Orbit Fit and Astrometric record for 20DJ6

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: 20DJ6     
# Created Sat May  4 01:18:33 2024
# Orbit generated from Bernstein formalism
# Fitting     22 observations of     22
# Arc:   3.97y
# First observation: 2019/04/07
#  Last observation: 2023/03/28
Preliminary a, adot, b, bdot, g, gdot:
  -0.000041   0.020184   0.000001  -0.000126   0.021890   0.000000
# Chi-squared of fit:    54.76 DOF:     38 RMS:  0.28
# Min/Max residuals:    -0.73    0.62
# Exact a, adot, b, bdot, g, gdot:
  1.352853E-05  2.004110E-02 -8.927683E-08 -1.250207E-04  2.224704E-02 -1.131803E-03
# Covariance matrix:
  7.2925E-13 -3.7369E-13 -1.6317E-15  1.5536E-15 -8.2206E-13 -2.7013E-12
 -3.7369E-13  8.5552E-13  2.8386E-15 -5.0912E-15 -3.3464E-13  9.8310E-12
 -1.6317E-15  2.8386E-15  2.1213E-13 -7.8177E-14  2.1518E-16  3.3028E-14
  1.5536E-15 -5.0912E-15 -7.8177E-14  4.2022E-14  2.7755E-15 -6.2152E-14
 -8.2206E-13 -3.3464E-13  2.1518E-16  2.7755E-15  2.3106E-12 -6.0471E-12
 -2.7013E-12  9.8310E-12  3.3028E-14 -6.2152E-14 -6.0471E-12  1.2065E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.302809 -161.948431    0.031211    0.005329   -0.999681  2458580.572391
# Heliocentric elements and errors
Epoch:              2458580.5000  =  2019/04/07
Mean Anomaly:          233.90030 +/-     0.205
Argument of Peri:      273.52167 +/-     0.203
Long of Asc Node:       57.37210 +/-     0.043
Inclination:             0.46715 +/-     0.000
Eccentricity:         0.07750592 +/-    0.0005
Semi-Major Axis:     43.79038704 +/-    0.0110
Time of Perihelion: 2495655.2433 +/-      58.7
Perihelion:          40.39637285 +/-    0.0238
Aphelion:            47.18440122 +/-    0.0246
Period (y)              289.7853 +/-      0.11
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -43.69512536 +/-    0.0029
Ecliptic Y          -14.21678719 +/-    0.0010
Ecliptic Z            0.23754683 +/-    0.0000
Ecliptic XDOT         0.00090492 +/-    0.0000
Ecliptic YDOT        -0.00230283 +/-    0.0000
Ecliptic ZDOT        -0.00001634 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.95038027 +/-    0.0028
Geocenter to KBO     44.94980508 +/-    0.0031
# Hcoef:  7.08

The following table shows the complete astrometric record for 20DJ6. 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 (20DJ6) followed by the observatory code and reference code for the source of the astrometry.

