Orbit Fit and Astrometric record for 23HA36

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: 23HA36    
# Created Sun Nov 24 02:11:14 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   0.88y
# First observation: 2023/04/22
#  Last observation: 2024/03/08
Preliminary a, adot, b, bdot, g, gdot:
  -0.000001   0.017480   0.000002  -0.004013   0.020973   0.000000
# Chi-squared of fit:     1.55 DOF:      6 RMS:  0.09
# Min/Max residuals:    -0.15    0.15
# Exact a, adot, b, bdot, g, gdot:
  1.227862E-05  1.725419E-02 -3.007587E-06 -3.986216E-03  2.100292E-02  1.790984E-03
# Covariance matrix:
  7.4696E-13  1.1972E-11  6.0949E-14 -2.4447E-12  9.0471E-12  6.7771E-10
  1.1972E-11  1.5445E-08  6.5632E-11 -2.5201E-09  6.1952E-09  6.9461E-07
  6.0949E-14  6.5632E-11  6.7735E-13 -1.1203E-11  2.6425E-11  2.9548E-09
 -2.4447E-12 -2.5201E-09 -1.1203E-11  4.1326E-10 -1.0159E-09 -1.1349E-07
  9.0471E-12  6.1952E-09  2.6425E-11 -1.0159E-09  2.5338E-09  2.8006E-07
  6.7771E-10  6.9461E-07  2.9548E-09 -1.1349E-07  2.8006E-07  3.1284E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.291250  158.852979   -0.801521   -0.003371   -0.619554  2460056.570111
# Heliocentric elements and errors
Epoch:              2460050.5000  =  2023/04/16
Mean Anomaly:          130.36580 +/-    74.675
Argument of Peri:       37.71009 +/-    71.769
Long of Asc Node:      338.56199 +/-     0.007
Inclination:            13.07140 +/-     0.043
Eccentricity:         0.17378241 +/-    0.1641
Semi-Major Axis:     42.77955930 +/-    2.2817
Time of Perihelion: 2423040.9276 +/-   20991.8
Perihelion:          35.34522448 +/-    7.2671
Aphelion:            50.21389412 +/-    7.5119
Period (y)              279.8096 +/-     22.39
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -45.26386196 +/-    0.1064
Ecliptic Y           16.65285604 +/-    0.0412
Ecliptic Z           -0.24216134 +/-    0.0006
Ecliptic XDOT        -0.00102893 +/-    0.0007
Ecliptic YDOT        -0.00200590 +/-    0.0003
Ecliptic ZDOT        -0.00052083 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   48.23062778 +/-    0.1009
Geocenter to KBO     47.61242772 +/-    0.1141
# Hcoef:  6.48

The following table shows the complete astrometric record for 23HA36. 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 (23HA36) followed by the observatory code and reference code for the source of the astrometry.

2023 04  22.06931  10 41 24.090  +07 58 50.07  23.3r 23HA36    304  C~7xZt      
2023 04  22.16273  10 41 23.849  +07 58 51.26  23.3r 23HA36    304  C~7xZt      
2023 05  15.10295  10 40 49.022  +08 01 33.10  23.2r 23HA36    304  C~7xZt      
2023 05  16.08428  10 40 48.367  +08 01 34.88  23.3r 23HA36    304  C~7xZt      
2024 03  07.27368  10 47 19.680  +07 09 51.78  23.2r 23HA36    304  C~7xZt      
2024 03  08.26799  10 47 15.587  +07 10 14.29  23.3r 23HA36    304  C~7xZt      

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     0.15       0.00     0.00
     2   0.0003     -3.77    -0.15      -0.24    -0.02
     3   0.0631   -544.05     0.13     -43.88     0.09
     4   0.0657   -553.74    -0.13     -45.87    -0.08
     5   0.8767   6006.00    -0.06    -733.40     0.00
     6   0.8794   5941.04     0.06    -735.57    -0.00

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.

23HA36    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