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. Take special note that while the original Bernstein software works with barycentric coordinates, we convert these results into a heliocentric coordinate system.

# Object: 93RP      
# Created Fri Nov 22 02:07:53 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     37 observations of     37
# Arc:  23.13y
# First observation: 1993/09/15
#  Last observation: 2016/11/02
# Chi-squared of fit:    38.58 DOF:     68 RMS:  0.18
# Min/Max residuals:    -0.59    0.75
# Exact a, adot, b, bdot, g, gdot:
  1.788474E-05  3.072626E-02  1.304794E-06 -2.330385E-03  2.918735E-02 -1.452844E-03
# Covariance matrix:
  2.4462E-13 -1.7103E-14 -6.7668E-17  4.7869E-16 -5.2733E-15 -7.2047E-15
 -1.7103E-14  6.0815E-14  5.9768E-16 -4.5294E-15  7.6820E-14  6.7985E-14
 -6.7668E-17  5.9768E-16  2.4382E-13 -1.0849E-14  6.6462E-16  6.7757E-16
  4.7869E-16 -4.5294E-15 -1.0849E-14  8.7007E-16 -5.6712E-15 -5.1115E-15
 -5.2733E-15  7.6820E-14  6.6462E-16 -5.6712E-15  1.4912E-13  8.4758E-14
 -7.2047E-15  6.7985E-14  6.7757E-16 -5.1115E-15  8.4758E-14  7.6737E-14
#      lat0       lon0       xBary       yBary       zBary        JD0
   -0.029523   13.310070    0.348016   -0.000438   -0.944317  2449245.996997
# Heliocentric elements and errors
Epoch:              2449246.5000  =  1993/09/16
Mean Anomaly:          265.45510 +/-     0.034
Argument of Peri:      281.36531 +/-     0.029
Long of Asc Node:      192.35959 +/-     0.000
Inclination:             4.34990 +/-     0.000
Eccentricity:         0.05681729 +/-    0.0000
Semi-Major Axis:     34.93618791 +/-    0.0014
Time of Perihelion: 2469054.8047 +/-       7.9
Perihelion:          32.95120835 +/-    0.0014
Aphelion:            36.92116747 +/-    0.0015
Period (y)              206.5007 +/-      0.01
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           34.33845393 +/-    0.0004
Ecliptic Y            7.76127527 +/-    0.0001
Ecliptic Z           -0.01759976 +/-    0.0000
Ecliptic XDOT        -0.00079256 +/-    0.0000
Ecliptic YDOT         0.00276856 +/-    0.0000
Ecliptic ZDOT        -0.00021862 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   35.20467837 +/-    0.0004
Geocenter to KBO     34.26148672 +/-    0.0005
# Hcoef:  9.11

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      
2015 08  20.56332  03 27 16.771  +15 58 01.35  24.8w 93RP      568  C~4nAh      
2015 09  07.60859  03 27 12.469  +15 55 54.67  24.6w 93RP      568  C~4nAh      
2015 09  12.45964  03 27 04.912  +15 54 58.30  24.6w 93RP      568  C~4nAh      
2015 10  07.50935  03 25 46.483  +15 47 58.02  24.6w 93RP      568  C~4nAh      
2015 10  07.56783  03 25 46.221  +15 47 56.93  24.8w 93RP      568  C~4nAh      
2015 10  09.54866  03 25 37.532  +15 47 15.86  24.6w 93RP      568  C~4nAh      
2015 11  06.32308  03 23 09.611  +15 36 35.05  23.9r 93RP      568  C~4nAh      
2015 11  06.38643  03 23 09.249  +15 36 33.32  24.2r 93RP      568  C~4nAh      
2015 11  06.45719  03 23 08.817  +15 36 32.06  24.5r 93RP      568  C~4nAh      
2015 11  07.47849  03 23 02.757  +15 36 07.12  24.5w 93RP      568  C~4nAh      
2015 11  17.45967  03 22 02.854  +15 32 07.99  24.5w 93RP      568  C~4nAh      
2015 11  17.54796  03 22 02.302  +15 32 05.91  24.4w 93RP      568  C~4nAh      
2015 12  06.32589  03 20 12.788  +15 25 11.15  24.8w 93RP      568  C~4nAh      
2015 12  06.45961  03 20 12.047  +15 25 08.43  24.6w 93RP      568  C~4nAh      
2015 12  31.37031  03 18 15.345  +15 18 31.36  24.6w 93RP      568  C~4nAh      
2016 01  07.39971  03 17 51.999  +15 17 23.72  24.7w 93RP      568  C~4nAh      
2016 02  05.29926  03 17 14.152  +15 16 51.31  24.9w 93RP      568  C~4nAh      
2016 02  11.25262  03 17 18.864  +15 17 35.09  24.7w 93RP      568  C~4nAh      
2016 09  07.60834  03 34 51.127  +16 16 40.42  25.0w 93RP      568  C~4nAh      
2016 09  27.53529  03 34 05.904  +16 12 06.31  24.8w 93RP      568  C~4nAh      
2016 10  07.52743  03 33 27.958  +16 09 02.87        93RP      568  C~4nAh      
2016 10  07.53507  03 33 27.942  +16 09 02.44        93RP      568  C~4nAh      
2016 10  07.62286  03 33 27.566  +16 09 00.71  24.6w 93RP      568  C~4nAh      
2016 10  09.52781  03 33 19.322  +16 08 22.92  24.2w 93RP      568  C~4nAh      
2016 10  09.59992  03 33 18.994  +16 08 21.40  24.8w 93RP      568  C~4nAh      
2016 10  10.55675  03 33 14.732  +16 08 02.07  24.6w 93RP      568  C~4nAh      
2016 10  10.60523  03 33 14.516  +16 08 01.06  24.8w 93RP      568  C~4nAh      
2016 10  28.47637  03 31 43.236  +16 01 30.75  24.5w 93RP      568  C~4nAh      
2016 10  29.53828  03 31 37.223  +16 01 06.43  24.6w 93RP      568  C~4nAh      
2016 10  29.55586  03 31 37.119  +16 01 05.89  24.5w 93RP      568  C~4nAh      
2016 11  02.59127  03 31 13.906  +15 59 32.45  24.7w 93RP      568  C~4nAh      

