Orbit Fit and Astrometric record for 13SO107

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: 13SO107   
# Created Sat Apr 20 01:15:09 2024
# Orbit generated from Bernstein formalism
# Fitting     23 observations of     23
# Arc:   1.15y
# First observation: 2012/09/17
#  Last observation: 2013/11/10
Preliminary a, adot, b, bdot, g, gdot:
   0.006500   0.713984  -0.002858   0.335821   0.260445   0.000000
# Chi-squared of fit:    84.53 DOF:     40 RMS:  0.34
# Min/Max residuals:    -1.03    0.76
# Exact a, adot, b, bdot, g, gdot:
  4.425715E-05  6.183444E-01  2.095235E-05  2.879229E-01  2.280742E-01 -7.766306E-03
# Covariance matrix:
  2.5030E-13  1.0564E-13 -9.8264E-15  1.6527E-13  1.3442E-13  4.2773E-13
  1.0564E-13  4.1561E-11 -1.2888E-12  2.2138E-11  8.8036E-12  5.7751E-11
 -9.8264E-15 -1.2888E-12  2.7326E-13 -9.0994E-13 -2.7337E-13 -1.8026E-12
  1.6527E-13  2.2138E-11 -9.0994E-13  1.2130E-11  4.6800E-12  3.0969E-11
  1.3442E-13  8.8036E-12 -2.7337E-13  4.6800E-12  2.1656E-12  1.2194E-11
  4.2773E-13  5.7751E-11 -1.8026E-12  3.0969E-11  1.2194E-11  8.0797E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.434239   12.394315    0.307624   -0.007231   -0.954998  2456187.852478
# Heliocentric elements and errors
Epoch:              2456180.5000  =  2012/09/10
Mean Anomaly:          346.99558 +/-     0.003
Argument of Peri:       19.30834 +/-     0.004
Long of Asc Node:        9.88041 +/-     0.000
Inclination:            24.99266 +/-     0.000
Eccentricity:         0.22217979 +/-    0.0000
Semi-Major Axis:      6.80249446 +/-    0.0001
Time of Perihelion: 2456414.5934 +/-       0.1
Perihelion:           5.29111770 +/-    0.0001
Aphelion:             8.31387122 +/-    0.0001
Period (y)               17.7423 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X            5.28290338 +/-    0.0000
Ecliptic Y            0.84803999 +/-    0.0000
Ecliptic Z           -0.03311702 +/-    0.0000
Ecliptic XDOT        -0.00166450 +/-    0.0000
Ecliptic YDOT         0.00723782 +/-    0.0000
Ecliptic ZDOT         0.00345702 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO    5.35063890 +/-    0.0000
Geocenter to KBO      4.38453866 +/-    0.0000
# Hcoef: 14.19

The following table shows the complete astrometric record for 13SO107. 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 (13SO107) followed by the observatory code and reference code for the source of the astrometry.

