Orbit Fit and Astrometric record for 17DG170

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: 17DG170   
# Created Tue Apr  1 01:11:05 2025
# Orbit generated from Bernstein formalism
# Fitting     18 observations of     18
# Arc:   3.00y
# First observation: 2016/04/04
#  Last observation: 2019/04/06
Preliminary a, adot, b, bdot, g, gdot:
  -0.000054   0.024433  -0.000001   0.000045   0.024365   0.000000
# Chi-squared of fit:    10.62 DOF:     30 RMS:  0.14
# Min/Max residuals:    -0.32    0.28
# Exact a, adot, b, bdot, g, gdot:
  1.539823E-05  2.433542E-02  2.329931E-07  4.330034E-05  2.456957E-02 -9.103529E-04
# Covariance matrix:
  2.4378E-13 -3.2309E-13 -2.4409E-17 -4.4292E-16 -1.0075E-13 -3.3020E-12
 -3.2309E-13  1.1629E-12 -3.7546E-15  1.6890E-15 -1.6308E-13  1.4973E-11
 -2.4409E-17 -3.7546E-15  1.5846E-13 -9.0339E-14  3.9958E-15 -5.3140E-14
 -4.4292E-16  1.6890E-15 -9.0339E-14  1.0647E-13  2.3187E-17  2.3945E-14
 -1.0075E-13 -1.6308E-13  3.9958E-15  2.3187E-17  5.7344E-13 -2.2992E-12
 -3.3020E-12  1.4973E-11 -5.3140E-14  2.3945E-14 -2.2992E-12  2.1222E-10
#      lat0       lon0       xBary       yBary       zBary        JD0
    4.314050 -171.879050   -0.116321    0.074553   -0.986552  2457482.960707
# Heliocentric elements and errors
Epoch:              2457480.5000  =  2016/04/02
Mean Anomaly:          323.39454 +/-     0.494
Argument of Peri:      129.39935 +/-     0.568
Long of Asc Node:       99.43705 +/-     0.010
Inclination:             4.21225 +/-     0.000
Eccentricity:         0.05472297 +/-    0.0003
Semi-Major Axis:     43.55558702 +/-    0.0065
Time of Perihelion: 2468156.4768 +/-     144.1
Perihelion:          41.17209577 +/-    0.0157
Aphelion:            45.93907828 +/-    0.0160
Period (y)              287.4577 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -41.14514646 +/-    0.0012
Ecliptic Y           -5.99082592 +/-    0.0002
Ecliptic Z            3.06168577 +/-    0.0001
Ecliptic XDOT         0.00048370 +/-    0.0000
Ecliptic YDOT        -0.00267721 +/-    0.0000
Ecliptic ZDOT        -0.00000281 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   41.69156979 +/-    0.0012
Geocenter to KBO     40.70075868 +/-    0.0013
# Hcoef:  9.45

The following table shows the complete astrometric record for 17DG170. 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 (17DG170) followed by the observatory code and reference code for the source of the astrometry.

2016 04  04.459918 12 36 38.16   +00 44 38.2         17DG170   T09  C~89UX      
2016 04  04.48066  12 36 38.06   +00 44 38.7   25.9g 17DG170   T09  C~8COu      
2016 04  04.52590  12 36 37.84   +00 44 40.2   26.3g 17DG170   T09  C~8COu      
2016 04  04.555772 12 36 37.73   +00 44 41.0         17DG170   T09  C~89UX      
2016 04  05.456299 12 36 33.69   +00 45 06.1         17DG170   T09  C~89UX      
2016 04  05.515208 12 36 33.42   +00 45 07.7         17DG170   T09  C~89UX      
2017 02  21.49884  12 44 41.41   -00 08 16.4   25.9z 17DG170   T09  C~89UX      
2017 02  21.52038  12 44 41.34   -00 08 16.1   25.8z 17DG170   T09  C~89UX      
2017 02  21.59574  12 44 41.07   -00 08 14.4   24.9z 17DG170   T09  C~89UX      
2017 02  23.54421  12 44 34.58   -00 07 24.0   25.4r 17DG170   T09  C~89UX      
2017 02  23.56973  12 44 34.49   -00 07 23.3   25.1r 17DG170   T09  C~89UX      
2017 02  23.61219  12 44 34.33   -00 07 22.3   25.3r 17DG170   T09  C~89UX      
2017 02  23.64192  12 44 34.22   -00 07 21.3   25.9r 17DG170   T09  C~89UX      
2017 02  23.65456  12 44 34.17   -00 07 21.3   25.9r 17DG170   T09  C~89UX      
2017 04  27.380876 12 40 09.74   +00 21 22.0         17DG170   T09  C~89UX      
2017 04  27.392208 12 40 09.70   +00 21 22.2         17DG170   T09  C~89UX      
2019 04  06.350099 12 52 00.99   -00 53 43.7         17DG170   T09  C~89UX      
2019 04  06.460461 12 52 00.49   -00 53 40.6         17DG170   T09  C~89UX      

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     0.05       0.00    -0.04
     2   0.0001     -1.58     0.02      -0.13    -0.15
     3   0.0002     -5.20    -0.26      -0.05    -0.02
     4   0.0003     -7.03     0.11       0.03     0.10
     5   0.0027    -72.61     0.04      -0.76    -0.10
     6   0.0029    -76.97     0.04      -0.88    -0.16
     7   0.8844   7916.92    -0.01     -62.34     0.18
     8   0.8845   7915.83     0.12     -62.48    -0.03
     9   0.8847   7911.43    -0.02     -62.52    -0.32
    10   0.8900   7801.94     0.14     -54.54     0.24
    11   0.8901   7800.42     0.11     -54.43     0.27
    12   0.8902   7797.82    -0.01     -54.46     0.11
    13   0.8903   7795.91    -0.19     -54.19     0.28
    14   0.8903   7795.22    -0.15     -54.48    -0.06
    15   1.0621   3467.27    -0.05     -33.27    -0.08
    16   1.0621   3466.64     0.05     -33.33    -0.09
    17   3.0031  15074.40    -0.06      28.10    -0.09
    18   3.0034  15066.24     0.06      28.00    -0.05

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.

17DG170    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.083    43.104    43.062
ecceobj         0.046     0.046     0.047
incobj          4.211     4.211     4.211
qmin           40.685    40.694    40.655
qmax           46.108    46.171    46.133
amean          43.307    43.328    43.286
amin           42.971    43.002    42.952
amax           43.647    43.685    43.628
emean           0.039     0.038     0.039
emin            0.020     0.020     0.020
emax            0.057     0.057     0.058
imean           2.453     2.458     2.446
imin            1.581     1.592     1.565
imax            3.236     3.234     3.241
excite_mean     0.058     0.058     0.058
fracstop        1.000     1.000     1.000
cjmean          3.089     3.089     3.089

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       190.0     190.8     189.8
kozaiamp        180.0     180.0     180.0