Orbit Fit and Astrometric record for 17BG231

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: 17BG231   
# Created Fri Nov 22 02:10:48 2024
# Orbit generated from Bernstein formalism
# Fitting     23 observations of     23
# Arc:   0.97y
# First observation: 2017/01/26
#  Last observation: 2018/01/17
Preliminary a, adot, b, bdot, g, gdot:
  -0.000000   0.020294  -0.000002  -0.010592   0.023631   0.000000
# Chi-squared of fit:    17.90 DOF:     40 RMS:  0.16
# Min/Max residuals:    -0.35    0.30
# Exact a, adot, b, bdot, g, gdot:
  1.298081E-05  2.043272E-02 -6.306747E-06 -1.065332E-02  2.362974E-02  4.390739E-03
# Covariance matrix:
  1.2064E-13  4.7028E-13  9.7657E-15 -2.8916E-13  3.4034E-13  2.7808E-11
  4.7028E-13  2.0451E-10  2.8053E-12 -9.4022E-11  5.2524E-11  9.1782E-09
  9.7657E-15  2.8053E-12  1.2151E-13 -1.3915E-12  7.3275E-13  1.2633E-10
 -2.8916E-13 -9.4022E-11 -1.3915E-12  4.3852E-11 -2.4355E-11 -4.2316E-09
  3.4034E-13  5.2524E-11  7.3275E-13 -2.4355E-11  1.4564E-11  2.3752E-09
  2.7808E-11  9.1782E-09  1.2633E-10 -4.2316E-09  2.3752E-09  4.1305E-07
#      lat0       lon0       xBary       yBary       zBary        JD0
  -12.483662  151.500258    0.420851   -0.192589   -0.870695  2457780.038741
# Heliocentric elements and errors
Epoch:              2457780.5000  =  2017/01/27
Mean Anomaly:           55.04799 +/-     1.113
Argument of Peri:      129.57654 +/-     1.739
Long of Asc Node:      308.91000 +/-     0.003
Inclination:            30.02063 +/-     0.003
Eccentricity:         0.19186770 +/-    0.0287
Semi-Major Axis:     47.00340644 +/-    0.5993
Time of Perihelion: 2439782.2039 +/-     117.8
Perihelion:          37.98497074 +/-    1.4318
Aphelion:            56.02184214 +/-    1.5250
Period (y)              322.2569 +/-      6.16
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -36.89834850 +/-    0.0059
Ecliptic Y           20.50630326 +/-    0.0032
Ecliptic Z           -9.14812725 +/-    0.0015
Ecliptic XDOT        -0.00132880 +/-    0.0001
Ecliptic YDOT        -0.00197755 +/-    0.0000
Ecliptic ZDOT        -0.00131519 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   43.19357391 +/-    0.0052
Geocenter to KBO     42.31955684 +/-    0.0068
# Hcoef:  8.02

The following table shows the complete astrometric record for 17BG231. 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 (17BG231) followed by the observatory code and reference code for the source of the astrometry.

