Orbit Fit and Astrometric record for 02PR170

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: 02PR170   
# Created Sat Apr 20 01:10:50 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     27 observations of     27
# Arc:  15.12y
# First observation: 2002/08/05
#  Last observation: 2017/09/17
# Chi-squared of fit:    62.74 DOF:     48 RMS:  0.27
# Min/Max residuals:    -0.52    0.77
# Exact a, adot, b, bdot, g, gdot:
  1.238493E-05  2.070156E-02  2.379307E-06  1.696461E-04  2.254934E-02  1.837745E-03
# Covariance matrix:
  1.8733E-13 -1.2730E-13  8.9485E-17 -1.0499E-15  1.0380E-13 -4.0334E-13
 -1.2730E-13  1.8215E-13 -6.3814E-16  1.5683E-15 -4.7598E-14  5.9217E-13
  8.9485E-17 -6.3814E-16  7.8237E-14 -5.9778E-15 -7.1702E-16 -2.0290E-15
 -1.0499E-15  1.5683E-15 -5.9778E-15  1.6878E-15 -4.0218E-16  5.1450E-15
  1.0380E-13 -4.7598E-14 -7.1702E-16 -4.0218E-16  1.9979E-13 -1.6989E-13
 -4.0334E-13  5.9217E-13 -2.0290E-15  5.1450E-15 -1.6989E-13  1.9440E-12
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.735764  -33.754021    0.240413   -0.012774   -0.989625  2452491.909723
# Heliocentric elements and errors
Epoch:              2452492.5000  =  2002/08/06
Mean Anomaly:          105.39410 +/-     0.074
Argument of Peri:      188.41223 +/-     0.062
Long of Asc Node:       22.86964 +/-     0.006
Inclination:             0.85874 +/-     0.000
Eccentricity:         0.08671043 +/-    0.0000
Semi-Major Axis:     44.02498601 +/-    0.0044
Time of Perihelion: 2421256.0935 +/-      22.3
Perihelion:          40.20756050 +/-    0.0044
Aphelion:            47.84241152 +/-    0.0051
Period (y)              292.1171 +/-      0.04
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           37.55793348 +/-    0.0007
Ecliptic Y          -25.38261250 +/-    0.0005
Ecliptic Z           -0.56933395 +/-    0.0000
Ecliptic XDOT         0.00157452 +/-    0.0000
Ecliptic YDOT         0.00196311 +/-    0.0000
Ecliptic ZDOT         0.00001794 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   45.33425611 +/-    0.0007
Geocenter to KBO     44.34717624 +/-    0.0009
# Hcoef:  6.97

The following table shows the complete astrometric record for 02PR170. 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 (02PR170) followed by the observatory code and reference code for the source of the astrometry.

