Orbit Fit and Astrometric record for 23FN57

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: 23FN57    
# Created Sun Nov 24 02:11:14 2024
# Orbit generated from Bernstein formalism
# Fitting      8 observations of      8
# Arc:   1.12y
# First observation: 2023/03/21
#  Last observation: 2024/05/04
Preliminary a, adot, b, bdot, g, gdot:
   0.000019   0.025691  -0.000002  -0.000860   0.025102   0.000000
# Chi-squared of fit:     4.92 DOF:     10 RMS:  0.14
# Min/Max residuals:    -0.28    0.23
# Exact a, adot, b, bdot, g, gdot:
  1.561017E-05  2.592476E-02 -1.087879E-06 -8.677573E-04  2.533400E-02 -8.786843E-04
# Covariance matrix:
  7.3621E-13  2.1953E-12 -1.9508E-14 -7.4918E-14  2.2246E-12  1.1524E-10
  2.1953E-12  7.9346E-11 -2.2371E-13 -2.2011E-12  3.7548E-11  3.8489E-09
 -1.9508E-14 -2.2371E-13  4.1563E-13 -3.9107E-13 -1.5746E-13 -1.0350E-11
 -7.4918E-14 -2.2011E-12 -3.9107E-13  7.5408E-13 -1.0606E-12 -1.0760E-10
  2.2246E-12  3.7548E-11 -1.5746E-13 -1.0606E-12  2.2045E-11  1.7888E-09
  1.1524E-10  3.8489E-09 -1.0350E-11 -1.0760E-10  1.7888E-09  1.8892E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
   -3.050767  157.442504   -0.387101   -0.049577   -0.926074  2460024.777431
# Heliocentric elements and errors
Epoch:              2460020.5000  =  2023/03/17
Mean Anomaly:          342.92812 +/-    11.515
Argument of Peri:      257.40680 +/-    13.460
Long of Asc Node:      280.32645 +/-     0.032
Inclination:             3.52728 +/-     0.001
Eccentricity:         0.07183770 +/-    0.0062
Semi-Major Axis:     43.34820570 +/-    0.0529
Time of Perihelion: 2464963.9939 +/-    3334.4
Perihelion:          40.23417015 +/-    0.2720
Aphelion:            46.46224125 +/-    0.2734
Period (y)              285.4072 +/-      0.52
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -37.39736744 +/-    0.0067
Ecliptic Y           15.11896706 +/-    0.0028
Ecliptic Z           -2.10080083 +/-    0.0004
Ecliptic XDOT        -0.00098449 +/-    0.0000
Ecliptic YDOT        -0.00261693 +/-    0.0000
Ecliptic ZDOT        -0.00008862 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.39256888 +/-    0.0063
Geocenter to KBO     39.47264392 +/-    0.0073
# Hcoef:  7.31

The following table shows the complete astrometric record for 23FN57. 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 (23FN57) followed by the observatory code and reference code for the source of the astrometry.

2023 03  21.27663  10 31 59.495  +05 56 36.26  23.1r 23FN57    T09  C~83ID      
2023 03  21.47104  10 31 58.634  +05 56 41.49  23.2r 23FN57    T09  C~83ID      
2023 04  22.10746  10 30 11.309  +06 08 37.23  23.2r 23FN57    304  C~83ID      
2023 05  16.02186  10 29 40.553  +06 13 13.89  23.1r 23FN57    304  C~83ID      
2024 04  12.02152  10 36 02.516  +05 30 09.93  23.7r 23FN57    304  C~83ID      
2024 04  12.13206  10 36 02.178  +05 30 12.44  23.8r 23FN57    304  C~83ID      
2024 05  04.00920  10 35 12.754  +05 36 26.49  23.4r 23FN57    304  C~83ID      
2024 05  04.07269  10 35 12.682  +05 36 27.26  23.3r 23FN57    304  C~83ID      

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     0.12       0.00     0.11
     2   0.0005    -13.87    -0.07       0.12     0.07
     3   0.0871  -1765.96    -0.28      74.71    -0.23
     4   0.1526  -2294.34     0.23     162.92     0.04
     5   1.0616   3957.17    -0.03    -131.05    -0.14
     6   1.0619   3951.55     0.11    -130.59     0.05
     7   1.1218   3127.34    -0.18     -56.80    -0.00
     8   1.1220   3126.05     0.09     -56.48     0.10

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.

23FN57    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.615    43.922    43.468
ecceobj         0.075     0.085     0.086
incobj          3.520     3.523     3.518
qmin           39.015    39.253    38.791
qmax           48.556    48.861    48.469
amean          43.638    43.925    43.509
amin           43.286    43.570    43.159
amax           44.009    44.300    43.886
emean           0.079     0.087     0.085
emin            0.057     0.070     0.067
emax            0.104     0.103     0.105
imean           5.408     5.184     5.430
imin            4.514     4.399     4.544
imax            6.309     5.948     6.257
excite_mean     0.123     0.126     0.128
fracstop        1.000     1.000     1.000
cjmean          3.079     3.082     3.076

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       181.2     182.9     176.8
kozaiamp        179.9     180.0     180.0