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: 19CS32 # Created Tue Apr 1 01:11:11 2025 # Orbit generated from Bernstein formalism # Fitting 32 observations of 32 # Arc: 97.00d # First observation: 2019/02/02 # Last observation: 2019/05/10 Preliminary a, adot, b, bdot, g, gdot: 0.000000 0.034131 0.000002 0.003125 0.028763 0.000000 # Chi-squared of fit: 4.72 DOF: 58 RMS: 0.07 # Min/Max residuals: -0.21 0.19 # Exact a, adot, b, bdot, g, gdot: 1.870889E-05 3.416496E-02 1.705611E-06 3.232492E-03 2.831549E-02 4.748136E-03 # Covariance matrix: 1.7893E-13 -5.7330E-11 -2.8972E-14 -1.2279E-11 -1.2561E-11 -9.1609E-11 -5.7330E-11 7.9400E-08 5.1883E-11 1.6472E-08 2.0721E-08 6.9982E-07 -2.8972E-14 5.1883E-11 1.8672E-13 9.1535E-12 1.8600E-11 1.3708E-09 -1.2279E-11 1.6472E-08 9.1535E-12 3.4864E-09 3.9936E-09 9.0100E-08 -1.2561E-11 2.0721E-08 1.8600E-11 3.9936E-09 6.8136E-09 4.3648E-07 -9.1609E-11 6.9982E-07 1.3708E-09 9.0100E-08 4.3648E-07 5.1996E-05 # lat0 lon0 xBary yBary zBary JD0 -18.576783 -145.436795 0.982031 -0.043831 -0.130764 2458516.728911 # Heliocentric elements and errors Epoch: 2458510.5000 = 2019/01/27 Mean Anomaly: 10.38796 +/- 16.312 Argument of Peri: 260.51275 +/- 39.529 Long of Asc Node: 288.05892 +/- 0.201 Inclination: 19.08981 +/- 0.016 Eccentricity: 0.36324347 +/- 0.1249 Semi-Major Axis: 54.45861013 +/- 6.2087 Time of Perihelion: 2454274.7933 +/- 6611.5 Perihelion: 34.67687571 +/- 7.8694 Aphelion: 74.24034456 +/- 10.8599 Period (y) 401.8908 +/- 68.73 # Ecliptic coordinates at JD0 (AU and AU/d) Ecliptic X -28.23707844 +/- 0.0804 Ecliptic Y -18.26918347 +/- 0.0554 Ecliptic Z -11.25092078 +/- 0.0328 Ecliptic XDOT 0.00144175 +/- 0.0005 Ecliptic YDOT -0.00302545 +/- 0.0004 Ecliptic ZDOT 0.00014980 +/- 0.0002 # Distances at JD0 (AU) Heliocenter to KBO 35.46376859 +/- 0.0708 Geocenter to KBO 35.31636069 +/- 0.1030 # Hcoef: 7.31
The following table shows the complete astrometric record for 19CS32. 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 (19CS32) followed by the observatory code and reference code for the source of the astrometry.