2017 01  26.53794  09 56 25.33   -00 44 43.6   23.8z 17BG231   T09  C~7xTl      
2017 01  26.54133  09 56 25.33   -00 44 43.4   24.2z 17BG231   T09  C~7xTl      
2017 01  26.55080  09 56 25.26   -00 44 43.1   23.9z 17BG231   T09  C~7xTl      
2017 01  26.56693  09 56 25.19   -00 44 43.1   23.9z 17BG231   T09  C~7xTl      
2017 01  26.58033  09 56 25.13   -00 44 42.9   24.2z 17BG231   T09  C~7xTl      
2017 01  26.58570  09 56 25.11   -00 44 42.9   24.7z 17BG231   T09  C~7xTl      
2017 01  26.59646  09 56 25.07   -00 44 43.1   24.2z 17BG231   T09  C~7xTl      
2017 01  26.59916  09 56 25.07   -00 44 42.7   24.6z 17BG231   T09  C~7xTl      
2017 01  26.60996  09 56 24.98   -00 44 42.6   24.1z 17BG231   T09  C~7xTl      
2017 02  02.37330  09 55 54.48   -00 43 24.9   24.4r 17BG231   T09  C~7xTl      
2017 02  02.37546  09 55 54.48   -00 43 25.1   24.3r 17BG231   T09  C~7xTl      
2017 02  02.39743  09 55 54.38   -00 43 24.4   24.1r 17BG231   T09  C~7xTl      
2017 02  02.41063  09 55 54.31   -00 43 24.2   24.1r 17BG231   T09  C~7xTl      
2017 02  02.42609  09 55 54.23   -00 43 24.2   24.4r 17BG231   T09  C~7xTl      
2017 03  06.37764  09 53 25.15   -00 33 22.4   23.8i 17BG231   T09  C~7xTl      
2017 03  06.44451  09 53 24.85   -00 33 21.3   24.2i 17BG231   T09  C~7xTl      
2017 03  06.44718  09 53 24.82   -00 33 20.6   24.1i 17BG231   T09  C~7xTl      
2017 03  06.45254  09 53 24.81   -00 33 20.6   23.9i 17BG231   T09  C~7xTl      
2017 03  06.46600  09 53 24.73   -00 33 20.2   23.9i 17BG231   T09  C~7xTl      
2018 01  17.46995  10 00 35.71   -01 44 27.2   23.8i 17BG231   T09  C~7xTl      
2018 01  17.52652  10 00 35.48   -01 44 27.0   24.5i 17BG231   T09  C~7xTl      
2018 01  17.55341  10 00 35.38   -01 44 27.0   24.6i 17BG231   T09  C~7xTl      
2018 01  17.57759  10 00 35.26   -01 44 26.9   24.5i 17BG231   T09  C~7xTl      

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     0.14       0.00    -0.17
     2   0.0000     -0.07     0.30       0.19     0.07
     3   0.0000     -1.16    -0.16       0.10     0.12
     4   0.0001     -2.14    -0.07      -0.27    -0.02
     5   0.0001     -3.06    -0.09      -0.39     0.04
     6   0.0001     -3.34    -0.02      -0.50     0.02
     7   0.0002     -3.83     0.20      -0.89    -0.23
     8   0.0002     -3.97     0.24      -0.52     0.18
     9   0.0002     -5.27    -0.34      -0.90    -0.04
    10   0.0187   -461.03    -0.10     -88.04    -0.06
    11   0.0187   -460.96     0.12     -88.23    -0.22
    12   0.0188   -462.61     0.01     -88.09     0.18
    13   0.0188   -463.66    -0.12     -88.27     0.16
    14   0.0189   -464.78    -0.15     -88.69    -0.07
    15   0.1063  -2770.28     0.11    -306.83     0.04
    16   0.1065  -2774.88     0.29    -307.38    -0.35
    17   0.1065  -2775.55    -0.18    -306.88     0.15
    18   0.1065  -2775.69     0.06    -306.93     0.11
    19   0.1066  -2776.96    -0.24    -306.98     0.09
    20   0.9745   4771.33    -0.00   -2046.03     0.09
    21   0.9746   4768.03    -0.01   -2047.05     0.05
    22   0.9747   4766.62     0.16   -2047.57    -0.01
    23   0.9748   4764.90    -0.15   -2048.11    -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.

17BG231    quality flag:2

Type:       SCATEXTD  SCATNEAR  SCATEXTD

axisobj        46.889    49.103    45.373
ecceobj         0.196     0.272     0.119
incobj         30.043    30.034    30.051
qmin           36.875    34.687    39.325
qmax           57.298    63.814    51.723
amean          46.852    49.015    45.373
amin           46.452    48.570    45.015
amax           47.312    49.582    45.759
emean           0.193     0.269     0.116
emin            0.176     0.249     0.103
emax            0.211     0.289     0.131
imean          31.456    31.447    31.485
imin           31.132    31.052    31.189
imax           31.862    32.017    31.771
excite_mean     0.556     0.587     0.535
fracstop        1.000     1.000     1.000
cjmean          2.731     2.711     2.743

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       186.4     197.9     182.5
kozaiamp        179.9     180.0     180.0