Orbit Fit and Astrometric record for 19CD30

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: 19CD30    
# Created Thu Oct 31 01:10:38 2024
# Orbit generated from Bernstein formalism
# Fitting     20 observations of     20
# Arc:   0.97y
# First observation: 2018/03/18
#  Last observation: 2019/03/08
Preliminary a, adot, b, bdot, g, gdot:
  -0.000055   0.022095  -0.000003   0.006479   0.023868   0.000000
# Chi-squared of fit:    10.45 DOF:     34 RMS:  0.13
# Min/Max residuals:    -0.26    0.40
# Exact a, adot, b, bdot, g, gdot:
  1.405456E-05  2.201713E-02  4.162650E-06  6.485800E-03  2.410329E-02 -1.547854E-04
# Covariance matrix:
  4.8869E-13  1.1475E-12 -2.2320E-14  4.6757E-13  1.1753E-12  7.2648E-11
  1.1475E-12  1.8738E-11 -2.6316E-13  5.1191E-12  8.4531E-12  7.9456E-10
 -2.2320E-14 -2.6316E-13  2.1492E-13 -3.0715E-13 -1.2910E-13 -1.1585E-11
  4.6757E-13  5.1191E-12 -3.0715E-13  1.8614E-12  2.6149E-12  2.2784E-10
  1.1753E-12  8.4531E-12 -1.2910E-13  2.6149E-12  5.5694E-12  4.0610E-10
  7.2648E-11  7.9456E-10 -1.1585E-11  2.2784E-10  4.0610E-10  3.5369E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.809410  175.453636   -0.029881    0.031471   -0.993403  2458195.963881
# Heliocentric elements and errors
Epoch:              2458190.5000  =  2018/03/13
Mean Anomaly:          202.69412 +/-    18.497
Argument of Peri:      164.51494 +/-    18.498
Long of Asc Node:      169.51721 +/-     0.001
Inclination:            16.48096 +/-     0.002
Eccentricity:         0.02292562 +/-    0.0031
Semi-Major Axis:     41.59947329 +/-    0.0102
Time of Perihelion: 2501013.0616 +/-    5035.4
Perihelion:          40.64577974 +/-    0.1279
Aphelion:            42.55316684 +/-    0.1279
Period (y)              268.3119 +/-      0.10
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.33146560 +/-    0.0040
Ecliptic Y            3.32886875 +/-    0.0003
Ecliptic Z            1.31017567 +/-    0.0001
Ecliptic XDOT        -0.00015116 +/-    0.0000
Ecliptic YDOT        -0.00250074 +/-    0.0000
Ecliptic ZDOT         0.00073564 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.48235996 +/-    0.0040
Geocenter to KBO     41.48811115 +/-    0.0041
# Hcoef:  8.30

The following table shows the complete astrometric record for 19CD30. 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 (19CD30) followed by the observatory code and reference code for the source of the astrometry.

2018 03  18.46308  11 46 11.15   +03 28 03.3   24.1i 19CD30    T09  C~83G7      
2018 03  18.50571  11 46 10.95   +03 28 04.6   23.9i 19CD30    T09  C~83G7      
2018 03  18.57871  11 46 10.62   +03 28 07.1   24.0i 19CD30    T09  C~83G7      
2018 04  24.37247  11 43 43.34   +03 45 51.9   23.9z 19CD30    T09  C~83G7      
2018 04  24.40148  11 43 43.24   +03 45 52.2   23.4z 19CD30    T09  C~83G7      
2018 04  24.44523  11 43 43.08   +03 45 53.0   23.9z 19CD30    T09  C~83G7      
2018 04  24.44791  11 43 43.08   +03 45 53.4   24.0z 19CD30    T09  C~83G7      
2018 04  24.48803  11 43 42.94   +03 45 54.0   24.1z 19CD30    T09  C~83G7      
2019 02  04.56598  11 54 10.23   +02 56 50.5   25.9g 19CD30    T09  C~83G7      
2019 02  04.58875  11 54 10.16   +02 56 51.2   25.3g 19CD30    T09  C~83G7      
2019 02  04.63313  11 54 10.03   +02 56 52.2   25.3g 19CD30    T09  C~83G7      
2019 02  04.66250  11 54 09.95   +02 56 52.8   25.6g 19CD30    T09  C~83G7      
2019 03  07.56739  11 52 13.96   +03 12 17.4   24.8y 19CD30    T09  C~83G7      
2019 03  07.60751  11 52 13.79   +03 12 18.7   25.2y 19CD30    T09  C~83G7      
2019 03  07.62089  11 52 13.72   +03 12 19.1   25.4y 19CD30    T09  C~83G7      
2019 03  08.35114  11 52 10.61   +03 12 43.1   24.3r 19CD30    T09  C~83G7      
2019 03  08.36022  11 52 10.58   +03 12 43.4   24.3r 19CD30    T09  C~83G7      
2019 03  08.37278  11 52 10.52   +03 12 43.9   24.0r 19CD30    T09  C~83G7      
2019 03  08.40431  11 52 10.39   +03 12 44.9   24.4r 19CD30    T09  C~83G7      
2019 03  08.43604  11 52 10.24   +03 12 45.9   24.3r 19CD30    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     0.08       0.00     0.02
     2   0.0001     -3.26    -0.01       0.00    -0.11
     3   0.0003     -8.79    -0.10       0.33    -0.01
     4   0.1011  -2455.23    -0.01     102.47     0.40
     5   0.1011  -2456.73     0.09     102.16     0.04
     6   0.1013  -2459.24    -0.02     101.94    -0.24
     7   0.1013  -2459.40    -0.03     102.31     0.12
     8   0.1014  -2461.56     0.00     102.03    -0.23
     9   0.8846   7330.48    -0.05    1139.40     0.06
    10   0.8847   7329.24    -0.11    1139.62     0.16
    11   0.8848   7327.05     0.01    1139.76     0.07
    12   0.8849   7325.71     0.20    1139.83    -0.01
    13   0.9695   5361.88    -0.10    1294.66    -0.18
    14   0.9696   5359.02    -0.03    1294.84    -0.16
    15   0.9696   5357.90    -0.18    1294.79    -0.26
    16   0.9716   5305.58    -0.02    1298.23    -0.00
    17   0.9717   5305.05     0.12    1298.32     0.06
    18   0.9717   5304.02     0.01    1298.42     0.11
    19   0.9718   5301.84     0.14    1298.56     0.13
    20   0.9719   5299.38     0.01    1298.58     0.04

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.

19CD30    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        41.356    41.419    41.315
ecceobj         0.028     0.029     0.035
incobj         16.544    16.544    16.545
qmin           39.668    39.662    39.431
qmax           43.440    43.630    43.633
amean          41.485    41.546    41.447
amin           41.184    41.235    41.137
amax           41.800    41.870    41.759
emean           0.027     0.029     0.032
emin            0.015     0.017     0.020
emax            0.040     0.042     0.045
imean          16.298    16.291    16.310
imin           15.679    15.681    15.678
imax           16.979    16.964    17.003
excite_mean     0.282     0.282     0.283
fracstop        1.000     1.000     1.000
cjmean          2.978     2.979     2.978

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       187.5     185.9     186.3
kozaiamp        180.0     180.0     179.9