Orbit Fit and Astrometric record for 19QM111

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: 19QM111   
# 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:
   0.000018   0.019611  -0.000000   0.000203   0.021904   0.000000
# Chi-squared of fit:    21.91 DOF:     10 RMS:  0.29
# Min/Max residuals:    -0.68    0.68
# Exact a, adot, b, bdot, g, gdot:
  1.390945E-05  1.953402E-02 -7.786401E-08  2.027586E-04  2.180887E-02 -1.825936E-03
# Covariance matrix:
  7.4125E-13  1.5081E-12 -3.3727E-16  2.0227E-14  1.8356E-12  4.7686E-11
  1.5081E-12  1.5251E-11 -5.0607E-15  1.8804E-13  9.9634E-12  4.4021E-10
 -3.3727E-16 -5.0607E-15  3.8122E-13 -1.8796E-13 -2.3648E-15 -1.5033E-13
  2.0227E-14  1.8804E-13 -1.8796E-13  1.8026E-13  1.2036E-13  5.5018E-12
  1.8356E-12  9.9634E-12 -2.3648E-15  1.2036E-13  9.6035E-12  2.8319E-10
  4.7686E-11  4.4021E-10 -1.5033E-13  5.5018E-12  2.8319E-10  1.2876E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.724855   -7.523198    0.274303   -0.045925   -0.965070  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          253.08736 +/-     1.481
Argument of Peri:       40.15950 +/-     1.370
Long of Asc Node:       69.70819 +/-     0.026
Inclination:             2.73229 +/-     0.000
Eccentricity:         0.10331725 +/-    0.0050
Semi-Major Axis:     45.05110676 +/-    0.0480
Time of Perihelion: 2491521.2043 +/-     451.3
Perihelion:          40.39655012 +/-    0.2274
Aphelion:            49.70566340 +/-    0.2295
Period (y)              302.3893 +/-      0.48
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           46.33156367 +/-    0.0064
Ecliptic Y           -6.40202952 +/-    0.0009
Ecliptic Z           -2.17984029 +/-    0.0003
Ecliptic XDOT         0.00010374 +/-    0.0000
Ecliptic YDOT         0.00246156 +/-    0.0000
Ecliptic ZDOT         0.00003610 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.82255309 +/-    0.0064
Geocenter to KBO     45.85289803 +/-    0.0065
# Hcoef:  8.94

The following table shows the complete astrometric record for 19QM111. 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 (19QM111) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 36 41.271  -05 29 16.95  25.6r 19QM111   W84  C~7XLj      
2019 08  30.387214 23 36 40.588  -05 29 21.71  25.6r 19QM111   W84  C~7XLj      
2019 09  28.012277 23 34 45.959  -05 41 37.57  25.6r 19QM111   W84  C~7XLj      
2019 09  28.177548 23 34 45.217  -05 41 42.44  25.6r 19QM111   W84  C~7XLj      
2021 09  09.073508 23 44 16.328  -04 38 45.20  25.4r 19QM111   W84  C~7XLj      
2021 09  09.192572 23 44 15.857  -04 38 49.10  25.4r 19QM111   W84  C~7XLj      
2021 10  06.002765 23 42 28.269  -04 50 09.46  25.5r 19QM111   W84  C~7XLj      
2021 10  06.167954 23 42 27.609  -04 50 13.33  25.5r 19QM111   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     0.05       0.00     0.05
     2   0.0005    -11.25    -0.06      -0.33    -0.21
     3   0.0788  -1874.06     0.68       1.20     0.24
     4   0.0793  -1886.16    -0.68       1.11    -0.07
     5   2.0284   7447.24     0.06      78.94     0.37
     6   2.0287   7439.22    -0.06      78.17    -0.41
     7   2.1021   5691.24     0.10      95.17    -0.03
     8   2.1025   5680.64    -0.10      95.55     0.06

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.

19QM111    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        45.170    45.287    45.070
ecceobj         0.106     0.119     0.094
incobj          2.733     2.733     2.733
qmin           39.079    38.276    39.589
qmax           51.234    52.420    50.592
amean          45.027    45.136    44.930
amin           44.654    44.714    44.572
amax           45.424    45.570    45.331
emean           0.113     0.130     0.100
emin            0.098     0.111     0.086
emax            0.129     0.150     0.116
imean           1.480     1.523     1.448
imin            0.677     0.638     0.703
imax            2.142     2.234     2.034
excite_mean     0.117     0.133     0.104
fracstop        1.000     1.000     1.000
cjmean          3.097     3.094     3.100

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       165.4     180.5     169.4
kozaiamp        180.0     180.0     180.0