Orbit Fit and Astrometric record for 23FP61

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: 23FP61    
# Created Mon Jul  7 01:12:06 2025
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:  31.84d
# First observation: 2023/03/21
#  Last observation: 2023/04/22
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.025836  -0.000000   0.000561   0.023313   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     0.39 DOF:      3 RMS:  0.06
# Min/Max residuals:    -0.08    0.08
# Exact a, adot, b, bdot, g, gdot:
  1.479557E-05  2.122333E-02  7.616601E-08  6.281604E-04  2.251387E-02  1.493451E-03
# Covariance matrix:
  7.1780E-11  9.5599E-08 -6.0253E-13 -1.2951E-09  1.8536E-08 -6.0180E-07
  9.5599E-08  1.2869E-04 -8.1141E-10 -1.7441E-06  2.4931E-05 -8.2253E-04
 -6.0253E-13 -8.1141E-10  7.3232E-13  2.6295E-12 -1.5701E-10  5.3011E-09
 -1.2951E-09 -1.7441E-06  2.6295E-12  2.3857E-08 -3.3744E-07  1.1433E-05
  1.8536E-08  2.4931E-05 -1.5701E-10 -3.3744E-07  4.8389E-06 -1.5355E-04
 -6.0180E-07 -8.2253E-04  5.3011E-09  1.1433E-05 -1.5355E-04  8.9324E-03
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.984837  157.532834   -0.385705   -0.016170   -0.927843  2460024.781511
# Heliocentric elements and errors
Epoch:              2460020.5000  =  2023/03/17
Mean Anomaly:           70.74819 +/-   218.118
Argument of Peri:      250.48527 +/-   318.970
Long of Asc Node:      187.44985 +/-    18.773
Inclination:             1.96274 +/-     1.140
Eccentricity:         0.08342196 +/-    4.3218
Semi-Major Axis:     46.31325055 +/-   21.1932
Time of Perihelion: 2437396.5116 +/-  184218.1
Perihelion:          42.44970846 +/-  201.0947
Aphelion:            50.17679263 +/-  201.4670
Period (y)              315.1854 +/-    216.35
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -42.03594839 +/-    4.0097
Ecliptic Y           16.96985333 +/-    1.6585
Ecliptic Z           -0.76342142 +/-    0.0746
Ecliptic XDOT        -0.00115723 +/-    0.0103
Ecliptic YDOT        -0.00230641 +/-    0.0052
Ecliptic ZDOT         0.00007323 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   45.33850121 +/-    3.7691
Geocenter to KBO     44.41706845 +/-    4.3398
# Hcoef:  7.26

The following table shows the complete astrometric record for 23FP61. 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 (23FP61) followed by the observatory code and reference code for the source of the astrometry.

2023 03  21.28071  10 35 24.641  +07 49 45.05  23.7r 23FP61    T09  C~8vOI      
2023 03  21.47603  10 35 23.860  +07 49 49.62  23.8r 23FP61    T09  C~8vOI      
2023 04  22.04981  10 33 45.379  +08 00 13.23  23.8r 23FP61    269  C~8vOI      
2023 04  22.11966  10 33 45.220  +08 00 14.38  23.8r 23FP61    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     0.08
     2   0.0005    -12.47    -0.02      -0.06    -0.08
     3   0.0870  -1602.56     0.05      36.94    -0.06
     4   0.0872  -1605.18    -0.05      37.13     0.06

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.

23FP61    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