Orbit Fit and Astrometric record for 99JD132

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: 99JD132   
# Created Fri Mar 29 01:09:58 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     67 observations of     67
# Arc:  18.92y
# First observation: 1999/05/10
#  Last observation: 2018/04/10
# Chi-squared of fit:    89.48 DOF:    128 RMS:  0.20
# Min/Max residuals:    -0.80    1.01
# Exact a, adot, b, bdot, g, gdot:
  1.608277E-05  2.293799E-02 -3.111764E-06 -4.242182E-03  2.404642E-02  1.349064E-03
# Covariance matrix:
  6.0620E-14  2.1566E-13  2.9502E-15 -4.1974E-14  4.7224E-13  1.4519E-12
  2.1566E-13  2.0276E-12  2.7106E-14 -3.7974E-13  3.3641E-12  1.3135E-11
  2.9502E-15  2.7106E-14  2.4873E-14 -9.4786E-15  4.5148E-14  1.7649E-13
 -4.1974E-14 -3.7974E-13 -9.4786E-15  8.1901E-14 -6.3809E-13 -2.4735E-12
  4.7224E-13  3.3641E-12  4.5148E-14 -6.3809E-13  6.5258E-12  2.2072E-11
  1.4519E-12  1.3135E-11  1.7649E-13 -2.4735E-12  2.2072E-11  8.5561E-11
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.282264 -147.962249   -0.292821   -0.005002   -0.972515  2451308.685963
# Heliocentric elements and errors
Epoch:              2451308.5000  =  1999/05/10
Mean Anomaly:           76.50722 +/-     0.158
Argument of Peri:       97.66212 +/-     0.225
Long of Asc Node:       30.95088 +/-     0.000
Inclination:            10.51866 +/-     0.000
Eccentricity:         0.06482496 +/-    0.0004
Semi-Major Axis:     43.02880916 +/-    0.0119
Time of Perihelion: 2429398.7543 +/-      46.2
Perihelion:          40.23946812 +/-    0.0192
Aphelion:            45.81815020 +/-    0.0201
Period (y)              282.2586 +/-      0.12
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -35.91280182 +/-    0.0038
Ecliptic Y          -22.82415472 +/-    0.0023
Ecliptic Z           -0.20501001 +/-    0.0000
Ecliptic XDOT         0.00125455 +/-    0.0000
Ecliptic YDOT        -0.00228542 +/-    0.0000
Ecliptic ZDOT        -0.00048373 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   42.55243766 +/-    0.0034
Geocenter to KBO     41.58624614 +/-    0.0044
# Hcoef:  7.65

The following table shows the complete astrometric record for 99JD132. 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 (99JD132) followed by the observatory code and reference code for the source of the astrometry.

