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: 19CC30
# Created Sun Apr 27 01:11:11 2025
# Orbit generated from Bernstein formalism
# Fitting 18 observations of 19
# Arc: 2.14y
# First observation: 2018/03/18
# Last observation: 2019/03/03
Preliminary a, adot, b, bdot, g, gdot:
-0.000356 0.023303 -0.000003 0.001072 0.023730 0.000000
# Chi-squared of fit: 8.04 DOF: 30 RMS: 0.12
# Min/Max residuals: -0.29 0.30
# Exact a, adot, b, bdot, g, gdot:
-1.485905E-07 2.289525E-02 -6.302894E-06 1.058581E-03 2.359691E-02 1.740485E-05
# Covariance matrix:
4.9340E-11 -9.5031E-11 5.8472E-12 -6.5492E-12 -5.6985E-11 -1.5789E-09
-9.5031E-11 2.0260E-10 -1.2912E-11 1.4327E-11 1.2927E-10 3.4527E-09
5.8472E-12 -1.2912E-11 2.0887E-12 -1.6240E-12 -8.3997E-12 -2.2188E-10
-6.5492E-12 1.4327E-11 -1.6240E-12 1.4399E-12 9.2700E-12 2.4571E-10
-5.6985E-11 1.2927E-10 -8.3997E-12 9.2700E-12 8.5366E-11 2.2336E-09
-1.5789E-09 3.4527E-09 -2.2188E-10 2.4571E-10 2.2336E-09 5.9211E-08
# lat0 lon0 xBary yBary zBary JD0
2.836270 177.384447 0.904802 0.019597 -0.391311 2457764.840053
# Heliocentric elements and errors
Epoch: 2457760.5000 = 2017/01/07
Mean Anomaly: 323.28574 +/- 13.195
Argument of Peri: 85.31207 +/- 14.405
Long of Asc Node: 130.10200 +/- 0.019
Inclination: 3.89722 +/- 0.001
Eccentricity: 0.03484184 +/- 0.0064
Semi-Major Axis: 43.99142628 +/- 0.0184
Time of Perihelion: 2468629.3287 +/- 3906.2
Perihelion: 42.45868396 +/- 0.2840
Aphelion: 45.52416859 +/- 0.2841
Period (y) 291.7832 +/- 0.18
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X -42.63589515 +/- 0.0166
Ecliptic Y 2.84927461 +/- 0.0005
Ecliptic Z 2.09664955 +/- 0.0009
Ecliptic XDOT -0.00011446 +/- 0.0000
Ecliptic YDOT -0.00266057 +/- 0.0000
Ecliptic ZDOT 0.00012272 +/- 0.0000
# Distances at JD0 (AU)
Heliocenter to KBO 42.78240129 +/- 0.0165
Geocenter to KBO 42.37842937 +/- 0.0166
# Hcoef: 7.59
The following table shows the complete astrometric record for 19CC30. 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 (19CC30) followed by the observatory code and reference code for the source of the astrometry.
2017 01 11.339252 11 54 54.989 +03 38 32.60 22.0z 19CC30 W84 C~8HR5 2018 03 18.46982 11 56 19.50 +03 36 46.6 23.7i 19CC30 T09 C~83G7 2018 03 18.51105 11 56 19.31 +03 36 47.7 23.8i 19CC30 T09 C~83G7 2018 03 18.58405 11 56 19.00 +03 36 49.9 23.8i 19CC30 T09 C~83G7 2018 04 12.121738 11 54 34.248 +03 48 04.07 23.6V 19CC30 W84 C~8HR5 2018 04 13.119460 11 54 30.310 +03 48 28.33 24.4V 19CC30 W84 C~8HR5 2018 04 24.40683 11 53 48.60 +03 52 39.7 23.3z 19CC30 T09 C~83G7 2018 04 24.45059 11 53 48.46 +03 52 40.4 23.8z 19CC30 T09 C~83G7 2018 04 24.45326 11 53 48.44 +03 52 40.7 23.9z 19CC30 T09 C~83G7 2018 04 24.50141 11 53 48.29 +03 52 41.6 23.3z 19CC30 T09 C~83G7 2019 02 05.54825 12 03 57.79 +02 49 20.4 23.9i 19CC30 T09 C~83G7 2019 02 05.59538 12 03 57.66 +02 49 21.3 23.9i 19CC30 T09 C~83G7 2019 02 05.62229 12 03 57.59 +02 49 21.8 23.7i 19CC30 T09 C~83G7 2019 02 05.66253 12 03 57.46 +02 49 22.6 23.7i 19CC30 T09 C~83G7 2019 03 03.51493 12 02 24.79 +03 00 46.2 23.9z 19CC30 T09 C~83G7 2019 03 03.52297 12 02 24.77 +03 00 46.4 23.8z 19CC30 T09 C~83G7 2019 03 03.57682 12 02 24.54 +03 00 48.1 23.9z 19CC30 T09 C~83G7 2019 03 03.57949 12 02 24.54 +03 00 48.3 24.1z 19CC30 T09 C~83G7 2019 03 03.61704 12 02 24.38 +03 00 49.1 23.9z 19CC30 T09 C~83G7
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 ( 3.20) 0.00 ( 1.45)
2 1.1804 1202.66 -0.06 406.74 0.01
3 1.1805 1199.61 -0.08 406.61 -0.12
4 1.1807 1194.48 0.12 406.78 0.03
5 1.2479 -512.31 -0.04 400.63 -0.00
6 1.2506 -576.04 0.14 399.42 -0.04
7 1.2815 -1248.77 -0.15 381.60 0.02
8 1.2816 -1250.97 0.10 381.41 -0.07
9 1.2816 -1251.36 -0.15 381.57 0.10
10 1.2818 -1253.78 0.11 381.50 0.14
11 2.0676 8636.74 -0.21 538.94 0.02
12 2.0678 8634.59 -0.02 538.98 -0.08
13 2.0679 8633.43 0.15 539.02 -0.12
14 2.0680 8631.32 0.04 538.97 -0.29
15 2.1387 7083.27 -0.16 610.07 -0.04
16 2.1388 7082.92 0.04 610.14 0.01
17 2.1389 7079.07 -0.05 610.32 0.12
18 2.1389 7078.99 0.06 610.50 0.30
19 2.1390 7076.47 0.14 610.28 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.
19CC30 quality flag:3 Type: CLASSICAL CLASSICAL CLASSICAL axisobj 43.591 43.680 43.544 ecceobj 0.026 0.023 0.037 incobj 3.904 3.905 3.903 qmin 41.936 41.851 41.317 qmax 45.749 46.014 46.333 amean 43.760 43.842 43.726 amin 43.420 43.496 43.375 amax 44.104 44.185 44.080 emean 0.023 0.026 0.040 emin 0.006 0.010 0.026 emax 0.038 0.042 0.052 imean 2.861 2.851 2.927 imin 2.184 2.189 2.162 imax 3.542 3.521 3.704 excite_mean 0.055 0.056 0.065 fracstop 1.000 1.000 1.000 cjmean 3.095 3.096 3.093 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 180.4 180.3 185.4 kozaiamp 180.0 180.0 179.9