Orbit Fit and Astrometric record for 19QJ110

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: 19QJ110   
# Created Tue Apr  1 01:11:14 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.10y
# First observation: 2019/08/28
#  Last observation: 2021/10/04
Preliminary a, adot, b, bdot, g, gdot:
   0.000017   0.025161  -0.000001  -0.000551   0.024941   0.000000
# Chi-squared of fit:     2.14 DOF:     10 RMS:  0.09
# Min/Max residuals:    -0.16    0.17
# Exact a, adot, b, bdot, g, gdot:
  1.546620E-05  2.510964E-02 -9.320042E-07 -5.494842E-04  2.486081E-02 -5.367369E-04
# Covariance matrix:
  7.4080E-13  1.6669E-12  2.0250E-15 -4.6908E-14  1.7234E-12  4.0350E-11
  1.6669E-12  1.9907E-11  2.1597E-14 -5.1287E-13  1.0828E-11  4.4077E-10
  2.0250E-15  2.1597E-14  3.8286E-13 -1.8973E-13  1.1828E-14  4.8257E-13
 -4.6908E-14 -5.1287E-13 -1.8973E-13  1.9255E-13 -2.7634E-13 -1.1467E-11
  1.7234E-12  1.0828E-11  1.1828E-14 -2.7634E-13  8.6520E-12  2.3763E-10
  4.0350E-11  4.4077E-10  4.8257E-13 -1.1467E-11  2.3763E-10  9.8548E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.829937   -8.203463    0.295635   -0.013904   -0.960033  2458723.711696
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          340.39916 +/-     2.710
Argument of Peri:      235.32065 +/-     3.166
Long of Asc Node:      138.64503 +/-     0.021
Inclination:             1.49882 +/-     0.001
Eccentricity:         0.07135248 +/-    0.0015
Semi-Major Axis:     44.12718586 +/-    0.0152
Time of Perihelion: 2464549.9829 +/-     805.9
Perihelion:          40.97860191 +/-    0.0680
Aphelion:            47.27576981 +/-    0.0685
Period (y)              293.1349 +/-      0.15
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           40.71914394 +/-    0.0047
Ecliptic Y           -6.17550121 +/-    0.0007
Ecliptic Z           -0.58266443 +/-    0.0001
Ecliptic XDOT         0.00034366 +/-    0.0000
Ecliptic YDOT         0.00274608 +/-    0.0000
Ecliptic ZDOT        -0.00005988 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.18889409 +/-    0.0047
Geocenter to KBO     40.22395814 +/-    0.0048
# Hcoef:  9.37

The following table shows the complete astrometric record for 19QJ110. 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 (19QJ110) followed by the observatory code and reference code for the source of the astrometry.

2019 08  28.210895 23 31 10.422  -04 00 58.99  25.5r 19QJ110   W84  C~7XLh      
2019 08  28.388381 23 31 09.648  -04 01 04.25  25.5r 19QJ110   W84  C~7XLh      
2019 09  29.013696 23 28 49.270  -04 16 16.73  25.2r 19QJ110   W84  C~7XLh      
2019 09  29.177510 23 28 48.554  -04 16 21.39  25.2r 19QJ110   W84  C~7XLh      
2021 09  06.108763 23 41 13.398  -03 00 20.14  25.3r 19QJ110   W84  C~7XLh      
2021 09  06.196686 23 41 12.992  -03 00 22.71  25.3r 19QJ110   W84  C~7XLh      
2021 10  04.002582 23 39 09.276  -03 13 48.98  25.6r 19QJ110   W84  C~7XLh      
2021 10  04.175328 23 39 08.505  -03 13 53.93  25.6r 19QJ110   W84  C~7XLh      

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     0.10       0.00     0.12
     2   0.0005    -12.72    -0.10      -0.26    -0.10
     3   0.0871  -2302.61    -0.04     -10.63     0.06
     4   0.0875  -2314.30     0.04     -10.69    -0.07
     5   2.0257   9737.77     0.09    -233.38    -0.04
     6   2.0260   9731.15    -0.09    -233.32     0.02
     7   2.1021   7706.72     0.17    -237.82     0.04
     8   2.1026   7694.14    -0.16    -237.78    -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.

19QJ110    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.194    44.242    44.150
ecceobj         0.075     0.074     0.076
incobj          1.494     1.495     1.494
qmin           39.862    40.015    39.746
qmax           48.490    48.488    48.572
amean          44.066    44.115    44.022
amin           43.721    43.757    43.669
amax           44.443    44.494    44.398
emean           0.076     0.074     0.078
emin            0.060     0.058     0.061
emax            0.092     0.090     0.094
imean           1.630     1.609     1.652
imin            0.824     0.825     0.824
imax            2.292     2.274     2.307
excite_mean     0.081     0.080     0.083
fracstop        1.000     1.000     1.000
cjmean          3.094     3.095     3.093

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       192.1     187.9     193.3
kozaiamp        179.9     180.0     180.0