Orbit Fit and Astrometric record for 13TS228

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: 13TS228   
# Created Fri May  3 01:15:29 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     27 observations of     27
# Arc:   6.05y
# First observation: 2013/10/13
#  Last observation: 2019/11/01
# Chi-squared of fit:     6.32 DOF:     48 RMS:  0.09
# Min/Max residuals:    -0.14    0.24
# Exact a, adot, b, bdot, g, gdot:
  1.558969E-05  2.408351E-02  3.191789E-07 -1.971917E-04  2.440578E-02  1.738801E-04
# Covariance matrix:
  2.8236E-13 -1.3121E-13 -1.3076E-15  7.7900E-16  1.1261E-13 -6.5336E-13
 -1.3121E-13  1.4683E-13  9.1612E-16 -1.0901E-15 -1.2967E-14  9.8188E-13
 -1.3076E-15  9.1612E-16  1.9175E-13 -3.9578E-14 -2.5828E-15  6.3759E-15
  7.7900E-16 -1.0901E-15 -3.9578E-14  1.1416E-14  2.5434E-16 -7.8876E-15
  1.1261E-13 -1.2967E-14 -2.5828E-15  2.5434E-16  3.7797E-13 -5.3801E-14
 -6.5336E-13  9.8188E-13  6.3759E-15 -7.8876E-15 -5.3801E-14  7.1234E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
   -1.511158    6.317722   -0.229151   -0.025487   -0.970411  2456578.612868
# Heliocentric elements and errors
Epoch:              2456578.5000  =  2013/10/13
Mean Anomaly:           16.36804 +/-     0.152
Argument of Peri:      235.05921 +/-     0.164
Long of Asc Node:      114.00899 +/-     0.009
Inclination:             1.54673 +/-     0.000
Eccentricity:         0.03570441 +/-    0.0001
Semi-Major Axis:     43.42781728 +/-    0.0049
Time of Perihelion: 2451825.7538 +/-      44.0
Perihelion:          41.87725276 +/-    0.0064
Aphelion:            44.97838179 +/-    0.0067
Period (y)              286.1938 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           41.64996575 +/-    0.0010
Ecliptic Y            4.84491533 +/-    0.0001
Ecliptic Z           -1.08056683 +/-    0.0000
Ecliptic XDOT        -0.00028467 +/-    0.0000
Ecliptic YDOT         0.00268593 +/-    0.0000
Ecliptic ZDOT        -0.00002249 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.94472457 +/-    0.0010
Geocenter to KBO     40.97393226 +/-    0.0010
# Hcoef:  7.63

The following table shows the complete astrometric record for 13TS228. 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 (13TS228) followed by the observatory code and reference code for the source of the astrometry.

