Orbit Fit and Astrometric record for 20KP54

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: 20KP54    
# Created Wed May  8 01:18:30 2024
# Orbit generated from Bernstein formalism
# Fitting     21 observations of     21
# Arc:  76.98d
# First observation: 2020/05/28
#  Last observation: 2020/08/13
Preliminary a, adot, b, bdot, g, gdot:
   0.000005   0.018139   0.000003  -0.001000   0.023691   0.000000
# Chi-squared of fit:     0.32 DOF:     36 RMS:  0.02
# Min/Max residuals:    -0.03    0.05
# Exact a, adot, b, bdot, g, gdot:
  1.579949E-05  2.471066E-02 -7.176830E-07 -1.012859E-03  2.480326E-02  2.924213E-03
# Covariance matrix:
  1.9892E-13  1.4523E-11 -8.0244E-15 -7.0426E-14  3.4964E-12  1.9060E-10
  1.4523E-11  1.9338E-07 -9.2873E-11 -5.3919E-10  3.6352E-08  6.5757E-07
 -8.0244E-15 -9.2873E-11  1.7260E-13 -6.8639E-13 -1.7465E-11 -3.1700E-10
 -7.0426E-14 -5.3919E-10 -6.8639E-13  1.6829E-11 -1.0159E-10 -1.8876E-09
  3.4964E-12  3.6352E-08 -1.7465E-11 -1.0159E-10  6.8389E-09  1.2478E-07
  1.9060E-10  6.5757E-07 -3.1700E-10 -1.8876E-09  1.2478E-07  2.5094E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.822199  -72.385185    0.658535    0.024181   -0.764103  2458997.947541
# Heliocentric elements and errors
Epoch:              2458990.5000  =  2020/05/21
Mean Anomaly:           55.11875 +/-     5.702
Argument of Peri:       75.34282 +/-     4.123
Long of Asc Node:      144.45132 +/-     0.523
Inclination:             2.91854 +/-     0.035
Eccentricity:         0.11528339 +/-    0.0725
Semi-Major Axis:     43.53436124 +/-    1.7709
Time of Perihelion: 2442926.8741 +/-    1341.8
Perihelion:          38.51557244 +/-    3.5243
Aphelion:            48.55315004 +/-    3.7238
Period (y)              287.2476 +/-     17.53
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           11.80381210 +/-    0.0407
Ecliptic Y          -39.34223183 +/-    0.1281
Ecliptic Z            1.28205056 +/-    0.0043
Ecliptic XDOT         0.00270656 +/-    0.0001
Ecliptic YDOT         0.00051808 +/-    0.0002
Ecliptic ZDOT        -0.00010171 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.09482740 +/-    0.1231
Geocenter to KBO     40.31727423 +/-    0.1344
# Hcoef: 10.25

The following table shows the complete astrometric record for 20KP54. 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 (20KP54) followed by the observatory code and reference code for the source of the astrometry.

2020 05  28.44674  19 15 20.563  -20 28 21.61  26.6r 20KP54    266  C~6c5Z      
2020 05  28.50129  19 15 20.359  -20 28 21.92  26.6r 20KP54    266  C~6c5Z      
2020 05  28.55756  19 15 20.148  -20 28 22.23  26.6r 20KP54    266  C~6c5Z      
2020 05  30.43935  19 15 13.139  -20 28 32.68  26.1r 20KP54    266  C~6c5Z      
2020 05  30.53044  19 15 12.786  -20 28 33.22  26.1r 20KP54    266  C~6c5Z      
2020 05  30.61862  19 15 12.443  -20 28 33.71  26.1r 20KP54    266  C~6c5a      
2020 06  01.43269  19 15 05.458  -20 28 44.45  26.4r 20KP54    266  C~6c5a      
2020 06  01.47325  19 15 05.296  -20 28 44.70  26.4r 20KP54    266  C~6c5a      
2020 06  01.60571  19 15 04.764  -20 28 45.50  26.4r 20KP54    266  C~6c5a      
2020 06  20.45583  19 13 41.179  -20 31 02.51  26.4r 20KP54    266  C~6c5a      
2020 06  20.52860  19 13 40.819  -20 31 03.12  26.4r 20KP54    266  C~6c5a      
2020 06  20.62233  19 13 40.357  -20 31 03.88  26.4r 20KP54    266  C~6c5a      
2020 06  22.44948  19 13 31.449  -20 31 19.31  26.2r 20KP54    266  C~6c5a      
2020 06  22.52092  19 13 31.091  -20 31 19.92  26.2r 20KP54    266  C~6c5a      
2020 06  22.59118  19 13 30.740  -20 31 20.50  26.2r 20KP54    266  C~6c5a      
2020 06  25.44823  19 13 16.599  -20 31 45.23  26.0r 20KP54    266  C~6c5a      
2020 06  25.53213  19 13 16.172  -20 31 45.96  26.0r 20KP54    266  C~6c5a      
2020 06  25.61487  19 13 15.753  -20 31 46.67  26.0r 20KP54    266  C~6c5a      
2020 08  13.24332  19 09 19.601  -20 39 26.47  26.5r 20KP54    266  C~6c5a      
2020 08  13.33331  19 09 19.231  -20 39 27.28  26.5r 20KP54    266  C~6c5a      
2020 08  13.42301  19 09 18.863  -20 39 28.07  26.5r 20KP54    266  C~6c5a      

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     0.01
     2   0.0001     -2.88    -0.01       0.06     0.01
     3   0.0003     -5.86    -0.01       0.13     0.01
     4   0.0055   -104.88    -0.03       2.42     0.04
     5   0.0057   -109.87    -0.03       2.52     0.04
     6   0.0059   -114.71    -0.02       2.65     0.05
     7   0.0109   -213.44     0.04       4.58    -0.03
     8   0.0110   -215.73     0.04       4.63    -0.03
     9   0.0114   -223.24     0.04       4.79    -0.03
    10   0.0630  -1405.54     0.02      18.08    -0.02
    11   0.0632  -1410.64     0.01      18.11    -0.02
    12   0.0635  -1417.17     0.01      18.17    -0.03
    13   0.0685  -1543.27    -0.00      18.62    -0.01
    14   0.0686  -1548.33    -0.01      18.64    -0.02
    15   0.0688  -1553.30    -0.01      18.69    -0.01
    16   0.0767  -1753.49    -0.01      19.09     0.00
    17   0.0769  -1759.54    -0.02      19.12     0.01
    18   0.0771  -1765.47    -0.01      19.15     0.00
    19   0.2103  -5113.73     0.00     -31.53     0.01
    20   0.2105  -5118.99    -0.00     -31.71     0.01
    21   0.2107  -5124.22     0.00     -31.88     0.01

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.

20KP54    quality flag:1

Type:      CLASSICAL  SCATNEAR CLASSICAL

axisobj        42.945    52.070    38.595
ecceobj         0.108     0.318     0.098
incobj          2.920     2.817     3.038
qmin           37.840    35.035    34.752
qmax           48.839    70.997    43.162
amean          43.189    52.269    38.777
amin           42.842    51.470    38.459
amax           43.583    53.277    39.135
emean           0.100     0.314     0.080
emin            0.076     0.296     0.058
emax            0.121     0.333     0.103
imean           2.842     2.339     1.525
imin            1.511     1.651     0.115
imax            4.009     3.046     2.573
excite_mean     0.113     0.316     0.085
fracstop        1.000     1.000     1.000
cjmean          3.077     3.076     3.038

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       178.4     180.8     178.1
kozaiamp        180.0     180.0     180.0