Orbit Fit and Astrometric record for 21RZ236

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: 21RZ236   
# Created Fri Nov 22 02:11:11 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.10y
# First observation: 2019/08/29
#  Last observation: 2021/10/03
Preliminary a, adot, b, bdot, g, gdot:
   0.000003   0.018667  -0.000007   0.004804   0.021875   0.000000
# Chi-squared of fit:     3.34 DOF:     10 RMS:  0.11
# Min/Max residuals:    -0.17    0.25
# Exact a, adot, b, bdot, g, gdot:
  1.340010E-05  1.862720E-02  3.921780E-06  4.794604E-03  2.179699E-02 -5.812038E-04
# Covariance matrix:
  7.0834E-13 -8.0378E-13  2.2653E-14 -1.3818E-13 -2.4835E-13 -1.3516E-11
 -8.0378E-13  4.2452E-11 -1.8269E-12  1.1066E-11  5.1789E-11  1.0820E-09
  2.2653E-14 -1.8269E-12  7.0385E-13 -8.1491E-13 -2.2323E-12 -4.6887E-11
 -1.3818E-13  1.1066E-11 -8.1491E-13  3.1597E-12  1.3517E-11  2.8402E-10
 -2.4835E-13  5.1789E-11 -2.2323E-12  1.3517E-11  6.4921E-11  1.3216E-09
 -1.3516E-11  1.0820E-09 -4.6887E-11  2.8402E-10  1.3216E-09  2.7771E-08
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.824969   -9.258856    0.261442   -0.013959   -0.969763  2458724.712719
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          205.37114 +/-     5.407
Argument of Peri:      154.99452 +/-     5.382
Long of Asc Node:      353.55132 +/-     0.000
Inclination:            14.44101 +/-     0.002
Eccentricity:         0.08045809 +/-    0.0027
Semi-Major Axis:     43.63390839 +/-    0.0485
Time of Perihelion: 2503939.6758 +/-    1579.5
Perihelion:          40.12320742 +/-    0.1272
Aphelion:            47.14460937 +/-    0.1302
Period (y)              288.2334 +/-      0.48
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           46.19348707 +/-    0.0167
Ecliptic Y           -7.80184044 +/-    0.0027
Ecliptic Z           -0.66036628 +/-    0.0002
Ecliptic XDOT         0.00032142 +/-    0.0000
Ecliptic YDOT         0.00232014 +/-    0.0000
Ecliptic ZDOT         0.00060300 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   46.85235368 +/-    0.0165
Geocenter to KBO     45.87789123 +/-    0.0170
# Hcoef:  9.12

The following table shows the complete astrometric record for 21RZ236. 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 (21RZ236) followed by the observatory code and reference code for the source of the astrometry.

2019 08  29.211918 23 27 16.561  -04 25 40.25  25.8r 21RZ236   W84  C~7XPn      
2019 08  29.387113 23 27 15.845  -04 25 44.08  25.8r 21RZ236   W84  C~7XPn      
2020 10  17.010669 23 27 30.918  -04 03 39.40  25.8r 21RZ236   W84  C~7XPn      
2020 10  17.174574 23 27 30.353  -04 03 42.49  25.8r 21RZ236   W84  C~7XPn      
2021 09  07.105479 23 33 40.026  -03 08 12.86  25.4r 21RZ236   W84  C~7XPn      
2021 09  07.194942 23 33 39.688  -03 08 15.19  25.4r 21RZ236   W84  C~7XPn      
2021 10  03.011907 23 31 53.986  -03 18 18.19  25.9r 21RZ236   W84  C~7XPn      
2021 10  03.165173 23 31 53.383  -03 18 21.72  25.9r 21RZ236   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     0.02       0.00    -0.09
     2   0.0005    -11.35    -0.04       0.70     0.11
     3   1.1357    717.58     0.03    1129.56     0.02
     4   1.1361    708.59     0.00    1130.05    -0.06
     5   2.0257   7110.63    -0.17    2005.90     0.25
     6   2.0260   7105.05     0.21    2005.76    -0.16
     7   2.0966   5410.95    -0.06    2077.32     0.05
     8   2.0971   5401.26     0.01    2077.64    -0.11

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.

21RZ236    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        43.696    43.824    43.601
ecceobj         0.080     0.092     0.073
incobj         14.420    14.422    14.418
qmin           38.975    38.310    39.256
qmax           48.450    49.502    48.007
amean          43.595    43.726    43.506
amin           43.243    43.327    43.163
amax           43.962    44.191    43.866
emean           0.088     0.104     0.081
emin            0.074     0.085     0.069
emax            0.102     0.122     0.095
imean          14.784    14.666    14.786
imin           14.233    14.018    14.249
imax           15.286    15.291    15.278
excite_mean     0.270     0.274     0.268
fracstop        1.000     1.000     1.000
cjmean          3.008     3.007     3.008

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       180.2     179.1     181.6
kozaiamp        179.9     180.0     180.0