Orbit Fit and Astrometric record for 19QC110

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: 19QC110   
# 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:
   0.000010   0.020911  -0.000000  -0.000029   0.022439   0.000000
# Chi-squared of fit:     0.43 DOF:     10 RMS:  0.04
# Min/Max residuals:    -0.07    0.07
# Exact a, adot, b, bdot, g, gdot:
  1.479504E-05  2.089629E-02 -1.098137E-07 -2.852036E-05  2.239281E-02  1.092846E-04
# Covariance matrix:
  7.4073E-13  1.4462E-12  1.9416E-16 -2.6800E-15  1.6863E-12  4.3287E-11
  1.4462E-12  1.5415E-11  1.4748E-15 -2.6222E-14  9.1803E-12  4.1601E-10
  1.9416E-16  1.4748E-15  3.8281E-13 -1.8917E-13  1.0264E-15  4.0001E-14
 -2.6800E-15 -2.6222E-14 -1.8917E-13  1.7954E-13 -1.5283E-14 -7.1699E-13
  1.6863E-12  9.1803E-12  1.0264E-15 -1.5283E-14  8.2249E-12  2.4541E-10
  4.3287E-11  4.1601E-10  4.0001E-14 -7.1699E-13  2.4541E-10  1.1369E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.581097   -7.873987    0.301152   -0.009717   -0.958369  2458723.711696
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:           12.48179 +/-    35.369
Argument of Peri:      248.78682 +/-    35.960
Long of Asc Node:       90.26257 +/-     0.115
Inclination:             0.57518 +/-     0.000
Eccentricity:         0.00793890 +/-    0.0013
Semi-Major Axis:     45.97657769 +/-    0.0139
Time of Perihelion: 2454772.4953 +/-   11187.4
Perihelion:          45.61157413 +/-    0.0605
Aphelion:            46.34158124 +/-    0.0605
Period (y)              311.7548 +/-      0.14
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           45.14483217 +/-    0.0057
Ecliptic Y           -6.55404748 +/-    0.0008
Ecliptic Z           -0.45291067 +/-    0.0001
Ecliptic XDOT         0.00037167 +/-    0.0000
Ecliptic YDOT         0.00252953 +/-    0.0000
Ecliptic ZDOT        -0.00000385 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.62035223 +/-    0.0056
Geocenter to KBO     44.65719382 +/-    0.0057
# Hcoef:  7.79

The following table shows the complete astrometric record for 19QC110. 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 (19QC110) followed by the observatory code and reference code for the source of the astrometry.

2019 08  28.210895 23 31 59.604  -03 39 27.73  24.3r 19QC110   W84  C~7XLh      
2019 08  28.388381 23 31 58.904  -03 39 32.22  24.3r 19QC110   W84  C~7XLh      
2019 09  29.013696 23 29 50.440  -03 53 19.09  24.3r 19QC110   W84  C~7XLh      
2019 09  29.177510 23 29 49.779  -03 53 23.15  24.3r 19QC110   W84  C~7XLh      
2021 09  06.108763 23 40 12.623  -02 46 40.85  24.2r 19QC110   W84  C~7XLh      
2021 09  06.196686 23 40 12.254  -02 46 43.16  24.2r 19QC110   W84  C~7XLh      
2021 10  04.002582 23 38 19.143  -02 58 52.97  24.3r 19QC110   W84  C~7XLh      
2021 10  04.175328 23 38 18.447  -02 58 57.33  24.3r 19QC110   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    -0.01       0.00     0.02
     2   0.0005    -11.40     0.01       0.01     0.00
     3   0.0871  -2104.51    -0.04      -1.15    -0.05
     4   0.0875  -2115.20     0.04      -0.98     0.03
     5   2.0257   8038.10     0.06     -14.13    -0.04
     6   2.0260   8032.10    -0.06     -14.06     0.01
     7   2.1021   6184.90     0.07     -12.19     0.00
     8   2.1026   6173.59    -0.07     -12.06     0.03

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.

19QC110    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        46.049    46.107    45.998
ecceobj         0.010     0.013     0.013
incobj          0.574     0.574     0.574
qmin           44.790    44.795    44.445
qmax           47.215    47.293    47.435
amean          45.910    45.969    45.858
amin           45.555    45.611    45.499
amax           46.267    46.332    46.217
emean           0.009     0.009     0.015
emin            0.000     0.000     0.001
emax            0.020     0.021     0.026
imean           1.115     1.116     1.114
imin            0.718     0.734     0.706
imax            1.438     1.434     1.445
excite_mean     0.022     0.022     0.025
fracstop        1.000     1.000     1.000
cjmean          3.125     3.125     3.124

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       201.9     184.7     212.7
kozaiamp        179.9     179.9     179.9