Orbit Fit and Astrometric record for 17BL231

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: 17BL231   
# Created Wed Jul 17 01:11:27 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     27 observations of     27
# Arc:  11.16y
# First observation: 2006/01/05
#  Last observation: 2017/03/06
# Chi-squared of fit:    14.54 DOF:     48 RMS:  0.13
# Min/Max residuals:    -0.40    0.22
# Exact a, adot, b, bdot, g, gdot:
  1.493332E-05  2.096458E-02  6.018014E-06  8.701793E-03  2.230673E-02 -7.927333E-03
# Covariance matrix:
  6.3938E-13 -2.9557E-13  8.5871E-14 -1.0538E-13 -2.7667E-13 -9.1278E-13
 -2.9557E-13  3.2063E-13 -1.0617E-13  1.3027E-13  3.4726E-13  1.1283E-12
  8.5871E-14 -1.0617E-13  4.6809E-13 -8.3422E-14 -1.1402E-13 -3.7887E-13
 -1.0538E-13  1.3027E-13 -8.3422E-14  5.7747E-14  1.3869E-13  4.6509E-13
 -2.7667E-13  3.4726E-13 -1.1402E-13  1.3869E-13  5.7721E-13  1.2000E-12
 -9.1278E-13  1.1283E-12 -3.7887E-13  4.6509E-13  1.2000E-12  4.0285E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
  -20.073915  134.765062    0.493887   -0.292210   -0.800007  2453740.976286
# Heliocentric elements and errors
Epoch:              2453740.5000  =  2006/01/05
Mean Anomaly:          335.65232 +/-     0.009
Argument of Peri:       22.73127 +/-     0.007
Long of Asc Node:      173.30979 +/-     0.000
Inclination:            29.54032 +/-     0.000
Eccentricity:         0.46958262 +/-    0.0001
Semi-Major Axis:     69.77820862 +/-    0.0176
Time of Perihelion: 2468139.5283 +/-      75.5
Perihelion:          37.01157481 +/-    0.0135
Aphelion:           102.54484242 +/-    0.0277
Period (y)              582.8918 +/-      0.22
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -29.90473067 +/-    0.0010
Ecliptic Y           30.84525088 +/-    0.0010
Ecliptic Z          -15.38669161 +/-    0.0005
Ecliptic XDOT        -0.00143879 +/-    0.0000
Ecliptic YDOT        -0.00220685 +/-    0.0000
Ecliptic ZDOT         0.00133710 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.63437575 +/-    0.0010
Geocenter to KBO     44.82980822 +/-    0.0015
# Hcoef:  7.31

The following table shows the complete astrometric record for 17BL231. 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 (17BL231) followed by the observatory code and reference code for the source of the astrometry.

