Orbit Fit and Astrometric record for 612166

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: 612166    
# Created Sun Apr 28 01:09:09 2024
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     65 observations of     65
# Arc:  21.12y
# First observation: 2000/07/31
#  Last observation: 2021/09/12
# Chi-squared of fit:   235.65 DOF:    124 RMS:  0.34
# Min/Max residuals:    -0.76    0.93
# Exact a, adot, b, bdot, g, gdot:
  1.500304E-05  2.147725E-02  1.174251E-06  1.825555E-04  2.306524E-02  3.793748E-04
# Covariance matrix:
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00  0.0000E+00
#      lat0       lon0       xBary       yBary       zBary        JD0
   -3.168426  -23.124887    0.489731   -0.049286   -0.887440  2451756.841063
# Heliocentric elements and errors
Epoch:              2451756.5000  =  2000/07/31
Mean Anomaly:          172.57116 +/-     0.000
Argument of Peri:      105.18507 +/-     0.000
Long of Asc Node:       58.10192 +/-     0.000
Inclination:             3.13591 +/-     0.000
Eccentricity:         0.02631289 +/-    0.0000
Semi-Major Axis:     43.12343223 +/-    0.0000
Time of Perihelion: 2402173.3494 +/-       0.0
Perihelion:          41.98873016 +/-    0.0000
Aphelion:            44.25813431 +/-    0.0000
Period (y)              283.1902 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X           40.44190722 +/-    0.0000
Ecliptic Y          -17.79584942 +/-    0.0000
Ecliptic Z           -2.39627087 +/-    0.0000
Ecliptic XDOT         0.00103655 +/-    0.0000
Ecliptic YDOT         0.00233196 +/-    0.0000
Ecliptic ZDOT         0.00001930 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   44.24909087 +/-    0.0000
Geocenter to KBO     43.35531195 +/-    0.0000
# Hcoef:  6.76

The following table shows the complete astrometric record for 612166. 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 (612166) followed by the observatory code and reference code for the source of the astrometry.

