Orbit Fit and Astrometric record for 773892

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: 773892    
# Created Sat Feb 22 02:07:56 2025
# Orbit generated by ELGB
# -->Covariance matrix from a Bernstein fit
# Fitting     50 observations of     50
# Arc:  18.58y
# First observation: 2005/03/12
#  Last observation: 2023/10/09
# Chi-squared of fit:    38.85 DOF:     94 RMS:  0.16
# Min/Max residuals:    -0.40    0.64
# Exact a, adot, b, bdot, g, gdot:
  2.709289E-05  1.453827E-01 -2.871055E-06 -1.477194E-02  8.464322E-02 -2.606207E-02
# 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
   19.450915  171.245091   -0.007826    0.329598   -0.933026  2453441.801100
# Heliocentric elements and errors
Epoch:              2453442.5000  =  2005/03/13
Mean Anomaly:          278.76150 +/-     0.000
Argument of Peri:      209.06150 +/-     0.000
Long of Asc Node:       62.28856 +/-     0.000
Inclination:            18.92736 +/-     0.000
Eccentricity:         0.17225343 +/-    0.0000
Semi-Major Axis:     12.71279643 +/-    0.0000
Time of Perihelion: 2457178.6084 +/-       0.0
Perihelion:          10.52297369 +/-    0.0000
Aphelion:            14.90261916 +/-    0.0000
Period (y)               45.3283 +/-      0.00
# Ecliptic coordinates at JD0 (AU and AU/d)
Ecliptic X          -11.99378865 +/-    0.0000
Ecliptic Y            1.83795978 +/-    0.0000
Ecliptic Z            3.93413701 +/-    0.0000
Ecliptic XDOT        -0.00008729 +/-    0.0000
Ecliptic YDOT        -0.00475164 +/-    0.0000
Ecliptic ZDOT        -0.00073119 +/-    0.0000
# Distances at JD0 (AU)
Heliocenter to KBO   12.75570155 +/-    0.0000
Geocenter to KBO     11.81439397 +/-    0.0000
# Hcoef: 11.45

The following table shows the complete astrometric record for 773892. 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 (773892) followed by the observatory code and reference code for the source of the astrometry.

