Orbit Fit and Astrometric record for 19QD111

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: 19QD111   
# Created Tue Apr  1 01:11:15 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.10y
# First observation: 2019/08/30
#  Last observation: 2021/10/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000004   0.020319   0.000000   0.000602   0.022474   0.000000
# Chi-squared of fit:     2.35 DOF:     10 RMS:  0.10
# Min/Max residuals:    -0.17    0.19
# Exact a, adot, b, bdot, g, gdot:
  1.414498E-05  2.030478E-02  9.863459E-07  6.026836E-04  2.244452E-02 -4.069641E-04
# Covariance matrix:
  7.3954E-13  6.0326E-13 -3.1097E-15  1.8688E-14  1.6402E-12  1.6287E-11
  6.0326E-13  4.4558E-12 -1.8484E-14  1.3921E-13  5.0366E-12  1.1472E-10
 -3.1097E-15 -1.8484E-14  3.5384E-13 -2.0577E-13 -2.0835E-14 -5.1488E-13
  1.8688E-14  1.3921E-13 -2.0577E-13  2.5239E-13  1.4310E-13  3.9959E-12
  1.6402E-12  5.0366E-12 -2.0835E-14  1.4310E-13  7.9913E-12  1.2052E-10
  1.6287E-11  1.1472E-10 -5.1488E-13  3.9959E-12  1.2052E-10  3.2709E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.206062   -7.692711    0.271444   -0.037216   -0.966253  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          204.17362 +/-     2.454
Argument of Peri:      106.39681 +/-     2.446
Long of Asc Node:       43.90624 +/-     0.023
Inclination:             2.74084 +/-     0.001
Eccentricity:         0.05838727 +/-    0.0010
Semi-Major Axis:     43.20140230 +/-    0.0160
Time of Perihelion: 2503614.0215 +/-     706.5
Perihelion:          40.67899035 +/-    0.0440
Aphelion:            45.72381425 +/-    0.0447
Period (y)              283.9586 +/-      0.16
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           45.04538282 +/-    0.0056
Ecliptic Y           -6.36504080 +/-    0.0008
Ecliptic Z           -1.71500985 +/-    0.0002
Ecliptic XDOT         0.00029366 +/-    0.0000
Ecliptic YDOT         0.00246139 +/-    0.0000
Ecliptic ZDOT         0.00007515 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.52517453 +/-    0.0055
Geocenter to KBO     44.55431469 +/-    0.0056
# Hcoef:  9.01

The following table shows the complete astrometric record for 19QD111. 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 (19QD111) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 35 14.277  -05 04 43.35  25.5r 19QD111   W84  C~7XLi      
2019 08  30.387214 23 35 13.561  -05 04 47.64  25.5r 19QD111   W84  C~7XLi      
2019 09  28.012277 23 33 15.647  -05 17 17.11  25.5r 19QD111   W84  C~7XLi      
2019 09  28.177548 23 33 14.956  -05 17 21.58  25.5r 19QD111   W84  C~7XLi      
2020 10  18.012125 23 36 10.987  -04 55 38.94  25.5r 19QD111   W84  C~7XLi      
2020 10  18.176134 23 36 10.426  -04 55 42.24  25.5r 19QD111   W84  C~7XLi      
2021 10  06.002765 23 41 11.034  -04 21 26.74  25.5r 19QD111   W84  C~7XLi      
2021 10  06.167954 23 41 10.380  -04 21 30.62  25.5r 19QD111   W84  C~7XLi      

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     0.03       0.00    -0.12
     2   0.0005    -11.52    -0.03       0.29     0.19
     3   0.0788  -1925.85     0.11       8.37     0.09
     4   0.0793  -1937.10    -0.11       8.34    -0.17
     5   1.1357    993.71    -0.11     164.42     0.05
     6   1.1361    984.71     0.11     164.71    -0.05
     7   2.1021   5927.31    -0.06     267.59    -0.02
     8   2.1025   5916.79     0.06     267.92     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.

19QD111    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.274    43.314    43.234
ecceobj         0.058     0.059     0.057
incobj          2.738     2.739     2.738
qmin           39.171    39.178    39.171
qmax           47.361    47.484    47.317
amean          43.159    43.198    43.128
amin           42.820    42.857    42.768
amax           43.529    43.556    43.491
emean           0.067     0.069     0.066
emin            0.047     0.049     0.045
emax            0.089     0.090     0.089
imean           1.849     1.846     1.839
imin            0.688     0.706     0.670
imax            2.813     2.791     2.804
excite_mean     0.076     0.077     0.074
fracstop        1.000     1.000     1.000
cjmean          3.085     3.085     3.085

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       162.0     160.6     162.3
kozaiamp        179.9     180.0     180.0