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: 01VN71 # Created Thu May 24 01:37:10 2012 # Orbit generated from Bernstein formalism # Fitting 15 observations of 16 # Arc: 4.12y # First observation: 2001/11/09 # Last observation: 2005/12/23 Preliminary a, adot, b, bdot, g, gdot: -0.000102 0.042236 -0.000130 0.013998 0.033521 0.000000 # Chi-squared of fit: 11.93 DOF: 24 RMS: 0.16 # Min/Max residuals: -0.41 0.23 # Exact a, adot, b, bdot, g, gdot: 2.066920E-05 4.196710E-02 5.794855E-06 1.381185E-02 3.453363E-02 -1.962335E-03 # Covariance matrix: 2.4602E-13 -2.8587E-13 2.3224E-14 -9.6976E-14 1.4363E-13 -1.6721E-12 -2.8587E-13 9.5158E-13 -9.4767E-14 3.4242E-13 8.0209E-14 5.8549E-12 2.3224E-14 -9.4767E-14 1.5491E-13 -8.5633E-14 -1.5689E-14 -6.1261E-13 -9.6976E-14 3.4242E-13 -8.5633E-14 1.8618E-13 1.6248E-15 2.2575E-12 1.4363E-13 8.0209E-14 -1.5689E-14 1.6248E-15 7.0165E-13 -3.1023E-14 -1.6721E-12 5.8549E-12 -6.1261E-13 2.2575E-12 -3.1023E-14 3.8647E-11 # lat0 lon0 xBary yBary zBary JD0 -4.322230 58.305989 0.193948 -0.072872 -0.963013 2452222.953023 # Heliocentric elements and errors Epoch: 2452220.5000 = 2001/11/07 Mean Anomaly: 351.60334 +/- 0.024 Argument of Peri: 1.28791 +/- 0.041 Long of Asc Node: 70.46956 +/- 0.000 Inclination: 18.62084 +/- 0.000 Eccentricity: 0.25329054 +/- 0.0001 Semi-Major Axis: 39.82062604 +/- 0.0059 Time of Perihelion: 2454361.2441 +/- 6.1 Perihelion: 29.73443823 +/- 0.0055 Aphelion: 49.90681384 +/- 0.0081 Period (y) 251.2872 +/- 0.06 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 15.84429554 +/- 0.0004 Ecliptic Y 25.29445114 +/- 0.0006 Ecliptic Z -2.18222269 +/- 0.0001 Ecliptic XDOT -0.00287778 +/- 0.0000 Ecliptic YDOT 0.00168658 +/- 0.0000 Ecliptic ZDOT 0.00110384 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 29.92679494 +/- 0.0005 Geocenter to KBO 28.95728248 +/- 0.0007 # Hcoef: 8.87
The following table shows the complete astrometric record for 01VN71. 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 (01VN71) followed by the observatory code and reference code for the source of the astrometry.
2001 11 09.45228 03 48 13.18 +15 33 57.1 23.9R 01VN71 568 Ce1330 2001 11 09.48072 03 48 13.02 +15 33 56.7 23.9R 01VN71 568 Ce1330 2001 11 09.56655 03 48 12.42 +15 33 55.4 23.8R 01VN71 568 Ce1330 2001 11 10.38146 03 48 06.96 +15 33 43.0 01VN71 568 Ce1330 2001 11 15.26506 03 47 33.76 +15 32 29.5 23.0R 01VN71 309 Ce4815 2001 11 15.29727 03 47 33.54 +15 32 29.0 23.2R 01VN71 309 Ce4815 2002 03 20.25280 03 43 07.88 +15 46 56.9 01VN71 568 Cf5138 2002 03 22.23602 03 43 18.86 +15 48 01.6 23. R 01VN71 568 Cf5138 2002 03 22.24346 03 43 18.88 +15 48 01.9 23. R 01VN71 568 Cf5138 2002 11 11.20716 03 57 10.83 +16 50 44.1 01VN71 695 Cg5849 2002 11 11.26984 03 57 10.37 +16 50 43.5 23.1R 01VN71 695 Cg5849 2002 11 12.20494 03 57 04.06 +16 50 30.4 23.1R 01VN71 695 Cg5849 2002 11 12.31522 03 57 03.32 +16 50 28.9 23.0R 01VN71 695 Cg5849 2002 11 12.38129 03 57 02.86 +16 50 28.1 23.1R 01VN71 695 Cg5849 2005 12 23.30711 04 20 32.26 +20 27 49.1 01VN71 568 Cp7644 2005 12 23.36550 04 20 31.87 +20 27 48.8 01VN71 568 Cp7644
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 -0.30 0.00 0.11 2 0.0001 -2.34 0.19 0.11 0.04 3 0.0003 -11.09 -0.01 0.72 0.11 4 0.0025 -90.80 -0.04 5.74 0.14 5 0.0159 -575.07 0.14 38.29 -0.06 6 0.0160 -578.28 0.19 38.49 -0.08 7 0.3581 -4130.51 0.01 1730.40 -0.15 8 0.3635 -3961.53 0.07 1758.18 -0.41 9 0.3636 -3961.18 -0.22 1758.41 -0.29 10 1.0041 8549.25 -0.04 2865.08 0.23 11 1.0043 8542.65 ( -0.42) 2865.86 ( 0.56) 12 1.0069 8451.15 -0.18 2871.71 0.15 13 1.0072 8440.42 0.10 2872.44 0.07 14 1.0073 8433.79 0.07 2873.01 0.18 15 4.1201 30834.59 0.07 11952.07 -0.08 16 4.1202 30829.01 -0.05 11952.72 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.
01VN71 quality flag:3 Type: 3:2E 3:2E 3:2E axisobj 39.854 39.872 39.837 ecceobj 0.253 0.254 0.253 incobj 18.623 18.623 18.623 qmin 27.268 27.012 29.512 qmax 51.828 52.205 49.587 amean 39.453 39.453 39.454 amin 39.333 39.316 39.348 amax 39.612 39.629 39.578 emean 0.244 0.250 0.218 emin 0.174 0.174 0.170 emax 0.309 0.318 0.253 imean 17.299 16.825 18.263 imin 13.672 13.155 17.082 imax 20.094 20.054 19.927 excite_mean 0.387 0.386 0.383 fracstop 1.000 1.000 1.000 cjmean 2.881 2.882 2.884 libcent 0 181.1 180.9 180.9 libamp 0 57.6 64.2 52.4 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 154.1 279.6 198.3 kozaiamp 180.0 180.0 180.0