2005 03  12.300357 12 00 11.53   +21 15 38.1   21.9r 773892    645  C~5rIu      
2005 03  12.301187 12 00 11.52   +21 15 38.2   21.9i 773892    645  C~5rIu      
2005 03  12.303674 12 00 11.48   +21 15 38.5   22.5g 773892    645  C~5rIu      
2013 05  05.273552 16 31 27.54   -23 53 38.7         773892    W84  C~5rIu      
2013 05  05.275614 16 31 27.50   -23 53 38.6         773892    W84  C~5rIu      
2013 05  30.245727 16 24 09.16   -23 55 38.1         773892    W84  C~5rIu      
2013 05  30.251049 16 24 09.06   -23 55 38.0         773892    W84  C~5rIu      
2017 08  08.049157 19 51 49.70   -38 00 09.9         773892    W84  C~5rIu      
2018 10  26.033167 20 41 45.60   -36 28 21.1         773892    W84  C~5rIu      
2018 10  26.089756 20 41 45.96   -36 28 15.1         773892    W84  C~5rIu      
2019 06  27.224917 21 59 27.75   -33 10 07.9         773892    W84  C~5rIu      
2020 11  07.122390 22 22 07.83   -30 58 23.0         773892    W84  C~5rIu      
2021 07  20.564569 23 27 19.160  -25 30 46.61  22.4G 773892    F51  C~5rIu      
2021 07  20.574260 23 27 19.104  -25 30 48.13  21.2G 773892    F51  C~5rIu      
2021 07  20.583920 23 27 19.062  -25 30 48.74  21.7G 773892    F51  C~5rIu      
2021 07  20.593603 23 27 18.958  -25 30 50.00  22.6G 773892    F51  C~5rIu      
2021 08  18.384812 23 22 08.90   -26 29 11.4   21.4i 773892    W84  C~5rIu      
2021 09  07.436763 23 17 00.460  -27 02 06.28  22.0G 773892    F52  C~5rIu      
2021 09  07.446949 23 17 00.286  -27 02 07.04  22.0G 773892    F52  C~5rIu      
2021 09  07.467328 23 16 59.950  -27 02 08.52  22.2G 773892    F52  C~5rIu      
2021 09  08.422662 23 16 44.517  -27 03 23.61  22.0G 773892    F51  C~5rIu      
2021 09  08.435166 23 16 44.307  -27 03 24.57  22.0G 773892    F51  C~5rIu      
2021 09  08.448481 23 16 44.084  -27 03 25.75  22.1G 773892    F51  C~5rIu      
2021 09  08.461962 23 16 43.864  -27 03 26.76  22.0G 773892    F51  C~5rIu      
2021 09  08.565753 23 16 42.151  -27 03 34.66  21.6G 773892    F51  C~5rIu      
2021 10  02.371738 23 10 31.593  -27 22 17.61  22.8G 773892    F51  C~5rIu      
2021 10  02.381421 23 10 31.462  -27 22 17.49  22.3G 773892    F51  C~5rIu      
2021 10  02.391096 23 10 31.331  -27 22 17.42  22.0G 773892    F51  C~5rIv      
2021 10  30.268018 23 05 26.136  -27 10 17.73  22.1G 773892    F52  C~5rIv      
2021 10  30.276924 23 05 26.075  -27 10 16.97  22.1G 773892    F52  C~5rIv      
2021 10  30.285867 23 05 26.014  -27 10 16.16  22.1G 773892    F52  C~5rIv      
2022 08  30.468151 23 58 13.306  -21 49 53.44  22.6G 773892    F52  C~5rIv      
2022 08  31.489266 23 57 59.088  -21 51 40.88  22.3G 773892    F52  C~5rIv      
2022 08  31.500133 23 57 58.936  -21 51 41.81  22.3G 773892    F52  C~5rIv      
2022 08  31.521814 23 57 58.636  -21 51 43.97  21.9G 773892    F52  C~5rIv      
2022 09  20.424247 23 53 00.074  -22 21 20.34  22.5w 773892    F51  C~5rIv      
2022 09  20.435417 23 52 59.877  -22 21 21.12  22.2w 773892    F51  C~5rIv      
2022 09  20.446532 23 52 59.715  -22 21 22.01  22.3w 773892    F51  C~5rIv      
2022 09  20.457529 23 52 59.531  -22 21 22.69  22.1w 773892    F51  C~5rIv      
2022 09  23.384707 23 52 14.136  -22 24 40.57  22.2G 773892    568  C~5rIv      
2022 09  23.385915 23 52 14.120  -22 24 40.62  22.0G 773892    568  C~5rIv      
2022 09  23.387122 23 52 14.100  -22 24 40.71  22.0G 773892    568  C~5rIv      
2022 09  26.361736 23 51 28.127  -22 27 41.82  21.5G 773892    F51  C~5rIv      
2022 09  26.372849 23 51 27.968  -22 27 42.33  21.7G 773892    F51  C~5rIv      
2023 09  11.423714 00 30 05.748  -16 59 02.66  22.1w 773892    F52  C~79O1      
2023 09  11.434632 00 30 05.578  -16 59 03.79  22.5w 773892    F52  C~79O1      
2023 09  11.445549 00 30 05.426  -16 59 04.45  21.9w 773892    F52  C~79O1      
2023 10  09.371568 00 23 14.911  -17 33 32.53  22.4w 773892    F51  C~7BoG      
2023 10  09.382784 00 23 14.715  -17 33 33.00  22.5w 773892    F51  C~7BoG      
2023 10  09.395571 00 23 14.543  -17 33 33.73  22.3w 773892    F51  C~7BoG      