1999 05  10.18522  13 59 02.99   -12 26 47.7   23.7R 99JD132   807  Ca5620      
1999 05  10.19209  13 59 02.96   -12 26 47.6   23.7R 99JD132   807  Ca5620      
1999 05  10.19896  13 59 02.93   -12 26 47.4   23.9R 99JD132   807  Ca5620      
1999 05  10.20584  13 59 02.91   -12 26 47.3   23.8R 99JD132   807  Ca5620      
1999 05  10.21271  13 59 02.88   -12 26 47.2   23.9R 99JD132   807  Ca5620      
1999 05  10.21958  13 59 02.84   -12 26 47.0   23.5R 99JD132   807  Ca5620      
1999 05  10.23333  13 59 02.78   -12 26 46.6   23.9R 99JD132   807  Ca5620      
1999 05  10.24708  13 59 02.71   -12 26 46.4   23.7R 99JD132   807  Ca5620      
1999 05  10.25395  13 59 02.69   -12 26 46.2   24.2R 99JD132   807  Ca5620      
1999 05  10.26082  13 59 02.65   -12 26 45.9   23.7R 99JD132   807  Ca5620      
1999 05  10.27456  13 59 02.60   -12 26 45.7   23.9R 99JD132   807  Ca5620      
1999 05  11.17804  13 58 58.62   -12 26 26.6   23.7R 99JD132   807  Ca5620      
1999 05  11.18491  13 58 58.59   -12 26 26.2   23.7R 99JD132   807  Ca5620      
1999 05  11.19178  13 58 58.56   -12 26 26.3   23.4R 99JD132   807  Ca5620      
1999 05  11.19865  13 58 58.54   -12 26 26.1   23.5R 99JD132   807  Ca5620      
1999 05  11.20553  13 58 58.50   -12 26 26.0   23.5R 99JD132   807  Ca5620      
1999 05  11.21239  13 58 58.47   -12 26 25.8   23.7R 99JD132   807  Ca5620      
1999 05  11.21926  13 58 58.44   -12 26 25.7   23.3R 99JD132   807  Ca5620      
1999 05  11.22613  13 58 58.40   -12 26 25.6   23.5R 99JD132   807  Ca5620      
1999 05  11.23300  13 58 58.37   -12 26 25.4   23.0R 99JD132   807  Ca5620      
1999 05  11.23987  13 58 58.34   -12 26 25.2   23.3R 99JD132   807  Ca5620      
1999 05  11.24674  13 58 58.31   -12 26 25.1   23.3R 99JD132   807  Ca5620      
1999 05  11.25362  13 58 58.28   -12 26 24.9   23.4R 99JD132   807  Ca5620      
1999 05  11.26048  13 58 58.25   -12 26 24.9   23.5R 99JD132   807  Ca5620      
1999 05  11.26735  13 58 58.22   -12 26 24.7   23.3R 99JD132   807  Ca5620      
1999 05  11.27422  13 58 58.20   -12 26 24.5   23.6R 99JD132   807  Ca5620      
1999 05  18.18001  13 58 28.65   -12 24 01.8   23.6R 99JD132   807  Ca5620      
1999 05  18.18765  13 58 28.63   -12 24 01.6   23.5R 99JD132   807  Ca5620      
1999 05  18.19452  13 58 28.60   -12 24 01.5   23.9R 99JD132   807  Ca5620      
1999 05  18.20139  13 58 28.58   -12 24 01.4   23.5R 99JD132   807  Ca5620      
1999 05  18.20826  13 58 28.55   -12 24 01.3   23.4R 99JD132   807  Ca5620      
1999 05  18.21515  13 58 28.52   -12 24 01.1   23.5R 99JD132   807  Ca5620      
1999 05  18.22202  13 58 28.49   -12 24 01.1   23.6R 99JD132   807  Ca5620      
1999 05  18.22889  13 58 28.46   -12 24 00.9   23.5R 99JD132   807  Ca5620      
1999 05  18.23605  13 58 28.43   -12 24 00.8   23.7R 99JD132   807  Ca5620      
1999 05  18.24293  13 58 28.40   -12 24 00.5   23.4R 99JD132   807  Ca5620      
1999 05  18.24980  13 58 28.37   -12 24 00.5   23.4R 99JD132   807  Ca5620      
1999 05  18.25677  13 58 28.35   -12 24 00.3   23.5R 99JD132   807  Ca5620      
1999 05  18.26364  13 58 28.32   -12 23 59.9   23.4R 99JD132   807  Ca5620      
1999 05  18.27050  13 58 28.29   -12 24 00.0   23.3R 99JD132   807  Ca5620      
1999 05  19.12854  13 58 24.75   -12 23 42.9   23.5R 99JD132   807  Ca5620      
1999 05  19.13541  13 58 24.72   -12 23 42.8   23.5R 99JD132   807  Ca5620      
1999 05  19.14229  13 58 24.70   -12 23 42.6   23.6R 99JD132   807  Ca5620      
1999 05  19.14915  13 58 24.67   -12 23 42.5   23.9R 99JD132   807  Ca5620      
1999 05  19.15607  13 58 24.64   -12 23 42.3   23.6R 99JD132   807  Ca5620      
1999 05  19.16294  13 58 24.61   -12 23 42.2   23.7R 99JD132   807  Ca5620      
1999 05  19.16982  13 58 24.58   -12 23 42.0   23.7R 99JD132   807  Ca5620      
1999 05  19.17669  13 58 24.56   -12 23 42.1   23.6R 99JD132   807  Ca5620      
1999 05  19.18356  13 58 24.53   -12 23 41.9   23.6R 99JD132   807  Ca5620      
1999 05  19.19043  13 58 24.49   -12 23 41.6   23.8R 99JD132   807  Ca5620      
1999 05  19.19730  13 58 24.47   -12 23 41.6   23.9R 99JD132   807  Ca5620      
1999 05  19.22727  13 58 24.34   -12 23 41.0   23.7R 99JD132   807  Ca5620      
1999 05  19.23442  13 58 24.31   -12 23 40.6   23.8R 99JD132   807  Ca5620      
1999 05  19.24130  13 58 24.28   -12 23 40.7   23.8R 99JD132   807  Ca5620      
1999 05  19.25504  13 58 24.23   -12 23 40.4   23.9R 99JD132   807  Ca5620      
1999 05  19.26191  13 58 24.19   -12 23 40.2   23.9R 99JD132   807  Ca5620      
1999 05  19.26878  13 58 24.17   -12 23 40.2   24.0R 99JD132   807  Ca5620      
2000 06  25.94209  14 01 07.21   -12 55 01.6         99JD132   950  Cb6484      
2000 06  25.97586  14 01 07.20   -12 55 01.4         99JD132   950  Cb6484      
2000 06  26.01143  14 01 07.11   -12 55 01.0         99JD132   950  Cb6484      
2000 06  26.93890  14 01 05.55   -12 54 54.4         99JD132   950  Cb6484      
2000 06  26.98511  14 01 05.45   -12 54 53.6         99JD132   950  Cb6484      
2006 04  26.22589  14 33 24.39   -17 06 23.4   22.1R 99JD132   807  Cr3547      
2006 04  26.31058  14 33 24.00   -17 06 21.7         99JD132   807  Cr3547      
2006 04  27.22965  14 33 19.65   -17 06 03.7         99JD132   807  Cr3547      
2018 04  10.33810  15 33 47.140  -23 55 08.76        99JD132   G37  C~2bGP      
2018 04  10.41361  15 33 46.727  -23 55 06.65        99JD132   G37  C~2bGP      