2000 07  31.34032  22 39 12.74   -11 55 43.1   22.6R 612166    807  Cc0956      
2000 07  31.42019  22 39 12.45   -11 55 44.9         612166    807  Cc0956      
2000 08  27.17980  22 37 22.47   -12 07 04.1   22.4R 612166    807  Cc0956      
2000 08  27.25472  22 37 22.13   -12 07 06.2         612166    807  Cc0956      
2000 09  21.20280  22 35 35.55   -12 17 06.9   22.5R 612166    695  Cc2364      
2000 09  21.28587  22 35 35.15   -12 17 09.2         612166    695  Cc2364      
2000 11  28.10022  22 33 22.94   -12 25 38.2   22.7R 612166    695  Cc3775      
2000 11  29.10082  22 33 23.75   -12 25 28.9   22.9R 612166    695  Cc3775      
2001 07  23.42834  22 44 19.156  -11 24 17.39        612166    568  Cl5584      
2001 07  23.49718  22 44 18.901  -11 24 19.06        612166    568  Cl5584      
2001 09  19.16421  22 40 24.35   -11 48 08.8         612166    695  Cd5762      
2001 09  19.33083  22 40 23.65   -11 48 13.1         612166    695  Cd5762      
2001 09  22.17673  22 40 12.08   -11 49 15.8         612166    290  Cd5762      
2001 09  22.20024  22 40 11.95   -11 49 16.6         612166    290  Cd5762      
2001 10  11.04564  22 39 03.49   -11 55 11.4   20.2  612166    304  Ce8850      
2001 10  11.07439  22 39 03.39   -11 55 12.1         612166    304  Ce8850      
2002 07  10.21546  22 49 32.09   -10 51 22.7   22.6R 612166    304  Cf9760      
2002 07  10.43898  22 49 31.57   -10 51 26.6         612166    304  Cf9760      
2002 07  12.36340  22 49 27.01   -10 51 59.5         612166    304  Cf9760      
2002 07  12.38310  22 49 26.95   -10 51 59.8         612166    304  Cf9760      
2002 07  13.35810  22 49 24.56   -10 52 17.8         612166    304  Cf9760      
2002 07  13.39053  22 49 24.49   -10 52 18.6         612166    304  Cf9760      
2007 05  10.20587  23 11 33.51   -08 25 50.7   22.9R 612166    250  S~06AN      
2007 05  10.21281  23 11 33.52   -08 25 50.7         612166    250  S~06AN      
2007 05  10.22045  23 11 33.54   -08 25 50.6         612166    250  S~06AN      
2007 05  10.27531  23 11 33.71   -08 25 49.8         612166    250  S~06AN      
2009 10  16.156939 23 15 21.47   -08 04 15.1         612166    645  C~1GLG      
2009 10  16.157769 23 15 21.46   -08 04 15.1         612166    645  C~1GLG      
2009 10  16.160256 23 15 21.45   -08 04 15.0         612166    645  C~1GLG      
2014 07  28.53780  23 42 57.219  -04 59 14.07  23.3G 612166    F51  C~2rXd      
2014 08  03.52799  23 42 41.416  -05 01 13.23  22.8G 612166    F51  C~2rXd      
2014 08  03.53933  23 42 41.364  -05 01 13.49  23.3G 612166    F51  C~2rXd      
2014 08  03.55064  23 42 41.320  -05 01 13.90  23.7G 612166    F51  C~2rXd      
2014 08  03.56194  23 42 41.327  -05 01 14.03  23.4G 612166    F51  C~2rXd      
2014 08  04.51886  23 42 38.563  -05 01 34.04  23.9G 612166    F51  C~2rXd      
2014 08  20.48054  23 41 45.795  -05 07 49.27  23.3G 612166    F51  C~2rXd      
2014 08  22.50230  23 41 38.260  -05 08 41.37  23.0G 612166    F51  C~2rXd      
2014 08  23.52404  23 41 34.379  -05 09 07.21  21.2G 612166    F51  C~2rXd      
2014 11  11.29426  23 36 37.825  -05 39 00.10  22.8G 612166    F51  C~2rXd      
2014 11  26.25318  23 36 14.889  -05 40 23.73  23.4G 612166    F51  C~2rXd      
2015 09  09.41690  23 44 56.050  -04 45 40.72  23.0G 612166    F51  C~2rXd      
2015 09  09.42905  23 44 55.996  -04 45 40.70  23.7G 612166    F51  C~2rXd      
2015 09  09.44122  23 44 55.940  -04 45 40.97  23.1G 612166    F51  C~2rXd      
2015 09  09.45342  23 44 55.902  -04 45 41.58  23.3G 612166    F51  C~2rXd      
2015 09  12.39454  23 44 43.468  -04 47 02.67  23.5G 612166    F51  C~2rXd      
2015 09  12.40629  23 44 43.425  -04 47 02.90  22.6G 612166    F51  C~2rXd      
2015 09  12.41804  23 44 43.392  -04 47 03.02  23.4G 612166    F51  C~2rXd      
2015 09  12.42981  23 44 43.330  -04 47 03.56  23.7G 612166    F51  C~2rXd      
2015 10  29.30197  23 41 39.452  -05 05 31.94  23.3G 612166    F51  C~2rXd      
2015 11  02.30643  23 41 27.669  -05 06 34.34  23.1G 612166    F51  C~2rXd      
2017 08  01.54515  23 56 05.810  -03 28 02.12  22.8G 612166    F51  C~2rXd      
2017 08  01.56895  23 56 05.774  -03 28 01.98  23.6G 612166    F51  C~2rXd      
2017 08  03.52437  23 56 00.807  -03 28 39.66  23.4G 612166    F51  C~2rXd      
2017 09  14.45116  23 53 29.488  -03 46 03.30  22.6G 612166    F51  C~2rXd      
2017 09  17.38477  23 53 17.021  -03 47 24.22  22.9G 612166    F51  C~2rXd      
2017 09  25.41391  23 52 42.740  -03 51 02.52  23.0G 612166    F51  C~2rXd      
2017 09  28.43034  23 52 29.911  -03 52 22.63  23.2G 612166    F51  C~2rXd      
2017 11  13.31793  23 49 51.493  -04 07 30.26  23.1G 612166    F51  C~2rXd      
2018 01  06.23418  23 49 51.233  -04 03 34.67  23.5G 612166    F51  C~2rXd      
2018 09  14.326400 23 57 59.32   -03 14 38.7   23.4G 612166    705  C~2r9h      
2018 09  14.374030 23 57 59.10   -03 14 40.0   23.1G 612166    705  C~2r9h      
2018 09  14.423360 23 57 58.90   -03 14 41.4   23.2G 612166    705  C~2r9h      
2021 09  12.315900 00 11 32.213  -01 39 27.99  23.2G 612166    G37  C~552i      
2021 09  12.375810 00 11 31.962  -01 39 29.48        612166    G37  C~552i      
2021 09  12.436290 00 11 31.705  -01 39 31.19        612166    G37  C~552i      

