Orbit Fit and Astrometric record for 00CN114

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: 00CN114   
# Created Sun Dec  5 02:08:43 2021
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     22 observations of     22
# Arc:  20.04y
# First observation: 2000/02/05
#  Last observation: 2020/02/18
# Chi-squared of fit:    29.48 DOF:     38 RMS:  0.20
# Min/Max residuals:    -0.47    0.72
# Exact a, adot, b, bdot, g, gdot:
  1.386986E-05  2.187737E-02 -3.236512E-07  3.351243E-04  2.318874E-02  9.374677E-04
# Covariance matrix:
  1.6166E-13 -2.1402E-14  7.3650E-16 -2.5131E-16  1.1442E-13 -3.4622E-14
 -2.1402E-14  2.3513E-14 -2.3161E-16  3.4655E-16  1.4528E-14  5.2599E-14
  7.3650E-16 -2.3161E-16  1.1174E-13 -6.8600E-15  1.6427E-15 -5.5074E-16
 -2.5131E-16  3.4655E-16 -6.8600E-15  1.1782E-15  1.4678E-16  8.1620E-16
  1.1442E-13  1.4528E-14  1.6427E-15  1.4678E-16  3.8875E-13  3.3064E-14
 -3.4622E-14  5.2599E-14 -5.5074E-16  8.1620E-16  3.3064E-14  1.2385E-13
#      lat0       lon0       xBary       yBary       zBary        JD0
    1.307944  137.993906    0.030356    0.022345   -0.988127  2451579.836713
# Heliocentric elements and errors
Epoch:              2451580.5000  =  2000/02/06
Mean Anomaly:           92.73960 +/-     0.112
Argument of Peri:      317.58153 +/-     0.098
Long of Asc Node:       82.43184 +/-     0.003
Inclination:             1.55123 +/-     0.000
Eccentricity:         0.04566372 +/-    0.0000
Semi-Major Axis:     43.92266583 +/-    0.0046
Time of Perihelion: 2424190.3642 +/-      33.4
Perihelion:          41.91699360 +/-    0.0044
Aphelion:            45.92833806 +/-    0.0049
Period (y)              291.0994 +/-      0.05
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -32.74382295 +/-    0.0009
Ecliptic Y           29.53832818 +/-    0.0008
Ecliptic Z            0.98435328 +/-    0.0000
Ecliptic XDOT        -0.00181581 +/-    0.0000
Ecliptic YDOT        -0.00183879 +/-    0.0000
Ecliptic ZDOT         0.00004219 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   44.10937712 +/-    0.0008
Geocenter to KBO     43.12439283 +/-    0.0012
# Hcoef:  7.19

The following table shows the complete astrometric record for 00CN114. 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 (00CN114) followed by the observatory code and reference code for the source of the astrometry.

2000 02  05.33597  09 23 24.57   +16 40 57.3   22.2R 00CN114   695  Cb4132      
2000 02  05.44067  09 23 24.06   +16 40 59.7         00CN114   695  Cb4132      
2000 03  29.17262  09 19 51.85   +16 56 50.8   24.0R 00CN114   695  Cb4132      
2000 03  29.29876  09 19 51.50   +16 56 51.8   23.8R 00CN114   695  Cb4132      
2000 03  30.11865  09 19 49.37   +16 57 00.8   23.3R 00CN114   695  Cb4132      
2000 03  30.12412  09 19 49.37   +16 57 00.8   23.6R 00CN114   695  Cb4132      
2000 03  30.14523  09 19 49.31   +16 57 01.0   23.4R 00CN114   695  Cb4132      
2000 03  30.21961  09 19 49.17   +16 57 01.8   23.7R 00CN114   695  Cb4132      
2000 03  30.23271  09 19 49.09   +16 57 01.9         00CN114   695  Cb4132      
2000 12  27.42549  09 31 04.027  +16 05 12.43  23.1R 00CN114   568  Cl4103      
2000 12  28.41872  09 31 00.928  +16 05 29.17  22.7R 00CN114   568  Cl4103      
2001 02  16.95009  09 27 26.39   +16 23 12.8   23.8R 00CN114   950  Ce8743      
2001 02  16.99424  09 27 26.18   +16 23 14.0         00CN114   950  Ce8743      
2002 02  06.23150  09 33 15.72   +15 56 24.9   23.0R 00CN114   695  Ce8743      
2002 02  06.32747  09 33 15.27   +15 56 27.3         00CN114   695  Ce8743      
2002 02  07.28651  09 33 10.82   +15 56 49.5         00CN114   695  Ce8743      
2013 03  12.16027  10 23 36.70   +11 39 02.9   23.3R 00CN114   695  C~0uco      
2013 03  12.22141  10 23 36.45   +11 39 04.2         00CN114   695  C~0uco      
2013 03  13.15346  10 23 32.54   +11 39 26.1         00CN114   695  C~0uco      
2020 02  18.254320 10 57 30.031  +08 20 58.64  23.4G 00CN114   G37  C~3i9V      
2020 02  18.346220 10 57 29.656  +08 21 01.24        00CN114   G37  C~3i9V      
2020 02  18.397080 10 57 29.433  +08 21 02.45        00CN114   G37  C~3i9V      

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     0.25       0.00     0.04
     2   0.0003      0.00     0.09       0.00     0.13
     3   0.1447      0.00    -0.12       0.00     0.22
     4   0.1450      0.00    -0.24       0.00    -0.13
     5   0.1472      0.00    -0.29       0.00     0.13
     6   0.1473      0.00    -0.08       0.00     0.07
     7   0.1473      0.00    -0.14       0.00     0.05
     8   0.1475      0.00     0.72       0.00     0.07
     9   0.1476      0.00     0.03       0.00     0.03
    10   0.8928      0.00    -0.43       0.00    -0.47
    11   0.8955      0.00    -0.16       0.00    -0.29
    12   1.0339      0.00     0.08       0.00    -0.30
    13   1.0340      0.00     0.03       0.00    -0.07
    14   2.0038      0.00     0.03       0.00    -0.08
    15   2.0041      0.00     0.07       0.00     0.12
    16   2.0067      0.00     0.11       0.00     0.40
    17  13.0974      0.00    -0.03       0.00     0.14
    18  13.0976      0.00     0.14       0.00    -0.01
    19  13.1001      0.00    -0.04       0.00     0.11
    20  20.0354      0.00    -0.13       0.00    -0.12
    21  20.0356      0.00     0.10       0.00     0.05
    22  20.0358      0.00    -0.01       0.00    -0.08

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.

00CN114    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.909    43.909    43.909
ecceobj         0.046     0.046     0.046
incobj          1.551     1.551     1.551
qmin           40.945    40.944    40.917
qmax           47.212    47.209    47.213
amean          43.971    43.971    43.971
amin           43.627    43.629    43.628
amax           44.325    44.325    44.327
emean           0.050     0.050     0.050
emin            0.033     0.033     0.033
emax            0.066     0.066     0.066
imean           0.674     0.674     0.674
imin            0.455     0.455     0.455
imax            0.896     0.896     0.896
excite_mean     0.051     0.051     0.051
fracstop        1.000     1.000     1.000
cjmean          3.098     3.098     3.098

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       201.8     201.9     201.9
kozaiamp        180.0     180.0     180.0