Orbit Fit and Astrometric record for 22RW88

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: 22RW88    
# Created Sat May  4 01:19:06 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:   1.10y
# First observation: 2022/09/01
#  Last observation: 2023/10/07
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.011386   0.000002   0.005772   0.017213   0.000000
# Chi-squared of fit:     2.78 DOF:      8 RMS:  0.11
# Min/Max residuals:    -0.21    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.066524E-05  1.132276E-02  6.334420E-06  5.753333E-03  1.707066E-02 -5.693356E-03
# Covariance matrix:
  9.2209E-13  1.5686E-11 -1.0029E-14  8.7443E-12  2.3886E-11  1.4319E-09
  1.5686E-11  1.4281E-09 -8.7834E-13  7.6097E-10  2.0851E-09  1.2459E-07
 -1.0029E-14 -8.7834E-13  7.3427E-13 -1.1593E-12 -1.2891E-12 -7.6397E-11
  8.7443E-12  7.6097E-10 -1.1593E-12  4.0698E-10  1.1106E-09  6.6490E-08
  2.3886E-11  2.0851E-09 -1.2891E-12  1.1106E-09  3.0515E-09  1.8178E-07
  1.4319E-09  1.2459E-07 -7.6397E-11  6.6490E-08  1.8178E-07  1.0888E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
    7.952970  -37.574482   -0.272152    0.133004   -0.953546  2459823.591031
# Heliocentric elements and errors
Epoch:              2459820.5000  =  2022/08/29
Mean Anomaly:          294.75483 +/-    27.372
Argument of Peri:      129.68399 +/-    12.437
Long of Asc Node:      307.55836 +/-     0.042
Inclination:            27.75476 +/-     0.062
Eccentricity:         0.40701111 +/-    0.2021
Semi-Major Axis:     60.16132434 +/-   12.3246
Time of Perihelion: 2490710.6737 +/-    8822.5
Perihelion:          35.67499668 +/-   14.1851
Aphelion:            84.64765199 +/-   21.1780
Period (y)              466.6425 +/-    143.39
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           46.92017243 +/-    0.1488
Ecliptic Y          -35.75016175 +/-    0.1145
Ecliptic Z            8.10552333 +/-    0.0262
Ecliptic XDOT         0.00028999 +/-    0.0004
Ecliptic YDOT         0.00207768 +/-    0.0003
Ecliptic ZDOT         0.00078744 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   59.54222161 +/-    0.1360
Geocenter to KBO     58.58005664 +/-    0.1896
# Hcoef:  6.96

The following table shows the complete astrometric record for 22RW88. 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 (22RW88) followed by the observatory code and reference code for the source of the astrometry.

2022 09  01.09023  21 28 45.066  -06 30 17.07  24.8r 22RW88    807  C~7BoF      
2022 09  02.08727  21 28 41.815  -06 30 32.01  24.7r 22RW88    807  C~7BoF      
2023 09  14.06353  21 30 09.644  -06 02 15.56  24.8r 22RW88    304  C~7BoF      
2023 09  14.11519  21 30 09.511  -06 02 16.38  24.6r 22RW88    304  C~7BoF      
2023 09  15.06055  21 30 06.743  -06 02 31.08  24.5r 22RW88    304  C~7BoF      
2023 10  06.11037  21 29 14.777  -06 07 42.82  24.4r 22RW88    304  C~7BoF      
2023 10  07.05545  21 29 12.955  -06 07 55.56  24.5r 22RW88    304  C~7BoF      

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    -0.04       0.00    -0.21
     2   0.0027    -50.69     0.04       1.21     0.21
     3   1.0348   1729.92    -0.19    1193.92     0.03
     4   1.0350   1727.78     0.12    1193.78    -0.08
     5   1.0376   1683.96     0.08    1192.96     0.09
     6   1.0952    849.93    -0.06    1143.63     0.04
     7   1.0978    820.12     0.06    1140.18    -0.07

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.

22RW88    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0