Orbit Fit and Astrometric record for 15HA197

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: 15HA197   
# Created Wed Nov 27 02:10:19 2024
# Orbit generated from Bernstein formalism
# Fitting      6 observations of      6
# Arc:   1.08y
# First observation: 2014/03/24
#  Last observation: 2015/04/22
Preliminary a, adot, b, bdot, g, gdot:
   0.000001   0.014780   0.000000   0.012255   0.021415   0.000000
# Chi-squared of fit:     0.50 DOF:      6 RMS:  0.05
# Min/Max residuals:    -0.10    0.09
# Exact a, adot, b, bdot, g, gdot:
  1.066116E-05  1.466986E-02  9.259996E-06  1.216740E-02  2.125217E-02 -6.457486E-03
# Covariance matrix:
  7.9397E-13  3.3966E-11  7.1906E-15  2.9472E-11  4.9501E-11  2.2406E-09
  3.3966E-11  3.9487E-09  7.7811E-13  3.4470E-09  5.6033E-09  2.6208E-07
  7.1906E-15  7.7811E-13  4.9010E-13  1.6210E-13  1.1711E-12  4.7034E-11
  2.9472E-11  3.4470E-09  1.6210E-13  3.0979E-09  4.7965E-09  2.3549E-07
  4.9501E-11  5.6033E-09  1.1711E-12  4.7965E-09  8.0588E-09  3.6466E-07
  2.2406E-09  2.6208E-07  4.7034E-11  2.3549E-07  3.6466E-07  1.7905E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
  -11.942272 -163.109675    0.232088   -0.200226   -0.947256  2456740.715758
# Heliocentric elements and errors
Epoch:              2456740.5000  =  2014/03/24
Mean Anomaly:          304.05341 +/-    19.107
Argument of Peri:       75.71491 +/-     2.933
Long of Asc Node:      210.31452 +/-     0.032
Inclination:            41.15294 +/-     0.070
Eccentricity:         0.33078501 +/-    0.2191
Semi-Major Axis:     52.76060529 +/-    8.9506
Time of Perihelion: 2478494.2539 +/-    4955.3
Perihelion:          35.30818778 +/-   13.0179
Aphelion:            70.21302280 +/-   16.5972
Period (y)              383.2418 +/-     97.52
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -45.04501764 +/-    0.1861
Ecliptic Y          -13.43289268 +/-    0.0565
Ecliptic Z           -9.73629270 +/-    0.0411
Ecliptic XDOT         0.00101190 +/-    0.0005
Ecliptic YDOT        -0.00166928 +/-    0.0002
Ecliptic ZDOT         0.00170583 +/-    0.0001
# Distances at JD0 (AU)
Heliocenter to KBO   48.00303756 +/-    0.1755
Geocenter to KBO     47.05402090 +/-    0.1988
# Hcoef:  6.81

The following table shows the complete astrometric record for 15HA197. 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 (15HA197) followed by the observatory code and reference code for the source of the astrometry.

2014 03  24.21498  12 43 10.657  -17 37 59.06  23.2R 15HA197   807  C~1MjT      
2014 03  24.28437  12 43 10.366  -17 37 56.92        15HA197   807  C~1MjT      
2014 03  25.28547  12 43 06.272  -17 37 28.17        15HA197   807  C~1MjT      
2015 04  18.07032  12 45 55.37   -17 06 15.7         15HA197   W84  C~2zsQ      
2015 04  21.06171  12 45 43.55   -17 04 30.7   23.7V 15HA197   W84  C~2zsQ      
2015 04  22.06118  12 45 39.66   -17 03 55.2         15HA197   W84  C~2zsQ      

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     0.05       0.00    -0.04
     2   0.0002     -4.67    -0.05       0.30     0.08
     3   0.0029    -69.81    -0.01       3.28    -0.03
     4   1.0674   1406.56    -0.00    2684.39     0.01
     5   1.0756   1209.34    -0.01    2713.65    -0.10
     6   1.0783   1144.05     0.01    2724.13     0.09

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.

15HA197    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