Orbit Fit and Astrometric record for 23FN61

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: 23FN61    
# Created Mon Jul  7 01:12:06 2025
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:  57.69d
# First observation: 2023/03/21
#  Last observation: 2023/05/18
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.023738  -0.000000   0.001572   0.021393   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     0.51 DOF:      3 RMS:  0.06
# Min/Max residuals:    -0.11    0.11
# Exact a, adot, b, bdot, g, gdot:
  1.395283E-05  1.789891E-02  9.196711E-07  1.439101E-03  2.044551E-02 -6.272078E-03
# Covariance matrix:
  2.4274E-12  2.1696E-09 -6.7368E-15  4.9667E-11  3.5813E-10 -3.2450E-09
  2.1696E-09  2.7888E-06 -8.5809E-12  6.3596E-08  4.5755E-07 -4.8196E-06
 -6.7368E-15 -8.5809E-12  7.2953E-13 -4.9055E-12 -1.4323E-12  5.8031E-12
  4.9667E-11  6.3596E-08 -4.9055E-12  1.5142E-09  1.0478E-08 -9.3853E-08
  3.5813E-10  4.5755E-07 -1.4323E-12  1.0478E-08  7.5800E-08 -5.2080E-07
 -3.2450E-09 -4.8196E-06  5.8031E-12 -9.3853E-08 -5.2080E-07  1.0833E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    8.175486 -162.046074    0.305821    0.135910   -0.947649  2460024.917531
# Heliocentric elements and errors
Epoch:              2460020.5000  =  2023/03/17
Mean Anomaly:          303.59256 +/-    56.738
Argument of Peri:      156.43248 +/-    25.787
Long of Asc Node:      137.68491 +/-     1.809
Inclination:             9.24868 +/-     0.168
Eccentricity:         0.34663842 +/-    0.5594
Semi-Major Axis:     54.54056929 +/-   26.8800
Time of Perihelion: 2483072.6701 +/-   15723.2
Perihelion:          35.63471228 +/-   35.2037
Aphelion:            73.44642631 +/-   47.3406
Period (y)              402.7984 +/-    297.78
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -47.05176605 +/-    0.6202
Ecliptic Y          -14.92775517 +/-    0.2009
Ecliptic Z            6.95540330 +/-    0.0937
Ecliptic XDOT         0.00155386 +/-    0.0013
Ecliptic YDOT        -0.00200670 +/-    0.0004
Ecliptic ZDOT         0.00007129 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   49.85061883 +/-    0.5886
Geocenter to KBO     48.91050255 +/-    0.6586
# Hcoef:  7.30

The following table shows the complete astrometric record for 23FN61. 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 (23FN61) followed by the observatory code and reference code for the source of the astrometry.

2023 03  21.41673  13 18 39.622  +00 31 17.33  24.2r 23FN61    T09  C~8vOI      
2023 03  21.61396  13 18 38.912  +00 31 22.39  24.3r 23FN61    T09  C~8vOI      
2023 05  16.06380  13 15 17.446  +00 51 16.40  24.2r 23FN61    269  C~8vOI      
2023 05  18.11047  13 15 11.279  +00 51 42.22  24.1r 23FN61    269  C~8vOI      

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     0.04
     2   0.0005    -11.77     0.02       0.65    -0.04
     3   0.1524  -3260.94     0.03     -37.38     0.11
     4   0.1580  -3356.35    -0.03     -48.46    -0.11

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.

23FN61    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