Orbit Fit and Astrometric record for 14SM350

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: 14SM350   
# Created Wed Nov 27 02:09:58 2024
# Orbit generated from Bernstein formalism
# Fitting      7 observations of      7
# Arc:  60.00d
# First observation: 2014/09/21
#  Last observation: 2014/11/20
Preliminary a, adot, b, bdot, g, gdot:
  -0.000001   0.013962   0.000003  -0.008266   0.018970   0.000000
# WARNING Fitting with energy constraint
# Chi-squared of fit:     1.91 DOF:      9 RMS:  0.09
# Min/Max residuals:    -0.17    0.16
# Exact a, adot, b, bdot, g, gdot:
  9.706175E-06  1.174112E-02 -6.118451E-06 -7.951149E-03  1.862716E-02 -7.652237E-03
# Covariance matrix:
  5.1344E-13  2.1401E-11  1.9949E-14 -3.7207E-12  4.4721E-12 -5.2360E-10
  2.1401E-11  2.1686E-08  1.9949E-11 -2.9301E-09  2.9917E-09 -8.4414E-07
  1.9949E-14  1.9949E-11  4.5226E-13 -5.8768E-12  2.7015E-12 -8.0115E-10
 -3.7207E-12 -2.9301E-09 -5.8768E-12  4.4570E-10 -4.1315E-10  1.1101E-07
  4.4721E-12  2.9917E-09  2.7015E-12 -4.1315E-10  4.3578E-10 -1.0768E-07
 -5.2360E-10 -8.4414E-07 -8.0115E-10  1.1101E-07 -1.0768E-07  3.6601E-05
#      lat0       lon0       xBary       yBary       zBary        JD0
   -9.967972  -17.287892   -0.261196   -0.168142   -0.957492  2456921.587018
# Heliocentric elements and errors
Epoch:              2456920.5000  =  2014/09/20
Mean Anomaly:          301.22339 +/-    42.707
Argument of Peri:      311.94046 +/-    18.736
Long of Asc Node:      148.83639 +/-     0.200
Inclination:            35.21323 +/-     0.374
Eccentricity:         0.47564634 +/-    0.3075
Semi-Major Axis:     56.53582836 +/-   22.2703
Time of Perihelion: 2482270.9743 +/-   10719.6
Perihelion:          29.64476831 +/-   20.9404
Aphelion:            83.42688840 +/-   37.1769
Period (y)              425.1027 +/-    251.18
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           51.48950651 +/-    0.0566
Ecliptic Y          -15.75055050 +/-    0.0176
Ecliptic Z           -9.29308686 +/-    0.0104
Ecliptic XDOT        -0.00074271 +/-    0.0008
Ecliptic YDOT         0.00203252 +/-    0.0003
Ecliptic ZDOT        -0.00095623 +/-    0.0002
# Distances at JD0 (AU)
Heliocenter to KBO   54.64074108 +/-    0.0536
Geocenter to KBO     53.68503896 +/-    0.0602
# Hcoef:  7.43

The following table shows the complete astrometric record for 14SM350. 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 (14SM350) followed by the observatory code and reference code for the source of the astrometry.

2014 09  21.08624  23 12 02.930  -15 58 34.37  24.7r 14SM350   807  C~1x8m      
2014 09  21.17603  23 12 02.592  -15 58 36.28        14SM350   807  C~1x8m      
2014 09  21.24113  23 12 02.358  -15 58 37.94        14SM350   807  C~1x8m      
2014 10  22.11564  23 10 24.845  -16 07 53.65        14SM350   304  C~1x8m      
2014 10  22.18678  23 10 24.654  -16 07 54.86        14SM350   304  C~1x8m      
2014 11  19.08101  23 09 35.773  -16 10 12.15        14SM350   304  C~1x8m      
2014 11  20.08150  23 09 34.952  -16 10 10.04        14SM350   304  C~1x8m      

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    -0.13
     2   0.0002     -5.23    -0.02       0.17     0.13
     3   0.0004     -8.99    -0.04      -0.02     0.00
     4   0.0850  -1519.90     0.11      43.30     0.16
     5   0.0851  -1522.91    -0.11      43.27    -0.17
     6   0.1615  -2224.57    -0.01     193.66    -0.01
     7   0.1643  -2234.62     0.00     200.24     0.01

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.

14SM350    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