2002 08  05.40898  21 54 58.23   -13 27 38.8   24.0R 02PR170   568  Cp2009      
2002 08  05.46821  21 54 57.97   -13 27 40.0   23.6R 02PR170   568  Cp2009      
2002 08  05.53088  21 54 57.72   -13 27 41.2   23.9R 02PR170   568  Cp2009      
2002 08  08.38708  21 54 45.60   -13 28 45.8         02PR170   568  Cp2009      
2002 09  04.14068  21 52 50.47   -13 38 45.0         02PR170   309  Cp2009      
2002 09  04.14680  21 52 50.45   -13 38 45.3         02PR170   309  Cp2009      
2002 09  04.18376  21 52 50.29   -13 38 46.1         02PR170   309  Cp2009      
2002 09  04.18988  21 52 50.26   -13 38 46.2         02PR170   309  Cp2009      
2002 11  07.040664 21 50 10.35   -13 51 45.6   23.5r 02PR170   309  C~5i0z      
2002 11  09.021200 21 50 10.21   -13 51 44.1   23.4r 02PR170   309  C~5i0z      
2002 11  28.197863 21 50 26.80   -13 49 55.9   23.3r 02PR170   568  C~5i0z      
2002 11  29.192179 21 50 28.53   -13 49 45.8         02PR170   568  C~5i0z      
2002 11  29.201388 21 50 28.55   -13 49 45.8   23.5r 02PR170   568  C~5i0z      
2002 11  30.199870 21 50 30.39   -13 49 35.5         02PR170   568  C~5i0z      
2003 06  22.505188 22 01 53.17   -12 49 44.5   23.0i 02PR170   568  C~5i0z      
2003 06  23.495701 22 01 51.23   -12 49 55.6   22.8i 02PR170   568  C~5i0z      
2003 06  23.547142 22 01 51.11   -12 49 56.2         02PR170   568  C~5i0z      
2003 06  23.595973 22 01 51.02   -12 49 56.7         02PR170   568  C~5i0z      
2004 08  22.362907 22 02 47.60   -12 44 33.3   23.2r 02PR170   568  C~5i0z      
2004 08  22.364901 22 02 47.59   -12 44 33.4         02PR170   568  C~5i0z      
2004 08  22.366898 22 02 47.59   -12 44 33.3         02PR170   568  C~5i0z      
2004 08  22.368895 22 02 47.58   -12 44 33.1   23.3r 02PR170   568  C~5i0z      
2017 09  16.463692 22 57 34.36   -07 15 43.6   23.4r 02PR170   568  C~5i0z      
2017 09  16.468904 22 57 34.33   -07 15 43.6         02PR170   568  C~5i0z      
2017 09  17.458496 22 57 30.35   -07 16 08.5   23.4r 02PR170   568  C~5i0z      
2017 09  17.463713 22 57 30.33   -07 16 08.7         02PR170   568  C~5i0z      
2017 09  17.523178 22 57 30.09   -07 16 09.9         02PR170   568  C~5i0z      

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     0.59       0.00    -0.29
     2   0.0002      0.00     0.49       0.00    -0.16
     3   0.0003      0.00     0.77       0.00     0.03
     4   0.0082      0.00     0.13       0.00    -0.52
     5   0.0814      0.00    -0.48       0.00     0.49
     6   0.0814      0.00    -0.39       0.00     0.32
     7   0.0815      0.00    -0.44       0.00     0.31
     8   0.0815      0.00    -0.50       0.00     0.34
     9   0.2563      0.00     0.03       0.00    -0.05
    10   0.2618      0.00    -0.09       0.00    -0.12
    11   0.3143      0.00     0.05       0.00     0.21
    12   0.3170      0.00    -0.04       0.00     0.18
    13   0.3170      0.00     0.02       0.00     0.09
    14   0.3198      0.00     0.17       0.00    -0.23
    15   0.8791      0.00    -0.01       0.00    -0.23
    16   0.8818      0.00    -0.08       0.00    -0.12
    17   0.8820      0.00    -0.29       0.00    -0.12
    18   0.8821      0.00    -0.12       0.00    -0.06
    19   2.0478      0.00     0.06       0.00    -0.11
    20   2.0478      0.00     0.04       0.00    -0.16
    21   2.0478      0.00     0.17       0.00    -0.01
    22   2.0478      0.00     0.15       0.00     0.23
    23  15.1158      0.00    -0.02       0.00     0.23
    24  15.1158      0.00    -0.15       0.00     0.36
    25  15.1185      0.00     0.03       0.00    -0.22
    26  15.1186      0.00     0.05       0.00    -0.29
    27  15.1187      0.00     0.10       0.00    -0.04

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.

02PR170    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        44.333    44.333    44.333
ecceobj         0.083     0.083     0.083
incobj          0.856     0.856     0.856
qmin           39.723    39.757    39.744
qmax           49.009    49.032    49.053
amean          44.266    44.266    44.266
amin           43.903    43.903    43.917
amax           44.645    44.640    44.637
emean           0.082     0.082     0.082
emin            0.066     0.066     0.066
emax            0.098     0.099     0.099
imean           1.793     1.793     1.793
imin            1.000     1.000     1.000
imax            2.467     2.466     2.463
excite_mean     0.089     0.089     0.088
fracstop        1.000     1.000     1.000
cjmean          3.095     3.095     3.095

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       166.4     166.6     166.5
kozaiamp        180.0     180.0     179.9