Orbit Fit and Astrometric record for 14PZ102

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: 14PZ102   
# Created Wed Jul 17 01:10:23 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     21 observations of     21
# Arc:   9.09y
# First observation: 2014/08/03
#  Last observation: 2023/09/06
# Chi-squared of fit:     9.93 DOF:     36 RMS:  0.12
# Min/Max residuals:    -0.20    0.32
# Exact a, adot, b, bdot, g, gdot:
  1.624432E-05  2.731933E-02  1.586264E-06  1.119853E-03  2.596436E-02  1.527413E-03
# Covariance matrix:
  3.6014E-13 -1.5599E-13  1.0487E-14 -6.2695E-15  1.0718E-12 -7.1970E-13
 -1.5599E-13  1.0627E-13 -5.9610E-15  4.3699E-15 -4.4233E-13  4.8208E-13
  1.0487E-14 -5.9610E-15  1.3088E-13 -2.2245E-14  5.0350E-14 -3.2369E-14
 -6.2695E-15  4.3699E-15 -2.2245E-14  8.1170E-15 -2.2783E-14  2.1839E-14
  1.0718E-12 -4.4233E-13  5.0350E-14 -2.2783E-14  6.6596E-12 -2.7929E-12
 -7.1970E-13  4.8208E-13 -3.2369E-14  2.1839E-14 -2.7929E-12  2.4466E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
   -4.015394   -8.987579    0.654634   -0.054447   -0.776791  2456873.038058
# Heliocentric elements and errors
Epoch:              2456872.5000  =  2014/08/03
Mean Anomaly:           17.86435 +/-     0.037
Argument of Peri:      277.69143 +/-     0.044
Long of Asc Node:       49.98155 +/-     0.002
Inclination:             4.54537 +/-     0.000
Eccentricity:         0.11000213 +/-    0.0003
Semi-Major Axis:     43.82345386 +/-    0.0212
Time of Perihelion: 2451614.2294 +/-      11.5
Perihelion:          39.00278075 +/-    0.0241
Aphelion:            48.64412697 +/-    0.0279
Period (y)              290.1136 +/-      0.21
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           38.61289203 +/-    0.0038
Ecliptic Y           -6.76801268 +/-    0.0006
Ecliptic Z           -2.69684674 +/-    0.0003
Ecliptic XDOT         0.00061191 +/-    0.0000
Ecliptic YDOT         0.00281482 +/-    0.0000
Ecliptic ZDOT         0.00010664 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   39.29417905 +/-    0.0037
Geocenter to KBO     38.51433193 +/-    0.0038
# Hcoef:  6.70

The following table shows the complete astrometric record for 14PZ102. 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 (14PZ102) followed by the observatory code and reference code for the source of the astrometry.

2014 08  03.53728  23 33 20.57   -07 15 07.4   22.9w 14PZ102   F51  C~77r0      
2014 08  03.54859  23 33 20.52   -07 15 07.4   22.9w 14PZ102   F51  C~77r0      
2014 08  03.55989  23 33 20.49   -07 15 07.8   22.9w 14PZ102   F51  C~77r0      
2014 08  20.47989  23 32 16.79   -07 22 45.6   23.0w 14PZ102   F51  C~77r0      
2014 08  20.49207  23 32 16.73   -07 22 46.1   22.6w 14PZ102   F51  C~77r0      
2014 08  20.51641  23 32 16.62   -07 22 46.8   22.8w 14PZ102   F51  C~77r0      
2014 08  22.47712  23 32 08.32   -07 23 44.0   22.6w 14PZ102   F51  C~77r0      
2014 08  22.51392  23 32 08.15   -07 23 45.0   22.9w 14PZ102   F51  C~77r0      
2017 08  01.54579  23 50 19.69   -05 11 57.8   23.2w 14PZ102   F51  C~77r0      
2017 08  01.55769  23 50 19.65   -05 11 58.1   23.1w 14PZ102   F51  C~77r0      
2017 08  01.5696   23 50 19.62   -05 11 58.4   22.9w 14PZ102   F51  C~77r0      
2017 08  03.52361  23 50 14.00   -05 12 42.6   22.8w 14PZ102   F51  C~77r0      
2017 08  03.53438  23 50 13.97   -05 12 42.4   22.8w 14PZ102   F51  C~77r0      
2017 08  03.54518  23 50 13.92   -05 12 42.9   23.0w 14PZ102   F51  C~77r0      
2017 08  03.55592  23 50 13.90   -05 12 43.2   22.9w 14PZ102   F51  C~77r0      
2017 08  17.47873  23 49 26.52   -05 18 34.6   22.9w 14PZ102   F51  C~77r0      
2017 08  17.48978  23 49 26.46   -05 18 35.3   22.7w 14PZ102   F51  C~77r0      
2017 08  17.51191  23 49 26.38   -05 18 35.7   22.4w 14PZ102   F51  C~77r0      
2023 09  06.404610 00 21 30.715  -01 19 47.58  23.0G 14PZ102   G37  C~7B3M      
2023 09  06.444290 00 21 30.537  -01 19 48.79        14PZ102   G37  C~7B3M      
2023 09  06.481210 00 21 30.381  -01 19 49.71        14PZ102   G37  C~7B3M      

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     0.15       0.00    -0.14
     2   0.0000      0.00    -0.03       0.00     0.14
     3   0.0001      0.00     0.09       0.00     0.02
     4   0.0464      0.00     0.14       0.00     0.11
     5   0.0464      0.00     0.02       0.00    -0.04
     6   0.0465      0.00    -0.06       0.00    -0.04
     7   0.0519      0.00     0.01       0.00    -0.20
     8   0.0520      0.00    -0.13       0.00    -0.13
     9   2.9952      0.00    -0.12       0.00     0.01
    10   2.9953      0.00    -0.20       0.00    -0.02
    11   2.9953      0.00    -0.13       0.00    -0.06
    12   3.0006      0.00     0.10       0.00    -0.16
    13   3.0007      0.00     0.14       0.00     0.29
    14   3.0007      0.00    -0.11       0.00     0.04
    15   3.0007      0.00     0.08       0.00    -0.01
    16   3.0389      0.00     0.16       0.00     0.32
    17   3.0389      0.00    -0.09       0.00    -0.07
    18   3.0389      0.00     0.01       0.00     0.13
    19   9.0920      0.00     0.07       0.00    -0.05
    20   9.0921      0.00    -0.03       0.00    -0.12
    21   9.0922      0.00     0.02       0.00     0.01

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.

14PZ102    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.171    44.171    44.171
ecceobj         0.117     0.117     0.117
incobj          4.543     4.543     4.543
qmin           38.228    38.221    38.224
qmax           50.124    50.063    50.114
amean          44.008    44.008    44.003
amin           43.640    43.627    43.635
amax           44.399    44.403    44.403
emean           0.110     0.109     0.110
emin            0.090     0.089     0.090
emax            0.129     0.128     0.129
imean           2.838     2.846     2.844
imin            1.824     1.851     1.841
imax            3.980     3.980     3.981
excite_mean     0.121     0.120     0.121
fracstop        1.000     1.000     1.000
cjmean          3.084     3.084     3.084

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       183.2     182.2     183.9
kozaiamp        180.0     179.9     180.0