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    -0.22
     2   0.0002      0.00     0.16       0.00    -0.12
     3   0.0735      0.00     0.38       0.00    -0.21
     4   0.0737      0.00     0.28       0.00    -0.38
     5   0.1420      0.00     0.33       0.00     0.24
     6   0.1422      0.00    -0.57       0.00    -0.27
     7   0.3279      0.00     0.17       0.00    -0.39
     8   0.3306      0.00     0.19       0.00    -0.63
     9   0.9777      0.00     0.51       0.00    -0.33
    10   0.9778      0.00     0.07       0.00    -0.48
    11   1.1357      0.00     0.23       0.00     0.17
    12   1.1362      0.00     0.20       0.00    -0.36
    13   1.1440      0.00     0.25       0.00     0.24
    14   1.1440      0.00    -0.25       0.00    -0.04
    15   1.1956      0.00    -0.32       0.00    -0.50
    16   1.1957      0.00    -0.43       0.00    -0.76
    17   1.9408      0.00     0.25       0.00    -0.31
    18   1.9414      0.00     0.31       0.00    -0.34
    19   1.9467      0.00    -0.28       0.00     0.87
    20   1.9467      0.00    -0.44       0.00     0.93
    21   1.9494      0.00    -0.46       0.00     0.73
    22   1.9495      0.00    -0.26       0.00     0.52
    23   6.7731      0.00    -0.40       0.00     0.89
    24   6.7731      0.00    -0.56       0.00     0.79
    25   6.7731      0.00    -0.61       0.00     0.77
    26   6.7733      0.00    -0.58       0.00     0.72
    27   9.2096      0.00     0.56       0.00     0.28
    28   9.2096      0.00     0.45       0.00     0.29
    29   9.2096      0.00     0.43       0.00     0.44
    30  13.9910      0.00     0.10       0.00    -0.20
    31  14.0074      0.00     0.19       0.00    -0.22
    32  14.0074      0.00    -0.10       0.00    -0.24
    33  14.0074      0.00    -0.27       0.00    -0.42
    34  14.0075      0.00     0.33       0.00    -0.31
    35  14.0101      0.00    -0.20       0.00    -0.13
    36  14.0538      0.00    -0.06       0.00     0.01
    37  14.0593      0.00    -0.06       0.00    -0.25
    38  14.0621      0.00    -0.23       0.00     0.39
    39  14.2805      0.00    -0.35       0.00    -0.03
    40  14.3215      0.00    -0.09       0.00    -0.19
    41  15.1077      0.00    -0.07       0.00    -0.17
    42  15.1077      0.00    -0.10       0.00     0.19
    43  15.1077      0.00    -0.16       0.00     0.25
    44  15.1078      0.00     0.06       0.00    -0.03
    45  15.1158      0.00    -0.10       0.00    -0.25
    46  15.1159      0.00     0.02       0.00    -0.16
    47  15.1159      0.00     0.28       0.00     0.05
    48  15.1159      0.00     0.12       0.00    -0.17
    49  15.2442      0.00     0.11       0.00    -0.17
    50  15.2552      0.00     0.14       0.00    -0.14
    51  17.0026      0.00    -0.35       0.00    -0.61
    52  17.0027      0.00     0.02       0.00    -0.01
    53  17.0080      0.00     0.08       0.00     0.03
    54  17.1228      0.00    -0.08       0.00     0.13
    55  17.1309      0.00     0.01       0.00    -0.11
    56  17.1528      0.00     0.25       0.00    -0.04
    57  17.1611      0.00    -0.00       0.00     0.15
    58  17.2867      0.00    -0.08       0.00     0.23
    59  17.4343      0.00    -0.13       0.00    -0.14
    60  18.1218      0.00     0.24       0.00    -0.11
    61  18.1219      0.00     0.00       0.00    -0.10
    62  18.1221      0.00     0.17       0.00    -0.14
    63  21.1170      0.00     0.09       0.00     0.15
    64  21.1171      0.00     0.10       0.00     0.29
    65  21.1173      0.00     0.05       0.00     0.23

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.

612166    quality flag:3

Type:      CLASSICAL CLASSICAL CLASSICAL

axisobj        43.200    43.200    43.200
ecceobj         0.025     0.025     0.025
incobj          3.136     3.136     3.136
qmin           40.618    40.618    40.620
qmax           45.628    45.633    45.620
amean          43.050    43.050    43.050
amin           42.724    42.724    42.723
amax           43.396    43.397    43.396
emean           0.033     0.033     0.033
emin            0.013     0.013     0.013
emax            0.052     0.052     0.052
imean           1.673     1.673     1.673
imin            0.681     0.681     0.681
imax            2.533     2.533     2.533
excite_mean     0.045     0.045     0.045
fracstop        1.000     1.000     1.000
cjmean          3.088     3.088     3.088

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       173.2     173.2     173.2
kozaiamp        180.0     180.0     179.9