Orbit Fit and Astrometric record for 17DD162

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: 17DD162   
# Created Tue Apr  1 01:11:04 2025
# Orbit generated from Bernstein formalism
# Fitting     18 observations of     19
# Arc:   2.08y
# First observation: 2015/03/30
#  Last observation: 2017/04/27
Preliminary a, adot, b, bdot, g, gdot:
   0.000014   0.023552   0.000000   0.000227   0.024015   0.000000
# Chi-squared of fit:     7.29 DOF:     30 RMS:  0.11
# Min/Max residuals:    -0.26    0.22
# Exact a, adot, b, bdot, g, gdot:
  1.518680E-05  2.361075E-02  9.008104E-08  2.275430E-04  2.420065E-02 -2.968414E-05
# Covariance matrix:
  7.3229E-13 -1.1523E-12  1.3296E-15 -7.8041E-15 -7.2998E-13 -1.6765E-11
 -1.1523E-12  5.3428E-12 -8.0829E-15  4.7531E-14  4.4103E-12  1.0297E-10
  1.3296E-15 -8.0829E-15  5.9602E-13 -3.1549E-13 -7.7163E-15 -1.6340E-13
 -7.8041E-15  4.7531E-14 -3.1549E-13  1.9398E-13  4.4660E-14  9.5927E-13
 -7.2998E-13  4.4103E-12 -7.7163E-15  4.4660E-14  4.4371E-12  8.9659E-11
 -1.6765E-11  1.0297E-10 -1.6340E-13  9.5927E-13  8.9659E-11  2.0624E-09
#      lat0       lon0       xBary       yBary       zBary        JD0
    3.912922 -171.206976   -0.006514    0.068061   -0.993190  2457111.860316
# Heliocentric elements and errors
Epoch:              2457110.5000  =  2015/03/29
Mean Anomaly:            0.98824 +/-     4.385
Argument of Peri:       80.83184 +/-     4.609
Long of Asc Node:      106.94490 +/-     0.016
Inclination:             3.85949 +/-     0.000
Eccentricity:         0.02446567 +/-    0.0001
Semi-Major Axis:     43.37864961 +/-    0.0083
Time of Perihelion: 2456824.0334 +/-    1271.0
Perihelion:          42.31736184 +/-    0.0093
Aphelion:            44.43993737 +/-    0.0097
Period (y)              285.7079 +/-      0.08
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -41.72626199 +/-    0.0035
Ecliptic Y           -6.46073567 +/-    0.0006
Ecliptic Z            2.81979440 +/-    0.0002
Ecliptic XDOT         0.00041006 +/-    0.0000
Ecliptic YDOT        -0.00264479 +/-    0.0000
Ecliptic ZDOT         0.00002554 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.31752929 +/-    0.0035
Geocenter to KBO     41.32121036 +/-    0.0036
# Hcoef:  7.86

The following table shows the complete astrometric record for 17DD162. 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 (17DD162) followed by the observatory code and reference code for the source of the astrometry.

2015 03  30.359538 12 38 28.19   +00 06 41.1         17DD162   T09  C~83F2      
2015 03  30.398433 12 38 28.01   +00 06 42.3         17DD162   T09  C~83F2      
2016 04  04.445379 12 43 02.71   -00 21 49.1         17DD162   T09  C~83F2      
2016 04  04.547236 12 43 02.25   -00 21 46.5         17DD162   T09  C~83F2      
2017 02  21.49208  12 50 53.33   -01 12 31.2   23.9z 17DD162   T09  C~7xU4      
2017 02  21.51771  12 50 53.25   -01 12 30.5   24.3z 17DD162   T09  C~7xU4      
2017 02  21.53924  12 50 53.18   -01 12 30.2   23.9z 17DD162   T09  C~7xU4      
2017 02  21.59034  12 50 53.01   -01 12 28.9   23.9z 17DD162   T09  C~7xU4      
2017 02  21.60376  12 50 52.97   -01 12 28.5   23.7z 17DD162   T09  C~7xU4      
2017 02  23.53285  12 50 46.78   -01 11 41.5   24.8r 17DD162   T09  C~7xU4      
2017 02  23.57183  12 50 46.66   -01 11 40.5   24.4r 17DD162   T09  C~7xU4      
2017 02  23.63562  12 50 46.43   -01 11 39.1   23.9r 17DD162   T09  C~7xU4      
2017 02  23.64611  12 50 46.39   -01 11 38.8   23.6r 17DD162   T09  C~7xU4      
2017 03  25.37615  12 48 49.12   -00 57 59.4   23.4y 17DD162   T09  C~7xU4      
2017 03  25.41476  12 48 49.02   -00 57 58.2   23.6y 17DD162   T09  C~7xU4      
2017 03  25.41743  12 48 48.94   -00 57 58.2   23.4y 17DD162   T09  C~7xU4      
2017 04  27.40255  12 46 26.25   -00 43 19.8   24.0i 17DD162   T09  C~7xU4      
2017 04  27.42613  12 46 26.16   -00 43 19.2   24.3i 17DD162   T09  C~7xU4      
2017 04  27.42903  12 46 26.15   -00 43 19.4   24.1i 17DD162   T09  C~7xU4      

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     0.01
     2   0.0001     -2.95    -0.04       0.04     0.06
     3   1.0160   4459.25    -0.06      46.16     0.02
     4   1.0163   4451.88     0.04      45.84    -0.22
     5   1.9004  12158.78     0.07      21.87     0.12
     6   1.9005  12157.40     0.07      22.05     0.22
     7   1.9006  12156.31     0.15      21.91     0.01
     8   1.9007  12153.45     0.05      22.11     0.04
     9   1.9007  12152.74     0.06      22.24     0.13
    10   1.9060  12048.55    -0.04      29.03     0.00
    11   1.9061  12046.50     0.10      29.24     0.10
    12   1.9063  12042.76    -0.06      29.17    -0.16
    13   1.9063  12042.09    -0.15      29.21    -0.15
    14   1.9877  10097.26    -0.26      92.17    -0.02
    15   1.9878  10095.41 (   0.71)     92.69 (   0.48)
    16   1.9878  10094.30    -0.20      92.22     0.01
    17   2.0781   7776.80    -0.00      59.16    -0.04
    18   2.0782   7775.32     0.05      59.18     0.05
    19   2.0782   7775.26     0.18      58.94    -0.18

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.

17DD162    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        42.972    42.991    42.953
ecceobj         0.015     0.015     0.015
incobj          3.860     3.860     3.860
qmin           41.578    41.617    41.482
qmax           44.994    44.995    45.040
amean          43.196    43.216    43.177
amin           42.864    42.884    42.843
amax           43.533    43.555    43.512
emean           0.017     0.016     0.018
emin            0.000     0.000     0.000
emax            0.034     0.033     0.035
imean           2.369     2.364     2.373
imin            1.497     1.501     1.493
imax            3.129     3.116     3.139
excite_mean     0.045     0.045     0.045
fracstop        1.000     1.000     1.000
cjmean          3.089     3.090     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       193.4     194.9     192.1
kozaiamp        180.0     180.0     180.0