Orbit Fit and Astrometric record for 21RR237

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: 21RR237   
# Created Wed May  8 01:18:46 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.11y
# First observation: 2019/08/30
#  Last observation: 2021/10/07
Preliminary a, adot, b, bdot, g, gdot:
   0.000006   0.023589  -0.000016   0.009040   0.025200   0.000000
# Chi-squared of fit:     7.41 DOF:     10 RMS:  0.17
# Min/Max residuals:    -0.29    0.46
# Exact a, adot, b, bdot, g, gdot:
  1.477645E-05  2.348285E-02  5.348673E-06  9.005382E-03  2.501273E-02 -1.526550E-03
# Covariance matrix:
  7.0260E-13 -6.8339E-13  2.6522E-14 -1.6035E-13 -8.5553E-14 -8.2942E-12
 -6.8339E-13  1.9759E-11 -1.2736E-12  7.5196E-12  2.2800E-11  3.8885E-10
  2.6522E-14 -1.2736E-12  7.0591E-13 -8.2563E-13 -1.4726E-12 -2.5455E-11
 -1.6035E-13  7.5196E-12 -8.2563E-13  3.1604E-12  8.6777E-12  1.5035E-10
 -8.5553E-14  2.2800E-11 -1.4726E-12  8.6777E-12  2.8069E-11  4.4873E-10
 -8.2942E-12  3.8885E-10 -2.5455E-11  1.5035E-10  4.4873E-10  7.7750E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -2.940651   -8.539771    0.257119   -0.049801   -0.969599  2458725.713221
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          314.03277 +/-     1.081
Argument of Peri:       45.29919 +/-     1.424
Long of Asc Node:      358.53688 +/-     0.000
Inclination:            21.15145 +/-     0.001
Eccentricity:         0.08280992 +/-    0.0031
Semi-Major Axis:     43.27865540 +/-    0.0404
Time of Perihelion: 2471999.1805 +/-     311.6
Perihelion:          39.69475326 +/-    0.1388
Aphelion:            46.86255754 +/-    0.1407
Period (y)              284.7206 +/-      0.40
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           40.40911126 +/-    0.0084
Ecliptic Y           -6.33445191 +/-    0.0013
Ecliptic Z           -2.05080367 +/-    0.0004
Ecliptic XDOT         0.00027514 +/-    0.0000
Ecliptic YDOT         0.00255975 +/-    0.0000
Ecliptic ZDOT         0.00099276 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.95396623 +/-    0.0083
Geocenter to KBO     39.97964243 +/-    0.0085
# Hcoef:  9.26

The following table shows the complete astrometric record for 21RR237. 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 (21RR237) followed by the observatory code and reference code for the source of the astrometry.

2019 08  30.212420 23 33 16.962  -06 05 17.40  25.3r 21RR237   W84  C~7XPo      
2019 08  30.387214 23 33 16.160  -06 05 21.87  25.3r 21RR237   W84  C~7XPo      
2020 10  16.001792 23 33 49.248  -05 23 10.97  25.4r 21RR237   W84  C~7XPo      
2020 10  16.175804 23 33 48.528  -05 23 14.02  25.4r 21RR237   W84  C~7XPo      
2021 09  09.073508 23 40 48.544  -04 08 06.05  25.1r 21RR237   W84  C~7XPo      
2021 09  09.192572 23 40 47.965  -04 08 09.93  25.1r 21RR237   W84  C~7XPo      
2021 10  07.004805 23 38 37.959  -04 19 22.69  25.3r 21RR237   W84  C~7XPo      
2021 10  07.169933 23 38 37.214  -04 19 26.36  25.3r 21RR237   W84  C~7XPo      

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     0.07
     2   0.0005    -12.75    -0.00       0.63    -0.08
     3   1.1302   1442.33     0.03    2129.65    -0.08
     4   1.1306   1431.25    -0.05    2131.10     0.08
     5   2.0284   8990.27     0.24    3777.70     0.46
     6   2.0287   8980.76    -0.27    3777.58    -0.29
     7   2.1048   6925.51     0.03    3933.67    -0.06
     8   2.1053   6913.81     0.01    3934.73    -0.10

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.

21RR237    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        43.340    43.415    43.271
ecceobj         0.087     0.093     0.081
incobj         21.114    21.116    21.112
qmin           38.889    38.683    39.045
qmax           47.801    48.125    47.450
amean          43.230    43.301    43.164
amin           42.900    42.964    42.827
amax           43.590    43.661    43.525
emean           0.084     0.090     0.079
emin            0.072     0.078     0.066
emax            0.097     0.103     0.091
imean          21.482    21.491    21.475
imin           21.077    21.089    21.074
imax           21.874    21.876    21.869
excite_mean     0.376     0.377     0.375
fracstop        1.000     1.000     1.000
cjmean          2.918     2.918     2.919

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       177.2     177.6     178.7
kozaiamp        180.0     179.9     180.0