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    -0.03       0.00    -0.59
     2   0.0002      0.00    -0.31       0.00    -0.52
     3   0.0026      0.00    -0.20       0.00    -0.16
     4   0.0027      0.00    -0.05       0.00    -0.01
     5   0.0054      0.00     0.32       0.00     0.75
     6   0.0055      0.00     0.31       0.00     0.54
     7  21.9276      0.00     0.03       0.00     0.08
     8  21.9770      0.00     0.09       0.00    -0.04
     9  21.9903      0.00     0.11       0.00     0.06
    10  22.0589      0.00    -0.04       0.00     0.05
    11  22.0591      0.00    -0.09       0.00     0.16
    12  22.0645      0.00     0.02       0.00     0.05
    13  22.1405      0.00    -0.17       0.00     0.00
    14  22.1407      0.00     0.11       0.00    -0.21
    15  22.1409      0.00     0.03       0.00     0.23
    16  22.1437      0.00     0.05       0.00    -0.02
    17  22.1710      0.00    -0.01       0.00    -0.01
    18  22.1713      0.00    -0.20       0.00     0.02
    19  22.2227      0.00    -0.17       0.00    -0.10
    20  22.2230      0.00    -0.02       0.00    -0.13
    21  22.2912      0.00     0.12       0.00    -0.04
    22  22.3105      0.00     0.14       0.00     0.03
    23  22.3896      0.00    -0.02       0.00     0.00
    24  22.4059      0.00     0.07       0.00     0.08
    25  22.9791      0.00    -0.05       0.00     0.01
    26  23.0336      0.00     0.04       0.00     0.02
    27  23.0610      0.00    -0.23       0.00     0.19
    28  23.0610      0.00     0.03       0.00    -0.09
    29  23.0613      0.00     0.12       0.00    -0.08
    30  23.0665      0.00     0.08       0.00     0.00
    31  23.0667      0.00     0.05       0.00    -0.06
    32  23.0693      0.00    -0.03       0.00    -0.05
    33  23.0694      0.00     0.07       0.00    -0.06
    34  23.1184      0.00     0.15       0.00    -0.04
    35  23.1213      0.00    -0.00       0.00     0.08
    36  23.1213      0.00    -0.04       0.00    -0.06
    37  23.1324      0.00    -0.09       0.00    -0.03

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:3

Type:           5:4E      5:4E      5:4E

axisobj        35.314    35.314    35.314
ecceobj         0.059     0.059     0.059
incobj          4.326     4.326     4.326
qmin           32.506    32.437    32.463
qmax           37.961    37.906    37.892
amean          34.950    34.951    34.950
amin           34.512    34.527    34.512
amax           35.383    35.386    35.386
emean           0.044     0.044     0.044
emin            0.012     0.011     0.014
emax            0.073     0.072     0.072
imean           3.852     3.877     3.822
imin            2.799     2.759     2.779
imax            4.865     4.909     4.851
excite_mean     0.081     0.081     0.081
fracstop        1.000     1.000     1.000
cjmean          3.009     3.009     3.009

libcent 0       185.4     178.6     179.3
libamp  0       145.4     144.7     140.8
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       180.0     179.4     180.1
kozaiamp        180.0     180.0     180.0