Orbit Fit and Astrometric record for 19CC30

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 Wed May 21 01:11:15 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     22 observations of     22
# Arc:   8.28y
# First observation: 2017/01/11
#  Last observation: 2025/04/23
# Chi-squared of fit:    40.51 DOF:     38 RMS:  0.24
# Min/Max residuals:    -0.45    0.73
# Exact a, adot, b, bdot, g, gdot:
  1.388097E-05  2.287945E-02 -3.759192E-06  1.056778E-03  2.359184E-02 -1.947133E-04
# Covariance matrix:
  8.4335E-12 -4.6419E-12  3.0643E-13 -2.7499E-13  1.8154E-12 -2.4922E-11
 -4.6419E-12  2.6607E-12 -1.7959E-13  1.5741E-13 -8.7269E-13  1.4265E-11
  3.0643E-13 -1.7959E-13  1.6449E-13 -4.2520E-14  5.2086E-14 -9.6506E-13
 -2.7499E-13  1.5741E-13 -4.2520E-14  2.1410E-14 -5.3025E-14  8.4817E-13
  1.8154E-12 -8.7269E-13  5.2086E-14 -5.3025E-14  6.2885E-13 -4.8071E-12
 -2.4922E-11  1.4265E-11 -9.6506E-13  8.4817E-13 -4.8071E-12  7.6866E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.836270  177.384447    0.904802    0.019597   -0.391311  2457764.840053
# Heliocentric elements and errors
Epoch:              2457764.5000  =  2017/01/11
Mean Anomaly:          312.95726 +/-     0.554
Argument of Peri:       96.74443 +/-     0.614
Long of Asc Node:      130.07545 +/-     0.003
Inclination:             3.89563 +/-     0.000
Eccentricity:         0.04071000 +/-    0.0001
Semi-Major Axis:     43.97065885 +/-    0.0114
Time of Perihelion: 2471681.0957 +/-     167.8
Perihelion:          42.18061342 +/-    0.0126
Aphelion:            45.76070429 +/-    0.0134
Period (y)              291.5766 +/-      0.11
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.64500249 +/-    0.0014
Ecliptic Y            2.84909535 +/-    0.0002
Ecliptic Z            2.09720777 +/-    0.0001
Ecliptic XDOT        -0.00008985 +/-    0.0000
Ecliptic YDOT        -0.00266043 +/-    0.0000
Ecliptic ZDOT         0.00012132 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.79151280 +/-    0.0014
Geocenter to KBO     42.38756294 +/-    0.0014
# Hcoef:  7.58

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      
2025 04  23.267130 12 28 42.383  +00 31 56.71  23.6G 19CC30    G37  C~8swX      
2025 04  23.304790 12 28 42.218  +00 31 57.40        19CC30    G37  C~8swX      
2025 04  23.343130 12 28 42.050  +00 31 58.68        19CC30    G37  C~8swX      

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     0.64       0.00     0.73
     2   1.1804      0.00    -0.38       0.00    -0.00
     3   1.1805      0.00    -0.45       0.00    -0.11
     4   1.1807      0.00    -0.20       0.00    -0.05
     5   1.2479      0.00    -0.15       0.00    -0.09
     6   1.2506      0.00     0.01       0.00    -0.20
     7   1.2815      0.00    -0.13       0.00    -0.06
     8   1.2816      0.00     0.06       0.00    -0.24
     9   1.2816      0.00    -0.10       0.00     0.00
    10   1.2818      0.00     0.16       0.00    -0.06
    11   2.0676      0.00    -0.34       0.00     0.20
    12   2.0678      0.00    -0.20       0.00     0.03
    13   2.0679      0.00    -0.06       0.00    -0.08
    14   2.0680      0.00    -0.23       0.00    -0.19
    15   2.1387      0.00     0.05       0.00    -0.04
    16   2.1388      0.00     0.26       0.00    -0.07
    17   2.1389      0.00     0.22       0.00     0.06
    18   2.1389      0.00     0.39       0.00     0.19
    19   2.1390      0.00     0.36       0.00    -0.10
    20   8.2791      0.00     0.25       0.00     0.04
    21   8.2792      0.00     0.02       0.00    -0.15
    22   8.2793      0.00    -0.22       0.00     0.23

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        43.568    43.568    43.568
ecceobj         0.033     0.033     0.033
incobj          3.902     3.902     3.902
qmin           41.576    41.570    41.575
qmax           46.115    46.119    46.116
amean          43.717    43.717    43.717
amin           43.376    43.376    43.376
amax           44.073    44.073    44.073
emean           0.024     0.024     0.024
emin            0.003     0.003     0.003
emax            0.047     0.047     0.047
imean           2.907     2.907     2.908
imin            2.205     2.205     2.205
imax            3.626     3.622     3.625
excite_mean     0.057     0.057     0.057
fracstop        1.000     1.000     1.000
cjmean          3.094     3.094     3.094

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       177.3     177.1     177.2
kozaiamp        180.0     179.9     179.9