Orbit Fit and Astrometric record for 20KN54

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: 20KN54    
# Created Wed May  8 01:18:30 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:  77.97d
# First observation: 2020/05/28
#  Last observation: 2020/08/14
Preliminary a, adot, b, bdot, g, gdot:
   0.000015   0.045453   0.000009   0.010084   0.048923   0.000000
# Chi-squared of fit:     0.11 DOF:     36 RMS:  0.01
# Min/Max residuals:    -0.03    0.02
# Exact a, adot, b, bdot, g, gdot:
  1.882736E-05  6.163817E-02  3.052516E-06  9.998039E-03  5.144382E-02 -1.512950E-02
# Covariance matrix:
  2.1080E-13 -4.1149E-11  1.8111E-14  6.8149E-14 -6.8667E-12  1.0961E-11
 -4.1149E-11  1.3324E-07 -7.3852E-11  3.1193E-10  2.4772E-08  1.9900E-07
  1.8111E-14 -7.3852E-11  1.7538E-13 -9.7053E-13 -1.3774E-11 -1.1503E-10
  6.8149E-14  3.1193E-10 -9.7053E-13  1.0664E-11  5.9611E-11  6.4584E-10
 -6.8667E-12  2.4772E-08 -1.3774E-11  5.9611E-11  4.6125E-09  3.7708E-08
  1.0961E-11  1.9900E-07 -1.1503E-10  6.4584E-10  3.7708E-08  3.7607E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.006723  -72.603240    0.655621    0.026730   -0.766520  2458997.947541
# Heliocentric elements and errors
Epoch:              2458990.5000  =  2020/05/21
Mean Anomaly:          247.82525 +/-     0.604
Argument of Peri:      152.68358 +/-     0.487
Long of Asc Node:      273.93811 +/-     0.070
Inclination:             9.50259 +/-     0.054
Eccentricity:         0.32690435 +/-    0.0088
Semi-Major Axis:     16.89777595 +/-    0.0286
Time of Perihelion: 2466896.1092 +/-      37.5
Perihelion:          11.37381943 +/-    0.1499
Aphelion:            22.42173246 +/-    0.1534
Period (y)               69.4628 +/-      0.18
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            5.41740212 +/-    0.0077
Ecliptic Y          -19.47297451 +/-    0.0245
Ecliptic Z            0.68080956 +/-    0.0009
Ecliptic XDOT         0.00289229 +/-    0.0000
Ecliptic YDOT         0.00177000 +/-    0.0000
Ecliptic ZDOT         0.00050334 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   20.22395816 +/-    0.0237
Geocenter to KBO     19.43868133 +/-    0.0257
# Hcoef: 11.40

The following table shows the complete astrometric record for 20KN54. 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 (20KN54) followed by the observatory code and reference code for the source of the astrometry.

2020 05  28.44674  19 14 19.186  -20 19 02.91  24.6r 20KN54    266  C~6c5Z      
2020 05  28.50129  19 14 18.780  -20 19 03.11  24.6r 20KN54    266  C~6c5Z      
2020 05  28.55756  19 14 18.360  -20 19 03.30  24.6r 20KN54    266  C~6c5Z      
2020 05  30.43935  19 14 04.427  -20 19 09.98  24.4r 20KN54    266  C~6c5Z      
2020 05  30.53044  19 14 03.723  -20 19 10.36  24.4r 20KN54    266  C~6c5Z      
2020 05  30.61862  19 14 03.040  -20 19 10.68  24.4r 20KN54    266  C~6c5Z      
2020 06  01.43269  19 13 49.104  -20 19 18.25  24.6r 20KN54    266  C~6c5Z      
2020 06  01.47325  19 13 48.780  -20 19 18.45  24.6r 20KN54    266  C~6c5Z      
2020 06  01.60571  19 13 47.718  -20 19 19.05  24.6r 20KN54    266  C~6c5Z      
2020 06  21.45390  19 10 49.708  -20 21 39.44  24.2r 20KN54    266  C~6c5Z      
2020 06  21.53376  19 10 48.904  -20 21 40.17  24.2r 20KN54    266  C~6c5Z      
2020 06  21.61261  19 10 48.112  -20 21 40.86  24.2r 20KN54    266  C~6c5Z      
2020 06  24.43648  19 10 19.980  -20 22 07.89  24.2r 20KN54    266  C~6c5Z      
2020 06  24.52180  19 10 19.106  -20 22 08.72  24.2r 20KN54    266  C~6c5Z      
2020 06  24.61708  19 10 18.132  -20 22 09.60  24.2r 20KN54    266  C~6c5Z      
2020 08  12.26680  19 02 21.935  -20 31 14.54  24.5r 20KN54    266  C~6c5Z      
2020 08  12.34843  19 02 21.269  -20 31 15.39  24.5r 20KN54    266  C~6c5Z      
2020 08  12.42950  19 02 20.609  -20 31 16.19  24.5r 20KN54    266  C~6c5Z      
2020 08  14.24286  19 02 06.431  -20 31 34.47  24.4r 20KN54    266  C~6c5Z      
2020 08  14.33285  19 02 05.721  -20 31 35.38  24.4r 20KN54    266  C~6c5Z      
2020 08  14.42134  19 02 05.024  -20 31 36.23  24.4r 20KN54    266  C~6c5Z      

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   0.0001     -5.69     0.02       0.53     0.00
     3   0.0003    -11.57     0.02       1.09     0.00
     4   0.0055   -206.83     0.00      19.28    -0.01
     5   0.0057   -216.71     0.00      20.15    -0.01
     6   0.0059   -226.28     0.01      21.05    -0.00
     7   0.0109   -421.69    -0.03      38.29    -0.00
     8   0.0110   -426.24    -0.03      38.66    -0.00
     9   0.0114   -441.14    -0.03      39.95    -0.01
    10   0.0657  -2943.09     0.00     210.61     0.01
    11   0.0659  -2954.40     0.00     211.26     0.01
    12   0.0662  -2965.54     0.00     211.93     0.02
    13   0.0739  -3361.60     0.01     233.04    -0.00
    14   0.0741  -3373.90     0.01     233.70     0.00
    15   0.0744  -3387.61     0.00     234.48     0.01
    16   0.2076 -10106.68    -0.02     461.62     0.00
    17   0.2078 -10116.09    -0.01     461.79    -0.00
    18   0.2080 -10125.42    -0.01     462.01    -0.00
    19   0.2130 -10325.89     0.01     465.47    -0.01
    20   0.2132 -10335.93     0.01     465.64    -0.00
    21   0.2135 -10345.78     0.01     465.86    -0.00

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.

20KN54    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        16.767    17.331    16.295
ecceobj         0.333     0.274     0.389
incobj          9.543     9.272     9.837
qmin           11.088    12.270     9.957
qmax           22.773    22.870    28.360
amean          16.811    17.144    18.063
amin           16.589    16.582    16.145
amax           17.057    17.898    19.365
emean           0.330     0.260     0.406
emin            0.305     0.218     0.360
emax            0.343     0.280     0.467
imean          11.087    10.238    10.458
imin           10.647     9.519     9.234
imax           12.879    10.832    11.903
excite_mean     0.382     0.315     0.445
fracstop        0.005     0.005     0.007
cjmean          3.178     3.193     3.063

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       198.8     243.1     177.4
kozaiamp         37.4      87.1     178.5