2006 01  05.475532 08 45 52.99   -02 50 44.1         17BL231   T14  C~81Bm      
2006 01  05.536530 08 45 52.75   -02 50 43.7         17BL231   T14  C~81Bm      
2008 01  05.436926 08 56 25.99   -02 33 29.3         17BL231   T14  C~81Bm      
2008 01  05.470824 08 56 25.87   -02 33 29.1         17BL231   T14  C~81Bn      
2016 04  04.244078 09 36 06.15   -00 33 03.2         17BL231   T09  C~81Bn      
2016 04  04.276582 09 36 06.08   -00 33 01.8         17BL231   T09  C~81Bn      
2016 12  25.44915  09 48 29.52   -01 05 55.1   23.8r 17BL231   T09  C~7xTm      
2016 12  25.46448  09 48 29.50   -01 05 55.1   23.6r 17BL231   T09  C~7xTm      
2016 12  25.48961  09 48 29.43   -01 05 55.0   23.8r 17BL231   T09  C~7xTm      
2016 12  25.49171  09 48 29.42   -01 05 55.0   23.7r 17BL231   T09  C~7xTm      
2017 01  26.45718  09 46 38.56   -00 59 13.1   23.3z 17BL231   T09  C~7xTm      
2017 01  26.46663  09 46 38.52   -00 59 12.9   23.3z 17BL231   T09  C~7xTm      
2017 01  26.47468  09 46 38.48   -00 59 13.1   23.0z 17BL231   T09  C~7xTm      
2017 01  26.48271  09 46 38.46   -00 59 12.7   23.0z 17BL231   T09  C~7xTm      
2017 01  26.49344  09 46 38.42   -00 59 12.4   23.2z 17BL231   T09  C~7xTm      
2017 01  26.50952  09 46 38.33   -00 59 12.1   23.0z 17BL231   T09  C~7xTm      
2017 01  28.42233  09 46 30.18   -00 58 29.4   24.6g 17BL231   T09  C~7xTm      
2017 01  28.44025  09 46 30.10   -00 58 28.9   24.3g 17BL231   T09  C~7xTm      
2017 01  28.45292  09 46 30.06   -00 58 28.9   24.3g 17BL231   T09  C~7xTm      
2017 01  28.46760  09 46 29.98   -00 58 28.4   24.2g 17BL231   T09  C~7xTm      
2017 03  04.39457  09 43 55.61   -00 41 00.7   23.2i 17BL231   T09  C~7xTm      
2017 03  04.39993  09 43 55.60   -00 41 00.0   23.1i 17BL231   T09  C~7xTm      
2017 03  04.43238  09 43 55.46   -00 40 59.2   23.0i 17BL231   T09  C~7xTm      
2017 03  06.35845  09 43 47.47   -00 39 50.6   23.0i 17BL231   T09  C~7xTm      
2017 03  06.39997  09 43 47.29   -00 39 49.3   23.0i 17BL231   T09  C~7xTm      
2017 03  06.40280  09 43 47.28   -00 39 49.3   23.1i 17BL231   T09  C~7xTm      
2017 03  06.41622  09 43 47.24   -00 39 48.5   23.1i 17BL231   T09  C~7xTm      

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    -0.01       0.00     0.03
     2   0.0002      0.00     0.01       0.00    -0.04
     3   1.9985      0.00    -0.09       0.00     0.06
     4   1.9986      0.00     0.07       0.00     0.01
     5  10.2444      0.00    -0.03       0.00    -0.40
     6  10.2445      0.00     0.09       0.00    -0.15
     7  10.9705      0.00    -0.07       0.00     0.03
     8  10.9705      0.00     0.21       0.00    -0.01
     9  10.9706      0.00     0.11       0.00     0.02
    10  10.9706      0.00     0.04       0.00     0.01
    11  11.0581      0.00    -0.07       0.00     0.17
    12  11.0582      0.00    -0.06       0.00     0.16
    13  11.0582      0.00    -0.14       0.00    -0.21
    14  11.0582      0.00     0.08       0.00     0.01
    15  11.0582      0.00     0.18       0.00     0.08
    16  11.0583      0.00    -0.13       0.00     0.03
    17  11.0635      0.00    -0.03       0.00     0.09
    18  11.0636      0.00    -0.06       0.00     0.18
    19  11.0636      0.00     0.17       0.00    -0.10
    20  11.0636      0.00    -0.06       0.00     0.06
    21  11.1593      0.00    -0.16       0.00    -0.30
    22  11.1593      0.00     0.03       0.00     0.21
    23  11.1594      0.00     0.01       0.00    -0.14
    24  11.1646      0.00    -0.06       0.00     0.18
    25  11.1647      0.00    -0.15       0.00    -0.00
    26  11.1648      0.00    -0.12       0.00    -0.10
    27  11.1648      0.00     0.13       0.00     0.22

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.

17BL231    quality flag:3

Type:       7:2EEEEE  7:2EEEEE  7:2EEEEE

axisobj        69.235    69.235    69.236
ecceobj         0.463     0.463     0.463
incobj         29.629    29.629    29.629
qmin           36.290    36.286    36.292
qmax          104.480   104.493   104.456
amean          69.408    69.408    69.408
amin           68.416    68.416    68.408
amax           70.786    70.785    70.786
emean           0.461     0.461     0.461
emin            0.445     0.445     0.445
emax            0.478     0.478     0.478
imean          29.313    29.311    29.313
imin           28.658    28.654    28.660
imax           29.760    29.758    29.761
excite_mean     0.672     0.672     0.672
fracstop        1.000     1.000     1.000
cjmean          2.784     2.784     2.784

libcent 0       178.2     178.4     178.7
libamp  0       147.4     147.6     147.8
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       100.4     100.4     100.3
kozaiamp         76.6      76.6      76.6