2019 04  07.07159  13 07 03.36   -06 48 01.2   23.4R 20DJ6     W93  C~4iU2      
2019 04  07.10118  13 07 03.22   -06 48 00.2   23.1R 20DJ6     W93  C~4iU2      
2020 02  28.20986  13 13 43.30   -07 29 11.7   21.3R 20DJ6     W93  C~44Aa      
2020 02  28.24544  13 13 43.20   -07 29 11.7         20DJ6     W93  C~44Aa      
2020 02  28.28222  13 13 43.07   -07 29 10.8         20DJ6     W93  C~44Aa      
2020 03  01.20628  13 13 37.28   -07 28 35.8         20DJ6     W93  C~44Aa      
2020 03  01.24589  13 13 37.14   -07 28 34.1   23.3R 20DJ6     W93  C~44Aa      
2020 03  01.28328  13 13 37.03   -07 28 33.4   23.0R 20DJ6     W93  C~44Aa      
2020 03  03.19854  13 13 31.05   -07 27 56.4         20DJ6     W93  C~44Aa      
2020 03  03.23509  13 13 30.89   -07 27 55.9         20DJ6     W93  C~44Aa      
2020 03  03.27422  13 13 30.75   -07 27 54.9   23.4R 20DJ6     W93  C~44Aa      
2021 03  22.18242  13 16 40.60   -07 47 28.9   23.7R 20DJ6     W93  C~4iU2      
2021 03  22.20353  13 16 40.51   -07 47 28.4   23.6R 20DJ6     W93  C~4iU2      
2021 03  22.22274  13 16 40.39   -07 47 28.2   23.8R 20DJ6     W93  C~4iU2      
2022 03  26.14347  13 20 43.95   -08 12 18.6   23.6R 20DJ6     W93  C~5ahW      
2022 03  26.18023  13 20 43.80   -08 12 18.1   24.1R 20DJ6     W93  C~5ahW      
2022 03  26.21168  13 20 43.71   -08 12 17.3         20DJ6     W93  C~5ahW      
2022 03  28.14190  13 20 35.85   -08 11 30.2   23.6R 20DJ6     W93  C~5ahW      
2022 03  28.17563  13 20 35.74   -08 11 29.2   23.2R 20DJ6     W93  C~5ahW      
2023 03  28.13990  13 24 55.99   -08 37 47.2         20DJ6     W93  C~7xXX      
2023 03  28.18352  13 24 55.77   -08 37 46.2   23.6R 20DJ6     W93  C~7xXX      
2023 03  28.22185  13 24 55.64   -08 37 45.7   23.3R 20DJ6     W93  C~7xXX      

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     0.15       0.00     0.00
     2   0.0001     -2.31    -0.14       0.13     0.14
     3   0.8957   6446.84    -0.40     -28.59     0.20
     4   0.8958   6445.46    -0.04     -29.15    -0.35
     5   0.8959   6443.33    -0.38     -29.05    -0.24
     6   0.9011   6350.29     0.52     -29.15    -0.73
     7   0.9012   6347.72    -0.05     -28.36     0.07
     8   0.9013   6345.94     0.06     -28.33     0.11
     9   0.9066   6249.52     0.54     -27.66     0.42
    10   0.9067   6247.13     0.06     -28.09    -0.01
    11   0.9068   6244.82    -0.20     -27.95     0.14
    12   1.9579   9306.09     0.10     -51.93     0.29
    13   1.9579   9304.66     0.03     -51.97     0.26
    14   1.9580   9302.93    -0.47     -52.45    -0.22
    15   2.9680  13227.45    -0.04     -78.26     0.04
    16   2.9681  13225.19     0.11     -78.63    -0.31
    17   2.9682  13223.64     0.62     -78.39    -0.06
    18   2.9735  13097.29    -0.34     -78.31    -0.02
    19   2.9736  13095.39    -0.00     -77.99     0.31
    20   3.9728  17289.80     0.14    -104.22     0.24
    21   3.9729  17286.38    -0.40    -104.50    -0.03
    22   3.9730  17284.39     0.14    -104.76    -0.26

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.

20DJ6    quality flag:1

Type:      CLASSICAL    7:4EEE  SCATNEAR

axisobj        43.423    43.457    43.389
ecceobj         0.081     0.080     0.083
incobj          0.464     0.464     0.464
qmin           39.292    39.712    36.597
qmax           48.514    48.034    51.522
amean          43.729    43.727    43.712
amin           43.321    43.364    43.236
amax           44.139    44.106    44.267
emean           0.074     0.077     0.135
emin            0.046     0.063     0.073
emax            0.099     0.089     0.164
imean           1.643     1.593     1.808
imin            0.751     0.755     0.034
imax            2.356     2.252     2.615
excite_mean     0.080     0.082     0.139
fracstop        1.000     1.000     1.000
cjmean          3.090     3.090     3.074

libcent 0      -180.0     182.6    -180.0
libamp  0      -180.0      99.1    -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       189.5     168.9     196.6
kozaiamp        180.0     168.1     180.0