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: 02VV130 # Created Thu Apr 25 01:11:11 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 22 observations of 22 # Arc: 18.85y # First observation: 2002/11/07 # Last observation: 2021/09/13 # Chi-squared of fit: 32.39 DOF: 38 RMS: 0.21 # Min/Max residuals: -0.42 0.58 # Exact a, adot, b, bdot, g, gdot: 1.838332E-05 2.990915E-02 -2.029667E-06 -1.097507E-03 2.760382E-02 -3.837394E-03 # Covariance matrix: 7.2481E-13 -2.1863E-13 -1.1992E-14 4.2615E-15 1.3308E-12 -1.6338E-13 -2.1863E-13 8.1920E-14 4.6063E-15 -1.7769E-15 -4.5932E-13 6.8718E-14 -1.1992E-14 4.6063E-15 1.6000E-13 -1.0515E-14 -2.6732E-14 3.8821E-15 4.2615E-15 -1.7769E-15 -1.0515E-14 1.3946E-15 8.3691E-15 -1.6895E-15 1.3308E-12 -4.5932E-13 -2.6732E-14 8.3691E-15 3.3846E-12 -3.1611E-13 -1.6338E-13 6.8718E-14 3.8821E-15 -1.6895E-15 -3.1611E-13 6.6080E-14 # lat0 lon0 xBary yBary zBary JD0 -1.188649 19.962750 -0.406790 -0.018720 -0.900528 2452585.644793 # Heliocentric elements and errors Epoch: 2452586.5000 = 2002/11/08 Mean Anomaly: 323.22670 +/- 0.026 Argument of Peri: 259.92286 +/- 0.037 Long of Asc Node: 171.48743 +/- 0.001 Inclination: 2.38283 +/- 0.000 Eccentricity: 0.17127015 +/- 0.0002 Semi-Major Axis: 42.39422552 +/- 0.0184 Time of Perihelion: 2462885.3468 +/- 59.3 Perihelion: 35.13336020 +/- 0.0176 Aphelion: 49.65509084 +/- 0.0233 Period (y) 276.0376 +/- 0.18 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 34.74937042 +/- 0.0024 Ecliptic Y 13.06099999 +/- 0.0008 Ecliptic Z -0.75155709 +/- 0.0001 Ecliptic XDOT -0.00138002 +/- 0.0000 Ecliptic YDOT 0.00265414 +/- 0.0000 Ecliptic ZDOT -0.00010073 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 37.13056440 +/- 0.0022 Geocenter to KBO 36.22698494 +/- 0.0025 # Hcoef: 7.51
The following table shows the complete astrometric record for 02VV130. 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 (02VV130) followed by the observatory code and reference code for the source of the astrometry.
2002 11 07.14405 01 15 31.88 +06 42 15.0 22.7R 02VV130 695 Cg8319 2002 11 07.25151 01 15 31.39 +06 42 11.9 02VV130 695 Cg8319 2002 12 01.31020 01 14 00.14 +06 33 14.6 23.4R 02VV130 568 Cg8319 2002 12 01.35629 01 14 00.00 +06 33 13.6 02VV130 568 Cg8319 2002 12 02.32582 01 13 57.23 +06 32 57.6 02VV130 568 Cg8319 2002 12 05.08615 01 13 49.65 +06 32 15.0 22.7R 02VV130 695 Ch1653 2002 12 05.19676 01 13 49.35 +06 32 13.5 02VV130 695 Ch1653 2002 12 06.21327 01 13 46.78 +06 31 59.2 02VV130 695 Ch1653 2003 10 23.16899 01 23 17.04 +07 24 46.6 22.5R 02VV130 695 Cj4694 2003 10 23.26429 01 23 16.54 +07 24 43.6 02VV130 695 Cj4694 2003 11 20.13563 01 21 08.19 +07 12 03.0 22.8R 02VV130 695 Cj4694 2003 11 20.21942 01 21 07.86 +07 12 01.1 02VV130 695 Cj4694 2004 09 17.50381 01 32 43.07 +08 17 03.6 23.2R 02VV130 568 Cl5726 2004 09 17.54577 01 32 42.88 +08 17 02.6 02VV130 568 Cl5726 2008 11 02.391039 01 55 57.03 +10 12 33.6 22.6V 02VV130 645 C~2Jx8 2008 11 02.391868 01 55 57.03 +10 12 33.7 22.8V 02VV130 645 C~2Jx8 2008 11 02.394356 01 55 57.01 +10 12 33.6 23.7V 02VV130 645 C~2Jx8 2014 08 29.59434 02 42 54.544 +13 52 05.27 23.2r 02VV130 568 C~18Ad 2014 08 29.63456 02 42 54.491 +13 52 04.90 23.2r 02VV130 568 C~18Ad 2021 09 13.38980 03 34 20.81 +17 01 54.5 02VV130 G37 C~553b 2021 09 13.41802 03 34 20.76 +17 01 54.3 02VV130 G37 C~553b 2021 09 13.47420 03 34 20.66 +17 01 53.7 02VV130 G37 C~553b
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 -0.35 0.00 0.17
2 0.0003 0.00 -0.30 0.00 -0.03
3 0.0662 0.00 0.10 0.00 -0.20
4 0.0663 0.00 0.10 0.00 -0.42
5 0.0689 0.00 0.58 0.00 -0.39
6 0.0765 0.00 -0.06 0.00 -0.07
7 0.0768 0.00 -0.09 0.00 0.06
8 0.0796 0.00 0.43 0.00 0.44
9 0.9583 0.00 0.01 0.00 0.29
10 0.9586 0.00 -0.17 0.00 0.18
11 1.0349 0.00 -0.35 0.00 0.00
12 1.0351 0.00 -0.26 0.00 0.01
13 1.8627 0.00 0.15 0.00 0.05
14 1.8628 0.00 0.05 0.00 0.17
15 5.9884 0.00 0.14 0.00 -0.21
16 5.9884 0.00 0.21 0.00 -0.09
17 5.9884 0.00 0.10 0.00 -0.11
18 11.8096 0.00 -0.22 0.00 0.09
19 11.8097 0.00 -0.11 0.00 0.13
20 18.8508 0.00 0.03 0.00 -0.04
21 18.8509 0.00 0.03 0.00 0.02
22 18.8510 0.00 0.03 0.00 -0.03
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.
02VV130 quality flag:3 Type: 5:3EE 5:3EE 5:3EE axisobj 42.721 42.721 42.721 ecceobj 0.174 0.174 0.174 incobj 2.377 2.377 2.377 qmin 34.724 34.723 34.724 qmax 50.320 50.314 50.326 amean 42.328 42.328 42.328 amin 41.940 41.940 41.940 amax 42.738 42.738 42.739 emean 0.163 0.163 0.163 emin 0.149 0.149 0.149 emax 0.178 0.178 0.178 imean 2.621 2.621 2.621 imin 2.140 2.140 2.140 imax 3.151 3.151 3.151 excite_mean 0.169 0.169 0.169 fracstop 1.000 1.000 1.000 cjmean 3.048 3.048 3.048 libcent 0 179.3 179.4 179.0 libamp 0 30.7 30.8 30.7 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 170.3 170.2 170.3 kozaiamp 180.0 180.0 180.0