Orbit Fit and Astrometric record for 21RU237

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: 21RU237   
# Created Tue Apr  1 01:11:26 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   2.10y
# First observation: 2019/08/28
#  Last observation: 2021/10/04
Preliminary a, adot, b, bdot, g, gdot:
   0.000014   0.024822   0.000000   0.001066   0.024719   0.000000
# Chi-squared of fit:     1.42 DOF:     10 RMS:  0.07
# Min/Max residuals:    -0.15    0.15
# Exact a, adot, b, bdot, g, gdot:
  1.556236E-05  2.477538E-02  9.849955E-07  1.063822E-03  2.464722E-02 -3.769444E-04
# Covariance matrix:
  7.4072E-13  1.6522E-12 -3.5917E-15  9.1037E-14  1.7211E-12  4.0608E-11
  1.6522E-12  1.9572E-11 -3.9647E-14  9.8499E-13  1.0713E-11  4.3959E-10
 -3.5917E-15 -3.9647E-14  3.8284E-13 -1.9114E-13 -2.1238E-14 -8.9979E-13
  9.1037E-14  9.8499E-13 -1.9114E-13  2.2929E-13  5.3457E-13  2.2344E-11
  1.7211E-12  1.0713E-11 -2.1238E-14  5.3457E-13  8.6240E-12  2.3849E-10
  4.0608E-11  4.3959E-10 -8.9979E-13  2.2344E-11  2.3849E-10  9.9719E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.656128   -7.228740    0.311926   -0.010932   -0.954903  2458723.711696
# Heliocentric elements and errors
Epoch:              2458720.5000  =  2019/08/25
Mean Anomaly:          344.53814 +/-     2.949
Argument of Peri:        3.09377 +/-     3.414
Long of Asc Node:        6.98207 +/-     0.005
Inclination:             2.53251 +/-     0.001
Eccentricity:         0.06928611 +/-    0.0012
Semi-Major Axis:     44.48639880 +/-    0.0144
Time of Perihelion: 2463375.2743 +/-     887.6
Perihelion:          41.40410937 +/-    0.0548
Aphelion:            47.56868823 +/-    0.0554
Period (y)              296.7215 +/-      0.14
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.15835333 +/-    0.0048
Ecliptic Y           -5.54152868 +/-    0.0006
Ecliptic Z           -0.46456772 +/-    0.0001
Ecliptic XDOT         0.00031456 +/-    0.0000
Ecliptic YDOT         0.00273587 +/-    0.0000
Ecliptic ZDOT         0.00011842 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.53232972 +/-    0.0048
Geocenter to KBO     40.57253340 +/-    0.0048
# Hcoef:  8.50

The following table shows the complete astrometric record for 21RU237. 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 (21RU237) followed by the observatory code and reference code for the source of the astrometry.

2019 08  28.210895 23 34 29.260  -03 28 18.17  24.7r 21RU237   W84  C~7XPo      
2019 08  28.388381 23 34 28.488  -03 28 22.87  24.7r 21RU237   W84  C~7XPo      
2019 09  29.013696 23 32 08.625  -03 43 03.74  24.6r 21RU237   W84  C~7XPo      
2019 09  29.177510 23 32 07.899  -03 43 08.35  24.6r 21RU237   W84  C~7XPo      
2021 09  06.108763 23 44 05.727  -02 18 07.54  24.4r 21RU237   W84  C~7XPo      
2021 09  06.196686 23 44 05.322  -02 18 10.25  24.4r 21RU237   W84  C~7XPo      
2021 10  04.002582 23 42 01.886  -02 31 09.97  24.6r 21RU237   W84  C~7XPo      
2021 10  04.175328 23 42 01.128  -02 31 14.62  24.6r 21RU237   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     0.07       0.00    -0.06
     2   0.0005    -12.48    -0.07       0.25     0.06
     3   0.0871  -2284.06     0.03      18.19     0.08
     4   0.0875  -2295.86    -0.03      18.24    -0.07
     5   2.0257   9604.44     0.15     442.99     0.08
     6   2.0260   9597.78    -0.15     442.92    -0.07
     7   2.1021   7586.85     0.03     461.83    -0.01
     8   2.1026   7574.57    -0.03     462.07     0.01

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.

21RU237    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.564    44.616    44.516
ecceobj         0.073     0.072     0.073
incobj          2.533     2.533     2.532
qmin           40.445    40.531    40.362
qmax           48.610    48.652    48.654
amean          44.425    44.478    44.377
amin           44.070    44.131    44.025
amax           44.792    44.846    44.757
emean           0.070     0.069     0.072
emin            0.055     0.054     0.056
emax            0.086     0.085     0.088
imean           2.836     2.848     2.824
imin            2.126     2.155     2.092
imax            3.447     3.440     3.449
excite_mean     0.086     0.086     0.087
fracstop        1.000     1.000     1.000
cjmean          3.097     3.098     3.097

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       182.2     183.2     181.1
kozaiamp        180.0     180.0     180.0