Orbit Fit and Astrometric record for 17DK170

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: 17DK170   
# Created Tue Apr  1 01:11:05 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     19 observations of     19
# Arc:   5.09y
# First observation: 2014/02/27
#  Last observation: 2019/04/03
# Chi-squared of fit:     7.45 DOF:     32 RMS:  0.11
# Min/Max residuals:    -0.28    0.36
# Exact a, adot, b, bdot, g, gdot:
  1.633486E-05  2.581113E-02 -5.040905E-07 -3.953235E-04  2.520510E-02  1.711297E-05
# Covariance matrix:
  7.3165E-13 -4.5723E-13 -3.9158E-15  4.7001E-15 -2.5970E-14 -2.6370E-12
 -4.5723E-13  4.5221E-13  4.7356E-15 -6.0060E-15  2.2211E-13  3.4790E-12
 -3.9158E-15  4.7356E-15  4.6987E-13 -1.6027E-13  1.5211E-15  4.2303E-14
  4.7001E-15 -6.0060E-15 -1.6027E-13  6.5428E-14 -3.0683E-15 -5.3920E-14
 -2.5970E-14  2.2211E-13  1.5211E-15 -3.0683E-15  7.4629E-13  2.1435E-12
 -2.6370E-12  3.4790E-12  4.2303E-14 -5.3920E-14  2.1435E-12  3.1320E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.348781 -174.588198    0.442743    0.051714   -0.882247  2456716.098874
# Heliocentric elements and errors
Epoch:              2456716.5000  =  2014/02/28
Mean Anomaly:          354.65033 +/-     0.142
Argument of Peri:      110.75069 +/-     0.167
Long of Asc Node:       80.30775 +/-     0.009
Inclination:             3.38270 +/-     0.000
Eccentricity:         0.07996688 +/-    0.0001
Semi-Major Axis:     44.06603382 +/-    0.0062
Time of Perihelion: 2458304.2368 +/-      47.6
Perihelion:          40.54221061 +/-    0.0073
Aphelion:            47.58985703 +/-    0.0081
Period (y)              292.5258 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -40.35306093 +/-    0.0014
Ecliptic Y           -3.37654826 +/-    0.0001
Ecliptic Z            2.31753741 +/-    0.0001
Ecliptic XDOT         0.00025431 +/-    0.0000
Ecliptic YDOT        -0.00279455 +/-    0.0000
Ecliptic ZDOT        -0.00004263 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.56035018 +/-    0.0013
Geocenter to KBO     39.67453233 +/-    0.0014
# Hcoef:  9.33

The following table shows the complete astrometric record for 17DK170. 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 (17DK170) followed by the observatory code and reference code for the source of the astrometry.

2014 02  27.598096 12 25 10.60   +00 55 29.7         17DK170   T09  C~89UY      
2014 02  27.603516 12 25 10.58   +00 55 29.8         17DK170   T09  C~89UY      
2016 04  04.43970  12 33 19.93   +00 00 08.6   26.2g 17DK170   T09  C~89UY      
2016 04  04.44255  12 33 19.93   +00 00 08.4   26.1g 17DK170   T09  C~89UY      
2016 04  04.47854  12 33 19.76   +00 00 09.6   26.0g 17DK170   T09  C~89UY      
2016 04  04.51309  12 33 19.61   +00 00 10.6   26.2g 17DK170   T09  C~89UY      
2016 04  04.54301  12 33 19.46   +00 00 11.5   25.6g 17DK170   T09  C~89UY      
2016 04  05.452301 12 33 15.30   +00 00 37.5         17DK170   T09  C~89UY      
2016 04  05.570256 12 33 14.76   +00 00 40.9         17DK170   T09  C~89UY      
2017 01  30.657082 12 42 42.25   -01 03 58.1         17DK170   T09  C~89UY      
2017 02  02.664746 12 42 36.55   -01 03 08.5         17DK170   T09  C~89UY      
2017 02  21.48870  12 41 44.93   -00 56 27.9   25.0z 17DK170   T09  C~89UY      
2017 02  21.53656  12 41 44.76   -00 56 26.4   24.3z 17DK170   T09  C~89UY      
2017 02  21.55809  12 41 44.67   -00 56 26.1   25.1z 17DK170   T09  C~89UY      
2017 02  21.60643  12 41 44.51   -00 56 24.9   24.7z 17DK170   T09  C~89UY      
2017 02  23.53005  12 41 37.86   -00 55 36.6   25.4r 17DK170   T09  C~89UY      
2017 02  23.56764  12 41 37.72   -00 55 35.7   25.7r 17DK170   T09  C~89UY      
2017 02  23.60167  12 41 37.60   -00 55 34.7   25.6r 17DK170   T09  C~89UY      
2019 04  03.469560 12 49 45.34   -01 50 27.1         17DK170   T09  C~89UY      

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     0.06
     2   0.0000      0.00     0.02       0.00     0.01
     3   2.0995      0.00    -0.23       0.00     0.00
     4   2.0995      0.00    -0.03       0.00    -0.28
     5   2.0996      0.00    -0.05       0.00    -0.11
     6   2.0997      0.00     0.11       0.00    -0.10
     7   2.0998      0.00    -0.05       0.00    -0.05
     8   2.1023      0.00    -0.06       0.00     0.01
     9   2.1026      0.00     0.06       0.00     0.05
    10   2.9242      0.00    -0.01       0.00    -0.04
    11   2.9324      0.00     0.09       0.00    -0.07
    12   2.9840      0.00     0.08       0.00     0.05
    13   2.9841      0.00     0.04       0.00     0.36
    14   2.9841      0.00    -0.19       0.00     0.13
    15   2.9843      0.00    -0.06       0.00     0.12
    16   2.9895      0.00     0.09       0.00     0.01
    17   2.9896      0.00     0.03       0.00    -0.05
    18   2.9897      0.00     0.07       0.00     0.08
    19   5.0948      0.00    -0.05       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.

17DK170    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.745    43.745    43.745
ecceobj         0.073     0.073     0.073
incobj          3.381     3.381     3.381
qmin           39.866    39.878    39.858
qmax           48.289    48.302    48.310
amean          43.969    43.969    43.969
amin           43.625    43.625    43.625
amax           44.352    44.350    44.340
emean           0.073     0.073     0.073
emin            0.057     0.057     0.057
emax            0.090     0.090     0.090
imean           1.690     1.690     1.690
imin            0.908     0.908     0.908
imax            2.337     2.337     2.337
excite_mean     0.079     0.079     0.079
fracstop        1.000     1.000     1.000
cjmean          3.093     3.093     3.093

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       193.8     193.8     193.7
kozaiamp        180.0     179.9     179.9