Orbit Fit and Astrometric record for 99JJ132

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: 99JJ132   
# Created Thu Apr 25 01:09:52 2024
# Orbit generated from Bernstein formalism
# Fitting      4 observations of      4
# Arc:   8.97d
# First observation: 1999/05/10
#  Last observation: 1999/05/19
Preliminary a, adot, b, bdot, g, gdot:
   0.000000   0.017583   0.000000   0.000993   0.020293   0.000000
# WARNING Fitting with energy constraint
# WARNING MRQMIN stopped after  16 iterations -- oscilliatory solution
# Chi-squared of fit:     0.88 DOF:      3 RMS:  0.08
# Min/Max residuals:    -0.13    0.14
# Exact a, adot, b, bdot, g, gdot:
  1.261870E-05  1.556475E-02  9.225653E-07  9.924135E-04  1.996071E-02 -8.433137E-03
# Covariance matrix:
  1.7385E-10  2.0819E-07  1.0059E-13  1.7493E-10  3.5901E-08  2.5218E-07
  2.0819E-07  2.5051E-04  1.2103E-10  2.1045E-07  4.3191E-05  3.0316E-04
  1.0059E-13  1.2103E-10  7.6830E-13 -3.4750E-11  2.0865E-11  1.4164E-10
  1.7493E-10  2.1045E-07 -3.4750E-11  3.2084E-09  3.6284E-08  2.5704E-07
  3.5901E-08  4.3191E-05  2.0865E-11  3.6284E-08  7.4465E-06  5.2301E-05
  2.5218E-07  3.0316E-04  1.4164E-10  2.5704E-07  5.2301E-05  4.5281E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
    0.123029 -147.793632   -0.290598    0.001876   -0.973199  2451308.724553
# Heliocentric elements and errors
Epoch:              2451300.5000  =  1999/05/02
Mean Anomaly:          298.89621 +/-    77.041
Argument of Peri:      118.50152 +/-    99.586
Long of Asc Node:      210.64547 +/-     1.837
Inclination:             3.65279 +/-     3.633
Eccentricity:         0.47301845 +/-    1.2812
Semi-Major Axis:     51.84824907 +/-   26.8205
Time of Perihelion: 2474445.9277 +/-   23001.5
Perihelion:          27.32307048 +/-   67.9172
Aphelion:            76.37342767 +/-   77.2903
Period (y)              373.3441 +/-    289.69
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -43.05001178 +/-    5.7954
Ecliptic Y          -27.46515527 +/-    3.6498
Ecliptic Z            0.10761301 +/-    0.0147
Ecliptic XDOT         0.00211413 +/-    0.0017
Ecliptic YDOT        -0.00118107 +/-    0.0031
Ecliptic ZDOT         0.00013366 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   51.06515298 +/-    5.2654
Geocenter to KBO     50.09840810 +/-    6.8490
# Hcoef:  8.75

The following table shows the complete astrometric record for 99JJ132. 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 (99JJ132) followed by the observatory code and reference code for the source of the astrometry.

1999 05  10.22381  14 00 16.19   -12 07 27.4   25.3R 99JJ132   807  Ca5911      
1999 05  11.22386  14 00 12.47   -12 07 06.8   25.6R 99JJ132   807  Ca5911      
1999 05  18.21988  13 59 47.11   -12 04 46.4   25.4R 99JJ132   807  Ca5911      
1999 05  19.19404  13 59 43.70   -12 04 27.8   25.6R 99JJ132   807  Ca5911      

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    -0.06       0.00    -0.03
     2   0.0027    -58.31     0.09       0.56     0.02
     3   0.0219   -455.86    -0.05       4.23     0.14
     4   0.0246   -509.23     0.05       4.45    -0.13

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.

99JJ132    quality flag:0

Type:      ERR2LARGE ERR2LARGE ERR2LARGE

axisobj         0.000     0.000     0.000
ecceobj        -1.000    -1.000    -1.000
incobj         -1.000    -1.000    -1.000
qmin            0.000     0.000     0.000
qmax            0.000     0.000     0.000
amean           0.000     0.000     0.000
amin            0.000     0.000     0.000
amax            0.000     0.000     0.000
emean           0.000     0.000     0.000
emin            0.000     0.000     0.000
emax            0.000     0.000     0.000
imean           0.000     0.000     0.000
imin            0.000     0.000     0.000
imax            0.000     0.000     0.000
excite_mean     0.000     0.000     0.000
fracstop        0.000     0.000     0.000
cjmean          0.000     0.000     0.000

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         0.0       0.0       0.0
kozaiamp          0.0       0.0       0.0