2012 09  17.35170  00 46 16.64   +04 29 52.4   21.1V 13SO107   G96  C~3znM      
2012 09  17.36088  00 46 16.35   +04 29 52.6   21.3V 13SO107   G96  C~3znM      
2012 09  17.37013  00 46 16.10   +04 29 52.6   20.9V 13SO107   G96  C~3znM      
2012 09  17.37941  00 46 15.78   +04 29 51.9   21.7V 13SO107   G96  C~3znM      
2012 11  04.244523 00 22 09.563  +04 14 11.69  21.8w 13SO107   F51  c~3znM      
2012 11  04.258630 00 22 09.221  +04 14 11.90  21.7w 13SO107   F51  c~3znM      
2012 11  04.272724 00 22 08.879  +04 14 12.18  21.8w 13SO107   F51  c~3znM      
2013 09  16.41991  02 43 50.09   +31 07 10.4   21.6V 13SO107   G96  C~3znM      
2013 09  16.42624  02 43 50.01   +31 07 11.3   21.5V 13SO107   G96  C~3znM      
2013 09  16.43248  02 43 49.90   +31 07 12.6   21.6V 13SO107   G96  C~3znM      
2013 09  16.43868  02 43 49.80   +31 07 14.3   21.4V 13SO107   G96  C~3znM      
2013 09  30.40140  02 39 06.04   +31 52 24.8   21.5V 13SO107   G96  C~3znM      
2013 09  30.41052  02 39 05.82   +31 52 26.5   21.6V 13SO107   G96  C~3znM      
2013 09  30.41963  02 39 05.57   +31 52 27.8   21.5V 13SO107   G96  C~3znM      
2013 09  30.42873  02 39 05.32   +31 52 29.1   21.4V 13SO107   G96  C~3znM      
2013 10  30.30284  02 22 30.03   +32 32 43.1   21.2V 13SO107   G96  C~3znM      
2013 10  30.30912  02 22 29.73   +32 32 43.6   22.0V 13SO107   G96  C~3znM      
2013 10  30.31623  02 22 29.41   +32 32 44.0   22.0V 13SO107   G96  C~3znM      
2013 10  30.32250  02 22 29.19   +32 32 43.6   22.2V 13SO107   G96  C~3znM      
2013 11  10.13270  02 15 44.97   +32 27 42.8   21.1V 13SO107   G96  C~3znM      
2013 11  10.13961  02 15 44.68   +32 27 41.9   21.3V 13SO107   G96  C~3znM      
2013 11  10.14650  02 15 44.41   +32 27 42.1   21.4V 13SO107   G96  C~3znM      
2013 11  10.15340  02 15 44.19   +32 27 41.5   21.5V 13SO107   G96  C~3znM      

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    -0.29       0.00    -0.20
     2   0.0000     -3.92    -0.24       1.87     0.16
     3   0.0001     -7.36     0.31       3.33     0.09
     4   0.0001    -12.04    -0.36       4.55    -0.22
     5   0.1311 -20342.57     0.35    7678.52    -0.03
     6   0.1312 -20347.23     0.18    7680.77     0.06
     7   0.1312 -20351.87     0.05    7683.08     0.21
     8   0.9968 148592.40     0.18   67576.68     0.68
     9   0.9968 148591.31     0.28   67578.06    -0.06
    10   0.9968 148589.85    -0.01   67580.05    -0.16
    11   0.9968 148588.77     0.08   67582.54     0.26
    12   1.0350 144563.84    -0.20   71856.12    -0.26
    13   1.0351 144560.57     0.30   71858.90    -0.00
    14   1.0351 144556.54     0.04   71861.22    -0.20
    15   1.0351 144552.51    -0.22   71863.54    -0.39
    16   1.1169 127882.23     0.76   77557.36    -1.03
    17   1.1169 127877.30     0.02   77558.83    -0.21
    18   1.1169 127871.98    -0.57   77560.22     0.45
    19   1.1170 127867.98    -0.38   77560.29    -0.11
    20   1.1466 120844.59     0.43   78308.87     0.47
    21   1.1466 120839.28    -0.42   78308.56    -0.16
    22   1.1466 120834.86    -0.39   78309.61     0.57
    23   1.1466 120830.87     0.09   78309.48     0.13

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.

13SO107    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj         6.762     6.762     6.761
ecceobj         0.218     0.218     0.218
incobj         25.079    25.079    25.080
qmin            5.042     5.025     4.903
qmax            8.487     8.546     8.618
amean           6.723     6.774     6.735
amin            6.642     6.762     6.674
amax            6.764     6.785     6.761
emean           0.235     0.239     0.241
emin            0.218     0.218     0.218
emax            0.255     0.259     0.275
imean          25.147    25.179    25.177
imin           25.049    25.026    25.013
imax           25.333    25.333    25.333
excite_mean     0.486     0.488     0.489
fracstop        0.000     0.000     0.000
cjmean          5.300     5.266     5.298

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       242.9     189.8     267.7
kozaiamp        169.4     169.3     169.6