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    -0.17       0.00     0.13
     2   0.0000      0.00    -0.16       0.00     0.09
     3   0.0000      0.00    -0.15       0.00     0.14
     4   0.0001      0.00     0.02       0.00     0.09
     5   0.0001      0.00     0.03       0.00     0.04
     6   0.0001      0.00    -0.11       0.00     0.09
     7   0.0001      0.00    -0.08       0.00     0.20
     8   0.0002      0.00    -0.20       0.00     0.10
     9   0.0002      0.00    -0.04       0.00     0.15
    10   0.0002      0.00    -0.18       0.00     0.31
    11   0.0002      0.00    -0.01       0.00     0.21
    12   0.0027      0.00    -0.04       0.00     0.04
    13   0.0027      0.00    -0.03       0.00     0.29
    14   0.0028      0.00    -0.02       0.00     0.05
    15   0.0028      0.00     0.14       0.00     0.10
    16   0.0028      0.00     0.00       0.00     0.05
    17   0.0028      0.00     0.01       0.00     0.11
    18   0.0028      0.00     0.02       0.00     0.06
    19   0.0028      0.00    -0.12       0.00     0.01
    20   0.0029      0.00    -0.11       0.00     0.07
    21   0.0029      0.00    -0.10       0.00     0.12
    22   0.0029      0.00    -0.09       0.00     0.07
    23   0.0029      0.00    -0.08       0.00     0.12
    24   0.0029      0.00    -0.07       0.00    -0.02
    25   0.0030      0.00    -0.06       0.00     0.03
    26   0.0030      0.00     0.10       0.00     0.08
    27   0.0219      0.00    -0.14       0.00    -0.05
    28   0.0219      0.00     0.04       0.00    -0.00
    29   0.0219      0.00     0.03       0.00    -0.04
    30   0.0219      0.00     0.16       0.00    -0.08
    31   0.0220      0.00     0.15       0.00    -0.12
    32   0.0220      0.00     0.13       0.00    -0.06
    33   0.0220      0.00     0.12       0.00    -0.20
    34   0.0220      0.00     0.10       0.00    -0.13
    35   0.0220      0.00     0.10       0.00    -0.18
    36   0.0221      0.00     0.09       0.00    -0.02
    37   0.0221      0.00     0.07       0.00    -0.16
    38   0.0221      0.00     0.21       0.00    -0.10
    39   0.0221      0.00     0.19       0.00     0.16
    40   0.0221      0.00     0.17       0.00    -0.07
    41   0.0245      0.00     0.05       0.00    -0.06
    42   0.0245      0.00     0.03       0.00    -0.09
    43   0.0245      0.00     0.16       0.00    -0.03
    44   0.0245      0.00     0.14       0.00    -0.07
    45   0.0246      0.00     0.13       0.00    -0.00
    46   0.0246      0.00     0.11       0.00    -0.04
    47   0.0246      0.00     0.09       0.00     0.02
    48   0.0246      0.00     0.22       0.00    -0.21
    49   0.0246      0.00     0.20       0.00    -0.15
    50   0.0247      0.00     0.03       0.00     0.01
    51   0.0247      0.00     0.16       0.00    -0.12
    52   0.0248      0.00     0.09       0.00    -0.12
    53   0.0248      0.00     0.08       0.00     0.14
    54   0.0248      0.00     0.06       0.00    -0.10
    55   0.0248      0.00     0.17       0.00    -0.08
    56   0.0249      0.00    -0.00       0.00    -0.01
    57   0.0249      0.00     0.13       0.00    -0.15
    58   1.1301      0.00    -0.53       0.00    -0.13
    59   1.1302      0.00     0.24       0.00    -0.18
    60   1.1303      0.00    -0.16       0.00    -0.06
    61   1.1328      0.00    -0.09       0.00    -0.21
    62   1.1329      0.00    -0.40       0.00     0.26
    63   6.9625      0.00    -0.34       0.00    -0.32
    64   6.9627      0.00    -0.07       0.00    -0.29
    65   6.9652      0.00     0.04       0.00    -0.31
    66  18.9190      0.00     0.94       0.00    -0.60
    67  18.9192      0.00    -0.80       0.00     1.01

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.

99JD132    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.022    43.022    43.022
ecceobj         0.066     0.066     0.066
incobj         10.518    10.518    10.518
qmin           39.541    39.560    39.534
qmax           47.368    47.352    47.357
amean          43.330    43.330    43.330
amin           42.997    42.988    42.988
amax           43.692    43.682    43.682
emean           0.069     0.069     0.069
emin            0.056     0.056     0.056
emax            0.085     0.084     0.085
imean           9.714     9.714     9.714
imin            8.976     8.977     8.976
imax           10.323    10.324    10.325
excite_mean     0.183     0.183     0.183
fracstop        1.000     1.000     1.000
cjmean          3.053     3.053     3.053

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       181.0     181.1     180.8
kozaiamp        180.0     180.0     180.0