Orbit Fit and Astrometric record for 23FW54

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: 23FW54    
# Created Wed Dec 25 02:11:19 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   0.97y
# First observation: 2023/03/21
#  Last observation: 2024/03/08
Preliminary a, adot, b, bdot, g, gdot:
  -0.000011   0.022321   0.000002  -0.000383   0.023107   0.000000
# Chi-squared of fit:     0.48 DOF:     10 RMS:  0.04
# Min/Max residuals:    -0.07    0.08
# Exact a, adot, b, bdot, g, gdot:
  1.504634E-05  2.213322E-02 -6.637969E-07 -3.804499E-04  2.330846E-02 -3.515421E-03
# Covariance matrix:
  7.4256E-13  4.9942E-12  4.5422E-14 -1.2242E-13  3.1660E-12  2.4475E-10
  4.9942E-12  7.1350E-10  3.2241E-12 -1.2370E-11  2.4532E-10  2.9257E-08
  4.5422E-14  3.2241E-12  3.1345E-13 -4.2786E-13  1.1794E-12  1.3371E-10
 -1.2242E-13 -1.2370E-11 -4.2786E-13  1.4360E-12 -4.3557E-12 -5.0985E-10
  3.1660E-12  2.4532E-10  1.1794E-12 -4.3557E-12  8.8792E-11  1.0156E-08
  2.4475E-10  2.9257E-08  1.3371E-10 -5.0985E-10  1.0156E-08  1.2032E-06
#      lat0       lon0       xBary       yBary       zBary        JD0
    2.814735  157.341705   -0.389097    0.045280   -0.925469  2460024.799871
# Heliocentric elements and errors
Epoch:              2460020.5000  =  2023/03/17
Mean Anomaly:          286.25530 +/-     4.381
Argument of Peri:      201.05390 +/-     0.142
Long of Asc Node:       47.41827 +/-     0.069
Inclination:             2.94024 +/-     0.001
Eccentricity:         0.14801816 +/-    0.0496
Semi-Major Axis:     44.72840661 +/-    0.6735
Time of Perihelion: 2482402.6533 +/-    1229.8
Perihelion:          38.10779005 +/-    2.2923
Aphelion:            51.34902318 +/-    2.3501
Period (y)              299.1461 +/-      6.76
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -40.54007264 +/-    0.0160
Ecliptic Y           16.50561984 +/-    0.0067
Ecliptic Z            2.10679587 +/-    0.0008
Ecliptic XDOT        -0.00062487 +/-    0.0001
Ecliptic YDOT        -0.00254848 +/-    0.0000
Ecliptic ZDOT        -0.00006494 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.82204428 +/-    0.0150
Geocenter to KBO     42.90287154 +/-    0.0173
# Hcoef:  6.59

The following table shows the complete astrometric record for 23FW54. 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 (23FW54) followed by the observatory code and reference code for the source of the astrometry.

2023 03  21.29907  10 40 26.202  +11 25 34.63  23.0r 23FW54    568  C~7xZn      
2023 03  21.49670  10 40 25.370  +11 25 38.97  23.0r 23FW54    568  C~7xZn      
2023 04  22.05788  10 38 39.934  +11 34 33.83  23.0r 23FW54    304  C~7xZn      
2023 04  22.12657  10 38 39.761  +11 34 34.55  23.0r 23FW54    304  C~7xZn      
2023 05  15.08792  10 38 05.888  +11 36 21.82  22.9r 23FW54    304  C~7xZn      
2023 05  15.96946  10 38 05.456  +11 36 20.66  23.0r 23FW54    304  C~7xZn      
2024 03  07.26173  10 46 09.458  +10 50 12.88  22.8r 23FW54    304  C~7xZn      
2024 03  08.25435  10 46 05.038  +10 50 38.64  22.9r 23FW54    304  C~7xZn      

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    -0.01       0.00     0.08
     2   0.0005    -12.97    -0.00      -0.56    -0.04
     3   0.0870  -1650.37     0.04     -83.74     0.03
     4   0.0871  -1653.00    -0.04     -84.02     0.02
     5   0.1500  -2154.88    -0.03    -170.07    -0.06
     6   0.1524  -2160.34     0.03    -173.51    -0.04
     7   0.9636   5480.35     0.07     -62.09    -0.01
     8   0.9663   5410.28    -0.07     -62.93     0.02

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.

23FW54    quality flag:2

Type:      CLASSICAL  SCATNEAR CLASSICAL

axisobj        44.949    46.911    44.467
ecceobj         0.147     0.270     0.060
incobj          2.936     2.939     2.934
qmin           37.791    31.171    41.113
qmax           52.631    65.948    48.178
amean          45.017    45.776    44.520
amin           44.635    37.987    44.166
amax           45.438    49.118    44.888
emean           0.140     0.283     0.059
emin            0.123     0.144     0.043
emax            0.159     0.346     0.073
imean           1.917     4.246     2.090
imin            1.091     1.320     1.457
imax            2.646     7.639     2.556
excite_mean     0.144     0.293     0.069
fracstop        1.000     1.000     1.000
cjmean          3.088     3.015     3.102

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       186.7     181.9     182.1
kozaiamp        180.0     180.0     180.0