Orbit Fit and Astrometric record for 14SU349

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: 14SU349   
# Created Sun Apr 21 01:16:13 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:   1.16y
# First observation: 2014/09/18
#  Last observation: 2015/11/15
Preliminary a, adot, b, bdot, g, gdot:
  -0.000003   0.012089  -0.000002   0.001075   0.016748   0.000000
# Chi-squared of fit:     5.74 DOF:      8 RMS:  0.16
# Min/Max residuals:    -0.21    0.39
# Exact a, adot, b, bdot, g, gdot:
  1.204121E-05  1.214563E-02 -8.742689E-07  1.100299E-03  1.684460E-02  9.145475E-03
# Covariance matrix:
  5.0925E-13  5.5408E-13 -7.7544E-14  2.5362E-12  3.1626E-12  1.0179E-09
  5.5408E-13  4.5962E-12 -3.7579E-13  1.2599E-11  1.5032E-11  5.0394E-09
 -7.7544E-14 -3.7579E-13  3.6435E-13 -2.0629E-12 -1.8762E-12 -7.0221E-10
  2.5362E-12  1.2599E-11 -2.0629E-12  6.4859E-11  6.6330E-11  2.5359E-08
  3.1626E-12  1.5032E-11 -1.8762E-12  6.6330E-11  7.1763E-11  2.6347E-08
  1.0179E-09  5.0394E-09 -7.0221E-10  2.5359E-08  2.6347E-08  1.0046E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
  -23.605117   11.175459    0.279423   -0.387427   -0.886952  2456918.835828
# Heliocentric elements and errors
Epoch:              2456910.5000  =  2014/09/10
Mean Anomaly:           33.99188 +/-    21.975
Argument of Peri:      172.44084 +/-     5.924
Long of Asc Node:       89.06588 +/-     0.157
Inclination:            23.68586 +/-     0.012
Eccentricity:         0.62747305 +/-    0.1971
Semi-Major Axis:     79.68700847 +/-   32.5529
Time of Perihelion: 2432377.4053 +/-    5053.8
Perihelion:          29.68555814 +/-   19.8437
Aphelion:           129.68845881 +/-   55.2584
Period (y)              711.3601 +/-    435.90
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           54.36849572 +/-    0.0268
Ecliptic Y           10.45879976 +/-    0.0053
Ecliptic Z          -23.77213725 +/-    0.0119
Ecliptic XDOT         0.00101921 +/-    0.0005
Ecliptic YDOT         0.00221000 +/-    0.0001
Ecliptic ZDOT        -0.00043124 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   60.25308564 +/-    0.0247
Geocenter to KBO     59.36620974 +/-    0.0299
# Hcoef:  7.14

The following table shows the complete astrometric record for 14SU349. 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 (14SU349) followed by the observatory code and reference code for the source of the astrometry.

2014 09  18.33505  01 18 52.787  -17 15 43.73        14SU349   807  C~1x8l      
2014 09  21.30612  01 18 43.59   -17 16 59.6         14SU349   W84  C~2gaD      
2014 09  22.31750  01 18 40.39   -17 17 24.9   25.0V 14SU349   W84  C~2gaD      
2014 09  22.39605  01 18 40.14   -17 17 26.8         14SU349   W84  C~2gaD      
2014 11  19.15759  01 15 31.718  -17 29 33.31        14SU349   304  C~1x8l      
2015 11  14.27733  01 18 18.716  -17 09 26.47        14SU349   304  C~1x8l      
2015 11  15.27362  01 18 15.826  -17 09 27.07        14SU349   304  C~1x8l      

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    -0.13       0.00     0.39
     2   0.0081   -151.23     0.09     -15.43    -0.11
     3   0.0109   -203.40    -0.01     -19.80    -0.21
     4   0.0111   -207.45     0.04     -20.08    -0.20
     5   0.1693  -2967.19     0.02     412.63     0.15
     6   1.1552   -291.60     0.15     543.71    -0.07
     7   1.1579   -329.66    -0.16     560.06     0.05

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.

14SU349    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