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: 04VX130 # Created Thu Apr 18 01:12:12 2024 # Orbit generated by ELGB # -->Covariance matrix from a Bernstein fit # Fitting 22 observations of 22 # Arc: 16.08y # First observation: 2004/11/09 # Last observation: 2020/12/09 # Chi-squared of fit: 72.81 DOF: 38 RMS: 0.32 # Min/Max residuals: -0.50 0.73 # Exact a, adot, b, bdot, g, gdot: 1.725494E-05 3.277187E-02 3.305876E-06 3.290422E-03 2.961564E-02 5.634018E-03 # Covariance matrix: 1.9305E-13 -1.2147E-13 1.1721E-14 -1.2089E-14 1.6880E-13 -2.2992E-13 -1.2147E-13 1.3545E-13 -1.3806E-14 1.4241E-14 -2.1984E-13 2.7112E-13 1.1721E-14 -1.3806E-14 9.6992E-14 -9.5953E-15 2.3541E-14 -2.8163E-14 -1.2089E-14 1.4241E-14 -9.5953E-15 3.8813E-15 -2.4315E-14 2.9052E-14 1.6880E-13 -2.1984E-13 2.3541E-14 -2.4315E-14 7.2244E-13 -4.6717E-13 -2.2992E-13 2.7112E-13 -2.8163E-14 2.9052E-14 -4.6717E-13 5.5331E-13 # lat0 lon0 xBary yBary zBary JD0 -0.331938 41.051423 -0.103737 -0.005616 -0.987383 2453318.888263 # Heliocentric elements and errors Epoch: 2453318.5000 = 2004/11/09 Mean Anomaly: 45.69964 +/- 0.019 Argument of Peri: 291.02927 +/- 0.024 Long of Asc Node: 44.42922 +/- 0.000 Inclination: 5.75477 +/- 0.000 Eccentricity: 0.20533385 +/- 0.0001 Semi-Major Axis: 39.33957709 +/- 0.0065 Time of Perihelion: 2441877.7825 +/- 5.5 Perihelion: 31.26183024 +/- 0.0060 Aphelion: 47.41732394 +/- 0.0084 Period (y) 246.7475 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 26.13501991 +/- 0.0007 Ecliptic Y 22.90275255 +/- 0.0006 Ecliptic Z -0.19551258 +/- 0.0000 Ecliptic XDOT -0.00159674 +/- 0.0000 Ecliptic YDOT 0.00262073 +/- 0.0000 Ecliptic ZDOT 0.00030125 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 34.75063282 +/- 0.0007 Geocenter to KBO 33.76588761 +/- 0.0010 # Hcoef: 7.64
The following table shows the complete astrometric record for 04VX130. 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 (04VX130) followed by the observatory code and reference code for the source of the astrometry.
2004 11 09.38752 02 34 55.59 +14 49 40.1 23.1g 04VX130 568 C~0Ur5 2004 11 09.41396 02 34 55.44 +14 49 39.5 23.1g 04VX130 568 C~0Ur5 2004 11 09.43995 02 34 55.30 +14 49 38.9 23.1g 04VX130 568 C~0Ur5 2004 11 10.30006 02 34 50.34 +14 49 17.5 23.0g 04VX130 568 C~0Ur5 2004 11 10.30379 02 34 50.36 +14 49 17.6 23.0g 04VX130 568 C~0Ur5 2005 01 05.22568 02 30 55.55 +14 32 44.7 23.1i 04VX130 568 C~0Ur5 2005 01 05.28317 02 30 55.44 +14 32 44.3 23.4i 04VX130 568 C~0Ur5 2005 01 05.35171 02 30 55.30 +14 32 44.2 23.0i 04VX130 568 C~0Ur5 2005 10 25.51435 02 43 29.59 +15 40 47.6 22.8r 04VX130 568 C~0Ur5 2005 10 25.58096 02 43 29.21 +15 40 46.1 23.1r 04VX130 568 C~0Ur5 2005 10 25.59068 02 43 29.15 +15 40 45.8 23.1r 04VX130 568 C~0Ur5 2005 10 26.55437 02 43 23.68 +15 40 22.6 23.2r 04VX130 568 C~0Ur5 2006 10 23.24732 02 50 48.55 +16 25 08.7 04VX130 675 C~0Ur5 2006 10 23.28645 02 50 48.33 +16 25 07.8 22.5R 04VX130 675 C~0Ur5 2006 10 23.33627 02 50 48.04 +16 25 06.7 04VX130 675 C~0Ur5 2007 11 08.21242 02 56 21.96 +17 01 13.5 23.4r 04VX130 695 C~0Ur5 2007 11 08.27227 02 56 21.61 +17 01 12.1 23.7r 04VX130 695 C~0Ur5 2009 08 18.45633 03 14 55.88 +18 35 55.7 04VX130 675 C~0Ur5 2009 08 19.45039 03 14 56.36 +18 36 00.3 04VX130 675 C~0Ur5 2020 12 09.284290 04 22 16.886 +23 56 25.81 22.7G 04VX130 G37 C~4Ty3 2020 12 09.327050 04 22 16.586 +23 56 25.42 04VX130 G37 C~4Ty3 2020 12 09.363010 04 22 16.387 +23 56 25.06 04VX130 G37 C~4Ty3
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 0.15 0.00 -0.29
2 0.0001 0.00 0.22 0.00 -0.22
3 0.0001 0.00 0.40 0.00 -0.17
4 0.0025 0.00 -0.29 0.00 0.02
5 0.0025 0.00 0.33 0.00 0.21
6 0.1556 0.00 -0.17 0.00 0.18
7 0.1558 0.00 -0.20 0.00 0.14
8 0.1560 0.00 -0.38 0.00 0.46
9 0.9586 0.00 0.07 0.00 -0.43
10 0.9588 0.00 0.11 0.00 -0.32
11 0.9588 0.00 0.05 0.00 -0.39
12 0.9614 0.00 -0.02 0.00 -0.50
13 1.9517 0.00 -0.23 0.00 0.73
14 1.9518 0.00 -0.23 0.00 0.70
15 1.9519 0.00 -0.36 0.00 0.72
16 2.9947 0.00 0.37 0.00 -0.11
17 2.9949 0.00 0.42 0.00 -0.15
18 4.7723 0.00 -0.07 0.00 -0.33
19 4.7750 0.00 -0.08 0.00 -0.27
20 16.0819 0.00 0.44 0.00 -0.11
21 16.0820 0.00 -0.30 0.00 0.04
22 16.0821 0.00 -0.12 0.00 0.14
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.
04VX130 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.847 39.847 39.847 ecceobj 0.213 0.213 0.213 incobj 5.730 5.730 5.730 qmin 30.504 30.506 30.503 qmax 48.923 48.918 48.926 amean 39.455 39.455 39.455 amin 39.091 39.090 39.091 amax 39.878 39.875 39.881 emean 0.206 0.207 0.206 emin 0.188 0.188 0.187 emax 0.227 0.227 0.227 imean 4.844 4.844 4.844 imin 4.278 4.278 4.278 imax 5.625 5.625 5.625 excite_mean 0.223 0.223 0.223 fracstop 1.000 1.000 1.000 cjmean 2.995 2.995 2.995 libcent 0 180.0 180.1 179.8 libamp 0 37.0 36.9 36.9 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 205.0 205.0 205.0 kozaiamp 180.0 180.0 180.0