Orbit Fit and Astrometric record for 93RP

The following information shows the result of the orbit fit based on Gary Bernstein's method. Most of the information should be self-explanatory.

# Object: 93RP      
# Created Fri May  2 02:36:25 2008
# Orbit generated from Bernstein formalism
# Fitting    6 observations of    6
# Arc:   2.00d
# First observation: 1993/09/15
#  Last observation: 1993/09/17
# WARNING Fitting with energy constraint
# WARNING and with gdot fixed = 0
# WARNING MRQMIN stopped after  13 iterations -- oscilliatory solution
# Chi-squared of fit:     2.43 DOF:    8 RMS:  0.11
# Min/Max residuals:    -0.23    0.21
# Exact a, adot, b, bdot, g, gdot:
  1.570208E-05  3.069954E-02 -5.552397E-07 -1.491890E-03  2.904286E-02  0.000000E+00
# Covariance matrix:
  4.4520E-11  8.0876E-08 -2.5467E-14  2.8201E-11  1.3676E-08  0.0000E+00
  8.0876E-08  1.4905E-04 -4.6875E-11  5.1893E-08  2.5159E-05  0.0000E+00
 -2.5467E-14 -4.6875E-11  4.9683E-13 -1.1451E-10 -7.9144E-12  0.0000E+00
  2.8201E-11  5.1893E-08 -1.1451E-10  5.2026E-08  8.7621E-09  0.0000E+00
  1.3676E-08  2.5159E-05 -7.9144E-12  8.7621E-09  4.2483E-06  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  3.2236E-04
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.029523   13.310070    0.348016   -0.000438   -0.944317  2449245.996997
# Heliocentric elements and errors
Epoch:              2449240.5000  =  1993/09/10
Mean Anomaly:          269.09370 +/-   143.977
Argument of Peri:      272.51329 +/-    74.974
Long of Asc Node:      192.14879 +/-     0.289
Inclination:             2.78986 +/-     1.195
Eccentricity:         0.00909657 +/-    0.5852
Semi-Major Axis:     35.36721881 +/-   18.1946
Time of Perihelion: 2468640.0333 +/-  798829.7
Perihelion:          35.04549852 +/-   27.4495
Aphelion:            35.68893910 +/-   27.6681
Period (y)              210.3340 +/-    162.31
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           34.50434144 +/-    2.3780
Ecliptic Y            7.80044610 +/-    0.5624
Ecliptic Z           -0.01775143 +/-    0.0013
Ecliptic XDOT        -0.00066262 +/-    0.0017
Ecliptic YDOT         0.00281145 +/-    0.0010
Ecliptic ZDOT        -0.00014073 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   35.37508802 +/-    2.3228
Geocenter to KBO     34.43187275 +/-    2.4436
# Hcoef:  9.36

The following table shows the complete astrometric record for 93RP. 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 (93RP) followed by the observatory code and reference code for the source of the astrometry.

1993 09  15.4963   00 49 01.88   +05 13 37.6   24.5R 93RP      568  C22539      
1993 09  15.5850   00 49 01.42   +05 13 34.8         93RP      568  C22539      
1993 09  16.4558   00 48 57.17   +05 13 07.0         93RP      568  C22539      
1993 09  16.4976   00 48 56.97   +05 13 05.8         93RP      568  C22539      
1993 09  17.4630   00 48 52.23   +05 12 35.1         93RP      568  C22539      
1993 09  17.4964   00 48 52.06   +05 12 33.8         93RP      568  C22539      

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     0.21       0.00    -0.05
  2   0.0002     -7.42    -0.06       0.09     0.07
  3   0.0026    -76.72    -0.23      -0.84    -0.05
  4   0.0027    -79.94    -0.05      -0.79     0.02
  5   0.0054   -157.11     0.13      -1.55     0.11
  6   0.0055   -159.95     0.02      -1.76    -0.09

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.

93RP    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
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