Orbit Fit and Astrometric record for 20KW11

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: 20KW11    
# Created Sun Nov 24 02:11:02 2024
# Orbit generated from Bernstein formalism
# Fitting     22 observations of     22
# Arc: 159.78d
# First observation: 2020/05/29
#  Last observation: 2020/11/05
Preliminary a, adot, b, bdot, g, gdot:
  -0.000017   0.021504  -0.000014  -0.001060   0.021454   0.000000
# Chi-squared of fit:     3.10 DOF:     38 RMS:  0.07
# Min/Max residuals:    -0.19    0.16
# Exact a, adot, b, bdot, g, gdot:
  1.364460E-05  1.791342E-02 -9.133681E-07 -1.244236E-03  2.087303E-02  1.920094E-03
# Covariance matrix:
  2.5431E-13 -7.6190E-13  2.1203E-15 -4.1093E-14  2.4677E-13  4.3499E-11
 -7.6190E-13  1.9284E-10 -8.1638E-13  1.2400E-11  7.9655E-12 -6.5629E-09
  2.1203E-15 -8.1638E-13  2.0596E-13 -6.1149E-13 -2.7977E-14  2.9000E-11
 -4.1093E-14  1.2400E-11 -6.1149E-13  3.1381E-12  3.8105E-13 -4.4677E-10
  2.4677E-13  7.9655E-12 -2.7977E-14  3.8105E-13  1.5947E-12 -9.4181E-11
  4.3499E-11 -6.5629E-09  2.9000E-11 -4.4677E-10 -9.4181E-11  2.5181E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.813304  -73.344993    0.632531    0.038460   -0.785249  2458998.947781
# Heliocentric elements and errors
Epoch:              2458990.5000  =  2020/05/21
Mean Anomaly:          121.68691 +/-     8.541
Argument of Peri:       12.57177 +/-     8.290
Long of Asc Node:      141.10037 +/-     0.040
Inclination:             4.79477 +/-     0.005
Eccentricity:         0.11583020 +/-    0.0194
Semi-Major Axis:     45.53130733 +/-    0.1767
Time of Perihelion: 2421058.5669 +/-    2653.2
Perihelion:          40.25740708 +/-    0.8984
Aphelion:            50.80520758 +/-    0.9064
Period (y)              307.2369 +/-      1.79
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           13.33947041 +/-    0.0008
Ecliptic Y          -46.78485607 +/-    0.0028
Ecliptic Z            2.35146717 +/-    0.0001
Ecliptic XDOT         0.00233358 +/-    0.0000
Ecliptic YDOT         0.00042831 +/-    0.0001
Ecliptic ZDOT        -0.00015088 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   48.70619700 +/-    0.0027
Geocenter to KBO     47.90870376 +/-    0.0029
# Hcoef:  8.95

The following table shows the complete astrometric record for 20KW11. 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 (20KW11) followed by the observatory code and reference code for the source of the astrometry.

2020 05  29.44698  19 10 45.888  -19 36 32.21  25.6r 20KW11    266  C~6VL7      
2020 05  29.53371  19 10 45.596  -19 36 32.57  25.6r 20KW11    266  C~5Zeh      
2020 05  29.61905  19 10 45.308  -19 36 32.92  25.6r 20KW11    266  C~5Zeh      
2020 05  31.44139  19 10 39.217  -19 36 40.67  25.8r 20KW11    266  C~5Zeh      
2020 05  31.52961  19 10 38.910  -19 36 41.07  25.8r 20KW11    266  C~5Zeh      
2020 05  31.61814  19 10 38.602  -19 36 41.45  25.8r 20KW11    266  C~6VL7      
2020 08  12.26680  19 05 41.422  -19 45 41.52  25.9r 20KW11    266  C~6VL7      
2020 08  12.34843  19 05 41.132  -19 45 42.20  25.9r 20KW11    266  C~6VL7      
2020 08  12.42950  19 05 40.844  -19 45 42.87  25.9r 20KW11    266  C~5Zeh      
2020 08  14.24286  19 05 34.636  -19 45 57.90  25.8r 20KW11    266  C~5Zeh      
2020 08  14.33285  19 05 34.325  -19 45 58.65  25.8r 20KW11    266  C~5Zeh      
2020 08  14.42134  19 05 34.020  -19 45 59.37  25.8r 20KW11    266  C~6VL7      
2020 10  18.323666 19 04 28.283  -19 51 51.34        20KW11    250  S~5zHB      
2020 10  18.329985 19 04 28.291  -19 51 51.42        20KW11    250  S~5zHB      
2020 10  18.336305 19 04 28.295  -19 51 51.48        20KW11    250  S~5zHB      
2020 10  18.342624 19 04 28.297  -19 51 51.50        20KW11    250  S~5zHB      
2020 10  18.348944 19 04 28.302  -19 51 51.45        20KW11    250  S~5zHB      
2020 11  05.201572 19 05 12.096  -19 51 52.67        20KW11    250  S~5zHB      
2020 11  05.207891 19 05 12.111  -19 51 52.63        20KW11    250  S~5zHB      
2020 11  05.214210 19 05 12.124  -19 51 52.57        20KW11    250  S~5zHB      
2020 11  05.220530 19 05 12.138  -19 51 52.50        20KW11    250  S~5zHB      
2020 11  05.226849 19 05 12.156  -19 51 52.45        20KW11    250  S~5zHB      

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    -0.01
     2   0.0002     -4.14    -0.01       0.14     0.00
     3   0.0005     -8.22    -0.02       0.29    -0.00
     4   0.0055    -94.59     0.02       3.00     0.00
     5   0.0057    -98.95     0.01       3.13    -0.00
     6   0.0059   -103.31     0.01       3.28     0.00
     7   0.2048  -4335.46    -0.01     -41.00     0.01
     8   0.2051  -4339.61    -0.01     -41.21     0.02
     9   0.2053  -4343.72    -0.01     -41.42     0.01
    10   0.2103  -4432.54     0.01     -46.40     0.00
    11   0.2105  -4436.99     0.01     -46.65     0.00
    12   0.2107  -4441.35     0.01     -46.88     0.00
    13   0.3884  -5403.31     0.16    -292.21     0.02
    14   0.3885  -5403.21     0.11    -292.30    -0.05
    15   0.3885  -5403.16     0.01    -292.37    -0.09
    16   0.3885  -5403.13    -0.11    -292.39    -0.08
    17   0.3885  -5403.05    -0.19    -292.35    -0.02
    18   0.4374  -4788.91     0.15    -362.98    -0.07
    19   0.4374  -4788.69     0.08    -362.97    -0.03
    20   0.4374  -4788.50    -0.01    -362.93     0.03
    21   0.4374  -4788.30    -0.09    -362.88     0.10
    22   0.4375  -4788.04    -0.12    -362.86     0.14

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.

20KW11    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.997    45.715    44.684
ecceobj         0.120     0.171     0.094
incobj          4.800     4.808     4.794
qmin           38.936    37.243    39.728
qmax           51.924    55.148    50.320
amean          45.242    45.976    44.911
amin           44.857    45.569    44.552
amax           45.673    46.436    45.305
emean           0.122     0.171     0.096
emin            0.107     0.157     0.082
emax            0.137     0.188     0.111
imean           3.821     3.704     3.897
imin            3.208     2.812     3.387
imax            4.533     4.620     4.523
excite_mean     0.139     0.183     0.118
fracstop        1.000     1.000     1.000
cjmean          3.093     3.084     3.096

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       178.8     180.2     175.5
kozaiamp        180.0     180.0     180.0