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: 19PS99 # Created Wed May 21 01:11:19 2025 # Orbit generated from Bernstein formalism # Fitting 12 observations of 12 # Arc: 1.04d # First observation: 2019/08/05 # Last observation: 2019/08/07 # WARNING Fitting with energy constraint # WARNING and with gdot fixed = 0 # Chi-squared of fit: 1.99 DOF: 20 RMS: 0.07 # Min/Max residuals: -0.13 0.12 # Exact a, adot, b, bdot, g, gdot: 1.765288E-05 3.663950E-02 -1.926334E-06 -3.844864E-03 3.251778E-02 0.000000E+00 # Covariance matrix: 5.3644E-11 1.0966E-07 -3.2019E-12 -6.6587E-09 1.9153E-08 0.0000E+00 1.0966E-07 2.2500E-04 -6.5650E-09 -1.3653E-05 3.9270E-05 0.0000E+00 -3.2019E-12 -6.5650E-09 3.3208E-13 3.6207E-10 -1.1462E-09 0.0000E+00 -6.6587E-09 -1.3653E-05 3.6207E-10 9.0229E-07 -2.3836E-06 0.0000E+00 1.9153E-08 3.9270E-05 -1.1462E-09 -2.3836E-06 6.8562E-06 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 0.0000E+00 4.5246E-04 # lat0 lon0 xBary yBary zBary JD0 -8.539955 -68.212917 -0.367326 -0.139271 -0.927383 2458701.479011 # Heliocentric elements and errors Epoch: 2458700.5000 = 2019/08/05 Mean Anomaly: 17.88075 +/- 123.933 Argument of Peri: 215.62484 +/- 193.651 Long of Asc Node: 57.98924 +/- 5.110 Inclination: 10.14542 +/- 0.661 Eccentricity: 0.03758396 +/- 0.5932 Semi-Major Axis: 32.86087742 +/- 17.6981 Time of Perihelion: 2455283.0633 +/- 161272.0 Perihelion: 31.62583564 +/- 25.8872 Aphelion: 34.09591920 +/- 26.7812 Period (y) 188.3766 +/- 152.18 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X 11.97966549 +/- 0.9087 Ecliptic Y -28.98099516 +/- 2.2740 Ecliptic Z -4.56673962 +/- 0.3677 Ecliptic XDOT 0.00285512 +/- 0.0011 Ecliptic YDOT 0.00118995 +/- 0.0017 Ecliptic ZDOT -0.00032035 +/- 0.0003 # Distances at JD0 (AU) Heliocenter to KBO 31.69014952 +/- 2.1084 Geocenter to KBO 30.75240279 +/- 2.4763 # Hcoef: 8.48
The following table shows the complete astrometric record for 19PS99. 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 (19PS99) followed by the observatory code and reference code for the source of the astrometry.
2019 08 05.97821 19 40 24.83 -30 06 00.7 23.8g 19PS99 W84 C~8r9E 2019 08 05.98548 19 40 24.79 -30 06 00.84 23.5r 19PS99 W84 C~8r9E 2019 08 05.99276 19 40 24.73 -30 06 01.0 19PS99 W84 C~8r9E 2019 08 06.00006 19 40 24.68 -30 06 00.97 19PS99 W84 C~8r9E 2019 08 06.00734 19 40 24.63 -30 06 01.1 19PS99 W84 C~8r9E 2019 08 06.01463 19 40 24.59 -30 06 01.03 19PS99 W84 C~8r9E 2019 08 06.02192 19 40 24.54 -30 06 01.1 19PS99 W84 C~8r9E 2019 08 06.02919 19 40 24.49 -30 06 01.25 19PS99 W84 C~8r9E 2019 08 06.98437 19 40 18.31 -30 06 11.1 19PS99 W84 C~8r9E 2019 08 06.99165 19 40 18.27 -30 06 11.23 19PS99 W84 C~8r9E 2019 08 07.01356 19 40 18.11 -30 06 11.3 19PS99 W84 C~8r9E 2019 08 07.02083 19 40 18.08 -30 06 11.37 19PS99 W84 C~8r9E
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 0.03 0.00 0.01
2 0.0000 -0.54 0.12 -0.05 -0.06
3 0.0000 -1.33 -0.05 -0.07 -0.11
4 0.0001 -1.96 -0.05 0.07 -0.00
5 0.0001 -2.63 -0.09 0.05 -0.04
6 0.0001 -3.13 0.04 0.21 0.09
7 0.0001 -3.78 0.02 0.25 0.10
8 0.0001 -4.44 -0.02 0.21 0.04
9 0.0028 -85.14 -0.03 4.18 -0.04
10 0.0028 -85.68 0.06 4.14 -0.11
11 0.0028 -87.74 -0.13 4.43 0.09
12 0.0029 -88.13 0.10 4.42 0.06
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.
19PS99 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