Orbit Fit and Astrometric record for 19QK110

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: 19QK110   
# Created Wed May  8 01:18:18 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.02y
# First observation: 2019/08/28
#  Last observation: 2021/09/05
Preliminary a, adot, b, bdot, g, gdot:
  -0.000013   0.015605  -0.000000   0.003372   0.019503   0.000000
# Chi-squared of fit:     1.26 DOF:     10 RMS:  0.07
# Min/Max residuals:    -0.13    0.13
# Exact a, adot, b, bdot, g, gdot:
  1.217274E-05  1.566466E-02  2.466636E-06  3.388941E-03  1.957360E-02  2.734081E-03
# Covariance matrix:
  7.3243E-13  4.5207E-13 -1.9397E-14  1.6230E-13  1.4559E-12  2.4745E-11
  4.5207E-13  3.2118E-12 -8.5941E-14  7.2588E-13  3.7525E-12  1.1065E-10
 -1.9397E-14 -8.5941E-14  3.6183E-13 -2.3752E-13 -1.0923E-13 -3.2301E-12
  1.6230E-13  7.2588E-13 -2.3752E-13  4.4674E-13  9.1840E-13  2.7285E-11
  1.4559E-12  3.7525E-12 -1.0923E-13  9.1840E-13  6.4309E-12  1.4001E-10
  2.4745E-11  1.1065E-10 -3.2301E-12  2.7285E-11  1.4001E-10  4.1591E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.141946   -8.394529    0.292432   -0.019151   -0.960923  2458723.711696
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          108.43434 +/-     0.730
Argument of Peri:      227.63460 +/-     0.639
Long of Asc Node:      356.45625 +/-     0.001
Inclination:            12.22496 +/-     0.002
Eccentricity:         0.18728374 +/-    0.0029
Semi-Major Axis:     47.85736529 +/-    0.0461
Time of Perihelion: 2422296.6411 +/-     239.5
Perihelion:          38.89445897 +/-    0.1417
Aphelion:            56.82027162 +/-    0.1472
Period (y)              331.0788 +/-      0.48
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           51.44279441 +/-    0.0065
Ecliptic Y           -7.89355997 +/-    0.0010
Ecliptic Z           -1.01804979 +/-    0.0001
Ecliptic XDOT         0.00071594 +/-    0.0000
Ecliptic YDOT         0.00211098 +/-    0.0000
Ecliptic ZDOT         0.00046609 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   52.05483465 +/-    0.0065
Geocenter to KBO     51.08923360 +/-    0.0066
# Hcoef:  7.55

The following table shows the complete astrometric record for 19QK110. 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 (19QK110) followed by the observatory code and reference code for the source of the astrometry.

2019 08  28.210895 23 30 57.815  -04 22 42.47  24.6r 19QK110   W84  C~7XLh      
2019 08  28.388381 23 30 57.164  -04 22 46.34  24.6r 19QK110   W84  C~7XLh      
2019 09  29.013696 23 29 00.329  -04 34 11.04  24.6r 19QK110   W84  C~7XLh      
2019 09  29.177510 23 28 59.732  -04 34 14.33  24.6r 19QK110   W84  C~7XLh      
2020 10  17.010669 23 30 56.919  -04 08 16.32  24.7r 19QK110   W84  C~7XLh      
2020 10  17.174574 23 30 56.399  -04 08 19.10  24.7r 19QK110   W84  C~7XLh      
2021 09  05.096099 23 36 26.592  -03 21 55.19  24.6r 19QK110   W84  C~7XLh      
2021 09  05.195929 23 36 26.204  -03 21 57.36  24.6r 19QK110   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     0.06
     2   0.0005    -10.47    -0.10       0.29     0.01
     3   0.0871  -1886.13    -0.06      60.10    -0.08
     4   0.0875  -1895.63     0.07      60.60    -0.01
     5   1.1384    329.53     0.02     801.13    -0.00
     6   1.1388    321.28    -0.02     801.65     0.04
     7   2.0230   5963.32     0.13    1404.70    -0.06
     8   2.0232   5957.12    -0.13    1405.01     0.04

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.

19QK110    quality flag:3

Type:           2:1E      2:1E      2:1E

axisobj        47.851    47.979    47.731
ecceobj         0.182     0.189     0.175
incobj         12.206    12.206    12.206
qmin           38.118    37.674    36.609
qmax           57.832    58.416    59.812
amean          47.798    47.798    47.795
amin           47.357    47.315    47.197
amax           48.302    48.342    48.478
emean           0.169     0.168     0.208
emin            0.134     0.128     0.172
emax            0.199     0.210     0.235
imean          13.512    13.648    12.468
imin           12.659    12.700    11.913
imax           14.449    14.681    13.076
excite_mean     0.289     0.290     0.300
fracstop        1.000     1.000     1.000
cjmean          3.044     3.043     3.036

libcent 0        87.0      90.1     180.1
libamp  0        27.3      38.7     149.6
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       180.1     168.4     197.4
kozaiamp        179.9     179.9     180.0