 20.533 +16 09 10.95 05BV49 G37 C~4TyC 2021 01 11.509080 10 06 20.396 +16 09 11.74 05BV49 G37 C~4TyC 2021 03 20.196870 10 01 18.749 +16 38 23.11 22.5G 05BV49 G37 C~4hk5 2021 03 20.235820 10 01 18.580 +16 38 23.88 05BV49 G37 C~4hk5 2022 03 02.238000 10 08 17.329 +16 11 48.04 22.4G 05BV49 G37 C~5RlV 2022 03 02.295210 10 08 17.091 +16 11 50.15 05BV49 G37 C~5RlV 2022 03 02.347930 10 08 16.851 +16 11 51.57 05BV49 G37 C~5RlV
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 0.03 0.00 -0.35
2 0.0001 0.00 0.08 0.00 -0.30
3 0.0001 0.00 0.09 0.00 -0.20
4 2.9213 0.00 0.20 0.00 0.13
5 2.9214 0.00 0.09 0.00 0.12
6 2.9214 0.00 0.07 0.00 -0.02
7 3.0170 0.00 0.25 0.00 -0.13
8 3.0171 0.00 -0.15 0.00 0.01
9 3.0172 0.00 0.05 0.00 0.23
10 3.2332 0.00 -0.00 0.00 0.14
11 3.2358 0.00 0.07 0.00 0.18
12 3.2360 0.00 0.07 0.00 0.16
13 4.0575 0.00 -0.31 0.00 -0.05
14 4.0603 0.00 -0.47 0.00 -0.07
15 4.8683 0.00 0.24 0.00 0.33
16 4.8710 0.00 -0.05 0.00 -0.03
17 4.8711 0.00 0.00 0.00 -0.04
18 4.8712 0.00 -0.06 0.00 0.05
19 5.0238 0.00 -0.20 0.00 0.21
20 5.0239 0.00 -0.41 0.00 0.07
21 5.0240 0.00 0.12 0.00 -0.04
22 5.0267 0.00 -0.02 0.00 -0.00
23 5.0268 0.00 -0.32 0.00 0.28
24 5.0268 0.00 0.32 0.00 0.02
25 5.9876 0.00 -0.21 0.00 -0.17
26 5.9878 0.00 -0.33 0.00 0.02
27 5.9908 0.00 -0.13 0.00 -0.19
28 5.9909 0.00 -0.09 0.00 -0.09
29 5.9909 0.00 -0.07 0.00 -0.29
30 8.0301 0.00 0.51 0.00 -0.03
31 8.0301 0.00 0.40 0.00 0.07
32 8.0302 0.00 0.41 0.00 0.01
33 11.1698 0.00 -0.23 0.00 0.11
34 11.1700 0.00 -0.04 0.00 -0.00
35 11.1725 0.00 0.13 0.00 0.18
36 17.0786 0.00 0.22 0.00 -0.18
37 17.0790 0.00 -0.00 0.00 0.01
38 19.0036 0.00 -0.09 0.00 -0.08
39 19.0037 0.00 -0.16 0.00 0.03
40 19.0038 0.00 -0.03 0.00 -0.18
41 19.1891 0.00 0.16 0.00 -0.11
42 19.1892 0.00 -0.00 0.00 -0.09
43 20.1393 0.00 -0.42 0.00 -0.37
44 20.1394 0.00 0.10 0.00 0.27
45 20.1396 0.00 0.26 0.00 0.34
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.
05BV49 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.783 43.783 43.783 ecceobj 0.046 0.046 0.046 incobj 7.978 7.978 7.978 qmin 40.436 40.427 40.449 qmax 47.288 47.279 47.279 amean 43.740 43.719 43.745 amin 43.354 43.357 43.377 amax 44.110 44.099 44.107 emean 0.050 0.046 0.049 emin 0.030 0.023 0.029 emax 0.073 0.073 0.073 imean 6.401 6.422 6.439 imin 5.671 5.747 5.766 imax 7.112 7.116 7.110 excite_mean 0.122 0.121 0.122 fracstop 1.000 1.000 1.000 cjmean 3.081 3.081 3.081 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 176.3 175.8 175.9 kozaiamp 180.0 180.0 180.0