Orbit Fit and Astrometric record for 19QE112

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: 19QE112   
# Created Sat May  4 01:18:26 2024
# Orbit generated from Bernstein formalism
# Fitting     22 observations of     22
# Arc:   2.98y
# First observation: 2019/08/30
#  Last observation: 2022/08/24
Preliminary a, adot, b, bdot, g, gdot:
  -0.000007   0.021475   0.000000   0.001194   0.022868   0.000000
# Chi-squared of fit:     3.16 DOF:     38 RMS:  0.07
# Min/Max residuals:    -0.21    0.14
# Exact a, adot, b, bdot, g, gdot:
  1.490454E-05  2.154196E-02  8.877744E-07  1.198808E-03  2.294472E-02  1.392202E-03
# Covariance matrix:
  5.7525E-13  6.7448E-14 -7.2204E-15  1.7013E-14  8.2583E-13  4.3830E-12
  6.7448E-14  1.1399E-12 -2.8295E-14  7.2065E-14  1.5454E-12  1.8626E-11
 -7.2204E-15 -2.8295E-14  2.6653E-13 -1.0415E-13 -4.6013E-14 -4.9937E-13
  1.7013E-14  7.2065E-14 -1.0415E-13  5.7486E-14  1.1435E-13  1.2647E-12
  8.2583E-13  1.5454E-12 -4.6013E-14  1.1435E-13  3.4045E-12  2.9525E-11
  4.3830E-12  1.8626E-11 -4.9937E-13  1.2647E-12  2.9525E-11  3.2680E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.708670   -7.653815    0.272100   -0.028821   -0.966355  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:           82.91092 +/-     0.102
Argument of Peri:      242.20747 +/-     0.155
Long of Asc Node:       19.76545 +/-     0.004
Inclination:             3.58265 +/-     0.001
Eccentricity:         0.06148006 +/-    0.0008
Semi-Major Axis:     44.72454754 +/-    0.0081
Time of Perihelion: 2433559.5749 +/-      30.0
Perihelion:          41.97487989 +/-    0.0378
Aphelion:            47.47421519 +/-    0.0380
Period (y)              299.1074 +/-      0.08
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           44.10030046 +/-    0.0035
Ecliptic Y           -6.20752123 +/-    0.0005
Ecliptic Z           -1.29949914 +/-    0.0001
Ecliptic XDOT         0.00051961 +/-    0.0000
Ecliptic YDOT         0.00252547 +/-    0.0000
Ecliptic ZDOT         0.00013780 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   44.55399554 +/-    0.0034
Geocenter to KBO     43.58302061 +/-    0.0035
# Hcoef:  7.25

The following table shows the complete astrometric record for 19QE112. 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 (19QE112) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 34 35.479  -04 36 23.47  23.3r 19QE112   W84  C~7XLk      
2019 08  30.387214 23 34 34.762  -04 36 27.99  23.3r 19QE112   W84  C~7XLk      
2019 09  28.012277 23 32 34.828  -04 48 59.72  23.2r 19QE112   W84  C~7XLk      
2019 09  28.177548 23 32 34.127  -04 49 03.80  23.2r 19QE112   W84  C~7XLk      
2020 10  18.01513  23 35 41.06   -04 23 56.5   24.1V 19QE112   W84  C~7XLk      
2020 10  18.07030  23 35 40.87   -04 23 57.6         19QE112   W84  C~7XLk      
2020 10  18.09799  23 35 40.77   -04 23 58.1         19QE112   W84  C~7XLk      
2020 10  18.15327  23 35 40.57   -04 23 59.2         19QE112   W84  C~7XLk      
2021 09  09.073508 23 42 45.072  -03 34 37.46  23.1r 19QE112   W84  C~7XLk      
2021 09  09.192572 23 42 44.560  -03 34 40.60  23.1r 19QE112   W84  C~7XLk      
2021 10  06.002765 23 40 52.786  -03 46 16.78  23.6r 19QE112   W84  C~7XLk      
2021 10  06.167954 23 40 52.112  -03 46 20.79  23.6r 19QE112   W84  C~7XLk      
2022 08  24.22448  23 48 13.84   -02 54 34.2   24.3V 19QE112   W84  C~7XLk      
2022 08  24.27272  23 48 13.64   -02 54 35.5   24.1V 19QE112   W84  C~7XLk      
2022 08  24.29691  23 48 13.56   -02 54 35.9   24.5V 19QE112   W84  C~7XLk      
2022 08  24.30727  23 48 13.53   -02 54 36.3   24.0V 19QE112   W84  C~7XLk      
2022 08  24.32105  23 48 13.47   -02 54 36.7   24.2V 19QE112   W84  C~7XLk      
2022 08  24.33136  23 48 13.43   -02 54 36.9   24.1V 19QE112   W84  C~7XLk      
2022 08  24.34509  23 48 13.38   -02 54 37.2   23.8V 19QE112   W84  C~7XLk      
2022 08  24.37953  23 48 13.25   -02 54 37.9   23.7V 19QE112   W84  C~7XLk      
2022 08  24.39332  23 48 13.20   -02 54 38.4   23.9V 19QE112   W84  C~7XLk      
2022 08  24.40369  23 48 13.15   -02 54 38.5   23.9V 19QE112   W84  C~7XLk      

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    -0.01       0.00    -0.01
     2   0.0005    -11.63    -0.01       0.09    -0.01
     3   0.0788  -1955.75     0.04      18.08    -0.10
     4   0.0793  -1966.99    -0.00      18.47     0.03
     5   1.1357   1196.22    -0.08     297.97     0.02
     6   1.1358   1193.18     0.02     298.09     0.01
     7   1.1359   1191.60     0.03     298.22     0.08
     8   1.1360   1188.42    -0.00     298.39     0.12
     9   2.0284   8198.56     0.06     496.09    -0.09
    10   2.0287   8190.26    -0.04     496.26    -0.02
    11   2.1021   6375.96     0.04     522.66    -0.05
    12   2.1025   6365.10    -0.03     522.99    -0.03
    13   2.9843  13687.79     0.08     739.09     0.02
    14   2.9844  13684.51    -0.21     739.10     0.00
    15   2.9845  13683.24     0.03     739.21     0.11
    16   2.9845  13682.67     0.10     739.02    -0.08
    17   2.9846  13681.68    -0.04     739.01    -0.10
    18   2.9846  13681.05    -0.03     739.07    -0.05
    19   2.9846  13680.24     0.01     739.09    -0.03
    20   2.9847  13678.16     0.07     739.23     0.10
    21   2.9848  13677.27     0.03     739.07    -0.07
    22   2.9848  13676.54    -0.06     739.27     0.14

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.

19QE112    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.762    44.786    44.739
ecceobj         0.057     0.057     0.058
incobj          3.578     3.578     3.578
qmin           41.470    41.554    41.480
qmax           48.004    48.015    47.994
amean          44.646    44.670    44.623
amin           44.296    44.313    44.275
amax           45.014    45.035    44.993
emean           0.053     0.053     0.054
emin            0.039     0.038     0.039
emax            0.067     0.066     0.067
imean           3.504     3.505     3.504
imin            2.922     2.929     2.915
imax            3.961     3.962     3.963
excite_mean     0.081     0.081     0.081
fracstop        1.000     1.000     1.000
cjmean          3.101     3.102     3.101

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       178.9     178.6     178.8
kozaiamp        180.0     180.0     179.9