Orbit Fit and Astrometric record for 17DN171

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: 17DN171   
# Created Wed Dec 25 02:10:55 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     21 observations of     21
# Arc:   5.99y
# First observation: 2013/04/05
#  Last observation: 2019/04/03
# Chi-squared of fit:    13.71 DOF:     36 RMS:  0.14
# Min/Max residuals:    -0.29    0.45
# Exact a, adot, b, bdot, g, gdot:
  1.672536E-05  2.523801E-02 -7.010722E-06 -8.510779E-03  2.586029E-02  1.620279E-03
# Covariance matrix:
  4.7905E-13 -2.1917E-13 -2.0287E-14  3.6620E-14 -5.5046E-14 -9.1076E-13
 -2.1917E-13  2.5941E-13  3.8900E-14 -7.0415E-14  2.1489E-15  1.7476E-12
 -2.0287E-14  3.8900E-14  4.2614E-13 -1.1921E-13  1.3600E-14  3.1060E-13
  3.6620E-14 -7.0415E-14 -1.1921E-13  5.5222E-14 -2.3245E-14 -5.6112E-13
 -5.5046E-14  2.1489E-15  1.3600E-14 -2.3245E-14  7.1649E-13  6.0203E-13
 -9.1076E-13  1.7476E-12  3.1060E-13 -5.6112E-13  6.0203E-13  1.3947E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
    5.774673 -176.191275   -0.205396    0.098706   -0.975626  2456387.832533
# Heliocentric elements and errors
Epoch:              2456388.5000  =  2013/04/06
Mean Anomaly:           40.82310 +/-     0.052
Argument of Peri:      114.07458 +/-     0.068
Long of Asc Node:       20.29326 +/-     0.000
Inclination:            19.47814 +/-     0.000
Eccentricity:         0.09720261 +/-    0.0001
Semi-Major Axis:     42.58492321 +/-    0.0065
Time of Perihelion: 2444878.2238 +/-      15.0
Perihelion:          38.44555771 +/-    0.0086
Aphelion:            46.72428871 +/-    0.0095
Period (y)              277.9022 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -39.35220534 +/-    0.0013
Ecliptic Y           -2.82379779 +/-    0.0001
Ecliptic Z            3.89051712 +/-    0.0001
Ecliptic XDOT        -0.00008956 +/-    0.0000
Ecliptic YDOT        -0.00268303 +/-    0.0000
Ecliptic ZDOT        -0.00087907 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.64470461 +/-    0.0012
Geocenter to KBO     38.66933021 +/-    0.0013
# Hcoef:  7.67

The following table shows the complete astrometric record for 17DN171. 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 (17DN171) followed by the observatory code and reference code for the source of the astrometry.

2013 04  05.331755 12 23 09.54   +03 47 08.6         17DN171   T14  C~89Ua      
2013 04  05.334260 12 23 09.53   +03 47 08.1         17DN171   T14  C~89Ua      
2013 04  05.336002 12 23 09.54   +03 47 08.0         17DN171   T14  C~89Ua      
2016 04  04.459918 12 36 44.90   +00 43 19.0         17DN171   T09  C~89Ua      
2016 04  04.48066  12 36 44.79   +00 43 19.4   24.5g 17DN171   T09  C~8COu      
2016 04  04.52590  12 36 44.58   +00 43 20.6   24.7g 17DN171   T09  C~8COu      
2016 04  04.555772 12 36 44.43   +00 43 21.3         17DN171   T09  C~89Ua      
2017 02  21.48870  12 44 22.22   -00 35 12.7   23.7z 17DN171   T09  C~89Ua      
2017 02  21.49884  12 44 22.20   -00 35 12.5   23.4z 17DN171   T09  C~89Ua      
2017 02  21.53656  12 44 22.04   -00 35 11.7   23.9z 17DN171   T09  C~89Ua      
2017 02  21.56614  12 44 21.94   -00 35 11.1   23.0z 17DN171   T09  C~89Ua      
2017 02  21.58766  12 44 21.88   -00 35 10.5   23.6z 17DN171   T09  C~89Ua      
2017 02  21.60643  12 44 21.79   -00 35 10.1   23.1z 17DN171   T09  C~89Ua      
2017 02  23.54421  12 44 14.73   -00 34 27.5   23.8r 17DN171   T09  C~89Ua      
2017 02  23.56973  12 44 14.63   -00 34 27.0   23.9r 17DN171   T09  C~89Ua      
2017 02  23.61219  12 44 14.46   -00 34 26.1   23.2r 17DN171   T09  C~89Ua      
2017 02  23.64192  12 44 14.36   -00 34 25.6   23.9r 17DN171   T09  C~89Ua      
2017 03  03.246632 12 43 44.446  -00 31 27.30  23.8g 17DN171   W84  C~8HKW      
2017 03  03.272194 12 43 44.321  -00 31 26.76  22.9r 17DN171   W84  C~8HKW      
2017 04  27.380876 12 39 28.78   -00 08 59.1         17DN171   T09  C~89Ua      
2019 04  03.469560 12 50 16.59   -02 19 09.4         17DN171   T09  C~89Ua      

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    -0.10       0.00     0.45
     2   0.0000      0.00    -0.06       0.00    -0.11
     3   0.0000      0.00     0.22       0.00    -0.25
     4   2.9983      0.00    -0.06       0.00    -0.03
     5   2.9984      0.00    -0.17       0.00    -0.15
     6   2.9985      0.00     0.02       0.00    -0.08
     7   2.9986      0.00    -0.03       0.00    -0.13
     8   3.8827      0.00    -0.06       0.00     0.13
     9   3.8827      0.00     0.20       0.00     0.11
    10   3.8828      0.00    -0.13       0.00     0.09
    11   3.8829      0.00     0.00       0.00     0.05
    12   3.8830      0.00     0.29       0.00     0.18
    13   3.8830      0.00    -0.03       0.00     0.17
    14   3.8883      0.00     0.07       0.00     0.05
    15   3.8884      0.00     0.03       0.00    -0.02
    16   3.8885      0.00    -0.11       0.00    -0.07
    17   3.8886      0.00     0.08       0.00    -0.24
    18   3.9094      0.00    -0.03       0.00     0.01
    19   3.9095      0.00    -0.29       0.00    -0.07
    20   4.0604      0.00     0.01       0.00     0.01
    21   5.9935      0.00     0.01       0.00    -0.02

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.

17DN171    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        42.413    42.413    42.413
ecceobj         0.094     0.094     0.094
incobj         19.509    19.509    19.509
qmin           37.758    37.770    37.762
qmax           47.681    47.665    47.688
amean          42.592    42.592    42.591
amin           42.258    42.242    42.249
amax           42.964    42.962    42.958
emean           0.094     0.094     0.094
emin            0.078     0.078     0.079
emax            0.110     0.110     0.111
imean          19.070    19.070    19.070
imin           18.522    18.524    18.521
imax           19.605    19.602    19.606
excite_mean     0.340     0.340     0.340
fracstop        1.000     1.000     1.000
cjmean          2.945     2.945     2.945

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       186.1     186.3     186.2
kozaiamp        179.9     180.0     180.0