Orbit Fit and Astrometric record for 14WM602

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: 14WM602   
# Created Sat Apr 20 01:16:52 2024
# Orbit generated from Bernstein formalism
# Fitting     19 observations of     19
# Arc:   4.01y
# First observation: 2014/11/27
#  Last observation: 2018/12/01
Preliminary a, adot, b, bdot, g, gdot:
  -0.000025   0.025910  -0.000161  -0.004976   0.025739   0.000000
# Chi-squared of fit:     4.47 DOF:     32 RMS:  0.09
# Min/Max residuals:    -0.18    0.24
# Exact a, adot, b, bdot, g, gdot:
  1.658575E-05  2.576397E-02 -3.280276E-06 -5.003734E-03  2.488423E-02 -7.711761E-04
# Covariance matrix:
  2.5690E-13 -2.4526E-13 -2.0326E-15  3.2188E-14 -5.2365E-14 -1.8470E-12
 -2.4526E-13  7.0312E-13  2.7012E-14 -1.3538E-13 -9.4624E-15  6.8897E-12
 -2.0326E-15  2.7012E-14  2.0506E-13 -7.7596E-14 -2.9855E-14  2.6478E-13
  3.2188E-14 -1.3538E-13 -7.7596E-14  6.8491E-14  2.2359E-14 -1.3948E-12
 -5.2365E-14 -9.4624E-15 -2.9855E-14  2.2359E-14  3.1750E-13  7.0682E-14
 -1.8470E-12  6.8897E-12  2.6478E-13 -1.3948E-12  7.0682E-14  7.1625E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
  -34.924389   -5.448020   -0.926977   -0.194032   -0.278232  2456988.672048
# Heliocentric elements and errors
Epoch:              2456980.5000  =  2014/11/19
Mean Anomaly:          356.81793 +/-     0.116
Argument of Peri:      259.92534 +/-     0.154
Long of Asc Node:      103.59726 +/-     0.001
Inclination:            35.91373 +/-     0.000
Eccentricity:         0.13792117 +/-    0.0001
Semi-Major Axis:     46.93289788 +/-    0.0061
Time of Perihelion: 2458018.5583 +/-      37.7
Perihelion:          40.45985756 +/-    0.0066
Aphelion:            53.40593819 +/-    0.0080
Period (y)              321.5320 +/-      0.06
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           33.22304425 +/-    0.0007
Ecliptic Y           -2.23596842 +/-    0.0001
Ecliptic Z          -23.00650645 +/-    0.0005
Ecliptic XDOT        -0.00011808 +/-    0.0000
Ecliptic YDOT         0.00285334 +/-    0.0000
Ecliptic ZDOT        -0.00040271 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   40.47307208 +/-    0.0007
Geocenter to KBO     40.18609151 +/-    0.0009
# Hcoef:  7.65

The following table shows the complete astrometric record for 14WM602. 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 (14WM602) followed by the observatory code and reference code for the source of the astrometry.

2014 11  27.17127  00 43 21.839  -33 47 40.86  23.9r 14WM602   W84  C~55TE      
2014 12  13.08888  00 42 49.851  -33 37 06.05  24.2g 14WM602   W84  C~55TE      
2014 12  13.09025  00 42 49.853  -33 37 06.17  24.0i 14WM602   W84  C~55TE      
2014 12  26.10498  00 42 43.865  -33 26 02.39  23.1i 14WM602   W84  C~55TE      
2014 12  26.10635  00 42 43.844  -33 26 02.27  23.8r 14WM602   W84  C~55TE      
2015 01  13.04672  00 43 06.808  -33 08 19.32  23.5i 14WM602   W84  C~55TE      
2015 11  08.10153  00 51 26.317  -33 27 02.80  23.5i 14WM602   W84  C~55TE      
2015 11  08.10290  00 51 26.305  -33 27 02.86  24.2g 14WM602   W84  C~55TE      
2016 08  26.41053  01 04 16.760  -32 26 24.95  23.4i 14WM602   W84  C~55TE      
2016 08  31.37428  01 03 58.042  -32 30 39.33  24.9g 14WM602   W84  C~55TE      
2016 11  28.03500  00 56 56.534  -32 50 10.90  23.6r 14WM602   W84  C~55TE      
2017 09  25.22511  01 08 48.686  -32 16 19.66  23.5r 14WM602   W84  C~55TE      
2017 09  25.22648  01 08 48.693  -32 16 19.68  24.3g 14WM602   W84  C~55TE      
2017 11  01.09818  01 05 32.956  -32 27 06.70  22.9z 14WM602   W84  C~55TE      
2017 11  20.20707  01 04 07.662  -32 23 14.50  24.2r 14WM602   W84  C~55TE      
2017 11  20.20844  01 04 07.654  -32 23 14.48  24.3g 14WM602   W84  C~55TE      
2017 12  11.16275  01 03 06.340  -32 11 47.53  23.7r 14WM602   W84  C~55TE      
2018 12  01.17615  01 10 09.562  -31 46 24.12  23.3r 14WM602   W84  C~55TE      
2018 12  01.17753  01 10 09.543  -31 46 24.09  24.6g 14WM602   W84  C~55TE      

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    -0.04       0.00     0.02
     2   0.0436    -48.93     0.02     748.28     0.10
     3   0.0436    -48.97    -0.03     748.16    -0.09
     4   0.0792    200.62     0.15    1367.79    -0.18
     5   0.0792    200.44    -0.07    1368.02    -0.01
     6   0.1283    959.28    -0.05    2166.22     0.03
     7   0.9471   5894.00     0.05   -1853.16     0.00
     8   0.9471   5893.84    -0.05   -1853.13    -0.03
     9   1.7474  16130.31    -0.08   -3638.67     0.10
    10   1.7610  15793.78     0.18   -3733.08     0.08
    11   2.0037  10599.70     0.02   -2008.12     0.24
    12   2.8283  19407.74    -0.12   -4938.06    -0.01
    13   2.8284  19407.81     0.05   -4938.13    -0.08
    14   2.9293  16937.51    -0.08   -4179.39    -0.09
    15   2.9816  16130.68     0.09   -3415.34    -0.04
    16   2.9816  16130.60     0.06   -3415.27    -0.03
    17   3.0390  15819.34    -0.08   -2421.50    -0.06
    18   4.0110  21248.72     0.09   -3957.39    -0.02
    19   4.0110  21248.53    -0.08   -3957.23     0.06

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.

14WM602    quality flag:3

Type:       SCATEXTD  SCATEXTD  SCATEXTD

axisobj        47.396    47.416    47.376
ecceobj         0.147     0.147     0.146
incobj         35.916    35.916    35.916
qmin           39.938    39.966    39.986
qmax           54.659    54.687    54.581
amean          47.130    47.150    47.110
amin           46.743    46.749    46.723
amax           47.572    47.578    47.517
emean           0.134     0.135     0.134
emin            0.121     0.120     0.120
emax            0.150     0.150     0.149
imean          34.367    34.367    34.366
imin           34.116    34.115    34.112
imax           34.646    34.640    34.615
excite_mean     0.580     0.580     0.580
fracstop        1.000     1.000     1.000
cjmean          2.686     2.686     2.685

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       185.6     185.5     185.5
kozaiamp        180.0     180.0     180.0