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: 19VE51
# Created Wed Nov 27 02:11:00 2024
# Orbit generated from Bernstein formalism
# Fitting 38 observations of 38
# Arc: 39.01d
# First observation: 2019/10/23
# Last observation: 2019/12/01
Preliminary a, adot, b, bdot, g, gdot:
-0.000000 0.029887 -0.000001 0.010054 0.027749 0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit: 22.19 DOF: 71 RMS: 0.14
# Min/Max residuals: -0.33 0.49
# Exact a, adot, b, bdot, g, gdot:
1.629207E-05 2.699772E-02 5.130990E-06 9.951757E-03 2.721016E-02 7.109126E-03
# Covariance matrix:
2.4125E-13 3.0239E-11 -4.0128E-15 2.0590E-12 8.1772E-12 -6.2052E-10
3.0239E-11 7.5468E-08 1.9356E-12 2.5966E-09 1.3868E-08 -4.0568E-06
-4.0128E-15 1.9356E-12 9.4939E-14 -1.0547E-12 2.6852E-13 -1.4245E-10
2.0590E-12 2.5966E-09 -1.0547E-12 1.1782E-10 4.9505E-10 -1.3180E-07
8.1772E-12 1.3868E-08 2.6852E-13 4.9505E-10 2.5929E-09 -7.2640E-07
-6.2052E-10 -4.0568E-06 -1.4245E-10 -1.3180E-07 -7.2640E-07 2.2661E-04
# lat0 lon0 xBary yBary zBary JD0
2.945267 -7.309297 -0.599750 0.040855 -0.794161 2458779.733531
# Heliocentric elements and errors
Epoch: 2458770.5000 = 2019/10/14
Mean Anomaly: 48.02969 +/- 23.833
Argument of Peri: 289.81845 +/- 27.985
Long of Asc Node: 345.83743 +/- 0.149
Inclination: 20.45203 +/- 0.363
Eccentricity: 0.28612494 +/- 0.5344
Semi-Major Axis: 43.24460487 +/- 13.2817
Time of Perihelion: 2444912.4028 +/- 2554.8
Perihelion: 30.87124491 +/- 24.9797
Aphelion: 55.61796483 +/- 28.7381
Period (y) 284.3846 +/- 131.01
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X 37.27251452 +/- 0.0681
Ecliptic Y -4.18273931 +/- 0.0087
Ecliptic Z 1.88852343 +/- 0.0035
Ecliptic XDOT 0.00101162 +/- 0.0015
Ecliptic YDOT 0.00261128 +/- 0.0002
Ecliptic ZDOT 0.00103653 +/- 0.0001
# Distances at JD0 (AU)
Heliocenter to KBO 37.55399003 +/- 0.0676
Geocenter to KBO 36.75098048 +/- 0.0688
# Hcoef: 9.01
The following table shows the complete astrometric record for 19VE51. 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 (19VE51) followed by the observatory code and reference code for the source of the astrometry.
2019 10 23.23273 23 28 30.00 -00 11 41.0 23.8z 19VE51 T09 C~7xXI 2019 10 23.24670 23 28 29.97 -00 11 41.5 24.4z 19VE51 T09 C~7xXI 2019 10 23.25018 23 28 29.94 -00 11 41.3 24.5z 19VE51 T09 C~7xXI 2019 10 23.26073 23 28 29.90 -00 11 41.7 23.9z 19VE51 T09 C~7xXI 2019 10 23.26421 23 28 29.89 -00 11 41.8 24.0z 19VE51 T09 C~7xXI 2019 10 27.23054 23 28 15.14 -00 13 06.1 24.9r 19VE51 T09 C~7xXI 2019 10 27.23299 23 28 15.14 -00 13 06.3 25.0r 19VE51 T09 C~7xXI 2019 10 27.24037 23 28 15.11 -00 13 06.3 25.2r 19VE51 T09 C~7xXI 2019 10 27.24280 23 28 15.11 -00 13 06.5 24.5r 19VE51 T09 C~7xXI 2019 10 27.24524 23 28 15.08 -00 13 06.5 25.0r 19VE51 T09 C~7xXI 2019 10 27.24768 23 28 15.08 -00 13 06.5 24.8r 19VE51 T09 C~7xXI 2019 11 01.29245 23 27 57.98 -00 14 44.7 25.1g 19VE51 T09 C~7xXI 2019 11 01.38109 23 27 57.68 -00 14 46.8 25.0g 19VE51 T09 C~7xXI 2019 11 01.45822 23 27 57.42 -00 14 48.1 24.4g 19VE51 T09 C~7xXI 2019 