Orbit Fit and Astrometric record for 19QP111

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: 19QP111   
# Created Tue Apr  1 01:11:15 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.03y
# First observation: 2019/08/30
#  Last observation: 2021/09/09
Preliminary a, adot, b, bdot, g, gdot:
   0.000011   0.022875   0.000000  -0.000444   0.023960   0.000000
# Chi-squared of fit:     3.83 DOF:     10 RMS:  0.12
# Min/Max residuals:    -0.26    0.26
# Exact a, adot, b, bdot, g, gdot:
  1.500286E-05  2.284899E-02 -3.104223E-07 -4.434748E-04  2.389840E-02  3.443106E-05
# Covariance matrix:
  7.3993E-13  7.1805E-13  1.0595E-15 -2.0086E-14  1.6711E-12  2.2283E-11
  7.1805E-13  4.9582E-12  9.3967E-15 -1.0289E-13  5.5622E-12  1.1550E-10
  1.0595E-15  9.3967E-15  3.5746E-13 -2.1407E-13  8.8196E-15  2.3379E-13
 -2.0086E-14 -1.0289E-13 -2.1407E-13  2.6564E-13 -1.2093E-13 -2.5322E-12
  1.6711E-12  5.5622E-12  8.8196E-15 -1.2093E-13  8.2175E-12  1.3499E-10
  2.2283E-11  1.1550E-10  2.3379E-13 -2.5322E-12  1.3499E-10  2.8433E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.973328   -7.998838    0.266274   -0.050226   -0.967103  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          194.14405 +/-    18.391
Argument of Peri:       54.87886 +/-    18.384
Long of Asc Node:      102.81942 +/-     0.022
Inclination:             3.11599 +/-     0.000
Eccentricity:         0.00707494 +/-    0.0005
Semi-Major Axis:     42.52375640 +/-    0.0128
Time of Perihelion: 2505383.6891 +/-    5174.1
Perihelion:          42.22290358 +/-    0.0245
Aphelion:            42.82460922 +/-    0.0246
Period (y)              277.3037 +/-      0.13
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           42.30569688 +/-    0.0050
Ecliptic Y           -6.22027249 +/-    0.0007
Ecliptic Z           -2.17049707 +/-    0.0003
Ecliptic XDOT         0.00037400 +/-    0.0000
Ecliptic YDOT         0.00259256 +/-    0.0000
Ecliptic ZDOT        -0.00005117 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.81559103 +/-    0.0049
Geocenter to KBO     41.84381114 +/-    0.0050
# Hcoef:  8.61

The following table shows the complete astrometric record for 19QP111. 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 (19QP111) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 35 19.801  -05 54 15.68  24.8r 19QP111   W84  C~7XLj      
2019 08  30.387214 23 35 19.057  -05 54 20.61  24.8r 19QP111   W84  C~7XLj      
2019 09  28.012277 23 33 15.014  -06 07 47.25  24.9r 19QP111   W84  C~7XLj      
2019 09  28.177548 23 33 14.290  -06 07 51.51  24.9r 19QP111   W84  C~7XLj      
2020 10  20.004233 23 36 37.449  -05 47 05.73  24.9r 19QP111   W84  C~7XLj      
2020 10  20.172968 23 36 36.817  -05 47 09.04  24.9r 19QP111   W84  C~7XLj      
2021 09  09.073508 23 44 21.366  -04 59 20.18  24.7r 19QP111   W84  C~7XLj      
2021 09  09.192572 23 44 20.817  -04 59 23.97  24.7r 19QP111   W84  C~7XLj      

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     0.02       0.00     0.00
     2   0.0005    -12.15    -0.03      -0.13     0.03
     3   0.0788  -2030.76     0.00      -9.02    -0.10
     4   0.0793  -2042.36    -0.00      -8.66     0.07
     5   1.1411   1234.20     0.16     -64.40    -0.12
     6   1.1416   1224.23    -0.16     -63.70     0.11
     7   2.0284   8735.50     0.26    -193.21     0.09
     8   2.0287   8726.45    -0.26    -193.41    -0.08

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.

19QP111    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        42.578    42.608    42.548
ecceobj         0.007     0.008     0.007
incobj          3.120     3.120     3.120
qmin           40.473    40.463    38.767
qmax           44.652    44.663    46.339
amean          42.470    42.499    42.440
amin           42.148    42.180    42.110
amax           42.800    42.820    42.785
emean           0.021     0.022     0.035
emin            0.000     0.000     0.000
emax            0.043     0.043     0.084
imean           1.685     1.695     1.660
imin            0.495     0.504     0.373
imax            2.889     2.868     2.914
excite_mean     0.037     0.037     0.048
fracstop        1.000     1.000     1.000
cjmean          3.082     3.082     3.080

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       170.0     174.1     176.5
kozaiamp        179.9     180.0     179.9