Orbit Fit and Astrometric record for 08TA239

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: 08TA239   
# Created Sat May  4 01:13:16 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     20 observations of     20
# Arc:  12.26y
# First observation: 2007/11/09
#  Last observation: 2020/02/11
# Chi-squared of fit:    29.57 DOF:     34 RMS:  0.21
# Min/Max residuals:    -0.49    0.76
# Exact a, adot, b, bdot, g, gdot:
  1.790993E-05  3.134761E-02  2.076225E-07  3.166243E-04  2.856866E-02 -9.298761E-04
# Covariance matrix:
  3.2183E-13  4.0259E-15 -1.5983E-14  1.9806E-14 -3.4026E-13  1.5577E-13
  4.0259E-15  5.0579E-13 -7.2457E-14  7.4247E-14 -8.1968E-13  1.5873E-12
 -1.5983E-14 -7.2457E-14  1.5146E-13 -2.7398E-14  1.4079E-13 -2.3604E-13
  1.9806E-14  7.4247E-14 -2.7398E-14  1.6519E-14 -1.5011E-13  2.4365E-13
 -3.4026E-13 -8.1968E-13  1.4079E-13 -1.5011E-13  1.8644E-12 -2.7531E-12
  1.5577E-13  1.5873E-12 -2.3604E-13  2.4365E-13 -2.7531E-12  5.0697E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
  -33.119531   36.261439   -0.182059   -0.534124   -0.818901  2454414.041677
# Heliocentric elements and errors
Epoch:              2454414.5000  =  2007/11/10
Mean Anomaly:          346.92634 +/-     0.064
Argument of Peri:      287.11077 +/-     0.076
Long of Asc Node:      125.04732 +/-     0.000
Inclination:            32.27704 +/-     0.000
Eccentricity:         0.09319439 +/-    0.0002
Semi-Major Axis:     39.37838387 +/-    0.0102
Time of Perihelion: 2457692.2808 +/-      37.5
Perihelion:          35.70853923 +/-    0.0115
Aphelion:            43.04822850 +/-    0.0131
Period (y)              247.1127 +/-      0.10
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           24.31845752 +/-    0.0011
Ecliptic Y           18.06051338 +/-    0.0008
Ecliptic Z          -19.12542399 +/-    0.0009
Ecliptic XDOT        -0.00181739 +/-    0.0000
Ecliptic YDOT         0.00238692 +/-    0.0000
Ecliptic ZDOT         0.00007400 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   35.82390781 +/-    0.0010
Geocenter to KBO     35.00343426 +/-    0.0017
# Hcoef:  7.58

The following table shows the complete astrometric record for 08TA239. 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 (08TA239) followed by the observatory code and reference code for the source of the astrometry.

2007 11  09.540923 02 59 24.42   -17 42 47.3   23.3i 08TA239   T14  C~66zf      
2008 10  02.276794 03 09 39.606  -16 43 20.72  23.3r 08TA239   309  C~66zf      
2008 10  02.278257 03 09 39.601  -16 43 20.75  23.3r 08TA239   309  C~66zf      
2008 10  02.282302 03 09 39.590  -16 43 20.94        08TA239   309  C~66zf      
2008 10  02.286132 03 09 39.568  -16 43 21.11        08TA239   309  C~66zf      
2008 10  02.289991 03 09 39.556  -16 43 21.27        08TA239   309  C~66zf      
2008 10  02.293829 03 09 39.541  -16 43 21.49        08TA239   309  C~66zf      
2008 10  02.297684 03 09 39.530  -16 43 21.69        08TA239   309  C~66zf      
2008 10  07.611547 03 09 16.78   -16 47 25.9   23.5g 08TA239   T14  C~66zf      
2008 10  07.617029 03 09 16.75   -16 47 26.4         08TA239   T14  C~66zf      
2008 10  27.22275  03 07 38.02   -16 59 48.6         08TA239   807  C~66zf      
2008 10  27.33402  03 07 37.40   -16 59 52.1         08TA239   807  C~66zf      
2008 11  02.525758 03 07 02.99   -17 02 41.8   22.6i 08TA239   T14  C~66zf      
2008 11  02.532128 03 07 02.94   -17 02 42.0         08TA239   T14  C~66zf      
2014 09  20.356162 03 51 31.69   -12 27 30.1   23.7g 08TA239   W84  C~66zf      
2014 09  20.357528 03 51 31.69   -12 27 30.4   23.2r 08TA239   W84  C~66zf      
2014 09  20.358903 03 51 31.70   -12 27 30.1   22.9z 08TA239   W84  C~66zf      
2020 02  11.078482 04 15 00.34   -08 52 06.5   22.5i 08TA239   W84  C~66zf      
2020 02  11.123487 04 15 00.32   -08 52 04.1         08TA239   W84  C~66zf      
2020 02  11.125520 04 15 00.31   -08 52 03.9         08TA239   W84  C~66zf      

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    -0.11       0.00    -0.05
     2   0.8973      0.00    -0.10       0.00    -0.06
     3   0.8973      0.00    -0.08       0.00    -0.02
     4   0.8973      0.00     0.01       0.00    -0.01
     5   0.8973      0.00    -0.08       0.00    -0.00
     6   0.8973      0.00    -0.02       0.00     0.02
     7   0.8973      0.00    -0.01       0.00    -0.02
     8   0.8973      0.00     0.07       0.00    -0.04
     9   0.9119      0.00     0.02       0.00     0.30
    10   0.9119      0.00    -0.05       0.00     0.04
    11   0.9656      0.00    -0.49       0.00     0.15
    12   0.9659      0.00    -0.49       0.00    -0.01
    13   0.9828      0.00     0.76       0.00    -0.02
    14   0.9829      0.00     0.55       0.00    -0.07
    15   6.8633      0.00    -0.01       0.00    -0.14
    16   6.8633      0.00     0.03       0.00    -0.37
    17   6.8633      0.00     0.22       0.00    -0.01
    18  12.2561      0.00    -0.11       0.00     0.04
    19  12.2562      0.00     0.06       0.00     0.07
    20  12.2562      0.00    -0.07       0.00     0.17

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.

08TA239    quality flag:3

Type:           3:2E      3:2E      3:2E

axisobj        39.833    39.833    39.833
ecceobj         0.103     0.103     0.103
incobj         32.267    32.267    32.267
qmin           33.362    33.363    33.361
qmax           45.884    45.884    45.884
amean          39.456    39.456    39.456
amin           39.098    39.098    39.098
amax           39.840    39.840    39.839
emean           0.113     0.113     0.113
emin            0.070     0.070     0.070
emax            0.154     0.154     0.154
imean          30.480    30.480    30.480
imin           29.897    29.897    29.898
imax           31.013    31.013    31.013
excite_mean     0.520     0.520     0.520
fracstop        1.000     1.000     1.000
cjmean          2.724     2.724     2.724

libcent 0       179.7     179.7     179.6
libamp  0        77.6      77.6      77.7
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       180.7     180.7     180.7
kozaiamp        179.9     179.9     179.9