2019 02 02.22811 13 40 38.48 -30 24 38.4 22.9r 19CS32 W84 C~8eYp 2019 02 02.23134 13 40 38.47 -30 24 38.5 19CS32 W84 C~8eYp 2019 02 02.23457 13 40 38.46 -30 24 38.6 19CS32 W84 C~8eYp 2019 02 02.38771 13 40 38.38 -30 24 43.3 19CS32 W84 C~8eYp 2019 02 02.39096 13 40 38.38 -30 24 43.3 19CS32 W84 C~8eYp 2019 02 03.25024 13 40 37.90 -30 25 08.7 19CS32 W84 C~8eYp 2019 02 03.25348 13 40 37.90 -30 25 09.0 19CS32 W84 C~8eYp 2019 02 03.25671 13 40 37.90 -30 25 09.2 19CS32 W84 C~8eYp 2019 02 03.34370 13 40 37.84 -30 25 11.7 19CS32 W84 C~8eYp 2019 02 03.34694 13 40 37.83 -30 25 11.9 19CS32 W84 C~8eYp 2019 02 03.35017 13 40 37.83 -30 25 11.9 19CS32 W84 C~8eYp 2019 05 09.05998 13 33 37.46 -30 12 11.6 22.7r 19CS32 W84 C~8eYp 2019 05 09.14622 13 33 36.99 -30 12 08.3 19CS32 W84 C~8eYp 2019 05 09.14945 13 33 36.97 -30 12 08.1 19CS32 W84 C~8eYp 2019 05 09.15267 13 33 36.95 -30 12 08.1 19CS32 W84 C~8eYp 2019 05 09.20906 13 33 36.65 -30 12 05.7 19CS32 W84 C~8eYp 2019 05 09.21228 13 33 36.63 -30 12 05.6 19CS32 W84 C~8eYp 2019 05 09.29103 13 33 36.19 -30 12 02.4 19CS32 W84 C~8eYp 2019 05 09.29425 13 33 36.18 -30 12 02.3 19CS32 W84 C~8eYp 2019 05 09.29747 13 33 36.16 -30 12 02.2 19CS32 W84 C~8eYp 2019 05 09.33052 13 33 35.99 -30 12 00.9 19CS32 W84 C~8eYp 2019 05 09.33375 13 33 35.99 -30 12 00.8 19CS32 W84 C~8eYp 2019 05 09.33697 13 33 35.96 -30 12 00.7 19CS32 W84 C~8eYp 2019 05 10.01415 13 33 32.41 -30 11 33.8 19CS32 W84 C~8eYp 2019 05 10.01737 13 33 32.39 -30 11 33.8 19CS32 W84 C~8eYp 2019 05 10.02060 13 33 32.37 -30 11 33.7 19CS32 W84 C~8eYp 2019 05 10.15850 13 33 31.63 -30 11 28.2 19CS32 W84 C~8eYp 2019 05 10.16172 13 33 31.61 -30 11 28.0 19CS32 W84 C~8eYp 2019 05 10.16494 13 33 31.60 -30 11 27.9 19CS32 W84 C~8eYp 2019 05 10.21743 13 33 31.32 -30 11 25.8 19CS32 W84 C~8eYp 2019 05 10.22066 13 33 31.30 -30 11 25.6 19CS32 W84 C~8eYp 2019 05 10.22388 13 33 31.29 -30 11 25.6 19CS32 W84 C~8eYp
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 0.02
2 0.0000 -0.08 -0.02 -0.14 -0.02
3 0.0000 -0.16 -0.12 -0.28 -0.06
4 0.0004 0.66 0.02 -5.02 -0.04
5 0.0004 0.66 0.00 -5.02 0.06
6 0.0028 4.57 -0.10 -30.88 0.19
7 0.0028 4.68 0.01 -31.16 0.01
8 0.0028 4.76 0.07 -31.34 -0.07
9 0.0031 4.99 0.06 -33.95 0.02
10 0.0031 4.95 0.01 -34.18 -0.11
11 0.0031 4.95 0.00 -34.18 -0.01
12 0.2624 -5317.64 0.06 -1421.56 0.08
13 0.2626 -5324.54 0.07 -1420.93 -0.02
14 0.2626 -5324.86 0.01 -1420.84 0.03
15 0.2626 -5325.10 0.03 -1420.95 -0.10
16 0.2628 -5329.62 0.03 -1420.27 0.08
17 0.2628 -5329.90 0.01 -1420.28 0.04
18 0.2630 -5336.41 -0.21 -1419.59 0.01
19 0.2630 -5336.57 -0.11 -1419.55 0.02
20 0.2630 -5336.84 -0.13 -1419.56 -0.02
21 0.2631 -5339.38 -0.04 -1419.23 -0.01
22 0.2631 -5339.42 0.18 -1419.14 0.05
23 0.2631 -5339.82 0.04 -1419.20 -0.04
24 0.2650 -5392.76 0.01 -1412.63 0.07
25 0.2650 -5393.00 0.02 -1412.73 -0.06
26 0.2650 -5393.27 0.00 -1412.74 -0.10
27 0.2654 -5404.27 -0.02 -1411.47 -0.06
28 0.2654 -5404.58 -0.08 -1411.39 -0.01
29 0.2654 -5404.74 0.02 -1411.34 0.00
30 0.2655 -5408.91 0.03 -1410.85 0.01
31 0.2656 -5409.23 -0.03 -1410.76 0.06
32 0.2656 -5409.35 0.11 -1410.82 -0.02
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.
19CS32 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