Orbit Fit and Astrometric record for 23FU54

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: 23FU54    
# Created Tue May  7 01:18:16 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:
  -0.000012   0.015213   0.000020  -0.010065   0.022424   0.000000
# Chi-squared of fit:     4.01 DOF:     10 RMS:  0.13
# Min/Max residuals:    -0.28    0.28
# Exact a, adot, b, bdot, g, gdot:
  1.036364E-05  1.492945E-02 -6.969179E-06 -9.933452E-03  2.259701E-02 -1.059135E-02
# Covariance matrix:
  6.9907E-13  5.5076E-14  6.9918E-14 -6.1356E-13  1.4938E-12  5.7033E-11
  5.5076E-14  1.4345E-10  5.9758E-12 -8.1922E-11  5.2856E-11  7.9721E-09
  6.9918E-14  5.9758E-12  5.5515E-13 -3.8588E-12  2.3943E-12  3.3924E-10
 -6.1356E-13 -8.1922E-11 -3.8588E-12  4.8728E-11 -3.1673E-11 -4.6219E-09
  1.4938E-12  5.2856E-11  2.3943E-12 -3.1673E-11  2.4098E-11  3.0732E-09
  5.7033E-11  7.9721E-09  3.3924E-10 -4.6219E-09  3.0732E-09  4.4955E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
    4.179892  157.011252   -0.394494    0.067149   -0.921851  2460024.803501
# Heliocentric elements and errors
Epoch:              2460020.5000  =  2023/03/17
Mean Anomaly:          294.80183 +/-     5.758
Argument of Peri:      296.07329 +/-     1.680
Long of Asc Node:      343.62640 +/-     0.001
Inclination:            33.88890 +/-     0.006
Eccentricity:         0.50198553 +/-    0.0227
Semi-Major Axis:     43.68562755 +/-    1.3263
Time of Perihelion: 2479120.7577 +/-    1445.2
Perihelion:          21.75607477 +/-    1.1919
Aphelion:            65.61518033 +/-    2.2255
Period (y)              288.7461 +/-     13.15
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -41.62693989 +/-    0.0088
Ecliptic Y           17.23531802 +/-    0.0038
Ecliptic Z            3.22526818 +/-    0.0007
Ecliptic XDOT         0.00038908 +/-    0.0001
Ecliptic YDOT        -0.00212207 +/-    0.0000
Ecliptic ZDOT        -0.00129389 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.16924470 +/-    0.0083
Geocenter to KBO     44.25363996 +/-    0.0096
# Hcoef:  6.16

The following table shows the complete astrometric record for 23FU54. 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 (23FU54) followed by the observatory code and reference code for the source of the astrometry.

2023 03  21.30270  10 41 16.814  +12 48 55.82  22.7r 23FU54    568  C~7xZn      
2023 03  21.50089  10 41 15.929  +12 48 59.33  22.8r 23FU54    568  C~7xZn      
2023 04  22.06545  10 39 21.074  +12 55 08.28  22.8r 23FU54    304  C~7xZn      
2023 04  22.13343  10 39 20.873  +12 55 08.84  22.8r 23FU54    304  C~7xZn      
2023 05  15.09913  10 38 39.044  +12 54 53.06  22.5r 23FU54    304  C~7xZn      
2023 05  16.08071  10 38 38.202  +12 54 46.58  22.6r 23FU54    304  C~7xZn      
2024 03  07.27091  10 44 40.945  +11 53 04.19  22.5r 23FU54    304  C~7xZn      
2024 03  08.26462  10 44 36.229  +11 53 24.81  22.5r 23FU54    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     0.02       0.00     0.00
     2   0.0005    -13.31     0.01      -1.61     0.04
     3   0.0870  -1708.81     0.09    -288.81    -0.16
     4   0.0871  -1711.74    -0.17    -289.39    -0.02
     5   0.1500  -2273.21    -0.04    -532.46     0.04
     6   0.1527  -2282.21     0.09    -543.07     0.12
     7   0.9636   4034.64     0.04   -1976.87     0.28
     8   0.9664   3962.73    -0.04   -1983.97    -0.28

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.

23FU54    quality flag:1

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        43.800    47.793    40.941
ecceobj         0.501     0.563     0.440
incobj         33.859    33.847    33.871
qmin           19.306    18.052    20.112
qmax           72.366    79.191    63.367
amean          44.538    47.566    41.220
amin           43.255    43.507    40.263
amax           45.955    49.721    41.936
emean           0.547     0.590     0.486
emin            0.498     0.562     0.439
emax            0.575     0.610     0.513
imean          32.214    32.638    32.570
imin           31.000    31.260    31.398
imax           34.765    34.798    34.777
excite_mean     0.764     0.800     0.725
fracstop        0.107     0.089     0.083
cjmean          2.386     2.331     2.442

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       295.4     316.4     324.7
kozaiamp        179.9      23.3      28.1