Orbit Fit and Astrometric record for 23PB5

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: 23PB5     
# Created Wed Apr 16 01:11:35 2025
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   1.14y
# First observation: 2023/08/13
#  Last observation: 2024/10/04
Preliminary a, adot, b, bdot, g, gdot:
  -0.000016   0.024702  -0.000001  -0.011834   0.026098   0.000000
# Chi-squared of fit:     1.39 DOF:     10 RMS:  0.07
# Min/Max residuals:    -0.22    0.09
# Exact a, adot, b, bdot, g, gdot:
  1.502894E-05  2.500978E-02 -6.940774E-06 -1.197631E-02  2.644769E-02 -1.771317E-03
# Covariance matrix:
  6.9347E-13  3.1071E-13  4.8219E-14 -2.0120E-13  1.2899E-12  1.4784E-11
  3.1071E-13  5.3966E-11  4.1712E-12 -5.8213E-11  2.2220E-11  3.7211E-09
  4.8219E-14  4.1712E-12  6.1627E-13 -4.8707E-12  1.7466E-12  2.9231E-10
 -2.0120E-13 -5.8213E-11 -4.8707E-12  6.5241E-11 -2.3149E-11 -4.1125E-09
  1.2899E-12  2.2220E-11  1.7466E-12 -2.3149E-11  1.1992E-11  1.4848E-09
  1.4784E-11  3.7211E-09  2.9231E-10 -4.1125E-09  1.4848E-09  2.6275E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    6.219042  -53.595552   -0.230761    0.106023   -0.975437  2460169.849191
# Heliocentric elements and errors
Epoch:              2460160.5000  =  2023/08/04
Mean Anomaly:          328.65247 +/-     6.600
Argument of Peri:      204.50771 +/-     8.627
Long of Asc Node:      139.19317 +/-     0.005
Inclination:            26.25131 +/-     0.009
Eccentricity:         0.10478217 +/-    0.0123
Semi-Major Axis:     42.44532750 +/-    0.1094
Time of Perihelion: 2468955.6656 +/-    1851.3
Perihelion:          37.99781392 +/-    0.5301
Aphelion:            46.89284108 +/-    0.5348
Period (y)              276.5369 +/-      1.07
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           23.08483723 +/-    0.0029
Ecliptic Y          -30.90320246 +/-    0.0040
Ecliptic Z            4.09579485 +/-    0.0005
Ecliptic XDOT         0.00205188 +/-    0.0000
Ecliptic YDOT         0.00158330 +/-    0.0000
Ecliptic ZDOT        -0.00125234 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   38.79037468 +/-    0.0036
Geocenter to KBO     37.81048801 +/-    0.0050
# Hcoef:  7.13

The following table shows the complete astrometric record for 23PB5. 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 (23PB5) followed by the observatory code and reference code for the source of the astrometry.

2023 08  13.34839  20 28 48.875  -12 38 34.75  23.1r 23PB5     T09  C~8nlW      
2023 08  13.48871  20 28 48.187  -12 38 38.57  23.0r 23PB5     T09  C~8nlW      
2023 09  14.01750  20 26 37.950  -12 52 48.29  23.1r 23PB5     269  C~8nlW      
2023 09  15.01885  20 26 34.858  -12 53 13.62  23.0r 23PB5     269  C~8nlW      
2023 10  06.05752  20 25 49.660  -13 01 17.19  22.9r 23PB5     269  C~8nlW      
2023 10  07.04406  20 25 48.558  -13 01 36.96  22.8r 23PB5     269  C~8nlW      
2024 10  03.21771  20 32 10.847  -13 19 29.81        23PB5     G37  C~8nlW      
2024 10  04.18112  20 32 09.432  -13 19 49.47        23PB5     G37  C~8nlW      

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    -0.05
     2   0.0004    -10.69     0.08      -1.27    -0.07
     3   0.0867  -2064.65    -0.22    -366.96     0.05
     4   0.0894  -2114.62     0.02    -380.70     0.09
     5   0.1470  -2872.04     0.05    -692.00    -0.03
     6   0.1497  -2892.41     0.08    -707.35     0.02
     7   1.1413   2265.62    -0.03   -3100.42    -0.02
     8   1.1440   2240.77     0.03   -3114.42     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.

23PB5    quality flag:1

Type:          5:3EE  SCATEXTD  SCATNEAR

axisobj        42.188    42.484    42.081
ecceobj         0.102     0.096     0.120
incobj         26.274    26.303    26.250
qmin           34.643    37.422    32.421
qmax           50.374    48.109    52.778
amean          42.326    42.644    42.326
amin           41.959    42.313    41.853
amax           42.744    43.007    42.833
emean           0.121     0.104     0.137
emin            0.050     0.089     0.020
emax            0.180     0.119     0.233
imean          24.635    24.970    24.597
imin           23.619    24.547    22.651
imax           25.602    25.363    26.173
excite_mean     0.435     0.435     0.443
fracstop        1.000     1.000     1.000
cjmean          2.850     2.852     2.842

libcent 0       182.5    -180.0    -180.0
libamp  0        64.6    -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       171.8     186.3     187.1
kozaiamp        180.0     180.0     154.4