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     0.02       0.00     0.02
     2   0.0000      0.00     0.06       0.00     0.04
     3   0.0000      0.00     0.01       0.00     0.13
     4   8.1478      0.00     0.07       0.00    -0.05
     5   8.1478      0.00    -0.03       0.00     0.07
     6   8.2161      0.00     0.03       0.00    -0.04
     7   8.2162      0.00     0.03       0.00     0.05
     8  12.4073      0.00    -0.18       0.00    -0.07
     9  13.6228      0.00     0.07       0.00    -0.04
    10  13.6230      0.00     0.07       0.00    -0.31
    11  14.2914      0.00    -0.17       0.00     0.64
    12  15.6573      0.00    -0.01       0.00     0.04
    13  16.3566      0.00     0.01       0.00    -0.06
    14  16.3567      0.00     0.20       0.00    -0.40
    15  16.3567      0.00     0.60       0.00     0.16
    16  16.3567      0.00     0.07       0.00     0.07
    17  16.4355      0.00     0.00       0.00     0.01
    18  16.4904      0.00    -0.04       0.00    -0.10
    19  16.4905      0.00    -0.12       0.00    -0.05
    20  16.4905      0.00    -0.11       0.00     0.09
    21  16.4931      0.00    -0.09       0.00     0.09
    22  16.4932      0.00    -0.14       0.00     0.10
    23  16.4932      0.00    -0.18       0.00    -0.04
    24  16.4933      0.00    -0.13       0.00    -0.01
    25  16.4935      0.00    -0.13       0.00     0.01
    26  16.5587      0.00    -0.21       0.00    -0.35
    27  16.5587      0.00    -0.06       0.00    -0.09
    28  16.5588      0.00     0.09       0.00     0.12
    29  16.6351      0.00     0.01       0.00    -0.31
    30  16.6351      0.00     0.08       0.00    -0.13
    31  16.6351      0.00     0.15       0.00     0.10
    32  17.4679      0.00    -0.33       0.00    -0.09
    33  17.4707      0.00    -0.02       0.00    -0.21
    34  17.4708      0.00     0.04       0.00    -0.00
    35  17.4708      0.00     0.21       0.00     0.10
    36  17.5253      0.00     0.24       0.00     0.05
    37  17.5254      0.00    -0.06       0.00     0.07
    38  17.5254      0.00     0.16       0.00    -0.04
    39  17.5254      0.00     0.01       0.00     0.06
    40  17.5334      0.00    -0.06       0.00     0.05
    41  17.5334      0.00    -0.01       0.00     0.08
    42  17.5334      0.00    -0.02       0.00     0.07
    43  17.5416      0.00    -0.24       0.00     0.07
    44  17.5416      0.00    -0.00       0.00     0.20
    45  18.5000      0.00     0.10       0.00    -0.05
    46  18.5000      0.00    -0.14       0.00    -0.13
    47  18.5001      0.00    -0.10       0.00     0.26
    48  18.5765      0.00     0.11       0.00     0.01
    49  18.5765      0.00    -0.30       0.00     0.07
    50  18.5766      0.00    -0.01       0.00    -0.06

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.

773892    quality flag:3

Type:       CENTAURR  CENTAURR  CENTAURR

axisobj        12.649    12.649    12.649
ecceobj         0.171     0.171     0.171
incobj         18.930    18.930    18.930
qmin            9.491     9.556     9.322
qmax           17.794    18.595    19.714
amean          12.508    12.559    12.550
amin           11.677    12.247    12.212
amax           13.819    14.372    14.533
emean           0.131     0.087     0.146
emin            0.003     0.000     0.015
emax            0.288     0.294     0.357
imean          19.415    16.735    18.431
imin           16.600    13.105    15.590
imax           21.003    20.243    20.191
excite_mean     0.361     0.304     0.352
fracstop        0.071     0.596     0.088
cjmean          3.611     3.628     3.609

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       207.6     173.2     176.2
kozaiamp        179.7     180.0     179.6