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: 19GX196
# Created Fri Jan 24 02:11:39 2025
# Orbit generated from Bernstein formalism
# Fitting 9 observations of 9
# Arc: 59.02d
# First observation: 2019/02/05
# Last observation: 2019/04/05
Preliminary a, adot, b, bdot, g, gdot:
-0.000000 0.021002 0.000000 -0.002186 0.026326 0.000000
# WARNING MRQMIN stopped after 13 iterations -- oscilliatory solution
# WARNING Fitting with energy constraint
# Chi-squared of fit: 2.14 DOF: 13 RMS: 0.09
# Min/Max residuals: -0.19 0.15
# Exact a, adot, b, bdot, g, gdot:
1.530954E-05 2.771367E-02 -1.207435E-06 -2.329975E-03 2.729627E-02 -2.165234E-03
# Covariance matrix:
2.4373E-11 4.2542E-08 -7.8322E-13 -1.0407E-09 7.8748E-09 1.5193E-07
4.2542E-08 7.5784E-05 -1.3949E-09 -1.8535E-06 1.4023E-05 2.6960E-04
-7.8322E-13 -1.3949E-09 5.1235E-13 3.1085E-11 -2.5833E-10 -5.0249E-09
-1.0407E-09 -1.8535E-06 3.1085E-11 4.5378E-08 -3.4322E-07 -6.6639E-06
7.8748E-09 1.4023E-05 -2.5833E-10 -3.4322E-07 2.5983E-06 5.0831E-05
1.5193E-07 2.6960E-04 -5.0249E-09 -6.6639E-06 5.0831E-05 1.2216E-03
# lat0 lon0 xBary yBary zBary JD0
4.170778 -177.294584 0.723195 0.049443 -0.677113 2458520.038641
# Heliocentric elements and errors
Epoch: 2458520.5000 = 2019/02/06
Mean Anomaly: 269.44756 +/- 185.180
Argument of Peri: 240.95395 +/- 162.176
Long of Asc Node: 42.39228 +/- 7.497
Inclination: 6.25308 +/- 0.956
Eccentricity: 0.09988030 +/- 1.2755
Semi-Major Axis: 36.91737189 +/- 8.3417
Time of Perihelion: 2479128.8036 +/- 41561.2
Perihelion: 33.23005353 +/- 47.6846
Aphelion: 40.60469025 +/- 47.9753
Period (y) 224.3130 +/- 76.03
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -37.20853462 +/- 2.1553
Ecliptic Y -1.04233696 +/- 0.1017
Ecliptic Z 2.66438982 +/- 0.1573
Ecliptic XDOT 0.00033863 +/- 0.0035
Ecliptic YDOT -0.00276885 +/- 0.0009
Ecliptic ZDOT -0.00024908 +/- 0.0002
# Distances at JD0 (AU)
Heliocenter to KBO 37.31836663 +/- 2.1490
Geocenter to KBO 36.63504772 +/- 2.1634
# Hcoef: 9.72
The following table shows the complete astrometric record for 19GX196. 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 (19GX196) followed by the observatory code and reference code for the source of the astrometry.
2019 02 05.53784 12 16 33.75 +02 45 05.0 24.9i 19GX196 T09 C~8SgA 2019 02 05.55837 12 16 33.67 +02 45 05.7 24.8i 19GX196 T09 C~8SgA 2019 02 05.62764 12 16 33.46 +02 45 07.2 25.1i 19GX196 T09 C~8SgA 2019 04 04.44950 12 12 13.23 +03 14 06.9 25.9g 19GX196 T09 C~8SgA 2019 04 04.45934 12 12 13.18 +03 14 07.1 26.3g 19GX196 T09 C~8SgA 2019 04 04.51398 12 12 12.91 +03 14 08.6 26.1g 19GX196 T09 C~8SgA 2019 04 05.52240 12 12 07.91 +03 14 38.2 25.5r 19GX196 T09 C~8SgA 2019 04 05.53497 12 12 07.84 +03 14 38.3 25.1r 19GX196 T09 C~8SgA 2019 04 05.55592 12 12 07.74 +03 14 39.2 25.4r 19GX196 T09 C~8SgA
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 -0.03
2 0.0001 -1.38 -0.14 0.17 0.07
3 0.0002 -4.86 0.02 0.29 -0.04
4 0.1586 -4273.91 -0.05 47.85 0.06
5 0.1586 -4274.68 -0.02 47.73 -0.02
6 0.1587 -4278.99 0.10 47.51 -0.07
7 0.1615 -4359.50 0.02 44.96 0.10
8 0.1615 -4360.50 0.03 44.63 -0.19
9 0.1616 -4362.24 -0.02 44.86 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.
19GX196 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