2013 10  13.11209  00 25 35.566  +01 07 15.08  23.0i 13TS228   W84  C~52Rg      
2013 10  28.07505  00 24 34.076  +01 00 50.13  23.8r 13TS228   W84  C~52Rg      
2013 11  22.09533  00 23 15.815  +00 53 02.51  23.2r 13TS228   W84  C~52Rg      
2013 11  22.09673  00 23 15.800  +00 53 02.67  23.6i 13TS228   W84  C~52Rg      
2013 11  23.10780  00 23 13.519  +00 52 49.68  23.8r 13TS228   W84  C~52Rg      
2013 11  23.10919  00 23 13.517  +00 52 49.60  24.6i 13TS228   W84  C~52Rg      
2014 10  28.18822  00 29 38.900  +01 32 53.26  23.8r 13TS228   W84  C~52Rg      
2016 09  09.28058  00 43 16.156  +02 58 51.61  23.7r 13TS228   W84  C~52Rg      
2016 09  09.28195  00 43 16.141  +02 58 51.65  23.3i 13TS228   W84  C~52Rg      
2016 11  08.14374  00 39 03.803  +02 32 14.46  23.3i 13TS228   W84  C~52Rg      
2016 11  18.08134  00 38 32.142  +02 29 07.87  23.5r 13TS228   W84  C~52Rg      
2016 11  26.10227  00 38 11.400  +02 27 10.03  23.8r 13TS228   W84  C~52Rg      
2016 11  26.10867  00 38 11.380  +02 27 09.92  23.6i 13TS228   W84  C~52Rg      
2017 08  28.27853  00 49 05.022  +03 35 29.48  22.9r 13TS228   W84  C~52Rg      
2017 09  27.22811  00 47 05.728  +03 22 24.55  23.6r 13TS228   W84  C~52Rg      
2017 10  22.19674  00 45 15.069  +03 10 47.00  23.3z 13TS228   W84  C~52Rg      
2018 10  10.23758  00 51 13.698  +03 48 01.33  23.6r 13TS228   W84  C~52Rg      
2018 10  18.19756  00 50 38.259  +03 44 20.17  23.5z 13TS228   W84  C~52Rg      
2018 10  18.19894  00 50 38.256  +03 44 20.18  23.7i 13TS228   W84  C~52Rg      
2018 11  26.07249  00 48 16.444  +03 30 13.07  23.4r 13TS228   W84  C~52Rg      
2018 11  26.07387  00 48 16.445  +03 30 13.04  23.9g 13TS228   W84  C~52Rg      
2019 11  01.28144  00 54 44.60   +04 09 53.7   25.4g 13TS228   T09  C~7bIF      
2019 11  01.32333  00 54 44.43   +04 09 52.6   24.6g 13TS228   T09  C~7bIF      
2019 11  01.33611  00 54 44.37   +04 09 52.4   24.8g 13TS228   T09  C~7bIF      
2019 11  01.34476  00 54 44.35   +04 09 52.0   24.8g 13TS228   T09  C~7bIF      
2019 11  01.42395  00 54 44.01   +04 09 50.0   25.0g 13TS228   T09  C~7bIF      
2019 11  01.42606  00 54 44.00   +04 09 50.2   25.0g 13TS228   T09  C~7bIF      

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     0.04       0.00    -0.08
     2   0.0410      0.00    -0.12       0.00    -0.01
     3   0.1095      0.00     0.14       0.00    -0.01
     4   0.1095      0.00    -0.04       0.00     0.17
     5   0.1122      0.00    -0.03       0.00    -0.00
     6   0.1122      0.00    -0.01       0.00    -0.06
     7   1.0406      0.00    -0.05       0.00     0.24
     8   2.9081      0.00     0.15       0.00    -0.06
     9   2.9081      0.00     0.00       0.00     0.01
    10   3.0720      0.00    -0.01       0.00     0.06
    11   3.0992      0.00    -0.08       0.00     0.00
    12   3.1211      0.00     0.08       0.00    -0.11
    13   3.1211      0.00     0.01       0.00    -0.14
    14   3.8745      0.00    -0.03       0.00    -0.06
    15   3.9565      0.00     0.02       0.00    -0.13
    16   4.0249      0.00     0.09       0.00    -0.04
    17   4.9914      0.00    -0.03       0.00     0.15
    18   5.0132      0.00    -0.05       0.00     0.01
    19   5.0132      0.00    -0.01       0.00     0.06
    20   5.1197      0.00     0.02       0.00    -0.06
    21   5.1197      0.00     0.09       0.00    -0.07
    22   6.0511      0.00    -0.03       0.00     0.10
    23   6.0512      0.00     0.02       0.00     0.02
    24   6.0513      0.00    -0.09       0.00     0.13
    25   6.0513      0.00     0.15       0.00    -0.06
    26   6.0515      0.00    -0.05       0.00    -0.13
    27   6.0515      0.00    -0.07       0.00     0.12

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.

13TS228    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.686    43.686    43.686
ecceobj         0.042     0.042     0.042
incobj          1.546     1.546     1.546
qmin           40.838    40.868    40.865
qmax           46.241    46.167    46.227
amean          43.447    43.445    43.447
amin           43.111    43.106    43.111
amax           43.788    43.783    43.787
emean           0.040     0.039     0.040
emin            0.021     0.020     0.021
emax            0.056     0.055     0.056
imean           1.217     1.216     1.221
imin            0.176     0.176     0.176
imax            1.838     1.835     1.847
excite_mean     0.046     0.045     0.046
fracstop        1.000     1.000     1.000
cjmean          3.092     3.092     3.092

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       180.8     180.7     181.3
kozaiamp        180.0     179.9     179.9