Orbit Fit and Astrometric record for 21RW209

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: 21RW209   
# Created Wed May  8 01:18:45 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   1.20y
# First observation: 2021/09/07
#  Last observation: 2022/11/20
Preliminary a, adot, b, bdot, g, gdot:
  -0.000001   0.011150  -0.000002  -0.009667   0.016908   0.000000
# Chi-squared of fit:     0.72 DOF:      6 RMS:  0.06
# Min/Max residuals:    -0.10    0.10
# Exact a, adot, b, bdot, g, gdot:
  9.934880E-06  1.124227E-02 -8.652012E-06 -9.732042E-03  1.705523E-02  3.875898E-03
# Covariance matrix:
  7.6283E-13  1.8925E-12  7.3945E-15 -2.2174E-12  3.9086E-12  1.9729E-10
  1.8925E-12  2.3319E-10  6.1907E-13 -1.9440E-10  3.5634E-10  1.7316E-08
  7.3945E-15  6.1907E-13  7.3439E-13 -1.1782E-12  9.5693E-13  4.8265E-11
 -2.2174E-12 -1.9440E-10 -1.1782E-12  1.6729E-10 -2.9931E-10 -1.4818E-08
  3.9086E-12  3.5634E-10  9.5693E-13 -2.9931E-10  5.4685E-10  2.6657E-08
  1.9729E-10  1.7316E-08  4.8265E-11 -1.4818E-08  2.6657E-08  1.3191E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
    8.955050    8.632735    0.399968    0.142293   -0.904025  2459465.117661
# Heliocentric elements and errors
Epoch:              2459460.5000  =  2021/09/03
Mean Anomaly:           32.46747 +/-     2.999
Argument of Peri:      103.96437 +/-     7.057
Long of Asc Node:      198.36413 +/-     0.009
Inclination:            41.41888 +/-     0.028
Eccentricity:         0.33616128 +/-    0.0778
Semi-Major Axis:     77.50349682 +/-    4.4028
Time of Perihelion: 2436984.1203 +/-     801.1
Perihelion:          51.44982202 +/-    6.7022
Aphelion:           103.55717162 +/-    8.4252
Period (y)              682.3232 +/-     58.14
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           58.23509425 +/-    0.0785
Ecliptic Y            8.43177646 +/-    0.0119
Ecliptic Z            9.12629687 +/-    0.0125
Ecliptic XDOT         0.00058194 +/-    0.0002
Ecliptic YDOT         0.00192087 +/-    0.0000
Ecliptic ZDOT        -0.00144655 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   59.54586763 +/-    0.0768
Geocenter to KBO     58.63302943 +/-    0.0804
# Hcoef:  7.38

The following table shows the complete astrometric record for 21RW209. 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 (21RW209) followed by the observatory code and reference code for the source of the astrometry.

2021 09  07.61686  00 17 21.596  +11 38 30.69  25.0r 21RW209   568  C~6DL3      
2021 09  08.61871  00 17 18.560  +11 38 09.18  25.1r 21RW209   568  C~6DL3      
2022 10  16.10870  00 18 40.571  +11 07 13.39  25.0r 21RW209   304  C~6DL3      
2022 10  16.17879  00 18 40.349  +11 07 11.35  25.0r 21RW209   304  C~6DL3      
2022 11  19.04598  00 17 15.856  +10 51 58.73  25.1r 21RW209   304  C~6DL3      
2022 11  20.04390  00 17 14.113  +10 51 34.33  25.2r 21RW209   304  C~6DL3      

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     0.10       0.00    -0.08
     2   0.0027    -49.49    -0.10      -1.79     0.07
     3   1.1047    311.06     0.05   -2185.53     0.04
     4   1.1049    307.25    -0.05   -2186.09    -0.01
     5   1.1976  -1198.57     0.05   -2523.20     0.03
     6   1.2003  -1231.89    -0.04   -2535.24    -0.05

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.

21RW209    quality flag:1

Type:       SCATNEAR  SCATNEAR  SCATEXTD

axisobj        77.093    98.990    70.368
ecceobj         0.332     0.555     0.154
incobj         41.400    41.325    41.473
qmin           50.563    42.947    58.534
qmax          104.140   157.113    81.975
amean          76.687    98.363    69.995
amin           75.794    96.849    69.326
amax           77.789   100.626    70.724
emean           0.323     0.549     0.148
emin            0.312     0.536     0.139
emax            0.339     0.562     0.159
imean          41.702    41.664    41.658
imin           41.383    41.286    41.453
imax           42.053    42.265    41.874
excite_mean     0.740     0.862     0.681
fracstop        1.000     1.000     1.000
cjmean          2.648     2.564     2.684

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       143.3     119.8     192.7
kozaiamp         41.6      27.3      50.1