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: 02VX130
# Created Thu Nov 21 02:08:24 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting 24 observations of 24
# Arc: 19.00y
# First observation: 2002/11/07
# Last observation: 2021/11/05
# Chi-squared of fit: 82.22 DOF: 42 RMS: 0.33
# Min/Max residuals: -0.67 1.19
# Exact a, adot, b, bdot, g, gdot:
2.009320E-05 4.190396E-02 -1.922429E-07 -7.390466E-05 3.351821E-02 -1.764591E-03
# Covariance matrix:
7.5600E-13 -3.0994E-13 3.7310E-15 2.2367E-16 8.5088E-13 -2.6643E-13
-3.0994E-13 1.4914E-13 -1.8580E-15 -1.0926E-16 -4.2294E-13 1.3126E-13
3.7310E-15 -1.8580E-15 1.4824E-13 -1.0480E-14 6.8598E-15 -1.6315E-15
2.2367E-16 -1.0926E-16 -1.0480E-14 1.5520E-15 2.3521E-16 -9.8240E-17
8.5088E-13 -4.2294E-13 6.8598E-15 2.3521E-16 1.4981E-12 -3.7223E-13
-2.6643E-13 1.3126E-13 -1.6315E-15 -9.8240E-17 -3.7223E-13 1.1680E-13
# lat0 lon0 xBary yBary zBary JD0
1.358358 31.368795 -0.221410 0.022802 -0.962924 2452585.690753
# Heliocentric elements and errors
Epoch: 2452586.5000 = 2002/11/08
Mean Anomaly: 352.84789 +/- 6.417
Argument of Peri: 106.18903 +/- 0.002
Long of Asc Node: 297.19079 +/- 0.002
Inclination: 1.32004 +/- 0.000
Eccentricity: 0.22543206 +/- 0.0024
Semi-Major Axis: 39.61503747 +/- 0.0014
Time of Perihelion: 2454395.8397 +/- 1623.4
Perihelion: 30.68453797 +/- 0.0968
Aphelion: 48.54553697 +/- 0.0968
Period (y) 249.3436 +/- 0.01
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 26.17247004 +/- 0.0036
Ecliptic Y 16.22177618 +/- 0.0021
Ecliptic Z 0.70725462 +/- 0.0001
Ecliptic XDOT -0.00191208 +/- 0.0000
Ecliptic YDOT 0.00284415 +/- 0.0000
Ecliptic ZDOT -0.00000924 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 30.80009354 +/- 0.0033
Geocenter to KBO 29.83459433 +/- 0.0042
# Hcoef: 8.34
The following table shows the complete astrometric record for 02VX130. 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 (02VX130) followed by the observatory code and reference code for the source of the astrometry.
2002 11 07.19001 01 54 56.64 +13 13 25.0 22.3R 02VX130 695 Cg8319 2002 11 07.29686 01 54 55.98 +13 13 21.5 02VX130 695 Cg8319 2002 12 01.34477 01 52 48.63 +13 01 14.9 23.0R 02VX130 568 Cg8319 2002 12 02.25460 01 52 44.64 +13 00 49.4 02VX130 568 Cg8319 2002 12 02.31430 01 52 44.38 +13 00 47.8 02VX130 568 Cg8319 2003 10 23.18857 02 05 48.67 +14 11 12.9 22.3R 02VX130 695 Cj4694 2003 10 23.28356 02 05 48.08 +14 11 09.9 02VX130 695 Cj4694 2003 11 20.14996 02 03 00.52 +13 56 09.5 22.9R 02VX130 695 Cj4694 2003 11 20.23472 02 03 00.06 +13 56 07.1 02VX130 695 Cj4694 2003 11 24.16271 02 02 38.93 +13 54 09.6 23.2R 02VX130 695 Cj4694 2003 11 24.23152 02 02 38.59 +13 54 07.7 02VX130 695 Cj4694 2003 12 17.26629 02 00 59.86 +13 44 37.1 23.2R 02VX130 568 Ck9585 2003 12 17.33675 02 00 59.61 +13 44 35.6 02VX130 568 Ck9585 2004 09 17.47950 02 18 23.03 +15 14 37.0 23.7R 02VX130 568 Cl5726 2004 09 17.51728 02 18 22.89 +15 14 36.2 02VX130 568 Cl5726 2008 08 31.06699 02 57 09.47 +18 09 58.9 23.9R 02VX130 250 S~06Aa 2008 08 31.07393 02 57 09.46 +18 09 58.8 02VX130 250 S~06Aa 2008 08 31.08018 02 57 09.45 +18 09 58.8 02VX130 250 S~06Aa 2008 08 31.08713 02 57 09.44 +18 09 58.8 02VX130 250 S~06Aa 2008 10 22.26115 02 53 35.14 +17 56 06.4 22.4r 02VX130 695 C~0gM1 2008 10 22.29270 02 53 34.95 +17 56 05.7 22.5r 02VX130 695 C~0gM1 2021 11 05.420400 05 01 16.336 +23 39 09.65 23.2G 02VX130 G37 C~5B6q 2021 11 05.461730 05 01 16.100 +23 39 09.50 02VX130 G37 C~5B6q 2021 11 05.503340 05 01 15.862 +23 39 09.29 02VX130 G37 C~5B6q
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 -0.08 0.00 0.01
2 0.0003 0.00 -0.29 0.00 0.03
3 0.0661 0.00 0.35 0.00 1.19
4 0.0686 0.00 0.57 0.00 -0.57
5 0.0688 0.00 0.69 0.00 -0.63
6 0.9582 0.00 -0.05 0.00 -0.12
7 0.9585 0.00 0.07 0.00 -0.06
8 1.0348 0.00 -0.35 0.00 -0.29
9 1.0350 0.00 -0.12 0.00 -0.11
10 1.0458 0.00 -0.10 0.00 0.00
11 1.0460 0.00 0.33 0.00 0.12
12 1.1090 0.00 -0.38 0.00 0.09
13 1.1092 0.00 -0.67 0.00 -0.05
14 1.8625 0.00 -0.17 0.00 -0.24
15 1.8626 0.00 0.20 0.00 -0.31
16 5.8149 0.00 0.19 0.00 0.32
17 5.8149 0.00 0.18 0.00 0.24
18 5.8149 0.00 0.16 0.00 0.27
19 5.8149 0.00 0.15 0.00 0.29
20 5.9578 0.00 -0.16 0.00 0.19
21 5.9578 0.00 -0.06 0.00 0.30
22 18.9958 0.00 0.09 0.00 -0.25
23 18.9960 0.00 0.00 0.00 -0.10
24 18.9961 0.00 -0.09 0.00 -0.00
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.
02VX130 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.916 39.916 39.916 ecceobj 0.231 0.231 0.231 incobj 1.320 1.320 1.320 qmin 29.917 29.915 29.917 qmax 49.432 49.435 49.429 amean 39.455 39.455 39.455 amin 39.059 39.060 39.060 amax 39.916 39.916 39.916 emean 0.223 0.223 0.223 emin 0.204 0.204 0.204 emax 0.240 0.240 0.240 imean 1.707 1.707 1.707 imin 0.662 0.659 0.664 imax 3.138 3.138 3.138 excite_mean 0.225 0.225 0.225 fracstop 1.000 1.000 1.000 cjmean 2.993 2.993 2.993 libcent 0 179.4 179.6 179.1 libamp 0 51.7 51.5 51.7 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 181.3 181.4 181.3 kozaiamp 180.0 180.0 179.9