Orbit Fit and Astrometric record for 21RJ237

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: 21RJ237   
# Created Tue Apr  1 01:11:26 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.10y
# First observation: 2019/08/30
#  Last observation: 2021/10/06
Preliminary a, adot, b, bdot, g, gdot:
   0.000006   0.022113   0.000000   0.000026   0.023354   0.000000
# Chi-squared of fit:     5.48 DOF:     10 RMS:  0.15
# Min/Max residuals:    -0.34    0.34
# Exact a, adot, b, bdot, g, gdot:
  1.528236E-05  2.211698E-02  4.784599E-07  2.624010E-05  2.331135E-02  6.529974E-04
# Covariance matrix:
  7.2805E-13 -1.9214E-12  1.0367E-15 -2.1163E-15 -1.4904E-12 -3.5279E-11
 -1.9214E-12  9.4343E-11 -8.7163E-14  1.2551E-13  1.0758E-10  2.0115E-09
  1.0367E-15 -8.7163E-14  6.2454E-13 -3.3479E-13 -1.0149E-13 -1.8558E-12
 -2.1163E-15  1.2551E-13 -3.3479E-13  2.5447E-13  1.4351E-13  2.6831E-12
 -1.4904E-12  1.0758E-10 -1.0149E-13  1.4351E-13  1.2438E-10  2.2942E-09
 -3.5279E-11  2.0115E-09 -1.8558E-12  2.6831E-12  2.2942E-09  4.3027E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.712391   -7.503463    0.274636   -0.028862   -0.965636  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:           82.72870 +/-     1.327
Argument of Peri:      186.17015 +/-     2.442
Long of Asc Node:       80.19798 +/-     0.046
Inclination:             1.67543 +/-     0.000
Eccentricity:         0.02641496 +/-    0.0093
Semi-Major Axis:     43.98418633 +/-    0.0198
Time of Perihelion: 2434235.6766 +/-     392.4
Perihelion:          42.82234581 +/-    0.4097
Aphelion:            45.14602686 +/-    0.4097
Period (y)              291.7112 +/-      0.20
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           43.43600509 +/-    0.0203
Ecliptic Y           -6.00471388 +/-    0.0027
Ecliptic Z           -1.28186281 +/-    0.0006
Ecliptic XDOT         0.00042376 +/-    0.0000
Ecliptic YDOT         0.00256589 +/-    0.0000
Ecliptic ZDOT         0.00000056 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.86782761 +/-    0.0201
Geocenter to KBO     42.89756041 +/-    0.0205
# Hcoef:  9.18

The following table shows the complete astrometric record for 21RJ237. 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 (21RJ237) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 35 09.066  -04 33 01.76  25.4r 21RJ237   W84  C~7XPn      
2019 08  30.387214 23 35 08.345  -04 33 06.23  25.4r 21RJ237   W84  C~7XPn      
2020 10  18.012125 23 36 26.331  -04 24 16.79  25.4r 21RJ237   W84  C~7XPn      
2020 10  18.176134 23 36 25.747  -04 24 20.54  25.4r 21RJ237   W84  C~7XPn      
2021 09  09.073508 23 43 46.339  -03 37 08.33  25.6r 21RJ237   W84  C~7XPn      
2021 09  09.192572 23 43 45.846  -03 37 11.58  25.6r 21RJ237   W84  C~7XPn      
2021 10  06.002765 23 41 52.769  -03 49 14.98  25.6r 21RJ237   W84  C~7XPn      
2021 10  06.167954 23 41 52.053  -03 49 19.53  25.6r 21RJ237   W84  C~7XPn      

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    -0.06       0.00    -0.10
     2   0.0005    -11.67     0.06       0.16     0.10
     3   1.1357   1268.88     0.00      24.75     0.14
     4   1.1361   1259.37    -0.00      24.76    -0.14
     5   2.0284   8439.29    -0.12       6.30    -0.02
     6   2.0287   8431.21     0.12       6.26    -0.08
     7   2.1021   6588.09     0.34      15.94     0.11
     8   2.1025   6576.44    -0.34      16.03    -0.02

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.

21RJ237    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.038    44.071    44.007
ecceobj         0.023     0.037     0.021
incobj          1.676     1.676     1.676
qmin           42.346    41.743    42.400
qmax           45.661    46.330    45.545
amean          43.918    43.954    43.888
amin           43.574    43.616    43.556
amax           44.270    44.307    44.229
emean           0.017     0.031     0.016
emin            0.000     0.014     0.000
emax            0.032     0.046     0.030
imean           0.656     0.658     0.660
imin            0.383     0.363     0.391
imax            0.864     0.887     0.865
excite_mean     0.021     0.033     0.020
fracstop        1.000     1.000     1.000
cjmean          3.100     3.100     3.100

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       187.8     187.7     186.8
kozaiamp        179.9     180.0     179.9