11 01.46066 23 27 57.42 -00 14 48.4 25.1g 19VE51 T09 C~7xXI 2019 11 02.21016 23 27 55.07 -00 15 01.7 24.5i 19VE51 T09 C~7xXI 2019 11 02.22066 23 27 55.04 -00 15 01.9 24.5i 19VE51 T09 C~7xXI 2019 11 02.22416 23 27 55.01 -00 15 02.0 24.4i 19VE51 T09 C~7xXI 2019 11 02.23475 23 27 54.98 -00 15 02.0 24.6i 19VE51 T09 C~7xXI 2019 11 02.23823 23 27 54.97 -00 15 02.2 24.5i 19VE51 T09 C~7xXI 2019 11 02.24883 23 27 54.94 -00 15 02.5 24.7i 19VE51 T09 C~7xXI 2019 11 02.25232 23 27 54.92 -00 15 02.5 24.5i 19VE51 T09 C~7xXI 2019 11 28.20491 23 27 03.32 -00 19 59.0 25.5g 19VE51 T09 C~7xXI 2019 11 28.20735 23 27 03.31 -00 19 59.1 25.2g 19VE51 T09 C~7xXI 2019 11 28.29279 23 27 03.24 -00 19 59.3 25.7g 19VE51 T09 C~7xXI 2019 11 28.29526 23 27 03.23 -00 19 59.5 25.6g 19VE51 T09 C~7xXI 2019 11 28.37006 23 27 03.16 -00 20 00.0 26.3g 19VE51 T09 C~7xXI 2019 11 28.37254 23 27 03.20 -00 19 59.5 25.7g 19VE51 T09 C~7xXI 2019 11 29.20334 23 27 02.59 -00 20 02.7 25.2r 19VE51 T09 C~7xXI 2019 11 29.20579 23 27 02.60 -00 20 02.9 24.8r 19VE51 T09 C~7xXI 2019 11 29.21333 23 27 02.58 -00 20 02.9 25.4r 19VE51 T09 C~7xXI 2019 11 29.21579 23 27 02.60 -00 20 02.7 25.3r 19VE51 T09 C~7xXI 2019 11 29.22334 23 27 02.58 -00 20 02.9 24.8r 19VE51 T09 C~7xXI 2019 11 29.24183 23 27 02.57 -00 20 03.0 24.5r 19VE51 T09 C~7xXI 2019 12 01.21144 23 27 01.47 -00 20 08.6 24.4i 19VE51 T09 C~7xXI 2019 12 01.21493 23 27 01.47 -00 20 08.6 24.4i 19VE51 T09 C~7xXI 2019 12 01.22561 23 27 01.49 -00 20 08.4 24.6i 19VE51 T09 C~7xXI 2019 12 01.23967 23 27 01.47 -00 20 08.4 24.5i 19VE51 T09 C~7xXI
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 -0.12 0.00 0.13
2 0.0000 -0.61 0.14 -0.28 -0.19
3 0.0000 -0.95 0.03 0.08 0.16
4 0.0001 -1.65 -0.02 -0.05 -0.00
5 0.0001 -1.83 0.02 -0.08 -0.05
6 0.0109 -238.39 -0.05 9.75 0.09
7 0.0110 -238.47 0.01 9.56 -0.10
8 0.0110 -238.88 0.03 9.74 0.05
9 0.0110 -238.96 0.10 9.56 -0.14
10 0.0110 -239.38 -0.17 9.73 0.03
11 0.0110 -239.38 -0.03 9.73 0.03
12 0.0248 -513.81 0.34 20.70 0.17
13 0.0250 -518.78 0.04 20.55 -0.21
14 0.0253 -522.87 -0.03 20.89 -0.05
15 0.0253 -522.99 -0.02 20.61 -0.33
16 0.0273 -560.63 0.07 22.30 0.02
17 0.0273 -561.12 0.11 22.29 -0.01
18 0.0274 -561.57 -0.16 22.38 0.07
19 0.0274 -561.99 -0.03 22.56 0.22
20 0.0274 -562.20 -0.07 22.43 0.08
21 0.0274 -562.74 -0.05 22.33 -0.04
22 0.0274 -563.01 -0.15 22.45 0.07
23 0.0985 -1391.22 0.15 55.37 -0.00
24 0.0985 -1391.39 0.00 55.33 -0.04
25 0.0987 -1392.44 0.09 55.56 0.08
26 0.0987 -1392.65 -0.09 55.44 -0.05
27 0.0989 -1393.82 -0.29 55.39 -0.18
28 0.0989 -1393.07 0.49 55.62 0.04
29 0.1012 -1402.74 -0.12 56.29 0.17
30 0.1012 -1402.68 -0.04 56.04 -0.08
31 0.1012 -1402.95 -0.22 56.16 0.03
32 0.1013 -1402.60 0.16 56.23 0.09
33 0.1013 -1402.95 -0.11 56.16 0.02
34 0.1013 -1403.13 -0.07 56.13 -0.04
35 0.1067 -1420.50 -0.19 57.49 -0.06
36 0.1067 -1420.50 -0.16 57.49 -0.06
37 0.1068 -1420.15 0.28 57.56 -0.01
38 0.1068 -1420.42 0.13 57.68 0.09
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.
19VE51 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