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: 95YY3 # Created Fri Nov 1 01:07:48 2024 # Orbit generated from Bernstein formalism # Fitting 21 observations of 21 # Arc: 0.72y # First observation: 1995/12/24 # Last observation: 1996/09/13 Preliminary a, adot, b, bdot, g, gdot: -0.000003 0.041072 -0.000002 0.000252 0.033016 0.000000 # Chi-squared of fit: 481.74 DOF: 36 RMS: 0.85 # Min/Max residuals: -2.40 1.60 # Exact a, adot, b, bdot, g, gdot: 2.000425E-05 4.043776E-02 -1.226373E-06 2.496433E-04 3.310478E-02 -3.036594E-02 # Covariance matrix: 3.0932E-13 5.7982E-11 -2.2690E-14 2.6924E-13 1.5950E-11 1.1567E-09 5.7982E-11 3.1831E-08 -1.2091E-11 1.4584E-10 8.4101E-09 6.2427E-07 -2.2690E-14 -1.2091E-11 9.6575E-14 -2.4690E-13 -3.1978E-12 -2.3723E-10 2.6924E-13 1.4584E-10 -2.4690E-13 2.3817E-12 3.8549E-11 2.8608E-09 1.5950E-11 8.4101E-09 -3.1978E-12 3.8549E-11 2.2252E-09 1.6503E-07 1.1567E-09 6.2427E-07 -2.3723E-10 2.8608E-09 1.6503E-07 1.2246E-05 # lat0 lon0 xBary yBary zBary JD0 -0.269161 62.378113 -0.494005 -0.004114 -0.859255 2450075.832758 # Heliocentric elements and errors Epoch: 2450070.5000 = 1995/12/19 Mean Anomaly: 357.21887 +/- 3.674 Argument of Peri: 40.94121 +/- 1.661 Long of Asc Node: 99.53829 +/- 0.146 Inclination: 0.44261 +/- 0.002 Eccentricity: 0.89216696 +/- 0.1007 Semi-Major Axis: 182.34149616 +/- 160.4915 Time of Perihelion: 2457018.2714 +/- 302.9 Perihelion: 19.66243723 +/- 25.2320 Aphelion: 345.02055510 +/- 304.2313 Period (y) 2462.2745 +/- 3250.83 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 13.96861082 +/- 0.0200 Ecliptic Y 27.74724370 +/- 0.0381 Ecliptic Z -0.14193609 +/- 0.0002 Ecliptic XDOT -0.00412002 +/- 0.0001 Ecliptic YDOT -0.00067273 +/- 0.0003 Ecliptic ZDOT 0.00003225 +/- 0.0000 # Distances at JD0 (AU) Heliocenter to KBO 31.06528234 +/- 0.0352 Geocenter to KBO 30.20711659 +/- 0.0430 # Hcoef: 8.50
The following table shows the complete astrometric record for 95YY3. 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 (95YY3) followed by the observatory code and reference code for the source of the astrometry.
1995 12 24.33205 04 01 26.13 +20 22 22.1 23.0R 95YY3 568 C26263 1995 12 24.35745 04 01 25.97 +20 22 21.7 23.0R 95YY3 568 C26263 1995 12 24.37531 04 01 25.87 +20 22 21.5 23.0R 95YY3 568 C26263 1995 12 25.29590 04 01 20.75 +20 22 06.4 23.0R 95YY3 568 C26263 1995 12 25.31176 04 01 20.67 +20 22 06.4 23.0R 95YY3 568 C26263 1995 12 25.32571 04 01 20.57 +20 22 06.1 23.0R 95YY3 568 C26263 1995 12 27.45651 04 01 08.97 +20 21 32.5 23.0R 95YY3 568 C26263 1995 12 27.47286 04 01 08.87 +20 21 32.0 23.0R 95YY3 568 C26263 1996 01 20.21134 03 59 28.40 +20 17 02.6 95YY3 711 C27070 1996 01 21.13715 03 59 25.82 +20 16 54.7 95YY3 711 C27070 1996 01 21.19957 03 59 25.73 +20 16 54.0 95YY3 711 C27070 1996 01 21.20087 03 59 25.69 +20 16 55.4 95YY3 675 C26660 1996 01 21.27806 03 59 25.50 +20 16 53.0 95YY3 711 C27070 1996 01 22.16962 03 59 23.08 +20 16 46.4 95YY3 711 C27070 1996 01 22.23699 03 59 22.78 +20 16 46.7 95YY3 711 C27070 1996 01 22.30343 03 59 22.62 +20 16 46.4 95YY3 711 C27070 1996 01 24.12365 03 59 18.04 +20 16 34.7 95YY3 675 C26660 1996 01 24.21181 03 59 17.87 +20 16 34.2 95YY3 675 C26660 1996 01 24.32038 03 59 17.57 +20 16 33.7 95YY3 675 C26660 1996 09 12.5785 04 20 00.73 +21 11 41.5 24. R 95YY3 568 C27786 1996 09 13.5135 04 20 00.15 +21 11 40.1 95YY3 568 C27786
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 -0.14 0.00 0.28
2 0.0001 -2.28 -0.33 0.05 0.31
3 0.0001 -3.70 -0.28 0.13 0.38
4 0.0026 -77.26 -0.12 -0.50 -0.62
5 0.0027 -78.37 0.06 -0.28 -0.41
6 0.0027 -79.80 -0.24 -0.30 -0.44
7 0.0086 -246.35 0.62 -1.10 -2.19
8 0.0086 -247.83 0.42 -1.32 -2.40
9 0.0736 -1686.47 -0.64 15.03 1.43
10 0.0761 -1723.62 -0.22 14.54 0.39
11 0.0763 -1725.00 0.98 14.10 -0.09
12 0.0763 -1725.27 0.71 15.59 1.41
13 0.0765 -1728.37 0.82 13.77 -0.46
14 0.0790 -1763.06 0.59 14.10 -0.67
15 0.0791 -1767.13 -0.84 15.24 0.42
16 0.0793 -1769.40 -0.53 15.40 0.55
17 0.0843 -1834.88 -0.63 16.81 0.87
18 0.0845 -1837.33 0.08 16.80 0.79
19 0.0848 -1841.56 -0.32 17.15 1.09
20 0.7207 15939.51 1.60 53.87 -0.45
21 0.7233 15931.23 -1.59 53.86 -0.11
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.
95YY3 quality flag:0 Type: ERR2LARGE ERR2LARGE ERR2LARGE axisobj 0.000 0.000 0.000 ecceobj -1.000 -1.000 -1.000 incobj -1.000 -1.000 -1.000 qmin 0.000 0.000 0.000 qmax 0.000 0.000 0.000 amean 0.000 0.000 0.000 amin 0.000 0.000 0.000 amax 0.000 0.000 0.000 emean 0.000 0.000 0.000 emin 0.000 0.000 0.000 emax 0.000 0.000 0.000 imean 0.000 0.000 0.000 imin 0.000 0.000 0.000 imax 0.000 0.000 0.000 excite_mean 0.000 0.000 0.000 fracstop 0.000 0.000 0.000 cjmean 0.000 0.000 0.000 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 0.0 0.0 0.0 kozaiamp 0.0 0.0 0.0